期刊
RESEARCH IN ASTRONOMY AND ASTROPHYSICS
卷 9, 期 9, 页码 953-958出版社
NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
DOI: 10.1088/1674-4527/9/9/001
关键词
Sun: activity; Sun: magnetic fields; sunspots
资金
- DST [SR/S2/HEP-15/2007]
We propose that the poloidal field at the end of the last sunspot cycle before the Maunder minimum fell to a very low value due to fluctuations in the Babcock-Leighton process. With this assumption, a flux transport dynamo model is able to explain various aspects of the historical records of the Maunder minimum remarkably well by suitably choosing the parameters of the model to give the correct growth time.
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