Electron Acceleration and Transport in Microwave Flaring Loops

Details Electron Acceleration and Transport in Microwave Flaring Loops Electron Acceleration and Transport in Microwave Flaring Loops

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spnr.conf...11m&link_type=abstract

Solar Physics with the Nobeyama Radioheliograph, Proceedings of Nobeyama Symposium 2004, held in Kiyosato, Japan, October 26- 29

Physics

5

Scientific paper

Nobeyama Radioheliograph has high spatial and temporal resolution at two frequencies where a nonthermal radio source is often optically thin. Such capabilities provide us with unique opportunity to get constraints on properties of mildly relativistic electrons accelerated and propagating in flaring magnetic loops. In this paper we review recent studies of Nobeyama observations concerning 1) spatial distribution of microwave brightness and spectral slope along flaring loops; 2) peculiarities of their temporal dynamics in different parts of a loop; 3) consequences of the obtained findings on spatial, spectral and pitch-angle distributions of high energy electrons.

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