Title of article :
Titanʹs induced magnetosphere Original Research Article
Author/Authors :
S.A. Ledvina، نويسنده , , J.G Luhmann، نويسنده , , S.H. Brecht، نويسنده , , T.E Cravens، نويسنده ,
Issue Information :
دوهفته نامه با شماره پیاپی سال 2004
Pages :
11
From page :
2092
To page :
2102
Abstract :
Titan possesses an extensive atmosphere and ionosphere and no obvious significant intrinsic magnetic field. Its ionosphere directly interacts with the surrounding plasma environment, forming an induced magnetosphere. Titan was located in Saturnʹs outer magnetosphere at the time of the Voyager encounter, where that interaction is subsonic, superAlfvénic and submagnetosonic. We present results on Titanʹs induced magnetosphere from numerical simulations for the Voyager encounter scenario, for other locations around Titanʹs orbit, and for a case when Titanʹs orbit at 20 Saturn radii is outside the magnetosphere. The comparison of Titanʹs induced magnetosphere with other induced magnetospheres at Venus, Mars, and other planetary satellites is briefly considered.
Keywords :
Titanיs induced magnetosphere , Saturnיs magnetosphere , Titan
Journal title :
Advances in Space Research
Serial Year :
2004
Journal title :
Advances in Space Research
Record number :
1129499
Link To Document :
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