NONLINEAR DYNAMOS IN TORUS GEOMETRY - TRANSITION TO CHAOS

被引:17
作者
BROOKE, JM [1 ]
MOSS, D [1 ]
机构
[1] UNIV MANCHESTER,DEPT MATH,MANCHESTER M13 9PL,ENGLAND
关键词
ACCRETION; ACCRETION DISKS; CHAOTIC PHENOMENA; MHD;
D O I
10.1093/mnras/266.3.733
中图分类号
P1 [天文学];
学科分类号
0704 [天文学];
摘要
We present results from integrating the non-linear mean field dynamo equations in the alpha omega-regime in a toroidal conducting volume. We assume a Keplerian rotation law, and impose axisymmetry. The non-linearity is a simple alpha-quenching. For`fat'tori, where the ratio of minor to major axis is not small, we find that solutions with negative dynamo number and dipolar parity are singly periodic for slightly supercritical dynamo numbers, and then undergo a further Hopf bifurcation to become doubly periodic, before becoming chaotic at dynamo numbers greater than about three times supercritical.
引用
收藏
页码:733 / 739
页数:7
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