Published July 1993
| public
Book Section - Chapter
New SEP-Based Solar Abundances
- Creators
- Garrard, T. L.
-
Stone, E. C.
- Others:
- Leahy, D. A.
- Hickws, R. B.
- Venkatesan, D.
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.Additional details
- Eprint ID
- 43793
- Resolver ID
- CaltechAUTHORS:20140212-100928259
- NASA
- NAS7-918
- Created
-
2014-02-24Created from EPrint's datestamp field
- Updated
-
2020-02-20Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory