Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh52a..05m&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SH52A-05
Astronomy and Astrophysics
Astrophysics
7514 Energetic Particles (2114), 7846 Plasma Energization, 7851 Shock Waves (4455), 7867 Wave/Particle Interactions (2483, 6984), 7868 Wave/Wave Interactions
Scientific paper
High Mach number shocks in space and astrophysical plasmas have been extensively studied, both observationally and theoretically, since it is a mine of various kinds of wave activities and mechanisms of particle accleration/heating. In particular, recent full particle simulation studies revealed that a variety of microinstabilities, for instance the Buneman instability, the electron cyclotron drift instability, the modified two-stream instability, etc., are generated in the foot of low beta supercritical quasi-perpendicular shocks. Since each instability has different propagation angle with respect to the ambient magnetic field, multi-dimensionality is important to discuss all instabilies simultaneously. In this study, a 2D PIC (particle-in-cell) simulation with periodic boundary conditions in both directions is performed as a proxy for the foot region which includes incoming and reflected ions, and electrons. The simulation shows that six types of different instabilities are excited in a time period shorter than ion gyro period of the reflected ions. The most dominant instability is the modified two-stream instability, which leads to strong electron heating through a so-called two step instability. Influences of the modified two-stream instability to shock stationarity are also discussed.
Matsukiyo Shuichi
Scholer Manfred
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