Modeling of Venus, Mars, and Titan

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Modeling of Venus, Mars, and Titan

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 (MH...

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Three-dimensional finite difference time domain modeling of the Schumann resonance parameters on Titan, Venus, and Mars

[1] The conducting ionosphere and conducting surface of Titan, Venus, and Mars form a concentric resonator, which would support the possibility of the existence of global electromagnetic resonances. On Earth, such resonances are commonly referred to as Schumann resonances and are excited by lightning discharges. The detection of such resonances on other planets would give a support for the exis...

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Comparison study of magnetic flux ropes in the ionospheres of Venus, Mars and Titan

0019-1035/$ see front matter 2009 Elsevier Inc. A doi:10.1016/j.icarus.2009.03.014 * Corresponding author. Address: 6862 Slichter Hal Angeles, 595 Charles E. Young Drive East, Los Angeles E-mail address: [email protected] (H.Y. Wei). Magnetic flux ropes are created in the ionosphere of Venus and Mars during the interaction of the solar wind with their ionospheres and also at Titan during the i...

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ژورنال

عنوان ژورنال: Space Science Reviews

سال: 2011

ISSN: 0038-6308,1572-9672

DOI: 10.1007/s11214-011-9814-8