Three solar filament disappearances associated with interplanetary low-energy particle events

Details Three solar filament disappearances associated with interplanetary low-energy particle events Three solar filament disappearances associated with interplanetary low-energy particle events

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..134..379s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 134, Aug. 1991, p. 379-394. Research supported by CAYCIT.

Physics

9

Charged Particles, Interplanetary Medium, Solar Corpuscular Radiation, Solar Prominences, International Sun Earth Explorer 3, Shock Waves, Solar Wind

Scientific paper

Three low-energy particle events (35-1600 keV) associated with interplanetary shocks, detected at 1 AU by ISEE-3, have been identified as originating in solar disappearing filaments instead of large flares. This increases to 14 the number of events of this kind presently known. The observational characteristics of these nonflare generated events are similar to the ones of the other 11 events already known (i.e., absence of type II or IV bursts, weak X-ray emission, H-alpha brightening in the surroundings of the filament disappearance, frequent presence of a double-ribbon event, slow propagation of the generated interplanetary shock, lack of shock deceleration).

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