Abundance ratios of He-4/2+//He-3/2+/ in the solar wind

Details Abundance ratios of He-4/2+//He-3/2+/ in the solar wind Abundance ratios of He-4/2+//He-3/2+/ in the solar wind

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85.6021o&link_type=abstract

Journal of Geophysical Research, vol. 85, Nov. 1, 1980, p. 6021-6024. Research supported by the Swiss National Science Foundati

Physics

9

Abundance, Helium Ions, Helium Isotopes, Satellite Observation, Solar Wind, International Sun Earth Explorer 3, Mass Spectrometers, Solar Corona, Solar Wind Velocity

Scientific paper

The ion composition experiment aboard the Isee 3 spacecraft has been used to measure the He-4(2+)/He-3(2+) ratio in the solar wind. Using 4334 observations made between Aug. 18 and Nov. 24, 1978, and March 24 and Aug. 25, 1979, the average ratio He-4(2+)/He-3(2+) was 2.1 + or - 0.2 x 1000, in agreement with previous foil measurements. Individual observations vary widely from the average and the low He-4(2+)/He-3(2+) ratios occur at times of low He-4(2+) flux.

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