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Praveen Kandpal Rajbir Kaur R.S. Pandey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):581-592
In this paper parallel flow velocity shear Kelvin-Helmholtz instability has been studied in two different extended regions of the inner magnetosphere of Saturn. The method of the characteristic solution and kinetic approach has been used in the mathematical calculation of dispersion relation and growth rate of K-H waves. Effect of magnetic field (B), inhomogeneity (P/a), velocity shear scale length (), temperature anisotropy (), electric field (E), ratio of electron to ion temperature (), density gradient () and angle of propagation () on the dimensionless growth rate of K-H waves in the inner magnetosphere of Saturn has been observed with respect to . Calculations of this theoretical analysis have been done taking the data from the Cassini in the inner magnetosphere of Saturn in the two extended regions of Rs ~4.60–4.01 and Rs ~4.82–5.0. In our study velocity shear, temperature anisotropy and magnitude of the electric field are observed to be the major sources of free energy for the K-H instability in both the regions considered. The inhomogeneity of electric field, electron-ion temperature ratio, and density gradient have been observed playing stabilizing effect on K-H instability. This study also indicates the effect of the vicinity of icy moon Enceladus on the growth of K-H instability. 相似文献
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Praveen Galav Shweta Sharma Rajesh Pandey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Results pertaining to the latitudinal extent of the ionospheric irregularities in terms of TEC depletions have been presented for the two nights namely; 28 October 2004 and 7 February 2005. This study has been carried out using the GPS–TEC over the Indian low latitude stations, at Udaipur, Hyderabad and Bengaluru. This is probably the first report of simultaneous GPS observation of TEC depletions over different latitudes from the Indian sector. The results show that the amplitude of TEC depletions due to the equatorial spread F may vary with time and the location of the observation. The maximum amplitude of the TEC depletion has been found to be about 30 TECU over Hyderabad. The depletions in TEC are found to be field aligned. 相似文献
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