1991
DOI: 10.1016/0021-9169(91)90091-k
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Disturbances of F-region electron density following solar terminator during the WITS period of 16–20 March 1988

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Cited by 8 publications
(10 citation statements)
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“…The obtained results concerning the LS structure agree with theoretical indications of ST effects (Cot and Teitelbaum, 1980;Somsikov, 1983Somsikov, , 1987Somsikov and Ganguly, 1995;Dungenbaeva and Ganguly, 2004;Antonova et al, 2006) and do not contradict the experimental results obtained by Mishin et al (1991), Beley et al (1995), and Galushko et al (1998Galushko et al ( , 2003. In particular, these results confirm the conclusion by Galushko et al (1998) that ST-generated AGWs can be observed at sunrise better than at sunset (corresponding data will be presented in future publications).…”
Section: Discussionsupporting
confidence: 81%
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“…The obtained results concerning the LS structure agree with theoretical indications of ST effects (Cot and Teitelbaum, 1980;Somsikov, 1983Somsikov, , 1987Somsikov and Ganguly, 1995;Dungenbaeva and Ganguly, 2004;Antonova et al, 2006) and do not contradict the experimental results obtained by Mishin et al (1991), Beley et al (1995), and Galushko et al (1998Galushko et al ( , 2003. In particular, these results confirm the conclusion by Galushko et al (1998) that ST-generated AGWs can be observed at sunrise better than at sunset (corresponding data will be presented in future publications).…”
Section: Discussionsupporting
confidence: 81%
“…The great variety of ST-linked phenomena in the atmosphere has resulted in a number of studies being carried out on the analysis of ionosphere parameter variations obtained by different methods of ionosphere sounding (Bezrodny and Yampolski, 1976;Popov and Yampolski, 1981;Galushko and Yampolski, 1983;Mishin et al, 1991;Drobzhev et al, 1992;Bezotosnyi et al, 1994;Beley et al, 1995;Sobral et al, 1997;Galushko et al, 1998;Hocke and Igarashi, 2002;Galushko et al, 2003). However, virtually all experimental data were obtained using indirect methods for analyzing the spectrum of ionosphere parameter variations, which can result from a number of factors.…”
Section: Introductionmentioning
confidence: 99%
“…This model assumes that ST passage leads to generation of currents in the conductive ionospheric layer, which produce slow magnetic sound waves. A mechanism has also been proposed for transferring the generated ST disturbances along magnetic field lines to another hemisphere [Leonovich et al, 2010]. Further studies have shown that TEC disturbances associated with ST passage may have a more complex structure, as, apparently, a superposition of ionospheric plasma oscillations caused by the influence of not only MHD waves but also of gravity waves.…”
Section: Introductionmentioning
confidence: 99%
“…Earlier studies of ionospheric conditions in the region of ST passage [Hines, 1960;Francis, 1974] have shown that ST passage causes wave generation as well as instabilities and fluctuations in ionospheric plasma. This led to a number of studies of ionospheric parameters during ST passage [Mishin et al, 1991;Somsikov, Ganguly, 1995;Galushko et al, 1998]. …”
Section: Introductionmentioning
confidence: 99%
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