D. E. Ionov
Russian Academy of Sciences
15 Papers
156 Citations
D. E. Ionov is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Planet & Atmosphere. The author has an hindex of 10, co-authored 15 publications.
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Papers
THREE-DIMENSIONAL GAS DYNAMIC SIMULATION OF THE INTERACTION BETWEEN THE EXOPLANET WASP-12b AND ITS HOST STAR
TL;DR: In this article, pure 3D gas dynamic simulations of the plasma interaction between WASP-12b and its host star and describe the flow pattern in the system, showing that the overfilling of the planet's Roche lobe leads to a noticeable outflow from the upper atmosphere in the direction of the and points.
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3D Gas Dynamic Simulation of the Interaction Between the Exoplanet WASP-12b and Its Host Star
TL;DR: In this article, pure 3D gas dynamic simulations of the plasma interaction between WASP-12b and its host star were performed, and the flow pattern in the system was described, showing that the overfilling of the planet's Roche lobe leads to a noticeable outflow from the upper atmosphere in the direction of the L1 and L2 points.
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Heating efficiency in hydrogen-dominated upper atmospheres
TL;DR: In this paper, the thermal-escape-related heating efficiency of the stellar XUV radiation in the hydrogen-dominated upper atmosphere of the extrasolar gas giant HD 209458b was modeled by solving the kinetic Boltzmann equation and applying a Direct Simulation Monte Carlo model.
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Heating efficiency in hydrogen-dominated upper atmospheres
TL;DR: In this article, the thermal-escape-related heating efficiency of the stellar XUV radiation in the hydrogen-dominated upper atmosphere of the extrasolar gas giant HD 209458b was modeled by solving the kinetic Boltzmann equation and applying a Direct Simulation Monte Carlo model.
Influence of Photoelectrons on the Structure and Dynamics of the Upper Atmosphere of a Hot Jupiter
TL;DR: A self-consistent, aeronomic model of the upper atmosphere of a hot Jupiter including reactions involving suprathermal photoelectrons is presented in this paper, which is used to compute the height profiles of the gas density, velocity, and temperature in the atmosphere of the exoplanet HD 209458b.
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