Radio emission from quasi-parallel shock waves in the corona

Details Radio emission from quasi-parallel shock waves in the corona Radio emission from quasi-parallel shock waves in the corona

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...68..199m&link_type=abstract

Space Science Reviews, Volume 68, Issue 1-4, pp. 199-203

Physics

Scientific paper

Shock waves in the solar corona manifest themselves in type II bursts in dynamic radio spectra. Recently, short large amplitude magnetic structures (SLAMS) have been observed in the vicinity of the quasi-parallel region of Earth's bow shock as an example of a collisionless shock wave in space plasmas. SLAMS are able to accelerate electrons to high energies by shock drift acceleration. Assuming that SLAMS also appear in the vicinity of super-critical, quasi-parallel shocks in the corona, electrons can also be accelerated at quasi-parallel shocks and, subsequently, generate radio waves manifesting in solar type II radio bursts.

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