Oxygen 16 to oxygen 18 abundance ratio in the solar wind observed by Wind/MASS

Details Oxygen 16 to oxygen 18 abundance ratio in the solar wind observed by Wind/MASS Oxygen 16 to oxygen 18 abundance ratio in the solar wind observed by Wind/MASS

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jgr...103....7c&link_type=abstract

Journal of Geophysical Research, vol. 10, p. 7

Computer Science

Sound

21

Solar Wind Velocity, Oxygen 18, Satellite Sounding, Gas Density, Photosphere, Solar Flux, Distribution Functions, Abundance, Energetic Particles

Scientific paper

Measurements of the O-16 and O-18 distribution functions in the solar wind at low to average solar wind speeds from the MASS instrument on the Wind spacecraft are reported. The O-16/O-18 density ratio is 450 +/- 130, a value consistent with terrestrial, solar photospheric, solar energetic particle, and galactic cosmic ray O-16/O-18 isotopic ratios. This study constitutes the first reported spacecraft measurement of the isotope O-18 in the core solar wind and may represent the best determination of the solar O-16/O-18 density ratio to date.

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