Understanding the solar dynamo

被引：14

作者：

Bushby, P ^{[1
]}

Mason, J ^{[1
]}

机构：

[1] Univ Cambridge, DAMTP, Cambridge CB2 1TN, England

来源：

ASTRONOMY & GEOPHYSICS | 2004年 / 45卷 / 04期

关键词：

D O I：

10.1046/j.1468-4004.2003.45407.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Becoming ever more tightly constrained by observations and theory, the solar dynamo model that we have now bears little resemblance to the model studied just 30 years ago and, furthermore, it is likely to be modified in the near future. Solar dynamo theorists have learnt much over recent years, however we are still far from a complete understanding of how the Sun generates its magnetic field. So what is the solar dynamo, how much do we understand, and why is it proving so difficult to model?

引用

页码：7 / 13

页数：7

共 30 条

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