Evolution of the ring current energy during May 2-4, 1998 magnetic storm
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概要
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We study the evolution of the ring current energy density during May 2-4, 1998 storm event as measured by Polar CAMMICE/MICS instrument and modelled by proton tracing in the guiding center approximation. Particle data from Polar shows that during the storm main phase protons with medium energies (20-80 keV) contribute more to the total ring current energy than the high energy protons (80-200 keV) whereas during the recovery phase high energies dominate. We trace protons with arbitrary pitch angles numerically in the guiding center approximation taking into account charge-exchange losses. Tracing is performed in the large-scale and smaller-scale time-dependent magnetic and electric field models. We model the substorm activity by several electric field pulses at times of the substorm onsets. It is shown that impulsive electric fields associated with substorms are effective in the proton transport and energization to higher energies more than 100 keV in the storm time ring current.
- 国立極地研究所の論文
著者
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Ejiri Masaki
National Institute of Polar Research
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Korhonen Jussi
University Of Helsinki
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Ebihara Yusuke
National Institute of Polar Research
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Pulkkinen Tuija
Finnish Meteorological Institute Geophysical Research Division
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Ganushkina Natalia
Finnish Meteorological Institute, Geophysical Research Division
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Fritz Ted
Boston University, Department of Astronomy
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Fritz Ted
Boston University Department Of Astronomy
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Ganushkina Natalia
Finnish Meteorological Institute Geophysical Research Division
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