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Thermosphere-ionosphere coupling in response to recurrent geomagnetic activity

机译:热球-电离层耦合对地磁活动的响应

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The paper presents the global thermosphere-ionosphere response to the high-speed solar wind streams and the subsequent recurrent geomagnetic variations with a period of 9 d during the period of time 1 October 2007-31 March 2009. The COSMIC electron density at fixed heights, as well as the ionospheric parameters f_oF2 and h_mF2, and the two coefficients characterizing the top and bottom side vertical gradients of the electron density profile, are used for investigating the ionospheric 9-d (s=0) wave response. The SABER temperature data are utilized for studying the response of the lower thermosphere to the recurrent auroral heating. The COSMIC and SABER measurements are analyzed by one and the same method where the atmospheric tides and planetary waves which are present in the temperature and electron density measurements are simultaneously extracted from the data. The use of such data analysis approach brings to light additional features of the ionospheric response to a recurrent geomagnetic activity which have not been found before.
机译:本文介绍了在2007年10月1日至2009年3月31日的9 d期间,全球热球-电离层对高速太阳风的响应以及随后的周期性地磁变化。固定高度的COSMIC电子密度电离层参数f_oF2和h_mF2以及表征电子密度分布的上下垂直梯度的两个系数都用于研究电离层9-d(s = 0)的波响应。 SABRE温度数据用于研究下部热层对反复极光加热的响应。 COSMIC和SABRE测量通过一种相同的方法进行分析,其中从数据中同时提取出温度和电子密度测量中存在的大气潮汐和行星波。这种数据分析方法的使用揭示了电离层对周期性地磁活动的响应的其他特征,这些以前从未发现过。

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