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Moist convection and the abundance of water in the troposphere of Jupiter
Institution:1. Física Aplicada, Escuela de Ingeniería de Bilbao, Universidad del País Vasco UPV/EHU, Plaza Ingeniero Torres Quevedo, 1, 48013 Bilbao, Spain;2. Astronomical Society of Southern Africa, Centurion, South Africa;3. British Astronomical Association, Burlington House, Piccadilly, London W1J 0DU, UK;4. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA;5. Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719-2395, USA;6. Independent scholar, Stuttgart, Germany;7. Planetario de Pamplona, 31008 Pamplona, Spain;8. Departamento de Ciencias Experimentales, Universidad Europea Miguel de Cervantes, Valladolid, Spain,;9. Departamento de Física Teórica, Atómica y Óptica, Universidad de Valladolid, Valladolid, Spain;10. Center for Integrative Planetary Science, University of California, Berkeley, CA, USA;11. Amateur Astronomical Society of Seltjarnarnes, Seltjarnarnes, Iceland;12. Association of Lunar and Planetary Observers-Japan, Japan;13. Physics Department-University of San Carlos, Cebu City, Philippines;1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;2. British Astronomical Association, London, UK;3. Independent Scholar, Stuttgart, Germany;4. Planetary Science Institute, Tucson, AZ, USA;5. Malin Space Science Systems, San Diego, CA, USA;6. Southwest Research Institute, San Antonio, TX, USA
Abstract:A model for narrow moist convective plumes in the lower troposphere of Jupiter can reconcile the apparent depletion of water in that region of the atmosphere with a near-solar abundance of oxygen throughout the interior.
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