Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model
Moritz Heimpel (),
Jonathan Aurnou and
Johannes Wicht
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Moritz Heimpel: University of Alberta
Jonathan Aurnou: UCLA
Johannes Wicht: Max Planck Institute for Solar System Research
Nature, 2005, vol. 438, issue 7065, 193-196
Abstract:
Catch the wind The characteristic bands in Jupiter's atmosphere are produced by a global system of powerful winds of two basic types: broad eastward equatorial jets, and smaller-scale, higher latitude jets that flow in alternating directions. A new numerical model succeeds where previous models have failed in that it simultaneously generates both of the two dominant zonal wind patterns.
Date: 2005
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Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:438:y:2005:i:7065:d:10.1038_nature04208
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DOI: 10.1038/nature04208
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