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Solar abundance determination from ultraviolet emission lines.Relative solar abundance for O, Si and Fe determined from intensities of far UV emission lines of solar corona
Document ID
19670046496
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00150858
Authors
Dupree, A. K.
Goldberg, L.
Date Acquired
August 3, 2013
Publication Date
March 1, 1967
Publication Information
Publication: SOLAR PHYSICS
Subject Category
Space Sciences
Accession Number
67A25225
Funding Number(s)
CONTRACT_GRANT: NSG-438
Distribution Limits
Public
Copyright
Other
Keywords
SPECTRAL LINE
CORONA
EMISSION SPECTRUM
ELEMENT ABUNDANCE
SOLAR RADIATION
ULTRAVIOLET RADIATION

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