Can intrasolar diffusion contribute to isotope anomalies in the solar wind?

Details Can intrasolar diffusion contribute to isotope anomalies in the solar wind? Can intrasolar diffusion contribute to isotope anomalies in the solar wind?

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91..473m&link_type=abstract

(Lunar and Planetary Institute, NASA, American Geophysical Union, et al., Lunar and Planetary Science Conference, 16th, Hoston,

Physics

2

Abundance, Chemical Fractionation, Gaseous Diffusion, Isotopes, Rare Gases, Solar Wind, Helium Isotopes, Neon Isotopes, Solar Interior, Stellar Composition, Xenon Isotopes

Scientific paper

The possible role of intrasolar diffusion is examined for the isotopes of He, Ne, and Xe to see if there is a theoretical basis for an empirical mass fractionation relationship between the isotopic compositions of planetary and solar-wind-implanted elements. It is shown that if diffusion is responsible, even in part, for the observed depletion of 4He in the solar wind, then significant fractionation effects across the isotopes of Ne and Xe as well as He can be predicted. It is also shown that isotopic fractionation need not necessarily infer extreme elemental abundance patterns in the solar interior.

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