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Preliminarily study of Saturn’s upper atmosphere density by observing Cassini plunging via China’s deep space station 被引量:1
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作者 Lue Chen Jin-Song Ping +10 位作者 Xiang Liu Na Wang Jian-Feng Cao Guang-Ming Chen Ming-Yuan Wang Wen-Xiao Li Jian-Hui Zhang Yong-Qiang Chen Shi-Lei Yue song-tao han Jing Sun 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2020年第7期112-116,共5页
When the Cassini spacecraft finally plunged into the Saturnian atmosphere on 2017 September15,China’s deep space telescope pointed to Saturn to observe Cassini and study the Saturnian upper neutral atmosphere.In this... When the Cassini spacecraft finally plunged into the Saturnian atmosphere on 2017 September15,China’s deep space telescope pointed to Saturn to observe Cassini and study the Saturnian upper neutral atmosphere.In this first Chinese Saturnian radio science experiment,X band Doppler velocity radio science data between the deep space telescope and the Cassini spacecraft were obtained.After removing Saturnian and solar gravity effects,Earth rotation effect,the remaining Saturnian atmosphere drag information was retrieved in the Cassini final plunge progress.Saturn’s upper neutral atmosphere mass density profile is approximately estimated based on atmosphere mass density derived principally by real orbit measurement data.Saturn’s upper neutral atmosphere mass density from 76000 km to 1400 km is estimated from the orbit measurement data,the mass density results are about from 1.4×10^-15 kg cm^-3 to 2.5×10^-14 kg cm^-3. 展开更多
关键词 CASSINI SATURN Doppler velocity neutral atmosphere mass density
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