Ultra high density disk reader/writer comprising two interferometers

Information

  • Patent Grant
  • 6366547
  • Patent Number
    6,366,547
  • Date Filed
    Thursday, July 27, 2000
    24 years ago
  • Date Issued
    Tuesday, April 2, 2002
    22 years ago
  • Inventors
  • Examiners
    • Hudspeth; David
    • Chu; Kim-Kwok
    Agents
    • Pawlak & Associates
    • Pawlak; Elizabeth J.
Abstract
An optical apparatus for reading from and writing to an ultra high density disk and comprising a light source emitting a pencil of light rays to an optical path along an optical axis; two interferometers, a beamsplitter, a quarter-wave plate, and an objective lens. The pencil of light rays is transmitted through the apparatus to become a narrow fringe ring which in turn is used to generate an ultra small spot of light. The resulting ultra small spot of light can address far more storage locations per a same unit area than a conventional much larger spot of light.
Description




BACKGROUND OF THE INVENTION




The technological growth of the computer industry has been progressing at an extremely fast pace. Products that are barely three years old are considered obsolete. The demand for more powerful computers translates into demands of faster data processing speed and greater data storage capacity. The present invention fits in the category of meeting the demand for greater data storage capacity. Presently, data stored on an optical data it storage device are retrieved by observing the behavior of light being reflected from the optical data storage device. As storage capacity increases, the amount of data per unit of area increases. A practical limitation of the storage capacity of an optical data storage device is the size of a spot of light that can be generated by a reader/writer head and the technology available to precisely move and control its position. The present invention discloses a spot of light that is considerably smaller than those currently being used in the market place.




SUMMARY OF THE INVENTION




The present invention discloses a novel method and apparatus to produce an extremely small spot of light and electronically control its position.











BRIEF DESCRIPTION OF THE DRAWINGS





FIG. 1

illustrates a first embodiment of an optical configuration using a Fabry-Perot interferometer and a spectral light source.





FIG. 2

illustrates an annular constructive interference fringe rings produced by the first embodiment as shown in FIG.


1


.





FIG. 2



a


illustrates an intensity distribution of the constructive interference fringes in a focal plane.





FIG. 3

illustrates a second embodiment of an optical configuration using a Fabry-Perot interferometer and a spectral light source.





FIG. 4

illustrates an annular constructive interference fringe rings produced by the second embodiment as shown in FIG.


3


.





FIG. 5

illustrates a third embodiment of an optical configuration using two Fabry-Perot interferometers and a spectral light source.





FIG. 6

illustrates two annular constructive interference fringe rings produced by the third embodiment as shown in FIG.


5


.





FIG. 7

illustrates a Fabry-Perot interferometer configured as an electro-optical device containing a media inside the interferometer that exhibits Kerr or Pockel effect.





FIG. 8

illustrates a first embodiment of an ultra high density optical disk reader/writer.





FIG. 9

illustrates a second embodiment of an ultra high density optical disk reader/writer.





FIG. 10

illustrates a third embodiment of an ultra high density optical disk reader/writer.





FIG. 11

illustrates a mechanism employed to electronically control the location of the ultra small spot of light.











DETAIL DESCRIPTION OF THE INVENTION





FIG. 1

shows an optical system employing a conventional Fabry-Perot interferometer. The Fabry-Perot interferometer is an angle filter and is the basis of this invention.




In

FIG. 1

, the X-axis is parallel to an optical axis


395


of the Objective lens


300


. The Y-axis lies in a plane of the drawing and is perpendicular to axis


395


. The Z-axis is perpendicular to the plane of the drawing.




A spectral light source


100


emits a pencil of light rays


190


. The central ray


195


of pencil


190


, is incident upon a Fabry-Perot interferometer


210


, in a direction normal to entrance face


211


as figuratively illustrated by a broken line


212


. Central ray


195


is parallel to an optical axis


395


of the Objective lens


300


.




It is a long established principal of multiple-beam interference phenomenon, well known to those skilled in the art of physical optics, that of the infinite number of light rays incident upon a Fabry-Perot interferometer, only those having angles normal to the entrance face


211


can successfully transited through the interferometer. All other light rays suffer destructive interference thus are filtered out.




Those light rays successfully transmit through interferometer


210


are collected by Objective lens


300


, to be converged into annular constructive interference fringe rings on a focal plane


400


. These annular constructive interference fringe rings are shown in FIG.


2


. The central fringe


500


is shown at the focal point of lens


300


with a first annular ring fringe


510


located at a radius r


1


from the central fringe


500


. r


1


is defined as:




r


1


=arctan(θ1/f)




where θ1 is an angle relative to the normal broken line


212


inside pencil


190


, and f is a focal length of lens


300


. Likewise r


2


, the radius of the second annular ring fringe,


520


, and r


3


, the radius of the second annular ring fringe


530


, are defined as:




r


2


=arctan(θ2/f); and




r


3


=arctan(θ3/f).





FIG. 2



a


shows the relation between these radii, angles, and lens


300


and focal plane


400


. Angles θ1, θ2, and θ3 are defined by a design of the interferometer as shown in a sample calculation included hereinbelow.




It should be noted that the closer is the fringe to the focal point of lens


300


, the wider is the fringe. Conversely, the farther is a fringe from the focal point of lens


300


, the narrower is the fringe. Since

FIG. 2

is drawn on white paper, the colors are reversed. The black rings actually represent high intensity constructive interference fringe rings and the white spacing therebetween represent regions void of light, also known as a regions of destructive interference where light rays have been filtered out of pencil


190


.




The second embodiment of an optical configuration using a Fabry-Perot interferometer and a spectral light source is shown in FIG.


3


. This is a modification of

FIG. 1

wherein interferometer


210


has been rotated by an angle θ1 about the Z-axis. This causes fringe


510


to be displaced in focal plane


400


along the Y-axis by a distance r


1


, as shown in FIG.


4


.




The third embodiment of an optical configuration using two Fabry-Perot interferometers and a spectral source is shown in FIG.


5


. This is a modification of

FIG. 3

wherein a second Fabry-Perot interferometer


220


has been added. For the sake of clarity, the fringe that would be transmitted by interferometer


210


is labeled as


510




a


while those that would be transmitted by interferometer


220


are labeled as


510




b.






Interferometer


220


has been rotated by an angle θ1 about the Y-axis and interferometer


210


has been rotated by an angle θ1 about the Z-axis. This causes fringe


510




a


to be displaced in the focal plane of lens


300


, along the Y-axis by a distance r


1


, and fringe


510




b


to be displaced in the focal plane of lens


300


, along the Z-axis by a distance r


1


, as shown in FIG.


6


.




Because interferometer


210


can only permit transmission of light rays making an angle θ1 with respect to the normal broken line


212


and interferometer


220


can only transmit rays making an angle θ1 with respect to the normal broken line


212


, spots only appear in the focal plane when these conditions are met. A preferred spot is located at the focal point of lens


300


. A complimentary spot lies diagonally bisecting the Y-axis and Z-axis. The complimentary spot is masked out.




The Fabry-Perot interferometer is only one member out of a family of instruments that employ the principals of multiple-beam interference. Other members of this family include the Lummer-Gehrcke interferometer, the interference filter, and the frustrated total reflection interference filter. All of these instruments regenerate every single light ray, from a pencil of light rays, into a multitude of parallel, geometrically degraded amplitude, phase related light rays. When a set of parallel rays are brought to separate points in the focal plane of a lens, they M will interfere with each other. The intensity of the light ray at each point depends on the number of optical paths between sequential parallel plates the light ray has traveled. If the path difference between sequential sets of rays is an integer number of wavelengths, then the intensity is at a maximum. If it is a half integer, the intensity is zero. Any other value of the path difference will yield an intermediate intensity.




Thus, in addition to the Fabry-Perot interferometer, this invention will function with either a Lummer-Gehrcke interferometer, an interference filter, or a frustrated total reflection interference filter.





FIG. 7

illustrates by way of an example a Fabry-Perot interferometer functioning as an electro-optical device employing the Kerr or Pockel effect. It should be noted that the electro-optical device can also be a Lummer-Gehreke interferometer, interference filter, or frustrated total reflection interference filter. The medium inside the Fabry-Perot interferometer, Lummer-Gehreke interferometer, interference filter, or frustrated total reflection interference filter can be an electro-optical material so that a voltage applied across therein will change an index of the medium thus causing angles that can propagate through the instrument to change. The medium can be various types of gases, liquids or solids, such as KD*P.




A design sample showing detailed calculations and designed parameters are included hereinbelow. As shown, the total number of bytes that can be easily generated by the present invention is in the order of 109.1 giga bytes on a 120-millimeter diameter disk.




If the medium between the reflecting surfaces is an electro-optical material, then the optical path changes when an electric or magnetic field is applied therethrough. This changes the angle of constructive interference, thus changing the location of the spot, or constructive interference fringe on focal plane


400


.




A magnetic or electric field applied to the spectral source changes the wavelength of the source. This also changes the location of the spot on focal plane


400


. It is desirable for the optical apparatus for reading information from and writing information to a data storage device to comprise: (a) a light source emitting a pencil of light rays to an optical path along an optical axis; (a) an interferometer; (c) a beamsplitter; (d) a quarter wave plate; and (e) an objective lens; wherein the pencil of light rays is transmitted respectively through the interferometer, the beamsplitter, the quarter-wave plate, and the objective lens to become constructive interference fringes of light upon reaching the data storage device and wherein the light source is a laser diode and the spectral source resides inside an electric field so that the wavelength of the pencil of light rays are Stark split into a plurality of wavelengths.




Additional embodiments of the apparatus of the present invention include an optical apparatus for reading information from and writing information to a data storage device, comprising: (a) a light source surrounded by a coil generating either an electric field or a magnetic field and emitting a pencil of light rays to an optical path along an optical axis; ˜(b) an interferometer; and (c) an objective lens and wherein the pencil of light rays is transmitted respectively through the interferometer and objective lens to become constructive interference fringes of light upon reaching said field-controlled location on a focal plane of the objective lens and wherein the light source is a laser diode with the spectral source residing inside an electric field so that a wavelength of the pencil of light rays are Stark split into a plurality of wavelengths.




Various embodiments of the ultra high density optical disk readers as shown in

FIG. 8

,

FIG. 9

, and

FIG. 10

are correspondingly based on various embodiments of ultra small spot generators as shown in

FIG. 1

, FIG.


3


and FIG.


5


.





FIG. 8

illustrates a read/write optical head wherein a spot in the focal plane of a lens is illuminated and characteristics of reflected light rays are detected. Here, source


100


emits a diverging pencil


190


, polarized in the plane of the drawing, which is transmitted through Fabry-Perot interferometer


210


, polarizing beam splitter


250


, quarter-wave plate


260


, and lens


300


to produce spot


500


on focal plane


400


. The quarter-wave plate rotates the polarization, about the optical axis by 45 degrees.




When spot


500


is reflected from focal plane


400


, the light rays return through lens


300


as a converging pencil into the quarter-wave plate


260


. Quarter-wave plate


260


rotates the polarization about the optical axis by an additional 45 degrees so that it is now perpendicular to the plane of the drawing. Thus the pencil of light rays will be totally reflected as they pass through polarizing beam splitter


250


. These light rays are then passed through lens


600


onto a photon detector


700


.





FIG. 9

is the same as

FIG. 8

except Fabry-Perot interferometer


210


has been rotated by an angle θ1 about the Z-axis.





FIG. 10

is the same as

FIG. 9

except an additional Fabry-Perot interferometer


220


has been added. Interferometer


220


has been rotated by an angle θ1 about the Y-axis and interferometer


210


has been rotated by an angle θ1 about the Z-axis.





FIG. 11

illustrates a mechanism that electronically controls the location of the ultra small spot of light on the focal plane


400


. Source


100


is subjected to a coil


103


generating a magnetic field parallel to the optical axis of lens


300


. This causes the wavelength of these light rays to split into multiple wavelengths. Ideally, there would be two wavelengths. A set of rays with one wavelength would be right circularly polarized and a set of rays with another wavelength would be left circularly polarized. The separation of these wavelengths is a function of the intensity of the magnetic field.




Both sets of light rays pass through a quarter-wave plate


150


that is constructed of a material with Kerr or Pockel effects. Thus, by impressing a specific electric field on plate


150


, both sets of circularly polarized rays become linearly polarized. For example, the right circularly polarized light will become linearly polarized in the plane of the drawing and the left circularly polarized light will become linearly polarized perpendicular to the plane of the drawing.




These rays are then transmitted through polarizing filter


160


where one ray is filtered out.




Thus, by changing the intensity of the electric field on plate


150


, the wavelength of the rays being transmitted by interferometer


210


and interferometer


220


is changed. This in turn will cause the constructive interference fringe of ultra small spot of light to appear at different locations of focal plane


400


.




By adjusting the intensity of the magnetic field at source


100


, the wavelength of the Zeeman split light ray can be adjusted to equal the pit width. The spot can then be made to oscillate from one side of a target to another by oscillating the electric field on quarter-wave plate


150


. Thus, the intensity of the signal at detector


700


will define the magnitude of any difference between where the spot should be and the pit and its phase will define the direction of the error.




From the foregoing detailed description, it will be evident that there are a number of changes, adaptations and modifications of the present invention which come within the province of those persons having ordinary skill in the art to which the aforementioned invention pertains. However, it is intended that all such variations not departing from the spirit of the invention be considered as within the scope thereof as limited solely by the appended claims.




Sample calculations of the present invention are shown hereinbelow.

















Fabry-Perot Configured ETOS (FPCD.mcd)













Wavelength of the laser




λ := 0.635 microns







Focal length of the objective lens




f := 1000.000 microns






Index of refraction of the Fabry-Perot (KD*P)




n := 1.502






Numerical aperture of the objective lens




NA := 0.45






Diameter of the objective lens




D := 2 · f · NA




D = 900 microns






Radius of the 3db intensity contour




r3db := 0.446 microns











Design objectives (based on the intensity contours used by the DVD System)






If the principal constructive interference fringe is at the center of the pit being read then












Ipw = intensity of the maximum circle inside the pit




Ipw := 0.811






Ipl = intensity of the circle encompassing the minimum pit




Ipl := 0.695






Ias = intensity at the center of the adjecent spiral




Ias := 0.257











The first constructive interference fringe ring [order of interference (M − 1)]













Radius in the focal plane




r1 := 15 microns














Angle with respect to the optical axis











θ1
:=

atan


(

r1
f

)












θ1 = 0.014999 radians













Transmission angle through the Fabry-Perot











φ1
:=

asin


(


sin


(
θ1
)


n

)












φ1 = 0.009986 radians


















Interferometer configuration parameters




















Order of interference











M
:=

floor


(

1

1
-

cos


(
φ1
)




)












M = 20057















sin(M · π)


2


= 0








sin((M − 0.5) · π)


2


= 1








sin((M − 1) · π)


2


= 0













Thickness of the Fabry-Perot Interferometer











T
:=


M
·
λ


2
·
n












T = 4.24 · 10


3


microns




















θ3db
:=

atan


(

r3db
f

)












θ3db = 0.000446




















φ3db
:=

asin


(

sin


(

θ3db
n

)


)












φ3db = 0.000297




















M3db
:=


2
·
T
·
n
·

cos


(
φ3db
)



λ











M3db = 2.0057 · 10


4






sin(M3db · π)


2


= 7.717 · 10


−6















Coefficient of reflection




R := 0.95




R = 0.95













Intensity distribution constance











F
:=


4
·
R



(

1
-
R

)

2












F = 1.52 · 10


3




















The second constructive interference fringe ring [order of interference (M − 2)]




















Transmission angle through the Fabry-Perot











φ2
:=

acos


(


M
-
2

M

)












φ2 = 0.014 radians













Angle with respect to the optical axis




θ2 := asin(n · sin(φ2))




θ2 = 0.021 radians






Radius in the focal plane




r2 := f · tan(θ2)




r2 = 21.216 microns











The third constructive interference fringe ring [orede of interference (M − 3)]




















Transmission angle through the Fabry-Perot











φ3
=

acos


(


M
-
3

M

)












φ3 = 0.017 radians













Angle with respect to the optical axis




θ3 := asin(n · sin(φ3))




θ3 = 0.026 radians






Radius in the focal plane




r3 := f · tan(θ3)




r3 = 25.986 microns











Radial distribution (from the center of the fringe) of the intensity at the surface of the disk














i := 0, 1 . . . 2000
























r
i

:=


r1
·
i

1000




























θ
i

:=

atan


(


r
i

f

)




















φ
i

:=

asin


(


sin


(

θ
i

)


n

)




















δ
i

:=


4
·
π
·
n
·
T
·

cos


(

φ
i

)



λ



















I
i

:=

1

1
+

F
·


sin


(


δ
i

2

)


2
























































δr
:=

r1
1000




















Radial distribution of the intensity of the Central fringe






I3db


i


:= if(I


i


< 0.5, 0, 1)


































Opertional Fringe Intensity distribution at the surface of the disk














j := 0, 1 . . . 2000
























r
j

:=

10
+

j
200





























θ
i

:=

atan


(


r
i

f

)




















φ
i

:=

asin


(


sin


(

θ
i

)


n

)




















δ
i

:=


4
·
π
·
n
·
T
·

cos


(

φ
i

)



λ



















I
j

:=

1

1
+

F
·


sin


(


δ
j

2

)


2

















































Opertional fringe intensity factors














pit


j


:= if(I


j


< Ipw, 0, 1)




mpl


j


:= if(I


j


< Ipl, 0, 1)




pitch


j


:= if(I


j


< Ias, 0, 1)




microns














































Sampleling interval











Δ
:=



r
2000

-

r
0


2000











Δ = 0.005 microns


















Fringe parameters














3db Beam width:




I


j


:= I


j






hpp


j


:= if(I


j


< 0.5, 0, 1)




half power points





























BW
:=

Δ
·



j



hpp
j























j



hpp
j


=
25










BW = 0.125 microns













Pit width:











pw
:=

Δ
·



j



pit
j























j



pit
j


=
11










pw = 0.055 microns













Minimum pit length:











pl
:=

Δ
·



j



mpl
j























j



mpl
j


=
17










pl = 0.085 microns













Pitch of the spiral:











pch
:=

0.5
·
Δ
·



j



pitch
j























j



pitch
j


=
41










pch = 0.1025 microns


















Disk storage












ro = outer radius of the data storage ring




ro := 5.8 · 10


4


microns






ri = inter radius of the data storage ring




ri := 2.5 · 10


4


microns




















ns = number of data spirls (revolutions of the disk)











ns
:=


ro
-
ri

pch











ns = 3.22 · 10


5


revolutions



















ls = length of the data spiral




ls := π · ns · (2 · ri | (ns 1) · pch)













ls = 8.395 · 10


10


microns




















nlpp = number of “land/pit” pairs in the data spiral











nlpp
:=

ls

2
·
pl












nlpp = 4.938 · 10


11















btp = bytes to pits conservision




btp := 0.221






tnb = total number of bytes




tnb := nlpp · btp




tnb = 1.091 · 10


11


bytes











Physical Constances













C = speed of light (microns/second)





C := 3 · 10


14








r = electro-optic coefficient (microns/volts)





r = 3.22 · 10


−5








ε = dielectric constant:





ε := 44.5






kZ = Zeeman constant




kZ := 7.142857 · 10


−7


· C




kZ = 2.143 · 10


8






























pr
:=

pw
2











pr = 0.0275




pch = 0.103




















θhpw
:=

atan


(


r1
-
pr

f

)












θ1 = 0.014999 θhpw = 0.014971











θpch
:=

atan


(


r1
-
pch

f

)












θpch = 0.014896




















φhpw
:=

asin


(


sin


(
θbpw
)


n

)












φ1 − 0.009986 φhpw = 0.009967











φpch
:=

asin


(

sin


(

θpch
n

)


)












φpch = 0.009918




















nhpw
:=



(

M
-
1

)

·
λ


2
·
T
·

cos


(
φhpw
)














nhpw = 1.501999724











npch
:=



(

M
-
1

)

·
λ


2
·
T
·

cos


(
φpch
)














npch = 1.501998982




















Vhpw
:=


2
·

(

n
-
nhpw

)

·
T


r
·

n
3













Vhpw = 21.427











Vpch
:=


2
·

(

n
-
npch

)

·
T


r
·

n
3













Vpch = 79.126




















λhpw
:=


2
·
T
·
n
·

cos


(
φhpw
)




M
-
1












λhpw = 0.635000117











λpch
:=


2
·
T
·
n
·

cos


(
φpch
)




M
-
1












λpch = 0.63500043













λlhpw := 2 · λ − λhpw




λlhpw = 0.634999883




λlpch := 2 · λ − λpch




λlpch = 0.63499957




















Hfppw
:=

kZ
·

(


1
λ

-

1
λhpw


)












Hfppw = 61.944











Hpch
:=

kZ
·

(


1
λ

-

1
λpch


)












Hpch = 228.753













Claims
  • 1. An optical apparatus for reading information from and writing information to a data storage device, comprising:a light source emitting a pencil of light rays to an optical path along an optical axis; a first interferometer; a second interferometer; a beamsplitter; a quarter wave plate; and an objective lens; wherein the pencil of light rays is transmitted respectively through the interferometer, the beamsplitter, the quarter-wave plate, and the objective lens to become constructive interference fringes of light upon reaching the data storage device.
  • 2. The optical apparatus of claim 1, wherein the first and second interferometers are in optical alignment to the optical axis.
  • 3. The optical apparatus of claim 1, wherein the first interferometer has a first interferometer optical axis intersecting the optical axis.
  • 4. The optical apparatus of claim 3, wherein the second interferometer has a second interferometer optical axis intersecting the optical axis.
  • 5. The optical apparatus of claim 4, wherein the data storage device is in a focal plane of the objective lens.
  • 6. The optical apparatus of claim 1, wherein a plane defined by the first interferometer optical axis and the optical axis perpendicularly intersects a plane defined by the second interferometer optical axis and the optical axis.
  • 7. The optical apparatus of claim 1, wherein the pencil of light rays is filtered by the first interferometer to produce a definable number of constructive interference fringe rings all sharing a center point and each ring has a unique radius as measured from the center point.
  • 8. The optical apparatus of claim 7, wherein the pencil of light rays that are filtered by the first interferometer and the second interferometer becomes a sector as manifested on a focal plane of the objective lens.
  • 9. The optical apparatus of claim 1, wherein one of or both of the first and second interferometers are Fabry-Perot interferometers.
  • 10. The optical apparatus of claim 9, wherein one of or both of the first and second Fabry-Perot interferometers are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 11. The optical apparatus of claim 1, wherein one of or both of the first and second interferometers are Lummer-Gehrcke interferometers.
  • 12. The optical apparatus of claim 11, wherein one of or both of the Lummer-Gehrcke interferometers are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 13. The optical apparatus of claim 1, wherein one of or both of the first and second interferometers are interference filters.
  • 14. The optical apparatus of claim 13, wherein one of or both of the first and second interference filters are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 15. The optical apparatus of claim 1, wherein one of or both of the first and second interferometers are frustrated total interference filters.
  • 16. The optical apparatus of claim 15, wherein one of or both of the first and second frustrated total interference filters are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 17. The optical apparatus for reading information from and writing information to a data storage device, comprising:a light source surrounded by a coil generating either an electric field or a magnetic field and emitting a pencil of light rays to an optical path along an optical axis; a first interferometer; a second interferometer; and an objective lens; wherein the pencil of light rays is transmitted respectively through the first and second interferometer and objective lens to become constructive interference fringes of light upon reaching said field-controlled location on a focal plane of the objective lens.
  • 18. The optical apparatus of claim 17, wherein the first and second interferometers are in the optical path.
  • 19. The optical apparatus of claim 17, wherein the first interferometer has a first interferometer optical axis intersecting the optical axis.
  • 20. The optical apparatus of claim 17, wherein the second interferometer has a second interferometer optical axis intersecting the optical axis.
  • 21. The optical apparatus of claim 17, wherein a plane defined by the first interferometer optical axis and the optical axis perpendicularly intersects a plane defined by the second interferometer optical axis and the optical axis.
  • 22. The optical apparatus of claim 17, wherein the pencil of light rays is filtered by the first interferometer to produce a definable number of constructive interference fringe rings all sharing a center point and each ring has a unique radius as measured from the center point.
  • 23. The optical apparatus of claim 22, wherein the pencil of light rays filtered by the first interferometer and the second interferometer becomes a sector as manifested on a focal plane of the objective lens.
  • 24. The optical apparatus of claim 17, wherein one of or both of the first and second interferometers are Fabry-Perot interferometers.
  • 25. The optical apparatus of claim 24, wherein one of or both of the first and second Fabry-Perot interferometers are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 26. The optical apparatus of claim 17, wherein one of or both of the first and second interferometers are Lummer-Gehrcke interferometers.
  • 27. The optical apparatus of claim 26, wherein one of or both of the Lummer-Gehrcke interferometers are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 28. The optical apparatus of claim 17, wherein one of or both of the first and second interferometers are interference filters.
  • 29. The optical apparatus of claim 28, wherein one of or both of the first and second interference filters are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
  • 30. The optical apparatus of claim 17, wherein one of or both of the first and second interferometers are frustrated total interference filters.
  • 31. The optical apparatus of claim 30, wherein one of or both of the first and second frustrated total interference filters are electro-optical devices containing a medium that exhibits one of a Kerr effect and a Pockel effect.
Parent Case Info

This application is a continuation-in-part of U.S. patent application Ser. No. 09/035,824, by Roland H. Chase, filed Mar. 6, 1998, now U.S. Pat. No. 6,269,066.

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Number Name Date Kind
3506334 Korpel Apr 1970 A
3597701 Cornillault Aug 1971 A
3603685 Heflinger Sep 1971 A
4789978 Shikama et al. Dec 1988 A
5071253 Chase Dec 1991 A
5119454 McMahon Jun 1992 A
5390203 Miller Feb 1995 A
5587983 Bailey Dec 1996 A
5646920 Raczynski Jul 1997 A
5677902 Brazas, Jr. Oct 1997 A
5708644 Hasegawa Jan 1998 A
5739943 Ohshima et al. Apr 1998 A
Continuation in Parts (1)
Number Date Country
Parent 09/035824 Mar 1998 US
Child 09/627076 US