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Response of low latitude D-region ionosphere to the total solar eclipse of 22 July 2009 deduced from ELF/VLF analysis

机译:根据ELF / VLF分析得出的低纬度D区电离层对2009年7月22日日全食的响应

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Response of the D-region of the ionosphere to the total solar eclipse of 22 July 2009 at low latitude, Varanasi (Geog. lat., 25.27° N; Geog. long., 82.98° E; Geomag. lat. = 14° 55' N) was investigated using ELF/VLF radio signal. Tweeks, a naturally occurring VLF signal and radio signals from various VLF navigational transmitters are first time used simultaneously to study the effect of total solar eclipse (TSE). Tweeks occurrence is a nighttime phenomena but the obscuration of solar disc during TSE in early morning leads to tweek occurrence. The changes in D-region ionospheric VLF reflection heights (h) and electron density (n_e: 22.6-24.6 cm~(-3)) during eclipse have been estimated from tweek analysis. The reflection height increased from ~89 km from the first occurrence of tweek to about ~93 km at the totality and then decreased to ~88 km at the end of the eclipse, suggesting significant increase in tweek reflection height of about 5.5 km during the eclipse. The reflection heights at the time of totality during TSE are found to be less by 2-3 km as compared to the usual nighttime tweek reflection heights. This is due to partial nighttime condition created by TSE. A significant increase of 3 dB in the strength of the amplitude of VLF signal of 22.2 kHz transmitted from JJI-Japan is observed around the time of the total solar eclipse (TSE) as compared to a normal day. The modeled electron density height profile of the lower ionosphere depicts linear variation in the electron density with respect to solar radiation as observed by tweek analysis also. These low latitude ionospheric perturbations on the eclipse day are discussed and compared with other normal days.
机译:低纬度瓦拉纳西电离层D区对2009年7月22日日全食的响应(地理纬度为25.27°N;地理纬度为82.98°E;地理纬度= 14°55使用ELF / VLF无线电信号调查了N)。 Tweeks首次同时使用自然发生的VLF信号和来自各种VLF导航发射机的无线电信号来研究日全食(TSE)的影响。 Tweek的发生是夜间现象,但在TSE期间清晨太阳盘的遮盖会导致Tweek的发生。根据t周分析,估计了日食期间D区电离层VLF反射高度(h)和电子密度(n_e:22.6-24.6 cm〜(-3))的变化。反射高度从第t周初次出现时的约89 km增加到总共约93 km,然后在日食结束时减小到〜88 km,这表明在月食时tweek反射高度显着增加了约5.5 km。 。与常规夜间tweek反射高度相比,在TSE期间进行总体观测时的反射高度降低了2-3 km。这是由于TSE创建的部分夜间条件造成的。与日相比,在日全食期间,从JJI-Japan传输的22.2 kHz的VLF信号的幅度强度明显增加了3 dB。下部电离层的模拟电子密度高度分布图也描绘了电子密度相对于太阳辐射的线性变化,这也可以通过tweek分析观察到。讨论了日食期间这些低纬度电离层扰动,并将其与其他正常日进行了比较。

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