44
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: not found
      • Article: not found

      Improved general circulation models of the Martian atmosphere from the surface to above 80 km

      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.

          Abstract

          Related collections

          Most cited references65

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

          Turbulence and stress owing to gravity wave and tidal breakdown

          R Lindzen (1981)
            Bookmark
            • Record: found
            • Abstract: not found
            • Article: not found

            Properties and effects of dust particles suspended in the Martian atmosphere

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

              A Quasi-equilibrium Turbulent Energy Model for Geophysical Flows

                Bookmark

                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res.
                American Geophysical Union (AGU)
                01480227
                October 25 1999
                October 25 1999
                : 104
                : E10
                : 24155-24175
                Article
                10.1029/1999JE001025
                3843b413-813f-42fb-a91f-7aabab15c351
                © 1999

                http://doi.wiley.com/10.1002/tdm_license_1.1

                History

                Comments

                Comment on this article