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机译:卡西尼号测量产生的Titan电离层电导率
Swedish Institute of Space Physics, Box 537, 751 21 Uppsala, Sweden;
Swedish Institute of Space Physics, Box 537, 751 21 Uppsala, Sweden;
Swedish Institute of Space Physics, Box 537, 751 21 Uppsala, Sweden;
Swedish Institute of Space Physics, Box 537, 751 21 Uppsala, Sweden, Centre d'Etude des Environments Terrestre et Planetaires, 10-12 Avenue de Yeurope, 78140 Velizy, France;
Solar System Mission Division, ESA/ESTEC, Keplerlaan 1, Noordwijk, The Netherlands;
Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA;
Space and Atmospheric Physics Croup, Imperial College London, Prince Consort Road, London SW7 2BW, UK;
Swedish Institute of Space Physics, Box 537, 751 21 Uppsala, Sweden, Vniversite de Toulouse (UPS), Toulouse, France, CESR (Centre d'Etude Spatiale des Rayonnements), CNRS, UMR 5187, Toulouse, France;
Space and Atmospheric Physics Croup, Imperial College London, Prince Consort Road, London SW7 2BW, UK;
titan; ionosphere; cassini; conductivity; dynamo region; electrodynamical coupling;
机译:泰坦电离层中冷等离子体的卡西尼测量
机译:卡西尼号在距泰坦很远的地方对电离层光电子的观测:对泰坦的大气层环境和磁尾的影响
机译:Cassini无线电暗层泰坦电离层的观察:全套电子密度型材
机译:结合Cassini雷达的结合使用活性和被动测量来表征泰坦形态学
机译:在封闭源中性模式下,通过卡西尼离子中性质谱仪测量分析泰坦的中性上层大气。
机译:卡西尼号观测显示暗淡的泰坦
机译:卡西尼号在距泰坦很远的地方对电离层光电子的观测:对泰坦大气圈环境和磁尾的影响
机译:预测Cassini-Huygens重力测量值是土卫六对土星吸引力的响应的函数