Titan's ionosphere: Model comparisons with Cassini Ta Data

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33901

Title:	Titan's ionosphere: Model comparisons with Cassini Ta Data
Authors:	Cravens,TE;Robertson,IP;Clark,J;Wahlund,JE;Waite,JH;Ledvina,SA;Niemann,HB;Yelle,RV;Kasprzak,WT;Luhmann,JG;McNutt,RL;Ip,WH;De La Haye,V;Muller-Wodarg,I;Young,DT;Coates,AJ
Contributors:	天文研究所
Keywords:	UPPER-ATMOSPHERE;MHD MODEL;PLASMA;MAGNETOSPHERE;SIMULATION
Date:	2005
Issue Date:	2010-07-07 11:52:50 (UTC+8)
Publisher:	中央大學
Abstract:	[ 1] On October 26, 2004, during its first encounter with Titan ( Ta), the Cassini Orbiter moved from the dayside to the nightside with a closest approach altitude of 1174 km. In situ measurements of the main part of Titan's ionosphere were made by the La
Relation:	GEOPHYSICAL RESEARCH LETTERS
Appears in Collections:	[天文研究所] 期刊論文

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