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pro vyhledávání: '"Koyena Das"'
Autor:
Koyena Das
In Titan, the two major gases nitrogen (N2) and methane (CH4) are ionized and/or photolyzed at high altitudes by the sunlight and the energetic particles from Saturn's magnetosphere, resulting in rich atmospheric chemistry and a wide variety of carbo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::595f3b1623e72999a1c7656158becd24
Autor:
Thomas Gautier, Joseph Serigano, Koyena Das, Maélie Coutelier, Sarah Hörst, Sandrine Vinatier, Cyril Szopa, Melissa Trainer
More than a decade after the arrival of the Cassini-Huygens mission in Saturn’s system, data returned by the Huygens probe during its descent remain a unique source of in-situ information on the lower atmosphere of Titan. Among the Huygens instrume
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8288269b565155c95efe9e7f53b6b29b
https://doi.org/10.5194/epsc2022-431
https://doi.org/10.5194/epsc2022-431
Introduction With 13 years of observations, the Ion and Neutral Mass Spectrometer (INMS) onboard the Cassini spacecraft has observed the upper atmosphere of Titan through two seasons: winter and spring. The complex atmosphere is mainly composed of N2
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::78c4592e201a9455d4a7e19cda9014b4
https://doi.org/10.5194/epsc2022-479
https://doi.org/10.5194/epsc2022-479
Autor:
Koyena Das, Thomas Gautier, Joseph Serigano, Cyril Szopa, Sarah M. Hörst, Maélie Coutelier, Sandrine Vinatier, Melissa G. Trainer
In Titan, the two major gases - dinitrogen (N2) and methane (CH4) are ionized and/or photolyzed at high altitudes by the sunlight and the energetic particles from Saturn's magnetosphere, resulting in rich atmospheric chemistry and a wide variety of c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0dcb5ed984a86f34ff46fd271a18d0e5
https://doi.org/10.5194/epsc2022-710
https://doi.org/10.5194/epsc2022-710