Suprathermal ions of solar and interstellar origin associated with the April 9-12, 2001, CMEs

Details Suprathermal ions of solar and interstellar origin associated with the April 9-12, 2001, CMEs Suprathermal ions of solar and interstellar origin associated with the April 9-12, 2001, CMEs

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004adspr..34..161b&link_type=abstract

Advances in Space Research, Volume 34, Issue 1, p. 161-165.

Physics

Suprathermal Ions, Solar Origin, Interstellar Origin, April 9-12, 2001 Cmes, Plasma Properties

Scientific paper

The distribution functions of suprathermal ions associated with the two interplanetary coronal mass ejections in the time period of April 9-12, 2001, are analyzed. The data on ions in the energy range 35-2000 keV/amu were recorded by the (Highly) Suprathermal Time-of-Flight (HSTOF/STOF) Spectrometer on board the Solar and Heliospheric Observatory (SOHO) at 1 AU. While the instrument passes the event the ion spectra undergo changes that correpond to the local plasma properties. In particular, there are significant differences between the spectra and the spatial distribution of singly charged interstellar 4He+ pick-up ions and of solar wind 4He2+ ions, respectively.

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