Chemical species in Titan's upper atmosphere observed by Cassini/UVIS stellar occultations
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The archive files contain the line-of-sight abundances and local densities of CH<sub>4</sub>, C<sub>2</sub>H<sub>2</sub>, C<sub>2</sub>H<sub>4</sub>, C<sub>2</sub>H<sub>6</sub>, C<sub>4</sub>H<sub>2</sub>, C<sub>6</sub>H<sub>6</sub>, HCN, HC<sub>3</sub>N, and haze particles in Titan's upper atmosphere retrieved using Cassini/UVIS stellar occultation observations during 18 Titan flybys. These results are shown in Figures 5-10 of the manuscript listed below. Fan, S., Zhao, D., Li, C., Shemansky, D. E., Liang, M. -C., and Yung, Y. L. (2022) Seasonal Variations of Chemical Species in Titan’s Upper Atmosphere. <em>The Planetary Science Journal.</em>
本存档文件包含土卫六（Titan）高层大气中CH₄、C₂H₂、C₂H₄、C₂H₆、C₄H₂、C₆H₆、HCN、HC₃N与霾粒子的视向丰度及局地密度，这些数据是通过18次土卫六飞掠期间卡西尼紫外成像光谱仪（Cassini/UVIS）的恒星掩星观测反演得到的。上述研究结果已在如下所列论文的图5至图10中展示：Fan, S., Zhao, D., Li, C., Shemansky, D. E., Liang, M. -C., and Yung, Y. L. (2022) 土卫六高层大气中化学组分的季节变化. 《行星科学期刊（The Planetary Science Journal）》
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创建时间：
2022-04-17
