Electron acceleration to relativistic energies at a strong quasi-parallel shock wave

被引：0

作者：

A. Masters

L. Stawarz

M. Fujimoto

S. J. Schwartz

N. Sergis

M. F. Thomsen

A. Retinò

H. Hasegawa

B. Zieger

G. R. Lewis

A. J. Coates

P. Canu

M. K. Dougherty

机构：

[1] Institute of Space and Astronautical Science,Department of Space and Climate Physics

[2] Japan Aerospace Exploration Agency,undefined

[3] Earth-Life Science Institute,undefined

[4] Tokyo Institute of Technology,undefined

[5] Space and Atmospheric Physics Group,undefined

[6] The Blackett Laboratory,undefined

[7] Imperial College London,undefined

[8] Office of Space Research and Technology,undefined

[9] Academy of Athens,undefined

[10] Soranou Efesiou 4,undefined

[11] Space Science and Applications,undefined

[12] Los Alamos National Laboratory,undefined

[13] Laboratoire de Physique des Plasmas,undefined

[14] Centre National de la Recherche Scientifique,undefined

[15] Observatoire de Saint-Maur,undefined

[16] Center for Space Physics,undefined

[17] Boston University,undefined

[18] Mullard Space Science Laboratory,undefined

[19] University College London,undefined

[20] The Centre for Planetary Sciences at UCL/Birkbeck,undefined

[21] Gower Street,undefined

来源：

Nature Physics | 2013年 / 9卷

关键词：

D O I：

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学科分类号：

摘要：

Data from the Cassini spacecraft identify strong electron acceleration as the solar wind approaches the magnetosphere of Saturn. This so-called bow shock unexpectedly occurs even when the magnetic field is roughly parallel to the shock-surface normal. Knowledge of the magnetic dependence of electron acceleration will aid understanding of supernova remnants.

引用

页码：164 / 167

页数：3

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