Multiscale simulations of type III solar radio emission via beam-driven Langmuir waves

Details Multiscale simulations of type III solar radio emission via beam-driven Langmuir waves Multiscale simulations of type III solar radio emission via beam-driven Langmuir waves

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..932...32r&link_type=abstract

TURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS; 6th Annual International Astrophysics Conference. AIP Conference P

Astronomy and Astrophysics

Astrophysics

Radio Emission, Mhd Waves, Plasma Waves, Turbulence, Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

In type III solar radio bursts, plasma emission is widely accepted to be the main emission mechanism. It involves quasilinear electron beam-Langmuir wave interactions, and nonlinear interactions among Langmuir, ion-sound, and electromagnetic waves. These take place amid ambient density fluctuations superposed on the large-scale density gradient in the solar corona and wind. We overview simulations that take into account these processes amid small-scale density fluctuations and large-scale gradients. Source properties and dynamic spectra are compared with observations and establishment of a stochastic growth state is demonstrated in the presence of fluctuations.

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