中纬度D区极低频信号传播路径地磁暴引起电离层变化的诊断研究

IF 1.7 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
V. Nwankwo, W. Denig, S. Chakrabarti, O. Ogunmodimu, M. P. Ajakaiye, J. Fatokun, Paul I. Anekwe, Omodara E. Obisesan, O. E. Oyanameh, O. V. Fatoye
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引用次数: 2

摘要

摘要我们通过量化位于英国坎布里亚郡(呼号GQD)和德国Rhauderfehn (DHO)的发射机的极低频(VLF)无线电信号的传播特性,并在法国南部(A118)接收到地磁风暴引起的干扰,对中纬度D地区耦合进行了诊断研究。我们将两个传播路径的VLF日振幅表征为五个指标,即日出前平均振幅(MBSR)、正午振幅峰值(MDP)、日落后平均振幅(MASS)、日出终止点(SRT)和日落终止点(SST)。我们分析和监测了多达20次风暴的信号指标变化趋势,以联系可归因于风暴的信号幅度偏差。进一步详细研究了五种风暴及其对信号的影响。结果表明,相对于风暴前水平,风暴日MDP在DHO-A118 (GQD-A118)传播路径上约80%(67%)的事件表现出特征性的减少。MBSR下降约60%(77%),而MASS下降67%(58%)。相反,SRT和SST的幅度分别下降了33%(25%)和47%(42%)。在两种传播路径中,DHO-A118传播路径信号的幅度下降更大,如Nwankwo等人(2016)先前指出的那样。为了更好地了解信号传播路径上电离层的状态以及它如何影响VLF振幅,我们进一步分析了位于发射机附近的电离层探空仪的虚拟高度(h'E, h'F1和h'F2)和临界频率(foE, foF1和foF2)。分析结果表明,在地磁风暴期间,f区临界频率和虚高都有显著的增加和波动。虚拟高度最大的增加发生在德国雷德芬(Rhauderfehn)的DHO发射机附近,表明该地区有强烈的风暴响应,这可能是DHO- a118传播路径上MDP下降较大的原因。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Diagnostic study of geomagnetic storm-induced ionospheric changes over very low-frequency signal propagation paths in the mid-latitude D region
Abstract. We performed a diagnostic study of geomagnetic storm-induced disturbances that are coupled to the mid-latitude D region by quantifying the propagation characteristics of very low-frequency (VLF) radio signals from transmitters located in Cumbria, UK (call sign GQD), and Rhauderfehn, Germany (DHO), and received in southern France (A118). We characterised the diurnal VLF amplitudes from two propagation paths into five metrics, namely the mean amplitude before sunrise (MBSR), the midday amplitude peak (MDP), the mean amplitude after sunset (MASS), the sunrise terminator (SRT) and the sunset terminator (SST). We analysed and monitored trends in the variation of signal metrics for up to 20 storms to relate the deviations in the signal amplitudes that were attributable to the storms. Five storms and their effects on the signals were examined in further detail. Our results indicate that relative to pre-storm levels the storm day MDP exhibited characteristic decreases in about 80 % (67 %) of the events for the DHO-A118 (GQD-A118) propagation path. The MBSR showed decreases of about 60 % (77 %), whereas the MASS decreased by 67 % (58 %). Conversely, the SRT and SST showed amplitude decreases of 33 % (25 %) and 47 % (42 %), respectively. Of the two propagation paths, the amplitude decreases for the DHO-A118 propagation path signal were greater, as previously noted by Nwankwo et al. (2016). To better understand the state of the ionosphere over the signal propagation paths and how it might have affected the VLF amplitudes, we further analysed the virtual heights (h'E, h'F1 and h'F2) and critical frequencies (foE, foF1 and foF2) from ionosondes located near the transmitters. The results of this analysis showed significant increases and fluctuations in both the F-region critical frequencies and virtual heights during the geomagnetic storms. The largest increases in the virtual heights occurred near the DHO transmitter in Rhauderfehn (Germany), suggesting a strong storm response over the region which might account for the larger MDP decrease along the DHO-A118 propagation path.
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来源期刊
Annales Geophysicae
Annales Geophysicae 地学-地球科学综合
CiteScore
4.30
自引率
0.00%
发文量
42
审稿时长
2 months
期刊介绍: Annales Geophysicae (ANGEO) is a not-for-profit international multi- and inter-disciplinary scientific open-access journal in the field of solar–terrestrial and planetary sciences. ANGEO publishes original articles and short communications (letters) on research of the Sun–Earth system, including the science of space weather, solar–terrestrial plasma physics, the Earth''s ionosphere and atmosphere, the magnetosphere, and the study of planets and planetary systems, the interaction between the different spheres of a planet, and the interaction across the planetary system. Topics range from space weathering, planetary magnetic field, and planetary interior and surface dynamics to the formation and evolution of planetary systems.
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