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Comparison of the Results on Precipitation of High-Energy Electrons in the Stratosphere and on Satellites
Cosmic Research ( IF 0.6 ) Pub Date : 2021-02-20 , DOI: 10.1134/s0010952521010020
G. A. Bazilevskaya , A. S. Dyusembekova , M. S. Kalinin , M. B. Krainev , V. S. Makhmutov , A. K. Svirzhevskaya , N. S. Svirzhevsky , Yu. I. Stozhkov , E. A. Tulekov

Abstract—

Energetic electron precipitation (EEP) into the atmosphere is one of the mechanisms of depleting the Earth’s outer radiation belt. Precipitating electrons generate bremsstrahlung that penetrates the stratosphere and is recorded by detectors on balloons. However, these observations can be carried out only when the balloon is located at altitudes higher than ~20 km. The near-Earth POES satellites are constantly recording the fluxes of precipitating electrons in the loss cone, but they move too quickly in the space. In this paper, EEPs are compared on the basis of observations in the stratosphere and on satellites during 2003 and estimates of a number of EEP events at Apatity are obtained, assuming that the radiosonde was continuously located at an altitude higher than 26 km.



中文翻译:

平流层和卫星高能电子沉淀结果的比较

摘要-

进入大气层的高能电子沉淀(EEP)是消耗地球外部辐射带的机制之一。沉淀出的电子产生致辐射,that致辐射穿透平流层,并由探测器记录在气球上。但是,只有在气球位于约20 km以上的高度时才能执行这些观察。近地POES卫星不断记录损耗锥中沉淀电子的通量,但它们在空间中的移动速度太快。在本文中,根据2003年平流层和卫星上的观测结果对EEP进行了比较,并假设无线电探空仪连续位于26 km以上的高度,从而获得了Apatity的许多EEP事件的估计值。

更新日期:2021-02-21
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