Physics – Plasma Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh51d1724s&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SH51D-1724
Physics
Plasma Physics
[7829] Space Plasma Physics / Kinetic Waves And Instabilities, [7845] Space Plasma Physics / Particle Acceleration, [7851] Space Plasma Physics / Shock Waves
Scientific paper
Recent progress of computational power enables us to perform really macro-scale three-dimensional situations with full particle codes. In this presentation, we will report results of a three-dimensional simulation of a quasi-perpendicular shock. The simulation parameters were selected to simulate a Cluster-II observational result reported by Seki et al. (2009), M_A=7.4 and beta=0.16. The realistic mass ratio mi/me=1840 was taken, and almost one ion inertia length square could be allocated to the plane perpendicular to the upstream flow axis. The result shows that both the self-reformation process and whistler emission are observed. However, the 3-D result is not a simple superposition of 2-D results. The most impressive feature is that quite complicated wave activity is found in the shock foot region. With the help of this wave activity, electron heating observed in the 3-D run is more efficient than those in the 1-D and 2-D runs with the same shock parameters. Moreover, non-thermal electrons are also produced only in the 3D run. In this paper, comparing the 3-D result with previous 1-D and 2-D simulation results, three dimensional nature of the shock transition region of quasi-perpendicular shock is discussed.
Fujimoto Minoru
Shinohara Iku
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