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Light noble gas composition of different solar wind regimes: results from genesis

Heber, V. S. and Baur, H. and Burnett, D. S. and Reisenfeld, D. B. and Wieler, R. and Wiens, R. C. (2007) Light noble gas composition of different solar wind regimes: results from genesis. Meteoritics and Planetary Science, 42 (S8). A63-A63. ISSN 1086-9379. https://resolver.caltech.edu/CaltechAUTHORS:20130130-151230007

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Abstract

The Genesis mission provided samples of solar wind (SW) from different regions on the Sun. These SW regime samples are important in understanding fractionation processes upon formation and acceleration of the SW to ultimately deduce solar composition from SW values. We present He and Ne isotopic and elemental compositions of the bulk SW (SW of entire collection period) and the 3 major SW regimes: slow (from the ecliptic plane, emanating from above streamers), fast (emanating from coronal holes), and coronal mass ejections (CME). At the conference we will also present Ar data.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/ 10.1111/j.1945-5100.2007.tb00601.xDOIUNSPECIFIED
http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.2007.tb00601.x/abstractPublisherUNSPECIFIED
ORCID:
AuthorORCID
Burnett, D. S.0000-0001-9521-8675
Reisenfeld, D. B.0000-0003-1874-9450
Wieler, R.0000-0001-5666-7494
Wiens, R. C.0000-0002-3409-7344
Additional Information:© 2007 The Meteoritical Society. Article first published online: 26 Jan. 2010.
Issue or Number:S8
Record Number:CaltechAUTHORS:20130130-151230007
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130130-151230007
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:36697
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:31 Jan 2013 19:39
Last Modified:09 Mar 2020 13:19

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