Towards Understanding Mass-Dependent Fractionation of Solar Wind Isotopic Compositions

Details Towards Understanding Mass-Dependent Fractionation of Solar Wind Isotopic Compositions Towards Understanding Mass-Dependent Fractionation of Solar Wind Isotopic Compositions

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2789h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2789

Computer Science

Scientific paper

The isotopic composition of the solar nebula for most highly-volatile
elements is best deduced from solar wind. We show that isotopic
fractionation of solar wind is basically quantifiable based on oxygen
and noble gas data from Genesis.

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