journal article·2019-12-01Open access

Mach number and plasma beta dependence of the ion temperature perpendicular to the external magnetic field in the transition region of perpendicular collisionless shocks

Ryo Yamazaki, Ayato Shinoda, Takayuki Umeda, Shuichi Matsukiyo

AIP Advances· Volume 9· Issue 12

Abstract

Ion temperature anisotropy is a common feature for (quasi-)perpendicular collisionless shocks. By using two-dimensional full particle simulations, it is shown that the ion temperature component perpendicular to the shock magnetic field at the shock foot region is proportional to the square of the Alfvén Mach number divided by the plasma beta. This result is also explained by a simple analytical argument in which the reflected ions get energy from an upstream plasma flow. By comparing our analytic and numerical results, it is also confirmed that the fraction of the reflected ions hardly depends on the plasma beta and the Alfvén Mach number when the square of the Alfvén Mach number divided by the plasma beta is larger than about 20.
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Research context

OpenAlex topics: Ionosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Magnetic confinement fusion research

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Physics and Mathematics, Aoyama Gakuin University 1 , Sagamihara 252-5258, Japan

Institute of Laser Engineering, Osaka University 2 , 2-6 Yamadaoka, Suita, Osaka 565-0871, Japan

Institute for Space-Earth Environmental Research, Nagoya University 3 , Nagoya 464-8601, Japan

Department of Earth System Science and Technology, Kyushu University 4 , Kasuga 816-8580, Japan

Funding

Ministry of Education, Culture, Sports, Science and Technology

References (29)

Show source-provided references
1. 2013
2. 2015
3. Plasma Phys. · 1971 · 13 · 28910.1088/0032-1028/13/4/302 ↗
4. Phys. Fluids · 1983 · 26 · 274210.1063/1.864468 ↗
5. J. Geophys. Res. · 1983 · 88 · 612110.1029/ja088ia08p06121 ↗
6. 1985 · 141
7. J. Geophys. Res. · 1989 · 94 · 878310.1029/ja094ia07p08783 ↗
8. Planet. Space Sci. · 1990 · 38 · 41910.1016/0032-0633(90)90108-3 ↗
9. J. Geophys. Res. · 1990 · 95 · 633710.1029/ja095ia05p06337 ↗
10. Phys. Fluids B · 1992 · 4 · 353310.1063/1.860361 ↗
11. J. Geophys. Res. · 1988 · 93 · 968110.1029/ja093ia09p09681 ↗
12. Ann. Geophys. · 2003 · 21 · 67110.5194/angeo-21-671-2003 ↗
13. Geophys. Res. Lett. · 2019 · 46 · 238110.1029/2018gl080240 ↗
14. J. Geophys. Res. · 2019 · 124 · 396110.1029/2018ja026197 ↗
15. Astrophys. J. · 2009 · 695 · 57410.1088/0004-637x/695/1/574 ↗
16. J. Geophys. Res. · 1996 · 101 · 1556910.1029/96ja00924 ↗
17. Geophys. Res. Lett. · 1997 · 24 · 251110.1029/97gl02524 ↗
18. J. Plasma Phys. · 2015 · 81 · 90581060310.1017/s0022377815001154 ↗
19. Phys. Plasmas · 2015 · 22 · 07230110.1063/1.4926452 ↗
20. J. Geophys. Res. · 2009 · 114 · A0910610.1029/2009ja014365 ↗
21. J. Geophys. Res. · 2013 · 118 · 182810.1029/2012ja018188 ↗
22. Comput. Phys. Commun. · 2003 · 156 · 7310.1016/s0010-4655(03)00437-5 ↗
23. Particle simulation of a perpendicular collisionless shock: A shock-rest-frame model10.1186/bf03352617 ↗
24. Astrophys. J. · 2008 · 681 · L8510.1086/590408 ↗
25. Comput. Phys. Commun. · 2001 · 137 · 28610.1016/s0010-4655(01)00182-5 ↗
26. Planet. Space Sci. · 1970 · 18 · 161110.1016/0032-0633(70)90036-x ↗
27. Phys. Plasmas · 2012 · 19 · 04210910.1063/1.3703319 ↗
28. Phys. Plasmas · 2014 · 21 · 02210210.1063/1.4863836 ↗
29. J. Geophys. Res. · 2003 · 108 · 123310.1029/2002JA009339 ↗