NOTES ON LEEP ARV-1 STEREOSCOPIC VIEWER OPTICS
FOCAL LENGTH: 41 mm ENTRANCE PUPIL DIAMETER: 60 mm
INTERAXIAL SPACING: 64 millimeters. For viewing comfort when shifting
from near to distant subjects, it is recommended that the infinity point
conjugate spacing of the images in the viewing plane be 62 mm. It is important
to note that this image spacing is not determined by the interpupillary distance
of any particular person using the viewer, but rather by the requirement that
nobody be required to cause their left and right visual axes to diverge, which
causes severe eyestrain, and which everybody would have to do to merge an
infinite image pair if the spacing exceeded 64 mm. In practice, a slight
convergence for infinitely distant subjects is preferable, which accounts (along
with a margin for system error) for the 2 mm closer spacing recommended for the
stereo pair of images.
FIELD OF VIEW: This is a wiggly parameter. The following remarks
pre-suppose that a properly scaled image in the LEEP compressed format is
present at the focal plane of the viewer. A 140 degree field is possible if the
eyes can move laterally with respect to the viewer - "peer about" through the
hole represented by the eye lens perimeter. In a head-mounted display, however,
the eyeballs normally are constrained to rotating in azimuth and elevation about
their centers. Accordingly the field is limited by the eye lens perimeter (which
is also the entrance pupil and the field stop) and by the proximity of the eye
to the apex of the eye lens. Most eyes can swivel only about 90 degrees, and it
is easy for most people to get close enough to see this much, though eyeglasses
may impose an added limit. The significant number is thus the eye lens entrance
pupil radius of 30 mm. If the center of rotation of the eyeball is 30 mm away
from the center of the entrance pupil , the directly viewed field is then (from
the geometry) 90 degrees. (Actually , refraction at the cornea gives a sensibly
wider field when looking straight ahead - we call this the "knothole" effect .)
The geometry gives us several more numbers: if 1/2" of lateral head motion is
allowed each way, the field is 110 degrees; if the eyeball center of rotation is
brought to (a possible) 20 mm, the field is 112 degrees; if both motions are
allowed, the field is 130 degrees.
LATERAL CHROMATISM: Called also, and more descriptively, "chromatic
difference of magnification" this aberration is normally observed as blue and
red "fringes" at the extremes of the field of an optical system. In the interest
of achieving high magnification and a wide field in the same design, no attempt
was made to achromatize individual elements in the LEEP optics. In fact the
basic LEEP invention consists mainly in compensating the viewer chromatism by an
opposite chromatism in the image viewed. Adequate electronic compensation can be
accomplished by making the red image about 1% larger (linearly) than the blue
image, with the green in between. LEEP video camera lenses provide a color
compensated image when used with a color video camera. The photographic LEEP
slides available in the VR demo set were taken with equivalent LEEP camera
lenses.
EXPANSION OF FIELD: In order to make the best possible use of
photographic resolution (or video channel bandwidth) most of the image area is
devoted to the central field, and the peripheral field is compressed into the
edges. The result is an extreme "fisheye-like" image, in which the radial
distance from the image center is approximately proportional to the sine of the
real, or computer-generated, object-space angle. This distortion is accurately
approximated by:
r = f (A - .18A^3)
Where: r is the radial distance from the optical axis to any point on
the (nominal) focal plane of the viewer, f is the axial focal length of
the viewer, and A is the apparent off-axis angle in radians of the image
of the same point as seen by a person using the viewer, which is also its angle
in object space.
To expand this image, i.e. to restore the orthoscopy of the space
(orthospace) the viewer optics must have a large compensating positive radial
distortion, so that A is the angle of the collimated beam the optics
produce from light emanating from the point in question.
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