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Modeling of magnetohydrodynamic flow in Earth's core

Modeling of magnetohydrodynamic flow in Earth's core
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摘要 Free convection heat transfer with internal sources of heat in a liquid core of the Earth by the account of magnetic forces is considered. The core of the Earth is considered as a spherical layer. For temperature the boundary conditions Ⅰ, Ⅱ, Ⅲ sorts were considered. As a result of the numerical decision of a task the fields of temperature, stream function, local and average of Nusselt number are obtained. Free convection heat transfer with internal sources of heat in a liquid core of the Earth by the account of magnetic forces is considered. The core of the Earth is considered as a spherical layer. For temperature the boundary conditions Ⅰ, Ⅱ, Ⅲ sorts were considered. As a result of the numerical decision of a task the fields of temperature, stream function, local and average of Nusselt number are obtained.
出处 《Journal of Harbin Institute of Technology(New Series)》 EI CAS 2000年第S1期91-93,共3页 哈尔滨工业大学学报(英文版)
基金 TheworkisexecutedatsupportFCP″Integration″,projectN 0 56 0 +K 0 92 8
关键词 CONVECTION MAGNETIC HEAT TRANSFER CORE EARTH convection magnetic heat transfer core earth
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参考文献3

  • 1PATANKAR S.Numerical heat transfer and fluid flow[]..1984
  • 2JANOVSKIY B M.Terrestrial magnetism[]..1978
  • 3KRAUSE F,RADLER K H.Mean-Field Magnetohydrodynamics and dynamo theory[]..1980

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