Published August 2007
| Published
Journal Article
Open
Solar wind argon from Genesis alos regime collectors
Abstract
Determining solar noble gas isotopic ratios are one piece of the puzzle needed to constrain models of the evolution of terrestrial planets, as well as to understand solar composition and processes. Solar wind (SW) remains the best available source of solar material, even though there is potential for fractionation between true solar values and the solar wind. Here we will focus on SW argon.
Additional Information
© 2007 The Meteoritical Society. Article first published online: 26 Jan. 2010. Supported by NASA grants NNJO4HI17G and NAG5-12885.Attached Files
Published - Burnett_2007pA95.pdf
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Additional details
- Eprint ID
- 36699
- DOI
- 10.1111/j.1945-5100.2007.tb00601.x
- Resolver ID
- CaltechAUTHORS:20130130-152240689
- NNJO4HI17G
- NASA
- NAG5-12885
- NASA
- Created
-
2013-01-31Created from EPrint's datestamp field
- Updated
-
2023-10-23Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences