The Atmospheric Structure of the Ice Giant Planets from In Situ Measurements by Entry Probes
Résumé
In situ measurements by an atmospheric entry probe allow for sounding and investigating atmospheric composition, structure and dynamics deep into the atmosphere of a Giant planet. In this paper, we describe an Atmospheric Structure Instrument (ASI) for an entry probe at Uranus and/or Neptune. The scientific objectives, the measurements and the expected results are discussed in the framework of a future opportunity for an NASA-ESA joint mission to the Ice Giant planets.
Domaines
Planète et Univers [physics]
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Ferri2020_Article_TheAtmosphericStructureOfTheIc.pdf (1.66 Mo)
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| Origine | Accord explicite pour ce dépôt |
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