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Predicting solar cycle 24 with a solar dynamo model

文献类型:期刊论文

作者Choudhuri, Arnab Rai; Chatterjee, Piyali; Jiang, Jie
刊名PHYSICAL REVIEW LETTERS
出版日期2007-03-30
卷号98期号:13
英文摘要Whether or not the upcoming cycle 24 of solar activity will be strong is being hotly debated. The solar cycle is produced by a complex dynamo mechanism. We model the last few solar cycles by "feeding" observational data of the Sun's polar magnetic field into our solar dynamo model. Our results fit the observed sunspot numbers of cycles 21-23 reasonably well and predict that cycle 24 will be about 35% weaker than cycle 23.
收录类别SCI
语种英语
WOS记录号WOS:000245331500012
源URL[http://ir.bao.ac.cn/handle/114a11/7238]  
专题国家天文台_太阳物理研究部
作者单位1.Indian Inst Sci, Dept Phys, Bangalore 560012, Karnataka, India
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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GB/T 7714
Choudhuri, Arnab Rai,Chatterjee, Piyali,Jiang, Jie. Predicting solar cycle 24 with a solar dynamo model[J]. PHYSICAL REVIEW LETTERS,2007,98(13).
APA Choudhuri, Arnab Rai,Chatterjee, Piyali,&Jiang, Jie.(2007).Predicting solar cycle 24 with a solar dynamo model.PHYSICAL REVIEW LETTERS,98(13).
MLA Choudhuri, Arnab Rai,et al."Predicting solar cycle 24 with a solar dynamo model".PHYSICAL REVIEW LETTERS 98.13(2007).

入库方式: OAI收割

来源:国家天文台

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