Moist convection and the 2010–2011 revival of Jupiter's South Equatorial Belt
The transformation of Jupiter's South Equatorial Belt (SEB) from its faded, whitened state in 2009-2010 (Fletcher et al., 2011b) to its normal brown appearance is documented via comparisons of thermal-infrared (5–20 µm) and visible-light imaging between November 2010 and November 2011. The SEB...
| Main Authors: | , , , , , , |
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| Format: | Journal article |
| Published: |
Elsevier
2017
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