Energy partition in two solar flare/CME events

Details Energy partition in two solar flare/CME events Energy partition in two solar flare/CME events

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004jgra..10910104e&link_type=abstract

Journal of Geophysical Research, Volume 109, Issue A10, CiteID A10104

Astronomy and Astrophysics

Astrophysics

77

Solar Physics, Astrophysics, And Astronomy: Flares, Solar Physics, Astrophysics, And Astronomy: Coronal Mass Ejections, Solar Physics, Astrophysics, And Astronomy: Energetic Particles (2114), Solar Physics, Astrophysics, And Astronomy: X Rays, Gamma Rays, And Neutrinos

Scientific paper

Using coordinated observations from instruments on the Advanced Composition Explorer (ACE), the Solar and Heliospheric Observatory (SOHO), and the Ramaty High Energy Solar Spectroscopic Imager (RHESSI), we have evaluated the energetics of two well-observed flare/CME events on 21 April 2002 and 23 July 2002. For each event, we have estimated the energy contents (and the likely uncertainties) of (1) the coronal mass ejection, (2) the thermal plasma at the Sun, (3) the hard X-ray producing accelerated electrons, (4) the gamma-ray producing ions, and (5) the solar energetic particles. The results are assimilated and discussed relative to the probable amount of nonpotential magnetic energy available in a large active region.

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