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Banded Surface Flow Maintained by Convection in a Model of the Rapidly Rotating Giant Planets

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Science  30 Apr 1993:
Vol. 260, Issue 5108, pp. 661-664
DOI: 10.1126/science.260.5108.661

Article Information

vol. 260 no. 5108 661-664

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History: 
  • Received for publication November 2, 1992
  • Accepted for publication March 18, 1993
  • .

Author Information

  1. Zi-Ping Sun1,
  2. Gerald Schubert2,
  3. Gary A. Glatzmaier3
  1. 1Department of Atmospheric Sciences, University of California, Los Angeles, CA 90024
  2. 2Department of Earth and Space Sciences and the Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90024
  3. 3Earth and Environmental Sciences Division and the Institute of Geophysics and Planetary Physics, Los Alamos National Laboratory, Los Alamos, NM 87545

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