Global-scale coherence modulation of radiation-belt electron loss from plasmaspheric hiss

被引:87
作者
Breneman, A. W. [1 ]
Halford, A. [2 ]
Millan, R. [2 ]
McCarthy, M. [3 ]
Fennell, J. [4 ]
Sample, J. [5 ]
Woodger, L. [2 ]
Hospodarsky, G. [6 ]
Wygant, J. R. [1 ]
Cattell, C. A. [1 ]
Goldstein, J. [7 ]
Malaspina, D. [8 ]
Kletzing, C. A. [6 ]
机构
[1] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[2] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[3] Univ Washington, Earth & Space Sci, Seattle, WA 98195 USA
[4] Aerosp Corp, Los Angeles, CA 90009 USA
[5] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[6] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[7] SW Res Inst, San Antonio, TX 78238 USA
[8] Univ Colorado, Lab Atmospher & Space Phys LASP, Boulder, CO 80303 USA
关键词
D O I
10.1038/nature14515
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
Over 40 years ago it was suggested that electron loss in the region of the radiation belts that overlaps with the region of high plasma density called the plasmasphere, within four to five Earth radii(1,2), arises largely from interaction with an electromagnetic plasma wave called plasmaspheric hiss(3-5) . This interaction strongly influences the evolution of the radiation belts during a geomagnetic storm, and over the course of many hours to days helps to return the radiation-belt structure to its 'quiet' pre-storm configuration. Observations have shown that the long-term electron-loss rate is consistent with this theory but the temporal and spatial dynamics of the loss process remain to be directly verified. Here we report simultaneous measurements of structured radiation-belt electron losses and the hiss phenomenon that causes the losses. Losses were observed in the form of bremsstrahlung X-rays generated by hiss-scattered electrons colliding with the Earth's atmosphere after removal from the radiation belts. Our results show that changes of up to an order of magnitude in the dynamics of electron loss arising from hiss occur on timescales as short as one to twenty minutes, in association with modulations in plasma density and magnetic field. Furthermore, these loss dynamics are coherent with hiss dynamics on spatial scales comparable to the size of the plasmasphere. This nearly global-scale coherence was not predicted and may affect the short-term evolution of the radiation belts during active times.
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页码:193 / U321
页数:8
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