2011
DOI: 10.1134/s0016793211060168
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Solar terminator and dynamic phenomena in the atmosphere: A review

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Cited by 36 publications
(31 citation statements)
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“…[], in the transition region between F1 and F2 layers, there exist sharp gradients in electron and ion concentrations due to the different response of F1 and F2 regions to the radiation flux changes induced by the solar terminators and solar eclipses. Somsikov [, ] have confirmed that the narrow region of sharp gradients of temperature, pressure, and density between two states of atmosphere corresponding to the coolings and heatings processes linked with the solar terminators can be the source of AGWs. The scales of AGWs excited by heatings and coolings depend on the scales of the heatings and coolings regions, as well as the time duration of the heatings and coolings processes [ Vadas and Fritts , ; Vadas , ].…”
Section: Resultsmentioning
confidence: 99%
“…[], in the transition region between F1 and F2 layers, there exist sharp gradients in electron and ion concentrations due to the different response of F1 and F2 regions to the radiation flux changes induced by the solar terminators and solar eclipses. Somsikov [, ] have confirmed that the narrow region of sharp gradients of temperature, pressure, and density between two states of atmosphere corresponding to the coolings and heatings processes linked with the solar terminators can be the source of AGWs. The scales of AGWs excited by heatings and coolings depend on the scales of the heatings and coolings regions, as well as the time duration of the heatings and coolings processes [ Vadas and Fritts , ; Vadas , ].…”
Section: Resultsmentioning
confidence: 99%
“…While solar occultation measurements across the terminator region can provide good vertical resolution, these measurements have very limited horizontal (LT) resolution. Somsikov (2011) provides the most recent review of theoretical and experimental work on the subject, including much smaller-scale inhomogeneities and waves associated with the terminator in both the neutral atmosphere and ionosphere. Forbes and Moudden (2009) used a high-resolution general circulation model to reveal TW in Mars' lower and upper atmosphere and achieved similar results and conclusions as Miyoshi et al (2009).…”
Section: Geophysical Research Lettersmentioning
confidence: 99%
“…The first two terms in Eq.7 correspond to the description of atmospheric perturbation in the linear approach [7]. These terms are responsible for acoustic-gravity wave's generation in the equilibrium atmosphere.…”
Section: The First Step To Grsmentioning
confidence: 99%
“…The interaction solar radiation with atmospheric gas in the ST region in some cases can lead to instability [8,18]. The mechanism of this instability is caused by the gradient of the solar radiation absorption coefficient during sunrise.…”
Section: The Linear Model Of the Atmosphereic Disturbances Generated mentioning
confidence: 99%
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