The relative abundance of 3He(++) in the solar wind

Details The relative abundance of 3He(++) in the solar wind The relative abundance of 3He(++) in the solar wind

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.591c&link_type=abstract

In JPL Solar Wind Five p 591-596 (SEE N84-13067 03-92)

Physics

3

Helium Ions, Helium Isotopes, Ion Concentration, Solar Wind, Flux Density, Solar Activity Effects, Solar Flares, Transit Time

Scientific paper

Continuous measurements of solar wind 3He++ and 4He++ from August, 1978 to December, 1981 have been made covering a full range of solar wind conditions. The average flux ratio >R< derived from these data is 2310±50, in excellent agreement with the Apollo foil measurements. A probable correlation between >R< and solar activity has been found; however, an examination of the data during periods of 3He++-rich solar flares shows no detectable increase in 3He++ in the solar wind.

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