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- W2018776482 abstract "The VHF amplitude scintillations recorded during the period from January 1991 to December 1993 in the declining phase of a solar cycle and April 1998 to December 1999 in the ascending phase of the next solar cycle and from January 2008 to July, 2008 at low latitude station Varanasi (geomag. lat. = 14° 55' N, long. = 154° E, Dip angle = 37.3°, Sub-ionospheric dip = 34°) have been analyzed to study the characteristics of ionospheric irregularities during the active solar and magnetic periods. In this paper, the expression for flux tube integrated linear growth rate of irregularities supposed to be produced through generalized Rayleigh-Taylor instability (GRTI) have been derived. Realistic atmospheric and ionospheric density model inputs are used to compute R-T growth rates for a range of geophysical conditions. The derived parameters of irregularities from scintillation data observed at low latitude are compared with computed values. An attempt is made to produce a model for ionospheric low latitude irregularities." @default.
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- W2018776482 date "2010-02-01" @default.
- W2018776482 modified "2023-10-17" @default.
- W2018776482 title "Modeling of VHF scintillation observed at low latitude" @default.
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- W2018776482 doi "https://doi.org/10.1088/1742-6596/208/1/012065" @default.
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