The Interaction between Magnetized Plasma Flow and Unmagnetized Celestial Bodies: Comparison of Mars, Venus and Titan

Details The Interaction between Magnetized Plasma Flow and Unmagnetized Celestial Bodies: Comparison of Mars, Venus and Titan The Interaction between Magnetized Plasma Flow and Unmagnetized Celestial Bodies: Comparison of Mars, Venus and Titan

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010phdt.......188w&link_type=abstract

ProQuest Dissertations And Theses; Thesis (Ph.D.)--University of California, Los Angeles, 2010.; Publication Number: AAT 3446842

Computer Science

Scientific paper

During the interaction of Mars and Venus with the solar wind and Titan with the Saturnian magnetospheric plasma, their ionospheres and atmospheres directly interact with the incoming plasma flow. Comparison studies of the interactions of Mars, Venus and Titan are useful to improve our knowledge of the interaction between magnetized plasma flow and an unmagnetized body with an atmosphere. The comparison studies are done from three aspects in this dissertation: I) atmospheric pickup process and ion cyclotron waves, 2) ionospheric magnetization and flux rope structures, 3) internal moment estimate.

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