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Image analysis of the AXAF VETA-1 X-ray mirrorInitial core scan data of the VETA-1 X-ray mirror proved disappointing, showing considerable unpredicted image structure and poor measured FWHM. 2-D core scans were performed, providing important insight into the nature of the distortion. Image deconvolutions using a raytraced model PSF was performed successfully to reinforce our conclusion regarding the origin of the astigmatism. A mechanical correction was made to the optical structure, and the minor was tested successfully (FWHM 0.22 arcsec) as a result.
Document ID
19930055616
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Freeman, M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Hughes, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Van Speybroeck, L.
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Bilbro, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Weisskopf, M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: In: Multilayer and grazing incidence X-ray(EUV optics for astronomy and projection lithography; Proceedings of the Meeting, San Diego, CA, July 19-22, 1992 (A93-39601 15-74)
Publisher: Society of Photo-Optical Instrumentation Engineers
Subject Category
Optics
Accession Number
93A39613
Distribution Limits
Public
Copyright
Other

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