Kinetic Simulations of Type II Radio Burst Emission Processes

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

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274..470g&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 470-472

Astronomy and Astrophysics

Astrophysics

1

Methods: Numerical, Radiation Mechanisms: Nonthermal, Shock Waves, Sun: Radio Radiation, Waves

Scientific paper

Using a fully relativistic, 3D particle in cell code we have studied Langmuir- and electromagnetic wave processes in a CME foreshock plasma with counterstreaming electron beams. Langmuir wave excitation in resonance with the plasma frequency is observed, with timescales in accordance with theoretical predictions. However, no three wave interaction leading to emission of electromagnetic waves were detectable within the timeframe of our simulations.

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