Persistent Identifier
|
hdl:2014/43931 |
Publication Date
|
2011-10-03 |
Title
| The 2010-2011 revival of Jupiter's south equatorial belt : perturbations of temperatures, clouds and composition from infrared observations |
Author
| Orton, G. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Fletcher, L. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Yanamandra-Fisher, P. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Sanchez-Lavega, A. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Perez-Hoyos, S. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Baines, K. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
de Pater, I. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Wong, M. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Goetz, R. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Valkov, S. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Greco, J. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Edwards, M. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.)
Rogers, J. (Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011.) |
Point of Contact
|
Use email button above to contact.
Orton, G. |
Description
| 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. |
Subject
| Other |
Production Date
| 2011-10-03 |