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High-resolution studies of the structure of the solar atmosphere using a new imaging algorithmThe results of the application of a new image restoration algorithm developed by Ayers and Dainty (1988) to the multiwavelength EUV/Skylab observations of the solar atmosphere are presented. The application of the algorithm makes it possible to reach a resolution better than 5 arcsec, and thus study the structure of the quiet sun on that spatial scale. The results show evidence for discrete looplike structures in the network boundary, 5-10 arcsec in size, at temperatures of 100,000 K.
Document ID
19910048315
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Karovska, Margarita
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Habbal, Shadia Rifai
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 14, 2013
Publication Date
April 10, 1991
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 371
ISSN: 0004-637X
Subject Category
Solar Physics
Funding Number(s)
CONTRACT_GRANT: NAGW-249
Distribution Limits
Public
Copyright
Other
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