Precession of Uranus and Neptune and their magnetic field

Details Precession of Uranus and Neptune and their magnetic field Precession of Uranus and Neptune and their magnetic field

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..419d&link_type=abstract

In Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F p 419-420 (SEE N94-12015 01-91)

Physics

Angular Velocity, Dynamo Theory, Neptune (Planet), Planetary Magnetic Fields, Precession, Uranus (Planet), Estimating, Heat Flux, Reynolds Number

Scientific paper

The strength of the dipole magnetic field of a planet, Hp, can be estimated relative to that of the Earth at the epoch of the observation. The generation of magnetic fields in Uranus and Neptune occurs at very different depths for different values of sigma. This assertion is confirmed by the estimation of the Reynolds number (Rm) and agrees with the difference of the contributions of the Joule heat losses into the observed heat fluxes of Uranus and Neptune.

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