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机译:基于卡西尼数据的泰坦大气主要成分的同位素演化
Space Science and Engineering Division, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA;
Space Science and Engineering Division, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA;
Space Science and Engineering Division, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA;
Space Science and Engineering Division, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA;
Space Science and Engineering Division, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA;
Lunar and Planetary Laboratory, University of Arizona, 1629 East University Boulevard, Tucson, AZ 85721, USA;
Lunar and Planetary Laboratory, University of Arizona, 1629 East University Boulevard, Tucson, AZ 85721, USA,Institut UTINAM, CNRS-UMR 6213, Observatoire de Besancon, BP 1615, 25010 Besancon Cedex, France;
Institut de Physique de Rennes, CNRS, UMR 6251, Universite de Rennes 1, Campus de Beaulieu, 35042 Rennes, France, Ecole Nationale Superieure de Chirnie de Rennes, Campus de Beaulieu, 35700 Rennes, France;
titan; atmospheric evolution; isotopes; atmospheric escape;
机译:基于卡西尼-惠更斯数据的土卫六大气中垂直声速和吸收曲线的模型
机译:卡西尼号上肢测深仪在泰坦大气中的同位素比:低纬和中纬度的co_2
机译:卡西尼号上肢测深仪在泰坦大气中的同位素比值:Hc_3n在北部
机译:钛和氮甲烷的起源和演变:后卡西尼·惠更斯的视角
机译:泰坦高层大气同位素组成的离子和中性质谱:对大气动力学和光化学的影响,以及主要物种在地质时间尺度上的演变。
机译:泰坦和火星大气中氮同位素历史的比较行星学
机译:卡西尼CIRS肢体测验在泰坦大气中的同位素比:低纬度和中纬度的CO2