Deep Convection in the Interior of Major Planets: A Review

Details Deep Convection in the Interior of Major Planets: A Review Deep Convection in the Interior of Major Planets: A Review

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aujph..51..875y&link_type=abstract

Australian Journal of Physics, vol. 51, p. 875

Physics

5

Convection, Planetary Cores, Gas Giant Planets, Earth Mantle, Oceanography, Jupiter (Planet), Saturn (Planet), Uranus (Planet)

Scientific paper

Theories for deep convection in the interior of major planets are
reviewed. The focus is on Busse's theory, whose problems are critically
analyzed the importance of the analogy and differences with the Earth's
mantle convection and oceanographic convection are emphasized.

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