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The 2010-2011 revival of Jupiter's south equatorial belt : perturbations of temperatures, clouds and composition from infrared observations

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dc.contributor.author Orton, G.
dc.contributor.author Fletcher, L.
dc.contributor.author Yanamandra-Fisher, P.
dc.contributor.author Sanchez-Lavega, A.
dc.contributor.author Perez-Hoyos, S.
dc.contributor.author Baines, K.
dc.contributor.author de Pater, I.
dc.contributor.author Wong, M.
dc.contributor.author Goetz, R.
dc.contributor.author Valkov, S.
dc.contributor.author Greco, J.
dc.contributor.author Edwards, M.
dc.contributor.author Rogers, J.
dc.date.accessioned 2013-10-25T21:28:10Z
dc.date.available 2013-10-25T21:28:10Z
dc.date.issued 2011-10-03
dc.identifier.citation Division for Planetary Science, American Astronomical Society, Nantes, France, October 3, 2011. en_US
dc.identifier.clearanceno 11-2144
dc.identifier.uri http://hdl.handle.net/2014/43931
dc.description.abstract On 2010 November 9, a perturbation appeared in Jupiter’s South Equatorial Belt (SEB), which began a classical “revival” of the SEB, returning the entire axisymmetric region to its normal dark color from its anomalous, light, “faded” state. The early revival is marked by strong upwelling gas at the outbreak location, to the west of which appear alternating clear and cloudy regions. Clear regions are correlated with dark clouds near the outbreak and in a southern retrograding branch but less so in a northern prograding branch. A 5-μm image from 2010 March 1 shows much of the SEB closer to a pre-faded state. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011. en_US
dc.subject Jupiter en_US
dc.subject atmosphere en_US
dc.subject distrubance en_US
dc.subject infrared en_US
dc.title The 2010-2011 revival of Jupiter's south equatorial belt : perturbations of temperatures, clouds and composition from infrared observations en_US
dc.type Preprint en_US


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