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首页> 外文期刊>Radio Science >Observations of fast Faraday polarization fluctuations at VHF and amplitude scintillations at VHF and UHF near the equatorial anomaly crest in the Indian sector
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Observations of fast Faraday polarization fluctuations at VHF and amplitude scintillations at VHF and UHF near the equatorial anomaly crest in the Indian sector

机译:观测印度洋赤道异常波峰附近的VHF处快速的法拉第极化波动以及VHF和UHF处的振幅闪烁

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Simultaneous measurements of fast Faraday polarization fluctuations (FPF's) and amplitude scintillations at 136 MHz during April 1977 to February 1980 and of amplitude scintillations at 136 MHz and 244 MHz during August 1981 to December 1982 made at Calcutta (27° dip subionospheric) have been utilized to investigate the nature of ionospheric irregularities during different seasons near the equatorial anomaly crest in the Indian sector. The irregularities occurring in the equinoxes under high solar activity conditions are found to be responsible for intense VHF/UHF scintillations and FPF's. The June solstice is characterized by irregularities producing slow and moderate to weak VHF scintillations but no significant FPF's and UHF scintillations. The occurrence of FPF's is mostly confined to premidnight hours and reduces significantly with respect to the amplitude scintillation occurrence in postmidnight hours. The results are assessed in terms of the strength of irregularities and the longitudinal behavior of global equatorial scintillation activities.
机译:1977年4月至1980年2月在136 MHz下快速法拉第极化起伏(FPF)和幅度闪烁以及1981年8月至1982年12月在加尔各答(27°垂直电离层)进行了136 MHz和244 MHz幅度闪烁的同时测量。调查印度地区赤道异常波峰附近不同季节电离层异常的性质。发现在高太阳活动条件下在春分点中出现的不规则现象是造成强烈的VHF / UHF闪烁和FPF的原因。六月的冬至的特征是不规则,产生缓慢和中度至弱的VHF闪烁,但没有明显的FPF和UHF闪烁。 FPF的发生主要限于午夜前的时间,并且相对于午夜后的幅度闪烁发生显着减少。根据不规则强度和全球赤道闪烁活动的纵向行为对结果进行评估。

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