Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows.

Details Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows. Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows.

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13q..75g&link_type=abstract

Advances in Space Research, Vol. 13, No. 6, p. 75 - 78

Computer Science

Scientific paper

For the March/April 1991 time period, the alpha/proton abundance ratio, the proton kinetic temperature and speed distributions, and the relative abundance of O+7 to O+6 is determined over each 13-minute duty cycle of the Solar Wind Ion Composition Spectrometer (SWICS) experiment on Ulysses. The ratio O+7/O+6 (as a relative measure of ionization temperature) is shown to be useful in identifying possible coronal mass ejection (CME) events.

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