Vertical structure of Jupiter's Oval BA before and after it reddened: What changed?

Details Vertical structure of Jupiter's Oval BA before and after it reddened: What changed? Vertical structure of Jupiter's Oval BA before and after it reddened: What changed?

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..215..211w&link_type=abstract

Icarus, Volume 215, Issue 1, p. 211-225.

Physics

Scientific paper

The reflectivity of haze above Oval BA and its progenitors was constant from 1994 to 2008. Velocity fields of Oval BA in 2000, 2006, and 2009 are identical to within uncertainties. Static stability varies with altitude and constrains the vertical extent of vortices. Oval BA and the Great Red Spot extend down to a level where water in supersolar abundance condenses. Oval BA's color change is consistent with a small undetected global or hemispherical temperature rise.

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