Hard X-rays Associated With Solar Type III Radio Bursts

Details Hard X-rays Associated With Solar Type III Radio Bursts Hard X-rays Associated With Solar Type III Radio Bursts

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.2904c&link_type=abstract

American Astronomical Society, SPD meeting #37, #29.04; Bulletin of the American Astronomical Society, Vol. 38, p.256

Astronomy and Astrophysics

Astronomy

Scientific paper

During a period of 12 minutes on 19 July 2002 14:23-14:35 UT, the WAVES instrument on the Wind spacecraft observed interplanetary type III radio bursts approximately every 2 minutes, and each was accompanied by a hard X-ray burst (12-15 keV) observed by RHESSI. We investigate the emission mechanism for the observed hard X-rays for each event. We find that the four smallest X-ray events are inconsistent with emission from a thermal plasma or a nonthermal beam suggesting that the observed emission is related to the acceleration mechanism of type IIIs.

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