高频多普勒探测电离层中来自自然和人为来源的干扰

L. Chernogor, L.S. Kostrov, V. Rozumenko
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引用次数: 0

摘要

在1995年至2000年期间,在2.8兆赫和3.0兆赫两个频率上进行了测量。移动的太阳终端只有在电离层没有其他干扰的情况下才会产生可探测的影响,而且最重要的是,在没有磁暴的情况下。对黎明终结的响应在日出后立即在电离层f区下部开始,那里探测无线电波被反射。高频多普勒雷达对与火箭发射有关的各种过程进行了同一时期的调查。对来自不同发射场(拜科努尔、普列谢茨克、卡纳维拉尔角、库鲁等)的32次发射的观测结果进行了分析。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
HF Doppler probing the disturbances originating in the ionosphere from natural and anthropogenic sources
Measurements were made in 1995 to 2000 at the two frequencies of 2.8 MHz and 3.0 MHz. The moving solar terminator generated detectable effects only in the absence of other disturbances in the ionosphere, and, most of all, in the absence of magnetic storms. The response to the dawn terminator commenced immediately after sunrise in the lower part of the ionospheric F-region where the probing radio waves are reflected. HF Doppler radar investigations of a variety of processes associated with rocket launches were performed over the same period of time. The observations have been analysed of thirty two launches from different cosmodromes (Baikonur, Plesetsk, Cape Canaveral, Kourou, and others).
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