U.S. patent number 3,782,822 [Application Number 05/196,698] was granted by the patent office on 1974-01-01 for method and apparatus for automatic ranging with variable power telescopic gun sight.
Invention is credited to Mack L. Spence.
United States Patent |
3,782,822 |
Spence |
January 1, 1974 |
METHOD AND APPARATUS FOR AUTOMATIC RANGING WITH VARIABLE POWER
TELESCOPIC GUN SIGHT
Abstract
In a variable power telescope gun sight, provided with stadia
and aim point at the rear focus between the ocular lens and zoom
system, an aim point is located above the optic center and
correlated with bullet trajectory. The distance of off set of the
aim point is such that, at minimum power, the aim point is zeroed
relative to the stadia for impact at minimum range, this usually
being the point blank range of the projectile, and at some higher
power relative to an increase in range the projectile is again
zeroed, in that the projectile impact and the aim point coincide.
The novel telescopic sight and method of its use are based on the
observations that (1) between approximately 1/3 and 2/3 maximum
range and maximum range the trajectory of a high velocity bullet is
substantially linear, (2) that as magnification is increased the
aim point will appear to move downwardly toward optic center and
(3) that the low power and some higher power of the telescope,
respectively, can be correlated with a zero at the minimum and
maximum range, respectively, with reference to the stadia.
Correlated in such manner, changes in magnification, in the optic
sense automatically set the aim point for firing without any
necessity of the observer knowing the actual distance to the
target.
Inventors: |
Spence; Mack L. (Denham
Springs, LA) |
Family
ID: |
22726484 |
Appl.
No.: |
05/196,698 |
Filed: |
November 8, 1971 |
Current U.S.
Class: |
356/21; 42/122;
359/428; 42/126; 359/422 |
Current CPC
Class: |
G02B
23/145 (20130101) |
Current International
Class: |
G02B
23/14 (20060101); G01c 003/20 () |
Field of
Search: |
;356/20,21 ;350/10
;33/246 |
References Cited
[Referenced By]
U.S. Patent Documents
Primary Examiner: Schonberg; David
Assistant Examiner: Godwin; Paul K.
Attorney, Agent or Firm: Proctor; Llewellyn A.
Claims
Having described the invention, what is claimed is:
1. In a variable power telescopic gun sight for mounting on a gun
wherein is included the combination of a barrel with enclosed
objective lens, ocular lens, zoom system comprised of erectors and
magnifiers, which provide a front focus and rear focus, and means
mounted on the barrel for changing the magnifying power of the
telescope, the improvement comprising locating a reticle, with
stadia and a fixed aim point physically located above the optic
center of the telescope, at the rear focus between the ocular lens
and the zoom system whereby power increases will cause the aim
point to appear to move downwardly toward the optic center of the
telescope and thereby automatically compensate for the trajectory
of a bullet fired from the gun.
2. The apparatus of claim 1 wherein the aim point of the reticle is
off-set above the optic center of the telescope by a distance
sufficient to correlate a linear bullet trajectory, at high
magnifying power, where the gun is zeroed, at maximum compensated
range for the gun and, at lower magnifying power, where the gun is
also zeroed, with a range defined by the formula M.sub.L /M.sub.H
of maximum; wherein M.sub.L equals the power of the telescope at
low power and M.sub.H equals the power of the telescope at high
power magnification.
3. The apparatus of claim 2 wherein the telescope contains a
reticle cell having a vertical cross hair and a pair of parallel
horizontal cross hairs, one located above optic center and the
other at optic center, the pair of horizontal cross hairs also
defining stadia as well as an off-set aim point and a conventional
aim point, respectively.
4. The apparatus of claim 1 wherein the stadia are comprised of a
pair of lines which adjoin one to the other at an angle of
45.degree..
5. The apparatus of claim 4 wherein one of the lines is horizontal,
and provided with indicia indicative of the height of a target
within the field of the telescope.
6. In a variable power telescopic gun sight for mounting on a gun
wherein is included the combination of a barrel with objective
lens, ocular lens, zoom system comprised of erectors and
magnifiers, which provide a front focus and rear focus, a reticle
located at the rear focus between the ocular lens and the zoom
system, stadia, and means for changing the power of the telescope,
a method for correlating the trajectory of a bullet fired from the
gun comprising physically locating a fixed aim point within the
rear focus above the optic center at a distance such that, at high
power, the aim point will be zeroed at the maximum range of impact
of the bullet and at low power the aim point will be zeroed at a
range defined by the formula M.sub.L /M.sub.H of maximum range;
wherein M.sub.L equals the power of the telescope at low power and
M.sub.H equals the power of the scope at high power
magnification.
7. The method of claim 6 wherein at minimum power the telescope
ranges from about one-fourth to about one-half of its maximum
power.
Description
Apparatus and method for automatic adjustment of the aim point of a
variable power telescope with changes in magnification, with
consequent changes in the bullet trajectory, without any necessity
of the observer knowing the actual distance to the target. The aim
point appears to move downwardly with increasing magnification,
this allowing power increases as range increases, as is desirable
for precision of aim.
Telescopic gun sights have been long known in the art, and it has
become commonplace for sportsmen to mount such devices on small
fire-arms, particularly rifles. In the standard telescopic gun
sight there are two points of focus at which a reticle, or device
which carries an aim point, e.g., cross hairs, can be located,
viz., at the front focus or rear focus. In variable power
telescopes it has now become most desirable to locate the reticle
at the point of rear focus so that as power is increased, the
apparent size or thickness of the reticle is not magnified, such as
would tend to obscure the target.
Recently introduced telescopes which include a variable power or
zoom element include the above described improvement in reticle
location, and also built-in rangefinders of various types. In most
telescopes now on the market, various indicia defining an aim
point, e.g., the point where the vertical and horizontal lines of
cross hairs intersect, is located within the telescope at the exact
optical center (the point which does not move when power is
changed). In most commercial variable power telescopes, once the
range has been determined by use of the built-in rangefinder, the
observer holds over the target to compensate for the difference
between the range at which the telescope and rifle are zeroed and
that estimated for the range of the target, and then fires.
A telescope with a built-in rangefinder of the above type, now in
wide commercial use, is described in U.S. Pat. No. 3,386,330. In
the telescope described therein, a target of known size is
precisely circumscribed between stadia wires, and by change of
power or magnification, the distance of the target from the
observer can be read from a scale. Knowing the range, the observer
can then select the magnification desired and then hold over the
target to compensate for the difference between the range at which
the telescope and rifle are zeroed and the distance to the target
as determined by the known ballistics of the type of cartridge
used, and then fire. The aim point is the optical center of the
telescope sight which is held over the target by an amount
estimated to compensate for the trajectory of the bullet, or bullet
drop. The time required for adjustments of power, to estimate
range, return to a desired magnification and mentally compute
hold-over obviously have their limitations.
Devices are now described, e.g., in U.S. Pat. Nos. 3,340,614 and
3,492,733 which automatically adjust the trajectory of the bullet
simultaneously with power changes, i.e., the steps of changing the
power for framing a target between a pair of stadia automatically
adjusts the trajectory for firing without any necessity of the
observer knowing the actual distance to the target. Telescopic
sights have thus been pivotally mounted in relation to a gun barrel
so that power adjustments made in framing a target between a pair
of stadia raises or lowers the telescope with relationship to the
barrel to align the optical center of the telescope upon the target
after the adjustments are completed. Hold-over is unnecessary, and
after the target is so framed, and the mechanical adjustment for
trajectory thus made, a pair of stationary cross hairs, one
horizontal and one vertical, which cross at the optical center of
the telescope, is then sighted upon the target, and the gun
fired.
U.S. Pat. No. 3,431,632 also described a telescopic gun sight
wherein power adjustments automatically compensate for bullet
trajectory without there being any necessity of the observer
knowing the actual distance between himself and the target. In the
device described, a scale ring is used to elevate and vertically
space a pair of movable horizontal cross hairs to circumscribe a
target of known size. The aim point defined by the lower horizontal
cross hair and a fixed vertical cross hair is automatically set at
the proper elevation to fix upon the circumscribed target. The
above patents are technically superb, however, they require major
modification to current design of telescopes or mounts and the
non-stationary mounting gives rise to accidental displacement by
rough service or the introduction of foreign particles between cam
and stationary mount stud.
The telescopic gun sight embodied by the present invention obviates
many of these disadvantages and provides further improvements over
these and other known prior art telescopic sighting devices.
Among the objects of this invention are:
To provide a new and improved variable power telescopic gun sight
which contains a rangefinder, or stadia, and means for changing
magnification power while simultaneously automatically adjusting
the reticle or aim point to compensate for the trajectory of the
bullet, whether or not the actual distance to the target is
known.
To provide a variable power telescope of the character described
wherein the reticle or aim point is located in a vertical plane
above the optic center of the telescope, and an exact relationship
is provided between the eccentric reticle or aim point and an
external ring which operates to produce magnification or power
changes such that increases in magnification causes the reticle or
aim point to move downwardly toward the optic center of the
telescope thereby optically compensating for the bullet trajectory
at increased ranges, whether or not the actual distance to the
target is known.
To provide a telescopic gun sight of the character described
wherein the relationship between the external ring which operates
power magnification changes and the reticle can be easily adjusted
to match the type of ammunition used.
To provide a more durable telescopic gun sight of simple structure,
particularly one wherein there are no complicated mechanical
adjustments to be made by changing the alignment between the
telescope and the gun barrel during ranging and firing.
To provide a new and improved reticle with rangefinder of design
particularly useful for fitting to targets of various known sizes
(from small game to that of elk or moose size), adapted for rapid
and efficient use by the observer, capable of both vertical and
horizontal measurement.
These and other objects are achieved in accordance with the present
invention which embodies improvements in telescopic gun sights,
comprising the usual combination of a telescopic tube which
contains objective lens, ocular lens, erectors and magnifiers for
effecting change in magnification (i.e., a zoom system) and a power
change mechanism or adjusting means for changing the magnification
or power. In the improved combination, a reticle with aim point
directly above the optic center, with respect to image, is located
within the rear focus of the lens system, with stadia as used for
estimating distance. The aim point is correlated, empirically or by
calculation, with the trajectory of the gun on which the telescope
is used, as determined by ballistics data, such that as
magnification or power is increased relative to the stadia the aim
point moves vertically downwardly to track the path of the bullet
in flight as it falls due to the influence of gravity.
By locating the reticle within the rear focus between the ocular
lens and the erectors and magnifiers of a variable power telescope,
with an eccentric aim point directly above optic center, it is thus
found that the aim point moves, in an optical sense, vertically
downwardly with respect to the field as power is increased. By
correlation between the paths defined by this optical change and
bullet trajectory, which of course is also downward, with the
combination of stadia, or rangefinder, a target can be ranged with
the desirable quality of allowing power increases as range is
increased. The degree of displacement of the aim point is such that
as magnification is increased on a linear relationship with range,
which can be read from the rangefinder, if desired, but whether or
not the observer has any knowledge of the actual distance to the
target, compensation is automatically made for the range and the
aim point is centered directly on the target.
The invention, and its principle of operation, will be more fully
understood by reference to the following detailed description of a
specific embodiment, and to the attached drawings to which
reference is made in the description. Subscripts are used to show a
plurality of similar parts or components.
In the drawings:
FIG. 1 depicts a side elevation view of a variable power telescopic
gun sight in accordance with this invention mounted on a rifle;
FIG. 2 depicts schematically the optical system of a standard
variable power telescopic gun sight as embodied in this
invention;
FIG. 3 depicts the essentials (the full field not being shown) of a
preferred type of reticle cell or reticle disk which includes both
aim point and stadia as embodied by the present invention;
FIGS. 4 and 5, taken together with the preceding fugure, depict a
series of views illustrating the method of enabling the observer to
circumscribe and range a target using a preferred type of stadia
while automatically setting the aiming indicia for firing, whether
or not the observer is aware of the actual distance to the target;
and
FIG. 6 depicts another preferred type of reticle for automatic
range compensation, this design providing a pair of horizontal
cross hairs which provide stadia, these intersecting with a
vertical cross hair, one cross hair or aim point being at optic
center and the other above optic center. The upper cross hairs
provide an eccentric aim point for automatic ranging and the other
an aim point for conventional aiming.
FIG. 7 depicts a ring scale with indicia markings correlating the
range to target as determined by stadia, which would allow the use
of the reticle on arms having vastly different trajectories. In
this case the ring scale is marked according to decrease from
maximum range.
Referring to FIG. 1 there is shown a variable power telescopic gun
sight or telescope 10 mounted via clamps 8.sub.1, 8.sub.2 on a
rifle 9, the latter per se forming no part of the present
invention. The telescope 10 includes the conventional barrel 11, an
eyepiece 12, an objective 13 and an adjustment ring 14, provided
with a handle 15 to facilitate adjustment and operation of internal
linkage (not shown) which actuates a zoom element within the
telescope so that the target image can be made to look larger or
smaller in proportion to the field.
The optical system, which is depicted schematically by reference to
FIG. 2, also includes the conventional objective lens, ocular lens
and erectors and magnifiers which constitute a zoom system. In
accordance with this invention the reticle, with its eccentric aim
point, and the stadia or rangefinder are located within the rear
focus of the optical system rather than within the front focus.
Reticle 20 with its eccentric aim point 21 above optical center 22,
with stadia or rangefinder, in combination with the conventional
optic system described, constitutes the apparatus features of the
present invention. The method and principles of circumscribing and
ranging a target using a preferred type of stadia or rangefinder
which in the optic sense automatically sets the aim point 21 for
firing, whether or not the observer is actually aware of the
distance to the target, is hereinafter described.
A preferred type of reticle, which can be illustrated by reference
to FIG. 3, comprises a reticle cell, preferably a disk 20
constituted of any suitable transparent material such as plastic or
glass, the disk being generally flat or of plano form. The
transparent reticle disk 20 is scribed with a vertical line 25 and
horizontal line 24, or indicia marks, which intersect to provide an
eccentric aim point 21, or point which lies above the optic center
22 which is also generally the geometric center of the disk. A
diaganol line or indicia mark 23 joins horizontal line 24 at a
45.degree. angle, and the segment of horizontal line 24 lying below
diaganol line 23 is scribed with numerals or other indicia
representative of the vertical distances between lines 23, 24 at
any given point on the horizontal scale. (Horizontal distances can
also be measured between the point of intersection of lines 23, 24
and a point located on the horizontal scale.)
The vertical distances between lines 23, 24 define stadia and, at a
preselected magnification, are a measure of distances between
corresponding points within the field of view. When a target of
known height, at such magnification, is framed between a pair of
verticaly aligned points lying on lines 23, 24 respectively,
therefore, the distance to the target is known, and it has been
conventional to provide means whereby such range could be read from
a scale. In accordance with the present invention, however, it is
unnecessary to actually know the distance to the target. Instead,
the eccentric aim point is automatically moved downwardly, in the
optic sense, in response to power increases, or conversely upwardly
in response to power decreases such that at the moment the target
is framed the aim point is set for sighting and firing.
The technique of sighting and firing is best illustrated by
reference to FIGS. 3 through 5, wherein it is assumed that both the
telescope and rifle have been zeroed at maximum magnification to
frame and strike a target at 400 yards distance, and that the
scribed numerals along horizontal line 24, lying vertically below
points on line 23, are read in inches. The observer sights in on a
circle or bull's eye known by him to be 15 inches in diameter as
shown in FIG. 3. The target does not fit between lines 23, 24 at
the 15-inch scale, but is too small. Magnification is too low,
e.g., 4 power. The observer knows, therefore, that the target is
far away and that if a shot were fired that it would fall too low.
The power is therefore increased, e.g., to 8 power, the full power
of the telescope, until the target fits the 15-inch scale as shown
by reference to FIG. 4. The range is known or can be easily
determined, but this is immaterial, for the aim point 21 is, in the
optic sense moved downwardly in the field, a distance shown by the
difference between the arrows, compensating for bullet trajectory
so that the muzzle of the rifle is raised when the shot is fired as
shown by reference to FIG. 5.
A preferred type of reticle design is also described by reference
to FIG. 6. A parallel pair of horizontal cross hairs 26,27 form
stadia, the lower cross hair 27 being located at optical center.
The point of intersection of vertical cross hair 28 forms an
off-set air point for automatic range compensation, the distance
between the cross hairs 26,27 being used to span an object of known
dimension. The compensation is generally from about 4 to 30 inches
above optical center at 100 yards, and preferably from about 4 to
17 inches above optical center at 100 yards. For most sporting
purposes, compensation of from about 6 to 12 inches above optical
center at 100 yards on lowest available magnification is most
preferred. The point of intersection of cross hairs 27,28 forms an
aim point for conventional firing.
Referring to FIG. 7, there is shown a power selector ring scribed
with an indicia scale representative of a range of values between a
maximum compensated range at full magnification (M.sub.H) and a
minimum range at low magnification (M.sub.L). For example, in
utilizing a scope where maximum magnification is three times the
power at minimum magnification, i.e., in a 3X-9X variable power
telescope, M.sub.H could be conveniently assigned a value of 1.0
and M.sub.L a value of 0.33. The power is linear within this range
and hence the witness mark could be used to clearly indicate the
range of values representative of distances in terms of fractional
units between minimum and maximum range, or fractional power units
between 3X and 9X.
The present invention is based on the recognition that, in the
optic sense, when the magnification of a variable power telescope
with a non-magnifying reticle is changed, all points outside the
optical center of the image will appear to shift inversely with
power change in a one-to-one ratio, e.g., points 6 inches apart at
4 power become 2 inches apart at 12 power. The change in an aim
point located above optic center, in conjunction with stadia which
will also appear to move downwardly with increases in range,
although linear with respect to range, can be correlated with a
given segment of a curve representative of the trajectory of a
bullet, the net change required being dependent on range, velocity,
and the ballistic coefficient of the bullet. Thus, the reticle
movement is selected such that at some low power relative to range
and stadia it is zeroed for trajectory and at some higher power
relative to range increase it is also zeroed by the downward
movement of the aim point. Thus, the low power magnification
M.sub.L is zeroed at M.sub.L /M.sub.H of the maximum range and the
higher power, M.sub.H, is zeroed at the maximum range, and between
these two ranges bullet drop is approximated very closely by the
off-set reticle. The best trajectory fit by the reticle is obtained
with a high power to low power ratio of 1.5 to 3.0. The power
ratio, however, is immaterial as all or only a portion of the full
power can be selected to compensate between the two zero ranges.
After a balance of maximum possible range to allowable error has
been made, the excess power ratio may be used to extend the range
finding capability and decrease hold-over normally required.
The degree of off-set may be found by trial and error or by
calculation, and for most sporting purposes will be 2 to 8 minutes
of angle above the optic center at the higher magnification. This
off-set is fitted to the trajectory by the distance of off-set, or
the trajectory may be fitted to the off-set by allowing the span
value of the stadia and the maximum range to become variables. The
movement of the reticle from minimum zeroed range (X.sub.L) to
maximum zeroed range (X.sub.M) is linear and continuous with range
changes. Therefore, the reticle describes a straight line between
the two points at which zero occurs, the actual trajectory is a
curve and at mid-ranges lies slightly above that line described by
the reticle movement between the two zero points. The error
introduced is greatest at the mid-point of minimum range and
maximum range, e.g., at 300 yards if the X.sub.L is 200 and X.sub.M
is 400 yards, this error being generally no more than 1 to 4 inches
up to distances of 400 or more yards for high velocity arms having
muzzle velocities ranging upward of about 2,700 feet per second
which fire bullets having 0.30 or greater ballistic coefficient
(Ingalls). The error is generally less than the precision of the
rifle.
The following parameters are typical for a 0.30-06 caliber rifle
when zeroed at 200 yards: ##SPC1##
In the above case the M.sub.H /M.sub. L = 2.0, the minimum range =
200 yards, maximum range = 400 yards. If the variable powers
M.sub.L and M.sub.H were 4 and 8, then at 200 yards the shot would
have been made at 4 power, at 400 yards on 8 power, at 300 yards at
300/400 times the M.sub.H (or 3/4 times 8X) on 6 power, etc.
It is apparent that various modifications and changes can be made
without departing the spirit of the present invention. The exact
amount of off-set of the aim point above optic center can thus be
determined empirically or by actual calculation.
Thus, an approximate calculation of these parameters is had by the
following formulas:
1. The desired distance to off-set the reticle, (Q), at highest
desired magnification, in inches at 100 yards, is defined by the
formula:
Q = M.sub.L /M.sub.H [B.sub.4 X.sub.M + B.sub.3)X.sub.M + B.sub.2 ]
X.sub.M.sup.2 (A)/X.sub.M
wherein: A = 1.049 where M.sub.H /M.sub.L = 2 and 0.960 where
M.sub.H /M.sub.L = 3
B.sub.2 = 17.6/V.sup.2
V = muzzle velocity in thousands of feet per second
B.sub.3 = 0.50 K (1 - 0.6/V)B.sub.2
B.sub.4 = 0.1815 K (1 - 1.2/V)B.sub.3
K = 1/CV.sup.3/4
m.sub.h = highest magnification
M.sub.L = lowest magnification
C = ballistic coefficient (Ingalls)
Q = off-set required at highest magnification, inches at one
hundred yards
X.sub.M = maximum desired range for automatic compensation in
hundreds of yards
2. The point bland range, (X.sub.L), the minimum range of automatic
compensation and also the range at which the rangefinder span is
calibrated at minimum magnification, in hundreds of yards, is given
by the formula:
X.sub.L = (M.sub.L /M.sub.H) .times. X.sub.M
3. Reticle movement, (T), in inches, from one range setting to
another is described by the following equation, the limits of the
range being defined as X.sub.L to X.sub.M.
T = X.sub.2 .sup.. X.sub.M .sup.. Q(1/X.sub.2 - 1/X.sub.o)
wherein:
X.sub.o = base or zero range in hundreds of yards
X.sub.2 = range in hundreds of yards for which movement is desired
from the base range
The reticle used to circumscribe the full field of view is
preferably of circular design, though the horizontal length can
also be greater than its vertical length (height). The reticle is
preferably constructed as a unitary member, and includes both the
aim point and the stadia, or rangefinder. The aim point can
comprise essentially any kind of indicia, cross hairs, a dot, an
open juncture between converging lines, and the like. The
rangefinder can be any type of device normally used for measuring
distance, but preferably the rangefinder is as described, though it
can be located virtually anywhere within the field away from the
optic center.
It is also feasible to grind ocular lens such that the optic center
does not correspond with the geometric center, and thus the off-set
or eccentric aim point may appear centered.
It is apparent that these and other various changes, such as in the
absolute or relative dimension of the parts, materials used, use of
constant off-set for manufacturing purposes with allowance of
maximum range variance to fit ballistics data, and the like, can be
made without departing the spirit and scope of the invention, as
will be apparent to those skilled in the art.
* * * * *