Solar wind heavy ion abundances

Details Solar wind heavy ion abundances Solar wind heavy ion abundances

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...43..463b&link_type=abstract

Solar Physics, vol. 43, Aug. 1975, p. 463-473. DOD-ERDA-sponsored research.

Physics

39

Abundance, Heavy Ions, Solar Atmosphere, Solar Corona, Solar Wind, Chemical Composition, Interplanetary Medium, Iron, Oxygen, Photosphere, Silicon, Stellar Evolution

Scientific paper

During periods in 1969-1971 when interplanetary flow conditions were quiet, 17 determinations of the solar wind Fe and Si abundances and 7 of the O abundance were made. On the average N(Fe)/N(H) = .000053, N(Si)/N(H) = .000076 and N(O)/N(H) = .00052. Variations from the averages over a total range of factors of about 4 for O, about 4 for Si, and about 10 for Fe have been observed. Although Fe and Si abundance variations appear to be correlated, no other element correlation pairs are unambiguously discernible from the present data set.

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