Earth-directed coronal mass ejection

Details Earth-directed coronal mass ejection Earth-directed coronal mass ejection

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pabei..20...33s&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 20, No. 1, p. 33 - 44 (2002)

Astronomy and Astrophysics

Astronomy

1

Earth-Directed Cme, Solar Activity, Magnetic Reconnection

Scientific paper

Coronal mass ejections (CMEs), known as the most spectacular form of solar magnetic activity, are of great scientific significance in the fields of solar physics. As one special kind of CMEs, earth-directed CMEs are usually associated with severe geomagnetic storms and interplanetary shocks as well as high-energy particle events. They are main factors of space weather and have strong geoeffectiveness. This paper summarizes the most recent progress of earth-directed CMEs, and mainly focuses on the evolution of the photosphere magnetic field associated with them. The relationships between earth-directed CMEs and filament eruptions, flares and other solar activities are discussed. Finally, some open questions and future researches are presented.

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