Van Allen Probes observation of localized drift resonance between poloidal mode ultra-low frequency waves and 60 keV electrons

被引:123
作者
Claudepierre, S. G. [1 ]
Mann, I. R. [2 ]
Takahashi, K. [3 ]
Fennell, J. F. [1 ]
Hudson, M. K. [4 ]
Blake, J. B. [1 ]
Roeder, J. L. [1 ]
Clemmons, J. H. [1 ]
Spence, H. E. [5 ]
Reeves, G. D. [6 ]
Baker, D. N. [7 ]
Funsten, H. O. [6 ]
Friedel, R. H. W. [6 ]
Henderson, M. G. [6 ]
Kletzing, C. A. [8 ]
Kurth, W. S. [8 ]
MacDowall, R. J. [9 ]
Smith, C. W. [10 ,11 ]
Wygant, J. R. [12 ]
机构
[1] Aerosp Corp, Dept Space Sci, El Segundo, CA 90245 USA
[2] Univ Alberta, Dept Phys, Edmonton, AB, Canada
[3] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[4] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[5] Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA
[6] Los Alamos Natl Lab, Space & Atmospher Sci Grp, Los Alamos, NM USA
[7] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80309 USA
[8] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[9] NASA, Goddard Space Flight Ctr, Solar Syst Explorat Div, Greenbelt, MD 20771 USA
[10] Univ New Hampshire, Dept Phys, Durham, NH 03824 USA
[11] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
[12] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
基金
加拿大自然科学与工程研究理事会;
关键词
drift-resonance; ultra-low frequency; radiation belt electron; radial diffusion; inner magnetosphere; ACCELERATION; PARTICLES;
D O I
10.1002/grl.50901
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We present NASA Van Allen Probes observations of wave-particle interactions between magnetospheric ultra-low frequency (ULF) waves and energetic electrons (20-500 keV) on 31 October 2012. The ULF waves are identified as the fundamental poloidal mode oscillation and are excited following an interplanetary shock impact on the magnetosphere. Large amplitude modulations in energetic electron flux are observed at the same period (approximate to 3 min) as the ULF waves and are consistent with a drift-resonant interaction. The azimuthal mode number of the interacting wave is estimated from the electron measurements to be similar to 40, based on an assumed symmetric drift resonance. The drift-resonant interaction is observed to be localized and occur over 5-6 wave cycles, demonstrating peak electron flux modulations at energies similar to 60 keV. Our observation clearly shows electron drift resonance with the fundamental poloidal mode, the energy dependence of the amplitude and phase of the electron flux modulations providing strong evidence for such an interaction. Significantly, the observation highlights the importance of localized wave-particle interactions for understanding energetic particle dynamics in the inner magnetosphere, through the intermediary of ULF waves.
引用
收藏
页码:4491 / 4497
页数:7
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