Numerical study on plasma dynamics in the Earth magnetosphere in association with characteristic distributions of aurora and field-aligned currents
Numerical study on plasma dynamics in the Earth magnetosphere in association with characteristic distributions of aurora and field-aligned currents
批准号:
07804029
负责人:
YAMAMOTO Takashi
金额:
$1.34万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
1995
资助国家:
日本
项目状态:
已结题
起止时间:
1995 至 1997
中文摘要
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英文摘要
So far, the theoretical models for the earth magnetosphere have normally assumed that the distribution of auroral particles with kinetic energies of 1-10 keV is uniform, in terms of the flux tube content, over the auroralzone. This implies that no charge separation occurs in that region, despite of the remarkable activity of aurora, and that boundary processes such as viscous interaction and magnetic reconnection play important roles in the auroral activity and production of region 1 field-aligned currents (FACs). We propose a new paradogm that during a period of southward interplanetary magnetic field (IMF), the so-called plasma 'torus' with plasma concentration on the auroral oval can be formed due to particle escape along the open field lines, and that distortion of the torus configuration by the two-cell convection results in the generaation of the region 1 and region 2 FACs. The plasma torus had been assumed to be absolutely interchange-unstable, and thus it had not been considered as a realistic distribution of the magnetospheric plasma. However, if reversal of the magnetic drift direction across the open-close boundary is taken into account, one can expect that the whole configuration of the torus can be maintained while the interchange instability occurs locally inside it. Our theory predicts that various phenomena such as production of region 0,1 and 2 FACs and formations of discrete aurora and omega band structure are interpreted as results of active behavior of the plasma torus which is "metabolized" through the processes of plasma flow into the tours from the solar wind the plasma escape. The purpose of our numerical simulation is to reproduce the metabolized torus as well as those auroral phenomena. Recently we have obtained the simulation results of the region 0,1 and 2 FACs and the formation of auroral omega band, which are consistent with the satellite servations.
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T.Yamamoto: "A theory for generation of the paired region 1 and region 2 field-aligned currents" J.Geophys. Res.102, A2. 27199-27222 (1996)
T.Yamamoto:“生成配对区域 1 和区域 2 场对准电流的理论”J.Geophys。
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T.Yamamoto: "Quasi-steady production of region 1 and region 2 field-aligned currents" Prod.NIPR Symp.Upper Atmos.Phys.11. 108-123 (1998)
T.Yamamoto:“区域 1 和区域 2 场对准电流的准稳定产生”Prod.NIPR Symp.Upper Atmos.Phys.11。
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T.Yamamoto: "Formation of auroral omega bands in the paired region 1 and region 2 field-aligned current system" J.Geophys. Res.101, A12. 2571-2544 (1997)
T.Yamamoto:“在配对的区域 1 和区域 2 场对准电流系统中极光欧米茄带的形成”J.Geophys。
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T.Yamamoto: "A theory for generation of the paired region 1 and region 2 field-aligned currents" J.Geophys.Res.101 A12. 27199-27222 (1996)
T.Yamamoto:“生成配对区域 1 和区域 2 场对准电流的理论”J.Geophys.Res.101 A12。
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T.Yamamoto: "Numerical study on dynamics and polarization of the hot plasma torus in the magneto-sphere:cause of generation of the paired region 1 and region 2 field-aligned currents" J.Geomag.Geoelectr.49,7. 879-922 (1997)
T.Yamamoto:“磁层中热等离子体环面动力学和极化的数值研究:成对区域 1 和区域 2 场对准电流的生成原因”J.Geomag.Geolectr.49,7。
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