Modeling of VLF network observations due to lower ionospheric perturbation during a solar eclipse
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14 citations
References
483 citations
"Modeling of VLF network observation..." refers methods in this paper
...We modeled the [h′,β ]ecl(lon, lat, t) parameters of 2component exponential Wait’s lower ionospheric model [7] according to the elliptical nature of the penumbral shadow of ASE-2012....
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...So, in this case, Wait’s 2-component exponential ionospheric model [7] is capable to represent it, because it is related with ‘Ne’ and ‘νe’....
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98 citations
"Modeling of VLF network observation..." refers background in this paper
...[3] presented the results of total solar eclipse (TSE) in Europe on 11th Aug 1999....
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...Though for a different eclipse, [3] has shown the same ‘-ve’ anomaly for shorter paths like, GBZ-Cambridge, FTA2-Cambridge etc....
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...But, it was proved at several occasions of short and long propagation path analysis, that 2-component exponential ionospheric model, which is simplified and at the same time approximated, works well [3]....
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...[3] explained them with LWPC analysis....
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92 citations
"Modeling of VLF network observation..." refers methods in this paper
...We choose the daytime ionosphere according to [4, 8, 1], i....
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41 citations
"Modeling of VLF network observation..." refers background in this paper
...According to [6], the first level approximation of ‘linear relationship’ between hecl and βecl , and the obscuration effect works well for VLF-ionosphere interaction modeling....
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14 citations