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Earth-Based Observations of the Galileo Probe Entry Site
Orton G; Ortiz JL; Baines K; Bjoraker G; Carsenty U; Colas F; Dayal A; Deming D; Drossart P; Frappa E; Friedson J; Goguen J; Golisch W; Griep D; Hernandez C; Hoffmann W; Jennings D; Kaminski C; Kuhn J; Laques P; Limaye S; Lin H; Lecacheux J; Martin T; McCabe G; Momary T; Parker D; Puetter R; Ressler M; Reyes G; Sada P; Spencer J; Spitale J; Stewart S; Varsik J; Warell J; Wild W; Yanamandra-Fisher P; Fazio G; Hora J; Deutsch L.
Afiliação
  • Orton G; G. Orton, J. Friedson, T. Martin, P. Yanamandra-Fisher, Mail Stop 169-237, Jet Propulsion Laboratory (JPL), California Institute of Technology, Pasadena, CA 91109; J. L. Ortiz, Mail Stop 169-237, JPL, and Instituto de Astrofisica de Andalucia, CSIC, P.O. Box 3004, 18080 Granada, Spain; K. Baines, Mail Stop 183-601, JPL; G. Bjoraker, D. Deming, D. Jennings, G. McCabe, P. Sada, Code 693, NASA Goddard Space Flight Center, Greenbelt, MD 20771; U. Carsenty, DLR Institute for Planetary Exploration, Ru
Science ; 272(5263): 839-40, 1996 May 10.
Article em En | MEDLINE | ID: mdl-8662571
ABSTRACT
Earth-based observations of Jupiter indicate that the Galileo probe probably entered Jupiter's atmosphere just inside a region that has less cloud cover and drier conditions than more than 99 percent of the rest of the planet. The visual appearance of the clouds at the site was generally dark at longer wavelengths. The tropospheric and stratospheric temperature fields have a strong longitudinal wave structure that is expected to manifest itself in the vertical temperature profile.
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Base de dados: MEDLINE Idioma: En Ano de publicação: 1996 Tipo de documento: Article
Buscar no Google
Base de dados: MEDLINE Idioma: En Ano de publicação: 1996 Tipo de documento: Article