Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh23b1542k&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SH23B-1542
Astronomy and Astrophysics
Astrophysics
[7531] Solar Physics, Astrophysics, And Astronomy / Prominence Eruptions
Scientific paper
Solar prominence eruptions are extremely important phenomena due to their association with coronal mass ejections and their effects on space weather near Earth and throughout the solar system. Some insights into the eruption mechanism have been made via MHD modeling and observational studies, but comparisons between the models and observations have been inconclusive thus far. A coordinated observational study of prominence eruptions is being carried out to measure and compare various precursors to eruption that have been found in previous studies, including: heating of the material, emerging or canceling magnetic flux, increase in cavity size, and changes in the prominence mass and its composition. Our analysis examines the timing and the relative degree of these observational trends prior to eruption, and utilizes a wide range of observatories and instruments.
Davila Jose Manuel
Kilper Gary K.
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