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ATM observations - X-ray resultsPreliminary results of the solar X-ray observations from Skylab are reviewed which indicate a highly structured nature for the corona, with closed magnetic-loop structures over a wide range of size scales. A description of the S-054 experiments is provided, and values are given for the parameters - including size, density, and temperature - describing a variety of typical coronal features. The structure and evolution of active regions, coronal holes, and bright points are discussed.
Document ID
19760038766
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Vaiana, G. S.
(American Science and Engineering, Inc. Cambridge, MA, United States)
Zombeck, M.
(Harvard College Observatory Cambridge, Mass., United States)
Krieger, A. S.
(American Science and Engineering, Inc. Cambridge, Mass., United States)
Timothy, A. F.
(NASA Headquarters Washington, DC United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1976
Publication Information
Publication: Astrophysics and Space Science
Volume: 39
Subject Category
Solar Physics
Accession Number
76A21732
Distribution Limits
Public
Copyright
Other

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