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Theoretical intensity ratios for some Fe XIII coronal lines.Using cross section values for collisional excitation by protons recently calculated by Landman (1973), theoretical values for the relative intensities of the Fe XIII 10747-, 10798-, and 3388-A lines are determined as functions of electron density. The obtained results are compared with those of Chevalier and Lambert (1969).
Document ID
19730059833
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00152669
Authors
Finn, G. D.
Landman, D. A. (Hawaii, University Honolulu, Hawaii, United States)
Date Acquired
August 7, 2013
Publication Date
June 1, 1973
Publication Information
Publication: Solar Physics
Volume: 30
Subject Category
Space Sciences
Accession Number
73A44635
Funding Number(s)
CONTRACT_GRANT: NSF GP-31750
CONTRACT_GRANT: NAS8-27950
Distribution Limits
Public
Copyright
Other

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