Low-energy particle events generated by solar disappearing filaments

Details Low-energy particle events generated by solar disappearing filaments Low-energy particle events generated by solar disappearing filaments

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...197..297h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 197, no. 1-2, May 1988, p. 297-305.

Astronomy and Astrophysics

Astrophysics

9

Particle Energy, Solar Prominences, Solar Protons, Solar Terrestrial Interactions, International Sun Earth Explorer 3, Interplanetary Medium, Shock Waves, Solar Flares

Scientific paper

Five large low-energy (E less than 2 MeV) proton events associated with interplanetary shocks, observed at 1 AU by the ISEE-3 probe, appeared to be triggered by solar disappearing filaments instead of solar flare activity. These events will join the other six events of this kind already known. In this paper these events are identified and a comparative study of the interplanetary proton for the nonflare and flaring situations is provided. Proton events that are triggered by disappearing filaments appears not to be associated with the strong X-ray or radio radiation that characterizes solar flares.

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