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Calculation of the upper atmosphere dynamic characteristics from ionospheric data
Conference Proceedings 2000 International Conference on Mathematical Methods in Electromagnetic Theory (Cat. No.00EX413), 2002Calculation of the thermospheric wind vertical component is discussed. Measured values of the vertical plasma drift velocity, charged particles' temperature and parameters of the electron density profile are used in the calculations.
V.I. Taran +3 more
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Mathematical Modeling of Dynamics Processes in the Upper Atmosphere and Ionosphere
2010In this chapter, the achievements of the basic researches on the upper atmosphere and ionosphere processes with the mathematical modeling methods are briefly presented. The mathematical problem of the model atmosphere/ionosphere description, the existing global theoretical model of environment, and the results of the investigations as well as their ...
I. V. Karpov, G. V. Golubkov
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Dynamics investigation in the Venus upper atmosphere
2020The O_2 nightglow emissions in the infrared spectral range are important features to investigate dynamics at the mesospheric altitudes, in the planetary atmosphere. In this work, we analyzed the profiles obtained at limb by the VIRTIS spectrometer on board the Venus Express mission, acquired during the mission period from 2006-07-05 to 2008-08-15 to ...
MIGLIORINI, Alessandra +5 more
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Contributions to the theory of the structure and dynamics of the earth's upper and outer atmosphere
2022The papers bound together here are my pubIished contributions to the theory of the structure and dynamics of the Earth's upper and outer atmosphere. This introduction is intended only as a guide to the areas in which my research has been conducted and as an aid to obtaining an overall view of my work.
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Solar system upper atmospheres: Photochemistry, energetics, and dynamics
2002The physical modeling of most upper atmospheric processes begins with the approximation and solution of one or more of the three primary equations of conservation-mass (i.e., continuity), energy, and momentum. Here we outline the main components of these equations as they relate to the upper atmospheres of the solar system, reviewing the salient ...
G. Randall Gladstone +2 more
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Dynamical implications of the observed thermal contrasts in Venus' upper atmosphere
Icarus, 1982Observational data on the Venusian upper atmosphere are analyzed to determine the dynamical implications of the large pressure change across the terminator, to study the change in diurnal contrast pattern at the 100 km level, and to investigate the viability of the most straightforward explanation of the cooling, radiative emission by CO2 in the 15 ...
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Dynamics of the Upper Atmosphere
Physics Today, 1981Susumu Kato, Samuel H. Francis
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