A ``perfect'' Late Phase Flare Loop: X-ray And Radio Studies

Details A ``perfect'' Late Phase Flare Loop: X-ray And Radio Studies A ``perfect'' Late Phase Flare Loop: X-ray And Radio Studies

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1917b&link_type=abstract

American Astronomical Society, SPD meeting #40, #19.17; Bulletin of the American Astronomical Society, Vol. 41, p.849

Astronomy and Astrophysics

Astronomy

Scientific paper

We present observations of a GOES X3.1 class flare which occurred on the 24th August 2002. The event was observed by a number of instruments including RHESSI, TRACE and NoRH. This flare is particularly interesting due to its position and orientation on the west limb of the Sun. The flare appears to be perpendicular to the line of sight making it possible to ascertain the geometrical parameters of the post flare arcade loops. We investigate the decay phase of the flare by comparing X-ray and radio observations of the post flare arcade loops with models of soft x-ray and thermal gyrosynchrotron emission to characterise the electron distribution present within the loop.
HMB gratefully acknowledges the support of an SPD and STFC studentship. LF gratefully acknowledges the support of an STFC Rolling Grant, and financial support by the European Commission through the SOLAIRE Network (MTRN-CT_2006-035484)

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