The Characteristics of Hard X-ray Production in Flares Driven by Filament Eruptions

Details The Characteristics of Hard X-ray Production in Flares Driven by Filament Eruptions The Characteristics of Hard X-ray Production in Flares Driven by Filament Eruptions

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp23b..04l&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP23B-04

Physics

7519 Flares, 7531 Prominence Eruptions

Scientific paper

We investigate the temporal and spatial relationship between filament eruptions and the production of hard X-ray emission using spatially resolved high cadence data from TRACE and RHESSI. In particular, we focus on comparing the characteristics of the hard X-ray production in `successful' and `failed' filament eruption cases. Our preliminary findings indicate even failed eruption events can generate significant energy release and hard X-ray emission with the hard X-ray production apparently correlated to the rate of expansion of the filament. The spatial distribution of the hard X-ray emission, while depending upon the overall strength of the event, also depends on the evolutionary behavior of the filament as it erupts, e.g. loop-like versus "zipper"-like.

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