中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
THE VARIABILITY OF HCN IN TITAN’S UPPER ATMOSPHERE AS IMPLIED BY THE CASSINI ION-NEUTRAL MASS SPECTROMETER MEASUREMENTS

文献类型:期刊论文

作者Cui,J.1,2; Cao,Y.-T.1; Lavvas,P. P.3; Koskinen,and T. T.4
刊名The Astrophysical Journal Letters
出版日期2016-07-13
卷号826期号:1
关键词planets and satellites: atmospheres planets and satellites: individual (Titan)
ISSN号2041-8205
DOI10.3847/2041-8205/826/1/L5
英文摘要ABSTRACT HCN is an important constituent in Titan’s upper atmosphere, serving as the main coolant in the local energy budget. In this study, we derive the HCN abundance at the altitude range of 960–1400 km, combining the Ion-Neutral Mass Spectrometer data acquired during a large number of Cassini flybys with Titan. Typically, the HCN abundance declines modestly with increasing altitude and flattens to a near constant level above 1200 km. The data reveal a tendency for dayside depletion of HCN, which is clearly visible below 1000 km but weakens with increasing altitude. Despite the absence of convincing anti-correlation between HCN volume mixing ratio and neutral temperature, we argue that the variability in HCN abundance makes an important contribution to the large temperature variability observed in Titan’s upper atmosphere.
语种英语
WOS记录号IOP:2041-8205-826-1-L5
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/36321]  
专题中国科学院国家天文台
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
2.Lunar and Planetary Science Laboratory, Macau University of Science and Technology, Macau, China
3.Groupe de Spectroscopie Moleculaire et Atmospherique, Universite de Reims, Champagne-Ardenne, CNRS UMR F-7331, France
4.Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
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GB/T 7714
Cui,J.,Cao,Y.-T.,Lavvas,P. P.,et al. THE VARIABILITY OF HCN IN TITAN’S UPPER ATMOSPHERE AS IMPLIED BY THE CASSINI ION-NEUTRAL MASS SPECTROMETER MEASUREMENTS[J]. The Astrophysical Journal Letters,2016,826(1).
APA Cui,J.,Cao,Y.-T.,Lavvas,P. P.,&Koskinen,and T. T..(2016).THE VARIABILITY OF HCN IN TITAN’S UPPER ATMOSPHERE AS IMPLIED BY THE CASSINI ION-NEUTRAL MASS SPECTROMETER MEASUREMENTS.The Astrophysical Journal Letters,826(1).
MLA Cui,J.,et al."THE VARIABILITY OF HCN IN TITAN’S UPPER ATMOSPHERE AS IMPLIED BY THE CASSINI ION-NEUTRAL MASS SPECTROMETER MEASUREMENTS".The Astrophysical Journal Letters 826.1(2016).

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来源:国家天文台

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