Computer Science – Sound
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh23a0341l&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #SH23A-0341
Computer Science
Sound
7534 Radio Emissions, 7829 Kinetic Waves And Instabilities, 7857 Stochastic Phenomena (3235, 3265, 4475), 7867 Wave/Particle Interactions (2483, 6984), 7868 Wave/Wave Interactions
Scientific paper
For type III solar radio bursts, plasma emission is generally accepted as the main emission mechanism. This mechanism consists of several steps that involve quasilinear electron beam-Langmuir wave interactions, and nonlinear interactions among Langmuir waves, ion-sound waves, and electromagnetic waves. Very recently, the effects of density inhomogeneities in the corona and the solar wind on type III electromagnetic radiations are numerically studied. We report here some of these results that taking into account both small-scale and large-scale density inhomogeneities, and the dynamics of the beam, Langmuir and ion-sound waves, and electromagnetic radiation. Dynamic spectra of the electromagnetic emission seen at a remote observer are presented, and compared quantitatively with observations at Earth. The establishment of a stochastic growth state for the beam-Langmuir wave system is also demonstrated.
Cairns Iver
Li Baowen
Robinson Patricia
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