OPTICAL SYSTEM FOR DISPLAY PANEL
BACKGROUND OF THE INVENΗON Field ofthe Invention
The present invention relates generally to the field of display devices. In particular, the present invention relates to an optical system and method for coupling an image onto a display device. More specifically, the present invention relates to an optical
system and method for coupling an image onto an ultrathin planar optical display device which is capable of reducing or eliminating distortions that typically occur when an image is projected onto a display device which is tilted in relation to the incident image.
Description ofthe Background
Optical screens typically use cathode ray tubes (CRTs) for projecting images onto the screen. The standard TV screen has a width to height ratio of 4:3 with 525 vertical lines of resolution. An electron beam is scanned both horizontally and vertically across the screen to form a number of pixels which collectively form the image.
Conventional cathode ray tubes have a practical limit in size, and are relatively deep to accommodate the required electron gun. Larger screens are available which typically include various forms of image projection. However, such screens have various viewing shortcomings including limited viewing angle, resolution, brightness, and
contrast, and such screens are typically relatively cumbersome in weight and shape. Furthermore, it is desirable for screens of any size to appear black in order to improve viewing contrast. However, it is impossible for direct view CRTs to actually be black
because they utilize phosphors to form images, and those phosphors are non-black.
Optical panels may be made by stacking optical waveguides, each waveguide having a first end and a second end, wherein an outlet face is defined by the plurality of first ends, and wherein an inlet face is defined by the plurality of second ends. Such a
panel may be thin in its depth compared to its height and width, and the cladding ofthe
waveguides may be made black to increase the black surface area, but such a panel may require expensive and cumbersome projection equipment to distribute the image light across the inlet face, which equipment thereby increases the total size and cost ofthe panel.
Therefore, the need exists for an optical panel which possesses the advantages corresponding to a stacked waveguide panel, but which does not require the use of expensive and cumbersome projection equipment, nor suffer from the increase in size and cost necessitated by such equipment.
In optical panels where the depth ofthe housing (containing the optical panel and projection equipment) is desired to be at a minimum, the projection equipment is typically positioned to accommodate these overall dimension constraints. The positioning ofthe projection equipment may therefore require the image path to be directed at an acute angle with respect to the targeted outlet face ofthe panel. Thus,
since the surface ofthe outlet face is generally highly tilted relative to the image path, an imaging system which is capable of producing an image which is focused and is without
distortions is critical. Not only is a properly focused image desired, but an image
produced on the surface ofthe outlet face must also have little or no chromatic distortion and must retain the desired aspect ratio while mamtaining a linear point-to-point mapping ofthe image.
Therefore, the need also exists for an optical system for an optical panel which is capable of producing an accurate image on a highly tilted inlet face surface relative to the image path, and which does not suffer from improperly focused images and image distortions which yield chromatic distortions, false aspect ratios, and inconsistent, linear point-to-point mapping ofthe image.
SUMMARY OF THE INVENTION
The present invention is directed to an optical system for projecting an image onto a display image plane at an incident angle which is greater than zero. The optical system comprises an image source and an imaging element. The imaging element creates an image from the image source. The optical system also comprises an anamorphic
telescope for reducing anormorphic distortion ofthe image, and a final mirror for reflecting the image toward the display image plane. The anamorphic telescope reduces magnification ofthe image in a first direction and enlarges magnification ofthe image in a second direction which is perpendicular to the first direction. Moreover, the anamorphic telescope includes a first lens group, a second lens group, and a third lens group. The first lens group and the second lens group form a first anamorphic telescopic
system, and the second lens group and the third lens group form a second anamorphic telescopic system. The anamorphic telescope also may be constructed of more than one
optical material tocorrect chromatic aberrations ofthe image. The present invention is also directed to a display system which includes the combination of an optical system and an optical panel.
The present invention solves problems experienced in the prior art, such as the use of expensive and cumbersome projection equipment, by providing an optical system
having a reduced optical path that produces an accurate image on a highly tilted inlet face surface relative to the image path, and which does not suffer from chromatic distortion, improperly focused images, image distortions which yield false aspect ratios or
inconsistent point-to-point mapping to the image. The present invention also retains the advantages which correspond to a stacked waveguide panel, such as improved contrast and minimized depth ofthe panel and surrounding housing.
Those and other advantages and benefits ofthe present invention will become
apparent from the detailed description ofthe invention hereinbelow.
BRIEF DESCRIPTION OF THE SEVERAL VIEWS OF THE DRAWINGS
For the present invention to be clearly understood and readily practiced, the
present invention will be described in conjunction with the following figures, wherein:
FIG. 1 is an isometric view partly cross sectional schematic illustrating an ultrathin optical panel;
FIG. 2 is a side view cross sectional schematic of an ultrathin optical panel and a
light generation system;
FIG. 3 is a schematic illustrating a horizontal and vertical cross section of an
ultrathin optical panel using a prismatic coupler;
FIG. 4 is a simplified rear view schematic illustrating an optical system in conjunction with an optical panel;
FIG. 5 is a side view schematic of an ultrathin optical panel using a preferred
optical system.
FIG. 6 is a detailed side view illustrating lens elements in the preferred optical system ofthe type generally depicted in FIG. 5 in conjunction with an optical panel;
FIG. 7 is a detailed rear view illustrating the lens elements in the preferred optical
system ofthe type generally depicted in FIG. 5 in conjunction with an optical panel;
FIG. 8 is a detailed rear view illustrating lens elements and a folding mirror in an alternate optical system in conjunction with an optical panel;
FIG. 9 is a detailed rear view illustrating lens elements and a folding mirror in
another alternate optical system in conjunction with an optical panel;
FIG. 10 is a detailed rear view illustrating lens elements and two folding mirrors in a further alternate optical system in conjunction with an optical panel;
FIG. 11 is a spot diagram illustrating image focusing performance using a preferred optical system and an optical panel; and
FIG. 12 is a grid distortion plot diagram illustrating image distortion using a preferred optical system and an optical panel.
DETAILED DESCRIPTION OF THE INVENTION
It is to be understood that the figures and descriptions ofthe present invention have been simplified to illustrate elements that are relevant for a clear understanding of
the present invention, while eliminating, for purposes of clarity, many other elements
found in a typical optical display panel. Those of ordinary skill in the art will recognize that other elements are desirable and/or required in order to implement the present invention. However, because such elements are well known in the art, and because they
do not facilitate a better understanding ofthe present invention, a discussion of such elements is not provided herein.
For purposes of this disclosure, the phrase "optical waveguide" is defined so as to include any type of light guiding member that utilizes total internal reflection to guide
light.
FIG. 1 is an isometric view schematic illustrating an optical panel 10. The optical
panel 10 includes a plurality of waveguides 10a, wherein one end of each waveguide 10a forms an inlet for that waveguide, and wherein the opposite end of each waveguide 10a forms an outlet for that waveguide, a light generation system 12, a housing 14 in which
the light generation system 12 and the plurality of waveguides 10a are mounted, and a coupler 16.
Each waveguide 10a extends horizontally, and the plurality of stacked waveguides 10a extends vertically. The plurality of inlet ends define an inlet face 20 for
receiving image light 22. The plurality of outlet ends define an outlet face 24 disposed substantially parallel with the inlet face 20 for displaying light 22. The light 22 may be displayed in a form such as, but not limited to, a video image 22a.
The housing 14 is sized larger in height and width than the combination of he
light generation system 12 and the plurality of waveguides 10a, to allow the placement of
tl e plurality of waveguides 10a and light generation system 12 therein. The housing 14 has an open front to allow for viewing ofthe outlet face 24, and has a closed depth D looking from the open front to the back ofthe housing 14.
The light generation system 12 provides the light 22 viewed through the waveguides 10a. The light generation system 12 includes a light source 30, and a light redirection element 32 that redirects incident light 22 from the light source 30 into the coupler 16, which light redirection element 32, in combination with the coupler 16,
allows for a reduction in the depth D ofthe housing 14. This reduction allowance occurs where the light redirection element 32 is configured for turning the light 22 from a source 30, which source 30 is placed within the housing 14 proximate to and parallel with the vertical stack ofthe plurality of waveguides 10a, into the coupler 16, which then acutely turns the light 22 into the waveguides 10a. The coupler 16 is preferably effective for turning the image light in an exemplary range of about 45° up to about 90°, in order to generate approximately horizontal transmission through the plurality of waveguides 10a.
The light generation system 12 may also include a modulator 62 and further imaging optics 64 and is discussed with more particularity with respect to FIG. 2.
The parallel surfaces ofthe inlet face 20 and the outlet face 24 allow the panel 10 and enclosing housing 14 to be made ultrathin in depth. The panel 10 has a nominal
thickness T which is the depth ofthe waveguides 10a between the inlet face 20 and the outlet face 24, and thickness T is substantially less than the height H and width W ofthe
outlet face 24. The panel 10 may be configured in typical television width to height ratios of 4:3 or 16:9, for example. For a height H of about 55 cm and a width W of about 73 cm, the panel thickness T ofthe present invention may be about 1 cm. The depth D may vary accordingly with the thickness T, but, in the embodiment described hereinabove, the depth D ofthe housing 14 is preferably no greater than about 17 cm.
FIG. 2 is a side view cross sectional schematic of an ultrathin optical panel 10.
The panel 10 includes a plurality of stacked waveguides 10a, a light generation system 12, a coupler 16, and a housing 14.
The light generation system 12, in one embodiment ofthe present invention, includes a projector 60 which is optically aligned with a light redirection element 32. An image is projected onto the light redirection element 32, and is then redirected to the coupler 16 for transmission through the waveguides 10a for display on the outlet face 24. In a preferred embodiment, the projector 60 is disposed adjacent to the top ofthe inlet
face 20 for projecting the image light 22 generally parallel thereto, and is spaced therefrom a distance sufficient to allow for a turning ofthe image light 22 from the light
redirection element 32 into the coupler 16 for transmission through the waveguides 10a.
The projector 60 may include a suitable light source 30 for producing the light 22. The light source 30 may be a light bulb (e.g. filament or arc type) or laser. The projector 60 may be a slide projector or video projector which may include a modulator 62 for
modulating the light 22 to form an image 22a. The modulator 62 may be, for example, a conventional Liquid Crystal Display (LCD), a Digital Micromirror Device (DMD), a
GLV, a laser raster scanner, a PDLC, an LCOS, a MEMS, or a CRT. The projector 60 may also include suitable image optics 64 for distributing or broadcasting tine image light 22 horizontally and vertically across the light redirection element 32 for properly
focused transmission to the coupler 16. The image optics 64 may include focusing and
expanding lenses and/or mirrors. One or more light generation systems 12, such as between 2 and 4 such systems, may be used to provide light to one or more portions of the coupler 16. Expansion lenses may be used for both the imaging optics 64 and the light redirection element 32 to expand the image light 22 both vertically and horizontally over the coupler 16. Alternatively, suitable rastering systems may be used as the light generation system 12 to form the image by rastering the image light 22 both horizontally
and vertically across tl e coupler 16.
In the illustrated embodiment, the light 22 is initially projected from the projector
60 vertically downward inside the housing 14 to the bottom thereof where the light
redirection elements 32 are mounted, and the light redirection elements 32 then redirect the image light 22 vertically upwardly at a large angle relative to the surface normal of the panel 10 for broadcast over the entire exposed surface ofthe coupler 16. In an alternative embodiment, the projector 60 could be placed beneath or to either side ofthe
inlet face 20 rather than behind the inlet face 20.
The allowable incidence angle ofthe image light 22 on the coupler 16 is determined by the capability ofthe coupler 16 to turn the light 22 into the inlet face 20 of
the panel 10. The greater the turning capability ofthe coupler 16, the closer the projector
60 may be mounted to the coupler 16 for reducing the required depth D ofthe housing 14.
FIG. 3 is a schematic illustrating a horizontal and vertical cross section of an ultrathin optical panel 10. The panel 10 includes a plurality of vertically stacked optical waveguides 10a, a light generation system 12 (see FIG. 2), a coupler 16, and a housing 14.
Each waveguide 10a ofthe plurality of waveguides 10a includes a central transparent core 80 having a first index of refraction. The core 80 may be formed of any
material known in the art to be suitable for passing light waves therethrough, such as, but
not limited to plexiglass or polymers. The central core 80 may be formed of an optical plastic, such as Lexan®, commercially available from the General Electric Company®, or glass, such as type BK7. A preferred embodiment ofthe present invention is implemented using individual glass sheets, which are typically in the range between 2
and 1000 microns thick, and which may be of a manageable length and width. The central core 80 is laminated between at least two cladding layers 82. The cladding layers 82 immediately in contact with the cores 80 have a second index of refraction lower than
that ofthe cores 80, thus allowing for substantially total internal reflection ofthe light 22
as it is transmitted through the cores 80. The cladding 82 may be a suitable plastic, plexiglass, glass, adhesive, polyurethane, low refractive index polymer, or epoxy, for example, and is preferably black in color. Where multiple cladding layers 82 are used, it
is preferable that a clear cladding layer contact the glass, and a black pigmented layer be disposed between adjacent clear cladding layers, thus improving both viewing contrast of the outlet face 24 and internal reflection ofthe light 22 through the core 80. The use of at least one black pigmented layer provides improved contrast by providing additional
blackness at the outlet face 24. Further, the exposed edges ofthe black pigmented layer at the outlet face 24 are directly viewable by the observer. Additionally, ambient light
which enters the waveguides off-axis through the outlet face 24 will be absorbed internally by the black pigmented layer. The black pigmented layer may be formed in any suitable manner such as with black spray paint, or carbon particles within an epoxy adhesive joining together the adjacent cores 80 in one or more black pigmented layers.
The manner of forming the cladding layers 82 and cores 80 is discussed with more specificity hereinbelow.
The waveguides 10a of a preferred embodiment are in the form of flat ribbons extending continuously in the horizontal direction along the width ofthe outlet face 24.
The ribbon waveguides 10a are preferably stacked vertically along the height ofthe outlet
face 24. The vertical resolution ofthe panel 10 is thus dependent on the number of waveguides 10a stacked along the height ofthe outlet face 24. For example, a stacking of 525 waveguides would provide 525 vertical lines of resolution. A greater number of waveguides can of course be envisioned resulting in a higher corresponding resolution.
The plurality of stacked waveguides 10a may be formed by first laying a first
glass sheet in a trough sized slightly larger than the first glass sheet. The trough may then be filled with a thermally curing epoxy. The epoxy is preferably black, in order to form a black layer between waveguides, thereby providing improved viewing contrast.
Furthermore, the epoxy should possess the properties of a suitable cladding layer 82, such as having a lower index of refraction than the glass sheets to allow substantially total internal reflection ofthe light 22 within the glass sheet. After filling ofthe trough,
glass sheets 80 are repeatedly stacked, and a layer of epoxy forms between each glass
sheet 80. The stacking is preferably repeated until between approximately 500 and 2000 sheets have been stacked. Uniform pressure may then be applied to the stack, thereby causing the epoxy to flow to a generally uniform level between glass sheets 80. In a
preferred embodiment of he present invention, the uniform level obtained is
approximately .0002" between glass sheets 80. The stack may then be baked to cure at an elevated temperature for such time as is necessary to cure the epoxy, and the stack is then allowed to cool slowly in order to prevent cracking ofthe glass. After curing, the stack may be placed against a saw, such as, but not limited to, a diamond saw, and cut to
a desired size. The cut portions ofthe panel 10 may then be polished to remove any saw marks.
In an alternative embodiment ofthe present invention, a plurality of glass sheets 80 are individually coated with, or dipped within, a substance having an index of refraction lower than that ofthe glass, and the plurality of coated sheets are fastened
together using glue or thermally curing epoxy, which is preferably black in color. A first coated glass sheet 10a is placed in a trough sized slightly larger than the first coated glass
sheet 10a, the trough is filled with a thermally curing black epoxy, and the coated glass sheets 10a are repeatedly stacked, forming a layer of epoxy between each coated glass sheet 10a. The stacking is preferably repeated until between approximately 500 and 2000 sheets have been stacked. Uniform pressure may then be applied to the stack, followed by
a cure ofthe epoxy, and a sawing ofthe stack into a desired size. The stack may be
sawed curved or flat, and may be frosted or polished after sawing.
In another alternative embodiment of he present invention, the glass sheets 80 preferably have a width in the range between 0.5" and 1.0", and are of a manageable
length, such as between 12" and 36". The sheets 80 are stacked, with a layer of black ultraviolet adhesive being placed between each sheet 80. Ultraviolet radiation is then used to cure each adhesive layer, and the stack may then be cut and/or polished.
After sawing and/or polishing the stack, each ofthe above embodiments ofthe method may also include bonding a coupler 16 to the inlet face 20 ofthe stack, and
fastening the stack, having the coupler 16 bonded thereto, within the rectangular housing
14. The stack is fastened such that the open front ofthe housing 14 is aligned with the
outlet face 24, and the light generator 12 within the housing 14 is optically aligned with the coupler 16.
The light generation system 12 provides light 22 which is incident on the coupler 16, and is configured substantially as discussed with respect to FIG. 2. The light source
30 ofthe light generation system 12 may be mounted within the housing 14 in a suitable
location to minimize the volume and depth ofthe housing 14. The source 30 can be mounted within the housing 14 directly behind the inlet face 20 at the top thereof to initially project light 22 vertically downwardly, which light 22 is then turned by light redirection elements 32 ofthe light generation system 12 vertically upwardly to optically
engage the coupler 16. In a preferred embodiment ofthe present invention, the individual waveguides 10a extend horizontally without inclination, thus allowing the image to be transmitted directly horizontally through the waveguides 10a for direct
viewing by an observer, thereby allowing the viewer to receive full intensity ofthe light 22 for maximum brightness. Another embodiment could include inclination ofthe waveguides 10a. A sheet of diffusing material may optionally be provided on the outlet face 24 to effect an improved viewing angle ofthe display. Alternatively, instead of a
sheet of diffusing material, a diffusing surface may be formed into the outlet face 24
itself to effect a similarly improved viewing angle. Thus, for maximum brightness, the light 22 incident from the light generation system 12 must be turned substantially
horizontally. A prismatic coupler 16 may be used to turn the light at an angle up to 90
degrees for entry into the inlet face 20. In one embodiment ofthe present invention, a Transmissive Right Angle Film (TRAF) turns the light at an angle of 81 degrees.
The light coupler 16 adjoins the entire inlet face 20 and may be suitably bonded thereto for coupling or redirecting the light 22 incident from the light generation system
12 into the inlet face 20 for transmission through the waveguides 10a. The waveguides 10a (i.e. more specifically, cores 80) ofthe present invention may have a limited
acceptance angle for receiving incident light 22, and the coupler 16 is aligned to ensure that the image light 22 is suitably turned to enter the waveguide cores 80 within the allowable acceptance angle.
In a preferred embodiment ofthe present invention, the coupler 16 includes
prismatic grooves 16a that are straight along the width ofthe inlet face 20 and are spaced
vertically apart along the height ofthe inlet face 20, which prismatic coupler 16 is capable of turning light up to an angle of 90 degrees. In another preferred embodiment ofthe present invention, the prismatic coupler 16 is a TRAF commercially available from the 3M Company® of St. Paul, Minneapolis, under the tradename TRAF π®. An
optional reflector may be disposed closely adjacent to the prismatic coupler 16 for reflecting back into the waveguides 10a any stray light 22 at the grooves 16a. As still
another preferred embodiment ofthe present invention, the coupler 16 (or light
redirecting surface) may instead be formed into the inlet face 20 itself.
The coupler 16 may also take the form of a diffractive element 16. The diffractive coupler 16 includes a diffractive grating having a large number of small grooves extending horizontally and parallel with the individual waveguides 10a, which
grooves are closely spaced together in the vertical direction over the height ofthe inlet
face 20. The coupler 16 may take other forms as well, including, but not limited to, holographic or Fresnel elements. It may also be envisioned that a coupler 16 may
optionally be omitted from the panel 10 depending on the orientation ofthe panel 10 with respect to the optical system employed.
The housing 14 supports the waveguide stack 10a and the light generation system 12 in a substantially closed enclosure. The outlet face 24 faces outwardly and is exposed to the viewer and ambient light, and the inlet face 20 and adjoining coupler 16 face inwardly toward preferably black surfaces within the housing 14, thereby providing
additional black for contrast at the outlet face 24. This additional black is provided at the
outlet face 24 due to the passive nature ofthe waveguides 10a and the coupler 16. When these passive devices are enclosed in a black area, the outlet face 24 will appear black when not illuminated by image light 22 incident on the inlet face 20.
FIG. 4 is a simplified rear view schematic illustrating an optical system 100 (i.e.
excluding the panel 10) used to project an image from an image source 110 onto an
optical panel 10 (also shown for illustration purposes in FIG. 4). The optical system 100
may replace the light generation system 12 as described above in conjunction with FIG. 2. The optical system 100 includes an image source 110, an imaging element 120, an anamorphic telescope 130, and a final mirror 140. The optical panel 10 may be ofthe type described in the above embodiments with respect to Figures 1-3. Alternatively, the optical panel 10 may be of different type dependent on design choice or routine
experimentation by the skilled artisan. For example, the optical panel 10 may be a
conventional lenticular rear projection screen. The image source 110, imaging element 120, anamorphic telescope 130, and final mirror 140 are preferably all nominally symmetric about a single plane that ideally contains all ofthe centers of curvature ofthe
optical elements. For purposes of this discussion only, this plane will be referred to herein as the "y-z plane".
As used herein, the incident angle θ is defined as the angle formed between a line
drawn from the center ofthe image source to the center ofthe display image plane, and a line perpendicular to the display image plane. As illustrated in FIG. 5, the line from the center ofthe image source to the center ofthe display image plane is reflected via final
mirror 140. The image is projected onto the display image plane at an incident angle θ
preferably greater than zero. In a preferred embodiment ofthe invention, incident angle
θ is in the range of approximately 50° - 85°. In a more preferred embodiment ofthe
invention, incident angle θ is approximately 78°.
Since the tilt associated with this configuration is substantial, optical tilting ofthe
image source or plane is preferably spread out gradually over the entire optical train. In other words, the optical elements in the optical train, i.e. the imaging element 120, the anamorphic telescope 130, and the final mirror 140, each effect a tilt on the image o the
object. However, it is possible to accomplish this using only one or some ofthe optical elements in the optical train. The image source 110 and the imaging element 120 are
each tilted about the x-axis. Tilting the image source 110, the imaging element 120, and
panel 10 in this way makes use ofthe Scheimpflug rule to effect an intermediate tilt on the virtual intermediate image plane.
The imaging element 120 creates a virtual image in a virtual intermediate image plane at an angle intermediate to the angle between the plane ofthe image source 110
(the "object plane") and the targeted inlet face 20 plane (the "display image plane"). The anamorphic telescope 130 and final mirror 140 are also tilted about the x-axis to effect a
further tilt ofthe final image plane. Although the tilting by the anamorphic telescope 130
is not required for the optical system 100 to produce a tilted image, it is useful to provide some degree of tilt by the anamorphic telescope 130 to thereby improve image quality.
The image source 110 may be an illuminated object, e.g. an LCD or a DMD, or an emissive object, e.g. an LED array or a laser. In a preferred embodiment, the image source 110 is a chromatic image-combining projector. The imaging element 120 enlarges magnification of an image from the image source 110 in a first direction and in a
second direction which is perpendicular to the first direction. In a preferred embodiment, the imaging element 120 enlarges magnification of an image from the image source 110
equally in a first direction and in a second direction which is perpendicular to the first direction. The imaging element 120 may include at least one lens which is comprised of a low color dispersion material, and at least one additional lens which is comprised of a
high color dispersion material such that chromatic aberration (i.e. in both lateral and longitudinal directions) ofthe image is corrected. For purposes of this disclosure, low
color dispersion material is a material which exhibits less color separation associated with it when light refracts at it's surface as compared to a high color dispersion material.
Examples of low color dispersion materials are acrylic and Zeonex®. Zeonex® is commercially available by Zeon Chemicals in Louisville, Kentucky. Examples of high color dispersion materials are polystyrene and polycarbonate. Other low and high color dispersion materials may of course be used in the practice of this invention.
When light refracts at the surface of a lens, for example, constructed of a low
color dispersion material, longitudinal color separation occurs. After the light has traversed through the lens and is refracted again at the second surface, both longitudinal
color separation and lateral color offset may be present. It is possible to utilize a second lens constructed of a high color dispersion material and having a compensating shape so
that when positioned adjacent to or in the vicinity ofthe first lens, the effect is to undo the color separation and color offset. In a preferred embodiment, a first lens is
constructed of a low color dispersion material which causes the color spread which may be undone by positioning a second lens constructed of a high color dispersion material adjacent to or in its vicinity. Of course, the first lens may alternatively be a high color
dispersion material followed by a compensating second lens of low color dispersion material. Utilizing a pair of materials exhibiting dissimilar color dispersion values allows each pair to function similarly to a (combined) singular element, i.e. without any color separation. In utilizing this type of "paired materials" for each lens group, colors
never separate beyond the respective lens groups and all the colors follow the same or
similar optical path.
A majority ofthe color correction is performed in the imaging element 120. In a preferred embodiment, the imaging element 120 includes three lenses which are comprised of a low color dispersion material, and two lenses which are comprised of a
high color dispersion material. The individual lenses which comprises the imaging element 120 are illustrated in detail in FIGs. 6-10. The imaging element 120 comprises at least one rotationally symmetric surface and the lenses comprising the imaging element 120 are comprised of either glass or plastic or a combination of glass and plastic. The imaging element 120 may comprise at least one surface ofthe spherical, aspherical, diffractive, or Fresnel type, or a combination of these surface types. Also, the imaging
element 120 comprises at least one lens which is tilted and decentered with respect to a
central longitudinal optical axis ofthe image source 110. Preferably, the imaging element 120 consists of lenses which are all tilted and decentered as an entire group with respect to the central longitudinal optical axis ofthe image source 110.
The anamorphic telescope 130 is provided in the optical system 100 mainly for
reducing anamorphic distortion ofthe image and is preferably positioned subsequent the imaging element 120 within the optical path ofthe optical system 100. Although, in
some configurations, it may be desirable to position the imaging element 120 subsequent the anamorphic telescope 130 within the optical path ofthe optical system 100. For
purposes of this disclosure, a fully focused anamorphic optical system has different magnification of an image in a first direction (e.g. horizontal) than in a second direction (e.g. vertical) which is perpendicular to the first direction. In a display system where a focused 4:3 projected image is to be displayed on a display image plane which is tilted
dramatically about a horizontal axis, the horizontal extent ofthe image is relatively
unaffected while the vertical extent ofthe image is significantly elongated. A conventional anamorphic optical system would typically either shrink the elongated
image vertically while leaving the horizontal aspect ofthe image unaffected, or enlarge the elongated image horizontally while leaving the vertical aspect ofthe image
unaffected. This type of "classic" anamorphic system utilizes two lens groups and may be referred to as a type of anamorphic telescope. However, utilizing a classic
anamorphic telescope (i.e. consisting of two lens groups) provides all the anamorphic
correction into one axis. To use this approach to achieve the result ofthe present
invention, very powerful optic lenses would be required that could yield serious design problems, such as the inability to provide pre-correction of trapezoidal image distortion (otherwise known as "keystone-type" distortion) resulting from utilizing a highly tilted display image plane, chromatic aberration and poor focus ofthe image.
To overcome the aforementioned drawbacks of a classic anamoφhic telescope,
the anamorphic telescope 130 of the present invention is utilized. The anamorphic telescope 130 reduces magnification ofthe image in a first direction and enlarges magnification ofthe image in a second direction which is perpendicular to the first direction. The anamoφhic telescope 130 includes three lens groups, i.e. a first lens
group 131, a second lens group 132, and a third lens group 133. The first lens group 131 and the second lens group 132 form a first anamoφhic telescopic system. The second
lens group 132 and the third lens group 133 form a second anamoφhic telescopic system. The first anamoφhic telescopic system is used to reduce magnification ofthe image in a
first direction, while the second anamoφhic telescopic system enlarges magnification of the image in a second direction which is peφendicular to the first direction. The
functions ofthe first and second anamoφhic telescopic systems may optionally be
reversed. In other words, the second anamoφhic telescopic system may be used to reduce magnification ofthe image in the first direction, while the first anamoφhic telescopic system enlarges magnification ofthe image in the second direction.
It is apparent that the second lens group 132 has the dual role of functioning as a
lens group for both the first anamoφhic telescopic system and the second anamoφhic telescopic system. The utilization ofthe second lens group 132 in this fashion (i.e. as part of both the first anamoφhic telescopic system and the second anamoφhic telescopic system) enables tlie optical system to provide a relatively gentle (i.e. as compared to a
classic anamoφhic system) reduction ofthe image in the first direction by having relatively gentle (i.e. as compared to a classic anamoφhic system) expansion ofthe image in the second direction, all the while providing a compact optical system. The combined use ofthe first anamoφhic telescopic system to reduce magnification ofthe image in the first direction and the second anamoφhic telescopic system to enlarge magnification ofthe image in the second direction result in an accurate final aspect ratio
ofthe image that has consistent linear point-to-point mapping ofthe image.
Within each ofthe three lens groups, there is at least one cylindrical or bi-laterally symmetrical element which may have an aspherical surface. In a preferred embodiment, the first lens group 131 comprises two off-axis rotationally symmetric surfaces and two
conic cylindrical surfaces although it may be envisioned that more or less lenses may be
utilized within the scope ofthe invention. The first lens group 131 produces negative power in the first direction and positive power in the second direction which is peφendicular to the first direction. The first lens group 131 may include at least one lens
which is comprised of a low color dispersion material, and at least one additional lens which is comprised of a high color dispersion material such that chromatic aberration of the image is corrected. Examples of low color dispersion materials are acrylic and
Zeonex®. An example of a high color dispersion material is polystyrene. Other low and high color dispersion materials may of course be used in the practice of this invention. In a preferred embodiment, the first lens group 131 includes one lens which is comprised of a low color dispersion material, and another lens which is comprised of a high color dispersion material. The individual lenses which comprises the first lens group 131 are
illustrated in detail in FIGs. 6-10. The first lens group 131 may comprise at least one
rotationally symmetric surface and the lenses comprising the first lens group 131 are comprised of either glass or plastic or a combination of glass and plastic. The first lens group 131 may comprise at least one surface ofthe spherical, aspherical, diffractive, or
Fresnel type, or a combination of these surface types. Also, the first lens group 131 may
comprise at least one lens which is tilted and decentered with respect to a central longitudinal optical axis ofthe lenses which comprise the imaging element 120. Preferably, the first lens group 131 consists of lenses which are all tilted and decentered with respect to the central longitudinal optical axis ofthe lenses which comprise the
imaging element 120.
The second lens group 132 preferably comprises two off-axis rotationally symmetric surfaces and two conic cylindrical surfaces although it may be envisioned that
more or less lenses may be utilized within the scope ofthe invention. The second lens group 132 produces positive power in the first direction and positive power in the second direction which is peφendicular to the first direction. The second lens group 132 may
include at least one lens which is comprised of a low color dispersion material, and at least one additional lens which is comprised of a high color dispersion material such that
chromatic aberration ofthe image is corrected. Examples of low color dispersion materials are acrylic and Zeonex®. An example of a high color dispersion material is polystyrene. Other low and high color dispersion materials may of course be used in the practice of this invention. In a preferred embodiment, the second lens group 132
includes one lens which is comprised of a low color dispersion material, and another lens which is comprised of a high color dispersion material. The individual lenses which comprises the second lens group 132 are illustrated in detail in FIGs. 6-10. The second
lens group 132 may comprise at least one rotationally symmetric surface and the lenses
comprising the second lens group 132 are comprised of either glass or plastic or a combination of glass and plastic. The second lens group 132 may comprise at least one
surface ofthe spherical, aspherical, diffractive, or Fresnel type, or a combination of these surface types. Also, the second lens group 132 may comprise at least one lens which is tilted and decentered with respect to a central longitudinal optical axis ofthe lenses which comprise the imaging element 120. Preferably, the second lens group 132 consists
of lenses which are all tilted and decentered with respect to the central longitudinal optical axis ofthe lenses which comprise the imaging element 120.
The third lens group 133 preferably comprises one off-axis rotationally symmetric surfaces and five conic cylindrical surfaces although it may be envisioned that more or less lenses may be utilized within the scope ofthe invention. The third lens group 133
produces positive power in the first direction and negative power in the second direction which is peφendicular to the first direction. The reduction in the magnification in the
first direction was accomplished by the negative power in the first lens group 131 and the
positive power in the second lens group 132. The enlargement in the magnification in the second direction was accomplished by the positive power in the second lens group
132 and the negative power in the third lens group 133. hi a preferred embodiment, the
first lens group 131 produces low positive power in the second direction, and the third lens group 133 produces low positive power in the first direction. The third lens group
133 may include at least one lens which is comprised of a low color dispersion material, and at least one additional lens which is comprised of a high color dispersion material
such that chromatic aberration ofthe image is corrected. Examples of low color
dispersion materials are acrylic and Zeonex®. An example of a high color dispersion material is polystyrene. Other low and high color dispersion materials may of course be used in the practice of this invention. In a preferred embodiment, the third lens group
133 includes one lens which is comprised of a low color dispersion material, and another
lens which is comprised of a high color dispersion material. The individual lenses which comprises the third lens group 133 are illustrated in detail in FIGs. 6-10. The third lens group 133 may comprise at least one rotationally symmetric surface and the lenses comprising the third lens group 133 are comprised of either glass or plastic or a combination of glass and plastic. The third lens group 133 may comprise at least one surface ofthe spherical, aspherical, diffractive, or Fresnel type, or a combination of these
surface types. Also, the third lens group 133 may comprise at least one lens which is
tilted and decentered with respect to a central longitudinal optical axis ofthe lenses which comprise the imaging element 120. Preferably, the third lens group 133 consists
of lenses which are all tilted and decentered with respect to the central longitudinal optical axis ofthe lenses which comprise the imaging element 120.
The various lenses within each lens group and the imaging element 120 may
each be tilted or de-centered with respect to the central longitudinal optical axis 101 (FIG. 4) ofthe optical system 100 dependent on the amount or type of correction desired. These adjustments to the individual component groups (i.e. tilting and de-centering) may be determined through routine experimentation and may therefore become apparent to
the skilled artisan in light ofthe present disclosure. Each ofthe lenses may be arranged
or adjusted independently from the other remaining elements ofthe optical system 100. For example, the arrangement or adjustment may require the second lens group 132 to have a positive tilt with respect to the central longitudinal optical axis 101 ofthe optical
system 100, while the first lens group 131 and third lens group 133 each have a negative tilt with respect to the central longitudinal optical axis 101 ofthe optical system 100. Other configurations will, or course, fall within the scope ofthe present invention in light of this description. Alternatively, the exact number of lenses within each lens group of the anamoφhic telescope 130 may be dependent on the overall configuration ofthe
optical system (including the above-mentioned tilting and chromatic aberration
correction), the value for incident angle θ, the magnification desired, and the image
quality desired.
By utilizing a significant amount of tilt and/or decentration within the first lens group 131, substantial correction of keystone distortion occurs. Some or all ofthe lenses
within the imaging element 120, second lens group 132, and the third lens group 133 may
also contribute to keystone correction although preferably to a lesser degree than that provided by lenses within the first lens group 131.
The final mirror 140 in the optical system 100 is used mainly to reflect the image toward the display image plane and is positioned subsequent the third lens group 133 within the optical path ofthe image. The final mirror 140 preferably comprises a biconic surface which is independently anamoφhic and conic in a first direction and in a second
direction which is peφendicular to the first direction. In a preferred embodiment, the final mirror 140 has positive power and is preferably configured to reflect light rays
which are non-parallel with respect to each other between the final mirror and the display image plane. Since keystone distortion correction occurs in the lenses as described
above (and mainly occurs in the first lens group 131 which preferably has the greatest tilt), keystone distortion is corrected without resorting to parallel rays. The other lenses
throughout the optical system 100 assist in the correction of keystone distortion to effect a gradual and therefore, more gentle correction than if it were performed by a single element. It may be alternatively desired to configure the final mirror 140 such that light rays between the final mirror and the display image plane are parallel with respect to each
other. Thus, in this particular configuration, principal light rays reflecting off the final mirror 140 of this type (i.e. having parallel rays being reflected therefrom) do not further separate (i.e. not conical in shape) and thus, this configuration results in the image source
appearing to come from an infinite distance. In either configuration, the final mirror 140
may optionally be configured to assist in the reduction or elimination of keystone distortion. Also, if desired, the final mirror 140 may optionally be used to introduce a tilt on the image ofthe object (as mentioned above) and may also optionally be used to focus
the image. Further, the final mirror 140 may alternatively comprise a spherical, aspherical, Fresnel, planar, or diffractive surface, or combinations thereof. The center of curvature ofthe imaging element 120, the anampφhic telescope 130, and the final mirror 140 are each preferably aligned within a common plane. Also, one or two elements
selected from the imaging element 120, the anamoφhic telescope 130, and the final mirror 140 effect a tilt on the image. More preferably, it is desired to have the imaging element 120, the anamoφhic telescope 130, and the final mirror 140 each effect a tilt on the image. Optionally, tlie final mirror 140 may be replaced by a transmissive element or
by a combined transmissive/reflective element. It may alternatively be possible to omit
the final mirror 140.
As an alternative to providing the keystone correction with the lenses within the
imaging element 120 or within the three groups comprising the anamoφhic telescope 130, the reduction or elimination ofthe keystone-type distortion may be performed
electronically. For example, image source 110 may be a DMD configured to produce an image having an "inverse keystone-type distortion" which compensates for the keystone-
type distortion caused by the optics ofthe projection path. Of course, this distortion correction technique can be used to compensate for any other distortion correction or
focusing elements provided in the optical system. Although this technique has been described with reference to a DMD modulator, other modulators such as a raster scanner
or an LCD may be used.
FIG. 5 is a side view schematic of an ultrathin optical panel 10 using a preferred optical system 100 ofthe type shown in FIG. 4. FIG. 6 is a detailed side view illustrating
particular lens elements in the preferred optical system ofthe type generally depicted in
FIG. 5 in conjunction with an optical panel. Commonly available optical design software such as, for example, ZEMAX, version 9.0 (Focus Software, ie.) may be used to assist
in describing the various characteristics (e.g. radius, thickness, glass type, diameter, and
whether the surface is conic) corresponding to each surface region of each individual element/group within the optical system 100. In the exemplary configuration shown in FIGs. 6-7, the ZEMAX software outputs surface data describing these surface
characteristics as illustrated in Table 1. The surface data for surfaces #OBJ-#3
(illustrated in the left-hand column of Table 1) correspond to the image source 110. The surface data for surfaces #6-#15, #24-#27, #30-#33, and #36-#41 correspond to the imaging element 120, the first lens group 131, the second lens group 132, and the third
lens group 133, respectively. The surface data for surface #44 correspond to the final
mirror 140. The surface data for surfaces #48-#IMA correspond to a model ofthe panel 10. The specific nomenclature representing the shapes, compositions, and definitions of the elements as presented in Table 1 follow standards as set forth in the ZEMAX manual.
Of course, other surface data values for each individual element/group will become apparent to those of ordinary skill in the art in light ofthe present disclosure and
may therefore be determined through routine experimentation dependent on the overall configuration and positioning ofthe individual elements/groups within the optical system
100 (including the above-mentioned tilting), the value for incident angle θ, and the
quality ofthe image desired.
Table 1
ZEMAX Software Output Describing Surface Data Summary and Detail for Each
Individual Element within the Optical System 100
SURFACE DATA SUMMARY :
Surf Type Radius Thickness Glass Diameter
Conic
OBJ STANDARD Infinity 10000 19.94653
0
STO STANDARD Infinity -10000 3554.857
0
2 STANDARD Infinity 90 SFL57 19.94653
0
3 STANDARD Infinity 0 37.08317
0
4 COORDBRK - 13
5 COORDBRK - 0
6 STANDARD 193.9193 3 POLYSTYR 62.24857
0
7 EVENASPH 77.12215 1.5 64.52058
0
8 STANDARD 218.4338 19 ZEON 80R 64.74043
9 EVENASPH 52.84822 0.5 66.36415
10 EVENASPH 49.08G24 18.5 ZEON480R 62.70585
11 EVENASPH 67.60375 2.481307 61.4723
12 EVENASPH 74.80689 4 POLYSTYR 46.89625
13 STANDARD 40.09159 1.066642 41.29904
14 EVENASPH 60.42716 5 ZEON 80R 41.10136
15 STANDARD 47.51392 4.344381 37.44564
16 STANDARD Infinity -59.39233 36.96545
17 COORDBRK - 69.39233
18 COORDBRK' - 45
19 COORDBRK - 2
20 COORDBRK - 0
21 TOROIDAL Infinity 0
22 COORDBRK - -2
23 COORDBRK _ 0
24 BICONICX Infinity 4.5 ACRYLIC 105.1232 0
25 EVENASPH 350.0003 7.5 99.38359 0
26 BICONICX Infinity 4.5 POLYSTYR 94.47566 0
27 EVENASPH 83.47696 -16.5 82.78123 0
28 COORDBRK 100
29 COORDBRK 0
30 BICONICX Infinity 17 POLYSTYR 152.1916 0
31 EVENASPH -498.0031 7.5 154.9292 0
32 BICONICX 328.9291 32 ACRYLIC 161.8571 0
33 EVENASPH -211.3969 -56.5 162.2234 0
34 COORDBRK 175
35 COORDBRK 0
36 BICONICX Infinity 11.875 ACRYLIC 534.5 0
37 BICONICX Infinity 20 532.8953 0
38 BICONICX Infinity 11.875 ACRYLIC 528.8599 0
39 BICONICX Infinity 10 527.2552 0
40 BICONICX Infinity -5 POLYSTYR 525.2375 0
41 EVENASPH 400 -48.75 520.4943 0
42 COORDBRK 708.75
43 COORDBRK 0
44 BICONICX -6038.072 0 MIRROR 716.4895 153.1398
45 COORDBRK -340
46 COORDBRK 0
47 COORDBRK 0
48 STANDARD Infinity -12.7 ACRYLIC 918.3966 0
IMA STANDARD Infinity BK7 933.8467
SURFACE DATA DETAIL:
Surface OBJ STANDARD Scattering None
Surface STO STANDARD' Scattering None
Surface 2 STANDARD
Scattering None
Surface 3 STANDARD Scattering None
Surface 4 COORDBRK Decenter X 0 Decenter Y 10.229896 Tilt About X -17.916146 Tilt About Y 0 Tilt About Z 0 Order Decenter then tilt Scattering None
Surface 5 COORDBRK Decenter X 0 Decenter Y 0 Tilt About X 21.963548 Tilt About Y 0 Tilt About Z 0 Order Decenter then tilt Scattering None
Surface 6 STANDARD Scattering None
Surface 7 EVENASPH Coeff on r 2 0 Coeff on r 4 -7.6365947e-006 Coeff on r 6 8.2389495e-009 Coeff on r 8 -6.4927098e-012 Coeff on r 10 3.8564522e-015 Coeff on r 12 -1.4897253e-018 Coeff on r 14 1.9404697e-022 Coeff on r 16 0 Scattering None
Surface 8 STANDARD Scattering None
Surface 9 EVENASPH Coeff on r 2 0 Coeff on r 4 1.1540499e-006 Coeff on r 6 -6.5212774e-010 Coeff on r 8 4.1919239e-013 Coeff on r 10 5.8009771e-017 Coeff on r 12 -2.3798683e-019 Coeff on r 14 1.8552364e-022 Coeff on r 16 0 Scattering None
Surface 10 EVENASPH Coeff on r 2 0 Coeff on r 4 -6.6616345e-006 Coeff on r 6 -2.9177847e-009 Coeff on r 8 4.0710706e-012 Coeff on r 10 -1.3118453e-015 Coeff on r 12 0 Coeff on r 14 0 Coeff on r 16 0 Scattering None
Surface 11 EVENASPH Coeff on r 2 Coeff on r 4 Coeff on r 6 Coeff on r 8 Coeff on r 10 Coeff on r 12
Coeff on r 14 0
Coeff on r 16 0
Scattering None
Surface 12 EVENASPH
Coeff on r 2 0
Coeff on r 4 -2.3046574e- 006
Coeff on r 6 4.9958897e- 009
Coeff on r 8 7.7451265e- 013
Coeff on r 10 -1.9299055e- 015
Coeff on r 12 0
Coeff on r 14 0
Coeff on r 16 0
Scattering None
Surface 13 STANDARD
Scattering None
Surface 14 EVENASPH
Coeff on r 2 0
Coeff on r 4 8.7986807e- 006
Coeff on r 6 -2.2204077e- 009
Coeff on r 8 -3.1936648e- 012
Coeff on r 10 0
Coeff on r 12 0
Coeff on r 14 0
Coeff on r 16 0
Scattering None
Surface 15 STANDARD
Scattering None -
Surface 16 STANDARD
Scattering None
Surface 17 COORDBRK
Decenter X 0
Decenter Y 0
Tilt About X -21.963548
Tilt About Y 0
Tilt About z 0
Order Tilt then decenter
Scattering None
Surface 18 COORDBRK
Decenter X 0
Decenter Y 0
Tilt About X 0
Tilt About Y 0
Tilt About z 0
Order Decenter then tilt
Scattering None
Surface 19 COORDBRK
Decenter X 0
Decenter Y 0
Tilt About X 0
Tilt About Y 0
Tilt About z 0
Order Decenter then tilt
Scattering None
Surface 20 COORDBRK
Decenter X 0
Decenter Y 0
Tilt About X 55
Tilt About Y 0
Tilt About z 0
Order Decenter then tilt
Scattering None
Surface 21 TOROIDAL
Rad of rev. 0
Coeff on yΛ2 0
Coeff on yΛ4 0
Coeff on yΛ6 0
Coeff on yΛ8 0
Coeff on yΛ10 0
Coeff on yΛ 12 0
Coeff on y"" 14 0
Scattering None
Surface 22 COORDBRK
Decenter X 0
Decenter Y 0
Tilt About X -55
Tilt About Y 0
Tilt About Z 0
Order • Decenter then tilt
Scattering None
Surface 23 COORDBRK
Decenter X 0
Decenter Y -66.296228
Tilt About X -30
Tilt About Y 0
Tilt About z 0
Order Decenter then tilt
Scattering None
Surface 24 BICONICX
X Radius -387.32209
X Conic -267.03867
Aperture Rectangular Aperture
X Half Width 15
Y Half Width 20
Y- Decenter 37.5
Scattering None
Surface 25 EVENASPH
Coeff on r 2 0
Coeff on r 4 -2.8438997e-007
Coeff on r 6 1.4417908e-010
Coeff on r 8 -4.3731403e-014
Coeff on r 10 5.1611474e-018
Coeff on r 12 0
Coeff on r 14 0
Coeff on r 16 0
Aperture Rectangular Aperture
X Half Width 15
Y Half Width 20
Y- Decenter 37.5
Scattering None
Surface 26 BICONICX
X Radius 127.25182
X Conic -0.73067967
Aperture Rectangular Aperture
X Half Width 15
Y Half Width 20
Y- Decenter 30
Scattering None
Surface 27 EVENASPH
Coeff on r 2 0
Coeff on r 4 1.7830073e-006
Coeff on r 6 -6.8248748e-010 Coeff on r 8 3.5235297e-013 Coeff on r 10 -6.940471e-017 Coeff on r 12 0 Coeff on r 14 0 Coeff on r 16 0 Aperture Rectangular Aperture X Half Width 15
Y Half Width 20 Y- Decenter 30 Scattering None
Surface 28 COORDBRK Decenter X 0 Decenter Y 66.296228 Tilt About X 30 Tilt About Y 0 Tilt About Z 0 Order Tilt then decenter Scattering None
Surface 29 COORDBRK Decenter X 0 Decenter Y -40.738965 Tilt About X -17.109512 Tilt About Y 0 Tilt About Z 0 Order Decenter then tilt Scattering None
Surface 30 BICONICX X Radius 183.73015 X Conic -0.43100708 Aperture Rectangular Aperture X Half Width 140
Y Half Width 50 Y- Decenter 35 Scattering None
Surface 31 EVENASPH Coeff on r 2 0 Coeff on r 4 -2.3071702e-008 Coeff on r 6 1.8940836e-012 Coeff on r 8 -1.5192564e-016 Coeff on r 10 0 Coeff on r 12 0 Coeff on r 14 0 Coeff on r 16 0 Aperture Rectangular Aperture X Half Width 40
Y Half Width 50 Y- Decenter 35 Scattering None
Surface 32 BICONICX X Radius 0 X Conic 0 Aperture Rectangular Aperture X Half Width 40
Y Half Width 50 Y- Decenter 35 Scattering None
Surface 33 EVENASPH Coeff on r 2 0 Coeff on r 4 2.6979e-009
Coeff on r • 6 -2.7244033e-014 Coeff on r 8 8.9679739e-017 Coeff on r 10 0 Coeff on r 12 0 Coeff on r 14 0 Coeff on r 16 0 Aperture Rectangular Aperture X Half Width 40
Y Half Width 50 Y- Decenter 35 Scattering None
Surface 34 COORDBRK Decenter X 0 Decenter Y 40.738965 Tilt About X 17.109512 Tilt About Y 0 Tilt About Z 0 Order Tilt then decenter Scattering None
Surface 35 COORDBRK Decenter X 0 Decenter Y 240.74828 Tilt About X 1.8789527 Tilt About Y 0 Tilt About Z 0 Order Decenter then tilt Scattering None
Surface 36 BICONICX X Radius -52.407587 X Conic -1.0669935 Aperture Rectangular Aperture X Half Width 40
Y Half Width 60 Y- Decenter -215 Scattering None
Surface 37 BICONICX X Radius 360.14619 X Conic 0 Aperture Rectangular Aperture X Half Width 60
Y Half Width 60 Y- Decenter -215 Scattering None
Surface 38 BICONICX X Radius -52.407587 X Conic -1.0669935 Aperture Rectangular Aperture X Half Width 40
Y Half Width 60 Y- Decenter -215 Scattering None
Surface 39 BICONICX X Radius 360.14619 X Conic 0 Aperture Rectangular Aperture X Half Width 60
Y Half Width 60 Y- Decenter -215 Scattering None
Surface 40 BICONICX
X Radius 111.4054 X Conic -8.322084 Aperture Rectangular Aperture X Half Width 70
Y Half Width 60 Y- Decenter -215 Scattering None
Surface 41 EVENASPH Coeff on r 2 0 Coeff on r 4 -2.1490064e-008 Coeff on r 6 2.3665096e-013 Coeff on r 8 -1.7247128e-018 Coeff on r 10 5.2496812e-024 Coeff on r 12 0 Coeff on r 14 0 Coeff on r 16 0 Aperture Rectangular Aperture X Half Width 80
Y Half Width 60 Y- Decenter -215 Scattering None
Surface 42 COORDBRK Decenter X 0 Decenter Y -240.74828 Tilt About X -1.8789527 Tilt About Y 0 Tilt About Z 0 Order Tilt then decenter Scattering None
Surface 43 COORDBRK Decenter X 0 Decenter Y 132.5782 Tilt About X 6.5 Tilt About Y 0 Tilt About Z 0 Order Tilt then decenter Scattering None
Surface 44 BICONICX X Radius -1988.3354 X Conic -5.5500196 Aperture Rectangular Aperture X Half Width 360
Y Half Width 80 Y- Decenter -120 Scattering None
Surface 45 COORDBRK Decenter X 0 Decenter Y -132.5782 Tilt About X 6.5 Tilt About Y 0 Tilt About Z 0 Order Decenter then tilt Scattering None
Surface 46 COORDBRK Decenter X 0 Decenter Y 12.127182 Tilt About X 78 Tilt About Y 0 Tilt About Z 0 Order Decenter then tilt
Scattering None
Surface 47 COORDBRK
Decenter X 0
Decenter Y 0
Tilt About X 0
Tilt About Y 0
Tilt About Z 0
Order Decenter then tilt
Scattering None
Surface 48 STANDARD
Aperture . Rectangular Aperture
X Half Width 360
Y Half Width 300
Scattering None
Surface IMA STANDARD
Aperture Rectangular Aperture
X Half Width 360
Y Half Width 300
Scattering None
The optical system 100 and panel 10 as described above produces a distortion free
image which corrects chromatic aberration ofthe image. This optical system 100 also produces a properly focused image on the surface ofthe outlet face 24 ofthe optical panel 10 as illustrated by the spot diagram of FIG. 11. FIG. 11 illustrates the image
focusing performance ofthe optical system 100 using geometric image spots projected at
various locations ofthe optical panel 10. The optical system 100 also retains the aspect ratio ofthe original image source while mamtaining a linear point-to-point mapping of the image having distortion of less than 2% as illustrated by the grid distortion plot diagram of FIG. 12. FIG. 12 is a grid distortion plot diagram wherein intersections ofthe
grid show the ideal image locations and the "x's" show the actual image locations. The grid is for a 12.48 mm x 15.56 mm image source. The grid distortion plot diagram depicts the outlet face 24 surface #TMA when an image with a grid or lattice pattern is
placed at the image source 110 surface #OBJ. The lenses used in optical system 100 of the present invention are preferably non-planar and plastic and therefore result in easier
manufacturability during the molding process. Moreover, significantly higher resolutions may be obtained using the optical system 100 ofthe present invention due to the reduction in the various distortions and chromatic aberrations mentioned above. The
multiple lenses required by the color correction scheme described above assist in adding a significant amount of minor tilts throughout the system that gradually correct the
keystone distortion in a more gentle fashion than if the correction were performed using a single element.
In another preferred embodiment, it may be desired to effect a fold or multiple
folds in the optical path ofthe optical system 100 within the anamoφhic telescope 130 to thereby reduce the overall height, width, and depth D ofthe housing 14 containing the optical panel 10 and optical system 100. FIG. 8 is a detailed rear view illustrating lens
elements and a folding mirror in an alternate optical system in conjunction with an
optical panel. The folding mirror 138 in this configuration is positioned between the first
lens group 131 and the second lens group 132. In yet another preferred embodiment, FIG. 9 is a detailed rear view illustrating lens elements and a folding mirror in an alternate optical system in conjunction with an optical panel. The folding mirror 139 in
this configuration is positioned between the second lens group 132 and the third lens
group 133. In still yet another preferred embodiment, FIG. 10 is a detailed rear view illustrating lens elements and two folding mirrors in an alternate optical system in
conjunction with an optical panel. The folding mirror 138 in this configuration is positioned between the first lens group 131 and the second lens group 132, while the
folding mirror 139 is positioned between the second lens group 132 and the third lens group 133. By providing folding ofthe optical path within the first and second
anamoφhic telescopic systems, image distortion (e.g. chromatic aberration) is reduced,
while reducing the required housing 14 size. Optionally, in another alternate optical system configuration, a folding mirror may be provided between the imaging element 120 and the first lens group 131. This particular folding mirror may be the only folding mirror within the optical system 100 or may be used in any combination with folding
mirror 138 and/or folding mirror 139.
Those of ordinary skill in the art will recognize that many modifications and variations ofthe present invention may be implemented. For example, instead of comprising lenses, the imaging element 120 and lens groups which comprise the
anamoφhic telescope 130 each may alternatively comprise additional mirror(s) or
lens/mirror combination(s). It may be desirable to substitute a lens within the imaging element 120 and or at least one lens within the anamoφhic telescope 130 with a mirror or to provide additional mirror elements to effect additional folds in the optical path of the optical system 100 to thereby reduce the overall depth D ofthe housing 14 (FIGs. 1-
3) containing the optical panel 10 and optical system 100. As another example of a
variation ofthe present invention, the anamoφhic telescope may alternatively be comprised of more than three lens groups. As yet another example of a variation ofthe present invention, the waveguides 10a within the optical panel 10 may extend vertically,
and the plurality of stacked waveguides 10a may then extend horizontally. In this optical panel 10 alternative configuration, the image source 110 would project light in a
correspondingly dimensioned manner and in a horizontal orientation. Thus, it may be envisioned that the optical system 100 ofthe present invention can be configured to
accommodate varying optical panel dimensions,sizes and /or orientations. In still another
example of a variation ofthe present invention, a system such as shown in Figures 6 and 7 could be used in a front projection format, for example, by replacing the panel 10 with a screen suitable for front projection. In a further example of a variation ofthe present invention, different elements such as those having air spaces and/or diffractive optics may alternatively be employed instead of, or in conjunction with, elements having low and high color dispersion in order to achieve chromatic correction. The foregoing description and the following claims are intended to cover all such modifications and variations.