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机译:热电子加热的重要性泰坦的电离层:与卡西尼T34进行比较飞越
Space and Atmospheric Physics Group, Blackett Laboratory, Imperial College London, London, UK;
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California, USA;
Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USAMullard Space Science Laboratory, University College London, Dorking, UKSwedish Institute of Space Physics, Uppsala, SwedenSouthwest Research Institute, San Antonio, Texas, USADepartment of Physics and Astronomy, University of Kansas, Lawrence, Kansas, USA;
机译:在外部Jovian磁极层中的精力充沛的氧气和硫充电状态:Cassini Jupiter Flyby的见解
机译:T118和T119 Cassini Flybys的泰坦的可变电离层
机译:泰坦(Titan)的冷案档案-卡西尼·惠更斯(Cassini-Huygens)之后的悬而未决的问题
机译:评估Cassini SpaceCraft对低空Titan Flybys Cassini SpaceCraft的每轴推进器控制权
机译:卡西尼(Cassini)/ VIMS在镜面反射下观察了泰坦(Titan)的庞加马雷(Punga Mare)上的粗糙表面
机译:泰坦的磁场签名在Cassini T34 Flyby期间:混合模拟与MAG数据之间的比较
机译:Cassini Titan flybys的操作热控制