2015/12/07 by Bin Chen, Timothy S. Bastian, Chengcai Shen +3 · 2 citations
Physics and Astronomy · #astro-ph.SR #astro-ph.HE
paper · pdf · doi:10.1126/science.aac8467
published as Science, 4 December 2015, Vol. 350 no. 6265 pp. 1238-1242 · Published on Science on December 4, 2015. 28 pages, 10 figures. Article url: http://www.sciencemag.org/content/350/6265/1238.short. Supplementary Movie S1 is available at https://web.njit.edu/~binchen/download/publications/Chen+2015_TS/
arxiv created 2015/12/07 · arxiv updated 2015/12/09
Solar flares - the most powerful explosions in the solar system - are also efficient particle accelerators, capable of energizing a large number of charged particles to relativistic speeds. A termination shock is often invoked in the standard model of solar flares as a possible driver for particle acceleration, yet its existence and role have remained controversial. We present observations of a solar flare termination shock and trace its morphology and dynamics using high-cadence radio imaging spectroscopy. We show that a disruption of the shock coincides with an abrupt reduction of the energetic electron population. The observed properties of the shock are well-reproduced by simulations. These results strongly suggest that a termination shock is responsible, at least in part, for accelerating energetic electrons in solar flares.