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首页|期刊导航|地球与行星物理(英文)|Wavelike perturbations in Titan's ionosphere and their compositional variation: A preliminary survey of Cassini Ion Neutral Mass Spectrometer measurements

Wavelike perturbations in Titan's ionosphere and their compositional variation: A preliminary survey of Cassini Ion Neutral Mass Spectrometer measurements

ShiQi Wu DanDan Niu WeiQin Sun XiaoShu Wu HaoYu Lu Jun Cui

地球与行星物理(英文)2022,Vol.6Issue(6):522-528,7.
地球与行星物理(英文)2022,Vol.6Issue(6):522-528,7.DOI:10.26464/epp2022045

Wavelike perturbations in Titan's ionosphere and their compositional variation: A preliminary survey of Cassini Ion Neutral Mass Spectrometer measurements

Wavelike perturbations in Titan's ionosphere and their compositional variation: A preliminary survey of Cassini Ion Neutral Mass Spectrometer measurements

ShiQi Wu 1DanDan Niu 2WeiQin Sun 3XiaoShu Wu 3HaoYu Lu 4Jun Cui1

作者信息

  • 1. School of Space and Environment,Beihang University,Beijing 100191,China
  • 2. Institute of Space Science and Applied Technology,Harbin Institute of Technology,Shenzhen 518055,Guangdong,China
  • 3. Planetary Environmental and Astrobiological Research Laboratory(PEARL),School of Atmospheric Sciences,Sun Yat-sen University,Zhuhai 519082,Guangdong,China
  • 4. Center for Excellence in Comparative Planetology,Chinese Academy of Sciences,Hefei 230026,China
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摘要

关键词

Titan/atmospheric gravity waves/ionospheric perturbations/ionospheric composition/Cassini

Key words

Titan/atmospheric gravity waves/ionospheric perturbations/ionospheric composition/Cassini

引用本文复制引用

ShiQi Wu,DanDan Niu,WeiQin Sun,XiaoShu Wu,HaoYu Lu,Jun Cui..Wavelike perturbations in Titan's ionosphere and their compositional variation: A preliminary survey of Cassini Ion Neutral Mass Spectrometer measurements[J].地球与行星物理(英文),2022,6(6):522-528,7.

基金项目

This work is supported by the B-type Strategic Priority Program No.XDB41000000 funded by the Chinese Academy of Sciences and the pre-research projects on Civil Aerospace Technologies No.s D020105 and D020103 funded by China's National Space Administration.The authors also acknowledge support from the National Science Foundation of China through grants 42030201,41904154 and 42104170.The data set used in this work is publicly available at the Planetary Plasma Interactions node of the NASA Planetary Data System public archives(http://ppi.pds.nasa.gov). (http://ppi.pds.nasa.gov)

地球与行星物理(英文)

OACSCDEI

2096-3955

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