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Published July 1993 | Version public
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New SEP-Based Solar Abundances

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Abstract

The relative abundances of various elements in the solar photosphere and the solar corona are re-determined from relative abundances of solar energetic particles (SEP) in the light of revised solar spectroscopic abundances. We find excellent correlation between SEP-based abundances and spectroscopic abundances, after correcting for fractionation due to ionic charge-to-mass ratio and first ionization potential.

Additional Information

© 1993 University of Calgary. This work has been partially supported by NASA under NAS7-918. We acknowledge excellent assistance from M. Looper in data analysis and presentation.

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Eprint ID
43793
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CaltechAUTHORS:20140212-100928259

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http://adsabs.harvard.edu/abs/1993ICRC....3..384G (URL)

Funding

NASA
NAS7-918

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Created
2014-02-24
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Updated
2020-02-20
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Space Radiation Laboratory