Composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini‐Huygens probe gas chromatograph mass spectrometer experiment

By H. Niemann, S. Atreya, J. Demick, D. Gautier, J. Haberman, D. Harpold, W. Kasprzak, Jonathan I. Lunine, T. Owen, F. Raulin. 2010

392 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Ecology

View Paper: https://www.semanticscholar.org/paper/c02af9f60f906e041d8420a3591f065ebe7c2aee

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Citations in the corpus

• Cryovolcanism on Titan: New results from Cassini RADAR and VIMS (2013, methodology): “The gas chromatograph mass spectrometer instrument on the Huygens probe detected the radiogenic isotope 40Ar in Titan’s atmosphere [Niemann et al., 2005, 2010].”
• Ice structures, patterns, and processes: A view across the icefields (2012, background): “For example, it has been argued (Sohl et al., 2002) that the interior of Jupiter’s moon Ganymede could consist of successive layers of ices Ih, III, V and VI. Similarly, the other largest icy Solar System moons, Callisto and Titan, might have ice VI in their depths, and layers of other ice phases in”