Published August 2006
| Published
Journal Article
Open
The solar wind FE/MG ratio
Chicago
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Abstract
To meet the Genesis mission goal for improved solar elemental abundances, we need to address the issue of fractionation of the abundances of elements in the solar wind compared to the solar photosphere. There is a well-established depletion of elements in the solar wind with high first ionization potential (FIP > 9eV) compared to lower FIP elements, but there is no evidence for fractionation between lower FIP elements.
Additional Information
© 2006 The Meteoritical Society.Attached Files
Published - Burnett_2006pA33.pdf
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Additional details
- Eprint ID
- 36712
- Resolver ID
- CaltechAUTHORS:20130131-131759052
- Created
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2013-02-27Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)