Physics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..253b&link_type=abstract
In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze
Physics
Hard X-Rays, Electron, Flare, Acceleration
Scientific paper
We address the idea that energetic particles may play a key role in the dissipation and transport of energy in flares. After three decades of predictions of spatial, spectral and temporal distributions of hard X- and γ-rays, the various models can now be quantitatively tested against RHESSI high resolution spectral imaging data. It is shown that RHESSI results for a number of HXR flares are in very good agreement with predictions of the basic thick target model (Brown 1971) regarding source height as a function of energy and of global HXR spectrum. A single power-law injection spectrum and purely collisional transport (no wave generation) fit well the decrease of source peak height with increasing energy for very plausible chromospheric density structures. When the target ionisation drop across the transition one is included, the global HXR spectrum agrees well with observed "knee" spectra without any feature added to a scale-less power-law electron injection spectrum. This result favours statistically distributed, as opposed to single large scale, E-field acceleration. Whether energetic electron beams actually dominate flare energy transport still depends on accurate inference of the low energy thermal/nonthermal spectral transition though RHESSI results to date support the idea. The ion energy budget is also briefly mentioned.
Aschwanden Markus J.
Brown John C.
Kontar Eduard
MacKinnon Alexander L.
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