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10.1.2. Subaperture corrector
examples (1)
▐
10.1.2. Subaperture correctors
for twomirror systems
► 10.1.2. Subaperture corrector: Fieldflattener
PAGE HIGHLIGHTS Image field curvature is not a serious detriment to visual observing, due to the natural ability of the eye to accommodate (refocus). In photographic use, however, field curvature induces defocus error, which can be significant. In order to flatten curved image field, an auxiliary lens, or group of lens is placed in front of the final focus, offsetting image curvature by generating one of similar magnitude but opposite in sign. In general, a positive lens, or group of lenses, generates curvature concave towards it, while a negative lens generates image curvature convex toward it. Singlelens flattener The simplest way to correct for field curvature is by placing a single thin lens just in front of the final focus. With proper choice of parameters, it flattens the field while inducing very low aberrations, except at very large relative apertures. Assuming no appreciable astigmatism induced by the lens itself  valid for telescopes, in general, but not for the Schmidt camera, or other very fast systems  the field is flattened when lens' Petzval curvature is equal, and opposite in sign, to the median field curvature of a telescope. This determines needed lens shape as planoconcave (negative) for for Cassegrainlike telescopes, and planoconvex (positive) for the Gregorian. By default, field flattener lens faces image with its flat side, and the sign of its curved surface is determined by the sign of image curvature. Needed radius of curvature of the lens is:
with n being the lens refractive, and Rm the telescope median (best astigmatic) image radius. This, of course, assumes that the lens itself generates zero astigmatism; if it is not so, the needed radius is modified according to the magnitude and sign of lens astigmatism. For the Schmidt camera, field flattener lens is positive, with the radius R=[1(1/n)]RM/2, with RM being the mirror radius of curvature (since it has no astigmatism in the Schmidt arrangement, its best surface coincides with its Petzval surface, which equals RM/2). For the Newtonian, field flattener lens is of negative power, with the radius R=[1(1/n)]Rm/2 (according to the sign convention, with the best field concave toward mirror, Rm is numerically positive in the Newtonian), and so is for the refractor. For the latter, median field curvature varies from one to another type; for a typical doublet achromat median field curvature is approximately /3, being the refractor focal length, and the field flattener's radius R~[1(1/n)]/3 (of negative power). EXAMPLE 1: Schmidt camera field flattener  Good example for the use of a singlelens flattener is the Schmidt camera, which is exclusively a photographic instrument. Its only remaining primary aberration is strong field curvature. This leaves two choices: either use of a curved detector, or sacrificing much of the exquisite field quality by using flat detector. In general, lens aberrations are low if it remains very close to the original focus. But even then, they can be significant with wide angular fields and/or fast focal ratios. Due to the lens thickness being significant relative to object and image separation, the thin lens equations are not appropriate. Instead, aberrations are calculated for each lens surface, similarly to the approach described with the generalized aberration coefficients. Only in this case, with the aperture stop displaced from the front lens surface, the relations need to account for this factor. Numerical value of the stop separation T is determined by system configuration: in the Schmidt camera, for the front lens (flattener's) surface it is the distance from the surface to the corrector (where the mirror reimages the stop), thus numerically negative. For the second lens surface the stop separation is given by T2=α'ch1, h1 being the chief ray height on the second surface (illustrated below; Schmidt flattener thickness exaggerated to show ray paths). In the Newtonian, T1 it is the distance from the lens' front surface to the mirror, numerically positive (ASM on the illustration below, as opposed to ASS, with the aperture stop at the surface and T1=0). In twomirror systems, it is the distance from the lens' surface to the image of the aperture stop (primary) formed by the secondary (exit pupil of the system, ExP on the illustration), numerically negative.
Likewise, the chief ray angle αc is determined by system configuration: in the Schmidt camera, the chief ray coming through the center of the corrector is reflected back to the same point, therefore converging toward the front lens surface at the same incident angle α. Since it is opening upward from the axis, it is numerically positive, and so is the projected normal to the surface angle δ at the axis. Since the angles are small enough to be expressed in radians, it determines the chief ray angle α'c after refraction at the front lens surface as α'c=δ(δα)/n, with all the angles in radians, n being the glass refractive. In a twomirror system, the lens field flattener is of negative power, with both α'cs (chief ray angle after reflection from the secondary, appearing to be coming from the image of the primary formed by the secondary) and the surface normal angle δ numerically negative, the chief ray angle after the front lens surface α'c=δ(δα)/n. Since the rear surface of the flattener is flat, α'c=nαc. The angle μ1=1/2nF for the marginal ray of axial cone determines location of the image formed by the first lens surface as L1'=h0/μ0 from the front lens surface, h0 being the height of marginal ray at the surface, given as h0=l/2F, l being the front lens surface to original focus separation, and F the focal ratio. This outlines the general procedure for calculating aberrations of a singlet field flattener lens facing focus with its flat side. With spherical lens surface, Q=0 and the aberration coefficients for spherical aberration, coma and astigmatism, from Eq. (k)(m), are given by s=NJ2/8, c=NJYh/2 and a=N(Yh)2/2, respectively, with N=n2[(1/n'L')(1/nL)], J=[(1/L)(1/R)], Y=[(1/T)(1/R)] and the height of incident point on the surface h=(Tα), where n, n' are the refractive indici of the incident and refractive/reflecting media, L, L' the surfacetoobject and image separation, respectively, R being the lens surface radius of curvature, T being the surfacetostop separation and α the chief ray angle in radians. Note that the refractive indici are numerically negative, which requires appropriate adjustment to some of the general relations. For instance, needed lens surface curvature to flatten the field is R=(11/nl)Rm/2 with the index n numerically positive, and R=(1+1/nl)Rm/2 with the index negative. With LĞR, Eq. 1 gives L'~n'L/n which, after substitution in the relation for N gives N~n(n2n'2)/(n'2L); also, J~(1/L) for the front lens surface. In terms of the final lens to image separation, L2', L1=L2'+(t/n), L1'=nL2'+t, and L2=nL2'. Stop separation for the front flattener surface is equal to its separation to the corrector, thus T1=Rm/2, Rm being the mirror radius of curvature, and the chief angle αc for the front surface equals the field angle α. For the rear lens surface, the chief ray angle is, from the ray geometry, αc'=(α'/n)[1+(1/n)]γ, with γ=αcT1/R being the lens radius of curvature angle at the front surface point of incidence, and the stop separation for the rear surface T2=(αc/α'c)T1. Alternately, from Eq. 1, T2=n2RT1/[(n2+1)T1R]. Note that all three angles are numerically positive. After laying down the formalism, here is the actual example: lowerorder aberrations induced by a singlet field flattener lens in 200mm /2 Schmidt camera (SPECS). For nearminimum lensimage separation of 2mm, lens thickness t=3mm, lens refractive n'1=n2=nl=1.5, the image shift caused by the lens is approximately [1+(1/nl)]t=1mm, which determines lens location such that its rear surface is ~1mm inside the original focus; thus, the front surface to the original focus separation l=4mm. At this location, the height of marginal ray at the front lens surface  determining the effective (and minimum) front lens aperture semidiameter d1  is d1=l/2F= 1mm (the converging angle represented by 1/2F is numerically negative, since opening counterclockwise, which is why it requires minus sign when expressed using the Fnumber). The indici are n1=1 and n'1=1.5. The front lens surface stop separation T1=404mm, and the height of the incidence point at the front surface for the field (and aperture stop) chief ray angle αc=α=2° is h1=αcT1=404αc=14.1mm. The object distance L equals the separation between lens surface and the image formed by preceding surface, thus L1=4mm. The radius of curvature of the front lens surface needed to flatten the field (assuming near zero lens astigmatism) is R=[1+(1/nl)]Rm/2=133mm. For the rear surface, n=1.5, n'=1. With L'1=nlL1=1.5L1, aperture radius d2=[1+(t/nlL1)]d1=0.5mm. Similar result is obtained using the refracted marginal ray angle of the axial cone μ=(1/2nF)+[1+(1/n)]d1/R, from d2=d1μt=0.49mm. The object distance for this surface is L2=L'1t=3mm, and the image distance L2'=2mm. The chief ray angle at the rear surface α'c=0.058, the stop separation T2=(αc/α'c)T1=242mm, and the incidence point height for the chief ray h2=h1T2/(T2+t)=13.9. The corresponding values of compounded parameters for the front lens surface are N1=0.139, J1=0.25, Y1=0.005, and h1=14.1, giving the aberration coefficients s1=0.0011, c1=0.0012, and a1=0.00035. For the rear surface, N2=0.625, J2=0.33, Y2=0.0041 and h2=13.9mm, giving the aberration coefficients s2=0.0085, c2=0.0059 and a2=0.001. The corresponding combined coefficients for both lens surfaces are sl=s1+(d2/d1)4s2=0.00057, cl=c1+(d2/d1)3c2=0.0019 and al=a1+(d2/d1)2c2=0.0001, with the resulting PV wavefront errors at paraxial focus, in units of 0.00055mm wavelength, Ws=sld14=1, Wc=2cld13=6.9 and Wa=2ald12=0.36 for spherical aberration, coma and astigmatism, respectively. At the best focus location, the errors are smaller by a factor 0.25 for spherical aberration, and 1/3 for coma (PV for the astigmatism remains unchanged, but the RMS error at the best focus is smaller by a factor of 1/√1.5), which gives the final values as Ws=0.25, Wc=2.3 and Wa=0.36. The exact raytrace by OSLO gives for this system Ws=0.2 (the differential mainly due to the residual spherical of the camera), Wc=2.36 and Wa=0.09 (the latter two based on the Zernike aberration coefficients for primary aberrations, with the higher order terms negligible) for the lowerorder aberrations at the best focus location. Most of the lens' astigmatism  about 3/4 of it  is offset by the corrector's astigmatism of opposite sign, with the effective system astigmatism coming at less than 1/10 wave at 2° off axis. Higherorder aberrations are still low, but increasing rapidly with larger relative apertures. Here is the raytrace plot:
Evidently, the most significant aberration induced by the flattener is
coma. An option for
eliminating this (negative) coma is to move Schmidt corrector somewhat
closer to the primary. For this particular system, the separation nearly
eliminating coma, with little effect on other aberrations, is 772mm
(28mm closer than the original camera), but the other aberrations induced by
the flattener remain. Spherical aberration induced by the 3mm thick
flattener lens is at 0.21 wave PV nearnegligible, less so the unbalanced chromatic defocus
(the two combined resulting in 1.6, 0.2 and 0.36 wave PV in the h,
e and r line on axis, respectively vs. 0.56, 0.03 and 0.22
wave PV in the camera w/o corrector) due to
the shift of the common crossing away from the best focus location
(0.707 zone), worsened by the lateral color
error. The latter is reduced if instead of the standard planoconvex (PCX) lens with
the flat side toward the focus a lens with the curved rear surface is
used. As the lens shape goes through the standard PCX, equiconvex (ECX), PCX facing
the focus with its curved side (middle right), and a meniscus also
facing the focus with its convex side, lateral color diminishes, to be
cancelled with a particular meniscus shape (bottom left). The asterisk is for corrector separation change needed to cancel coma. Corrector radius changes significantly with both, meniscus and PCX+PPP flatteners, which means that it shape also changes significantly. Since the radius is inversely proportional to the defocus parameter Λ, and for the standalone camera Λ=1 (0.707 neutral zone), the integrated meniscus flattener has Λ~2.1, i.e. Schmidt profile shape which would without flattener have brought all the wavelengths to a common focus slightly inside (toward mirror) marginal focus (convex profile with the neutral zone at 1.025, or slightly out of the effective surface). And the profile with the PCX+PPP flattener has Λ~0.386, i.e. neutral zone at 0.44 radius, with the profile edge higher than its inner portion. Both profiles are harder to fabricate than the standard 0.707 neutral zone. Reducing lenstoimage separation would proportionally reduce the cone width at the lens, i.e. the effective aperture at the lens surfaces, and with it the level of aberrations. However, since the only significant aberration at the 2mm separation is coma, which can be cancelled by moving Schmidt corrector slightly closer, further reducing the lenstoimage separation would not produce practical benefits. For the same reason  i.e. due to the smaller effective (cone) aperture at the lens  aberrations induced by the singlelens fieldflattener will be much smaller in slow systems for any given lenstoimage separation: in proportion to the fourth power, third power and square of the inverse Fnumber for spherical aberration, coma and astigmatism, respectively. For that reason, monochromatic aberrations of a singlelens flattener are not the limiting factor to widening the lenstoimage separation in a system like Cassegrain. The limiting factors are lateral color, increasing approximately with the lenstoimage separation, and the magnification factor, since the flattener has negative power. Doublets field flatteners Twolens subaperture corrector can flatten field in the Cassegrain or, in general, any of other popular two mirror systems. A longfocus Cassegrain gains less from field flattening than, for instance RitcheyChretien or DallKirkham, both having stronger offaxis aberrations, which are also greatly reduced with adequately designed flattener. Similarly, flattening field in the SCT with spherical mirrors would produce little benefit if not correcting for the system coma as well.
Example 2: SCT with spherical mirrors  A
near zeropower pair of BK7 lenses for flattening the field of the
commercial 9inch /2/10 SCT. Coma is removed
by the rear surface of the front lens, and the rear lens mainly produces
net astigmatism that flattens the field. For the nearcomplete
correction, a pair of lenses has to be an integral part of the system,
i.e. Schmidt corrector adjustment is required. This flattener  somewhat
tweaked version of the flattener/corrector for a /2.8/10 SCT by Richard
Snashall  leaves a trace of residual coma, and induces near 1/4 wave
(0.24) PV of undercorrection. Either can be cancelled at the expense of
the other becoming somewhat greater (for instance, zero coma would
result in about 0.3 wave PV of spherical aberration, and for negligible
spherical  about 1/6 wave PV or less  the RMS error would only
slightly increase, but would have noticeably more of comalike
deformation toward the edge). A pair of simple plano CX/CV lenses can eliminate curvature of field in a Cassegrain without inducing significant chromatism, spherical aberration or coma. If the positive element is made of common crown, and the negative of common flint, the flattener also somewhat reduces the focal length, generally desirable with longfocus Cassegrains.
Example 3: Simple field flattener for a Cassegrain. 300mm
/4/14 Classical Cassegrain with a flattener
that improves its performance over wide field (there is no noticeable
change in the blur size if the spectral range is widened). The flattener
induces astigmatism which flattens the field. It also reduces the focal
length by 78%. This particular flattener only illustrates the effect;
somewhat better correction could be possible if optimized for the
location, spacing and shape. But any further
improvement wouldn't be significant in practical terms, since the
dominant residual aberration is the fieldflattening astigmatism. Similar form of a field flattener can be used for refractors. Since most of them are fairly similar in their field curvature properties, the parameters of such flattener can be defined, at least in general terms, in terms of the refractor's focal length. A pair of plano CX/CV lenses of the common crown and flint (respectively) will induce fieldflattening astigmatism and low residual aberrations if the crown lens has focal length of nearly 1/3 of the focal length of the refractor  which sets its radius at ~/3(n1)  with the flint lens radius twice larger, and the two placed in near contact at about 0.1 in front of the original focus. The astigmatism is nearly halved in magnitude, but becomes different in sign to somewhat stronger Petzval, with the net effect being nearflat field with roughly half the astigmatism of the objective lens alone. Typically such flattener will reduce off axis error by a factor of 3. While it does flatten image field in both, achromats and apochromats, it is less beneficial in achromats, due to their large longitudinal chromatic defocus, as plots below illustrate. While the error is significantly reduced in the green, farther offaxis chromatic error with the flattener is larger than without it, because field curvature in part compensates for the chromatic defocus. With the red/green/blue blur being similar in size at 1° off axis, here would be little change in imaging, but visual field definition would be noticeably improved, since eye sensitivity is much higher for the green.
Example 4: Simple flattener for refractors 
At left, farther off axis the green (e) blur in the achromat is
noticeably smaller with flattener, but the red/blue (C/F) blur is
actually larger, due to the curvature actually bringing C/F closer to
focus. With CCD chip nearly as sensitive in the red/blue as in the
green, there is little to gain in imaging. On the other hand, the gain
is evident with apo refractors (note that the flattener reduces focal
length by 1015%). With such a generic prescription, best location for the flattener varies from one system to another, but it should be within 1020mm. At the optimum location, coma is near zero, and the median astigmatic surface is nearly flat (the error is actually slightly smaller with a very mild residual curvature, than with flat median surface, which requires more of astigmatism). Moving corrector away from the optimum location worsens the curvature/astigmatism error, and also induces coma (small changes in the lens spacing have little effect, the two lenses can be in full contact). Again, optimization would probably somewhat improve the best flattener's performance, put not significantly in practical terms, since the dominant aberration is the astigmatism flattening the field.
Example 5: Eyepiece flattener  Finally, for visuall use it is possible to flatten field of the objective with a zeropower singlet lens pair inserted into eyepiece barrel. Being very close to the image, the only significant aberration of such corrector is astigmatism, which can flatten the final visual field. Shown is such corrector that flattens field of a 150mm f/5 achromat, by inducing astigmatism of opposite sign to that of achromat's Petzval curvature. Final result is flat visual field and more than twice lower astigmatism. ◄ 10.1.2. Subaperture corrector examples (1) ▐ 10.1.2. Subaperture correctors for twomirror systems ►
