STEREO Observations of Slow Coronal Mass Ejections

Details STEREO Observations of Slow Coronal Mass Ejections STEREO Observations of Slow Coronal Mass Ejections

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.2103l&link_type=abstract

American Astronomical Society, SPD meeting #40, #21.03; Bulletin of the American Astronomical Society, Vol. 41, p.855

Astronomy and Astrophysics

Astronomy

Scientific paper

We have studied the STEREO/COR1 coronal mass ejection (CME) catalog for the period January-September 2008. Many of the observed CMEs exhibit slow liftoff speeds, commonly taking over 24 hours for the entire CME to exit the COR1 field of view. We will present a detailed overview of these slowly rising CMEs and trace their evolution from the on-disk source region, where possible, through the field of view of both STEREO coronagraphs. This is a first step towards studying the evolution of these CMEs in interplanetary space.

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