CN1995943A - Omnibearing detection method for large-diameter aspherical mirror - Google Patents
Omnibearing detection method for large-diameter aspherical mirror Download PDFInfo
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- CN1995943A CN1995943A CN 200710048201 CN200710048201A CN1995943A CN 1995943 A CN1995943 A CN 1995943A CN 200710048201 CN200710048201 CN 200710048201 CN 200710048201 A CN200710048201 A CN 200710048201A CN 1995943 A CN1995943 A CN 1995943A
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Abstract
The big caliber nonspherical lens inspection controls the moving conoscope through the computer, continuously scanning the big caliber nonspherical lens along the symmetrical axis, acquiring the interference thread changing through time. The generated reference ball surface wave automatically matching with the nonspherical ball surface to be inspected, the best matching zone with low frequency distinguishable interference thread, moving from the center to the edge in the scanning process. Through acquiring the best matching point data to make overall caliber restructuring before the wave, it can acquire the overall information of the nonspherical surface. It is free from design and nonspherical surface compensator, and junction of sub caliber, providing an efficient tool to overall inspection for big caliber nonspherical lens with broad prospect.
Description
Technical field
The present invention relates to a kind of optical detective technology, particularly a kind of at rotational symmetric heavy caliber aspherical mirror detection method, belong to the advanced optical length of schooling and make and the detection technique field.
Technical background
So-called aspherical optical element, be meant face shape by the multinomial equation of higher degree determine, the radius optical element all inequality of each point on the face shape.Aspheric mirror belongs to special surface, and it has the character of many uniquenesses.Do not have spherical aberration as quadric surface at appropriate conjugate position, aspheric surface be used for optical system, can the minimizing system in the quantity of optical element maybe can improve image quality.Along with the development of optical precision processing, aspheric surface is applied in the various optical systems more and more widely, as: high-quality camera, video camera etc.In numerous areas such as uranoscopy, space communication system, light laser weapon emission coefficient, use heavy caliber aspherical mirror widely, it has image quality height, little, the lightweight characteristics of volume, and in these fields, aspheric surface plays the irreplaceable effect of sphere.Therefore, along with aspheric surface application more and more widely, the aspheric high-acruracy survey of the dark type of aspheric measurement especially heavy caliber is become a present hot issue.
Usually, the quantitative detecting method of check aspheric mirror has aberrationless point method, compensator method and calculation holographic method.Aberrationless point method is only applicable to check reflective secondary aspherical, and it is formed around the axis rotation that connects its geometrical focus by quafric curve.Except that check concave ellipsoidal surface mirror, remaining quadric aberrationless detects and all needs to utilize auxiliary plane or spherical mirror.This method is all very difficult to design and the manufacturing that detects the auxiliary mirror of the required high-precision heavy-caliber of heavy caliber deep aspherical mirror, in fact can't adopt.
The compensator method is with suitable compensator, the non-spherical wavefront that the compensation aspheric surface produces, make it to overlap with the theoretical face shape of plane was seized, and the normal of each point does not meet at a bit on the aspheric surface, make each light that light source point sends through after the bucking-out system along aspheric normal incidence on aspheric surface, return along former road then, interfere with reference wave, be the spherical aberration and the match of aspheric normal aberration of compensator, its result of interference demonstrates aspheric surface form deviation then.If wavefront and reference wavefront after the compensation are perfectly mated, interference fringe is exactly the vertical bar line so, otherwise striped is crooked, and crooked degree has just shown that non-spherical surface departs from the degree of ideal surfaced.Most important opticator is a compensator in the penalty method.The compensating interferometer measurement is the very high method of a kind of measuring accuracy, and compensator can be little more a lot of than tested aspheric surface.Therefore, penalty method is widely used in the measurement of aperture aspherical now.But, increase along with minute surface bore and relative aperture, need design and the more complicated compensator of assembling, and the requirement of precision and its arrangement precision to itself are also higher, this is that the cost of high-accuracy compensator is very high simultaneously because the precision of compensator should be higher than the precision of measured lens, and every suit compensator can only be measured one type aspheric surface, measure dumbly, limited the application of penalty method.Maximum difficulty be can not the independent measurement compensator compensation effect.
Lohrnann and Paris proposed the calculation holographic technology in 1967, its principle of interference is that to generate hologram with computing machine be holographic model, can reproduce various standard non-spherical wavefronts, plays reference surface or compensator.Adopt computed hologram, can compensate the systematic error wavefront of aspheric surface and sphere, play compensator.But for bigbore aspheric surface, the strain line frequency of hologram is very high, thus its make in fact become impossible.Also there is the problem that is difficult to aim in computed hologram in test macro.
Nineteen eighty-two, the C.J.Kim of U.S. Arizona optical centre has at first proposed sub-aperture test concept, uses small-bore plane reflection lens array to replace the heavy-calibre planar catoptron to realize the autocollimation check of paraboloidal mirror.Up to the present, sub-aperture measuring technology has obtained continuous development.The key issue of technology is that accurate extraction, the data splicing of annular sub-aperture data are handled and the necessary guarantee of hardware aspect.Especially measure for the heavy caliber deep aspherical mirror, the sub-aperture number of required measurement is many, measuring period is long, in testing process, be vulnerable to surrounding environment influence, data processing amount is big, the stitching algorithm complexity in aperture, and can cause propagation of error and accumulation in this process, these factors all can have influence on last measuring accuracy.
Summary of the invention
For overcoming the deficiency of above-mentioned several measuring methods, the detection method of a kind of heavy caliber aspherical mirror whole audience continuous sweep is proposed, this method can solve the problem that existing several quantitative detecting method exists effectively, and is too high as the auxiliary required precision of mirror, makes difficulty, the cost height, data volume is big, and post-processed trouble etc., this method need not design and make complicated aspheric surface compensator, need not to carry out sub-aperture stitching, system architecture is simple, advantages such as data volume Xiao Yi processing.
The present invention is the detection method of a kind of heavy caliber aspherical mirror whole audience continuous sweep, it is characterized in that: make sphericity interferometer optical axis and tested aspheric mirror axis of symmetry realize relative continuous sweep measurement under the condition that overlaps.Measurement mechanism comprises interferometer (for example Feisuo type interferometer), the standard spherical lens as the interferometer annex, tested aspheric mirror, electronic control translation stage and computer control system thereof.The standard spherical lens is placed between interferometer and the tested aspheric surface, is arranged in parallel input path.Move tested aspheric mirror or interferometer (comprising the standard spherical lens) by the computer control electronic control translation stage, perhaps standard spherical lens, make interferometer optical axis and tested aspheric mirror optical axis realize that under the condition that overlaps the relative continuous sweep between interferometer (comprising the standard spherical lens) and the tested aspheric mirror measures, be radiated on the tested aspheric mirror by the spherical wave front that the standard spherical lens converts standard to from the reference planes wavefront of interferometer outgoing, can interfere with reference light wave after reflecting, form interference pattern.This is the two-dimentional interferogram with two space variables, corresponding to the XY coordinate.Good and the part that frequency is minimum of fringe contrast is spherical wave front and tested aspheric optimum matching zone in the pattern, and these zones could be by interferometer institute resolved measurement.When moving interferometer (comprising the standard spherical lens) by electronic control translation stage continuous precision on optical axis direction by the empty system of computing machine, perhaps standard aspheric mirror, during perhaps tested aspheric mirror, interferometer will detect a series of so two-dimentional interferograms, these matching areas also can along with scanning process on aspheric surface therefrom the mind-set edge move.Introduce and move the time variable that is experienced continuously, corresponding with the moving coordinate (Z coordinate) of electronic control translation stage.We have just obtained comprising the three-dimensional interference bar graph of 2 space variables and 1 time variable like this.In fact, pixel is that the XY coordinate is corresponding with two space variables in the detector.Each pixel in the detector all has the corresponding XY value of determining in three-dimensional fringe figure coordinate system, remaining Z coordinate correspondence time variable, proposing this separately is the one dimension striped of variable with Z, just obtains corresponding on this pixel coordinate, that detect, time dependent interference light intensity and distribute in the continuous sweep process.By being carried out digital space filtering, this one dimension striped extracts best match position, just can XYZ coordinate combined calculation corresponding go out tested aspheric wave aberration with it, after each pixel in the detector all finished this processing, also just finished tested aspheric detection has been measured.
The present invention's advantage compared with prior art
1. the present invention has the design of need not and makes the aspheric surface compensator, need not to design and make the advantage of calculation holographic zero compensation machine, overcome the auxiliary mirror that exists in aspheric surface compensator method and the holography method manufacturing, check, debug shortcoming such as difficulty.
2. the present invention can detect rotational symmetric secondary aspherical and high order aspheric surface, has broken through the restriction that traditional aberrationless point method only can detect the secondary aspherical mirror.
3. only used among the present invention simple in structure, the standard spherical lens that manufacturing process is very ripe, the precision height, cheap, it is convenient to buy, and has saved cost greatly.
4. the measuring method of the present invention's employing is the measurement of full field to tested aspheric mirror, does not need to carry out sub-aperture (comprising annular sub-aperture) splicing, so do not need complicated stitching algorithm, does not have stitching error.
5. can obtain the three-dimensional relationship figure of axial spherical aberration δ L and aspheric surface normal angle easily, and ideal value relatively can be observed out visually the difference between tested aspheric surface and the desirable aspheric surface very much, have very high sensitivity, its difference value can be come quantificational expression with wave aberration.
6. the evaluation result of native system is represented with wave aberration, be to measure itself and apex sphere or the most approaching relatively ball or other relatively bias of ball arbitrarily, than having reflected aspheric characteristic more accurately with both coordinate difference representations on optical axis direction along aspheric normal direction.
In sum, native system is simple in structure, principle is clear, needed device is easy to make, and cheap, the result estimates with wave aberration, visual pattern, overcome the more existing limitation of existing aberrationless point method, compensator method, holography method and sub-aperture stitching, can detect the secondary and the high order deep aspherical mirror of heavy caliber, big relative aperture, the field is widely used.
Description of drawings
The detection method principle schematic of Fig. 1 for mentioning among the present invention;
In Fig. 2 continuous sweep process, the automatic matched position of reference spherical wave front that interferometer produces and tested aspheric surface changes synoptic diagram;
Fig. 3 is in the continuous sweep measuring process, the time dependent interference fringe of the whole audience that obtains, i.e. three-dimensional interference striped synoptic diagram;
Fig. 4 obtains one of time dependent interference fringe of the whole audience for what mention among the present invention, when mating with tested aspheric surface axis of symmetry center circle territory with reference to spherical wave front, promptly is similar to the Z among Fig. 3
0The simulation interferogram at coordinate position place;
That mentions among Fig. 5 the present invention obtains two of the time dependent interference fringe of the whole audience, during with reference to spherical wave front and ring belt area, tested aspheric surface semiaperture coupling, promptly is similar to the Z among Fig. 3
1The simulation interferogram at coordinate position place;
That mentions among Fig. 6 the present invention obtains three of the time dependent interference fringe of the whole audience, during with reference to spherical wave front and outer ring region, tested aspheric surface edge coupling, promptly is similar to the Z among Fig. 3
2The simulation interferogram at coordinate position place;
In Fig. 7 continuous sweep process, tested aspheric surface is crossed on the section of axis of symmetry, promptly among Fig. 3 on the ∑ plane of transversal three-dimensional interference figure, and the time dependent simulation interferogram of each point;
Fig. 8 is in the three-dimensional interference striped of mentioning among the present invention, and a pixel is the time dependent intensity distribution that the O point detects in the continuous sweep process among Fig. 3 and Fig. 7 in the detector center circle territory;
Fig. 9 is in the three-dimensional interference striped of mentioning among the present invention, and a pixel is the time dependent intensity distribution that the A point detects in the continuous sweep process among Fig. 3 and Fig. 7 in the ring belt area, detector semiaperture;
Figure 10 is in the three-dimensional interference striped of mentioning among the present invention, and the pixel in the outside, detector edge is the time dependent intensity distribution that the B point detects in the continuous sweep process among Fig. 3 and Fig. 7;
Figure 11 calculates synoptic diagram for wave aberration;
Embodiment
As shown in Figure 1, native system mainly is made up of interferometer (for example Feisuo type interferometer), spherical lens 9, tested aspheric mirror 10, electronic control translation stage 11, digit driver 12 and computer system 14.Interferometer wherein mainly is made up of LASER Light Source 1, collimation lens 2, plane standard lens 3, Amici prism 4, imaging len 5 and ccd detector 6.Standard spherical lens 9 is between interferometer and tested aspheric mirror 10, and three's optical axis is located along the same line.One of implementation method is that tested aspheric mirror 10 is placed on the electronic control translation stage, it carries out accurately moving on optical axis direction by digit driver 12 controls by computer system 14, makes tested aspheric mirror 10 and the spherical wave front that is produced by interferometer and spherical lens 9 form relative scanning.This relative scanning also can realize by other two kinds of embodiments.Two of implementation method: move interferometer (comprising the standard spherical lens) by the computer control electronic control translation stage, make tested aspheric mirror 10 and the spherical wave front that produces by interferometer and spherical lens 9 form relative scanning.Three of implementation method: move the standard spherical lens by the computer control electronic control translation stage, make tested aspheric mirror 10 and the spherical wave front that produces by interferometer and spherical lens 9 form relative scanning.In the following narration, will be that example describes with one of implementation method.
The principle of work of native system: when the laser beam collimation, incide collimating and beam expanding system 7 by Amici prism 4,8, light beam is a parallel beam, again by behind the standard flat camera lens 3, a part is reflected and returns to form reference wavefront, a part incides and forms the standard spherical wave front on the standard spherical lens 9, after reflecting, aspheric mirror to be measured converts the plane wave front that has been out of shape again to, wherein just carried tested aspheric face shape error information, it is interfered with reference beam by Amici prism 4 reflection backs, and the interference fringe of generation is placed on the CCD device 6 of imaging len 5 positions of focal plane and surveys.Because with reference to having big slope differences between spherical wave front and the aspheric mirror surface, this will cause interference pattern to have very high fringe density.Fig. 4 is the simulation interferogram during with reference to spherical wave front and tested aspheric surface axis of symmetry center circle territory coupling, and the interference fringe corresponding with place, center circle territory has lower spatial frequency.The interference fringe of other parts has higher spatial frequency; 5 for after moving axially a segment distance.Simulation interferogram during with reference to spherical wave front and ring belt area, tested aspheric surface semiaperture coupling, the interference fringe corresponding with the ring belt area, semiaperture has lower spatial frequency, and the interference fringe of other parts has higher spatial frequency; Fig. 6 is after axially continuing to move certain distance, simulation interferogram during with reference to spherical wave front and tested aspheric surface outer ring region coupling, the interference fringe corresponding with the outer ring region has lower spatial frequency, and the interference fringe of other parts has higher spatial frequency.As can be seen from the figure, have only the fraction fringe contrast good and frequency is lower in these interference fringes, can be differentiated by interferometer, this zone is exactly spherical wave front and tested aspheric optimum matching zone.We control motorized precision translation stage with computing machine 14 by digit driver 12 and move continuously at optical axis direction, different reference spherical wave fronts will be mated automatically with different ring belt area on the tested aspheric mirror, and these matching areas can move at the mind-set edge from aspheric surface.In this process, note these interference patterns with interferometer continuous sweep, just got access to the time dependent interference fringe of the whole audience, i.e. three-dimensional interference striped, as shown in Figure 3.With time t (Z is corresponding with coordinate) is variable, volume coordinate XY is a constant, the one dimension bar graph that changes with moving process is proposed from the three-dimensional interference bar graph, promptly be in the detector therewith certain pixel of coordinate XY value correspondence in the continuous sweep process, continue to detect time dependent interference optical field intensity.Fig. 8 is the time dependent simulation interferogram that detects of O point among Fig. 3 and Fig. 7 for pixel in the detector center circle territory that extracts from the three-dimensional interference striped; Fig. 9 is the time dependent simulation interferogram that detects of A point among Fig. 3 and Fig. 7 for certain pixel between the detector center that extracts from the three-dimensional interference striped and the edge; Figure 10 is the time dependent simulation interferogram of B point among Fig. 3 and Fig. 7 for pixel in detector edge of extracting from the three-dimensional interference striped.After these one dimension stripeds are carried out digital space filtering and extract best match position Z, note this value, and corresponding with the XY coordinate of this moment.Each pixel in the detector is all done same this processing.Z value from optimal match point can draw axial spherical aberration δ L like this, can obtain the three-dimensional relationship figure at δ L and XY.With the ideal value contrast, can find out the difference between tested aspheric surface and the desirable aspheric surface very visually.Can draw the angle of tested aspheric surface normal and optical axis again from the XY value, but go out it with respect to the wave aberration N that compares ball, promptly among the figure according to following wave aberration formula 1 integration quantitative Analysis
Distance, obtain the face shape information of full aperture.Δ in the formula
xRelatively ball is with respect to the centre of sphere side-play amount of apex sphere for this reason, and R is paraboloidal vertex curvature radius.
Detection step of the present invention is as follows:
The first step: select high-precision spherical lens, what guarantee to produce is the reference spherical wave front of standard.
Second step: build measuring system according to schematic diagram 1, correct mounting spherical lens 9 also carry out careful adjustment, require spherical lens 9, tested aspheric mirror 10 and are all overlapped as far as possible with laser beam axis by the centers of 7, the 8 collimator and extender parts that constitute.
The 3rd step: the tested aspheric mirror that places on the platform is moved on optical axis direction by computing machine 14 control electronic control translation stages 11, the standard spherical wave front and the tested aspheric mirror 10 that make plane light wave see through spherical lens 9 generations mate in center circle territory part, depart from minimum, obtained being similar to the interference pattern of Fig. 3, core interference fringe density is little, and marginal portion interference fringe density is big.
The 4th step: the tested aspheric mirror that places on the platform is moved continuously on optical axis direction away from spherical lens 9 by computing machine 14 control electronic control translation stages 11, at this moment plane light wave is moved by middle mind-set edge through the standard spherical wave front of spherical lens 9 generations and the matching area of tested aspheric mirror 10, obtain being similar to the interferogram of Fig. 4, when matching area just moves on to tested aspheric surface edge, obtain being similar to the interferogram of Fig. 5.In this process, interferometer continuous sweep, and with this a series of interference pattern under the computing machine continuous recording, be exactly the time dependent interference fringe of the whole audience, promptly the three-dimensional interference striped comprises two volume coordinates and a time coordinate.
The 5th step: find out optimal match point.Pixel is that the XY coordinate is corresponding with two space variables in the detector, with volume coordinate XY is constant, time Z is a variable, one dimension bar graph with the moving process variation is proposed from the three-dimensional interference bar graph, promptly be in the detector therewith certain corresponding pixel of coordinate XY value in the continuous sweep process, continue to detect time dependent interference optical field intensity, the one dimension that obtains being similar to Fig. 8, Fig. 9, Figure 10 is simulated the interference strength distribution plan.All pixels of detector are all done this handle, can obtain the one dimension bar graph of pixel resolution number altogether.These one dimension stripeds are carried out digital space filtering extract best match position, note the XYZ coordinate value of this moment.
The 5th step: wave aberration calculates.The imagination aspheric surface has the wavefront by the optical system outgoing of very big aberration in fact, and the normal of aspheric surface is exactly the light by this system's outgoing.When the bias of aspheric surface and apex sphere during, it can be regarded as the wave aberration of this system along aspheric normal measure.Be worth shaft to spherical aberration δ L from the Z of optimal match point, be worth the angle of tested aspheric surface normal and optical axis from XY.For example, when detecting the tested paraboloidal mirror of no central obscuration, the value of optimal match point in coordinate system is XYZ, and obviously, XY all is integers, can get:
Wherein, CCD resolution is L * L, and-L/2≤X, Y≤L/2, R are paraboloidal vertex curvature radius, D is the parabolic lens bore,
Be the maximum slope of aspheric surface normal, z
0It is the vertex curvature ball centre of sphere.Calculate the wave aberration that compares ball with vertex curvature according to top wave aberration to formula 1 integrating meter again, obtain tested aspheric surface whole audience information.
Claims (7)
1, a kind of Omnibearing detection method for large-diameter aspherical mirror.It is characterized in that: move interferometer or tested aspheric mirror by the computer control electronic control translation stage, make interferometer optical axis and tested aspheric mirror optical axis under the condition that overlaps, realize relative continuous sweep measurement, obtain the time dependent interference fringe of the whole audience, i.e. the three-dimensional interference striped.In the continuous sweep process, the reference spherical wave front that interferometer produces will be mated automatically with tested aspheric surface, the distinguishable interference fringe of the corresponding low frequency in optimum matching zone (annular region), with scanning process on aspheric mirror therefrom the mind-set edge move.The three-dimensional interference striped is carried out data processing, extract the optimum matching point data of interference fringe and carry out the full aperture wavefront reconstruction, thereby obtain tested aspheric surface whole audience information.
2, a kind of Omnibearing detection method for large-diameter aspherical mirror according to claim 1, it is characterized in that: described interferometer optical axis and the tested aspheric mirror axis of symmetry of making realized relative continuous sweep measurement under the condition that overlaps, comprise by the computer control electronic control translation stage and move interferometer (for example Feisuo type interferometer), along tested aspheric mirror axis of symmetry heavy caliber aspherical mirror is carried out continuous sweep and measure, obtain the time dependent interference fringe of the whole audience; Comprise that also moving tested aspheric mirror by the computer control electronic control translation stage carries out the continuous sweep survey along the aspheric mirror axis of symmetry to interferometer, obtains the time dependent interference fringe of the whole audience; Comprised also that the computer control electronic control translation stage moved the standard spherical lens that produces spherical wave in the interferometer (for example Feisuo type interferometer) and along tested aspheric mirror axis of symmetry heavy caliber aspherical mirror carried out the continuous sweep measurement, obtained the time dependent interference fringe of the whole audience.
3, a kind of Omnibearing detection method for large-diameter aspherical mirror according to claim 1, it is characterized in that: the time dependent interference fringe of the described whole audience, be that the three-dimensional interference striped is an intensity distribution function that comprises 3 variablees, wherein 2 variablees are space variables, corresponding XY coordinate system, 1 variable is a time variable, under the situation of uniform speed scanning corresponding with the electronic control translation stage moving coordinate (Z coordinate).
4, a kind of Omnibearing detection method for large-diameter aspherical mirror according to claim 1, it is characterized in that: described electronic control translation stage has the repeatable accuracy and the bearing accuracy of μ m level, control by digit driver by computer system, be intended in the measuring process accurately locating along the displacement of Z axle.
5, a kind of Omnibearing detection method for large-diameter aspherical mirror according to claim 1, it is characterized in that: described the three-dimensional interference striped is carried out data processing, extract the optimum matching point data of interference fringe and carry out the full aperture wavefront reconstruction, optimal match point refers to this position relatively ball and aspheric points of tangency, with the optimal match point position that the method for digital space frequency domain filtering is extracted interference fringe, electronic control translation stage moving coordinate (Z coordinate) and the detector pixel point corresponding XY coordinate corresponding with this point calculate heavy caliber aspherical mirror whole audience face shape.
6, a kind of Omnibearing detection method for large-diameter aspherical mirror according to claim 1, it is characterized in that: described measuring method is the measurement of full field to tested aspheric mirror, do not need to carry out sub-aperture (comprising annular sub-aperture) splicing, do not have stitching error.
7, a kind of Omnibearing detection method for large-diameter aspherical mirror according to claim 1, it is characterized in that: the evaluation result of described full aperture wavefront reconstruction is represented with wave aberration, be to measure itself and apex sphere or the most approaching relatively ball or other relatively bias of ball arbitrarily, than having reflected aspheric characteristic more accurately with both coordinate difference representations on optical axis direction along aspheric normal direction.
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