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Solar X-ray spectroscopy with spatial resolutionPreliminary results from a solar X-ray spectroscopic experiment are presented. The data emphasize the nonhomogeneous and multithermal nature of the corona. The oxygen-to-neon abundance ratio in the corona is found to be about 4.7, as derived from the O VIII-to-Ne IX resonance-line photon flux ratio.
Document ID
19750051496
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Acton, L. W.
Catura, R. C.
Joki, E. G.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Subject Category
Solar Physics
Meeting Information
Meeting: International Conference on X-Rays in Space - Cosmic, Solar, and Auroral X-Rays, Calgary
Location: Alberta
Country: Canada
Start Date: August 14, 1974
End Date: August 21, 1974
Accession Number
75A35568
Funding Number(s)
CONTRACT_GRANT: NAS2-6723
Distribution Limits
Public
Copyright
Other

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