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AGU: Geophysical Research Letters

 

Keywords

  • rings
  • Saturn
  • spokes

Index Terms

  • Atmospheric Processes: Lightning
  • Planetary Sciences: Fluid Planets: Rings and dust
  • Planetary Sciences: Fluid Planets: Atmospheres
  • Planetary Sciences: Fluid Planets: Interactions with particles and fields
  • Planetary Sciences: Solar System Objects: Planetary rings

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 33, L21202, 6 PP., 2006
doi:10.1029/2006GL028146

Formation of Saturn's ring spokes by lightning-induced electron beams

G. H. Jones

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

N. Krupp

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

H. Krüger

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

E. Roussos

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

W.-H. Ip

Institutes of Astronomy and Space Science, National Central University, Chung-li, Taiwan

D. G. Mitchell

Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA

S. M. Krimigis

Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA

J. Woch

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

A. Lagg

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

M. Fränz

Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany

M. K. Dougherty

The Blackett Laboratory, Imperial College London, London, UK

C. S. Arridge

The Blackett Laboratory, Imperial College London, London, UK

H. J. McAndrews

Mullard Space Science Laboratory, Department of Space and Climate Physics, University College London, Dorking, UK

Spokes are near-linear markings sometimes visible on Saturn's rings. They are widely accepted as being electrostatically-levitated sheets of ∼0.6 micron-radius charged grains. Previously-suggested causes of the grains' charging do not agree with all spoke characteristics, which include their rapid generation, localized formation primarily in Saturn's midnight-dawn sector, the seasonality of their apparitions, and, crucially, their morphologies. We contend that spokes are caused by lightning-induced electron beams striking the rings, at locations magnetically-connected to thunderstorms. This view is supported by a semi-quantitative spoke morphology simulation. Spokes' formation locations are further controlled by Saturn's ionospheric density, which reaches a near-dawn minimum where electron beams can most easily propagate to the rings. The beams may generate observed X-ray emission, supply particles to Saturn's radiation belts, and over time will modify the rings' constituents. Finally, we report Cassini MIMI instrument observations of an electron burst which displays some characteristics expected of a lightning-induced event.

Received 12 September 2006; accepted 10 October 2006; published 9 November 2006.

Citation: Jones, G. H., et al. (2006), Formation of Saturn's ring spokes by lightning-induced electron beams, Geophys. Res. Lett., 33, L21202, doi:10.1029/2006GL028146.

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