Role of the overshoot in the shock self-organization

被引:6
|
作者
Gedalin, Michael [1 ]
Dimmock, Andrew P. [2 ]
Russell, Christopher T. [3 ]
Pogorelov, Nikolai V. [4 ]
Roytershteyn, Vadim [5 ]
机构
[1] Ben Gurion Univ Negev, Dept Phys, Beer Sheva, Israel
[2] Swedish Inst Space Phys, Uppsala, Sweden
[3] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA USA
[4] Univ Alabama Huntsville, Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USA
[5] Space Sci Inst, Boulder, CO 80301 USA
基金
欧盟地平线“2020”; 美国国家航空航天局;
关键词
space plasma physics; plasma heating; astrophysical plasmas; QUASI-PERPENDICULAR SHOCKS; COLLISIONLESS SHOCK; JUMP;
D O I
10.1017/S0022377823000090
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
A collisionless shock is a self-organized structure where fields and particle distributions are mutually adjusted to ensure a stable mass, momentum and energy transfer from the upstream to the downstream region. This adjustment may involve rippling, reformation or whatever else is needed to maintain the shock. The fields inside the shock front are produced due to the motion of charged particles, which is in turn governed by the fields. The overshoot arises due to the deceleration of the ion flow by the increasing magnetic field, so that the drop of the dynamic pressure should be compensated by the increase of the magnetic pressure. The role of the overshoot is to regulate ion reflection, thus properly adjusting the downstream ion temperature and kinetic pressure and also speeding up the collisionless relaxation and reducing the anisotropy of the eventually gyrotropized distributions.
引用
收藏
页数:15
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