Astronomy and Astrophysics – Astronomy
Scientific paper
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.
Burkart Thomas
Ganse Urs
Spanier Felix
Vainio Rami
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