A dynamo driven by zonal jets at the upper surface in the giant planets

Details A dynamo driven by zonal jets at the upper surface in the giant planets A dynamo driven by zonal jets at the upper surface in the giant planets

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1511g&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1511

Physics

Scientific paper

A dynamo mechanism explains the dipolar magnetic field of Jupiter and
the multipolar magnetic field of Neptune in terms of the width of the
zonal jet streams observed at their surfaces.

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