Abstract
A technique has been developed to separate the signal of CMEs from the
background quiescent corona. The method works best for a radial corona
(SECCHI/COR 2 or LASCO/C2 & C3 for example), but can be adapted to
cope with non-radial coronal structure (SECCHI/COR 1 or MLSO
coronameters). A brief summary of the technique will be given, followed
by an overview of results, a discussion of limitations, and the
implications for both CME and quiescent coronal science. The high
temporal cadence of observations by the SECCHI instruments allow the
viewing of dynamic events from the low corona (EUVI regions) to the
extended corona. For the first time, even fairly small events can be
tracked as they propogate and evolve through the corona. The CME
separation technique provides a very useful tool to view this evolution,
particularly in the white light coronagraph images where faint CME
signals cannot be effectively viewed in regions containing bright
streamers.
Original language | English |
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Pages | 893 |
Publication status | Published - 01 May 2010 |