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• W1661322684 abstract "The Sun is the largest reservoir of matter in the solar system, which formed 4.6 Gy ago from the protosolar nebula. The solar wind carries a nearly unfractionated sample of heavy isotopes at energies of about 1 keV/amu from the Sun into interplanetary space. Data from space missions and theoretical models indicate that the isotopes of the volatile elements N, O, Ne, and Ar are fractionated by at most a few percent per atomic mass unit in different solar wind regimes. In contrast, isotopic abundances of solar and heliospheric energetic particles at energies larger than about 100 keV/amu are observed to strongly vary relative to solar abundances. Processes such as resonant acceleration or pre-acceleration by plasma waves, first-order Fermi acceleration, or propagation in the interplanetary plasma are discussed as causes for charge-to-mass dependent fractionation." @default.
• W1661322684 created "2016-06-24" @default.
• W1661322684 creator A5079441788 @default.
• W1661322684 date "2003-01-01" @default.
• W1661322684 modified "2023-09-26" @default.
• W1661322684 title "Isotopic Fractionation by Plasma Processes" @default.
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• W1661322684 doi "https://doi.org/10.1007/978-94-010-0145-8_20" @default.
• W1661322684 hasPublicationYear "2003" @default.
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