Polar Lightning and Decadal-Scale Cloud Variability on Jupiter

Author:

Baines Kevin H.12345,Simon-Miller Amy A.12345,Orton Glenn S.12345,Weaver Harold A.12345,Lunsford Allen12345,Momary Thomas W.12345,Spencer John12345,Cheng Andrew F.12345,Reuter Dennis C.12345,Jennings Donald E.12345,Gladstone G. R.12345,Moore Jeffrey12345,Stern S. Alan12345,Young Leslie A.12345,Throop Henry12345,Yanamandra-Fisher Padma12345,Fisher Brendan M.12345,Hora Joseph12345,Ressler Michael E.12345

Affiliation:

1. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena CA 91109, USA.

2. NASA/Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA.

3. The Johns Hopkins University Applied Physics Laboratory, 1110 Johns Hopkins Road, Laurel, MD 20723, USA.

4. Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, USA.

5. Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238. USA.

Abstract

Although lightning has been seen on other planets, including Jupiter, polar lightning has been known only on Earth. Optical observations from the New Horizons spacecraft have identified lightning at high latitudes above Jupiter up to 80°N and 74°S. Lightning rates and optical powers were similar at each pole, and the mean optical flux is comparable to that at nonpolar latitudes, which is consistent with the notion that internal heat is the main driver of convection. Both near-infrared and ground-based 5-micrometer thermal imagery reveal that cloud cover has thinned substantially since the 2000 Cassini flyby, particularly in the turbulent wake of the Great Red Spot and in the southern half of the equatorial region, demonstrating that vertical dynamical processes are time-varying on seasonal scales at mid- and low latitudes on Jupiter.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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