On the internal structure and magnetic fields of venus

DOI10.1007/BF00643786zbMath0850.76840WikidataQ57919833 ScholiaQ57919833MaRDI QIDQ1911219

Yanyan Li

Publication date: 5 June 1996

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (2)

A comparison between Venus and Earth ⋮ Uranus and Neptune interior models

Cites Work

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• Spiralling columnar convection in rapidly rotating spherical fluid shells
• Convection driven magnetohydrodynamic dynamos in rotating spherical shells
• On coupling between the Poincaré equation and the heat equation: non-slip boundary condition
• On the thermal instability of a rotating-fluid sphere containing heat sources
• Thermal instabilities in rapidly rotating systems

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