SYMMETRY-BREAKING IN A NONLINEAR ALPHA-OMEGA-DYNAMO

被引:41
作者
JENNINGS, RL [1 ]
机构
[1] UNIV NEWCASTLE UPON TYNE, DEPT MATH & STAT, NEWCASTLE TYNE NE1 7RU, TYNE & WEAR, ENGLAND
关键词
ALPHA-OMEGA-DYNAMO; NONLINEAR DYNAMOS; STELLAR MAGNETISM; STABILITY; MEAN-FIELD DYNAMO; STELLAR CONVECTIVE DYNAMOS; NON-LINEAR DYNAMOS; ROTATING SPHERICAL-SHELL; DIFFERENTIAL-ROTATION; NUMERICAL SIMULATIONS; MAGNETIC-FIELDS; ASTROPHYSICAL DYNAMOS; SOLAR DYNAMO; STABILITY;
D O I
10.1080/03091929108225233
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An idealized nonlinear αω-dynamo is investigated. Emphasis is placed upon the different spatial symmetries, and the asymmetries that arise after secondary bifurcations. On varying the main control parameter D (the dynamo number), many transitions are found involving solutions without an equatorial symmetry, and solutions with quasiperiodic time dependence, but no chaos. Instead of a cascade to smaller spatial scales when D is highly supercritical it is found that additional asymmetries are introduced at tertiary bifurcations. Our complete bifurcation diagrams allow us to follow in detail how stability is passed from one solution to another as D varies. In these diagrams there are typically multiple stable solutions at any value of D, which suggests that similar stars can have different magnetic patterns. © 1991, Taylor & Francis Group, LLC. All rights reserved.
引用
收藏
页码:147 / 189
页数:43
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