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Title: CHARACTERIZATION OF CLOUDS IN TITAN'S TROPICAL ATMOSPHERE

Journal Article · · Astrophysical Journal (Online)
;  [1];  [2];  [3]; ; ;  [4];  [5];  [6];  [7]
  1. Department of Planetary Sciences, University of Arizona, Tucson, AZ 85719 (United States)
  2. Laboratoire AIM, Universite Paris 7/CNRS/CEA-Saclay, DSM/IRFU/SAp (France)
  3. Laboratoire de Planetologie et Geodynamique, CNRS, UMR-6112, Universite de Nantes, 44000 Nantes (France)
  4. Jet Propulsion Laboratory, Pasadena, CA 91109 (United States)
  5. U.S. Geological Survey, Denver, CO 80225 (United States)
  6. Department of Astronomy, Cornell University, Ithaca, NY (United States)
  7. Institute of Planetary Exploration, Deutsche Zentrum, fuer Luft- und Raumfahrt (Germany)

Images of Titan's clouds, possible over the past 10 years, indicate primarily discrete convective methane clouds near the south and north poles and an immense stratiform cloud, likely composed of ethane, around the north pole. Here we present spectral images from Cassini's Visual Mapping Infrared Spectrometer that reveal the increasing presence of clouds in Titan's tropical atmosphere. Radiative transfer analyses indicate similarities between summer polar and tropical methane clouds. Like their southern counterparts, tropical clouds consist of particles exceeding 5 {mu}m. They display discrete structures suggestive of convective cumuli. They prevail at a specific latitude band between 8 deg. - 20 deg. S, indicative of a circulation origin and the beginning of a circulation turnover. Yet, unlike the high latitude clouds that often reach 45 km altitude, these discrete tropical clouds, so far, remain capped to altitudes below 26 km. Such low convective clouds are consistent with the highly stable atmospheric conditions measured at the Huygens landing site. Their characteristics suggest that Titan's tropical atmosphere has a dry climate unlike the south polar atmosphere, and despite the numerous washes that carve the tropical landscape.

OSTI ID:
21336037
Journal Information:
Astrophysical Journal (Online), Vol. 702, Issue 2; Other Information: DOI: 10.1088/0004-637X/702/2/L105; Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-4357
Country of Publication:
United States
Language:
English

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