caa a22 4500 44581585X CHVBK 20180317145228.0 cr unu---uuuuu 170323e20111201xx s 000 0 eng 10.1007/s11214-011-9814-8 doi (NATIONALLICENCE)springer-10.1007/s11214-011-9814-8 Modeling of Venus, Mars, and Titan [Elektronische Daten] [Esa Kallio, Jean-Yves Chaufray, Ronan Modolo, Darci Snowden, Robert Winglee] Increased computer capacity has made it possible to model the global plasma and neutral dynamics near Venus, Mars and Saturn's moon Titan. The plasma interactions at Venus, Mars, and Titan are similar because each possess a substantial atmosphere but lacks a global internally generated magnetic field. In this article three self-consistent plasma models are described: the magnetohydrodynamic (MHD) model, the hybrid model and the fully kinetic plasma model. Chamberlain and Monte Carlo models of the Martian exosphere are also described. In particular, we describe the pros and cons of each model approach. Results from simulations are presented to demonstrate the ability of the models to capture the known plasma and neutral dynamics near the three objects. The Author(s), 2011 Numerical modeling nationallicence Full kinetic model nationallicence Hybrid model nationallicence Magnetohydrodynamic model nationallicence Exosphere model nationallicence Venus nationallicence Mars nationallicence Titan nationallicence Planetary magnetospheres nationallicence Planetary exospheres nationallicence Kallio Esa Finnish Meteorological Institute, Helsinki, Finland aut Chaufray Jean-Yves Laboratoire de Météorologie Dynamique, Institut Pierre Simon Laplace, Centre National de la Recherche Scientifique, Paris, France aut Modolo Ronan Université de Versailles Saint-Quentin, 45 avenue des Etats-Unis, 78035, Versailles cedex, France aut Snowden Darci Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA aut Winglee Robert Department of Earth and Space Sciences, University of Washington, Johnson Hall, Box 351310, 98195-1310, Seattle, WA, USA aut Space Science Reviews Springer Netherlands 162/1-4(2011-12-01), 267-307 0038-6308 162:1-4<267 2011 162 11214 https://doi.org/10.1007/s11214-011-9814-8 text/html Onlinezugriff via DOI 1 review-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/s11214-011-9814-8 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Kallio Esa Finnish Meteorological Institute, Helsinki, Finland aut NATIONALLICENCE 700 1- Chaufray Jean-Yves Laboratoire de Météorologie Dynamique, Institut Pierre Simon Laplace, Centre National de la Recherche Scientifique, Paris, France aut NATIONALLICENCE 700 1- Modolo Ronan Université de Versailles Saint-Quentin, 45 avenue des Etats-Unis, 78035, Versailles cedex, France aut NATIONALLICENCE 700 1- Snowden Darci Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA aut NATIONALLICENCE 700 1- Winglee Robert Department of Earth and Space Sciences, University of Washington, Johnson Hall, Box 351310, 98195-1310, Seattle, WA, USA aut NATIONALLICENCE 773 0- Space Science Reviews Springer Netherlands 162/1-4(2011-12-01), 267-307 0038-6308 162:1-4<267 2011 162 11214 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer