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The solar EUV-emitting plasma.The extreme ultraviolet (EUV), covering a decade in wavelength from about 300 A to about 3000 A, is considered. The general characteristics of the quiet solar atmosphere are reviewed, with emphasis on how the observed emission may be used as a tool to infer this structure. Many of the same techniques are applied to the study of overall properties of active regions.
Document ID
19730029150
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Noyes, R. W. (Smithsonian Astrophysical Observatory and Harvard College Observatory Cambridge, Mass., United States)
Withbroe, G. L. (Harvard College Observatory Cambridge, Mass., United States)
Date Acquired
August 7, 2013
Publication Date
November 1, 1972
Subject Category
Space Radiation
Accession Number
73A13952
Funding Number(s)
CONTRACT_GRANT: NAS5-9274
CONTRACT_GRANT: NGR-22-007-211
Distribution Limits
Public
Copyright
Other

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