Search Results - "Hansen, Kenneth C"

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    Statistical validation of a solar wind propagation model from 1 to 10 AU by Zieger, Bertalan, Hansen, Kenneth C.

    “…A one‐dimensional (1‐D) numerical magnetohydrodynamic (MHD) code is applied to propagate the solar wind from 1 AU through 10 AU, i.e., beyond the heliocentric…”
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    Magnetospheric configuration and dynamics of Saturn's magnetosphere: A global MHD simulation by Jia, Xianzhe, Hansen, Kenneth C., Gombosi, Tamas I., Kivelson, Margaret G., Tóth, Gabor, DeZeeuw, Darren L., Ridley, Aaron J.

    “…We investigate the solar wind interaction with Saturn's magnetosphere by using a global magnetohydrodynamic simulation driven by an idealized time‐varying…”
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    Three-dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars by Ma, Yingjuan, Nagy, Andrew F., Sokolov, Igor V., Hansen, Kenneth C.

    “…We present the results of model calculations, using our new, four‐species, spherical MHD model. Our results are compared with the relevant and limited…”
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    Monte Carlo modeling of neutral gas and dust in the coma of Comet 1P/Halley by Rubin, Martin, Tenishev, Valeriy M., Combi, Michael R., Hansen, Kenneth C., Gombosi, Tamas I., Altwegg, Kathrin, Balsiger, Hans

    Published in Icarus (New York, N.Y. 1962) (01-06-2011)
    “…► Direct Simulation Monte Carlo model of Comet 1P/Halley’s coupled neutral gas and dust coma. ► In situ measurements as well as remote sensing observations…”
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    An interplanetary shock traced by planetary auroral storms from the Sun to Saturn by Prangé, Renée, Pallier, Laurent, Hansen, Kenneth C, Howard, Russ, Vourlidas, Angelos, Courtin, Régis, Parkinson, Chris

    Published in Nature (04-11-2004)
    “…A relationship between solar activity and aurorae on Earth was postulated long before space probes directly detected plasma propagating outwards from the Sun…”
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    Comparisons between MHD model calculations and observations of Cassini flybys of Titan by Ma, Yingjuan, Nagy, Andrew F., Cravens, Thomas E., Sokolov, Igor V., Hansen, Kenneth C., Wahlund, Jan-Erik, Crary, Frank J., Coates, Andrew J., Dougherty, Michele K.

    “…The Cassini spacecraft passed by Titan on 26 October 2004 (Ta flyby) and 13 December 2004 (Tb flyby). In both cases the Cassini Orbiter entered Titan's…”
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    Three-dimensional multispecies MHD studies of the solar wind interaction with Mars in the presence of crustal fields by Ma, Yingjuan, Nagy, Andrew F., Hansen, Kenneth C., DeZeeuw, Darren L., Gombosi, Tamas I., Powell, K. G.

    “…We present the results of model calculations using a multispecies MHD model of the interaction of the solar wind with Mars. The three ions considered are H+,…”
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    A global model of cometary tail disconnection events triggered by solar wind magnetic variations by Jia, Ying-Dong, Combi, Michael R., Hansen, Kenneth C., Gombosi, Tamas I.

    “…Presented in this paper are the results of a time‐dependent, fully three‐dimensional self‐consistent ideal magneto‐hydrodynamics (MHD) model of disconnection…”
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    Three-dimensional MHD simulations of the magnetosphere of Uranus by Tóth, Gábor, Kovács, Dániel, Hansen, Kenneth C., Gombosi, Tamas I.

    “…We have successfully simulated the magnetosphere of Uranus for the time period of the Voyager 2 flyby in January 1986. On the basis of the Voyager…”
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    Upstream conditions at Mercury during the first MESSENGER flyby: Results from two independent solar wind models by Zieger, Bertalan, Hansen, Kenneth C., Cohen, Ofer, Gombosi, Tamas I., Zurbuchen, Thomas H., Anderson, Brian J., Korth, Haje

    Published in Geophysical research letters (01-05-2009)
    “…The primary goal of this paper is to provide estimates of upstream solar wind plasma conditions at Mercury during the January 2008 MESSENGER flyby, based on…”
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    3-D global MHD model prediction for the first close flyby of Titan by Cassini by Ma, Ying-Juan, Nagy, Andrew F., Cravens, Thomas E., Sokolov, Igor V., Clark, John, Hansen, Kenneth C.

    Published in Geophysical research letters (01-11-2004)
    “…The global features of the interaction between Saturn's magnetospheric plasma flow and Titan's atmosphere/ionosphere are simulated by using a 3‐D,…”
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