Particle anisotropies observed within ejecta during solar particle onsets

Details Particle anisotropies observed within ejecta during solar particle onsets Particle anisotropies observed within ejecta during solar particle onsets

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..453r&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 453

Physics

Particle Emission, Solar Wind

Scientific paper

We demonstrate that the anisotropies of energetic particles (>0.2 MeV electrons and >1 MeV protons) can provide information on the magnetic topology of ejecta. In particular, we have examined 38 solar energetic particle events for which the onset phase was observed by ISEE 3 when the spacecraft was located inside an ejecta. Around 30% of these particle events exhibit unusual flows from the east of the Sun at event onset. Such flows are rarely found in 34 events which were observed outside ejecta. The observations are consistent with the presence of looped magnetic structures in ejecta.

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