Coronal Mass Ejection

Details Coronal Mass Ejection Coronal Mass Ejection

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991rspta.336..401h&link_type=abstract

Philosophical Transactions: Physical Sciences and Engineering, Volume 336, Issue 1643, pp. 401-412

Physics

26

Scientific paper

We summarize the observational aspects of the transient solar coronal features known as coronal mass ejections. Recognizing the importance of understanding this form of solar activity, particularly in the light of relations to flare and prominence activity, and geomagnetic effects, we consider the spectrum of models which have been used to describe these events and assess their viability. We find most models to be unphysical and all represent a gross over simplification of solar conditions. In conclusion we set up a cartoon model which best fits the observations and which we feel should be further developed.

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