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Modelling the North-Pole hexagon of Saturn using a supersymmetric wave-equation
Uppsala University, Science for Life Laboratory, SciLifeLab. Uppsala University, Disciplinary Domain of Science and Technology, Biology, Department of Cell and Molecular Biology, Computational Biology and Bioinformatics. Fjordforsk A/S, Midtun, Vangsnes, Norway.ORCID iD: 0000-0003-4240-513x
A&E Trounev IT Consulting.
2019 (English)Report (Other academic)
Abstract [en]

Planetary atmospheric dynamics is a critical part of astrophysics, which aids in understanding the fluctuations in the atmosphere on other planets as well as planet Earth. Saturn has been known to display a peculiar behaviour on its North Pole, forming a hexagonal geometry in the atmosphere, driven by high-speed winds. Several models have been published over the last 40 years describing its structure and dynamics. Here we use a supersymmetric Hamiltonian originally developed for quantized systems to describe the hexagonal shape on Saturns North Pole. The hexagon is analyzed numerically and its properties are discussed. The results here are important by two aspects, the use of quantum operators to describe continuum phenomena and the novel results which are here reported on the dynamical properties of Saturn's hexagon.

Place, publisher, year, edition, pages
Vangsnes, 2019.
Keywords [en]
Saturn, hexagon, vorticity, model
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Astronomy with specialization in Astrophysics
Identifiers
URN: urn:nbn:se:uu:diva-392030DOI: 10.13140/RG.2.2.25077.52963OAI: oai:DiVA.org:uu-392030DiVA, id: diva2:1346514
Projects
Modeling of quantum vorticity and turbulence in two- and three-dimensional systems.Available from: 2019-08-28 Created: 2019-08-28 Last updated: 2019-09-02Bibliographically approved

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Manzetti, Sergio

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