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机译:泰坦电离层的结构:与卡西尼号数据的模型比较
Department of Physics and Astronomy, Malott Hall, University of Kansas, Lawrence, KS 66045, USA;
Department of Physics and Astronomy, Malott Hall, University of Kansas, Lawrence, KS 66045, USA;
Southwest Research Institute, P.O. Drawer 28510, San Antonio, TX 78284, USA;
Lunar and Planetary Laboratory, University of Arizona, P.O. Box 210092, Tucson, AZ 85721, USA;
Laboratoire de Planetologie de Crenoble, BP 53, 38041 Grenoble Cedex, France;
University College London, Mullard Space Sciences Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK;
Swedish Institute of Space Physics, Box 537, SE-751 21 Uppsala, Sweden;
Swedish Institute of Space Physics, Box 537, SE-751 21 Uppsala, Sweden;
Southwest Research Institute, P.O. Drawer 28510, San Antonio, TX 78284, USA;
Southwest Research Institute, P.O. Drawer 28510, San Antonio, TX 78284, USA;
Department of Physics and Astronomy, Malott Hall, University of Kansas, Lawrence, KS 66045, USA;
Department of Physics and Astronomy, Malott Hall, University of Kansas, Lawrence, KS 66045, USA;
titan; ionospheres; atmospheres; chemistry; composition; dayside;
机译:泰坦的电离层组成和结构:卡西尼INMS数据的光化学建模
机译:泰坦电离层的能量学:与卡西尼号数据的模型比较
机译:泰坦电离层中力平衡的研究:卡西尼T5飞越模型/数据比较
机译:建模Cassini-Titan反向散射数据
机译:泰坦高层大气中的日冕形成和加热效率:构造离子,中性和热力结构耦合模型以解释第一个INMS卡西尼号数据。
机译:泰坦白天电离层的光电离建模
机译:泰坦的电离层组成和结构:卡西尼INMS数据的光化学建模