0
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: not found
      • Article: not found

      Heat balance in Titan's atmosphere

      , , , , ,
      Planetary and Space Science
      Elsevier BV

      Read this article at

      ScienceOpenPublisher
      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Related collections

          Most cited references15

          • Record: found
          • Abstract: not found
          • Article: not found

          A model of Titan's aerosols based on measurements made inside the atmosphere

            Bookmark
            • Record: found
            • Abstract: found
            • Article: not found

            Titan's Atmospheric Temperatures, Winds, and Composition

            F Flasar (2005)
            Temperatures obtained from early Cassini infrared observations of Titan show a stratopause at an altitude of 310 kilometers (and 186 kelvin at 15 degrees S). Stratospheric temperatures are coldest in the winter northern hemisphere, with zonal winds reaching 160 meters per second. The concentrations of several stratospheric organic compounds are enhanced at mid- and high northern latitudes, and the strong zonal winds may inhibit mixing between these latitudes and the rest of Titan. Above the south pole, temperatures in the stratosphere are 4 to 5 kelvin cooler than at the equator. The stratospheric mole fractions of methane and carbon monoxide are (1.6 +/- 0.5) x 10(-2) and (4.5 +/- 1.5) x 10(-5), respectively.
              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              Gaseous abundances and methane supersaturation in Titan's troposphere

                Bookmark

                Author and article information

                Journal
                Planetary and Space Science
                Planetary and Space Science
                Elsevier BV
                00320633
                April 2008
                April 2008
                : 56
                : 5
                : 648-659
                Article
                10.1016/j.pss.2007.10.012
                c5246d61-c052-4eea-b1e5-6b7a84214f87
                © 2008

                http://www.elsevier.com/tdm/userlicense/1.0/

                History

                Comments

                Comment on this article