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Claims  |
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I claim:
1. A method for determining the distance between a first preselected point
and a second point comprising the steps of:
(a) providing a first beam of electromagnetic radiation at a first optical
wavelength;
(b) splitting said first beam at said first preselected point into a beam
following a first path and a beam following a second path, said first path
beam being focused onto a first reflective surface a known distance from
said preselected point, said known distance being defined as L.sub.r, said
second path beam being focused onto a reflective surface at said second
point an unknown distance from said preselected point, said unknown
distance being defined as L.sub.x ;
(c) defining L.sub.x -L.sub.r =L and 2L=N.sub.1 .lambda..sub.1 +l.sub.1 ;
wherein N.sub.1 =the integer number of wavelengths in said 2L;
.lambda..sub.1 =said first wavelength; and l.sub.1 =the residual
fractional wavelength in said distance 2L and wherein l.sub.1 =.phi..sub.1
.lambda..sub.1 /2.pi. where .phi..sub.1 =the optical phase difference of
said first beam between L.sub.x and L.sub.r at said first wavelength;
(d) determining the optical phase difference, .phi..sub.1 ;
(e) replacing said first beam with at least a second beam of
electromagnetic radiation at a second optical wavelength, said second beam
following the same optical path as said first beam such that said second
beam is split into a beam following said first path and a beam following
said second path, said first path beam of said second beam being focused
onto said first reflective surface said known distance from said
preselected point, said known distance being defined as L.sub.r, said
second path beam of said second beam being focused onto said reflective
surface at said second point an unknown distance from said preselected
point, said unknown distance being defined as L.sub.x ;
(f) defining L.sub.x -L.sub.r =L and 2L=N.sub.2 .lambda..sub.2 +l.sub.2 ;
wherein N.sub.2 =the integer number of wavelengths in said 2L;
.lambda..sub.2 =said second wavelength and l.sub.2 =the residual
fractional wavelength of said distance 2L and wherein l.sub.2 =.phi..sub.2
.lambda..sub.2 /2.pi. where .phi..sub.2 =the optical phase difference of
said second beam between L.sub.x and L.sub.r at said second wavelength;
(g) selecting said second wavelength, .lambda..sub.2, at a wavelength
different than said first wavelength but closely spaced thereto such that
N.sub.1 =N.sub.2 ;
(h) determining the optical phase difference .phi..sub.2,
(i) utilizing the determined .phi..sub.1 and .phi..sub.2 in order to
determine l.sub.1 and l.sub.2 from the relationships l.sub.1 =.phi..sub.1
.lambda..sub.1 /2.pi. and l.sub.2 =.phi..sub.2 .lambda..sub.2 /2.pi.,
respectively;
(j) determining the integer number of wavelengths, N.sub.1, in 2L by
inserting the previously determined l.sub.1 and l.sub.2 in the equation
N.sub.1 =N.sub.2 =(l.sub.1 -l.sub.2)/(.lambda..sub.2 -.lambda..sub.1);
(k) determining L by inserting the determined N in the equation L=(N.sub.1
.lambda..sub.1 +l.sub.1)/2;
(l) determining said unknown distance, L.sub.x, by inserting L determined
in step (k) in the equation L.sub.x =L-L.sub.r.
2. A method for determining the distance between a first preselected point
and a second point as defined in claim 1 wherein said first and said
second beams of electromagnetic radiation are provided by a laser.
3. A method for determining the distance between a first preselected point
and a second point as defined in claim 2 wherein said optical phase
differences .phi..sub.1 and .phi..sub.2 are determined by an
interferometer.
4. A method for determining the distance between a first preselected point
and a second point as defined in claim 1 wherein range determining means
are provided for producing said first and said second beams of
electromagnetic radiation and determining said phase differences
.phi..sub.1 and .phi..sub.2, said range finding means having a preselected
unambiguous range.
5. A method for determining the distance between a first preselected point
and a second point as defined in claim 4 wherein said preselected
unambiguous range is defined as L.sub.u and said second wavelength can be
determined by the equation 2L.sub.u =c/(f.sub.1 -f.sub.2) wherein c=the
speed of light and f.sub.1 =c/.lambda..sub.1 and f.sub.2
=c/.lambda..sub.2.
6. A method for determining the distance between a first preselected point
and a second point comprising the steps of:
(a) providing a first beam of electromagnetic radiation at a first optical
wavelength;
(b) splitting said first beam at said first preselected point into a beam
following a first path and a beam following a second path, said first path
beam being focused onto a first reflective surface a known distance from
said preselected point, said second path beam being focused onto a
reflective surface at said second point an unknown distance from said
preselected point;
(c) determining an optical phase difference of said first beam as said
first beam traverses said first path said known distance from said
preselected point and said second path said unknown distance from said
preselected point;
(d) replacing said first beam with at least a second beam of
electromagnetic radiation at a second optical wavelength, said second beam
following the same optical path as said first beam such that said second
beam is split into a beam following said first path and a beam following
said second path, said first path beam of said second beam being focused
onto said first reflective surface said known distance from said
preselected point, said second path beam of said second beam being focused
onto said reflective surface at said second point said unknown distance
from said preselected point;
(e) selecting said second wavelength at a wavelength different than said
first wavelength but closely spaced thereto such that a number of whole
wavelengths in the path difference between said unknown distance and said
known distance is the same for both said first and said second
wavelengths;
(f) determining the optical phase difference of said second beam as said
second beam traverses said first path said known distance from said
preselected point and said second path said unknown distance from said
preselected point;
(g) utilizing said optical phase difference of said first beam, said
optical phase difference of said second beam, said first wavelength and
said second wavelength to establish said number of whole wavelengths in
said path difference between said unknown distance and said known
distance;
(h) combining said number of whole wavelengths with said optical phase
difference of said first beam and said first wavelength in order to
establish said path difference between said unknown distance and said
known distance; and
(i) determining said unknown distance between said first preselected point
and said second point by combining said known distance with said path
difference between said unknown distance and said known distance. |
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Claims  |
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Description  |
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BACKGROUND OF THE INVENTION
This invention relates generally to distance measurement techniques, and,
more particularly to an interferometric distance measurement method for
optically measuring distance over relatively long paths with resolution to
a small fraction of an optical wavelength, but without the range ambiguity
inherent in conventional interferometry.
In today's highly industrialized and highly technological society it
becomes more and more essential to provide devices and/or techniques
capable of measuring distances over relatively long paths. Such a case
would be, for example, in the alignment of large telescopes constructed
from small subapertures wherein accuracies of less than 0.1 .mu.m over
ranges of up to 50 meters are required. There are several conventional
techniques which are utilized in making such distance measurements,
however, most of these techniques combine the utilization of both
interferometry and geodimetry. Such systems, therefore, utilize complex
hardware made up of modulators, phase detectors, phase matched amplifiers,
etc.
In relying on interferometry as a technique for distance measurement it is
generally necessary to measure the distance between an unknown path and a
reference path in which an ambiguity factor must be resolved in achieving
these measurements. Heretofore, ambiguity resolution was achieved by
making a plurality of measurements at increasingly longer wavelengths. For
example, if the first measurement was made using a wavelength of 1 .mu.m,
a second measurement might be made at 100 .mu.m, and a third measurement
at 10 cm etc., with each successive measurement used to resolve the
ambiguity in the previous measurement wherein the actual choice of
wavelengths is a function of the precision that is achieved in the phase
measurement process. Unfortunately, it is extremely inconvenient to make
measurements at all of these wavelengths, since each regime requies
different techniques and different equipment. In addition, operation at
longer wavelengths (as set forth hereinabove) makes beam confinement more
difficult.
To overcome these problems many techniques of the past have utilized a
subcarrier technique, where the longer wavelength signal is used to
modulate an optical carrier which is propagated over the path. In such a
technique, a lower frequency modulation is placed on the optical or other
carrier beams transmitted over the unknown path to a reflector and back,
demodulated to recover the modulation, and then compared in phase to the
modulating signal. The phase difference would be a function of the path
delay which is proportional to the path length.
As clearly set forth hereinabove, it is quite apparent that the devices and
techniques of the past leave much to be desired in the precise measurement
of distance over relatively long paths. Therefore, an interferometric
measurement method capable of overcoming the above-mentioned problems is
highly desirable.
SUMMARY OF THE INVENTION
The instant invention overcomes the problems encountered in the past by
providing an interferometric distance measurement method utilizing a
single instrument and which is capable of optically measuring distance
over relatively long paths with resolution of up to a small fraction of an
optical wavelength. Consequently, this invention eliminates equipment
necessary to generate the subcarriers, modulate the carrier and demodulate
the received signals.
The interferometric distance measurement method of this invention performs
the equivalent of measuring distances at a relatively long wavelength (as
in the past) by measuring the phase difference at two closely spaced
optical wavelengths and computing the effective phase measurement at a
wavelength which corresponds to the frequency difference between the two
optical wavelengths measured. In general, an approximate distance
measurement can be performed by any of the prior instruments for distance
measurement. The accurate measurement, however, is performed by the method
of this invention wherein the determination of range or distance requires
the measurement of optical paths or phase differences between two paths, a
reference or known path and an unknown path. This phase difference can be
measured by any conventional interferometer utilized within the system of
this invention.
With this invention any suitable source of electromagnetic radiation, in
the optical wavelength region is utilized to provide a beam which can be
directed to a reflective element located at the unknown distance, L.sub.x,
and to a reflective element at a known distance, L.sub.r. The phase
difference between the receipt of these two signals can be detected by any
conventional interferometer. The distance which is measured by this
invention, L, is the difference L.sub.x -L.sub.r. By utilizing the formula
2L=N.lambda.+l where N is the integer number of wavelengths in the path
2L, .lambda. is the wavelength, l is the residual fractional wavelength of
the distance 2L and wherein l=.phi..lambda./2.pi. where .phi. is the
optical phase difference of a beam directed between distances L.sub.x and
L.sub.r ; the distance L can be determined. This determination is made by
a series of measurements at closely spaced optical frequencies or
wavelengths. In so doing, the necessity of subcarrier technique is
eliminated.
It is therefore an object of this invention to provide an interferometric
distance measurement method which is extremely accurate over relatively
long paths.
It is another object of this invention to provide an interferometric
distance measurement method which is substantially more simplified than
techniques heretofore in use.
It is a further object of this invention to provide an interferometric
distance measurement method which is capable of using only a single
instrument and repetitive measurements using only closely spaced optical
wavelengths.
For a better understanding of the present invention, together with other
and further objects thereof, reference is made to the following
description taken in conjunction with the accompanying drawing and its
scope will be pointed out in the appended claims.
DETAILED DESCRIPTION OF THE DRAWING
The only FIGURE of the drawing is a schematic representation of the
interferometric distance measurement method of this invention.
DETAILED DESCRIPTION OF THE PREFERRED METHOD OF THE INVENTION
Reference is now made to the only FIGURE of the drawing which schematically
illustrates the interferometric distance measurement instrument 10
utilized in the performance of the distance measurement method or
technique of this invention. Measurement instrument 10 incorporates
therein any conventional source of electromagentic radiation 12,
preferably in the form of a laser emitting a beam 14 in the optical
wavelength region. Also forming part of instrument 10 is any conventional
beam dividing device such as beam splitter 16 capable of dividing beam 14
into two portions, hereinafter referred to as beams 18 and 20. Beam 18 is
directed a known distance, L.sub.r, away from beam splitter 16 to any
suitable reflective element 22 in the form of a mirror. Beam 20 is
directed an unknown distance, L.sub.x, away from beam splitter 16 to
another reflective element 24 in the form of another mirror.
Upon striking reflective elements 22 and 24, respectively, beams 18 and 20
are reflected therefrom and are received by any conventional detector 26
capable of measuring the phase difference, .phi., between beams 18 and 20.
Detector 26 may be in the form of a conventional interferometer, for
example. Since the components making up the interferometric distance
measurement instrument 10 utilized with the method of this invention are
conventional, the detailed description set forth hereinbelow will describe
with specificity only the method of this invention.
As pointed out hereinabove the unknown distance is depicted as L.sub.x,
however, for purposes of convenience and ease of understanding of this
invention the distance that will be measured by this invention will be
hereinafter referred to as, L, the difference between the unknown distance
L.sub.x and the known distance L.sub.r (i.e., L=L.sub.x -L.sub.r). Since
the distance L is travelled in two directions the more common expression
2L=N.lambda.+l will be the basic expression utilized with the method of
this invention. In this expression, N=the integer number of wavelengths in
distance 2L, .lambda.=the wavelength of beam 14 and l=the residual
wavelength in distance 2L.
In the past, resolution of the ambiguity or residual wavelength in the
distance l was achieved by a plurality of measurements made at
increasingly larger wavelengths. Such a procedure was extremely
inconvenient since it required a plurality of techniques and different
instruments at different wavelengths. For example, the wavelengths
generally ranged between the optical and the radiowave. The method of the
instant invention overcomes this problem, not by the subcarrier technique
described hereinabove, but by a method wherein measurements are made at
closely space optical wavelengths with a single instrument. Such a
procedure, as set forth in detail hereinbelow, is the equivalent of making
measurements at relatively long wavelengths by measuring the phase
difference of at least two closely spaced optical wavelengths and
computing the effective phase measurement at a wavelength which
corresponds to the frequency difference between the two optical
frequencies measured.
More specifically, and still referring to the only FIGURE of the drawing a
first beam of electromagnetic radiation having an optical wavelength
.lambda..sub.1 is emitted by laser 12. Consequently, the general
expression for 2L set forth hereinabove can be rewritten as
2L=N.sub.1 .lambda..sub.1 +l.sub.1 where l.sub.1 =.phi..sub.1
.lambda..sub.1 /2.pi. (1)
for the first beam.
In equation (1) there are two unknown quantities, L and N.sub.1 and
therefore additional information is necessary to solve this equation. To
obtain this additional information, a second beam is emitted by laser 12
having an optical wavelength .lambda..sub.2 closely spaced to the optical
wavelength of the first beam. Therefore,
2L=N.sub.2 .lambda..sub.2 +l.sub.2 where l.sub.2 =.phi..sub.2
.lambda..sub.2 /2.pi. (2)
for the second beam.
Proceeding mathematically
2L=N.sub.1 .lambda..sub.1 +l.sub.1 =N.sub.2 .lambda..sub.2 +l.sub.2 (3)
Since these are independent measurements, there are two independent
measured quantities (l.sub.1 and l.sub.2) and three unknowns L, N.sub.1
and N.sub.2. In order to solve this equation, the second wavelength
.lambda..sub.2 must be established.
To do so, an assumption must be made that N.sub.1 =N.sub.2, that is, the
integer number of wavelengths at the two closely spaced optical
wavelengths .lambda..sub.1 and .lambda..sub.2 will be equal. Under this
assumption (from equation 3).
N.sub.1 =N.sub.2 =N=(l.sub.1 -l.sub.2)/(.lambda..sub.2 -.lambda..sub.1) (4)
The range of measurement instrument 10 would again become ambiguous when
the term N.sub.1 =N.sub.2 +l (where .lambda..sub.1 =the shortest
wavelength). At the exact point of unambiguity, l.sub.1 =l.sub.2 =0.
Consequently, at the point wherein l.sub.1 =l.sub.2 =0, the unambiguous
range of the two-wavelength combination is
2L.sub.u =N.sub.1 .lambda..sub.1 =(N.sub.1 -1).lambda..sub.2 (5)
or, 2L.sub.u =N.sub.1 .lambda..sub.1 (6)
or, N.sub.1 .lambda..sub.1 =(N.sub.1 -1).lambda..sub.2 (7)
Rearranging equation (7)
N.sub.1 .lambda..sub.2 -N.sub.1 .lambda..sub.1 =.lambda..sub.2 (8)
or, N.sub.1 =.lambda..sub.2 /(.lambda..sub.2 -.lambda..sub.1) (9)
Substituting equation (9) into equation (6) gives
2L.sub.u =(.lambda..sub.2 /(.lambda..sub.2 -.lambda..sub.1)).lambda..sub.1
=(.lambda..sub.2 .lambda..sub.1)/(.lambda..sub.2 -.lambda..sub.1) (10)
The relationship between wavelength and frequency is .lambda.=c/f where
c=speed of ligh and f=frequency. (11)
Substituting equation (11) into equation (10)
2L.sub.u =.lambda..sub.2 .lambda..sub.1 /(.lambda..sub.2
-.lambda..sub.1)=(c/f.sub.2)(c/f.sub.1)/((c/f.sub.2)-(c/f.sub.1))=(c.sup.2
/f.sub.2 f.sub.1)/c((f.sub.1 -f.sub.2)/f.sub.2 f.sub.1) (12)
or, 2L.sub.u =c/(f.sub.1 -f.sub.2) (13)
Consequently, knowing the unambiguous region of instrument 10 and f.sub.1 ;
f.sub.2, that is, .lambda..sub.2 can be determined from equation (13).
In principle, .lambda..sub.1 and .lambda..sub.2 may be selected to achieve
any desired unambiguous range. In practice, however, the maximum range is
set by the accuracy to which the wavelengths are known and to which the
phase may be measured.
If the expression for N.sub.1 from equation (4) is now substituted into
equation (3)
2L=((l.sub.1 -l.sub.2)/(.lambda..sub.2 -.lambda..sub.1)).lambda..sub.1
+l.sub.1 (14)
Since l.sub.1 =.phi..sub.1 .lambda..sub.1 /2.pi. and l.sub.2 =.phi..sub.2
.lambda..sub.2 /2.pi., the values for l.sub.1 and l.sub.2 can be
substituted in equation (14) and after rearranging,
2L=((.phi..sub.1 -.phi..sub.2)/2.pi.)(.lambda..sub.1 .lambda..sub.2
/(.lambda..sub.2 -.lambda..sub.1)) (15)
or, 2L=(.phi..sub.1 .phi..sub.2 /2.pi.)(c/(f.sub.1 -f.sub.2)) (16)
wherein equation (16) represents a phase measurement at the wavelength of
the difference frequency.
EXAMPLE OF THE METHOD OF THE INVENTION
With the method of this invention it is first necessary to establish the
maximum distance (i.e., the unambiguous range, L.sub.u) instrument 10 is
to measure. Let us assume this to be 5 m, thus twice that distance
2L.sub.u =10 m. Let us also assume instrument 10 is to operate at 10.0
.mu.m, an infrared wavelength corresponding to the CO.sub.2 laser. We will
therefore assume an accuracy of measurement of better than 1:1000, and, in
fact it is possible to measure to an accuracy of .+-.3:10,000.
It should further be realized that all references to distance in the
following discussion are related to 2L. Therefore, the result achieved by
the method of this invention would represent 2L and would have to be
divided by 2 to get the distance L which could then be substituted in the
equation L=L.sub.x -L.sub.r to get unknown distance L.sub.x.
Let us choose our first measurement at wavelength .lambda..sub.1 at exactly
10.0 .mu.m, represented by the frequency f.sub.1 =3.times.10.sup.13. Since
it has been established hereinabove that 2L.sub.u =10.0 m, equation (13)
can be utilized to compute frequency f.sub.2 or the second measurement
wavelength .lambda..sub.2. Frequency f.sub.2 computes to be
2.99999.times.10.sup.13 or a wavelength of 10.000001 .mu.m.
Measurements of phase difference .phi..sub.1 and .phi..sub.2 are now made
with instrument 10 at the above two wavelength .lambda..sub.1 and
.lambda..sub.2. A calculation of distance using equation (16) will yield
2L=6.714, for example. Since there is an uncertainty of 3 parts in 10,000
corresponding to 0.003 meters, we know the actual distance (2L) is between
6.711 and 6.717 meters.
We will now make a measurement with an ambiguity range of 0.01 m or 10 mm.
To do this we again use equation (13) and set 2L.sub.u =0.01 m. Using the
original f.sub.1 =3.times.10.sup.13, we compute a new f.sub.2 or
.lambda..sub.2 but for purposes of clarity we will call the new frequency
f.sub.3. Frequency f.sub.3 =2.997.times.10.sup.13 corresponding to a third
wavelength .lambda..sub.3 =10.01001 m. Measurements are now taken of the
phase difference at f.sub.3 or .lambda..sub.3 and the distance 2L from
equation (16) is calculated at 0.005216 meters (5.216 mm). It is to be
recalled that since we assumed N.sub.1 =N.sub.2 the maximum range we can
measure with these frequencies is 0.01 m, and the result must be less than
0.01 m.
Since we picked a convenient value of 0.01 m for our ambiguous range, this
really means that each time the range increases by 0.01 m, N.sub.2 becomes
larger than N.sub.1 by another count. Thus we know that the range can be
0.005216 meters, 0.015216 meters, 0.025216 meters, etc. If we extend this
series of possible ranges, we will eventually realize that the range can
be 6.705216, 6.715216, 6.725216, 6.735216, etc. as N.sub.1 and N.sub.2
diverge by ever increasing amounts. Since we already know (from our first
two measurements) that the distance is between 6.711 and 6.717 m, we
immediately know that the range must be 5.715216 meters, since this is the
only possible value that falls in this range. We have used our first
measurement to resolve the ambiguity in our second measurement.
Of course, our second set of measurements has an uncertainty too. Since we
are now measuring at 0.01 m, our uncertainty of 3 parts in 10,000 means
that we have a possible error of 0.000003 m, thus our range is known to
lie in the region between 6.715213 and 6.715219 m. We can now make a
measurement at 10 .mu.m, which is our optical wavelength. Since we are
measuring directly at f.sub.1, a second frequency is unnecessary.
Assume that this measurement at f.sub.1 results in a range of 0.000008125 m
(8.125 .mu.m). As set forth above, we known that the range can be any
multiple of 10 .mu.m+8.125 .mu.m, thus the values 6.715208125,
6.715218125, 6.715228125, etc., are all valid values for this last
measurement. Again, from our previous measurements, we know that the range
must be 6.715218125, since the other two are outside our previously
established range limits. Of course, we still have our uncertainty in this
last measurement, which is 0.000000003 m, thus we have again bracketed our
range as somewhere between 6.715218122 and 6.715218128 m.
If we need even more accuracy, it is necessary to go to shorter
wavelengths. To do this, we must select a different optical region for
instrument 10. For instance, we may decide to work at 1 .mu.m instead of
10. This, of course, will mean a whole new set of frequencies calculated
from equation (13), and may mean we need to make more than three steps.
However, the principle remains the same. In fact, the original selection
of operating wavelength is determined by the ultimate accuracy required in
the measurements, and is an engineering choice to be made when instrument
10 is designed.
Although this invention has been described with reference to a particular
method, it will be understood to those skilled in the art that this
invention is also capable of a variety of alternate methods within the
scope and spirit of the appended claims.
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Description  |
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