Determination of solar wind elemental abundances from M/Q observations during three periods in 1980

Details Determination of solar wind elemental abundances from M/Q observations during three periods in 1980 Determination of solar wind elemental abundances from M/Q observations during three periods in 1980

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...88..359k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 88, Oct. 1983, p. 359-376. Research supported by the Swiss National Science Foundation.

Physics

17

Abundance, Plasma Composition, Solar Wind, Helium Ions, International Sun Earth Explorer 3, Ion Temperature, Mass Spectra, Oxygen Ions, Positive Ions

Scientific paper

Mass spectra in the range 2 ≤ M/Q ≤ 3 provided by a high resolution mode of the ISEE-3 Plasma Composition Experiment were evaluated for three selected periods during early 1980. The observed Ne/O ratios are compatible with estimated solar abundance ratios. In two of the three periods, the He/Ne-ratios agree with the Apollo foil results. Freezing-in temperatures for oxygen are similar to those obtained by other groups. Possible reasons for an unexpectedly high flux at M/Q = 2.4 are discussed.

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