Observational properties of the coronal mass ejection.

Details Observational properties of the coronal mass ejection. Observational properties of the coronal mass ejection.

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pabei..15...44s&link_type=abstract

Prog. Astron., Vol. 15, No. 1, p. 44 - 52

Other

Solar Corona: Mass Ejection, Solar Corona: Magnetic Fields

Scientific paper

The observational properties of the coronal mass ejection (CME) are summarized. After a brief introduction, the discovery and the statistic properties of CMEs are given, with an emphasis on the correlations of CMEs to other kinds of solar activity. Afterwards, their general properties are given, including the observational properties of some physical processes which are possibly relevant to CMEs. A preliminary conclusion is: CMEs are phenomena of evolving magnetic structures.

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