INTERMEDIATE DYNAMO MODELS

被引:11
|
作者
GLATZMAIER, GA [1 ]
ROBERTS, PH [1 ]
机构
[1] UNIV CALIF LOS ANGELES, INST GEOPHYS & PLANETARY PHYS, LOS ANGELES, CA 90024 USA
来源
关键词
D O I
10.5636/jgg.45.1605
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We describe a nonlinear, axisymmetric, spherical-shell model of a planetary dynamo. This intermediate-type dynamo model requires a prescribed helicity field (the alpha effect) and a prescribed buoyancy force or thermal wind (the omega effect) and solves for the axisymmetric time-dependent magnetic and velocity fields. Three very different time dependent solutions are obtained from different prescribed sets of alpha and omega fields.
引用
收藏
页码:1605 / 1616
页数:12
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