An active sun throughout the Maunder Minimum

被引:324
作者
Beer, J [1 ]
Tobias, S
Weiss, N
机构
[1] EAWAG, CH-8600 Dubendorf, Switzerland
[2] Univ Colorado, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
[3] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 9EW, England
基金
美国国家航空航天局;
关键词
D O I
10.1023/A:1005026001784
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Measurements of (10)Be concentration in the Dye 3 ice core show that magnetic cycles persisted throughout the Maunder Minimum, although the Sun's overall activity was drastically reduced and sunspots virtually disappeared. Thus the dates of maxima and minima can now be reliably estimated. Similar behaviour is shown by a nonlinear dynamo model, which predicts that, after a grand minimum, the Suns toroidal field may switch from being antisymmetric to being symmetric about the equator. The presence of cyclic activity during the Maunder Minimum limits estimates of the solar contribution to climatic change.
引用
收藏
页码:237 / 249
页数:13
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