Properties of coronal mass ejections

Details Properties of coronal mass ejections Properties of coronal mass ejections

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..181m&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Solar Physics, Space Weather, Cmes

Scientific paper

We report the properties of all coronal mass ejections (CMEs) recorded
by SOHO/LASCO coronagraph from January 1996 through December 2001. We
show preliminary statistical considerations describing velocity,
acceleration, widths and angle position of CMEs. We compare them to the
previous surveys.

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