Electron Acceleration in the Heart of the Van Allen Radiation Belts

被引:495
作者
Reeves, G. D. [1 ]
Spence, H. E. [2 ]
Henderson, M. G. [1 ]
Morley, S. K. [1 ]
Friedel, R. H. W. [1 ]
Funsten, H. O. [1 ]
Baker, D. N. [3 ]
Kanekal, S. G. [4 ]
Blake, J. B. [5 ]
Fennell, J. F. [5 ]
Claudepierre, S. G. [5 ]
Thorne, R. M. [6 ]
Turner, D. L. [7 ]
Kletzing, C. A. [8 ]
Kurth, W. S. [8 ]
Larsen, B. A. [1 ]
Niehof, J. T. [1 ]
机构
[1] Los Alamos Natl Lab, Space Sci & Applicat Grp, Los Alamos, NM 87545 USA
[2] Univ New Hampshire, Each Inst Study Earth Oceans & Space, Durham, NH 03824 USA
[3] Univ Colorado, Lab Atmospher & Space Res, Boulder, CO 80309 USA
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[5] Aerosp Corp, El Segundo, CA 90245 USA
[6] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
[7] Univ Calif Los Angeles, Dept Earth & Space Sci, Los Angeles, CA 90095 USA
[8] Univ Iowa, Dept Phys, Iowa City, IA 52242 USA
关键词
RELATIVISTIC ELECTRONS; ULF; ENERGIZATION; STORM; CHORUS; POWER;
D O I
10.1126/science.1237743
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 contain ultrarelativistic electrons trapped in Earth's magnetic field. Since their discovery in 1958, a fundamental unanswered question has been how electrons can be accelerated to such high energies. Two classes of processes have been proposed: transport and acceleration of electrons from a source population located outside the radiation belts (radial acceleration) or acceleration of lower-energy electrons to relativistic energies in situ in the heart of the radiation belts (local acceleration). We report measurements from NASA's Van Allen Radiation Belt Storm Probes that clearly distinguish between the two types of acceleration. The observed radial profiles of phase space density are characteristic of local acceleration in the heart of the radiation belts and are inconsistent with a predominantly radial acceleration process.
引用
收藏
页码:991 / 994
页数:4
相关论文
共 31 条
[21]   On the origin of relativistic electrons in the magnetosphere associated with some geomagnetic storms [J].
Rostoker, G ;
Skone, S ;
Baker, DN .
GEOPHYSICAL RESEARCH LETTERS, 1998, 25 (19) :3701-3704
[22]   Resonant enhancement of relativistic electron fluxes during geomagnetically active periods [J].
Roth, I ;
Temerin, M ;
Hudson, MK .
ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, 1999, 17 (05) :631-638
[23]  
Schulz M., 1974, Physics and Chemistry in Space, DOI DOI 10.1007/978-3-642-65675-0
[24]   On the source location of radiation belt relativistic electrons [J].
Selesnick, RS ;
Blake, JB .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2000, 105 (A2) :2607-2624
[25]   Radiation belt electron observations following the January 1997 magnetic cloud event [J].
Selesnick, RS ;
Blake, JB .
GEOPHYSICAL RESEARCH LETTERS, 1998, 25 (14) :2553-2556
[26]   Review of modeling of losses and sources of relativistic electrons in the outer radiation belt II: Local acceleration and loss [J].
Shprits, Yuri Y. ;
Subbotin, Dmitriy A. ;
Meredith, Nigel P. ;
Elkington, Scot R. .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2008, 70 (14) :1694-1713
[27]   Model of the energization of outer-zone electrons by whistler-mode chorus during the October 9, 1990 geomagnetic storm [J].
Summers, D ;
Ma, C ;
Meredith, NP ;
Horne, RB ;
Thorne, RM ;
Heynderickx, D ;
Anderson, RR .
GEOPHYSICAL RESEARCH LETTERS, 2002, 29 (24)
[28]   Relativistic theory of wave-particle resonant diffusion with application to electron acceleration in the magnetosphere [J].
Summers, D ;
Thorne, RM ;
Xiao, FL .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1998, 103 (A9) :20487-20500
[29]   Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms [J].
Tsyganenko, NA ;
Sitnov, MI .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2005, 110 (A3)
[30]   Impact of ULF oscillations in solar wind dynamic pressure on the outer radiation belt electrons [J].
Ukhorskiy, AY ;
Anderson, BJ ;
Takahashi, K ;
Tsyganenko, NA .
GEOPHYSICAL RESEARCH LETTERS, 2006, 33 (06)