SOLWIND observations of coronal mass ejections during 1979-1985

Details SOLWIND observations of coronal mass ejections during 1979-1985 SOLWIND observations of coronal mass ejections during 1979-1985

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sfcp.nasa..241s&link_type=abstract

In NASA. Marshall Space Flight Center Solar Flares and Coronal Physics Using P/OF as a Research Tool p 241-256 (SEE N86-24614

Physics

2

Mass Transfer, Solar Corona, Solar Wind, Sunspot Cycle, Interplanetary Medium, Magnetic Fields, Solar X-Rays

Scientific paper

Coronal observations have been processed for parts of each year during the interval 1979-1985. Around sunspot maximum, coronal mass ejections (CMEs) occurred at the rate of approximately 2 per day, and had a wide range of physical and morphological properties. During the recent years of relatively low sunspot number, CMEs occurred at the rate of only 0.2 per day, and were dominated by the class of so-called streamer blowout. These special CMEs maintained a nearly constant occurrence rate of roughly 0.1 per day during the entire interval.

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