同步全球可观测的超短周期脉冲

R. Marchuk, A. Potapov, V. Mishin
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引用次数: 1

摘要

我们研究了脉冲地磁扰动的特性,这些扰动是由日地物理研究所(ISTP SB RAS)的感应磁力计网络和CARISMA项目的加拿大站同步观测到的[Mann, et al, 2008]。我们检测到的脉冲的一个特征是,它们的频率范围(f~ 5-30 Hz)位于两类已知电磁振荡范围的交界处:超低频(ULF)振荡(f< 5-10 Hz)或地磁脉动,以及特低频(ELF)振荡(f~ 30-300 Hz);因此,对5-30赫兹范围的研究很少。这项工作无疑对磁层-电离层-大气系统过程的物理学具有重要意义。利用ISTP站的数据对检测到的脉冲进行了形态学分析。结果,我们获得了脉冲的统计特征,绘制了它们的动态光谱,并确定了一些不寻常的特性,这些特性一方面区分了脉冲型地磁脉冲(Pi1B型的不规则脉冲),另一方面区分了更高频率的ELF和VLF信号(大气、哨声等)。根据这些结果,我们假设所研究的脉冲的一个来源可能是中低纬度地区强雷暴引起的电精灵。利用Wang等(2019)对华北精灵时空固定的研究结果,我们证实了精灵出现后会出现超短周期脉冲。局地和全球雷暴活动被认为是电离层alvsamn谐振器(IAR)的主要激发源之一,它在电离层和磁层的耦合中起着重要的作用。我们感兴趣的脉冲振荡可能是雷暴能量转移到IAR的因素之一,因此在考虑的系统中包括了大气。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Synchronous globally observable ultrashort-period pulses
We have studied the properties of impulsive geomagnetic disturbances, which are observed synchronously at the network of induction magnetometers of the Institute of Solar-Terrestrial Physics (ISTP SB RAS) and Canadian stations of the CARISMA project [Mann, et al., 2008]. A feature of the pulses we detected is that their frequency range (f~5–30 Hz) lies at the junction of the ranges of two known classes of electromagnetic oscillations: ultra-low-frequency (ULF) oscillations (f<5–10 Hz), or geomagnetic pulsations, and extra-low frequency (ELF) oscillations (f~30–300 Hz); therefore, the 5–30 Hz range is poorly studied. The work is of undoubted interest for physics of processes in the magnetosphere–ionosphere–atmosphere system. Morphological analysis of the pulses detected has been carried out using data from ISTP stations. As a result, we obtained statistical characteristics of the pulses, plotted their dynamic spectra, and determined a number of unusual properties that distinguish them, on the one hand, from geomagnetic pulsations of the pulsed type (irregular pulsations of the Pi1B type), and, on the other hand, from higher frequency ELF and VLF signals (atmospherics, whistlers, etc.). On the basis of the results, we have made an assumption that a source of the pulses under study can be electrical sprites caused by powerful thunderstorms at middle and low latitudes. Using the results obtained by Wang, et al. in 2019 on spatial and temporal fixation of sprites in North China, we have confirmed that ultra-short-period pulses occur following the emergence of sprites. Thunderstorm activity, both local and global, is considered to be one of the main sources of excitation of the ionospheric Alfvén resonator (IAR), which plays an important role in coupling the ionosphere and the magnetosphere. The pulsed oscillations of interest may be one of the agents through which the energy of thunderstorms is transferred to IAR, thereby including the atmosphere in the system considered.
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