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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Long-period prompt-penetration electric fields derived from CHAMP satellite magnetic measurements
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Long-period prompt-penetration electric fields derived from CHAMP satellite magnetic measurements

机译:从CHAMP卫星磁测量中得出的长时速穿透电场

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摘要

The prompt penetration of the interplanetary electric field to the equatorial ionosphere is conveniently modeled with a frequency-dependent transfer function. However, long-period responses (>3 h) of previously estimated transfer functions differ considerably due to insufficient ionospheric eastward electric field (EEF) data useful for spectral analysis. The EEF derived from the Challenging Minisatellite Payload (CHAMP) satellite provides a new opportunity to reliably estimate the long-period transfer function for the first time. Our objectives in this paper are twofold: first, we analyze the frequency spectra of the equatorial ionospheric eastward electric field for periods greater than 6 h; second, we test the hypothesis that the average prompt-penetration effect lasts less than 3 h after an initial perturbation in the interplanetary electric field (IEF). We find that atmospheric sources dominate the EEF at diurnal frequencies, and its subharmonics and magnetospheric sources dominate the EEF for other frequencies. The CHAMP-derived transfer function has smaller errors than the previous estimates, and we confirm that the average prompt-penetration response of the equatorial ionospheric electric field to a 1 mV/m change in the IEF is negligible after 3 h and up to the maximum analysis period of 32 h. We update our transfer function model with the new data sets and make the filter coefficients available to the scientific community. The transfer function prediction matched reasonably well with the EEF observation in both the South American and Indian sectors. A transfer function model of the prompt-penetration effects, driven by the interplanetary electric field, can be highly beneficial to the real-time specification of the ionosphere. Key Points Prompt penetration of interplanetary electric field to equatorial ionosphereFrequency-dependent transfer function model of prompt penetrationEquatorial ionospheric electric field derived from CHAMP magnetic data
机译:利用与频率有关的传递函数可以方便地对行星际电场迅速穿透到赤道电离层进行建模。但是,由于电离层东向电场(EEF)数据不足,无法用于频谱分析,因此先前估计的传递函数的长时间响应(> 3小时)差异很大。来自具有挑战性的微型卫星有效载荷(CHAMP)卫星的EEF提供了新的机会,可以首次可靠地估算长周期传递函数。本文的目标是双重的:首先,我们分析了赤道电离层东向电场大于6小时的频谱;其次,我们检验了这样一种假设:在行星际电场(IEF)产生初始扰动后,平均快速穿透效应持续不到3小时。我们发现,大气源在昼夜频率主导着EEF,而其次谐波和磁层源在其他频率主导着EEF。 CHAMP衍生的传递函数的误差小于以前的估计,并且我们确认,赤道电离层电场对IEF的1 mV / m变化的平均快速渗透响应在3 h后可以忽略不计。分析时间为32小时。我们使用新的数据集更新了传递函数模型,并使滤波器系数可供科学界使用。在南美和印度,传递函数的预测与EEF的观测值相当吻合。由行星际电场驱动的瞬态渗透效应的传递函数模型对电离层的实时规范非常有用。关键点行星际电场对赤道电离层的快速穿透与频率有关的瞬变穿透函数模型基于CHAMP磁数据的赤道电离层电场

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