Wave acceleration of electrons in the Van Allen radiation belts

被引:511
|
作者
Horne, RB
Thorne, RM
Shprits, YY
Meredith, NP
Glauert, SA
Smith, AJ
Kanekal, SG
Baker, DN
Engebretson, MJ
Posch, JL
Spasojevic, M
Inan, US
Pickett, JS
Decreau, PME
机构
[1] British Antarctic Survey, Cambridge CB3 0ET, England
[2] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
[3] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80303 USA
[4] Augsburg Coll, Dept Phys, Minneapolis, MN 55454 USA
[5] Stanford Univ, STAR Lab, Stanford, CA 94305 USA
[6] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[7] LPCE, F-45071 Orleans, France
基金
英国自然环境研究理事会; 美国国家科学基金会; 美国国家航空航天局;
关键词
D O I
10.1038/nature03939
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Van Allen radiation belts(1) are two regions encircling the Earth in which energetic charged particles are trapped inside the Earth's magnetic field. Their properties vary according to solar activity(2,3) and they represent a hazard to satellites and humans in space(4,5). An important challenge has been to explain how the charged particles within these belts are accelerated to very high energies of several million electron volts. Here we show, on the basis of the analysis of a rare event where the outer radiation belt was depleted and then re-formed closer to the Earth(6), that the long established theory of acceleration by radial diffusion is inadequate; the electrons are accelerated more effectively by electromagnetic waves at frequencies of a few kilohertz. Wave acceleration can increase the electron flux by more than three orders of magnitude over the observed timescale of one to two days, more than sufficient to explain the new radiation belt. Wave acceleration could also be important for Jupiter, Saturn and other astrophysical objects with magnetic fields.
引用
收藏
页码:227 / 230
页数:4
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