Wang, J. and Nittler, L. R. and Burnett, D. S. (2007) Nanosims measurements of solar wind Mg, Fe, and Cr fluences. Meteoritics and Planetary Science, 42 (S8). A160. ISSN 1086-9379. doi:10.1111/j.1945-5100.2007.tb00601.x. https://resolver.caltech.edu/CaltechAUTHORS:20130131-094242068
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Abstract
The chemical composition of the Sun provides the reference standard for a wide variety of astronomical, cosmochemical, and geochemical studies. To better determine the solar composition, the Genesis spacecraft collected solar wind at the L1 point in the space for 27 months prior to returning samples to Earth in September 2004. Prior ion probe analyses of Genesis samples have found discrepant results for the Mg and Fe solar wind fluences from different collector materials [1]. We report measurements of Mg, Fe, and Cr depth profiles in Genesis diamond-like C sample 60062 using the Carnegie Institution Cameca NanoSIMS 50L ion microprobe. Our results for Mg and Fe are similar to previous analyses of the same sample using different instruments.
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| Additional Information: | © 2007 The Meteoritical Society. Article first published online: 26 Jan. 2010. This work is supported by NASA grant NNX07AG19G. | |||||||||
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| Issue or Number: | S8 | |||||||||
| DOI: | 10.1111/j.1945-5100.2007.tb00601.x | |||||||||
| Record Number: | CaltechAUTHORS:20130131-094242068 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20130131-094242068 | |||||||||
| Official Citation: | (2007), Abstracts. Meteoritics & Planetary Science, 42: A11–A171. doi: 10.1111/j.1945-5100.2007.tb00601.x | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 36704 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 31 Jan 2013 19:29 | |||||||||
| Last Modified: | 09 Nov 2021 23:24 |
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