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Mutual position of drift trajectories and projections of geomagnetic latitudes in the magnetosphere

机译:磁层中漂移轨迹和地磁纬度投影的相互位置

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We have used the magnetic field model developed by Ostapenko and Maltsev (J. Geophys. Res. 102(A8), 17,467-17,473 1997) for calculations of the drift trajectories of the charged particles and for mapping geomagnetic latitudes and longitudes to the equatorial plane of the magnetosphere under various geomagnetic conditions. The model is valid for distances from 3 to 10 R-E. It depends on the Dst and Kp-indices, solar wind pressure, IMF vertical component and tilt angle of the Earth dipole. The model provides better agreement with measurements than previous ones. (C) 1999 Elsevier Science Ltd. All rights reserved. [References: 16]
机译:我们使用了由Ostapenko和Maltsev开发的磁场模型(J. Geophys。Res。102(A8),17,467-17,473 1997)来计算带电粒子的漂移轨迹,并将地磁纬度和经度映射到赤道面。在各种地磁条件下的磁层厚度该模型对3到10 R-E的距离有效。它取决于Dst和Kp指数,太阳风压,IMF垂直分量和地球偶极子的倾斜角。与以前的模型相比,该模型提供了更好的测量一致性。 (C)1999 Elsevier ScienceLtd。保留所有权利。 [参考:16]

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