Coronal Streamer Formation Post CME - Numerical Simulation

Details Coronal Streamer Formation Post CME - Numerical Simulation Coronal Streamer Formation Post CME - Numerical Simulation

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..370..103d&link_type=abstract

Solar and Stellar Physics Through Eclipses ASP Conference Series, Vol. 370, proceedings of the conference held 27-29 March, 2006

Physics

1

Scientific paper

A numerical experiment shows the possibility of a coronal streamer to
form after an eruptive process, e.g. after one or more CMEs `en
raffale'. This situation is sustained by some observations existing in
the literature.

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