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Nonstorm time scattering of ring current protons by electromagnetic ion cyclotron waves
被引:50
作者:
Xiao, Fuliang
[1
,2
]
Yang, Chang
[1
]
Zhou, Qinghua
[1
]
He, Zhaoguo
[1
]
He, Yihua
[1
]
Zhou, Xiaoping
[1
]
Tang, Lijun
[1
]
机构:
[1] Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha 410004, Hunan, Peoples R China
[2] Chinese Acad Sci, State Key Lab Space Weather, Beijing, Peoples R China
基金:
中国国家自然科学基金;
关键词:
RADIATION BELT ELECTRONS;
QUASI-LINEAR DIFFUSION;
PITCH-ANGLE SCATTERING;
LOSS-CONE DISTRIBUTION;
MAGNETIC STORM;
GEOMAGNETIC STORMS;
SOLAR-WIND;
GEOSYNCHRONOUS ORBIT;
ENERGETIC PARTICLES;
STOCHASTIC ACCELERATION;
D O I:
10.1029/2012JA017922
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We report correlated observation of enhanced electromagnetic ion cyclotron (EMIC) waves and dynamic evolution of ring current proton flux collected by Cluster satellite near the location L = 4.5 during March 26-27, 2003, a nonstorm period (D-st > -10). Energetic (5-30 keV) proton fluxes are found to drop rapidly (e.g., a half hour) at lower pitch angles, corresponding to intensified EMIC wave activities. By adopting a Gaussian fit to the observed spectra of EMIC waves, we present two-dimensional (2D) numerical simulations which demonstrate that EMIC wave can yield such decrements in proton flux within 30 minutes, consistent with the observational data. The current result provides a further understanding of ring current dynamics driven by wave-particle interaction under different geomagnetic activities.
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页数:8
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