Journal cover Journal topic
Annales Geophysicae An open-access journal of the European Geosciences Union
Ann. Geophys., 32, 1463-1476, 2014
http://www.ann-geophys.net/32/1463/2014/
doi:10.5194/angeo-32-1463-2014
© Author(s) 2014. This work is distributed
under the Creative Commons Attribution 3.0 License.
Regular paper
04 Dec 2014
A possible influence of the Great White Spot on Saturn kilometric radiation periodicity
G. Fischer1,2, S.-Y. Ye2, J. B. Groene2, A. P. Ingersoll3, K. M. Sayanagi4, J. D. Menietti2, W. S. Kurth2, and D. A. Gurnett2 1Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, 8042 Graz, Austria
2Department of Physics and Astronomy, The University of Iowa, 203 Van Allen Hall, Iowa City, Iowa 52242, USA
3Division of Geological and Planetary Sciences, 150-21, California Institute of Technology, Pasadena, California 91125, USA
4Department of Atmospheric and Planetary Sciences, Hampton University, 23 E. Tyler Street, Hampton, Virginia 23668, USA
Abstract. The periodicity of Saturn kilometric radiation (SKR) varies with time, and its two periods during the first 5 years of the Cassini mission have been attributed to SKR from the northern and southern hemisphere. After Saturn equinox in August 2009, there were long intervals of time (March 2010 to February 2011 and September 2011 to June 2012) with similar northern and southern SKR periods and locked SKR phases. However, from March to August 2011 the SKR periods were split up again, and the phases were unlocked. In this time interval, the southern SKR period slowed down by ~ 0.5% on average, and there was a large jump back to a faster period in August 2011. The northern SKR period speeded up and coalesced again with the southern period in September 2011. We argue that this unusual behavior could be related to the so-called Great White Spot (GWS), a giant thunderstorm that raged in Saturn's atmosphere around that time. For several months in 2011, the visible head of the GWS had the same period of ~ 10.69 h as the main southern SKR modulation signal. The GWS was most likely a source of intense gravity waves that may have caused a global change in Saturn's thermospheric winds via energy and momentum deposition. This would support the theory that Saturn's magnetospheric periodicities are driven by the upper atmosphere. Since the GWS with simultaneous SKR periodicity measurements have only been made once, it is difficult to prove a physical connection between these two phenomena, but we provide plausible mechanisms by which the GWS might modify the SKR periods.

Citation: Fischer, G., Ye, S.-Y., Groene, J. B., Ingersoll, A. P., Sayanagi, K. M., Menietti, J. D., Kurth, W. S., and Gurnett, D. A.: A possible influence of the Great White Spot on Saturn kilometric radiation periodicity, Ann. Geophys., 32, 1463-1476, doi:10.5194/angeo-32-1463-2014, 2014.
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Short summary
In this paper we show that the large thunderstorm called the "Great White Spot", which raged for about 9 months in Saturn's troposphere in 2010/2011, was accompanied by changes in the periodicity and phasing of auroral radio emissions. We suggest that the thunderstorm was a source of intense gravity waves causing a global change in Saturn’s ionospheric winds via energy and momentum deposition. This supports the theory that Saturn’s magnetospheric periodicities are driven by the upper atmosphere.
In this paper we show that the large thunderstorm called the "Great White Spot", which raged for...
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