Current collection by a conducting spherical satellite in the ionosphere

V. Chaganti, N. Singh
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Abstract

The current collection by a conducting satellite moving in a magnetized plasma across the Earth's magnetic field was studied by means of numerical simulations. The satellite was assumed to be a conducting sphere. In the low Earth orbit, the satellite moves with an orbital velocity V/sub 0/ approximately=8 km/s perpendicular to the Earth's magnetic field lines. This orbital velocity V/sub 0/ is relative to the plasma. Numerical simulations have been carried out to determine the current collected by the satellite moving in a magnetized plasma. For comparison, simulations for the plasma having no relative motion between the plasma and the satellite have been also carried out. The results from the later simulations agree with the canonical upper bound on the collected current calculated by Parker and Murphy (1967). Results from simulations with the relative drift of 8 km/s show that the collected current by the satellite is appreciably greater than that collected without the relative drift.<>
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电离层中导电球形卫星的电流收集
用数值模拟的方法研究了在磁化等离子体中移动的导电卫星在地球磁场中的电流收集。这颗卫星被假定为一个导电球体。在近地轨道上,卫星以垂直于地球磁力线的轨道速度V/sub /约=8 km/s运行。轨道速度是相对于等离子体的。对卫星在磁化等离子体中运动所收集的电流进行了数值模拟。为了比较,还对等离子体与卫星之间没有相对运动的等离子体进行了模拟。后来的模拟结果与Parker和Murphy(1967)计算的收集电流的规范上限一致。相对漂移为8 km/s时的模拟结果表明,卫星收集的电流明显大于没有相对漂移时收集的电流
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