Abstract
This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan’s atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn’s famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter.
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Owen, T., Gautier, D. (2003). Touring the Saturnian System: The Atmospheres of Titan and Saturn. In: Russell, C.T. (eds) The Cassini-Huygens Mission. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3251-2_9
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