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Low-Energy (<200 eV) Electron Acceleration by ULF Waves in the Plasmaspheric Boundary Layer: Van Allen Probes Observation
被引:25
|作者:
Ren, Jie
[1
,2
]
Zong, Q. -G.
[1
]
Miyoshi, Y.
[2
]
Zhou, X. Z.
[1
]
Wang, Y. F.
[1
]
Rankin, R.
[3
]
Yue, C.
[4
,5
]
Spence, H. E.
[6
]
Funsten, H. O.
[7
]
Wygant, J. R.
[8
]
Kletzing, C. A.
[9
]
机构:
[1] Peking Univ, Inst Space Phys & Appl Technol, Beijing, Peoples R China
[2] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi, Japan
[3] Univ Alberta, Dept Phys, Edmonton, AB, Canada
[4] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA USA
[5] Univ Corp Atmospher Res, Boulder, CO USA
[6] Univ New Hampshire, Dept Phys, Inst Earth Oceans & Space, Durham, NH 03824 USA
[7] Los Alamos Natl Lab, Los Alamos, NM USA
[8] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[9] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
基金:
中国国家自然科学基金;
加拿大自然科学与工程研究理事会;
关键词:
CHARGED-PARTICLE BEHAVIOR;
FREQUENCY GEOMAGNETIC-PULSATIONS;
DRIFT MIRROR INSTABILITY;
SOLAR-WIND;
MAGNETIC PULSATIONS;
HYDROMAGNETIC-WAVES;
ALFVEN WAVES;
RING CURRENT;
ION FLUX;
MAGNETOSPHERE;
D O I:
10.1002/2017JA024316
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We report observational evidence of cold plasmaspheric electron (< 200 eV) acceleration by ultralow frequency (ULF) waves in the plasmaspheric boundary layer on 10 September 2015. Strongly enhanced cold electron fluxes in the energy spectrogram were observed along with second harmonic mode waves with a period of about 1 min which lasted several hours during two consecutive Van Allen Probe B orbits. Cold electron (< 200 eV) and energetic proton (10-20 keV) bidirectional pitch angle signatures observed during the event are suggestive of the drift-bounce resonance mechanism. The correlation between enhanced energy fluxes and ULF waves leads to the conclusions that plasmaspheric dynamics is strongly affected by ULF waves. Van Allen Probe A and B, GOES 13, GOES 15, and MMS 1 observations suggest that ULF waves in the event were strongest on the duskside magnetosphere. Measurements from MMS 1 contain no evidence of an external wave source during the period when ULF waves and injected energetic protons with a bump-on-tail distribution were detected by Van Allen Probe B. This suggests that the observed ULF waves were probably excited by a localized drift-bounce resonant instability, with the free energy supplied by substorm-injected energetic protons. The observations by Van Allen Probe B suggest that energy transfer between particle species in different energy ranges can take place through the action of ULF waves, demonstrating the important role of these waves in the dynamical processes of the inner magnetosphere.
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页码:9969 / 9982
页数:14
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