Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.1313w&link_type=abstract
American Astronomical Society, SPD meeting #37, #13.13; Bulletin of the American Astronomical Society, Vol. 38, p.242
Astronomy and Astrophysics
Astronomy
Scientific paper
We are combining thermal plasma and non-thermal particle numerical models in order to improve flare simulations. Non-thermal particle collision models provide heating and momentum deposition for the thermal plasma. The thermal plasma models in turn provide an evolving temperature and density structure for the non-thermal particles' target plasma. This allows us to simulate thermal and non-thermal flare emission under a variety of increasingly realistic solar conditions. In this work we inject non-thermal, energetic particles into plasmas contained in loops defined by three different analytic magnetic field models. We monitor the evolution of these loops over time as it would be seen by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI), The Transition Region and Coronal Explorer (TRACE), the Soft X-ray Telescope (SXT) and the Hard X-ray Telescope (HXT) onboard the Yohkoh satellite as well as the upcoming X-Ray Telescope (XRT) onboard Solar-B and the Atmospheric Imaging Array (AIA) on the Solar Dynamics Observatory.This work is supported by NASA grant NAG5-12820.
Martens Petrus C.
Winter Henry D. III
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