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    Article

    WSO–UV Project: New Touches

    Abstract—A general description is given of the international (with Russia as the key contributor) project World Space Observatory–Ultraviolet (WSO–UV; in Russian named SPEKTR–UF). The project is aimed at creating...

    B. M. Shustov, M. E. Sachkov, S. G. Sichevsky, R. N. Arkhangelsky in Solar System Research (2021)

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    Article

    Changes in the Martian atmosphere induced by auroral electron precipitation

    Typical auroral events in the Martian atmosphere, such as discrete and diffuse auroral emissions detected by UV spectrometers onboard ESA Mars Express and NASA MAVEN, are investigated. Auroral electron kinetic en...

    V. I. Shematovich, D. V. Bisikalo, J.-C. Gérard, B. Hubert in Solar System Research (2017)

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    Article

    Monte Carlo study of interaction between solar wind plasma and Venusian upper atmosphere

    Isolated events of proton and alpha particle precipitation in the Venusian atmosphere were recorded with the use of the ASPERA-4 analyzer on board the ESA Venus Express spacecraft. Using a Monte Carlo simulati...

    V. I. Shematovich, D. V. Bisikalo, S. Barabash, G. Stenberg in Solar System Research (2014)

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    Article

    Ionization fraction in the thermosphere of the exoplanet HD 209458b

    Dissociation and ionization of hydrogen molecules and ionization of hydrogen atoms due to extreme UV radiation from the parent star are accompanied by the formation of a concurrent photoelectron flux with exce...

    D. E. Ionov, D. V. Bisikalo, V. I. Shematovich, B. Huber in Solar System Research (2014)

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    Article

    Influence of the hot oxygen corona on the satellite drag in the Earth’s upper atmosphere

    Calculation results on the possible influence of the hot oxygen fraction on the satellite drag in the Earth’s upper atmosphere on the basis of the previously developed theoretical model of the hot oxygen geoco...

    V. I. Shematovich, D. V. Bisikalo, S. Krauss, W. Hausleitner in Solar System Research (2011)

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    Chapter

    On Possible Nature of Pre-eclipse Dips in Light Curves of Semi-detached Systems with Steady-state Disks

    In order to explain pre-eclipse dips at phases ∼0.7 in light curves of cataclysmic variables, the hypothesis of the thickening at the outer edge of the accretion disk is usually used. Shock-free nature of the ...

    D. V. Bisikalo, P. V. Kaygorodov in Close Binaries in the 21st Century: New Op… (2006)

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    Chapter

    Numerical Modeling of Mass Transfer in Close Binaries

    The review of gasdynamic models used for the description of the mass exchange in close binaries is presented. Main features of the flow structure are summarized. Special attention is paid to physics of accreti...

    D.V. Bisikalo in Zdeněk Kopal’s Binary Star Legacy (2005)