Quasi-parallel shock structure and processes

被引：125

作者：

Burgess, D ^{[1
]}

Lucek, EA

Scholer, M

Bale, SD

Balikhin, MA

Balogh, A

Horbury, TS

Krasnoselskikh, VV

Kucharek, H

Lembège, B

Möbius, E

Schwartz, SJ

Thomsen, MF

Walker, SN

机构：

[1] Univ London, Queen Mary, Astron Unit, London, England

[2] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London, England

[3] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany

[4] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[5] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[6] Univ Sheffield, Sheffield, S Yorkshire, England

[7] CNRS, LPCE, F-45071 Orleans, France

[8] Univ New Hampshire, Inst Study Earth Oceans & Space, Ctr Space Sci, Durham, NH 03824 USA

[9] IPSL, CETP, Velizy Villacoublay, France

[10] Univ New Hampshire, Dept Phys, Durham, NH 03824 USA

[11] Los Alamos Natl Lab, Los Alamos, NM USA

来源：

SPACE SCIENCE REVIEWS | 2005年 / 118卷 / 1-4期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1007/s11214-005-3832-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The role of the quasi-parallel shock in the development and testing of theories of particle acceleration is discussed. A standard model was developed in which the quasi-parallel shock transition was viewed as a patchwork of magnetic field enhancements, which grew from the interaction between upstream waves in the plasma frame and a gradient in the supra-thermal particle pressure. These magnetic field enhancements were termed SLAMS (short large amplitude magnetic structure) and were proposed to be the building blocks of the shock. The overall ordering of transitions indicate anti-sunward convection, but sometimes the ordering varies between leading and trailing edges and also between pulsations.

引用

页码：205 / 222

页数：18

共 34 条

[1] OUTWARD FLOW OF PROTONS FROM EARTHS BOW SHOCK [J].