Variations of electron density in the regional middle latitude D-region of the ionosphere, conditioned by the morning solar terminator during magnetic storm of the 7–11th of november, 2004

A. M. Gokov, O. F. Tyrnov
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Abstract

The results of experimental investigations by the partial reflection radar of the electron density variations in the middle latitude ionospheric D-region during the morning solar terminator passage in the period of the magnetic storm dated the 7-11th of November, 2004, are presented. There was found the increase of the electron density more than 200% both in the period of the morning solar terminator passage and during tens min after this event. To explain such events a hypothesis concerning electron precipitations from the magnetosphere stimulated by the morning solar terminator is used. There were made estimations of the ionization rate. On the basis of the experimental data of electron density changes over the electron precipitation periods, corresponding fluxes were estimated, being p ≈ (0.6-8.8) 109 m-2 sec-1.
2004年11月7日至11日磁暴期间,以太阳晨光终止为条件的区域中纬度d区电离层电子密度变化
本文介绍了2004年11月7日至11日磁暴期间,利用部分反射雷达对中纬度电离层d区晨昏通过期间电子密度变化的实验研究结果。结果表明,在晨昏结束后的10分钟内,电子密度增加了200%以上。为了解释这类事件,使用了一个关于由早晨太阳终结点刺激的磁层电子沉淀的假设。人们对电离速率做了估计。根据电子沉降周期内电子密度变化的实验数据,估算出相应的通量为p≈(0.6-8.8)109 m-2 sec-1。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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