on-orbit adjustment calculation for the generation-x x-ray mirror figure d. a. schwartz, r. j....

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On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P. B. Reid, S. J. Wolk, (Harvard- Smithsonian Center for Astrophysics), S. L. O’Dell, J. K. Kolodziejczak (NASA/MSFC), W. W. Zhang (NASA/GSFC), for the Gen-X Team SPIE Conference 7011 Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray 2008 24 June 2008

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Page 1: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

On-Orbit Adjustment Calculation for the Generation-X X-ray mirror

Figure

D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P. B. Reid, S. J. Wolk, (Harvard-Smithsonian Center for Astrophysics), S. L.

O’Dell, J. K. Kolodziejczak (NASA/MSFC), W. W. Zhang (NASA/GSFC), for the Gen-X Team

SPIE Conference 7011Space Telescopes and Instrumentation II: Ultraviolet to

Gamma Ray 200824 June 2008

Page 2: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Generation-X Science Objectives

• Detection of first black holes at z~10-20

• Evolution of Black Holes, Galaxies, Elements, from formation to the present

• Behavior of matter in extreme environments of Density, Gravity, Magnetic fields, Kinetic Energy.

Page 3: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Key Mission Requirements:

• Large Area, ~50 m2 at 1 keV• Fine angular resolution, 0."1

Page 4: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

High Resolution Imaging enables Gen-X science objectives

Page 5: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Wolter I Grazing Incidence X-ray reflection

Page 6: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

A Gen-X Mirror Configuration

• 204 shells, 0.2mm thick • 16m outer diameter, (partially filled)• 8.3m completely filled, 3.5m inner

diameter• 60m focal length• 1m Shell length (each, P or H), 50mm gap• 5' radius FOV• 10mm shell clearance

Page 7: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Gen-X enabled by Ares V

Page 8: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Adjust figure via strain parallel to reflecting surface.

Page 9: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Ring Images (Chandra at MSFC cal facility)

Page 10: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Profile across ring diagnosis axial quality

Page 11: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Raytrace Study Objectives:

1. Detector requirements1. Placement

2. Resolution

2. Can we detect deviations from ideal figure?

3. Are the measurements practical?

Page 12: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Raytrace Study

• Shells 1, 2, 203, 204• Uniform incident rays, perfect reflection• Perfect Wolter I Geometry• Perfect kinematic mounting, alignment• Trace single axial strip• Perturb surface figure by low order

Legendre Polynomials• Introduce "toy" actuators

Page 13: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Measure ~50,000 axial positions (1cm2), ~1000 at once. 500s exposure to Sco X-1 at 2 104 s-1 gives 104 counts per azimuth per ring. Iterate 10

times at 50% duty cycle, factor 10 margin, 120day initial adjustment

Resolve 100 bins with detector resolution 10µ. Require 8.17m

forward of focus.

Page 14: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Spacing of the figure detector to resolve 40 shells into 100 bins

Page 15: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Ring profile for Pn distortions proportional to 0.0001/n mm.Image size in focal plane is 0."21 rms and 0."11 half-power

Ring Profile can Diagnose Figure Errors!

Page 16: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Tilt of P to H by 1µ displaces ring by ~200 µ

Page 17: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Poorer quality figure spreads the ring further

19" rms10" rms

4.8" rms 2.2" rms

Page 18: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Requirements on Figuring Detector

• X-ray range ~0.2 – 4 keV• Count 2x104 s-1 per field• Resolve events to 10µm• 100mm x 100mm field• Position ~1 to 10 m forward of focus

– accuracy ~1cm axial, 1mm radial• Radial positioning knowledge better than

10 µ

Page 19: On-Orbit Adjustment Calculation for the Generation-X X-ray mirror Figure D. A. Schwartz, R. J. Brissenden, M. Elvis, G. Fabbiano, D. Jerius, M. Juda, P

Conclusions (so far)

• Ring Profile, Position and Spread are extremely sensitive to figure quality

• On-orbit Measurements are practical• Concept would "forward-fit" a distorted raytrace

model shell to the ring profile measurement• Actuator design is critical for

– Sufficient correction amplitude– Avoiding transfer of low spatial frequency

figure errors to higher frequencies