Solar coronal mass ejections

Details Solar coronal mass ejections Solar coronal mass ejections

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..165c&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 70, no. 1, p. 165-187.

Astronomy and Astrophysics

Astronomy

9

Solar Corona, Solar Flares, Solar Radio Emission, Stellar Mass Ejection, Coronagraphs, Solar Planetary Interactions, Solar Prominences

Scientific paper

New data on solar coronal mass ejections (CMEs) and associated events are summarized. Topics addressed include general information on CMEs and methods of observing them; differences between measurements of CME parameters and white-light coronagraphs on board the P78-1 and SMM satellites; relationships between CME, precursor, and flare; and eruption of filaments (prominences) and the onset of CMEs. Also discussed are models of CME eruption; CME radio emission; CMEs and the final phase of the flare; CMEs and slow shock waves; variations of CME parameters during the solar activity cycle; CMEs and coronal evolution; the 3D structure of CMEs; interplanetary manifestations of CMEs; and CMEs from flares and disappearing filaments as a single spectrum of solar eruptive phenomena.

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