Kinetic Simulations of Solar Type II Radio Burst Emission Processes

Details Kinetic Simulations of Solar Type II Radio Burst Emission Processes Kinetic Simulations of Solar Type II Radio Burst Emission Processes

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..245g&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 245-248 (2010).

Astronomy and Astrophysics

Astronomy

Corona, Radio Sources (Astronomical), Magnetohydrodynamics, Particle Sources, Coronal Mass Ejection, Radio Sources, Magnetohydrodynamics And Plasmas, Particle-In-Cell Method

Scientific paper

Using our kinetic Particle-in-Cell simulation code, we have examined the behavior of different plasma modes in the environment close to a CME shock front, with special focus on the modes that may contribute to the formation of type II radio bursts. Apart from electron velocity spectra, numerical dispersion plots obtained from simulation data allow for analysis of wave modes in the simulated plasma, especially showing growth and damping of these modes over time. These plots reveal features at 2ωp which are not predicted by linear wave theory, that may be results of nonlinear three wave interaction processes as theoretically predicted for type II emission processes.

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