The Evolution of Prominence Mass and its Relation to CMEs

Details The Evolution of Prominence Mass and its Relation to CMEs The Evolution of Prominence Mass and its Relation to CMEs

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh41b1672g&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH41B-1672

Astronomy and Astrophysics

Astrophysics

[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7531] Solar Physics, Astrophysics, And Astronomy / Prominence Eruptions

Scientific paper

Prominences have long been associated with coronal mass ejections (CMEs) and provide an important component in our understanding of the Sun-Earth system as a whole. Although some prominences are long-lived and others erupt or disappear on short time scales, all types of prominences are dynamical and many show mass loss in observations through draining. Such mass loss often occurs without an eruption, while sometimes occurring prior to and/or during an eruption. We explore the relationship between the nature of a prominence eruption (i.e., full, partial, failed) and the associated CME properties (e.g., speed, mass, and energy).

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