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Product Overview:
M92D Elbow Telescope
NSN: 1240-00-564-6339
P/N: 8299680

Description
Elbow telescope M92D is a fixed-focus fixed-reticle-type elbow telescope having 3-power magnification and a
field of view of 12 degrees 12 minutes. When the elbow telescope M92D is installed in the telescope mount M90
(T183) which, in turn, is mounted on the rear bracket of the 106-M recoilless rifle
M40 (T170E1), it is the direct sight for this weapon.
Functional Description
a. Mechanical Components
The objective end of the body of the elbow is tapered and slotted to fit the bore and key of telescope
mount M90 (T183), and the extreme end is threaded so that the elbow telescope can be locked in place
in the telescope mount by means of a round nut which is an integral part of the telescope mount. A level
vial at the elbow of the body is used in conjunction with the cant correction mechanism of the telescope
mount M90 (T183) to determine when the elbow telescope M92D is level. The band assembly serves as a means
for attachment of the lamp bracket of the instrument light M42, to illuminate the reticle through a window
in the body. The eyeshield enables the observer to sight on the target without interference from light or
wind and to position his eye at the proper distance from the eyepiece.
b. Optical System
(1) General. The image of the target enters the elbow telescope M92D and the objective lens in its correct
upright condition. The objective lens focuses or converges the light rays to a point, and when this lens is
properly positioned, it will cause this focal point to fall exactly on the etched side of the reticle.
Because the image would then appear inverted and reversed due to the crossing of the light rays at the
focal point, the amici prism is positioned between the reticle and objective lens. In this position it
serves two purposes: (a) It changes the direction of the light rays 90 degrees so they will leave through
the telescope eyepiece. (b) It inverts and reverses the image before it appears on the reticle, so that
when it is reversed and inverted a second time at the focal point it will then appear in its correct upright
position. The image appearing on the reticle, however, would now be to small to serve any practical purpose.
The eye and field lens correct this difficulty by magnifying the image and brightening it to make all details
stand out sharply throughout the entire field.
(2) Objective. The objective is simply a converging lens whose
function it is to focus the light rays on the reticle forming an image
of the field of view on that lens.
(3) Amici Prism. The amici prism bends the light rays 90 degrees so
they are projected towards the reticle. This prism also inverts and
reverses the image so that the image will appear in its normal upright
position when seen by the observer.
(4) Reticle. The reticle provides reference lines etched or
engraved into the glass for keeping the target centered in the field
of view and for making angular measurements. The reticle pattern
includes curved stadia lines for estimating target range on targets of
known dimensions (10 or 20 feet), and a series of broken horizontal
and vertical lines. At the top of the pattern is a cross hair
representing zero deflection and zero range and is used as the bore
sight cross. Each vertical line and each space represent 100 yards of
range. Each horizontal line and each space represent an angular lead
of 5 mils. The center point of the small circles within the reticle
pattern represents the ends of lead lines that have been eliminated to
insure a clearer field of view through the reticle. At the bottom of
the reticle is a horizontal and vertical mil scale to permit emergency
use of the direct sighting instruments for indirect fire. The
horizontal scale is marked in 1-mil increments from 0 to 30 mils right
and left of the vertical centerline. Note that the first mark right and
left of the centerline represents 2 mils. The mark for 1 mil has been
eliminated for greater clarity. At the center of the scale is a
vertical mil scale graduated in 1-mil increments, 5 mils above and 5
mils below the horizontal scale. At approximately the 800-yard range
point, a horizontal dash line indicates the centerline of the reticle.
(5) Field Lens. The field lens is one of the lenses that forms the
eyepiece of the elbow telescope M92D. Its main function is to gather
light from the objective and converge or direct it into the eyelens.
Without the light gathering qualities of the field lens, the image as
viewed through the eyelens would not be clearly and uniformly
illuminated, but would be dark and shadowed along the edges.
(6) Eyelens. The eyelens is that lens of the elbow telescope M92D
eyepiece which is closest to the observer's eye. This lens acts as a
magnifying lens and enlarges the image and the reticle pattern so that
it can be more readily seen.
Tabulated Data
| a. Optical Characteristics |
Magnification 3x Field of view 12 degrees 12 minutes |
| b. General |
Height (elbow to eyeshield): 3 3/4 in Length (objective end
to level vial) 4 1/16 in Width (body) 1 3/8 in (eyeshield) 1 3/4 in Weight: 1 lb |
| c. Illumination |
Source Instrument light M42 |
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