Shock Waves, Particle Acceleration, SEPs and Type II Bursts

Details Shock Waves, Particle Acceleration, SEPs and Type II Bursts Shock Waves, Particle Acceleration, SEPs and Type II Bursts

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh32a..01r&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH32A-01

Physics

7513 Coronal Mass Ejections (2101), 7514 Energetic Particles (2114), 7534 Radio Emissions, 7549 Ultraviolet Emissions

Scientific paper

Type II radio bursts have long been used as the main indicator of shocks in the corona, giving both the density and an estimate of shock speed. This talk compares radio with white light and UV diagnostics for shocks, with particular attention to pre-shock coronal conditions and the conditions needed for efficient acceleration of Solar Energetic Particles (SEPs).

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