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Geometrical theory of aberration for off-axis reflecting telescope and its applications. Seunghyuk Chang 2013.02.14. SSG13. On-Axis vs Off-Axis. On-Axis. Off-Axis. Secondary mirror blocks incoming rays. No obstruction. Clear aperture. On-Going Off-Axis Telescope Project. - PowerPoint PPT Presentation
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Geometrical theory of aberration for off-axis reflecting telescope
and its applications
Seunghyuk Chang
2013.02.14.
SSG13
On-Axis vs Off-Axis
On-Axis Off-Axis
Secondary mirror blocks incoming rays.
No obstruction.Clear aperture.
On-Going Off-Axis Telescope ProjectAdvanced Technology Solar Telescope (ATST)
4-m aperture, largest solar telescope, off-axis Gregorian design
On-Going Off-Axis Telescope Project
Wide Field Infrared Survey Telescope (WFIRST)
• Top-ranked large space mission in the New Worlds, New Horizon Decadal Survey of Astronomy and Astrophysics• Sky surveys, Exoplanet – Microlensing, Dark Energy• 1.3m aperture off-axis Three Mirror Anastigmat (TMA) design
Basic Off-Axis Telescope
Eccentric section of an on-axis parent system
Confocal Plane-Symmetric Off-Axis Two-Mirror System
The mirrors of a confocal system do not need to have a common axis for a perfect image at the system focus
Vertex Equation for Off-Axis Portion of Conic Sections of Revolution
2 22 (1 ) 0Rz K z
2 20
0 20
2 2 20
(1 cos )
2sin 2 )
1 sin
(1 sin ) 0
K z
RxK z
K
K x y
• A localized coordinate system is convenient to describe a mirror near a point (x0’, z0’)
• Vertex equation of conic sections of revolution :
Expansion of Vertex Equation
2 2 3 21 2 3 4 (4)z a x a y a x a xy O
32 2
01
(1 sin )
2
Ka
R
12 2
02
(1 sin )
2
Ka
R
2 20 0
3 2
sin 2 (1 sin )
4
K Ka
R
20 0
4 2
sin 2 (1 sin )
4
K Ka
R
Optical Path Length (OPL)
2 2 3 21 1 2 2 (4)OPL s s A x A y A x A xy O
Astigmatism Coma
• To compute the aberrations, the OPL for an arbitrary reflection point on the mirror is necessary
• The OPL is constant in a perfect focusing mirror
• The variance of the OPL
yields aberrations
Astigmatic Images
1 0A
TangentialAstigmatic Image:
32cos1 1
cos( )s
stR ss
1 0A
SagittalAstigmatic Image:
2cos cos( )1 1s s
sR ss
The second order terms yields the two astigmatic image points
2 2 3 21 1 2 2OPL s s A x A y A x A xy
Tilted Astigmatic Image Planes
Tangential AstigmaticImage Plane
22cos1 1(1 tan )s
s
tR ss
Sagittal AstigmaticImage Plane
22cos1 1(1 tan )s
s
sR ss
2sin 2 s
t s
s
Rs s
Linear Astigmatism:
Expanding the two astigmatic image distances to the first order of yields the tangential and sagittal astigmatic image planes and linear astigmatism
IMAGE PLANES OF PARABOLOID
On-Axis Off-Axis
Coma and Third Order Astigmatism
32
20
cos 1 1 1 1sin (cos sin ) coss
s s sAR s s s R
22sin 2 2 1 1s
t st s
s
R R s ss s
• The A2 term yields tangential coma aberration
• Expanding the two astigmatic image points to second order on yields third order astigmatism
2 2 3 21 1 2 2 (4)OPL s s A x A y A x A xy O
Aberrations of Classical Off-axis Two-mirror Telescopes
• Aberrations of classical off-axis two-mirror telescopes can be obtained by cascading the aberrations of each mirror
• Assume the aperture stop is located at the primary mirror
Aperture Stop
When aperture stop is displaced from the mirror surface,the reflection point of the chief ray depends on the field angle.
Aperture Stop
2
0 0 0
1 1 tan s
W W W
s s s
0 0
1 1
2s s
W
s s
• A displaced aperture stop yields a new field angle and a new chief ray incidence angle s for the mirror
Aperture Stop
0
2 2
0 0 0 00
sin 22 1
2 1 1 21 1 cos 2 sin
s
t s
s s
s W
s Rs s
W W WW
R s s s ss
32 2
2 20 0 0
cos 1 1 1 1sin cos 1 cos sins
s s s s
W WA
R s s s s R s
• A displaced aperture stop yields new astigmatism and coma aberration coefficient.
Aberrations of Classical Off-Axis Two-mirror Telescopes
Astigmatism
0
2
0
sin 2 sin 22
1 tan tan
m m s
s m s
m s
s
f R R
W f
Coma
0
cos s s
ATCf x
Rm
Rs
Rm (Rs) is the radius of curvature of the primary (secondary) parent mirror at its vertex.
Linear Astigmatism of a Two-mirror Telescope
2
2
21
1
1
2
2 2sin2sinarctan iR
iRt
Elimination of Linear Astigmatism and Third Order Coma
• Linear astigmatism can be eliminated by enforcing
sin 2 sin 2m sm s
m sR R
• Third order coma is identical to an on-axis paraboloid
202
3
4
xATC
f
Example
• D=1000mm, f=2000mm• Satisfies zero-linear-astigmatism condition
Astigmatism
Spot Diagram Comparison
Example On-Axis Paraboloid
Spot diagrams of the two systems are identical as the presented theory predicted
Example
1m f/8 classical Cassegrain
Off-axis On-axis
Side View
Spot Diagrams
Example
1m f/20 classical Gregorian
Off-axis On-axis
Side View
Spot Diagrams
Example
2.4m f/24 aplanatic Cassegrain
Off-axis On-axis
Side View
Spot Diagrams
Example
10cm f/4 off-axis Schwarzschild flat-field anastigmat
Side View Spot Diagrams
M1
M2
Off-axis Reflector Design forSPICA Channel 1 MIR Camera
22:53:54
SPICA ch1 MIR Dcl:70 centered field Scale: 0.04 11-Jul-08
595.24 MM
Collimator
Camera
• Both the collimator and the camera are off-axis reflecting telescopes with zero linear astigmatism.
13:31:39
SPICA ch4 MIR Dcl:50 offset field Scale: 0.04 20-Jul-08
609.76 MM
Off-axis Reflector Design forSPICA Channel 4 MIR Camera
Collimator
Camera
• Both the collimator and the camera are off-axis reflecting telescopes with zero linear astigmatism.
6.5-m TAO Telescope
• Mid-infrared re-imaging optics of 6.5m-TAO telescope has been developed based on linear-astigmatism theory.
Off-axis Reflector Design forMcDonald 2.1-m Telescope Focal Reducer
• Both the collimator and the camera are off-axis reflecting telescopes with zero linear astigmatism.• Reduce the telescope focal ratio from f/13.6 to f/4.56
Camera
Collimator
Three-Mirror Off-Axis Telescope
3rd order aberration
Two Mirror Three Mirror
Cassegrain Gregorian Couder SchwartzschildThree Mirror Anastismat
(TMA)
Spherical R R R R R
Coma R R R R R
Astigmatism X X R R R
Field Curvature X X X R R
Two Mirror vs. Three Mirror
R: removable, X:not removable
Linear Astigmatism of Confocal Off-Axis N-Mirror System
Image Planes of Kth mirror inConfocal Off-Axis N-Mirror System
KK
KTKK
TK i
Rm 2sintantan 1
KK
KSKK
SK i
Rm 2sintantan 1
K
KKm
KR : Radius of curvature of the parent mirror at its vertex
Image Planes of Confocal Off-AxisN-Mirror System
NN
Np
N
p p
pN
pqq
TN
pp
TN i
Ri
Rmm 2sin2sintantan
1
1 10
1
Tangential image plane:
Sagittal image plane: NN
Np
N
p p
pN
pqq
SN
pp
TN i
Ri
Rmm 2sin2sintantan
1
1 10
1
Elimination of Linear Astigmatism in Confocal Off-axis N-mirror System
SN
TN tantan
STN
ppN
N
Np
N
p p
pN
pqq mi
Ri
Rm 00
1
1
1 1
tantan2
12sin2sin
Two-mirror telescope : 02sin1
2sin 22
2
21
1
1
iRm
iR
Three-mirror telescope : 02sin1
2sin1
2sin 33
3
322
2
2
21
1
1
iRmm
iRm
iR
Advanced Technology Solar Telescope (ATST)
• 4m-aperture off-axis Gregorian design• Off-axis section of an on-axis telescope• Gregorian focus does not satisfy linear-astigmatism-free condition
02sin1
2sin 22
2
21
1
1
iRm
iR
• Linear astigmatism can be eliminated by adding M3
02sin1
2sin1
2sin 33
3
322
2
2
21
1
1
iRmm
iRm
iR
Advanced Technology Solar Telescope (ATST)
ATST ATST + M3
WFIRST 1.3m-Aperture Off-Axis TMA Telescope
WFIRST 1.3m-Aperture Off-Axis TMA Telescope
Linear-astigmatism-free modification
02sin1
2sin1
2sin 33
3
322
2
2
21
1
1
iRmm
iRm
iR
WFIRST 1.3m-Aperture Off-Axis TMA Telescope
NASA DesignLinear-astigmatism-
free Design
Aperture diameter 1.3m
Focal length 20675mm
l1 ~ 3330mm 3330mm
i1 ~ -12 deg. -12 deg.
l2 ~ -800mm -800mm
i2 ~ 12 deg. 12 deg.
m2 ~ -3.25 -3.25
l3 ~ 2700mm 2696mm
i3 ? -7.9427239 deg.
m3 ? 1.910339
Residual RMS wave front error for 0.8 deg x 0.46 deg FOV
12 ~ 18 nm* 0.9 ~ 3.5 nm
* : “Wide Field Infrared Survey Telescope [WFIRST]: telescope design and simulated performance,” Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84421U (September 21, 2012); doi:10.1117/12.927808
References
• S. Chang and A. Prata, Jr., "Geometrical theory of aberrations near the axis in classical off-axis reflecting telescopes," Journal of the Optical Society of America A 22, 2454-2464 (2005)
• S. Chang, J. H. Lee, S. P. Kim, H. Kim, W. J. Kim, I. Song, and Y. Park, "Linear astigmatism of confocal off-axis reflective imaging systems and its elimination," Applied Optics 45, 484-488 (2006)
• S. Chang, " Off-axis reflecting telescope with axially-symmetric optical property and its applications," Proc. SPIE, Vol. 6265, 626548 (2006)
• S. Chang, “Elimination of linear astigmatism in N-confocal off-axis conic mirror imaging system,” in preparation