Solar energetic particle events observed by SOHO/CELIAS/STOF

Details Solar energetic particle events observed by SOHO/CELIAS/STOF Solar energetic particle events observed by SOHO/CELIAS/STOF

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3144h&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

Since the launch of the Solar and Heliosheric Observatory (SOHO) on Dec. 2, 1995, the Suprathermal TimeOf-Flight (STOF) energetic particle sensor of the Charge, Element and Isotope Analysis System (CELIAS) has observed gradual and impulsive solar particle events from solar activity cycle minimum to maximum. The instrument CELIAS/ STOF has the capability of detecting energetic ions between 35 and 630 keV/q and determine the mass, energy and charge of each particle. We report on the measurements of the detected energetic particle events from 1996 to 2000, i.e. the daily averages of the He/Pr, the He charge state and the Fe/O ratios. For selected events we analyse the velocity dispersion of the suprathermal ions and estimate the onset of the solar event and set limits on the propagation length along the connecting magnetic field line.

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