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Normal-incidence soft X-ray telescopesPhotos obtained during 5 min of observation time from the flight of a 25-cm-diameter normal-incidence soft-X-ray (63.5 A) telescope on September 11, 1989, are analyzed, and the data are compared to the results expected from tests of the mirror surfaces. These tests cover a range of spatial periods from 25 cm to 1 A. The photos demonstrate a resolution close to the photon shot-noise limit and a reduction in the scattering of the multilayer mirror compared to a single surface for scattering angles above 1 arcmin, corrresponding to surface irregularities with spatial periods below 10 microns. These results are used to predict the possible performance of future telescopes. Sounding rocket observations might be able to reach a resolution around 0.1 arcsec.
Document ID
19910064265
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Spiller, Eberhard
(IBM Watson Research Center Yorktown Heights, NY, United States)
Mccorkle, R. A.
(IBM Watson Research Center Yorktown Heights, NY, United States)
Wilczynski, J. S.
(IBM Thomas J. Watson Research Center Yorktown Heights, NY, United States)
Golub, Leon
(IBM Watson Research Center Yorktown Heights, NY, United States)
Nystrom, G.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Takacs, P. Z.
(Brookhaven National Laboratory Upton, NY, United States)
Welch, C.
(Lockheed Missiles and Space Co., Inc. Las Cruces, NM, United States)
Date Acquired
August 14, 2013
Publication Date
August 1, 1991
Publication Information
Publication: Optical Engineering
Volume: 30
ISSN: 0091-3286
Subject Category
Astronomy
Accession Number
91A48888
Funding Number(s)
CONTRACT_GRANT: DE-AC02-76CH-00016
CONTRACT_GRANT: NAG5-626
Distribution Limits
Public
Copyright
Other

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