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在地球磁尾的磁重联扩散区域中,存在电子加速至约300keV的证据。

Evidence for electron acceleration up to approximately 300 keV in the magnetic reconnection diffusion region of earth's magnetotail.

作者信息

ØIeroset M, Lin R P, Phan T D, Larson D E, Bale S D

机构信息

Space Sciences Laboratory, University of California, Berkeley, California 94720, USA.

出版信息

Phys Rev Lett. 2002 Nov 4;89(19):195001. doi: 10.1103/PhysRevLett.89.195001. Epub 2002 Oct 18.

Abstract

We report direct measurements of high-energy particles in a rare crossing of the diffusion region in Earth's magnetotail by the Wind spacecraft. The fluxes of energetic electrons up to approximately 300 keV peak near the center of the diffusion region and decrease monotonically away from this region. The diffusion region electron flux spectrum obeys a power law with an index of -3.8 above approximately 2 keV, and the electron angular distribution displays strong field-aligned bidirectional anisotropy at energies below approximately 2 keV, becoming isotropic above approximately 6 keV. These observations indicate significant electron acceleration inside the diffusion region. Ions show no such energization.

摘要

我们报告了“风”号航天器在地球磁尾扩散区罕见穿越期间对高能粒子的直接测量结果。能量高达约300 keV的高能电子通量在扩散区中心附近达到峰值,并从此区域向外单调递减。扩散区电子通量谱在约2 keV以上遵循指数为 -3.8的幂律,并且在能量低于约2 keV时电子角分布呈现出强烈的场向双向各向异性,在能量高于约6 keV时变为各向同性。这些观测结果表明在扩散区内存在显著的电子加速。离子则未表现出这种能量增加。

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