Projection exposure apparatus and method

Abstract

The present invention relates to a projection exposure apparatus (10) for and method of imaging a reticle (R) having patterned surface onto a substrate (W) in photolithographic processes for manufacturing a variety of devices. The invention further relates to an optical system (C) having a folding member (M1) suited to the projection exposure apparatus, and a method for manufacturing the optical system. The projection exposure apparatus comprises an illumination optical system (IS) and a reticle stage (RS) capable of holding the reticle so the normal line to its patterned surface is in the direction of gravity. The apparatus also includes a substrate stage (WS) capable of holding the substrate with its surface normal parallel to the direction of gravity. The optical system includes a first imaging optical system (A) comprising a concave reflecting mirror and a dioptric optical member arranged along a first optical axis. The first imaging optical system (A) forms an intermediate image of the patterned surface. The optical system also includes a second imaging optical system (B) having a second optical axis, and forms a reduced image of the intermediate image on the substrate. The first folding member is arranged in the optical path from the first imaging optical system to the second imaging optical system. The first and second imaging optical systems and the first and second folding members are positioned so that a reduced image of the pattered surface is formed parallel to the pattern surface of the reticle, and the first and second optical axes are positioned so that they are substantially parallel to the direction of gravity.

Description

FIELD OF THE INVENTION

The present invention relates to a projection exposure apparatus and method used when transferring a projection master plate (mask, reticle and the like) onto a substrate in photolithographic processes for manufacturing devices like semiconductor devices, image pickup devices, liquid crystal display devices and thin film magnetic heads, and further relates to an optical system having a folding member suited to the projection exposure apparatus, and a method for manufacturing the optical system.

BACKGROUND OF THE INVENTION

In photolithographic processes for manufacturing semiconductor devices and the like, a projection exposure apparatus is used that exposes the pattern image of a photomask or reticle (hereinafter, collectively referred to as “reticle”) as the projection master plate onto a substrate (wafer or glass plate and the like) coated with a photosensitive material like photoresist via a projection optical system.

With the increase in the level of integration of semiconductor devices and the like in recent years, the resolving power required by projection optical systems used in projection exposure apparatuses has been rapidly increasing. To meet this requirement, it has become necessary to shorten the wavelength of the exposure light and to increase the numerical aperture (NA) of the projection optical system. However, if the wavelength of the illumination light is shortened, particularly below 300 nm, the number of types of glass materials that can be used for practical purposes is limited to a few due to the absorption of light. Accordingly, the correction of chromatic aberration becomes problematic if the projection optical system is constructed with just dioptric optical elements. In addition, a dioptric optical system requires numerous lenses to correct the Petzval sum.

In contrast, a catoptric system not only has no chromatic aberration, but can also easily correct the Petzval sum by the use of a concave reflecting mirror. Accordingly, the construction of projection optical systems with so-called catadioptric optical systems that combine a catoptric system with a dioptric system has heretofore been proposed. Such catadioptric optical systems have been proposed in, for example, U.S. Pat. Nos. 5,537,260, 4,747,678, 5,052,763 and 4,779,966.

An increase in the NA and exposure region of projection optical systems has been demanded in recent years, and the aperture diameter of the optical members that constitute catadioptric optical systems has likewise increased. In light of the resolution required by projection exposure apparatuses, the effect of deformation of large optical members due to gravity cannot be ignored. A catadioptric optical system may be constructed with optical members in which the direction of the optical axes is not identical, as is typical of the prior art. One or more such optical members having power tend to be deformed asymmetrically with respect to the optical axis. This gives rise to asymmetric aberrations, which are difficult to correct during manufacturing, making it difficult to obtain sufficient resolution.

When correcting chromatic aberration in a conventional catadioptric optical system, high-order chromatic aberrations like transverse chromatic aberration, cannot be sufficiently corrected with just a concave reflecting mirror and quartz glass, and the image size cannot be increased. Consequently, attempts are being made to realize satisfactory correction of chromatic aberration over the entire exposure region by forming a number of lenses with fluorite. Nevertheless, since the volume and refractive index of lenses made of fluorite change much more than quartz glass and other optical glasses when environmental factors, like temperature, change, the optical performance of conventional optical systems deteriorates greatly when the environmental conditions fluctuate.

Catadioptric optical systems and catoptric optical systems typically require the use of a folding member to separate the optical path of the going path toward the concave mirror from the optical path of the returning path from the concave mirror. As a result, a plurality of partial optical systems having mutually different optical axes becomes necessary, and it follows that a plurality of lens barrels having different axes becomes necessary. Consequently, there is the problem that, compared with dioptric optical systems, errors are easily generated in the adjustment between the plurality of optical axes when assembling catadioptric optical systems and catoptric optical systems. In addition, even after assembly, the stability is poor due to the complex construction, and the positional relationships between optical axes gradually deviate, creating a tendency for the image to deteriorate. In addition, the folding member has an incident optical axis and an exit optical axis, which are not formed symmetrically. For this reason, rotating the folding member about the incident optical axis or about the exit optical axis due to, for example, factors like vibration, causes rotation of the image. In addition, rotating the folding member about the axis orthogonal to both the incident optical axis and the exit optical axis causes distortion of the image, making it difficult to stably obtain an image of high resolution.

Furthermore, optical adjustment of a dioptric optical system is disclosed in U.S. Pat. No. 4,711,567 and Japanese Patent Application Kokai No. Hei 10-54932, and optical adjustment of a catadioptric optical system is disclosed in U.S. Pat. No. 5,638,223.

SUMMARY OF THE INVENTION

The present invention relates to a projection exposure apparatus and method used when transferring a projection master plate (mask, reticle and the like) onto a substrate in photolithographic processes for manufacturing devices like semiconductor devices, image pickup devices, liquid crystal display devices and thin film magnetic heads, and further relates to an optical system having a folding member suited to the projection exposure apparatus, and a method for manufacturing the optical system.

Accordingly, the first goal of the present invention is to provide a large numerical aperture in the ultraviolet wavelength region, and to achieve high resolution without any substantial impact of gravity and the like.

The second goal of the present invention is to achieve a large numerical aperture in the ultraviolet wavelength region and a large exposure region, and to achieve an optical system of a practical size, satisfactorily corrected for chromatic aberration over the entire exposure region, having stable optical performance even during environmental fluctuations, and having a high resolution.

The third goal of the present invention is to make the optical adjustment of an optical system having a plurality of optical axes easy.

The fourth goal of the present invention is to reduce deterioration in imaging performance even after an optical system having a plurality of optical axes is assembled.

The fifth goal of the present invention is to perform with high precision optical adjustment of an optical system having a folding member.

Accordingly, a first aspect of the invention is a projection exposure apparatus for exposing a mask having a patterned surface onto a substrate having a photosensitive surface. The apparatus comprises an illumination optical system, and a reticle stage capable of holding the reticle so that the normal line of the patterned surface is substantially in the direction of gravity. The apparatus further includes a substrate stage capable of holding the substrate so that the normal line of the photosensitive surface of the substrate is substantially in the direction of gravity. The apparatus further includes, between the reticle and substrate stages, a projection optical system comprising first and second imaging optical systems. The first imaging optical system comprises a concave reflecting mirror and a dioptric optical member arranged along a first optical axis, and is designed to form an intermediate image of the patterned surface. The second imaging optical system has a second optical axis and forms a reduced image of the intermediate image onto the photosensitive surface. A first folding member is arranged in the optical path from the first imaging optical system to the second imaging optical system, and is provided with a reflecting surface having a reflective region that is substantially planar. Also, a second folding member is arranged between the first folding member and the second imaging optical system, and is provided with a reflecting surface having a reflecting region that is substantially planar. The first and second imaging optical systems and the first and second folding members are positioned so that a reduced image of the pattered surface is formed parallel to the pattern surface of the reticle, and the first and second optical axes are positioned so that they are substantially parallel to the direction of gravity.

A second aspect of the invention is a method for exposing a pattern on a reticle onto a substrate. The method comprises the steps of first illuminating the reticle, then projecting an image of the reticle with the projection exposure apparatus as described immediately above, and then exposing the pattern over an exposure region having either a slit-shape and arcuate shape, wherein the exposure region does not include the optical axis of the second imaging optical system in the image plane. In the exposure process, it is preferable to simultaneously scan the reticle stage and the substrate stage.

A third aspect of the invention is a projection exposure apparatus for forming an image of a first surface onto a second surface. The apparatus comprises a projection optical system having a lens, a concave mirror, a folding member and two or more optical axes. An optical member is arranged along each of the two or more optical axes, each optical member being held by a barrel provided along each of the two or more optical axes. Each of the barrels includes one or more lens barrel units each having one or more lens assemblies (or alternatively, lens elements) designed so as to be inclinable and translatable with respect to the optical axis. Also, at least one of the barrels is provided with at least one adjustment apparatus capable of inclining and translating the at least one barrel with respect to the optical axis passing therethrough.

BRIEF DESCRIPTION OF THE DRAWINGS

FIG. 1 a is a schematic diagram of the projection exposure apparatus according to the present invention;

FIG. 1 b is a plan view showing the exposure region EA on wafer W for the apparatus of FIG. 1 ;

FIG. 2 is an optical path diagram of the catadioptric optical system according to a first mode for carrying out the present invention;

FIGS. 3 a , 3 b are plots of the shape of the aspherical surfaces provided in the catadioptric optical system of FIG. 2 , wherein the horizontal axis is the distance from the optical axis in mm and the vertical axis is the deviation from an approximately spherical surface in mm.

FIGS. 4 a - 4 f are aberration plots of the catadioptric optical system of FIG. 2 , wherein FIG. 4 a is a lateral aberration plot in the meridional direction at an image height Y of 17.1 mm, FIG. 4 b is a lateral aberration plot in the meridional direction at an image height Y of 11 mm, FIG. 4 c is a lateral aberration plot in the meridional direction at an image height Y of 5 mm, FIG. 4 d is a lateral aberration plot in the sagittal direction at an image height Y of 17.1 mm, FIG. 4 e is a lateral aberration plot in the sagittal direction at an image height Y of 11 mm, and FIG. 4 f is a lateral aberration plot in the sagittal direction at an image height Y of 5 mm;

FIG. 5 is an optical path diagram of the catadioptric optical system according to a second mode for carrying out the present invention;

FIGS. 6 a , 6 b are plots of the shape of the aspherical surfaces provided in the catadioptric optical system of FIG. 5 , similar to those in FIGS. 3 a , 3 b;

FIGS. 7 a - 7 f are aberration plots of the catadioptric optical system of FIG. 5 , wherein FIG. 7 a is a lateral aberration plot in the meridional direction at an image height Y of 17.1 mm, FIG. 7 b is a lateral aberration plot in the meridional direction at an image height Y of 11 mm, FIG. 7 c is a lateral aberration plot in the meridional direction at an image height Y of 5 mm, FIG. 7 d is a lateral aberration plot in the sagittal direction at an image height Y of 17.1 mm, FIG. 7 e is a lateral aberration plot in the sagittal direction at an image height Y of 11 mm, and FIG. 7 f is a lateral aberration plot in the sagittal direction at an image height Y of 5 mm;

FIG. 8 is a cross-sectional view of the support structure and optical elements of the projection optical system according to a third mode for carrying out the present invention;

FIGS. 9 a - 9 c show the first to third barrels, respectively, according to the third mode for carrying out the present invention, wherein FIG. 9 a is an oblique view of the second barrel, FIG. 9 b is an oblique view of the first barrel, and FIG. 9 c is an oblique view of the third barrel;

FIG. 10 is an oblique view of the upper and lower frames, and the main support for the projection optical system of FIG. 8 ;

FIG. 11 is an explanatory diagram showing the relationship between the center of rotation and the image deviation of the imaging optical system;

FIGS. 12 a , 12 b show the projection optical system and the support structure thereof according to a fourth mode for carrying out the present invention, wherein FIG. 12 a is an XY plan view, and FIG. 12 b is a longitudinal cross-sectional view (YZ cross-sectional view);

FIG. 13 a is a partial cross-sectional front view (YZ partial cross-sectional view) of the attachment-removal mechanism and the adjustment mechanism of the second barrel;

FIG. 13 b is a longitudinal cross-sectional view (YZ cross-sectional view) of the third barrel;

FIG. 14 a is a longitudinal cross-sectional view (YZ cross-sectional view) of a translating and tilting mechanism;

FIG. 14 b is a plan cross-sectional view (XY cross-sectional view) that shows another example of a tilting mechanism;

FIG. 15 a is an optical path diagram of the projection optical system used in the catadioptric projection exposure apparatus according to the fifth mode for carrying out a present invention;

FIG. 15 b is a plan view (cross-sectional view taken in the direction of the arrows along the line 15 b — 15 b in FIG. 15 a ) of the exposure region of the projection optical system of FIG. 15 a;

FIG. 16 a is an optical path diagram of the projection optical system used in the catadioptric projection exposure apparatus according to a sixth mode for carrying out the present invention;

FIG. 16 b is a plan view (cross-sectional view taken in the direction of the arrows along the line 16 b — 16 b in FIG. 16 a ) of the exposure region of the projection optical system of FIG. 16 a;

FIG. 17 is a schematic diagram of the configuration of the optical system according to the seventh mode for carrying out the present invention;

FIG. 18 a is a schematic diagram illustrating the alignment method according to a seventh mode for carrying out the present invention;

FIG. 18 b is a view that shows the internal construction of the interferometer 121 of FIG. 18 a;

FIG. 19 a is a diagram illustrating the positioning of the folding mirrors and reflecting surface with respect to the support body of the optical system of FIG. 17 ;

FIG. 19 b is a diagram illustrating the positioning of the reflecting surface with respect to the axis of first lens barrel of the optical system of FIG. 17 ; and

FIG. 20 is a flowchart setting forth the steps for carrying out a device manufacturing method according to one mode of the present invention.

DETAILED DESCRIPTION OF THE INVENTION

The present invention relates to a projection exposure apparatus and method used when transferring a projection master plate (mask, reticle and the like) onto a substrate in photolithographic processes for manufacturing devices like semiconductor devices, image pickup devices, liquid crystal display devices and thin film magnetic heads, and further relates to an optical system having a folding member suited to the projection exposure apparatus, and a method for manufacturing optical system.

The following explains the projection exposure apparatus provided with a catadioptric optical system according to the present invention, based on the drawings. FIG. 1 a is a schematic of the projection exposure apparatus 10 according to the first and second modes for carrying out the present invention. An XYZ coordinate system is employed, as shown.

In apparatus 10 , reticle R, as the projection master plate whereon a predetermined circuit pattern is formed, is arranged in an object plane OP of a catadioptric optical system C. A wafer W (substrate), serving as a workpiece having a coating of a photosensitive material like photoresist, is arranged in an image plane IP of catadioptric optical system C. Reticle R is held by a reticle stage RS so that the normal line of the patterned surface is in the direction of gravity (the Z direction in FIG. 1 a ). Wafer W is held by a wafer stage WS so that the normal line of that surface is substantially parallel to the direction of gravity (Z direction). Reticle stage RS is constructed so that it is moveable along the ±Y direction for the purpose of scanning and exposure. In addition, wafer stage WS is constructed so that it is moveable in the XY plane, and so that the position in the Z direction and the tilt in the Z direction of wafer W are adjustable.

An illumination optical apparatus IS is arranged above reticle R (on the −Z direction side) to evenly illuminate a slit-shaped (rectangular or oblong) illumination region on reticle R. In the present example, the length direction of the slit-shaped illumination region is set to the X direction in the Figure. Furthermore, instead of a slit-shaped illumination region, an annular illumination region may also be used.

Catadioptric optical system C further includes first and second imaging optical systems A and B, respectively, and an aperture stop AS with a variable aperture diameter, located at the pupil position thereof. System C is substantially telecentric on the reticle R side and the wafer W side. Furthermore, a pupil filter such as disclosed in, for example, Japanese Patent Application Kokai No. Hei 6-349698 and the like, may also be arranged at the position of aperture stop AS.

Illumination optical apparatus IS comprises an exposure light source (not shown) comprising an ArF excimer laser light source, an optical integrator (not shown) to make the illumination intensity distribution of the exposure light having a wavelength of 193.3 nm from this light source uniform, an illumination system aperture stop, a variable field stop (reticle blind) (not shown) and a condenser lens system (not shown), and the like. Furthermore, a 248 nm wavelength KrF excimer laser light, a 157 nm wavelength F 2 laser light, the higher harmonics of a YAG laser, or a mercury lamp that supplies ultraviolet light below 300 nm may also be used as the exposure light source.

With continuing reference to FIG. 1 a , illumination light IL is supplied by illumination optical apparatus IS and proceeds along the +Z direction, and illuminates reticle R. The light from reticle R enters catadioptric-type first imaging optical system A wherein a concave reflecting mirror MC and a plurality of dioptric optical members (lenses) L 1 -L 3 are arranged along optical axis Z 1 . System A forms an intermediate image (not shown) of the pattern on the exposure region on reticle R on the exit side of first imaging optical system A. The light emerging from first imaging optical system A travels substantially along the −Z direction, is reflected by a plane mirror M 1 as a first folding member, and proceeds to a plane mirror M 2 as a second folding member substantially along the +Y direction (along optical axis Z 2 ) after the direction of travel thereof is folded substantially by 90°. The light reflected by mirror M 2 travels substantially along the +Z direction after the direction of travel thereof is folded substantially by 90°, and then enters dioptric-type second imaging optical system B comprising dioptric optical members L 4 and L 5 arranged along optical axis Z 3 parallel to optical axis Z 1 . The image of the light source of illumination optical apparatus IS is formed at the pupil position (position of aperture stop AS) of catadioptric optical system C. In other words, reticle R is Köhler illuminated. Then, the image of the pattern of Köhler illuminated reticle R is reduced via catadioptric optical system C by projection magnification β (|β| is ¼ in the present example, but may be another projection magnification like ⅕, ⅙ and the like), and is formed in image plane (second surface) IP of catadioptric optical system C.

FIG. 1 b shows the exposure region EA in image plane IP. Catadioptric optical system C in the present example is aberration-corrected in circular region CA having a radius of 17.1 mm about optical axis Z 3 . Slit-shape exposure region EA is 25×6 mm and is set in aberration corrected region CA and outside of shaded region SHA having a radius of 5 mm about optical axis Z 3 . Accordingly, exposure region EA can be set substantially freely, and may be set, for example, to an arcuate exposure region having the shape of one part of a ring.

Returning to FIG. 1 a , an autofocus/leveling sensor AF for detecting the position in the Z direction of exposure region EA on wafer W and the inclination with respect to the Z direction is provided in front of lens barrel 20 of catadioptric optical system C. A wafer stage control unit (WSCU) in electrical communication with sensor AF and wafer stage WS controls the drive of the wafer stage based on the output from sensor AF. This allows the exposure region EA on wafer W to substantially coincide with image plane IP of catadioptric optical system C.

Before the actual exposure operation, reticle stage RS positions reticle R in the X direction, Y direction and rotational direction, and wafer stage WS aligns the surface of wafer W with image plane IP of catadioptric optical system C and positions wafer W in the X direction and Y direction. Subsequently, the illumination region on reticle R is illuminated by illumination optical apparatus IS while reticle R and wafer W are synchronously scanned along the Y direction with a speed ratio corresponding to projection magnification β of the catadioptric optical system. After exposure of the pattern image of reticle R onto one exposure region on wafer W is finished, the next exposure region on wafer W is scanned and exposed by stepping wafer stage WS. These operations are repeated by the step-and-scan system. Since this type of step-and-scan system should obtain satisfactory imaging performance in the slit-shaped exposure region, a larger shot region on wafer W can be obtained without increasing the size of catadioptric optical system C.

In the present example, as shown in FIG. 1 a , each of the optical members (lenses L 1 -L 3 and concave reflecting mirror MC) that constitute first imaging optical system A are arrayed along optical axis Z 1 parallel to the direction of gravity. Each of the optical members (lenses L 4 and L 5 and aperture stop AS) that constitute second imaging optical system B are arrayed along optical axis Z 3 parallel to the direction of gravity. Lenses are not provided along optical axis Z 2 in the direction that traverses the direction of gravity. Consequently, the generation of asymmetric aberrations due to the effect of gravity on these optical members can be controlled. Furthermore, the lens barrel of a conventional right cylinder-type catadioptric optical system, which is a field-proven support technology, can be applied as is to the optical members in first imaging optical system A and second imaging optical system B. Accordingly, there are advantages in that the manufacture of catadioptric optical system C is easy and the performance stability after installation of the apparatus can be improved. Furthermore, in the present invention, the substantial coincidence of the normal lines of the reticle R surface and wafer W surface with the direction of gravity includes the state wherein the normal lines are inclined by a minute amount to adjust the reticle surface or wafer surface.

In the above mode for carrying out the present invention, the NA of the light beam passing through first imaging optical system A, which is a catadioptric optical system, is smaller than that in second imaging optical system B, which is a dioptric optical system. Accordingly, separation of the optical paths in first imaging optical system A is easy, and the NA can be made larger than the case wherein the second imaging optical system is made a catadioptric optical system. In addition, a light beam of a small NA passes through first imaging optical system A. Accordingly, the aperture diameter of concave reflecting mirror MC can be reduced.

In projection exposure apparatus 10 of the present mode for carrying out the present invention, one intermediate image is formed in the optical system, and first folding member M 1 is arranged in the vicinity of this intermediate image. Since the diameter of the light beam is reduced in the vicinity of the intermediate image, separation of the optical paths by first folding member M 1 can be realized easily. Only one intermediate image is formed in the optical system of the present mode for carrying out the present invention. Thus, the total length of the optical system can be shortened, as compared to the case wherein a plurality of intermediate images is formed.

Also, only one concave mirror, and not a plurality thereof, is used in projection exposure apparatus 10 . This has the advantage that the optical paths can be separated even if exposure region EA is not very remote from the optical axis, thus not causing an increase in the size of the optical system.

Reticle R may be illuminated so that projection optical system (catadioptric optical system) C can form a slit-shaped or arcuate exposure region EA that does not include the optical axis of the second imaging optical system in the image plane. If reticle stage RS and wafer stage WS are scanned, then first folding member M 1 that folds the light passing through first imaging optical system A toward the second imaging optical system B can be easily arranged at a position that does not interfere with the light beam proceeding from the reticle to the concave mirror. Thus, the use of a beam splitter having a transmitting-reflecting surface for optical path separation becomes unnecessary. Consequently, the generation of stray light caused by flare and illumination unevenness can be reduced, and the risk of causing deterioration in image quality is extremely small.

Next, a mode for carrying out the present invention will be explained using numerical values. FIG. 2 and FIG. 5 show optical path diagrams of the catadioptric optical system according to the first and second modes for carrying out the present invention, respectively. In FIG. 2 and FIG. 5 , an XYZ coordinate system, the same as that in FIG. 1 a , is employed.

With reference now to FIGS. 2 and 5 , a catadioptric optical systems C 1 and C 2 according to first and second modes for carrying out the present invention is one now set forth. System C 1 comprises catadioptric-type first imaging optical system A, dioptric-type second imaging optical system B, and plane mirror M 1 as the first folding member and plane mirror M 2 as the second folding member arranged between the first and second imaging optical systems.

In FIG. 2 and FIG. 5 , first imaging optical system A according to the first and second modes for carrying out the present invention comprises 1-1th lens group G 11 , 1-2th lens group G 12 and concave reflecting mirror MC. Lens groups G 11 , G 12 and concave reflecting mirror MC are arranged coaxially so that the light from the first surface (reticle R) sequentially passes through lens group G 11 , lens group G 12 and then reaches concave reflecting mirror MC. The light reflected by concave reflecting mirror MC emerges from lens group G 12 . First imaging optical system A forms an intermediate image of reticle R at a position separated from the optical axis in the optical path between lens group G 11 and lens group G 12 . First imaging optical system A according to the first and second modes for carrying out the present invention has slight reduction magnification.

Second imaging optical system B according to the first and second modes for carrying out the present invention comprises a lens group G 21 having positive refractive power, aperture stop AS and 2-2th lens group G 22 having a positive refractive power. Lens groups G 21 , G 22 and aperture stop AS are arranged coaxially so that the light from the intermediate image passing from plane mirrors M 1 , M 2 sequentially passes through lens group G 21 , aperture stop AS and lens group G 22 .

First imaging optical system A is in the optical path between reticle R and concave reflecting mirror MC. The pupil plane thereof is at a position remote from concave reflecting mirror MC. The light source image formed by illumination optical system IS is relayed to the pupil plane of first imaging optical system A. However, if a light source having a high output like a laser light source, for example, is used, a concentration of energy will occur at the position of the light source image. If the pupil plane thereof coincides with the reflecting surface of concave reflecting mirror MC, there is a risk that the reflective film on the reflecting surface will be damaged. Nevertheless, since the light source image is formed at a position remote from the reflecting surface of concave reflecting mirror MC, it does not cause damage to the reflective film. The position of the pupil plane is positioned in the optical path between the reticle and the concave reflecting mirror. Thus, the exit pupil of first imaging optical system A can be set on the second imaging optical system B side of the intermediate image. Thereby, it becomes unnecessary to make second imaging optical system B telecentric on the intermediate image side. In this case, system C 1 , which has no lens equivalent to a field lens between the first and second folding members M 1 and M 2 , has the advantage that the aperture diameter of second imaging optical system B can be reduced.

In the first mode for carrying out the present invention shown in FIG. 2 , lens group G 11 in first imaging optical system A comprises two negative meniscus lenses L 111 , L 112 whose concave surfaces face the reticle R side. These two lenses L 11 , L 12 are both formed of synthetic quartz.

Lens group G 12 in first imaging optical system A comprises, in order from the reticle R side, a biconvex positive lens L 121 , a positive meniscus lens L 122 whose convex surface faces the reticle R side, a biconcave negative lens L 123 , a biconvex positive lens L 124 , a positive meniscus lens L 125 whose convex surface faces the reticle R side, and a negative meniscus lens L 126 whose concave surface faces the reticle R side. Furthermore, biconvex positive lens L 124 is formed of fluorite, and the other lenses L 121 to L 123 , L 125 to L 126 in lens group G 12 are formed of synthetic quartz.

The reflecting surface of plane mirror M 1 has an oblong-shaped effective region, and is planar over the entire effective region. Furthermore, this reflecting surface is provided between lens group G 11 and lens group G 12 so that the lengthwise direction of the effective region is in the X direction and the widthwise direction is inclined by 45° with respect to the Z direction.

The reflecting surface of plane mirror M 2 as the second folding member has an approximately elliptical-shaped effective region, and is planar over the entire effective region. Furthermore, the reflecting surface of plane mirror M 2 is provided so that the minor axis of the elliptical-shaped effective region is in the X direction, and the major axis of the elliptical-shaped effective region is inclined by 45° with respect to the Z direction. In other words, in the present example, the reflecting surface of plane mirror M 1 and the reflecting surface of plane mirror M 2 are arranged so that they are mutually orthogonal.

Lens group G 21 in second imaging optical system B comprises, in order from the plane mirror M 2 side (light entrance side), a biconvex positive lens L 211 , a negative meniscus lens L 212 whose convex surface faces the wafer W side, a negative meniscus lens L 213 whose concave surface faces the wafer W side, and a biconvex positive lens L 214 . Furthermore, the concave surface on the wafer W side of negative meniscus lens L 213 is aspherical. Biconvex positive lens L 214 is formed of fluorite, and the other lenses L 211 to L 213 in lens group G 21 are formed of synthetic quartz.

Lens group G 22 in second imaging optical system B comprises, in order from the group G 21 side (light entrance side), a biconcave negative lens L 221 , a biconvex positive lens L 222 , two positive meniscus lenses L 223 , L 224 whose concave surfaces face the wafer W side, a biconcave negative lens L 225 , and two biconvex positive lenses L 226 , L 227 . Furthermore, the concave surface (*) on the wafer W side of biconcave negative lens L 225 is aspherical. In addition, all lenses L 221 to L 227 that constitute lens group G 22 are formed of synthetic quartz.

In the second mode for carrying out the present invention shown in FIG. 5 , system C 2 includes lens group G 11 in first imaging optical system A, which comprises, in order from the reticle R side, a planoconvex negative lens L 111 whose planar surface faces the reticle R side, a negative meniscus lens L 112 whose concave surface faces the reticle R side, and a positive meniscus lens L 113 whose concave surface faces the reticle R side. All lenses L 111 to L 113 that constitute lens group G 11 are formed of synthetic quartz.

Lens group G 12 in first imaging optical system A comprises, in order from the reticle R side, a biconvex positive lens L 121 , a positive meniscus lens L 122 whose convex surface faces the reticle R side, a biconcave negative lens L 123 , a biconvex positive lens L 124 , a positive meniscus lens L 125 whose convex surface faces the reticle R side, and a negative meniscus lens L 126 whose concave surface faces the reticle R side. In lens group G 12 , biconvex positive lens L 124 is formed of fluorite, and the other lenses L 121 to L 123 , and L 125 to L 126 are formed of synthetic quartz.

The reflecting surface of plane mirror M 1 as the first folding member has an oblong-shaped effective region, and is planar over the entire effective region. This reflecting surface is provided between lens group G 11 and lens group G 12 so that the lengthwise direction of the effective region is in the X direction and the widthwise direction is inclined by 45° with respect to the Z direction.

The reflecting surface of plane mirror M 2 as the second folding member has an approximately elliptical-shaped effective region, and is planar over the entire effective region. The reflecting surface of plane mirror M 2 is provided so that the minor axis of the elliptical-shaped effective region is in the X direction, and the major axis of the elliptical-shaped effective region is inclined by 45° with respect to the Z direction. In other words, in the present example as well, the reflecting surface of plane mirror M 1 and the reflecting surface of plane mirror M 2 are arranged so that they are mutually orthogonal.

Lens group G 21 in second imaging optical system B comprises, in order from the plane mirror M 2 side (light entrance side), a biconvex positive lens L 211 , a negative meniscus lens L 212 whose convex surface faces the wafer W side, a negative meniscus lens L 213 whose convex surface faces the wafer W side, and a biconvex positive lens L 214 . In lens group G 21 , biconvex positive lens L 214 is formed of fluorite, and the other lenses L 211 to L 213 are formed of synthetic quartz. In addition, the concave surface (*) on the wafer W side of the negative meniscus lens L 213 is aspherical.

Lens group G 22 in second imaging optical system B comprises, in order from the lens group G 21 side (light entrance side), a negative meniscus lens L 221 whose convex surface faces the wafer W side, a positive meniscus lens L 222 whose convex surface faces the wafer W side, a biconvex positive lens L 223 , a positive meniscus lens L 224 whose convex surface faces the wafer W side, a biconcave negative lens L 225 , a positive meniscus lens L 226 whose convex surface faces the wafer W side, and a biconvex positive lens L 227 . Furthermore, the concave surface on the wafer W side of biconcave negative lens L 225 is aspherical surface. In addition, all lenses L 221 to L 227 that constitute lens group G 22 are formed of synthetic quartz.

As described in the above first and second modes for carrying out the present invention, by providing second imaging optical system B with lens group G 21 having a positive refractive power, aperture stop AS arranged between lens group G 21 and the reduced image, and lens group G 22 arranged between aperture stop AS and the reduced image, and by providing at least one aspherical surface each in lens group G 21 and lens group G 22 , spherical aberration and coma can be satisfactorily corrected with good balance, and optical performance can be improved. Alternatively, for substantially the same optical performance, a large exposure region can be achieved without the attendant increase in the size of the optical system. Furthermore, by making the aperture diameter of aperture stop AS variable, it can be adjusted to the optimal resolving power and depth of focus for the particular exposure pattern.

First imaging optical system A in the first and second modes for carrying out the present invention (i.e., systems C 1 and C 2 ) forms an intermediate image in the optical path between first folding member M 1 and first imaging optical system A. Thus, the optical paths can be easily separated by the first folding member.

At this point, it is preferable the present invention satisfy condition (1) below, wherein LF 1 is the distance between the intermediate image plane and the effective region of the first folding member, and S 1 is the area of the effective region of the first surface.

LF 1 / S 1 >0.002  (1)

Condition (1) stipulates the appropriate position for plane mirror M 1 . If condition (1) is not satisfied, a deterioration in optical performance, such as illumination unevenness due to flaws in the fabrication of the reflecting surface of first folding member M 1 , defects in the reflective film, and dirt on the reflecting surface cannot be prevented, and a sufficient resolving power cannot be obtained over the entire exposure region. Accordingly, it is preferable to set an upper limit value to condition (1) of 4 in order to make separation of the optical paths by first folding member M 1 easy. In addition, it is preferable to set the lower limit value to 0.005 in order to improve the ability to mass-produce the projection optical system.

In condition (1), distance LF 1 between the intermediate image plane and first folding member M 1 is the distance along a direction parallel to the optical axis between the intermediate image plane and the position closest to the intermediate image plane in the effective region of first folding member M 1 .

In addition, it is preferable in the first and second modes for carrying out the present invention to satisfy condition (2) below, wherein c 1 is the maximum effective diameter among the effective diameters of the optical members that constitute first imaging optical system A, c 2 is the maximum effective diameter among the effective diameters of the optical members that constitute second imaging optical system B, and LO 2 is the distance between optical axis Z 1 of the first imaging optical system and optical axis Z 3 of the second imaging optical system.

LO 2 /( c 1 +c 2 )>0.7  (2)

Condition (2) stipulates an appropriate interaxis distance between the first and second imaging optical systems. If condition (2) is not satisfied, the spacing to stably hold the optical members that constitute these optical systems cannot be ensured, making it difficult to continuously realize sufficient optical performance of the projection optical system. To prevent increasing the size of second folding member M 2 , it is preferable to set an upper limit value to condition (2) of 2.5. In addition, to make adjustment of the optical system easier, it is preferable to set the lower limit value of condition (2) to 0.9.

In addition, in the catadioptric optical system according to the first and second modes for carrying out the present invention, at least one positive lens among the dioptric optical members arranged in the round-trip optical path in first imaging optical system A, namely the optical path from first surface R to concave mirror MC and the optical path from concave mirror MC to the intermediate image, is formed of fluorite. Chromatic aberration is corrected with a comparatively small number of fluorite lenses by making the chromatic aberration-correcting effect of the fluorite function in both directions of the round-trip optical path. In the first and second modes for carrying out the present invention, the pupil plane is formed at a position apart from the reflecting surface of concave reflecting mirror MC to prevent damage to the reflective film. Thus, the direction of fluctuations in optical performance of the first imaging optical system due to fluctuations in environmental factors like temperature varies with the positional relationship between the pupil plane and concave reflecting mirror MC. In other words, the state of the light beam that passes through the positive lens made of fluorite in first imaging optical system A loses symmetry between the going path (optical path from first surface R to concave reflecting mirror MC) and the returning path (optical path from concave reflecting mirror MC to the intermediate image). The direction of fluctuations in the optical performance varies depending on whether the pupil plane is positioned in the going path or returning path. Volumetric changes due to changes in the temperature of the fluorite cause expansion proportional to the change in temperature. Thus, the radius of curvature of the lens increases as the temperature rises. In addition, since changes in the refractive index due to changes in the temperature of the fluorite are inversely proportional to the change in temperature, the refractive index decreases as the temperature increases. Since both of the above cases work to lower the refractive power of the surface, the focal length of a fluorite lens increases as the temperature of the lens rises.

If the pupil plane of first imaging optical system A is positioned between first surface R and concave reflecting mirror MC, as in the first and second modes for carrying out the present invention, fluctuations in optical performance due to changes in the temperature of the positive lenses made of fluorite in first imaging optical system A have a stronger effect in the going path. Accordingly, in the first and second modes for carrying out the present invention, fluctuations in optical performance are generated in the direction the reverse of that in the first imaging optical system and the total amount of fluctuation in the optical system is reduced by arranging the positive lens made of fluorite in lens group G 21 on the intermediate image side of the pupil plane of second imaging optical system B.

If the pupil plane of first imaging optical system A is arranged between concave reflecting mirror MC and the intermediate image, fluctuations in optical performance due to changes in the temperature of the positive lens made of fluorite in first imaging optical system A have a stronger effect in the returning path. In this case, by arranging the positive lens made of fluorite in lens group G 22 on the secondary image side of the pupil plane of second imaging optical system B, fluctuations in optical performance in the direction the reverse of that in the first imaging optical system can be generated, and the total amount of fluctuation in the optical system can be reduced.

The abovementioned fluctuations in optical performance caused by temperature changes are fluctuations principally in the direction of the image height as represented by fluctuations in magnification, and do not include fluctuations in the direction of the optical axis as represented by fluctuations in focus. Nevertheless, since fluctuations in the direction of the optical axis can be easily corrected by autofocus mechanisms and the like, this is actually a small problem for projection exposure. Furthermore, to reduce fluctuations in both the image height direction and in the optical axis direction, we can consider the use of fluorite in the negative lens on the second surface side of the pupil plane of second imaging optical system B. However, this cannot lead to a realistic solution because the efficiency of chromatic aberration correction is poor in the initial state (i.e., the state wherein environmental optical performance fluctuations are not generated).

It is preferable in the first and second modes for carrying out the present invention that the catadioptric optical system be an optical system telecentric on the first and second surface sides.

It is also preferable that systems C 1 and C 2 satisfy condition (3) below, wherein LP 3 is the distance between the pupil plane of first imaging optical system A and concave reflecting mirror MC, and D 1 is the effective radius of concave reflecting mirror MC.

2.50> LP 3 /D 1 >0.15  (3)

Condition (3) stipulates an appropriate distance between the pupil plane and the concave reflecting mirror to achieve satisfactory correction of chromatic aberration while avoiding damage to the reflective film by the laser, and to make the optical axes of all optical members that constitute the catadioptric optical system mutually parallel. If L 3 /D 1 exceeds the upper limit in condition (3), the correction of high-order chromatic aberrations like transverse chromatic becomes difficult. In addition, if LP 3 /D 1 falls below the lower limit in condition (3), damage to the reflective film by the laser cannot be avoided, and it is also difficult to make the optical axes of all lenses parallel.

If the pupil plane of first imaging optical system A is positioned between the first surface and the concave reflecting mirror, and at least one positive lens made of fluorite is arranged in lens group G 21 on the intermediate image side of the pupil plane of second imaging optical system B, then it is preferable to satisfy condition (4) below, wherein f 12 is the sum of the focal lengths of the positive lenses made of fluorite in lens group G 12 , and f 21 is the sum of the focal lengths of the positive lenses made of fluorite in 2-1th lens group G 21 .

2.0> f 12 /f 21 >0.5  (4)

Condition (4) stipulates an appropriate range for the focal lengths of the positive lenses made of fluorite, to reduce fluctuations in optical performance when the environment changes. If f 12 /f 21 exceeds the upper limit or falls below the lower limit in condition (4), fluctuations in optical performance due to changes in environmental factors, particularly temperature, become excessively large, and a sufficient resolving power can no longer be continuously maintained. Furthermore, if two or more positive lenses made of fluorite are arranged in lens group G 112 or lens group G 21 , each of the sums of the focal lengths of the positive lenses made of fluorite should be considered.

The Tables below list the values of the specifications of systems C 1 and C 2 of the first and second modes for carrying out the present invention. Table 1 and Table 3 include the lens data of the catadioptric optical systems according to the first and second modes for carrying out the present invention, respectively. In Table 1 and Table 3, the leftmost column (first column) S indicates the surface number of each optical surface (lens surface and reflecting surface), the next column to the right (second column) R indicates the radius of curvature of each optical surface, the next column to the right (third column) d indicates the surface spacing between each optical surface, the next column to the right (fourth column) Re indicates the effective radius of each optical surface, and the next column to the right (fifth column) “material” indicates the name of the material of which the optical member is made. In addition, in Table 1 and Table 3, d 0 is the distance from the object plane (reticle surface) to the optical surface most reticle-wise, WD is the distance from the most wafer-wise optical surface to the wafer surface (image plane), β is the lateral magnification of the projection system when light enters the projection system from the reticle side, and NA is the numerical aperture on the wafer side. Furthermore, in Table 1 and Table 3, the sign of the radius of curvature and surface spacing reverses around a reflecting surface.

In addition, in Table 1 and Table 3, an asterisk (*) appended to a surface number, indicates an aspherical surface, and the radius of curvature for such aspherical surfaces indicates the vertex radius of curvature. This aspherical surface shape is represented by condition (a) below. For a tangential plane at the apex of the aspherical surface, the origin is the position that the optical axis passes through at the tangential plane, and z(y) is based on the vertex of the aspherical surface, the displacement in the direction of the optical axis of the aspherical surface at the position of height y in the tangential plane when the direction of travel of the ray is positive. $$ x ⁡ ( y ) = y 2 r 1 + 1 - ( 1 + κ ) ⁢ y 2 r 2 + Ay 4 + By 6 + Cy 8 + Dy 10 + Ey 12 + Fy 14 ( a )

In formula (a), r is the vertex radius of curvature, κ is the conical coefficient, and A, B, C, D, E, F are the aspherical surface coefficients. Table 2 and Table 4 list conical coefficient κ and aspherical coefficients A, B, C, D, E, F as the aspherical surface data in the first and second modes for carrying out the present invention.

Furthermore, in the first and second modes for carrying out the present invention, the dioptric optical members are formed of synthetic quartz (SiO 2 ) or fluorite (CaF 2 ). The refractive index n at the working reference wavelength (193.3 nm) and the inverse ν of the dispersion value at the reference wavelength ±1 pm thereof are as follows. $$ Synthetic ⁢   ⁢ quartz ⁢ : n = 1.56033 v = 1762 × 10 2 Fluorite ⁢ : ⁢   n = 1.50146 v = 2558 × 10 2

The dispersion value 1/ν is represented by condition (b) below, wherein the refractive index at the working reference wavelength is n(o), the refractive index at the reference wavelength+1 pm is n(L), and the refractive index at the working wavelength−1 pm is n(S).

1 /ν=[n ( o )−1 ]/[n ( S ) n ( L )]  (b)

In the fourth column that indicates the effective radius of each optical surface, the length of the long side and short side is indicated for plane mirror M 1 , which has an oblong effective region, and the length of the major axis and minor axis of the ellipse is indicated for plane mirror M 2 , which has an elliptical effective region.

TABLE 1
LENS DESIGN DATA, FIRST MODE
d0 = 66.2181
WD = 12.0000
|β| = 1/4
NA = 0.75
S	R	d	Re	Material
1	−173.2198	59.9763	77.54	Synthetic Quartz	L111
2	−199.3558	2.4684	93.84
3	−1413.5392	42.7237	97.79	Synthetic Quartz	L112
4	−60064.7315	87.0000	104.07
5	1092.1574	26.0439	124.31	Synthetic Quartz	L121
6	−832.9175	3.1990	125.18
7	245.6137	35.000	128.10	Synthetic Quartz	L122
8	565.3602	304.9236	125.79
9	−220.6579	20.4061	85.82	Synthetic Quartz	L123
10	391.9184	5.7049	88.75
11	594.4147	29.9442	89.29	Fluorite	L124
12	−412.6301	72.7628	90.63
13	410.4514	26.1344	94.43	Synthetic Quartz	L125
14	669.5983	138.8597	93.16
15	−238.4760	25.0000	113.89	Synthetic Quartz	L126
16	−837.0357	16.6526	129.65
17	−356.5760	−16.6526	130.61	Concave Reflect-
				ing mirror MC
18	−837.0357	−25.0000	129.99	Synthetic Quartz	L126
19	−238.4760	−138.8597	118.38
20	669.5983	−26.1344	110.10	Synthetic Quartz	L125
21	410.4514	−72.7628	110.23
22	−412.6301	−29.9442	95.29	Fluorite	L124
23	594.4147	−5.7049	93.24
24	391.9484	−20.4061	92.49	Synthetic Quartz	L123
25	−220.6579	−304.9236	86.06
26	565.3602	−35.0000	94.14	Synthetic Quartz	L122
27	245.6137	−3.1990	95.98
28	−832.9175	−26.0439	92.73	Synthetic Quartz	L121
29	1092.1574	−1.0000	90.76
30	∞	530.0000	134 × 53	Plane Mirror M1
			(oblong)
31	∞	−129.6727	260 × 220	Plane Mirror M2
			(ellipse)
32	−416.5064	−43.6858	130.51	Synthetic Quartz	L211
33	1614.8553	−19.8749	129.15
34	375.6187	−40.1637	128.76	Synthetic Quartz	L212
35	992.3735	−154.0322	130.25
36	−540.0532	−30.6056	124.67	Synthetic Quartz	L213
37*	−280.2053	−4.7489	119.84
38	−269.7063	−59.8107	120.36	Fluorite	L214
39	1000.1381	−18.8527	118.99
40	∞	−20.0376	114.42	Aperture Stop AS
			(variable)
41	638.2931	−25.0000	113.74	Synthetic Quartz	L221
42	−6260.2239	−10.3928	116.87
43	−337.6474	−45.2717	122.52	Synthetic Quartz	L222
44	2063.2498	−33.0583	121.91
45	−239.6600	−45.1169	116.23	Synthetic Quartz	L223
46	−4631.0389	−1.0027	112.20
47	−167.6364	−40.2179	99.72	Synthetic Quartz	L224
48	−1732.6245	−6.1992	94.74
49	2730.6200	−25.0000	92.94	Synthetic Quartz	L225
50*	−306.7043	−1.8667	75.85
51	−254.0551	−24.4188	74.92	Synthetic Quartz	L226
52	4420.0238	−1.2986	69.49
53	−316.0614	−65.0000	62.88	Synthetic Quartz	L227
54	12272.4820	(WD)	30.79

TABLE 2
ASPHERICAL DATA OF THE FIRST MODE FOR
CARRYING OUT THE PRESENT INVENTION
37                                                                        th                                                                     Surface
κ = 0.0000
A = −1.3249 × 10                                                                        −08
B = −1.2617 × 10                                                                        −13
C = 1.4089 × 10                                                                        −18
D = −6.4967 × 10                                                                        −23
E = 3.4235 × 10                                                                        −27
F = −1.5167 × 10                                                                        −31
50                                                                        th                                                                     Surface
κ = 0.0000
A = −5.0678 × 10                                                                        −08
B = −3.8316 × 10                                                                        −13
C = −5.6799 × 10                                                                        −17
D = −6.9166 × 10                                                                        −22
E = 0.0000
F = 0.0000

TABLE 3
SECOND MODE FOR CARRYING OUT THE PRESENT INVENTION
d0 = 50.0980
WD = 12.3836
|β| = 1/4
NA = 0.75
S	R	d	Re	Material
1	∞	30.8769	71.96	Synthetic Quartz	L111
2	1358.1393	25.6596	82.00
3	−173.9366	29.5956	82.54	Synthetic Quartz	L112
4	−262.5027	3.9549	93.62
5	−243.7585	32.1846	94.30	Synthetic Quartz	L113
6	−198.6141	78.6305	102.23
7	705.6754	29.6916	128.29	Synthetic Quartz	L121
8	−853.6854	7.1157	128.85
9	243.8837	35.0000	130.00	Synthetic Quartz	L122
10	393.9524	334.9670	126.27
11	−228.4608	20.5261	87.25	Synthetic Quartz	L123
12	324.6767	7.3561	90.62
13	359.7325	40.5663	92.51	Fluorite	L124
14	−554.2952	58.0131	94.34
15	588.9791	33.3872	97.95	Synthetic Quartz	L125
16	3573.1266	113.1955	97.48
17	−249.4612	25.0000	111.74	Synthetic Quartz	L126
18	−1326.9703	25.8354	126.13
19	−367.4917	−25.8354	129.94	Concave Reflect-
				ing Mirror MC
20	−1326.9703	−25.0000	127.54	Synthetic Quartz	L126
21	−249.4612	−113.1955	117.01
22	3573.1266	−33.3872	112.48	Synthetic Quartz	L125
23	588.9791	−58.0131	111.89
24	−554.2952	40.5663	100.25	Fluorite	L124
25	359.7325	−7.3561	97.36
26	324.6767	−20.5261	94.44	Synthetic Quartz	L123
27	−228.4608	−334.9670	87.51
28	393.9524	−35.0000	93.84	Synthetic Quartz	L122
29	243.8837	−7.1157	96.50
30	−853.6854	−29.6916	93.81	Synthetic Quartz	L121
31	705.6754	−1.6203	92.09
32	∞	530.0000	135 × 53	Plane Mirror M1
			(oblong)
33	∞	−100.0000	260 × 220	Plane Mirror M2
			(ellipse)
34	−473.4614	−50.8662	130.00	Synthetic Quartz	L211
35	1218.5628	−18.9785	128.42
36	357.1688	−31.0635	128.11	Synthetic Quartz	L212
37	818.7536	−209.4034	129.93
38	−571.9096	−31.2079	123.89	Synthetic Quartz	L213
39*	−295.8211	−4.7127	119.48
40	−291.2028	−53.9868	119.84	Fluorite	L214
41	858.6769	−19.1416	119.00
42	∞	−24.0577	115.27	Aperture Stop
				AS
43	719.7751	−25.0000	113.83	Synthetic Quartz	L221
44	6715.0030	−22.3498	117.19
45	−314.9647	−45.0000	124.79	Synthetic Quartz	L222
46	−5036.3103	−16.5385	123.55
47	−265.1907	−45.0000	120.07	Synthetic Quartz	L223
48	9375.9412	−1.1109	116.54
49	−177.9561	−50.1531	103.37	Synthetic Quartz	L224
50	−18823.9455	−4.9217	94.91
51	1624.4953	−25.0000	93.03	Synthetic Quartz	L225
52*	−247.3912	−1.0000	74.54
53	−210.5206	−24.3364	73.99	Synthetic Quartz	L226
54	−35247.2125	−1.0621	69.21
55	−293.7588	−65.0000	63.01	Synthetic Quartz	L227
56	56893.1197	(WD)	31.15

TABLE 4
ASPHERICAL DATA OF THE SECOND MODE FOR
CARRYING OUT THE PRESENT INVENTION
39                                                                        th                                                                     Surface
κ = 0.0000
A = −1.3500 × 10                                                                        −08
B = −1.2494 × 10                                                                        −13
C = −1.3519 × 10                                                                        −18
D = −9.1832 × 10                                                                        −23
E = 3.6355 × 10                                                                        −27
F = −1.6744 × 10                                                                        −31
52                                                                        nd                                                                     Surface
κ = 0.0000
A = −4.8204 × 10                                                                        −08
B = −1.1379 × 10                                                                        −12
C = −6.8704 × 10                                                                        −17
D = −2.8172 × 10                                                                        −21
E = 0.0000
F = 0.0000

Table 5 below lists the numerical values corresponding to the conditions of the first and second modes for carrying out the present invention.

TABLE 5
NUMERICAL VALUES CORRESPONDING TO CONDITIONS
OF THE FIRST MODE FOR CARRYING OUT THE PRESENT
INVENTION
L1 =               11.55
S1 =               2400
L2 =               530
C1 =               261.22
C2 =               259.88
L3 =               118.11
D1 =               130.61
f12 =              490.57
f22 =              430.38
(1) L12/S1 =       0.0556
(2) L2/(c1 + c2) = 1.0171
(3) L3/D1 =        0.904
(4) f12/f21 =      1.0171
NUMERICAL VALUES CORRESPONDING TO CONDITIONS
OF THE SECOND MODE FOR CARRYING OUT THE PRESENT
INVENTION
L1 =               6.07
S1 =               2400
L2 =               530
C1 =               261.02
C2 =               261.22
L3 =               100.93
D1 =               129.99
f12 =              441.59
f22 =              440.56
(1) L12/S1 =       0.0154
(2) L2/(c1 + c2) = 1.0149
(3) L3/D1 =        0.776
(4) f12/f21 =      1.002

FIG. 3 a shows the amount of displacement (deviation) from an approximate spherical surface of the rotationally symmetric aspherical surface formed on the concave surface on the wafer side of negative meniscus lens L 213 in catadioptric optical system C of the first mode for carrying out the present invention. FIG. 3 b shows the amount of displacement (deviation) from an approximate spherical surface of the rotationally symmetric aspherical surface formed on the concave surface on the wafer side of biconcave negative lens L 225 in the catadioptric optical system C 1 of the first mode for carrying out the present invention. In addition, FIG. 6 a shows the amount of displacement (deviation) from an approximate spherical surface of the rotationally symmetric aspherical surface formed on the concave surface on the wafer side of negative meniscus lens L 213 in the catadioptric optical system C 2 of the second mode for carrying out the present invention. FIG. 6 b shows the amount of displacement (deviation) from an approximate spherical surface of the rotationally symmetric aspherical surface formed on the concave surface on the wafer side of biconcave negative lens L 225 in the catadioptric optical system C 2 of the second mode for carrying out the present invention. In each graph, the abscissa is the distance of the aspherical surface from the optical axis, and the ordinate is the amount of displacement along the optical axis direction from the approximate spherical surface (spherical surface having a vertex radius of curvature).

As can be seen from FIG. 3 a , FIG. 3 b , FIG. 6 a and FIG. 6 b , among the aspherical surfaces that second imaging optical system B possesses in catadioptric optical systems C 1 and C 2 of the first and second modes for carrying out the present invention, the cross-sectional shape that includes the optical axis of the rotationally symmetric aspherical surface having a paraxial negative refractive power is a shape having first and second inflection points facing from the optical axis toward the lens periphery with respect to the approximate spherical surface. The first inflection point is on the optical axis, and the cross-sectional shape from the optical axis to the second inflection point has less curvature than the curvature of an approximate spherical surface. The cross-sectional shape from the second inflection point to the lens periphery has greater curvature than the curvature of an approximate spherical surface.

FIGS. 4 a - 4 f and FIGS. 7 a - 7 f are plots of the lateral aberration on wafer W of catadioptric optical systems C 1 and C 2 respectively. In each lateral aberration plot, the solid line represents the aberration curve at wavelength λ of 193.3 nm, the broken line represents the aberration curve at wavelength λ of 193.3 nm+1 pm, and the chain line represents the aberration curve at wavelength λ of 193.3 nm−1 pm.

As can be seen from each aberration plot, the catadioptric optical systems C 1 and C 2 according to the first and second modes for carrying out the present invention achieve satisfactory aberration correction in a large exposure region. Accordingly, by incorporating catadioptric optical systems C 1 and C 2 into the projection exposure apparatus shown in FIG. 1 , for example, extremely fine patterns can be transferred onto the wafer.

The pupil plane of first imaging optical system A in systems C 1 and C 2 in the abovementioned modes for carrying out the present invention is positioned between concave reflecting mirror MC and first folding member M 1 . Thus, only positive lens L 124 in lens group G 12 and positive lens L 214 in lens group G 21 are formed of fluorite, and all other lenses are formed of synthetic quartz. By this construction, fluctuations in the image height direction in the optical performance in the image plane of catadioptric optical systems C 1 and C 2 can be ignored, for practical purposes, even if environmental factors, such as temperature, fluctuate. Furthermore, the fluorite lens in lens group G 112 is not limited to positive lens L 124 , and other positive lenses, whose number is not limited to one, may also be formed of fluorite. In addition, the fluorite lenses in lens group G 21 are also not limited to positive lens L 214 , and other lenses, whose number is not limited to one, may also be formed of fluorite.

The pupil plane of first imaging optical system A is preferably positioned between the first surface (reticle R) and concave reflecting mirror MC. Accordingly, all lenses that constitute lens group G 21 may be formed of synthetic quartz, and at least any one positive lens among the positive lenses in lens group G 22 may be formed of fluorite. By this construction, fluctuations in the image height direction in the optical performance in the image plane of catadioptric optical systems C 1 and C 2 can be ignored, for practical purposes, even if environmental factors, such as temperature, fluctuate.

In systems C 1 and C 2 , the two lens surfaces having negative refractive power that interpose aperture stop AS are aspherical surfaces. However, to further improve optical performance or to realize greater compactness and a reduction in the number of lenses, two or more lens surfaces may be formed in an aspherical surface shape.

Also, in systems C 1 and C 2 , the imaging performance can be microadjusted by adjusting, for a lens of at least any one lens group among lens group G 11 , lens group G 12 , lens group G 21 and lens group G 22 , the position in the optical axis direction, the position in a direction orthogonal to the optical axis, the position in the rotational direction about the optical axis, or the position in the rotational direction with the direction orthogonal to the optical axis as the axis.

Also, the atmosphere in lens barrel 20 of catadioptric optical system C of FIG. 1 may be replaced with a gas other than air (for example, nitrogen, helium and the like).

Next, the third mode for carrying out the present invention will be explained with reference to FIG. 8 and FIG. 11 and apparatus 200 . FIG. 8 is a cross-sectional view that shows the support structure of the catadioptric-type projection optical system used in the projection exposure apparatus of the third mode for carrying out the present invention. Furthermore, since projection optical system C 2 is used in the projection exposure apparatus according to the third mode for carrying out the present invention as set forth in Table 3and Table 4 above, a detailed explanation thereof is omitted.

In apparatus 200 of FIG. 8 , first imaging optical system A that forms an intermediate image of object plane R (mask surface) is housed in first lens barrel 201 , and second imaging optical system B that reimages this intermediate image (secondary image) in the image plane (wafer W surface) is housed in third lens barrel 203 .

First and second plane mirrors M 1 , M 2 serving as folding members for guiding the light from first imaging optical system A to the second imaging optical system B are housed in second lens barrel 202 . Therein, the optical axis (first optical axis Z 1 ) of the first imaging optical system is arranged in the vertical Z direction. Furthermore, first plane mirror M 1 arranged in the vicinity of the position at which the intermediate image is formed folds first optical axis Z 1 of the first imaging optical system by 90° and transforms it to second optical axis Z 2 extending horizontally in the Y direction. Second plane mirror M 2 is arranged along second optical axis Z 2 , and second optical axis Z 2 is further folded 90° by plane mirror M 2 and transformed to third optical axis Z 3 extending in the vertical Z direction. Plane mirrors M 1 , M 2 are mutually orthogonal and are held by second lens barrel 202 so that they both form an angle of 45° with respect to second optical axis Z 2 .

The support structure for supporting projection optical system C 2 as part of apparatus 200 is now explained, referring to FIGS. 9 a - 9 c , which are oblique views that shows lens barrels 201 - 203 . First lens barrel 201 holds first imaging optical system A and third lens barrel 203 holds the second imaging optical system. These lens barrels are formed substantially as cylinders. Second lens barrel 202 that holds plane mirrors M 1 , M 2 is formed substantially as a truncated pyramid. Furthermore, first lens barrel 201 is provided with opening 201 b , and part of second lens barrel 202 enters into opening 201 b when assembling the projection optical system.

FIG. 10 is an oblique view of the frame structure that supports lens barrels 201 - 203 . In FIG. 10 , lower frame 205 is formed as a plate and is provided with openings 205 a , 205 b through which first lens barrel 201 and third lens barrel 203 pass. Among these openings, at the perimeter of opening 205 a for the first lens barrel is provided in a standing state four main supports 206 a to 206 d , and upper frame 207 is affixed to the top surfaces of main supports 206 a to 206 d . Upper frame 207 is provided with U-shaped opening 207 a that supports first lens barrel 201 .

The upper part of first lens barrel 201 is provided with flange 201 a that protrudes sideways. First lens barrel 201 is supported by mounting the bottom surface of flange 201 a onto the peripheral top surface of U-shaped opening 207 a of upper frame 201 . Likewise, the lower part of third lens barrel 203 is provided with flange 203 a that protrudes sideways. Third lens barrel 203 is supported by mounting the bottom surface of flange 203 a onto the peripheral top surface of opening 205 b , for the third lens barrel, of lower frame 205 .

On the other hand, a pair of auxiliary supports 208 a , 208 b is formed in an inverted L shape and are affixed midway between first lens barrel opening 205 a and third lens barrel opening 205 b of lower frame 205 . Second lens barrel 202 is supported by these auxiliary supports 208 a , 208 b.

The frame of the exposure apparatus of the present working example as described above comprises lower frame 205 , main supports 206 a to 206 d , upper frame 207 and auxiliary supports 208 a , 208 b , and each of the lens barrels 201 , 202 , 203 are supported mutually independently by the frame.

Next, first lens barrel 201 is supported by the bottom surface of flange 201 a provided on first lens barrel 201 . The bottom surface of flange 201 a is located at a position wherein the spacing between the pattern surface of the reticle (object plane R) to the intermediate image is internally divided by a ratio of 1:(−βA). Here, βA is the imaging magnification of first imaging optical system A. Imaging magnification βA of first imaging optical system A according to the present working example shown in Table 1 and Table 2 above is substantially −1.25. Accordingly, as shown in FIG. 8 , the bottom surface of flange 201 a of first lens barrel 201 is located substantially at the midpoint of the distance from the reticle (object plane R) to the intermediate image, namely at a position 106 mm below object plane OP (horizontal plane through which point PA shown in FIG. 8 passes).

Third lens barrel 203 is supported by the bottom surface of flange 203 a provided on third lens barrel 203 . The bottom surface of flange 203 a is located at a position wherein the spacing from the intermediate image to the photosensitive surface of the wafer (image plane W) is internally divided by a ratio of 1:(−βB). Therein, βB is the imaging magnification of second imaging optical system B. Imaging magnification βB of second imaging optical system B according to the present working example shown in Table 1 and Table 2 above is substantially −0.20. Accordingly, as shown in FIG. 8 , the bottom surface of flange 203 a of third lens barrel 203 is located at the point wherein the distance from the intermediate image to image plane W is internally divided by a ratio of 1:0.20, namely at a position at a distance of 232 mm measured along the optical axis upward from image plane IP (horizontal plane through which point PB shown in FIG. 8 passes).

The operation of this construction is now briefly explained, referring to FIG. 11 . If h 0 is the object height for an arbitrary imaging optical system, y 0 is the image height and β is the lateral magnification, then:

β= y 0 /h 0.  (c)

Therein, the height of the object and the image are measured in the same direction. Accordingly, h 0 <0 and y 0 >0 in the example shown in FIG. 11 . In addition, since the specific configuration and arrangement position of the imaging optical system does not present a problem, only optical axis z 0 of the imaging optical system is shown in FIG. 11 .

If the imaging optical system is rotated by just microangle θ in the counterclockwise direction about point P on optical axis z 0 , the optical axis after rotation changes to Z 1 . Even if a light beam passes through a single lens two times as in a catadioptric system, object height h 1 and image height y 1 after rotation are as follows, wherein the axial distance measured from the object point to the image point is positive, the axial distance from the object point to center of rotation P is a, and the axial distance from the center of rotation P to the image point is b.

h 1 =h 0 + aθ   (d)

y 1 =y 0 − b 0  (e)

If the following relationship between object height h 1 and image height y 1 after rotation holds, then the image point does not deviate even after rotation of the imaging optical system.

y 1 /h 1 =β  (f)

The following condition is obtained based on conditions (c) to (f):

a:b= 1:(−β)  (g)

In other words, it can be seen that it is preferable to support the imaging optical system at point P, since the image point does not deviate even if the imaging optical system is rotated about a point (external dividing point when β is positive) wherein the object-image distance is internally divided by a ratio of 1:(−β).

The following explains the effect of the present working example. The degrees of freedom for a position that can be obtained in a three-dimensional object are the six degrees of freedom of the positions in the X, Y and Z directions and the angular positions about the X, Y and Z axes. Since first lens barrel 201 and third lens barrel 203 are separately supported by a frame at the bottom surfaces of flanges 201 a , 203 a , parallel movement in the vertical Z direction, parallel movement in the horizontal X and Y directions, and rotation about the vertical Z axis are difficult to produce in particular, the vertical Z axis is in the direction of optical axes Z 1 , Z 3 , and both first imaging optical system A and second imaging optical system B are formed symmetrically about optical axes Z 1 , Z 3 . Thus, no aberrations whatsoever are generated even if rotation about the vertical Z axis is produced.

Based on the above, the only motion that can be produced in first lens barrel 201 and third lens barrel 203 is rotational motion about the horizontal X and Y axes. Moreover, first lens barrel 201 is supported by a plane surface, wherein the object-image distance of first imaging optical system A supported by first lens barrel 201 is internally divided by a ratio of 1:(−βA). Third lens barrel 203 is also supported by a plane surface, wherein the object-image distance of second imaging optical system B to be supported by third lens barrel 203 is internally divided by a ratio of 1:(−βB). Consequently, the amount of image deviation produced is small, even if first lens barrel 201 or third lens barrel 203 is rotated about the horizontal X and Y axes.

In addition, image deviation caused by first lens barrel 201 and third lens barrel 203 is difficult to produce. Thus, it is clear that, if image deviation is produced, the cause thereof is due to one of the wafer stage, the reticle stage or second lens barrel 202 . In other words, specification of the cause of image deviation is simplified.

Next, although parallel movement of second lens barrel 202 in the vertical Z direction and parallel movement in the horizontal X and Y directions are difficult to produce, there is a risk of rotation about the X, Y and Z axes. If any one of these occurs, image deviation will be produced. However, even if first lens barrel 201 or third lens barrel 203 vibrates, that vibration is not transmitted and does not vibrate second lens barrel 202 , since second lens barrel 202 is directly held by the frame. Accordingly, if the stability of the frame is increased, the vibration of second lens barrel 202 can be sufficiently prevented.

The configuration of the present working example is effective even when assembling the projection optical system. To assemble projection optical system C 2 , as shown in FIG. 8 , lens barrels 201 to 203 are first assembled. At this point, lens barrels 201 to 203 are easy to assemble, since they have a single optical axis. Among these, first lens barrel 201 and third lens barrel 203 should be stacked so that optical axes Z 1 , Z 3 do not deviate from the optical members below. In addition, second lens barrel 202 should be assembled so that plane mirrors M 1 , M 2 form a right angle.

Next, to complete the assembly of projection optical system C 2 , first lens barrel 201 and third lens barrel 203 are first fitted on the frame shown in FIG. 10 . At this point, it may be difficult to make the positional relationship of both lens barrels 201 , 203 perfectly conform to the design data.

For deviations in the positional relationship between first lens barrel 201 and third lens barrel 203 , a deviation in height in the vertical Z direction, and a deviation in the interaxis distance in the horizontal Y direction is considered. Among these, if there is a deviation in height in the vertical Z direction between first lens barrel 201 and third lens barrel 203 , the total axial length from reticle R to the wafer W will deviate from the design data. In this case, the total length can be set in accordance with the design value by adjusting the height at which second lens barrel 202 is attached when fitting second lens barrel 202 to auxiliary supports 208 a , 208 b.

If there is a deviation in the interaxis distance between first lens barrel 201 and third lens barrel 203 , it can be absorbed by adjusting in the horizontal Y direction the position at which second lens barrel 202 is attached. Thus, by adjusting the position between each barrel, projection optical system C 2 can be assembled with ease in accordance with the design data.

In apparatus 200 of FIG. 8 , a plurality of optical members arrayed along first optical axis Z 1 are supported by one lens barrel 201 . Also, a plurality of optical members are arrayed along third optical axis Z 3 and are supported by one lens barrel 203 . At least one of first lens barrel 201 and third lens barrel 203 may have a split construction, namely at least one of first lens barrel 201 and third lens barrel 203 may comprise a plurality of lens barrels.

As discussed above, the third mode for carrying out the present invention can provide a catadioptric optical system that does not invite deterioration of the image and for which the assembly adjustment is easy.

The following explains the fourth mode for carrying out the present invention, using FIGS. 12 a , 12 b to FIGS. 14 a , 14 b . The fourth mode for carrying out the present invention relates to a support structure 300 of a catadioptric-type projection optical system used in a projection exposure apparatus. Furthermore, since the projection optical system used in the projection exposure apparatus according to the fourth mode for carrying out the present invention is catadioptric optical system C 2 described in Table 3 and Table 4, mentioned above, the explanation thereof is hereby omitted.

FIG. 12 a is an XY plan view of support structure 300 that supports system C 2 , and FIG. 12 b is a longitudinal cross-sectional view (YZ cross-sectional view) of the support structure.

Projection optical system C 2 of the fourth mode for carrying out the present invention shown in FIG. 12 has three optical axes Z 1 , Z 2 , Z 3 . First optical axis Z 1 is folded to second optical axis Z 2 by first plane mirror M 1 , and second optical axis Z 2 is folded back to third optical axis Z 3 by second plane mirror M 2 . In other words, first plane mirror M 1 is arranged so that it passes through the point of intersection of first optical axis Z 1 and second optical axis Z 2 , and second plane mirror M 2 is arranged so that it passes through the point of intersection of second optical axis Z 2 and third optical axis Z 3 .

As shown in FIG. 12 b , the optical members arranged on first optical axis Z 1 are held by first barrel 301 , and the optical members arranged on third optical axis Z 3 are held by third barrel 303 . In addition, first plane mirror M 1 and second plane mirror M 2 are held by a second barrel 302 .

At the time of projection and exposure, the light that passes through first barrel 301 is relayed through second barrel 302 , is conducted to third barrel 303 and reaches image plane IP. Second barrel 302 extends an arm from the vicinity of its center, and is directly affixed to a frame 305 so that second optical axis Z 2 is horizontal.

The following explains the assembly adjustment method of the projection optical system according to the fourth mode for carrying out the present invention.

First, since first to third barrels 301 to 303 are independent structures, they can each be assembled independently. In other words, since first barrel 301 and third barrel 303 do not include a plane mirror, and the lenses and concave reflecting mirror MC are merely lined up with respect to one of optical axes Z 1 , Z 3 , assembly can be performed with the same technique as that of a conventional dioptric system. On the other hand, since second barrel 302 holds plane mirrors M 1 , M 2 , and the number of parts to be held is small, assembly adjustment can be performed by using, for example, a three-dimensional measuring machine.

Next, the three barrels 301 to 303 are connected. Incidentally, if adjustments between the barrels are performed, deviations from the design values may arise. This error is not produced by conventional dioptric system lenses. This deviation between barrels can also be eliminated up to a certain amount by using various adjustment mechanisms of the type used in conventional dioptric systems. However, if the deviation between barrels is, for example, on the order of a millimeter, the adjustment stroke in conventional adjustment methods becomes inadequate, or the amount of residual high-order aberration unfortunately increases even if within the adjustment stroke. Therefore, the design performance can no longer be realized. Consequently, it is necessary to perform adjustments between barrels in advance up to the millimeter order. The following describes this procedure.

First, first barrel 301 and third barrel 303 are assembled into frame 305 . At this time, first barrel 301 and third barrel 303 are assembled so that they are as mutually parallel as possible. If optical axes Z 1 , Z 3 are perpendicular to the holding surface of frame 305 , it is preferable since subsequent adjustment becomes easier.

As can be seen from the design data, positional relationships in the predetermined design values exist between first barrel 301 and third barrel 303 , and it is necessary that these be satisfied on the micron order. However, it is extremely difficult to install an object of large size and heavy weight, like first and third barrels 301 , 303 , on a micron order from the outset. In addition, the inclination of first and third barrels 301 , 303 must also be on the order of a few seconds with respect to one another, and this too is difficult to realize with just the initial placement.

Accordingly, first barrel 301 or third barrel 303 may be provided with a movement and inclination adjustment mechanism. Even in this case, it is quite difficult to adjust on the order of microns large and heavy objects like first and third barrels 301 , 303 with them mounted on frame 305 as is. Consequently, a realistic procedure is one wherein first barrel 301 or third barrel 303 is first removed from frame 305 , frame 305 and the like are adjusted, and then first barrel 301 or third barrel 303 is reattached. Consequently, first and third barrels 301 , 303 , as shown in FIG. 12 b , are made removable in the working example by using kinematic joint 306 . It is therefore possible to remove first barrel 301 or third barrel 303 , adjust the thickness of the flange position, and then reattach the barrel.

However, in the present working example, if first and third barrels 301 , 303 are inclined and adjusted on the order of a few microns, then a deviation from the design value of the spacing between first and third barrels 301 , 303 , or a deviation from the design value of the height in the upward or, downward direction can be adjusted by moving second barrel 302 , if within the adjustment range of second barrel 302 . In other words, a deviation in the spacing between first and third barrels 301 , 303 and a deviation in height can be adjusted to an optical path length position equivalent to the design value by moving second barrel 302 vertically or horizontally.

As described above, if the optical members immediately after reticle R or immediately before wafer W are not included, and second barrel 302 having one or more folding members is provided with an adjustment mechanism, then an adjustment mechanism in the other barrels 301 , 303 may become unnecessary. Accordingly, in the present mode for carrying out the present invention, adjustment is performed using only the adjustment mechanism of second barrel 302 .

Next, second barrel 302 is also installed on frame 305 at a predetermined position. However, as mentioned above, the deviation in spacing and the deviation in height of first and third barrels 301 , 303 are premeasured, and the amounts of those deviations are added as an offset to the design value of second barrel 302 . Even if the above value is known, second barrel 302 is also quite large, and it is difficult to install with an accuracy on the order of microns and seconds from the ideal position on the first installation. Consequently, the positions between first to third barrels 301 to 303 are measured and, to correct these, second barrel 302 is provided with a translation and inclination mechanism.

In other words, as shown in the longitudinal cross-sectional view (YZ cross-sectional view) of second barrel 302 and frame 305 in FIG. 13 a , second barrel 302 is installed on frame 305 via washers 307 and balls 308 . Washers 307 function as an adjustment mechanism, and balls 308 function as a removal mechanism. In this case as well, it is difficult to make an adjustment on the order of microns with second barrel 302 mounted as is on frame 305 , as was shown with first and third barrels 301 , 303 . Consequently, a practical procedure is one wherein second barrel 302 is first removed, washers 307 are adjusted, and second barrel 302 is reattached. Thus, it is effective to attach a removal mechanism to second barrel 302 . In addition, second barrel 302 is the lightest barrel among the three barrels 301 , 302 , 303 shown in FIG. 12 b . Consequently, its removal and adjustment is the easiest. Thus, adjustment is easiest if an adjustment means is provided for adjusting the inclination and translation of the lightest barrel.

Next, optical adjustment is performed. This is carried out by performing a fine adjustment of the lens spacings, and by inclining (tilting) or moving (shifting) in a direction perpendicular to the optical axis one or a plurality of lenses. In this connection, the case of a catadioptric system is disclosed in, for example, U.S. Pat. No. 5,638,223. When performing optical adjustment of a catadioptric system, as disclosed in this reference, a mechanism is preferred that optically adjusts only the required optical element unit without affecting other optical element units as much as possible.

In accordance with this requirement in the present example, the optical elements of first barrel 301 are further distributed and housed in a plurality of lens barrel units 311 to 314 . Further, the optical elements of third barrel 303 are distributed and housed in a plurality of lens barrel units 331 to 333 , as shown in FIG. 12 b . Furthermore, each of lens barrel units 311 to 314 , 331 to 333 house one or more optical elements. These lens barrel units are provided with a mechanism that moves or inclines the lens barrel unit along the optical axis or in a direction orthogonal to the optical axis by making adjustments between the lens barrel units.

The following describes the optical adjustment procedure for this case. First, the amount of aberration of the lens is measured by a print test and the like. Based thereon, the amount of movement or inclination of the lens barrel unit is indicated. Based on that, lens barrel units 311 to 314 , 331 to 333 of first and third barrels 301 , 303 are moved. However, as can be seen from FIG. 12 b , it is nearly impossible to move lens barrel units 311 to 314 , 331 to 333 of first and third barrels 301 , 303 without removing second barrel 302 . Accordingly, since second barrel 302 is removable, as previously explained, second barrel 302 is removed and lens barrel units 311 to 314 , 331 to 333 in first and third barrels 301 , 303 are moved in accordance with the indicated value. In this case, if first and third barrels 301 , 303 are removable, first and third barrels 301 , 303 may be removed and adjusted on a separate adjustment bench. An aspect of this is shown in FIG. 13 b for the case of third barrel 303 .

FIG. 13 b is a longitudinal cross-sectional view (YZ cross-sectional view) of third barrel 303 . In FIG. 13 b , third barrel 303 is further internally divided into three lens barrel units 331 to 333 that include optical elements. In FIG. 13 b , uppermost part and lowermost part lens barrel units 331 , 333 are affixed, and middle lens barrel unit 332 is moved in the optical axis direction by replacing washers 307 , and is also moved in the direction orthogonal to the optical axis. After completing the adjustment, first and third barrels 301 , 303 are assembled and, lastly, second barrel 302 is returned to its original position.

By repeating the above optical adjustment one or more times, the lens performance approaches the design value.

Nevertheless, even if the above adjustment procedure is repeated, if second barrel 302 or the adjustment indication of first and third barrels 301 , 303 is reproduced, microscopic errors with respect to the indicated value inevitably arise. When adjusting aberrations due to these errors, it is inevitable with just the above adjustment procedure that second barrel 302 and first and third barrels 301 , 303 must be removable, which is extremely laborious. Consequently, it is preferable that this portion of the final aberration adjustment be able to be performed without removing the barrels. Furthermore, even after a lens is completed, for example, aberrations of the lens change microscopically due to mounting on the stage, movement when used as a product, and changes in the installation environment and the like. It is necessary to perform this portion of the aberration adjustment externally without removing any barrels.

Consequently, the present working example enables the adjustment of the five Seidel aberrations by changing at least five optical path lengths, as disclosed in Japanese Patent Application Kokai No. Hei 10-54932. Furthermore, decentered aberrations are made adjustable by providing a function that inclines at least five sets of lens elements or lens assemblies LA 1 to LA 5 , without externally affecting other optical members. A technique to tilt a lens element or lens group is disclosed in Japanese Patent Application Kokai No. Hei 10-133105. In this technique, a lens element near the reticle is tilted. However, although this mechanism is effective for a case like correcting distortion due to decentering, it is inadequate for correcting coma due to decentering. Moreover, the technique in Japanese Patent Application Kokai No. Hei 10-133105 is for a dioptric system, which is substantially different from the case wherein a catadioptric system lens is used, as in the present invention.

Lens assemblies LA 1 -LA 5 are preferable in that making the lens elements or lens assemblies coincide is efficient for changing the optical path length. The five lens elements or lens assemblies mentioned herein correspond to the five types of third order decentered aberrations as described in the reference by Yoshiya MATSUI, entitled “A Study of Third Order Aberrations in Optical Systems Wherein Decentering Exists,” 1990, Japan Optomechatronics Society, p. 5. Namely, these five aberrations include two types of decentered distortion, decentered astigmatism inclination of the image plane, and decentered coma. By using this optical path changing mechanism and decentered adjustment mechanism, performance the same as the design value can ultimately be realized. These five sets of lens elements or lens assemblies LA 1 to LA 5 are shown in FIG. 12 b . In this manner, the mechanism that tilts the lens elements or lens assemblies is extremely effective, particularly in a catadioptric system.

This adjustment mechanism is shown in FIGS. 14 a and 14 b . A variety of mechanical mechanisms can be considered with regard to this adjustment mechanism. FIG. 14 a shows a mechanism that translates and tilts the lens elements and lens assemblies. Three adjustment rods 341 protrude in the direction of 0°, 120°, and 240° from lens holder 340 , and a vertical drive mechanism 343 is attached to each of the three adjustment rods 341 , which pass through the side wall of lens barrel unit 342 . A piezoelectric device or ultrasonic motor can be used as vertical drive mechanism 343 .

In addition, FIG. 14 b shows a mechanism that tilts the lens elements or lens groups. Lens holder 340 is provided with X shafts 345 that extend in the +X direction and −X direction. X shafts 345 are pivoted by intermediate barrel 346 , provided with Y shafts 347 that extend in the +Y direction and −Y direction. Y shafts 347 are pivoted by lens barrel unit 342 , and rotational drive mechanisms 348 are attached to X shafts 345 and Y shafts 347 .

In this manner, it is essential that the catadioptric exposure apparatus having a plurality of optical axes have, as described above, a process that adjusts by an adjustment apparatus the mutual relationship between optical axes Z 1 , Z 2 , Z 3 for each of the barrels 301 - 303 , a process that positions each of the lens barrel units 311 to 314 , 331 to 333 , and a process that positions the simple lenses or lens assemblies LA 1 to LA 5 . Having the above adjustment processes is essential so that performance in accordance with the design values can ultimately be achieved.

By the adjustment mechanism and adjustment process according to the fourth mode for carrying out the present invention as explained above, a catadioptric projection exposure apparatus can be provided ultimately having optical performance substantially equal to the design value.

Next, the fifth mode for carrying out the present invention will be explained, referencing FIGS. 15 a and 15 b . The fifth mode for carrying out the present invention relates to a support method suitable for, for example, supporting second lens barrel 302 in the third mode for carrying out the present invention.

FIG. 15 a is an optical path diagram of a fifth embodiment of a projection optical system C 3 for carrying out the present invention. Projection optical system C 3 forms an intermediate image S of the pattern on reticle R located in object plane OP by first imaging optical system A. Intermediate image S is then imaged onto the photosensitive surface located in image plane IP of wafer W by second imaging optical system B. Furthermore, first imaging optical system A comprises a front group A 1 , and a rear group A 2 that constitutes a round-trip optical system. The optical specifications for the projection optical system shown in FIG. 15 a are those of system C 2 and are listed in Table 3 and Table 4 above. Furthermore, exposure region EA on wafer W is an oblong region (slit-shaped region) measuring 25 mm in the X direction and 6 mm in the Y direction, as shown in FIG. 15 b . FIG. 15 b is an enlarged view taken in the direction of the arrows along the line 15 b - 15 b in FIG. 15 a.

Plane mirrors M 1 , M 2 in the present working example are held by second lens barrel 302 as a single holding member. In other words, plane mirrors M 1 , M 2 are held as a single body. Second lens barrel 302 is supported from the front (+X direction) and from the rear (−X direction) by support members 308 a , 308 b that are provided in a standing condition on frame 305 , the same as in the third mode for carrying out the present invention discussed earlier.

In FIG. 15 a , if the point of intersection of first optical axis Z 1 and second optical axis Z 2 is assigned point P, then point P lies in a plane that includes the reflecting surface of first plane mirror M 1 . If the point of intersection of second optical axis Z 2 and third optical axis Z 3 is assigned point Q, then point Q lies in a plane that includes the reflecting surface of second plane mirror M 2 . Line segment PQ constitutes second optical axis Z 2 .

The midpoint of the positions where support members 308 a , 308 b , shown in FIG. 10 , support second lens barrel 302 is generally at a pivotal point G located 30 mm directly below a midpoint K of second optical axis Z 2 (namely, line segment PQ). Although support members 308 a , 308 b provide support so that no motion whatsoever arises in second lens barrel 302 , in actuality, there is a possibility that rotational motion will arise in second lens barrel 302 . This rotational motion is about the X axis, Y axis and Z axis through which pivotal point G passes.

In this manner, plane mirrors M 1 , M 2 are held as a single body, and the following describes the effectiveness of configuration wherein midpoint K or that vicinity of second optical axis Z 2 (line segment PQ) is set to pivotal point G. For comparative purposes, consider the case wherein plane mirrors M 1 , M 2 are supported separately, and examine the distortion of the image when first plane mirror M 1 is rotated, and the distortion in the image when second plane mirror M 2 is rotated. Then, examine the distortion of the image when both plane mirrors M 1 , M 2 are rotated as a single body, based on the construction of the present working example.

The amount of distortion of the image depends on how much center position IP 1 of exposure region EA and positions IP 2 to IP 5 at the four corners, as shown in FIG. 15 b , are moved before and after rotation of plane mirror M 1 . Accordingly, exposure region EA is an oblong shape measuring 25 mm×6 mm, as mentioned earlier, and center position IP 1 of exposure region EA in the image plane is at a position deviated from third optical axis Z 3 by 5+3=8 mm in the Y direction.

First, the results of the distortion of the image when first plane mirror M 1 is rotated independently will be explained. Let the hypothetical rotational motion be about the X axis, Y axis and Z axis through which pivotal point P passes, with the point of intersection P of first optical axis Z 1 and second optical axis Z 2 as the pivotal point. The direction of rotation and rotational angle is 3″ in the counterclockwise direction viewed from the +X direction, 3″ in the counterclockwise direction viewed from the +Y direction, and 3″ in the clockwise direction viewed from the +Z direction. Furthermore, pivotal point P is in the plane wherein the reflecting surface of first plane mirror M 1 extends. However, it is not the case that pivotal point P lies on the reflecting surface of first plane mirror M 1 itself because first imaging optical system A includes a round-trip optical system.

The image is deformed due to this rotational motion. Table 6 shows the amount of displacement of center position IP 1 of exposure region EA and four corners IP 2 to IP 5 of exposure region EA.

Furthermore, if first plane mirror M 1 is rotated, the position on the wafer surface of third optical axis Z 3 will also displaced. The contents of Table 6 show the remaining amount of displacement of points IP 1 to IP 5 when the post-displacement position of third optical axis Z 3 is drawn back so that it superposes the pre-displacement position of third optical axis Z 3 .

Likewise, Table 7 shows the distortion of the image when second plane mirror M 2 is rotated independently. The pivotal point is the point of intersection Q of second optical axis Z 2 and third optical axis Z 3 , and the other conditions are the same as described above.

Likewise, Table 8 shows the distortion of the image when both plane mirrors M 1 , M 2 are rotated as a single body. The pivotal point is point G, which lies 30 mm directly below midpoint K of second optical axis Z 2 (line segment PQ), and the other conditions are the same as described above. The unit of displacement amounts dX, dY shown in Table 6 to Table 8 is nm.

TABLE 6
COMPARATIVE EXAMPLE:
ROTATION ONLY OF FIRST PLANE MIRROR M1
	Rotation		Rotation		Rotation
	About X Axis		About Y Axis		About Z Axis
	dX	dY	dX	dY	dX	dY
IP1	0	−14	−106.7	0	106.7	0
IP2	73.2	19.2	−159.7	−145.3	159.7	145.2
IP3	32.9	41.5	−86.5	−165.4	86.5	165.3
IP4	−73.1	19.2	−159.8	145.2	159.7	−145.3
IP5	−32.9	41.5	−86.5	165.3	86.5	−165.4

TABLE 7
COMPARATIVE EXAMPLE:
ROTATION ONLY OF SECOND PLANE MIRROR M1
	Rotation		Rotation	Rotation
	About X Axis		About Y Axis	About Z Axis
	dX	dY	dX	dY	dX	dY
IP1	0	−7.7	124.8	0	−124.8	0
IP2	−19.9	−56.1	185.5	191.7	−185.5	−191.7
IP3	−9.1	−44.3	85.5	186.3	−85.4	−186.3
IP4	19.9	−56.1	185.5	−191.7	−185.5	191.7
IP5	9.1	−44.3	85.4	−186.3	−85.5	186.3

TABLE 8
PRESENT WORKING EXAMPLE:
FIRST AND SECOND PLANE MIRRORS M1, M2
ROTATED AS A SINGLE BODY
	Rotation		Rotation	Rotation
	About X Axis		About Y Axis	About Z Axis
	dX	dY	dX	dY	dX	dY
IP1	0	−10.9	18.1	0	231.5	−0.1
IP2	26.7	−18.4	25.7	46.5	345.3	336.9
IP3	12	−1.4	−1.1	21	172.1	351.6
IP4	−26.7	−18.4	25.8	−46.4	345.1	−337
IP5	−12	−1.4	−1	−20.9	171.9	−351.7

As shown in Table 6 to Table 8 above, distortion of the image arises when the target member is rotated about the X axis. In addition, rotation of the image arises if the target member is rotated about the Y axis or if rotated about the Z axis. Among these, consider first rotation about the X axis. It can be seen that distortion of the image in the present working example (example of Table 8, Rotation About X Axis) is smaller than independent rotation of first plane mirror M 1 (example of Table 6, Rotation About X Axis) and independent rotation of second plane mirror M 2 (example of Table 7, Rotation About X Axis). In other words, since image distortion when first plane mirror M 1 is independently rotated and image distortion when second plane mirror M 2 is independently rotated tend to be in substantially the reverse directions, they are both canceled. Image distortion is thereby reduced in the present working example. This is because nearly no deviation occurs in the ray with respect to the ideal position and the amount of aberration generated is small, since the two optical axes Z 1 , Z 3 do not mutually deviate even if plane mirrors M 1 , M 2 deviate at the same angle.

For the case where plane mirrors M 1 , M 2 are held as a single body, it is preferable to make the pivotal point midpoint K of second optical axis Z 2 (line segment PQ). This is because, if the pivotal point is at midpoint K of second optical axis Z 2 (line segment PQ), the axial distance from reticle R to wafer W does not change even if the holding member through which the pivotal point passes is rotated about the X axis. Therefore, almost no rotationally symmetric aberrations or magnification deviation occurs.

On that basis, it is preferable that distance KG between midpoint K of second optical axis Z 2 (line segment PQ) and pivotal point G be small and, generally, it is preferable that it be within 0.2 times length PQ of second optical axis Z 2 , or:

KG≦ 0.2 ×PQ.   (5)

Condition (5) is satisfied in the present working example, since KG=30 mm and PQ=530 mm.

With continuing reference to FIG. 15 a , pivotal point G is inside a holding member (e.g., barrel 302 ). The holding member can only provide support at an external surface thereof. Accordingly, a realistic support position for the holding member is in the vicinity of the plane that passes through midpoint K of second optical axis Z 2 and is orthogonal to second optical axis Z 2 .

Now considered is rotation about the Y axis. It can be seen that rotation of the image in the present working example (example of Table 8, Rotation About Y Axis) is smaller than independent rotation of first plane mirror M 1 (example of Table 6, Rotation About Y Axis) and independent rotation of second plane mirror M 2 (example of Table 7, Rotation About Y Axis). In other words, since rotation of the image when first plane mirror M 1 is independently rotated and rotation of the image when second plane mirror M 2 is independently rotated tend to be in substantially the reverse directions, both are canceled and rotation of the image is reduced in the present working example.

Now considered is rotation about the Z axis. Rotation of the image is unfortunately generated to a great extent in the present working example (example of Table 8, Rotation About Z Axis) compared with independent rotation of first plane mirror M 1 (example of Table 6, Rotation About Z Axis) and independent rotation of second plane mirror M 2 (example of Table 7, Rotation About Z Axis).

However, since lens barrel 302 that holds plane mirrors M 1 , M 2 as a single body has its direction of length in the Y direction, the amount of rotation about the Z axis (and amount of rotation about the X axis) can be easily controlled by strengthening support member 300 at the edge of the length direction of holding member H, and the like. Furthermore, since the direction of gravity is in the direction of the Z axis, the gravity balance of holding member H is not disturbed even if rotation about the Z axis occurs. Accordingly, based also on this point, the amount of rotation about the Z axis can be easily controlled.

As can be seen from the present working example, if the folding member is a surface reflecting mirror, holding is comparatively easy. In contrast, if an element like a beam splitter is included, it is unpreferable since the weight of the holding member increases and support of the holding member becomes comparatively difficult.

Furthermore, although second lens barrel 302 as a holding member supports only folding members M 1 , M 2 in the fifth mode for carrying out the present invention, a lens (not shown in FIG. 15 a ) as a dioptric optical member may also be interposed between folding members M 1 , M 2 held by second lens barrel 302 . An example of such a case will be explained, referencing FIG. 16 .

With reference now to FIG. 16 a , which is an optical path diagram of the projection optical system C 4 according to the sixth mode for carrying out the present invention, the principal points of difference from the projection optical system C 3 of FIG. 15 mentioned earlier are that a lens L is arranged between plane mirrors M 1 , M 2 , and that the glass material of all lenses is quartz glass.

The following lists the principal specifications of projection optical system C 4 according to the sixth mode for carrying out the present invention.

N.A. on wafer side: 0.65

Magnification: 0.25×

Working wavelength: 193.3 nm (ArF excimer laser)

Exposure region EA is an oblong region measuring 25 mm in the longitudinal X direction and 8 mm in the horizontal Y direction, as shown in FIG. 16 b.

Table 9 and Table 10 below list the specifications of the optical members projection optical system C 4 according to the sixth mode for carrying out the present invention. Since the glass material of all lenses is quartz, such is omitted from Table 9. In addition, an optical surface to which an asterisk (*) is appended to the surface number in Table 9 indicates an aspherical surface, and the radius of curvature for aspherical surfaces in Table 9 indicates the vertex radius of curvature. The aspherical surface shape is represented by condition (a), above. For each aspherical surface, the conical coefficient κ is 0, and E and F among the aspherical coefficients are 0. Consequently, the aspherical surface data for Table 10 is not listed.

TABLE 9
SIXTH MODE FOR CARRYING OUT THE PRESENT INVENTION
S	R	d	Re	Material
0	∞	52.5105		R
1	567.1430	40.1245	84.49	A1
2	3470.8704	2.2743	86.20
3	12580.6849	29.5354	86.34	A1
4	919.5973	2.0000	88.19
5	355.8404	35.8420	89.51	A1
6	645.8193	78.2133	89.37
7	523.4723	23.5558	95.17	A2
8	−1724.9806	14.1444	94.91
9	−544.7152	22.0000	94.37	A2
10	−996.4488	0.5000	94.96
11	222.1244	22.0000	94.48	A2
12	285.0673	270.9667	91.66
13	−448.3590	20.0001	69.82	A2
14	483.2437	7.1773	69.86
15	450.0000	27.4588	73.46	A2
16	−581.8071	98.1108	77.12
17	−164.5653	25.0000	97.01	A2
18	−686.3758	18.1361	116.87
19	−274.4169	−18.1361	117.82	A2	MC
20	−686.3758	−25.0000	117.22	A2
21	−164.5653	−98.1108	102.36
22	−581.8071	−27.4588	99.27	A2
23	450.0000	−7.1773	98.55
24	483.2437	−20.0001	96.16	A2
25	−448.3590	−270.9667	92.30
26	285.0673	−22.0000	83.28	A2
27	222.1244	−0.5000	84.79
28	−996.4488	−22.0000	82.76	A2
29	−544.7152	−14.1444	80.48
30	−1724.9806	−23.5558	79.87	A2
31	523.4723	−0.5000	78.99
32	∞	255.9374		M1
33	604.6543	31.2039	116.51	B	L
34	−787.6549	200.0000	116.86
35	∞	−152.7463		M2
36	−445.7714	−30.0000	103.97	B
37	−10477.3479	−0.5000	102.01
38*	−704.6939	−24.4152	101.24	B
39	−217.6002	−46.6658	96.30
40	−262.5805	−32.4068	100.37	B
41	−1345.5908	−82.6445	98.92
42	—	−47.7302	91.14	AS
43	−313.2008	−39.4658	97.58	B
44	584.6659	−0.8283	97.17
45	−473.1823	−27.4850	94.61	B
46	487.4609	−8.0932	93.17
47	304.5680	−25.0000	92.05	B
48*	1295.3943	−0.6535	87.95
49	−210.3586	−42.6899	84.21	B
50	−716.6193	−4.1246	76.28
51	−240.1793	−60.0000	72.13	B
52	1038.2875	−1.1901	55.47
53	−280.1800	−40.0000	50.65	B
54	−2803.1853	−18.2145	34.10
55	∞			W

TABLE 10
ASPHERICAL DATA OF THE SIXTH MODE FOR
CARRYING OUT THE PRESENT INVENTION
38                                                                        th                                                                     Surface
A = 2.1892 × 10                                                                        −8
B = 2.7825 × 10                                                                        −13
C = 1.4089 × 10                                                                        −18
D = −6.4967 × 10                                                                        −23
48                                                                        th                                                                     Surface
A = −1.3381 × 10                                                                        −8
B = −4.2757 × 10                                                                        −13
C = 4.5484 × 10                                                                        −18
D = −2.4978 × 10                                                                        −22

For comparative purposes, as in system C 3 of FIGS. 15 a and 15 b , consider the case wherein plane mirrors M 1 , M 2 are separately supported, and examine the distortion of the image when first plane mirror M 1 is rotated and the distortion of the image when second plane mirror M 2 is rotated. Subsequently, next examined is the distortion of the image when plane mirrors M 1 , M 2 are rotated as a single body, based on the configuration of the present working example.

Table 11 shows the distortion of the image when first plane mirror M 1 is independently rotated. The pivotal point is the point of intersection P of first optical axis Z 1 and second optical axis Z 2 , and other conditions are the same as those in the fifth mode for carrying out the present invention.

Table 12 shows the distortion of the image when second plane mirror M 2 is independently rotated. The pivotal point is the point of intersection Q of second optical axis Z 2 and third optical axis Z 3 , and other conditions are the same as those above.

Table 13 shows the distortion of the image when plane mirrors M 1 , M 2 are rotated as a single body. The pivotal point is point G located +50 mm in the Z direction and −10 mm in the Y direction from midpoint K of second optical axis Z 2 (line segment PQ), and other conditions are the same as those above. Furthermore,

KG =[50 2 +(−10) 2 ] ½ =51

and since PQ is 487 mm, condition (5) is satisfied.

TABLE 11
COMPARATIVE EXAMPLE:
ROTATION ONLY OF FIRST PLANE MIRROR M1
	Rotation		Rotation	Rotation
	About X Axis		About Y Axis	About Z Axis
	dX	dY	dX	dY	dX	dY
IP1	0	−9.8	−120.1	0	120.1	0
IP2	63.4	20.4	−176.2	−150.2	176.3	150.1
IP3	24.3	38.4	−78.8	−169.7	78.9	169.7
IP4	−63.4	20.4	−176.3	150.1	176.2	−150.2
IP5	−24.3	38.4	−78.9	169.7	78.8	−169.7

TABLE 12
COMPARATIVE EXAMPLE:
ROTATION ONLY OF SECOND PLANE MIRROR M2
	Rotation		Rotation	Rotation
	About X Axis		About Y Axis	About Z Axis
	dX	dY	dX	dY	dX	dY
IP1	0	0.9	139.8	0	−139.8	0
IP2	−38.4	−32.3	206.8	201	−206.7	−210
IP3	−14.7	−34.3	74.5	189.1	−74.5	−189.1
IP4	38.4	−32.3	206.7	−201	−206.8	201
IP5	14.7	−34.3	74.5	−189.1	−74.5	189.1

TABLE 13
PRESENT WORKING EXAMPLE:
FIRST AND SECOND PLANE MIRRORS M1, M2 ROTATED
AS A SINGLE BODY
	Rotation		Rotation	Rotation
	About X Axis		About Y Axis	About Z Axis
	dX	dY	dX	dY	dX	dY
IP1	0	−31	19.7	0	259.9	−0.1
IP2	49.4	−44.1	30.6	50.8	390.6	343.2
IP3	41.8	−12.6	−4.2	19.4	160.9	355.8
IP4	−49.4	−44.1	30.3	−50.8	390.4	−343.4
IP5	−41.8	−12.6	−4.5	−19.4	160.7	−355.9

As shown in Table 11 to Table 13 above, distortion of the image arises when the target member is rotated about the X axis. Rotation of the image arises if the target member is rotated about the Y axis or if rotated about the Z axis. Among these, first considered is rotation about the X axis. Substantially the same amount of image distortion is generated in the present working example (example of Table 13, Rotation About X Axis) as with independent rotation of first plane mirror M 1 (example of Table 11, Rotation About X Axis) and with independent rotation of second plane mirror M 2 (example of Table 12, Rotation About X Axis). This is because, since lens L is interposed between plane mirrors M 1 , M 2 , rays reflected by first plane mirror M 1 are deviated by passing through lens L and subsequently impinge on second plane mirror M 2 . Consequently, aberrations are generated since the effect wherein the optical axis is undeviated is unfortunately lost.

The length direction of second lens barrel 302 is the Y direction, as mentioned previously. Hence, the amount of rotation about the X axis can be easily controlled by reinforcing the support member at the edge of the length direction of second lens barrel 302 , and the like. Nevertheless, if holding plane mirrors M 1 , M 2 , which form a right angle as a single body, it is preferable that lens L not be provided therebetween. Even in the case where lens L is arranged, it is preferable to limit such to two members.

Next, consider rotation about the Y axis. It can be seen that rotation of the image in the present working example (example of Table 13, Rotation About Y Axis) is smaller than independent rotation of first plane mirror M 1 (example of Table 11, Rotation About Y Axis) and independent rotation of second plane mirror M 2 (example of Table 12, Rotation About Y Axis). In other words, since rotation of the image when first plane mirror M 1 is independently rotated and rotation of the image when second plane mirror M 2 is independently rotated tend to be in substantially the reverse directions, they are both canceled, and rotation of the image is thereby reduced in the present working example.

Next, consider rotation about the Z axis. A large rotation of image is generated in the present working example (example of Table 13, Rotation About Z Axis) compared with independent rotation of first plane mirror M 1 (example of Table 11, Rotation About Z Axis) and independent rotation of second plane mirror M 2 (example of Table 12, Rotation About Z Axis). However, as discussed above, the amount of rotation about the Z axis can be controlled easily.

As explained above, the fifth and sixth modes for carrying out the present invention reduce the amount of image distortion generated by rotation of the folding member and, accordingly, can obtain a stabilized high resolution.

Next, the seventh mode for carrying out the present invention will be explained, referencing FIG. 17 to FIGS. 19 and 19 b.

FIG. 17 shows a schematic of the configuration of a projection optical system 400 for implementing the alignment method and manufacturing method according to the seventh mode for carrying out the present invention. The seventh mode for carrying out the present invention is related to a relative alignment method between a plurality of lens barrel axes and folding members in a catadioptric-type projection optical system having two folding members, and a manufacturing method for a projection optical system (optical system having folding members) that uses this alignment method.

In FIG. 17 , the Z axis is set parallel to optical axis Z 1 of first imaging optical system A, the Y axis is set parallel to the paper surface of FIG. 17 in a plane perpendicular to the Z axis, and the X axis is set perpendicular to the paper surface of FIG. 17 in a plane perpendicular to the Z axis. Furthermore, the YZ plane, which is the paper surface of FIG. 17 , is a plane that includes optical axis Z 1 of first imaging optical system A and optical axis Z 3 of second imaging optical system B.

Projection optical system 400 in FIG. 17 is provided with first imaging optical system A to form the intermediate image of the pattern based on the light from mask R, whereon a fine circuit pattern, for example, is formed. Second imaging optical system B to form a reduced image of the pattern onto wafer W, which is a photosensitive substrate, based on the light from the intermediate image. First folding mirror M 1 arranged in the vicinity of the position where the intermediate image is formed, and to fold in the +Y direction the light that passes through first imaging optical system A. Second folding mirror M 2 is provided to fold the light from first folding mirror M 1 in the +Z direction toward second imaging optical system B.

First imaging optical system A comprises, in order from reticle R, three lens components L 1 to L 3 and concave reflecting mirror MC, shown by solid lines in the drawing. Furthermore, each of lens components L 1 to L 3 and concave reflecting mirror MC is arrayed inside cylindrical first lens barrel 401 along one optical axis Z 1 parallel to the Z axis. Namely, optical axis Z 1 of first imaging optical system A and the axis of first lens barrel 401 coincide.

On the other hand, second imaging optical system B comprises, in order from reticle R (namely, the second folding mirror side), five lens components L 4 to L 8 , as shown by solid lines in the drawing. Furthermore, each of the lens components L 4 to L 8 is arrayed inside cylindrical second lens barrel 403 along one optical axis Z 3 parallel to the Z axis. In other words, optical axis Z 3 of second imaging optical system B and the axis of second lens barrel 403 coincide. In addition, optical axis Z 3 of second imaging optical system B and optical axis Z 1 of first imaging optical system A are mutually parallel.

Furthermore, first folding mirror M 1 and second folding mirror M 2 arranged in the optical path between first imaging optical system A and second imaging optical system B have reflecting surfaces inclined by just 45° with respect to optical axis Z 1 and optical axis Z 3 so that they are mutually opposing and so that they are orthogonal to the YZ plane (paper surface of FIG. 17 ) that includes optical axis Z 1 of first imaging optical system A and optical axis Z 3 of second imaging optical system B. In other words, the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 are mutually orthogonal, and the line of intersection formed extending along the two reflecting surfaces is parallel to the X axis. First folding mirror M 1 and second folding mirror M 2 are attached to a support body 402 .

Thus, projection optical system 400 is a catadioptric-type optical system having two folding mirrors M 1 , M 2 , and has two lens barrels 401 , 403 having different axes. According to another viewpoint, projection optical system 400 has three different optical axes, namely optical axis Z 1 of first imaging optical system A, optical axis Z 3 of second imaging optical system B, and third optical axis Z 2 parallel to the Y axis. In the present mode for carrying out the present invention, optical axis Z 2 is defined as the tracing of a ray entering along optical axis Z 1 to the reflecting surface of first folding mirror M 1 (strictly speaking, the extended surface of the effective reflecting region) aligned at a predetermined position. In addition, optical axis Z 2 is likewise defined as the tracing of a ray entering along optical axis Z 3 to the reflecting surface of second folding mirror M 2 aligned at a predetermined position.

In projection optical system 400 , the light from the pattern region decentered from optical axis Z 1 in the −Y direction on reticle R positioned parallel to the XY plane is reflected by concave reflecting mirror MC via each of the lens components L 1 to L 3 that constitute first imaging optical system A. The latter then forms an intermediate image via each of the lens components L 3 to L 1 . The light from the intermediate image is reflected in the +Y direction by the reflecting surface of first folding mirror M 1 , is then reflected in the +Z direction by the reflecting surface of second folding mirror M 2 and is then guided to second imaging optical system B. The light guided to second imaging optical system B passes through each of the lens components L 4 to LE and then forms a reduced image of the mask pattern in the exposure region, decentered from optical axis Z 3 in the +Y direction, on wafer W positioned parallel to the XY plane.

In projection optical system 400 , as well as in the above mode for carrying out the present invention, first lens barrel 401 and second lens barrel 403 can be positioned with high precision so that the axis of first lens barrel 401 and the axis of second lens barrel 403 are mutually parallel and spaced apart by a predetermined spacing. In addition, first and second folding mirrors M 1 , M 2 can be positioned with high precision with respect to support member 402 so that their reflecting surfaces are mutually orthogonal. Furthermore, the positioning of first and second folding mirrors M 1 , M 2 is discussed later.

As discussed earlier, when positioning each of the optical members L 1 to L 3 , MC with respect to first lens barrel 401 , the axis of first lens barrel 401 and the optical axes of each of the optical members L 1 to L 3 , MC of first imaging optical system A can be made to coincide with an accuracy in units of microns. Likewise, when positioning each of the optical members L 4 to L 8 with respect to second lens barrel 403 , the axis of second lens barrel 403 and the optical axes of each of the optical members L 4 to L 8 of second imaging optical system B can be made to coincide with an accuracy in units of microns.

Accordingly, to position each of the optical members L 1 to L 8 , MC, M 1 , M 2 with high precision when manufacturing projection optical system 400 , it is necessary to align the relative positions of folding mirrors M 1 , M 2 and the two optical axes Z 1 , Z 3 with high precision. In other words, the relative positions of first lens barrel 401 having an axis coincident with optical axis Z 1 , second lens barrel 403 having an axis coincident with optical axis Z 3 , and folding mirrors M 1 , M 2 must be aligned with high precision. Specifically, folding mirrors M 1 , M 2 must be aligned with high precision with respect to the two lens barrels 401 , 403 so that, for example, the distance along optical axes Z 1 , Z 2 , Z 3 from reference point RA, which is the center of first lens barrel 401 , to reference point RB, which is the center of second lens barrel 403 , is a predetermined length.

FIG. 18 a is a view that corresponds to FIG. 17 , and is a drawing for explaining the alignment method of the seventh mode for carrying out the present invention.

FIG. 18 a shows first lens barrel 401 and second lens barrel 403 already positioned with high precision. In the present mode for carrying out the present invention, folding mirrors M 1 , M 2 are aligned with high precision with respect to first lens barrel 401 and second lens barrel 403 when manufacturing the projection optical system. Subsequently, the other optical members are positioned with respect to first lens barrel 401 and second lens barrel 403 . Furthermore, the X axis, Y axis and Z axis in FIG. 18 a are set in the same manner as in FIG. 17 .

In the alignment method of the present working example, a concave reflecting mirror MO having a reflecting surface MS 1 is attached at a predetermined position inside first lens barrel 401 so that the optical axis thereof coincides with the axis of first lens barrel 401 (and in turn, optical axis Z 1 ), as shown in FIG. 18 a . Accordingly, reflecting surface MS 1 is formed as an aspherical surface and, in a state wherein concave reflecting mirror MO is attached to first lens barrel 401 , faces the first folding mirror side.

As shown in FIG. 18 a , a lens group FL as the optical element for adjustment is attached at a predetermined position inside second lens barrel 403 so that the optical axis thereof coincides with the axis of second lens barrel 403 (and in turn, optical axis Z 3 ). The lens surface most on the second folding mirror side of lens group FL in a state wherein it is attached to second lens barrel 403 constitutes a reference surface BS 11 as the Fizeau reference surface.

Techniques to make the optical axis of concave reflecting mirror MO and the axis of first lens barrel 401 , as well as the optical axis of lens group FL and the axis of second lens barrel 403 coincide with an accuracy in units of microns, are widely known. In addition, radius of curvature R of reflecting surface MS 1 , and distance F along the optical axis from the focal point on the reference surface BS 1 side of lens group FL to reference surface BS 1 can be accurately premeasured in accordance with the prior art. Furthermore, distance 430 a along the optical axis from reference point RA to reflecting surface MS 1 , and distance 430 b along the optical axis from reference point RB to reference surface BS 1 can also be accurately measured based on prior art using, for example, a digital micrometer and the like.

In the present working example, concave reflecting mirror MO and lens group FL are respectively positioned with respect to first lens barrel 401 and second lens barrel 403 so that the relationship shown in condition (h) below holds.

LD=430 a +430 b+R+F.   (h)

Therein, LD is the design distance (distance specified based on the design) along the optical axis from reference point RA to reference point RB.

Accordingly, in the state wherein folding mirrors M 1 , M 2 are accurately aligned with respect to first lens barrel 401 and second lens barrel 403 , the focal point of concave reflecting mirror MO (namely, the point removed by just radius of curvature R along the optical axis from reflecting surface MS 1 ) and the focal point of lens group FL (namely, the point removed by just distance F along the optical axis from reference surface BS 1 ) coincide. In other words, if a parallel light beam parallel to optical axis Z 3 on the wafer side of lens group FL is guided to lens group FL in this state, the light beam that passes through lens group FL and second folding mirror M 2 converges at point 424 on optical axis Z 2 (namely, the focal point of lens group FL and the focal point of concave reflecting mirror MO). The divergent light beam from convergent point 424 passes through first folding mirror M 1 and perpendicularly impinges upon concave reflecting mirror MO. The light beam reflected by reflecting surface MS 1 of concave reflecting mirror MO reconverges at point 424 via first folding mirror M 1 along an optical path completely the same as the going path, and then changes to a parallel light beam parallel to optical axis Z 3 via second folding mirror M 2 and lens group FL.

In other words, in the state wherein folding mirrors M 1 , M 2 are accurately aligned with respect to first lens barrel 401 and second lens barrel 403 , a predetermined interference fringe is obtained between the first light beam that returns after being reflected by reference surface BS 1 without transmitting through reference surface BS 1 of lens group FL and the second light beam that returns after transmitting through reference surface BS 1 of lens group FL and being reflected by concave reflecting mirror MO. Accordingly, in the present working example, folding mirrors M 1 , M 2 are aligned with respect to first lens barrel 401 and second lens barrel 403 based on the interference between the first light beam and the second light beam mentioned above. The following explains the detection of the interference between the first light beam and the second light beam, and the alignment of folding mirrors M 1 , M 2 .

First, the detection of the interference between the first light beam and the second light beam will be explained.

With continuing reference to FIG. 18 a , parallel light supplied from interferometer 421 passes through opening 422 formed in second lens barrel 403 , and is guided to the inside of second lens barrel 403 . The parallel light beam guided to the inside of second lens barrel 403 is folded in the −Z direction by reflecting mirror 423 attached to the inside of second lens barrel 403 , and enters lens group FL unchanged as parallel light. To make the convergent point of the parallel light beam that entered lens group FL coincident with the focal point of lens group FL (point on optical axis Z 2 ), the parallel light beam parallel to optical axis Z 3 must enter lens group FL. Accordingly, in addition to providing interferometer 421 with a function to detect the interference between the first light beam and the second light beam, it is provided with an adjustment function that injects into lens group FL the parallel light beam parallel to optical axis Z 3 .

FIG. 18 b shows the internal construction of interferometer 421 shown in FIG. 18 a . As shown in FIG. 18 b , interferometer 421 is provided with laser light source 431 that supplies coherent parallel light. First, when performing the incident adjustment of the parallel light beam, the light supplied from laser light source 431 is reflected in the −Z direction by beam splitter 432 , and then impinges on adjustment reflecting mirror 433 rotatable about two axes. The light reflected in the −Y direction by adjustment reflecting mirror 433 enters lens group FL (not shown in FIG. 18 b ) via opening 422 formed in second lens barrel 403 and via reflecting mirror 423 . The light reflected by reference surface BS 1 of lens group FL impinges on beam splitter 432 via reflecting mirror 423 and adjustment reflecting mirror 433 . The reflected light from reference surface BS 1 that impinges on beam splitter 432 is transmitted through beam splitter 432 , and then impinges on detector 434 . Furthermore, the light that transmitted through reference surface BS 1 of lens group FL is shaded by a shutter (not shown) installed in the optical path between, for example, lens group FL and second folding mirror M 2 .

Of the light supplied from laser light source 431 , the light transmitted through beam splitter 432 passes through shutter 435 and then perpendicularly impinges on reflecting mirror 136 . The light reflected by reflecting mirror 436 impinges on beam splitter 432 via shutter 435 . The reflected light from reflecting mirror 436 that impinged on beam splitter 432 is reflected by beam splitter 432 and then impinges on detector 434 . Thus, the interference fringe between the reflected light from reference surface BS 1 and the reflected light from reflecting mirror 436 that functions as a Twyman mirror is detected at detector 434 .

If the parallel light beam parallel to optical axis Z 3 enters lens group FL, the parallel light beam perpendicularly impinges on reference surface BS 1 of lens group FL. As a result, a predetermined interference fringe is detected in detector 434 between the reflected light from reference surface BS 1 and the reflected light from reflecting mirror 436 . By rotationally jogging adjustment reflecting mirror 433 based on the interference fringe detected in detector 434 , the parallel light beam parallel to optical axis Z 3 can be injected into lens group FL. In this manner, after performing the incident adjustment of the parallel light beam with respect to lens group FL, the interference between the first light beam and the second light beam is detected in a state wherein shutter 435 is closed.

In other words, when detecting the interference between the first light beam and the second light beam, the light supplied from laser light source 131 is reflected in the +Z direction by beam splitter 432 and then enters lens group FL via adjustment reflecting mirror 433 and reflecting mirror 123 . The first light beam reflected by reference surface BS 1 of lens group FL impinges on beam splitter 432 via reflecting mirror 123 and adjustment reflecting mirror 433 . The first light beam, which is the reflected light from reference surface BS 1 that impinged on beam splitter 432 , is transmitted through beam splitter 432 and then impinges on detector 434 .

Referring once again to FIG. 18A , the second light beam transmitted through reference surface BS 1 of lens group FL is reflected by second folding mirror M 2 , converges once and impinges on concave reflecting mirror MO via first folding mirror M 1 . The second light beam reflected by reflecting surface MS 1 of concave reflecting mirror MO converges once via first folding mirror M 1 , and then enters lens group FL via second folding mirror M 2 . The second light beam that enters lens group FL impinges on beam splitter 432 via reflecting mirror 123 and adjustment reflecting mirror 433 . The second light beam, which is the reflected light from reflecting surface MS 1 of concave reflecting mirror MO that impinged on beam splitter 432 , is transmitted through beam splitter 432 , and then impinges on detector 434 . Thus, the interference fringe between the first light beam, which is the reflected light from reference surface BS 1 as the Fizeau reference surface, and the second light beam, which is the reflected light from reflecting surface MS 1 , is detected at detector 434 .

As discussed earlier, the focal point of concave reflecting mirror MO and the focal point of lens group FL coincide, in the state wherein folding mirrors M 1 , M 2 are accurately aligned with respect to first lens barrel 401 and second lens barrel 403 . Thus, the parallel light beam perpendicularly impinges reflecting surface MS 1 of concave reflecting mirror MO. As a result, a predetermined interference fringe between the reflected light from reference surface BS 1 and the reflected light from concave reflecting mirror MO is detected in detector 434 . In other words, by jogging folding mirrors M 1 , M 2 with respect to first lens barrel 401 and second lens barrel 403 based on the interference fringe detected in detector 434 , folding mirrors M 1 , M 2 can be accurately aligned with respect to first lens barrel 401 and second lens barrel 403 .

Next, the alignment of folding mirrors M 1 , M 2 with respect to first lens barrel 401 and second lens barrel 403 is explained.

In the present working example, folding mirrors M 1 , M 2 are accurately positioned with respect to support body 402 so that the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 are orthogonal. In addition, reflecting surface MS 2 , which is parallel to the line of intersection between the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 accurately positioned so that they are orthogonal, is set with respect to support body 402 . Positioning of folding mirrors M 1 , M 2 and reflecting surface MS 2 with respect to support body 402 is achieved easily with prior art that uses, for example, an autocollimator (apparatus that detects angular displacement of a reflecting mirror by collimated light). The following briefly explains the positioning of reflecting surface MS 2 and folding mirrors M 1 , M 2 with respect to support body 402 , referencing FIG. 19 a.

First, in FIG. 19 a , folding mirrors M 1 , M 2 are positioned with respect to support body 402 so that the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 are substantially orthogonal to a certain degree of accuracy. In this state, reflecting surface 441 a of reflecting member 441 is positioned so that it is substantially parallel to a certain degree of accuracy to the line of intersection between the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 . Then, autocollimator 442 is installed at a position to collimate the reflecting surface of first folding mirror M 1 , and first plane parallel plate 443 is set using autocollimator 442 so that it is parallel to reflecting surface 441 a . Next, autocollimator 442 is moved to a position to collimate reflecting surface MS 2 of reflecting member 446 attached to support body 402 , and third plane parallel plate 445 is set using autocollimator 442 so that it is parallel to reflecting surface 441 a . Last, autocollimator 442 is moved to a position to collimate the reflecting surface of second folding mirror M 2 , and second plane parallel plate 444 is set using autocollimator 442 so that it is parallel to reflecting surface 441 a . In this manner, first plane parallel plate 443 , second plane parallel plate 444 and third plane parallel plate 445 are set mutually parallel at the required accuracy.

In this state, reflecting member 441 is removed from the optical path, and the light from autocollimator 442 impinges on second folding mirror M 2 via second plane parallel plate 444 . The light reflected by second folding mirror M 2 is reflected by first folding mirror M 1 , and impinges on first plane parallel plate 443 . The light reflected by first plane parallel plate 443 returns to autocollimator 442 via first folding mirror M 1 , second folding mirror M 2 and second plane parallel plate 444 . In this case, since plane parallel plates 443 , 444 are arranged geometrically parallel, the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 can be made orthogonal with high precision if the plane parallel plates 443 , 444 are set optically parallel by jogging first folding mirror M 1 . In addition, by moving autocollimator 442 again to the position to collimate reflecting surface MS 2 of reflecting member 446 , and by using autocollimator 442 to adjust reflecting surface MS 2 of reflecting member 446 so that it is parallel to third plane parallel plate 445 , reflecting surface MS 2 , which is parallel to the line of intersection between the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 , can be set with high precision with respect to support body 402 .

Generally, when performing alignment of first folding mirror M 1 and second folding mirror M 2 with respect to first lens barrel 401 and second lens barrel 403 by moving or rotating as a single body first folding mirror M 1 and second folding mirror M 2 , which are set so that their reflecting surfaces are mutually orthogonal, first folding mirror M 1 and second folding mirror M 2 have five degrees of freedom for adjustment. Namely, these are movement (shift) in the Y direction, movement in the Z direction, rotation (tilt) about the X axis, rotation about the Y axis and rotation about the Z axis. In contrast, the focal point position deviation information obtained by interferometer 421 , namely the relative positional deviation information of the focal point of lens group FL and the focal point of concave reflecting mirror MO, is of three types: positional deviation information in the x direction, positional deviation information in the y direction and positional deviation information in the z direction. Accordingly, z is the local coordinate along optical axes Z 1 to Z 2 , and x and y are the local axes parallel to the paper surface of each drawing in a plane perpendicular to the z axis, and are perpendicular local coordinates. In the present mode for carrying out the present invention, by setting reflecting surface MS 2 , which is parallel to the line of intersection between the reflecting surface of first folding mirror M 1 and the reflecting surface of second folding mirror M 2 , perpendicular to the axis of first lens barrel 801 along the Z axis, the number of degrees of freedom for adjustment needed with respect to first folding mirror M 1 and second folding mirror M 2 is reduced to three, comprising movement in the Y direction, movement in the Z direction, and rotation about the Z axis.

Setting reflecting surface MS 2 perpendicular to the axis of first lens barrel 401 is easily achieved by the use of, for example, an autocollimator and the like. The following briefly explains the positioning of reflecting surface MS 2 with respect to the axis of first lens barrel 401 , referencing FIG. 17 and FIGS. 19 a and 19 b . In the present mode for carrying out the present invention, a plane parallel plate perpendicular to the axis of first lens barrel 401 is installed at the peripheral part of first lens barrel 401 , and reflecting surface MS 2 is positioned perpendicular to the axis of first lens barrel 401 by setting this plane parallel plate and reflecting surface MS 2 parallel. Furthermore, since the two lens barrels 401 , 403 are positioned so that the axis of first lens barrel 401 and the axis of second lens barrel 403 are mutually parallel, as discussed earlier, the only way to set reflecting surface MS 2 perpendicular to the axis of second lens barrel 403 is by positioning reflecting surface MS 2 with respect to the axis of first lens barrel 401 . Accordingly, it is understood that a plane parallel plate perpendicular to the axis of second lens barrel 403 may be installed at the peripheral part of second lens barrel 403 , and that this plane parallel plate and reflecting surface MS 2 may be set parallel.

First, plane parallel plate 451 is positioned inside first lens barrel 401 along the axis thereof, as shown in FIG. 19 B. Furthermore, the explanation related to the setting of plane parallel plate 451 perpendicular to the axis (optical axis Z 1 ) of first lens barrel 401 is omitted. Then, autocollimator 452 is installed at a position to collimate plane parallel plate 451 , and autocollimator 452 is used to set plane parallel plate 453 parallel to plane parallel plate 451 .

Next, autocollimator 452 is moved to a position to collimate reflecting surface MS 2 and, using autocollimator 452 , plane parallel plate 154 is installed at the peripheral part of first lens barrel 401 so that it is parallel to plane parallel plate 453 . In this state, plane parallel plate 453 is removed from the optical path, and support body 402 is positioned and adjusted (see FIG. 18A ) using autocollimator 452 so that reflecting surface MS 2 is parallel to reference surface BS 2 of plane parallel plate 454 .

In this manner, reflecting surface MS 2 of support body 402 can be set perpendicular to the axis of first lens barrel 401 and the axis of second lens barrel 403 along the Z axis. Namely, reflecting surface MS 2 of support body 402 can be set parallel to the XY plane. In other words, it can be set so that the light impinging on first folding mirror M 1 along optical axis Z 1 is reflected in the Y direction. As a result, the five degrees of freedom for adjustment, mentioned earlier, for first folding mirror M 1 and second folding mirror M 2 can be reduced to two degrees of freedom for adjustment, comprising rotation about the X axis and rotation about the Y axis. In other words, the three degrees of freedom comprising movement in the Y direction, movement in the Z direction and rotation about the Z axis, which correspond to the three types of positional deviation information comprising positional deviation information in the x direction, positional deviation information in the y direction and positional deviation information in the z direction, should each be independently adjusted.

Generally, the relationship shown in condition (i) below holds between change in wavefront aberration ΔW and wavefront deviations εx, εy, εz between the first light beam, which is the reflected light from reference surface BS 1 , and the second light beam, which is the reflected light from reflecting surface MS 1 of concave reflecting mirror MO, (as described in the reference by Kazumi Murata, entitled “ Optics ”, Science Co., Section 1151):

Δ W=[ε z /(8·( F FL ) 2 )]−[(ε x +ε y )/(2 ·F FL )]  (i)

Therein, F FL is the F number of lens group FL as the Fizeau lens. In addition, εx, εy and εz are the positional deviations between the center of curvature of the wavefront of the first light beam and the center of curvature of the wavefront of the second light beam in the local coordinate system x, y, z; namely, the wavefront deviations.

Referring to condition (i), the smaller (brighter) the F number F FL of lens group FL, the greater is the detection sensitivity of wavefront deviations εx, εy, εz. For example, if the change in wavefront aberration ΔW that is detectable in the interferometer is 0.1 μm, by setting the value of F number F FL of lens group FL to less than 4, the wavefront deviations can be adjusted with an accuracy in units of microns and, in turn, folding mirrors M 1 , M 2 can be aligned with respect to lens barrels 401 , 403 with an accuracy in units of microns. If F number F FL of lens group FL exceeds 4, the alignment accuracy becomes larger than 10 microns, which is unsuitable as the alignment accuracy in a projection optical system of a projection exposure apparatus. By further preferably setting the value of F number F FL of lens group FL to less than 3, alignment of higher accuracy can be realized.

As described above, first and second folding mirrors M 1 , M 2 in the present working example can be aligned with high precision with respect to first lens barrel 401 and second lens barrel 403 by jogging first folding mirror M 1 and second folding mirror M 2 as a single body so that the focal length of the concave reflecting mirror MO installed inside first lens barrel 401 and the focal length of lens group FL installed inside second lens barrel 403 coincide. In other words, third optical axis Z 2 , specified by the arrangement of first and second folding mirrors M 1 , M 2 , can be aligned with high precision with respect to optical axis Z 1 of first lens barrel 401 and optical axis Z 3 of second lens barrel 403 .

After first and second folding mirrors M 1 , M 2 have been aligned with high precision with respect to first lens barrel 401 and second lens barrel 403 in the present mode for carrying out the present invention, manufacture of the optical system is completed by positioning each optical member in first lens barrel 401 and second lens barrel 403 . Namely, as shown in FIG. 17 , after concave reflecting mirror MO has been removed from first lens barrel 401 and lens group FL has been removed from second lens barrel 403 , each of the optical members L 1 to L 3 , MO is positioned inside and along the axis (namely, Z 1 ) of first lens barrel 401 based on reference point A, and each of the optical members L 3 to L 8 is positioned inside and along the axis (namely, Z 3 ) of second lens barrel 403 based on reference point B.

The assembly with high precision of each of the optical members inside each of the lens barrels while making the optical axis of each of the optical members coincide with an accuracy in units of microns with respect to the axis of first lens barrel 401 and the axis of second lens barrel 403 is well known in the prior art, and redundant explanation is herein omitted.

Thus, in an optical system having a folding member according to the present mode for carrying out the present invention, the relative position of a plurality of lens barrels and a folding member having different axes, namely the relative position between each optical axis and the folding member, can be aligned with high precision and, as a result, an optical system having a folding member can be manufactured with high precision.

In the mode for carrying out the present invention discussed above, the present invention is applied to an alignment method and manufacturing method of a catadioptric-type projection optical system. Nevertheless, the need to perform with high precision the alignment of the relative position between a folding member and a plurality of lens barrels (in turn, a plurality of optical axes) is not limited to a catadioptric-type projection optical system, and is generally common to an optical system having a folding member. In other words, the present invention can be applied in the same manner as the working example described above even if a plurality of catoptric optical systems comprising only catoptric optical members like concave reflecting mirrors are optically connected via one or a plurality of folding members, or if a plurality of dioptric optical systems comprising only dioptric optical members are optically connected via one or a plurality of folding members.

In addition, in the mode for carrying out the present invention discussed above, the present invention is applied to an optical system wherein two lens barrels are arranged via two folding members. However, it will be understood that the present invention could also be applied to an optical system wherein a plurality of lens barrels are arranged via one or three or more folding members.

In the working example discussed above, concave reflecting mirror MO is installed inside first lens barrel 401 and lens group FL is installed inside second lens barrel 403 . However, lens group FL may be installed in first lens barrel 401 and concave reflecting mirror MO may be installed inside second lens barrel 403 .

The present mode for carrying out the present invention discussed above takes into consideration ease of adjustment, ease of ensuring the required accuracy and the like, makes the axis of first lens barrel 401 and the optical axis of concave reflecting mirror MO coincide and makes the axis of second lens barrel 403 and the optical axis of lens group FL coincide. In addition, reference point RA and the center of first lens barrel 401 are made to coincide, and reference point RB and the center of second lens barrel 403 are made to coincide. Nevertheless, reference points RA, RB are not necessarily set on the axis of first lens barrel 401 and the axis of second lens barrel 403 , and can be set to an arbitrary positional relationship with respect to first lens barrel 401 and second lens barrel 403 . In addition, the optical axis of concave reflecting mirror MO and the optical axis of lens group FL are not necessarily made to coincide with the axis of first lens barrel 401 and the axis of second lens barrel 403 .

In the working example discussed above, the positional deviation between the focal point of lens group FL and the focal point of concave reflecting mirror MO is adjusted based on the interference between the first light beam and the second light beam detected by the interferometer. Nevertheless, the positional deviation between the focal point of lens group FL and the focal point of concave reflecting mirror MO can be detected based on the positional deviation between the convergent point of the first light beam and the convergent point of the second light beam, without the use of an interferometer, and mirrors M 1 , M 2 can subsequently be aligned with respect to lens barrels 401 , 403 .

Furthermore, when detecting the interference between the first light beam and the second light beam in the working example discussed above, lens group FL that functions as a Fizeau lens is installed inside second lens barrel 403 . Nevertheless, a zone plate having a known focal length can be used in place of lens group FL. In this case, the pattern surface of the zone plate comprises reference surface BS 1 .

According to the seventh mode for carrying out the present invention as discussed above, in an optical system having a folding member, the relative position between a plurality of lens barrels and the folding member having different axes, namely the relative position between each optical axis and the folding member, can be aligned with high precision. Furthermore, an optical system having a folding member can be manufactured with high precision using this alignment method.

Next, a method of forming a predetermined circuit pattern on a wafer using the projection exposure apparatus according to the present invention is explained, referencing flowchart 500 in FIG. 20 .

First, in Step 502 , a metal film is vapor deposited onto one lot of wafers. Next, in Step 504 , photoresist is coated onto the metal film on the wafers of the first lot. Subsequently, in Step 503 , using a projection exposure apparatus according to one of the configurations of the above modes for carrying out the present invention, the image of the pattern on reticle R is successively exposed and transferred onto each exposure region on the wafers of that one lot. Afterwards, in Step 508 , the photoresist on the wafers of that one lot is developed and then, in Step 510 , the circuit pattern corresponding to the pattern on reticle R is formed in each exposure region on each wafer by etching with the resist pattern on the wafers of that one lot as the masks. Subsequently, devices like semiconductor devices having extremely fine circuits are manufactured by further forming circuit patterns of upper layers, and the like.

Ultraviolet light having a wavelength of 100 nm or greater, for example, far ultraviolet (DUV) light like the g-line, the i-line or a KrF excimer laser, or vacuum ultraviolet (VUV) light like an ArF excimer laser or an F 2 laser (wavelength of 157 nm) can be used as the exposure illumination light in the above modes for carrying out the present invention. In a scanning-type exposure apparatus that uses an F 2 laser as the light source, a catadioptric optical system is employed as the projection optical system, as in the above modes for carrying out the present invention, the dioptric optical members (lens elements) used in the illumination optical system or projection optical system are all made of fluorite (CaF 2 ), the air inside the F 2 laser light source, the illumination optical system and the projection optical system is replaced with helium gas, and the space between the illumination optical system and the projection optical system and the space between the projection optical system and the wafer are also filled with helium gas. In addition, in an exposure apparatus that uses an F 2 laser, a reticle is used that is made of at least one of fluorite, synthetic quartz doped with fluorine, magnesium fluoride or crystalline quartz. Furthermore, as the dioptric optical member used in the projection optical system, at least one type among the following materials can be used: fluorine crystal materials like fluorite (calcium fluoride), barium fluoride (BaF), lithium fluoride (LiF), magnesium fluoride (MgF 2 ), lithium calcium aluminum fluoride (LiCaAlF 6 ), lithium strontium aluminum fluoride (LiSrAlF 6 ) and crystalline quartz; synthetic quartz doped with fluorine and quartz doped with germanium, and the like.

The higher harmonics of a solid state laser like a YAG laser having an oscillation spectrum in, for example, one of the wavelengths of 248 nm, 193 nm or 157 nm, may be used in place of an excimer laser.

In addition, higher harmonics may also be used wherein a laser of a single wavelength in the visible region or infrared region oscillated from a DFB semiconductor laser or a fiber laser is amplified by a fiber amplifier doped with, for example, erbium (or, both erbium and indium), and the wavelength is then transformed to ultraviolet light using a non-linear optical crystal.

For example, if the oscillation wavelength of a single wavelength laser is in the range of 1.51 to 1.59 μm, then the eighth harmonic, that generates wavelengths in the range of 189 to 199 nm, or the tenth harmonic, that generates wavelengths in the range of 451 to 159 nm, is output. In particular, if the oscillated wavelength is set within the range of 1.544 to 1.553 μm, then the eighth harmonic in the range of 193 to 194 nm, namely ultraviolet light of substantially the same wavelength as an ArF excimer laser, is obtained. If the oscillation wavelength is set in the range of 1.57 to 1.58 μm, then the tenth harmonic in the range of 157 to 158 nn, namely ultraviolet light of substantially the same wavelength as an F 2 laser, is obtained.

If the oscillation wavelength is set in the range of 1.03 to 1.12 μm, then the seventh harmonic, that generates wavelengths in the range of 147 to 160 nm, is output. In particular, if the oscillation wavelength is set in the range of 1.099 to 1.106 μm, then the seventh harmonic, that generates wavelengths in the range of 157 to 158 nm, namely ultraviolet light of substantially the same wavelength as an F 2 laser, is obtained. An yttrium doped fiber laser may be used as the single wavelength oscillation laser.

The wavelength of the exposure illumination light in the above modes for carrying out the present invention is naturally not limited to 100 nm or greater. For example, to expose a pattern with less than 70 nm wavelength light, EUV (extreme ultraviolet) light in the soft X-ray region (for example, the 5 to 15 nm wavelength region) is generated using an SOR or a plasma laser as the light source, an EUV exposure apparatus is being developed that uses a catoptric-type reduction optical system and a catoptric-type mask designed based on such an exposure wavelength (for example, 13.5 nm). Since a construction wherein a folding member is applied to a catoptric-type reduction optical system is also conceivable in this apparatus, this apparatus is also included in the range of application of the present invention. The projection optical system may use not only a reduction system, but also a unity magnification system or an enlargement system (for example, an exposure apparatus and the like for manufacturing liquid crystal displays).

The present invention can be applied not only to exposure apparatuses used in the manufacture of semiconductor devices, but also to exposure apparatuses used in the manufacture of displays that include liquid crystal displays and the like, those used in the manufacture of thin film magnetic heads and exposure apparatuses that transfer a display pattern onto a glass plate, and those used in the manufacture of image pickup devices (CCDs and the like) and exposure apparatuses that transfer a device pattern onto a ceramic wafer. In addition, the present invention can be applied to exposure apparatuses that transfer a circuit pattern onto a glass substrate or silicon wafer and the like in order to manufacture a reticle or a mask.

As described above, the present invention is not limited to the abovementioned modes for carrying out the present invention, and it is understood that various configurations can be obtained in a range that does not depart from the purport of the present invention.

Claims

1. A catadioptric projection optical system that makes first and second planes optically conjugate, the catadioptric projection optical system comprising:a catadioptric imaging optical subsystem; and a refractive imaging optical subsystem; wherein a position that is optically conjugate to the first and second planes is formed in an optical path between the catadioptric imaging optical subsystem and the refractive imaging optical subsystem; the catadioptric imaging optical subsystem is arranged in the optical path between the first plane and the conjugate position; the refractive imaging optical subsystem is arranged in an optical path between the second plane and the conjugate position; and the catadioptric imaging optical subsystem includes: a concave reflecting surface; at least one lens; and a first barrel that holds the concave reflecting surface and the at least one lens of the catadioptric imaging optical subsystem integrally, the catadioptric projection optical system further comprising: an optical path folding mirror arranged in an optical path between the concave reflecting surface and the refractive imaging optical subsystem; and a second barrel that holds the optical path folding mirror independently of the first barrel.

2. The catadioptric projection optical system according to claim 1, wherein the catadioptric imaging optical subsystem includes at least one lens arranged between the first plane and the optical path folding mirror, and a third barrel that holds the at least one lens arranged between the first plane and the optical path folding mirror,wherein the third barrel is independent of the first barrel.

3. The catadioptric projection optical system according to claim 2, wherein the at least one lens arranged between the first plane and the optical path folding mirror includes a positive lens.

4. The catadioptric projection optical system according to claim 3, wherein the at least one lens held by the first barrel includes a negative lens.

5. The catadioptric projection optical system according to claim 1, wherein the at least one lens arranged between the first plane and the optical path folding mirror includes a positive lens.

6. The catadioptric projection optical system according to claim 5, wherein the at least one lens held by the first barrel includes a negative lens.

7. The catadioptric projection optical system according to claim 1, wherein the at least one lens held by the first barrel includes a negative lens.

8. A catadioptric projection optical system including a plurality of lens surfaces and a plurality of reflecting surfaces, and that forms a reduced image of a first plane at a second plane, comprising:a catadioptric imaging optical subsystem; and a refractive imaging optical subsystem; wherein an intermediate image of the first plane is formed in an optical path between the catadioptric imaging optical subsystem and the refractive imaging optical subsystem, the catadioptric imaging optical subsystem is arranged in an optical path between the first plane and a formation position of the intermediate image, the refractive imaging optical subsystem is arranged in an optical path between the second plane and the intermediate image formation position, the catadioptric imaging optical subsystem includes a concave reflecting surface, the plurality of reflecting surfaces includes a first reflecting surface arranged in an optical path between the concave reflecting surface and the refractive imaging optical subsystem, and a second reflecting surface arranged in an optical path between the first plane and the refractive imaging optical subsystem, the catadioptric optical system further comprising a first barrel that holds the first reflecting surface and the second reflecting surface integrally.

9. The catadioptric projection optical system according to claim 8, wherein the first reflecting surface and the second reflecting surface are perpendicular to each other.

10. The catadioptric projection optical system according to claim 9, further comprising a second barrel that holds at least two lenses of the refractive imaging optical subsystem,wherein the second barrel is independent of the first barrel.

11. The catadioptric projection optical system according to claim 10, further comprising:at least one lens between the first surface and one of the first and second reflecting surfaces; and a third barrel that holds the at least one lens between the first surface and one of the first and second reflecting surfaces, wherein the third barrel is independent of the first barrel.

12. The catadioptric projection optical system according to claim 8, further comprising a second barrel that holds at least two lenses of the refractive imaging optical subsystem,wherein the second barrel is independent of the first barrel.

13. The catadioptric projection optical system according to claim 12, further comprising:at least one lens between the first surface and one of the first and second reflecting surfaces; and a third barrel that holds the at least one lens between the first surface and one of the first and second reflecting surfaces, wherein the third barrel is independent of the first barrel.

14. The catadioptric projection optical system according to claim 8, further comprising a second barrel that holds the concave reflecting surface and at least one lens of the catadioptric imaging optical subsystem,wherein the second barrel is independent of the first barrel.

15. The catadioptric projection optical system according to claim 14, wherein the at least one lens held by the second barrel includes a negative lens.

16. A projection exposure apparatus that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the projection exposure apparatus comprising:a mask stage that positions the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; and a substrate stage that positions the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; wherein the projection optical system is provided with the catadioptric projection optical system according to claim 1.

17. A projection exposure method that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the method comprising the steps of:positioning the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; positioning the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; and forming the reduced image of the pattern onto the substrate by using the catadioptric projection optical system as set forth in claim 1.

18. A projection exposure apparatus that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the projection exposure apparatus comprising:a mask stage that positions the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; and a substrate stage that positions the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; wherein the projection optical system is provided with the catadioptric projection optical system according to claim 4.

19. A projection exposure method that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the method comprising the steps of:positioning the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; positioning the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; and forming the reduced image of the pattern onto the substrate by using the catadioptric projection optical system as set forth in claim 4.

20. A projection exposure apparatus that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the projection exposure apparatus comprising:a mask stage that positions the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; and a substrate stage that positions the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; wherein the projection optical system is provided with the catadioptric projection optical system according to claim 8.

21. A projection exposure method that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the method comprising the steps of:positioning the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; positioning the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; and forming the reduced image of the pattern onto the substrate by using the catadioptric projection optical system as set forth in claim 8.

22. A projection exposure apparatus that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the projection exposure apparatus comprising:a mask stage that positions the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; and a substrate stage that positions the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; wherein the projection optical system is provided with the catadioptric projection optical system according to claim 11.

23. A projection exposure method that illuminates a mask, in which a predetermined pattern is provided, by an illumination optical system and transfers a reduced image of the pattern onto a substrate by a projection optical system, the method comprising the steps of:positioning the mask at a first plane so that a normal line of a pattern surface of the mask is substantially in a direction of gravity; positioning the substrate at a second plane so that a normal line of the substrate is substantially in the direction of gravity; and forming the reduced image of the pattern onto the substrate by using the catadioptric projection optical system as set forth in claim 11.