Constraints on electron acceleration/injection from NoRH observations

Details Constraints on electron acceleration/injection from NoRH observations Constraints on electron acceleration/injection from NoRH observations

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..257m&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Solar Flares, Microwave Emission, Particle Acceleration And Transport

Scientific paper

Nobeyama Radioheliograph microwave data provide us with unique information about radio brightness distribution along flaring loops. In particular it has been found for several events that the brightness maximum at 17 and 34 GHz is located at the top of extended flaring loops. The detailed analysis of these events strongly suggests that the distribution of mildly relativistic electrons along an extended flaring loop must be highly inhomogeneous: accelerated electrons are concentrated in the upper part of the loop. This finding impose important new constraints on the acceleration/injection mechanisms and kinetics of high energy particles in solar flares.

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