上层电离层自然和受激辐射的群e观测

A. Yau, H. G. James, G. W. Perry, R. Langley, P. Bernhardt, C. Siefring
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引用次数: 0

摘要

Swarm- e(原CASSIOPE增强型极流探测器,e-POP)于2013年9月发射到椭圆极轨道(325-1500公里,81°倾角),目前已经运行了第六年(也是作为Swarm星座组成部分的第二年)。其科学重点之一是研究上层电离层中无线电波传播和波-等离子体相互作用过程的微物理学[1],利用其无线电科学仪器与地面设施和其他航天器协调进行各种独特的主动实验和被动观测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Swarm-E observations of natural and stimulated emissions in the topside ionosphere
Swarm-E (formerly CASSIOPE Enhanced Polar Outflow Probe, e-POP) was launched in September 2013 into an elliptical polar orbit (325–1500 km, 81° inclination), and is currently in its sixth year of operation (and second year of operation as an integral part of the Swarm constellation). One of its science thrusts is to investigate the microphysics of radio-wave propagation and wave-plasma interaction processes in the topside ionosphere [1], using its trio of radio science instruments to perform a variety of unique active experiments and passive observations in coordination with ground facilities and other spacecraft.
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