Interplanetary signatures of solar mass ejections

Details Interplanetary signatures of solar mass ejections Interplanetary signatures of solar mass ejections

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..107b&link_type=abstract

Advances in Space Research, vol. 20, p. 107

Computer Science

4

Solar Corona, Interplanetary Medium, Solar Wind, Coronal Mass Ejection, Solar Flux, Plasma Composition, Magnetic Clouds, Solar Electrons, Ion Density (Concentration), Solar Flares

Scientific paper

The transient interplanetary signatures of bidirectional electron and ion fluxes, He enhancements and magnetic clouds observed in the solar wind at 1 AU have been subjected to a correlative analysis with the corresponding solar observations, in order to distinguish their solar origins. Over 90 percent of these signatures correspond to the occurrence of a flare or prominence eruption near the solar central meridian 1-4 days prior to the observation of the disturbance at 1 AU. Differerent signatures belong to different plasma regions within the ejecta.

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