PLASMA EMISSION BY COUNTER-STREAMING ELECTRON BEAMS

Abstract

ABSTRACT The radiation emission mechanism responsible for both type-II and type-III solar radio bursts is commonly accepted as plasma emission. Recently Ganse et al. suggested that type-II radio bursts may be enhanced when the electron foreshock geometry of a coronal mass ejection contains a double hump structure. They reasoned that the counter-streaming electron beams that exist between the double shocks may enhance the nonlinear coalescence interaction, thereby giving rise to more efficient generation of radiation. Ganse et al. employed a particle-in-cell simulation to study such a scenario. The present paper revisits the same problem with EM weak turbulence theory, and show that the fundamental ( F ) emission is not greatly affected by the presence of counter-streaming beams, but the harmonic ( H ) emission becomes somewhat more effective when the two beams are present. The present finding is thus complementary to the work by Ganse et al.