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Coated Mandrel

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Hard X-ray Astronomy (20- 100 keV) is rich but: ... etc. : Al Krieger, Dan Parsignault, Derrick Mancini, Matt Steele, Peter Takcas, ... – PowerPoint PPT presentation

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Title: Coated Mandrel


1
Prof. Mel Ulmer DEPT OF PHYSICS
ASTRONOMY
2
The Concept
Intact Electroforming Multilayer Process
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Coated Mandrel
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Astrophysical Motivation
  • Hard X-ray Astronomy (20- 100 keV) is rich but
  • Need focusing for improved sensitivity and
    imaging
  • Flexible design of focal length
  • Need the best angular resolution possible

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resolution 1.5 2.25
3. arc min
45 arc sec
resolution 15
22.5 arc sec
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Gal. Cen.
Cas A
8.5 x 8.5 arc min
1.3 x 1.3 arc min
3C 273
Per A
24 x 24 arc sec
3.5 x 3.5 arc min
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Advantages of IEMP
  • Coat Mandrel gt Focal Length, small
    as 1-2 meters gt
    SMEX is possible
  • Electroforming offers the best angular
    resolution (lt 10 arc sec) outside custom figuring
  • An additional advantage of proccess at NU
  • CNx coating (10 nm) smooths protects

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Now the entire process
Coat mandrel with CNx
Coat mandrel with release layer
Coat with multilayers
Coat with adhesion layers
Electroform
Remove electroform
Remove release layer
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Therefore, Total Institutional Integration
is
VERY IMPORTANT
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Two different orientations about optical axis,
same energy
About 90 deg rotation
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Higher Energy
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Conclusion Excellent Multilayers because
  • Same Bragg angles at different energies, more
    penetrating versus less
  • Narrow Bragg peaks
  • One multilayer d-spacing 5.29 nm fits all
  • Same Bragg angles at different axis rotations
  • All the above plus fits indicate well over 10
    efficiency. How high? Perhaps near theoretical
    80

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30 cm long, 12 cm dia. 2 m focal length Wolter
I With multilayers
First Light
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Where do we go from here?
  • Further analysis of in hand mirror to cement
    reflectivity efficiency estimates
  • Advance to an even better truncated cone mandrel
  • Move to graded d-spacing with new multilayer
    coating chamber
  • Advance to Wolter I mirrors and fly them!!

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Co-Authors Bob I. Altkorn, Anita Madan, Mike
Graham, and Yong S. Chu
Helpers, collaborators, etc. Al Krieger, Dan
Parsignault, Derrick Mancini, Matt Steele, Peter
Takcas, Yip-Wah Chung, Jane Chang
NASA Support SRT and Con X
www.astro.nwu.edu/astro/faculty/ulmer
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We are ready to go! Just send money!!
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The
End
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