On the association of eruptive prominences, coronal holes and current sheets with the coronal mass ejections

Details On the association of eruptive prominences, coronal holes and current sheets with the coronal mass ejections On the association of eruptive prominences, coronal holes and current sheets with the coronal mass ejections

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20.2355s&link_type=abstract

Advances in Space Research, Volume 20, Issue 12, p. 2355-2358.

Physics

2

Scientific paper

In this paper, a study of the coronal mass ejections (CMEs) observed by Solar Maximum Mission satellite (SMM) during the period March - September, 1980, is presented. An attempt to identify various possible associations of the solar phenomena, for example, the location of coronal holes, the role of eruptive filaments or prominences, and current-sheets with the CMEs is carried out. It is shown that the combined associations of these three play an important role in the occurrence of geoeffective CMEs and also act as a tool to predict the associated geomagnetic activity.

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