Published October 15, 1997 | Version Published
Book Section - Chapter Open

Investigation of substrates and mounting techniques for the High Energy Focusing Telescope (HEFT)

Abstract

The high energy focusing telescope (HEFT) is a balloon-borne system for obtaining arcminute imagery in the 20 - 100 keV energy band. The hard x-ray optics are baselined to use thin epoxy-replicated aluminum foil substrates coated with graded-d multilayers, and we show some results on x-ray performance of prototype foil substrates. We also propose an extremely promising alternative substrate -- thermally formed glass. The advantages of thermally formed glass substrates, their fabrication and preliminary metrology on sample pieces are discussed. If ultimately feasible, the thermally formed glass is a better substrate due to its superior hard x-ray reflectivity and scattering properties in comparison to similarly coated epoxy-replicated aluminum foil. We also discuss some preliminary work on the HEFT mirror mounting concept and the associated angular resolution error budget.

Additional Information

© 1997 Society of Photo-Optical Instrumentation Engineers (SPIE). This work is Columbia Astrophysics Laboratory contribution number 642.

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Eprint ID
88385
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CaltechAUTHORS:20180731-114053130

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2018-07-31
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2021-11-16
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Space Radiation Laboratory
Series Name
Proceedings of SPIE
Series Volume or Issue Number
3114