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Published August 2007 | Published
Journal Article Open

Solar wind argon from Genesis alos regime collectors

Mabry, J. C.
Meshik, A. P.
Hohenberg, C. M.
Marrocchi, Y.
Pravdivtseva, O. V. ORCID icon
Allton, J.
McNamara, K.
Stansbery, E.
Burnett, D. S. ORCID icon
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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.

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