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Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model

Author

Listed:
  • Moritz Heimpel

    (University of Alberta)

  • Jonathan Aurnou

    (UCLA)

  • Johannes Wicht

    (Max Planck Institute for Solar System Research)

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.

Suggested Citation

  • Moritz Heimpel & Jonathan Aurnou & Johannes Wicht, 2005. "Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model," Nature, Nature, vol. 438(7065), pages 193-196, November.
    • Handle: RePEc:nat:nature:v:438:y:2005:i:7065:d:10.1038_nature04208
    DOI: 10.1038/nature04208
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