The Enigma of Saturn's North-Polar Hexagon
Gerald E. Marsh

TL;DR
This paper explores the mysterious hexagonal shape of Saturn's north pole, proposing it results from a spectrum of Rossby waves influenced by the jet's velocity profile.
Contribution
It introduces a hypothesis that a spectrum of Rossby waves explains the hexagon's shape and discusses the conditions leading to its polygonal form.
Findings
Spectrum of Rossby waves likely causes the hexagon shape
Velocity profile of the jet influences wave formation
Hexagon's shape is a result of wave interactions
Abstract
It has been suggested that the north-polar hexagon found on Saturn is an unusual Rossby wave. If this is to be the case, one must not only explain how a Rossby wave can be hexagonal in shape, albeit with curved corners, but also why it is hexagonal rather than in the form of some other polygon. It is likely that a spectrum of Rossby waves with different amplitudes and wavelengths resulting from the velocity profile of the hexagonal jet is responsible for its shape.
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Taxonomy
TopicsAstro and Planetary Science · Geology and Paleoclimatology Research · Geomagnetism and Paleomagnetism Studies
