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arxiv: 0804.4041 · v1 · submitted 2008-04-25 · 🌌 astro-ph

Parametric instabilities of large-amplitude parallel propagating Alfven waves: 2-D PIC simulation

classification 🌌 astro-ph
keywords wavesalfvenparallelpropagatinginstabilitysimulationdifferentheated
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We discuss the parametric instabilities of large-amplitude parallel propagating Alfven waves using the 2-D PIC simulation code. First, we confirmed the results in the past study [Sakai et al, 2005] that the electrons are heated due to the modified two stream instability and that the ions are heated by the parallel propagating ion acoustic waves. However, although the past study argued that such parallel propagating longitudinal waves are excited by transverse modulation of parent Alfven wave, we consider these waves are more likely to be generated by the usual, parallel decay instability. Further, we performed other simulation runs with different polarization of the parent Alfven waves or the different ion thermal velocity. Numerical results suggest that the electron heating by the modified two stream instability due to the large amplitude Alfven waves is unimportant with most parameter sets.

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