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    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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