A giant thunderstorm on Saturn

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G. Fischer, W.S. Kurth, D.A. Gurnett, P. Zarka, U.A. Dyudina, A.P. Ingersoll, S.P. Ewald, C.C. Porco, A. Wesley, C. Go, M. Delcroix

2011 Nature Vol. 475 Issue 7354 Article Cited by 108 Quartile

Abstract

Lightning discharges in Saturng's atmosphere emit radio waves with intensities about 10,000 times stronger than those of their terrestrial counterparts. These radio waves are the characteristic features of lightning from thunderstorms on Saturn, which last for days to months. Convective storms about 2,000 kilometres in size have been observed in recent years at planetocentric latitude 35° south (corresponding to a planetographic latitude of 41° south). Here we report observations of a giant thunderstorm at planetocentric latitude 35-north that reached a latitudinal extension of 10,000 kilometres-comparable in size to a Great White Spotgabout three weeks after it started in early December 2010. The visible plume consists of high-altitude clouds that overshoot the outermost ammonia cloud layer owing to strong vertical convection, as is typical for thunderstorms. The flash rates of this storm are about an order of magnitude higher than previous ones, and peak rates larger than ten per second were recorded. This main storm developed an elongated eastward tail with additional but weaker storm cells that wrapped around the whole planet by February 2011. Unlike storms on Earth, the total power of this storm is comparable to Saturngtotal emitted power. The appearance of such storms in the northern hemisphere could be related to the change of seasons, given that Saturn experienced vernal equinox in August 2009. © 2011 Macmillan Publishers Limited. All rights reserved.

Affiliations

Space Research Institute, Austrian Academy of Sciences, A-8042 Graz, Schmiedlstrasse 6, Austria; Department of Physics and Astronomy, University of Iowa, 203 Van Allen Hall, Iowa City, IA 52242, United States; Observatoire de Paris-Meudon, 92195 Meudon Cedex, 5 Place Jules Janssen, France; Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, United States; Cassini Imaging Central Laboratory for Operations, Space Science Institute, Boulder, CO 80301, 4750 Walnut Street, United States; Murrumbateman, 2582 NSW, 82 Merryville Drive, Australia; Physics Department, University of San Carlos, Nasipit, Talamban, 6000 Cebu City, Philippines; Commission des Observations Plané Taires, Société Astronomique de France, 31170 Tournefeuilee, 2 rue de l'Ardèche, France