The present invention relates to optical devices, in general, and more particularly, to optical spot displacement apparatus.
Generally, an optical interconnection or cross-connection device, like a White cell optical switch, for example, comprises a plurality of optical elements disposed in a predetermined spatial three dimensional pattern for directing one or more light beams from an input through a plurality of reflections to an output. Multiple light beams may bounce through various stages of the device simultaneously. Typically, the interconnection device allows a set of Nin optical inputs to be switched among Nout outputs in a free-space approach, in which light beams bounce multiple times in a White cell. On each bounce a given beam can be switched between different paths, and thus transferred to different outputs.
In some applications, an optical stage is included in the interconnection device to shift the position of a light beam in a particular plane which displaces the illuminating spot image thereof. Thus, this spot displacement stage may be used in the optical interconnection device to shift spot images of the light beams to different outputs. The number of outputs that can be reached is controlled by the switching mechanism of the White Cell and the particular spot shifting stage. In a binary design, the number of outputs is proportional to 2m, where m is the number of bounces.
The optical elements of current spot displacement stages are not without improvement. The present invention provides for optical spot displacement apparatus that is easily modified to produce small as well as large spot displacements, rendering an improved scaling of the displacement, which will be better understood from the description found herein below.
In accordance with one aspect of the present invention, optical spot displacement apparatus comprises: a face that is divided into a plurality of columns; each column of the plurality including a predetermined number of prisms, the predetermined number of prisms of a same column configured within the corresponding column to displace at least one incident light beam a common predetermined distance from incidence, and the predetermined number of prisms of different columns configured within each corresponding column to displace the at least one incident light beam a different predetermined distance from incidence.
In accordance with another aspect of the present invention, optical spot displacement apparatus comprises: a first plane and a second plane; a mirror disposed at the first plane, the mirror including an entrance region and an exit region; a series of spherical mirrors disposed along a path at the second plane; wherein at least one light beam incident the entrance region will enter and travel along the path by reflections between the spherical mirrors of the second plane and mirror of the first plane until the at least one light beam reaches the exit region where it exits rendering the at least one light beam displaced by a predetermined distance commensurate with a distance between the entrance and exit regions of said mirror.
In accordance with yet another aspect of the present embodiment, optical waveguide based spot displacement apparatus comprises: a substrate of a first refractive index; a core channel of a second refractive index disposed within the substrate, the second refractive index being greater than the first refractive index, the core channel including an entrance region and an exit region spaced apart a predetermined distance; a first optical element disposed at the entrance region for coupling at least one incident light beam into the core channel at a first predetermined angle to cause said at least one incident light beam to travel through the core channel; and a second optical element disposed at the exit region for coupling the at least one traveling light beam from the core channel at a second predetermined angle to cause the at least one traveling light beam to exit from the core channel.
a is a connectivity diagram of the light beam flow in a dual White cell configuration.
a is an exploded front view of an input cell of the alternate dual White cell embodiment.
a and 9b are isometric and side cross-sectional views, respectively, of a roof top prism assembly suitable for use in the spot displacement device of
a and 12b are isometric perspective views of other alternate prism embodiments of a spot displacement device.
a and 22b are isometric perspectives of a lens configuration illustrating principles of astigmatism.
An optical switch based on the principles of an optical White cell will exemplify an optical cross-connection device for the purposes of describing one or more embodiments of the present invention. The optical White cell is an example of a multi-pass light beam optical system for generating a series of spot illuminations in sequence for an input light beam as will be better understood from the following description. Other examples of multi-pass light beam systems include a Herriot cell or any of the alternative spot pattern generators disclosed in U.S. Pat. No. 6,266,176. For the present example, optical switching is performed by allowing each of a large number of input beams to be switched between two different White cells. One White cell produces two rows of spots for each input beam, and the second White cell incorporates a spot displacement device that will continue the spot image patterns but displace them by some number of rows, thus changing the exit location of each beam.
In the example, a large number of potential outputs is allowed for each of the input beams, but with the smallest possible number of bounces. Reducing the number of bounces reduces the loss, which will accumulate on every bounce. A “binary White cell” in which the number of outputs is equal to 2m, where m is the number of bounces in the White cell, will be used by way of example. Two White cells may be combined to produce a suitable binary optical interconnection configuration for the present embodiment as illustrated in
Referring to
A lens 18 is disposed in front of and in close proximity to side 16 of beam splitter 14 facing the mirror pair B and C. Another lens 20 is disposed in front of and in close proximity to the side adjacent side 16 of beam splitter 14 facing the mirror pair E and F. An auxiliary mirror 22 is disposed above and substantially in the same plane of the SLM 12 and located a distance d5 from side 16 of the beam splitter 14. Another auxiliary mirror 24 is disposed above the beam splitter 14 facing the mirror pair E and F and located a distance d4 from the adjacent side of the beam splitter 14. The surface area of lens 18 is large enough to cover both the side 16 of the beam splitter 14 and the mirror 22, and the surface area of lens 20 is large enough to cover both the adjacent side of the beam splitter 14 and the mirror 24.
One White cell of configuration 10 comprises the spatial light modulator 12, the mirror pair B and C, lens 18 and auxiliary mirror 22. The other White cell comprises the SLM 12, the mirror pair E and F, lens 20 and auxiliary mirror 24. Auxiliary mirror 24 may be replaced with a spot displacement optical element or elements for shifting the spots of light beams incident on it to new positions in the same plane of the auxiliary mirror 24 which will become more evident from the description found herein below. However, for the purposes of describing the operation of the exemplary dual White cell configuration, the auxiliary mirror 24 will be a simple mirror.
An exemplary operation of the dual White cell configuration of
If the polarization of the light beam is changed by the SLM 12, then the light beam returning from the SLM 12 will be directed to Mirror E instead of mirror C by the polarizing beam splitter 14. Mirror E will focus the light beam to a spot on the auxiliary mirror 24 via an optical path through lens 20. From mirror 24, the light beam will be directed back to mirror F and from there directed to the SLM 12 over an optical path through lens 20 and beam splitter 14. In the present embodiment, lens 18 images mirror B onto mirror C via the beam splitter 14 and SLM 12, and images mirror C onto mirror B via auxiliary mirror 22. Also, lens 20 images mirror E onto mirror F via auxiliary mirror 24, and images mirror F onto mirror E via the beam splitter 14 and SLM 12. It is known that the even-numbered bounces lie on an auxiliary mirror 22 or 24, and that the odd bounces will lie on the SLM 12.
In
As mentioned above, auxiliary mirror 24 may be replaced with a device that will shift a spot image to a new position on the same plane (in this case a new row on the face of the mirror). The distance by which a spot image is shifted will be different for different columns in the replaced auxiliary mirror 24. Each column may shift a light beam by a number of rows equal to twice that of the previous column, producing a binary counting system.
The spot image pattern for a single input beam on auxiliary mirror 24 and on the SLM 12 is shown in
If the mirror 24 is replaced with a spot displacement device (SDD) as noted above, a light beam going to the auxiliary mirror 24 (or more accurately, its replacement) on the second bounce may be shifted by one row (pixel). Likewise, a light beam incident on the SDD on the fourth bounce will be shifted by two rows, on the sixth bounce by four rows and so on. On any given bounce, if a light beam is not meant to be shifted, it is sent from the beam splitter 14 to auxiliary mirror 22 which does nothing except keep the light beam bouncing.
In the alternate embodiment of
In this alternate embodiment, the dual White cell configuration is modified to control the output location of the spot illumination. To do this, the MEMS tilting micro-mirror array 52 selects between two different paths on each light beam bounce. The two White cells produce a similar spot pattern on the MEMS array 52, but the illuminating spot images resulting from the White cell comprising the SDD 24′ are shifted such that they return in a different row of the MEMS array 52 than if they returned from the White cell comprising the mirror 22.
Referring to
The embodiment of
Let us assume that an input beam going from the plane of the MEMS array 52 is directed to mirror A, for example, after light beam bounce 1. A light image reflected from this spot on mirror A is imaged to a new spot image on auxiliary mirror 22, in a column 77 at the far left thereof as shown in
Accordingly, when micro mirror of the MEMS array 52 that the light beam strikes on bounce 3 is tipped to −θ, the light returns to auxiliary mirror 22 via mirror A and may be focused a spot in column 4, for example. On the other hand, if the micro mirror of the MEMS array 52 that the light beam strikes at bounce 3 is instead turned to +θ, then the light beam from mirror B will be reflected from the MEMS array 52 at an angle of +3θ along the plane of axis 76 with respect to the normal axis 72. Recall that there are two more mirrors E and F along the axis 76. So, when the reflecting micro mirror is set at +θ, a light beam from mirror B will be directed to mirror E instead of mirror A. In the present embodiment, a light beam is always directed to an upper mirror A or E from the MEMS array 52.
When a light beam is directed from MEMS array 52 to mirror E, the light beam is refocused to the SDD mirror 24′ and forms a spot image in a column 4 of that mirror, for example. From there the light beam is directed to the lower mirror F, and then back to the MEMS plane 52. Accordingly, mirrors E and F together with the MEMS array 52, lens 54, the SDD mirror 24′ and lens 20 comprise another White Cell of the embodiment. If the micro mirror in the MEMS array 52 struck by the light beam on bounce 5 is tilted to −θ, the light beam from mirror F is again directed to the other White cell (specifically to mirror A). Conversely, if the same micro mirror at bounce 5 is set tilted to +θ, the light beam from mirror F is instead reflected at +4θ, a direction that is not being used in this design, and the beam is lost.
Thus, according to the connectivity diagram shown in
Note also that an input light beam may be sent to mirror A from the MEMS array 52 every even-numbered bounce, and to mirror E every fourth bounce (i.e. 4, 8, 12 . . . ). Spot images from odd-numbered bounces always appear on the MEMS array 52, and spot images from the even-number bounces can appear either on auxiliary mirror 22 or SDD mirror 24′. The light beam may be directed to The SDD mirror 24′ by the MEMS array 52 on any particular even-numbered bounce, but when the light beam is directed there, four consecutive light beam bounces are required before the light beam may be sent to mirror 24′ again.
In the embodiment of
Shifting the spot images can control at which row any given input light beam reaches the output turning mirror and in the present example, each row may be associated with a different output. The number of possible outputs is determined by the total number of possible shifts for a given number of bounces. In the embodiment of
Nbinary=2m/4 (1)
where m is the number of bounces.
In the mirror face diagrams of
The example of
In operation, the “white” beam should be directed to the SDD 24′ on the fourth and twelfth bounces, which correspond to row displacements of 4Δ and Δ, respectively. Accordingly, the “white” beam may initially bounce in the A, B White Cell (i.e. the corresponding micro mirrors on the MEMS array 52 are tilted to −θ position) for three bounces. Then, the “white” beam is directed to the SDD 24′ on the fourth bounce (i.e. the corresponding micro mirror on the MEMS array 52 is tilted to +θ), and more particularly to the column in the SDD 24′ that has a shift value of 4Δ. After being shifted four rows in the SDD 24′, the “white” beam is directed back to the MEMS array 52 on the fifth bounce and images on the row four (4) instead of row zero (0). The “white” beam is then kept bouncing in the A, B White cell, until the 12th bounce, when it is again directed to the SDD 24′, and more specifically directed to land in the column with the shift value of Δ. After being shifted an additional row in the SDD 24′, the “white” beam is directed back to the MEMS array 52 on the next bounce and images on the row five (5) of the output column 40.
In a similar manner, the “shaded” beam may be shifted to the row two (2) of the output column 40 in twelve bounces (12). The “black” beam may be left unshifted throughout the 12 bounces to be output at row zero (0) of the output column 40.
So far the input to the configuration has been treated as a single beam. Instead of a single beam, let's assume that the input is an array of independent beams that may be referred to as the “input cell” 44 (see
To find the optimum shape of the input cell we need to consider the final size of the SLM 12 or micro mirrors in the MEMS device 52 employed on the White Cell. For ease of manufacturing, it is preferable to have a square-shaped SLM 12 or MEMS array 52. Thus, a relationship between the dimensions of the input cell 44 to the dimensions of the SLM 12 or MEMS array 52 will be determined. To do so, the number of spot image positions in the input cell 44 as a function of the number of bounces should be found. For any input cell, the number of spot positions or pixels (p q) is equal to the number of outputs (2m/2), which may be formulated in the following equation:
pq=2m/4 (1)
where m is the number of bounces on the White Cell.
The number of spot positions on the MEMS array 52 (or SLM 12) is a function of the number of outputs, and therefore of the number of bounces. Let's call X the number of spot positions on the vertical direction and Y the number of spot positions or micro mirrors on the horizontal direction on the MEMS array 52. So for any number of bounces the number of spot positions is:
So in order to have X=Y (a square MEMS array):
Substituting equation (1) into (4), after some simple manipulation we have:
p=(m/4)1/2 (5)
For a 32 bounce system (256 outputs) p=2.828, which can be rounded to 3 to have a input cell of 3×85 (actually it would be two columns of 86 spots plus one of 84 spots).
Next will be discussed how the shifts are produced in the substituted spot displacement device (SDD) 24′. Recall that the objective is to treat each virtual column on the face of SDD 24′ as an independent entity. A spot image from a light beam landing anywhere on the first column of the SDD 24′ will experience a displacement of Δ. This shifts the spot image onto the next row of the SDD 24′. A spot image directed to the second column will be shifted by a displacement of 2Δ (2 rows), a spot image directed to the third column will be shifted by 4Δ and so on.
Each column on the SDD 24′ will have a corresponding column on auxiliary mirror 22. Thus, as illustrated in
Imaging conditions also need to be fulfilled. The SDD 24′ may be analyzed independently from the White Cell. The SDD 24′ may change the position of the light beam and still meet the imaging conditions of the White Cell, as long as the properties of the light beams at the input and output of the SDD 24′ are the same (e.g. spot size, angle of propagation, . . . etc.). Based on these conditions, four different embodiments of the SDD 24′ are presented below by way of example. They are: 1) a roof prism; 2) a concatenated prism; 3) a lens train and 4) a waveguide SDD. All of them cause a spot displacement from the entrance cell array to the exit cell array in the same plane as shown in the illustration of
One approach to generating a spot displacement in the SDD 24′ is by using prisms disposed on the face thereof. The total internal reflection (TIR) caused by a prism may be taken advantage of to change the position of the input light beam to any desired position. TIR may occur when the incident light beam is in a higher refractive index medium striking an interface with a lower index medium at an angle greater than the critical angle. In this case, the light beam is reflected into the incident medium without losses. In
Referring to
a and 9b are isometric and side view perspectives of an exemplary prism 110 on the face 92 of the SDD 90. As shown in
The location of the light beam waist can be calculated with equation 6:
where z′ is the location of the new beam waist, zo is the Rayleigh distance and f is the focal length of the lens 116. Equation 6 will have a maximum and minimum distance at which the new beam waist will be placed. The beam's divergence will be reduced by making the location of the new waist z′ as distant as possible from the lens 116. This is achieved by using the smallest ratio
(short depth of focus and long focal length). It may be possible, depending on the beam characteristics, that several lenses may be needed, spaced at equal intervals, to produce longer shifts.
Another embodiment for the SDD 24′ referred to as the concatenated prism embodiment is also based on the use of total internal reflection. In this embodiment, several prisms may be joined together, so that the light traveling inside the joined prisms will experience TIR at the boundaries where the incident angle is greater than the critical angle. An exemplary concatenated prism embodiment 140 is illustrated in
One possible lens placement is shown in the illustration of
Yet another embodiment of the SDD 24′ is based on an optical waveguide built with lenses and referred to as a lens train. In
We now apply the stability condition as defined below:
where A is the element [1,1] of the matrix T and D is the element. [2,2] of the same matrix. Substituting eq. 7 into eq. 8 we have:
0≦d≦4f (9)
The lens train will be stable as long as the distance between the lenses doesn't exceed 4f. But it is preferred not to use a lens train on the SDD's input/output plane. It is desirable to take advantage of the stability of the train lens, but instead of lenses it is preferred to use spherical mirrors as shown in the lens train embodiment of
The lens train embodiment of
Referring to
The distance d from plane 200 to plane 210 may be again limited by the divergence of the beam. To calculate the distance d, the spot size at the input plane 200 should be considered. The smaller the spot size at the input plane 200, the faster the divergence and the smaller d can be. One way to overcome this condition is to use the embodiment illustrated in
where w(d) is the final beam radius, wo is the waist radius at upper plane, d is the distance from the beam waist to the second plane and zo is the Rayleigh distance, πω02/λ, where λ is the wavelength. In order to make w(d) twice wo, the distance d is then defined as:
d=√{square root over (3z0)}. (11)
The final size of this embodiment of the SDD will depend on the spot size at the input plane. The bigger the spot size, the lower the divergence will be, also the lower the astigmatism will be. Astigmatism is of concern because it can cause an elliptical spot shape which will cause coupling losses when going into a fiber, for example, at the output of the interconnection device.
There are ways to reduce the astigmatism on the SDD. One way involves the use of cylindrical lenses instead of the spherical lenses 214 in the lower plane 210 of the embodiment described in connection with
Astigmatism is analyzed in Appendix A to this specification.
In the lens train SDD embodiment, losses are generated during the multiple bounces inside the SDD. This is because the mirrors have finite reflectivity, as opposed to the TIR embodiments described herein above. Assuming 256 bounces, and a reflectivity of 0.995 for each mirror inside the SDD, a loss of: (0.995)256=0.2771 is likely to occur, which represents a loss of 5.57 dB. If a 0.999 reflecting coating is assumed, the losses are reduced to 1.11 dB, but the cost may increase.
Yet another embodiment of the SDD 24′ involves combining the already established manufacturing techniques of semiconductor devices, and simple geometric shapes, yielding an embodiment that is highly scalable, and of simple manufacture based on waveguides. This SDD embodiment uses waveguides rather than freespace as in foregoing described embodiments. The basic principle for a waveguide involves a medium of a particular refractive index that is surrounded by another material or materials with a lower refractive index. The light is transmitted through the inner medium (core) and by total internal refraction at the boundaries a light beam can travel long distances.
One way to increase this efficiency is to use what is referred to as a prism coupler.
βp=npko cos θp (12)
Where np is the refractive index of the prism 250 and ko is defined as:
ko=2π/λ0 (13)
where λ0 is the beam wavelength.
The transverse field extends outside the prism and decays exponentially in the space separating the prism and the core. If d is sufficiently small, the beam or wave is coupled to a mode of the waveguide with a matching propagation constant βp≈βwg, where βwg is given by equation 14:
βwg=√{square root over (k02)}ncore2−k2 (14)
where k is the effective refractive index and may be found by graphical methods.
The foregoing described operation may be reversed to make an output coupler, which extracts a light beam 258 from the waveguide as shown in the illustration of
There is another approach to coupling an optical beam 260 coming from a normal incidence angle into the waveguide by using diffraction gratings as shown in the cross-sectional view of
When using diffraction gratings, the efficiency depends on the degree of matching between optical field and waveguide mode. The coupling matching equation is:
where m is the order of the diffraction mode, θi is the incident angle to respect to the normal, and A is the grating period.
Note that the angle of diffraction may be controlled by altering the grating periods A or the incident angle θi. For coupling into a waveguide, βg should be matched to a mode of the waveguide.
In order to have 90-degree matching coupling from a normal incident beam(i.e θi, =0). and from equations 15 and 14, the grating period may be defined as:
where neff is defined as
Likewise, column 2 may include two waveguide sections 278 with each section 278 including an input grating coupler 280 and an output grating coupler 282. Accordingly, each section 278 of column 2 is configured to shift a light beam incident on its input grating coupler 280 a unit 2Δ before outputing the beam at the respective output grating coupler 282. The 1st column of the SDD 270 may include a waveguide section 284 with an input grating coupler 286 and an output grating coupler 288. Waveguide section 284 may be configured to shift a light beam 290 incident its input grating coupler 286 a unit 4Δ before outputing the beam at the respective output grating coupler 288.
An example of operation of the waveguide-based SDD 270 that illustrates the switching steps to send a particular input beam to the seventh output in three bounces on the SDD 270. To accomplish this operational description, the SDD 270 is virtually divided into eight (8) rows corresponding to outputs 0 to 7, respectively, as shown in
In the waveguide section 278, the beam is shifted two positions (2Δ) to the seventh row where it exits through an output grating 282 of section 278 (see dashed line). The beam is directed again to the White cell (see
A plurality of different embodiments for a spot displacement device (SDD) are used in an optical interconnection device by way of example. Two embodiments of the SDD are based on total internal reflection, one based on roof prisms in which an added array of micro lenses lowers the divergence of the input light beams and the other is based on a series of concatenated prisms also with a micro lens array at the input/output plane that decreases the beam divergence. Another SDD embodiment presented above is based on a lens train, in which the light divergence is controlled regardless the number of bounces. Yet another SDD embodiment is based on waveguides in which the light is coupled from free space to the waveguide. By coupling a free-space beam into a waveguide, the beam may propagate the necessary distance (shift) before coupling back the light into free-space.
For the waveguide-based SDD embodiment, the diffraction grating coupler offers an advantage over the prism coupler in that it can be made by regular semiconductor procedures, which facilitates the manufacture and reduces costs. An additional advantage that the grating coupler has over the prism coupler is of particular interest in our application in that it allows coupling to the waveguide coming from a normal incidence angle. Even though each SDD embodiment has specific characteristics, all of them share the same principle: each SDD column may produce a spot displacement twice the one produced by the previous SDD column (1Δ for the first column).
While the foregoing described SDD embodiments have been presented in connection with a binary White cell configuration optical interconnection device, it will be appreciated that they could be applied to other situations in which beams need to be displaced. In addition, the various embodiments described above were presented merely by way of example and not intended to limit the present invention in any way. Rather, the present invention should be construed in breadth and broad scope in accordance with the recitation of the claims appended hereto.
In this appendix, the astigmatism for the train lens SDD embodiment described herein above is analyzed for two different spot sizes and their maximum displacements. The objective is to compare the accumulated astigmatism to the depth of focus (DOF) of the system. In general, if the accumulated astigmatism is less than the DOF, then the astigmatism can be ignored and there is no need for correction. If, for a particular case, the accumulated astigmatism is larger that the-DOF, the astigmatism may have to be corrected at least to a value that is lower than the DOF.
Astigmatism is an optical aberration; it occurs when rays propagating in one plane are focused at one particular point and the rays traveling in a perpendicular plane focus at a different point along the optical axis.
Further along the optical axis 306, the rays 300 will come to a vertical focus 310 and create a horizontal line 312 as show in the illustration of
First of all, let assume a Gaussian beam with waist radius wo and a wavelength λ. To calculate the spot size at a distance z we use:
where w(z) is the spot size at z. From (A.1) we can calculate z as a function of w(z) as follows:
where zo is the Rayleigh range and is calculated as
Astigmatism may be measured as the absolute value of the difference between the sagittal focal length and the tangential focal length.
ΔT=abs(ft−fs) (A.3)
where ft and fs are given by:
and R is the radius of curvature of the spherical mirror. In Table A.1 we show the calculated astigmatism for a one-row-shift SDD for wo=5 μm and wo=10 μm.
We can see that the astigmatism is greatly reduced by just increasing the spot size. Table A.2 shows the accumulative astigmatism for a 8-position shift.
It can be seen from table A.2 that the accumulated astigmatism is greater than the depth of focus for both cases, so it will be necessary to correct it. One way to correct the astigmatism is by substituting the spherical mirror with the use of cylindrical mirrors instead of spherical ones. Another conclusion from Table A.2 is that the accumulated astigmatism decreases by increasing the spot size.
This utility application claims the benefit of the filing date of the U.S. Provisional Application 60/588,732, entitled “Spot Displacement Device For White Cell-Based Binary Optical Interconnection Device”, and filed Jul. 16, 2004.
Number | Name | Date | Kind |
---|---|---|---|
3428391 | Newcomer | Feb 1969 | A |
3463571 | Boehm et al. | Aug 1969 | A |
3755676 | Kinsel | Aug 1973 | A |
3892468 | Duguay | Jul 1975 | A |
4225938 | Turpin | Sep 1980 | A |
4344671 | Lang | Aug 1982 | A |
4474434 | Carlsen et al. | Oct 1984 | A |
4474435 | Carlsen et al. | Oct 1984 | A |
4546249 | Whitehouse et al. | Oct 1985 | A |
4929956 | Lee et al. | May 1990 | A |
5018816 | Murray et al. | May 1991 | A |
5018835 | Dorschner | May 1991 | A |
5117239 | Riza | May 1992 | A |
5231405 | Riza | Jul 1993 | A |
5274385 | Riza | Dec 1993 | A |
5276758 | Hughes | Jan 1994 | A |
5319477 | DeJule | Jun 1994 | A |
5329118 | Riza | Jul 1994 | A |
5418880 | Lewis et al. | May 1995 | A |
5463497 | Muraki et al. | Oct 1995 | A |
5465175 | Woodgate et al. | Nov 1995 | A |
5475525 | Tournois et al. | Dec 1995 | A |
5512907 | Riza | Apr 1996 | A |
5592333 | Lewis | Jan 1997 | A |
5623360 | Gesell et al. | Apr 1997 | A |
5724163 | David | Mar 1998 | A |
5726752 | Uno et al. | Mar 1998 | A |
5767956 | Yoshida | Jun 1998 | A |
5852693 | Jeong | Dec 1998 | A |
5859967 | Kaufeld et al. | Jan 1999 | A |
5936759 | Buttner | Aug 1999 | A |
5973727 | McGrew et al. | Oct 1999 | A |
6014244 | Chang | Jan 2000 | A |
6040880 | Tsuboi | Mar 2000 | A |
6064506 | Koops | May 2000 | A |
6181367 | McGrew et al. | Jan 2001 | B1 |
6188817 | Goodfellow | Feb 2001 | B1 |
6236506 | Cao | May 2001 | B1 |
6266176 | Anderson et al. | Jul 2001 | B1 |
6323981 | Jensen | Nov 2001 | B1 |
6388815 | Collins, Jr. et al. | May 2002 | B1 |
6429976 | Yamamoto et al. | Aug 2002 | B1 |
6480323 | Messner et al. | Nov 2002 | B1 |
6522404 | Mikes et al. | Feb 2003 | B2 |
6525889 | Collins, Jr. et al. | Feb 2003 | B1 |
6535340 | Saruwatari | Mar 2003 | B1 |
6637899 | Sunaga et al. | Oct 2003 | B2 |
6647164 | Weaver et al. | Nov 2003 | B1 |
6674939 | Anderson et al. | Jan 2004 | B1 |
6711316 | Ducellier | Mar 2004 | B2 |
6724535 | Clabburn | Apr 2004 | B1 |
6724951 | Anderson et al. | Apr 2004 | B1 |
6734955 | Wight et al. | May 2004 | B2 |
6760140 | Argueta-Diaz et al. | Jul 2004 | B1 |
6816307 | Sun | Nov 2004 | B1 |
6922277 | Moon et al. | Jul 2005 | B2 |
6934069 | Moon et al. | Aug 2005 | B2 |
6952306 | Anderson | Oct 2005 | B1 |
6958861 | Argueta-Diaz | Oct 2005 | B1 |
7171068 | Bartlett et al. | Jan 2007 | B2 |
7215474 | Argueta-Diaz | May 2007 | B2 |
7236238 | Durresi et al. | Jun 2007 | B1 |
20020030814 | Mikes et al. | Mar 2002 | A1 |
20030202731 | Ionov et al. | Oct 2003 | A1 |
20040190823 | Leuthold et al. | Sep 2004 | A1 |
20050007668 | Serati et al. | Jan 2005 | A1 |
20060034567 | Anderson et al. | Feb 2006 | A1 |
20060061893 | Anderson et al. | Mar 2006 | A1 |
20060062517 | Anderson et al. | Mar 2006 | A1 |
20060114568 | Argueta-Diaz | Jun 2006 | A1 |
Number | Date | Country |
---|---|---|
10333089 | Dec 1998 | JP |
WO 0114924 | Mar 2001 | WO |
WO 0229436 | Apr 2002 | WO |
WO 03075048 | Sep 2003 | WO |
WO 03083521 | Oct 2003 | WO |
WO 03083541 | Oct 2003 | WO |
Number | Date | Country | |
---|---|---|---|
20060044987 A1 | Mar 2006 | US |
Number | Date | Country | |
---|---|---|---|
60588732 | Jul 2004 | US |