The launch of solar coronal mass ejections - Results from the coronal mass ejection onset program

Details The launch of solar coronal mass ejections - Results from the coronal mass ejection onset program The launch of solar coronal mass ejections - Results from the coronal mass ejection onset program

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95..917h&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, Feb. 1, 1990, p. 917-937.

Physics

94

Solar Activity Effects, Solar Corona, Solar Flares, Stellar Mass Ejection, Chromosphere, Solar Atmosphere, Solar Magnetic Field, Solar Prominences

Scientific paper

A set or solar coronal mass ejection (CME) events is described where coincident data sets from both X-ray and white light instruments have been made available through deliberate planning. These have been used to put tight limits on possible descriptions of the typical sequence of events and related to interpretations of models involving flares and CMEs. The findings confirm recent suggestions that CME onsets precede any related flare activity and that the associated flaring commonly lies to one side of the CME span.

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