The role of the Yoshizawa effect in the Archontis dynamo
The role of the Yoshizawa effect in the Archontis dynamo
复制标题
吉泽效应在 Archontis 发电机中的作用
DOI:
10.1111/j.1365-2966.2009.15254.x
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发表时间:
2009
影响因子:
4.8
通讯作者:
A. Brandenburg
中科院分区:
文献类型:
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作者:
S. Sur;A. Brandenburg
The generation of mean magnetic fields is studied for a simple non-helical flow where a net cross helicity of either sign can emerge. This flow, which is a lso known as the Archontis flow, is a generalization of the Arnold‐Beltrami‐Childress flow, but with the cosine terms omitted. The presence of cross helicity leads to a mean-field dynamo effect that is known as the Yoshizawa effect. Direct numerical simulations of such flows demonstrate the presence of magnetic fields on scales larger than the scale of the flow. Con trary to earlier expectations, the Yoshizawa effect is found to be proportional to the mean magnetic field and can therefore lead to its exponential instead of just linear amplification for magnetic Reynolds numbers that exceed a certain critical value. Unlike α effect dynamos, it is found that the Yoshizawa effect is not noticeably constrained by the presence of a conservat ion law. It is argued that this is due to the presence of a forcing term in the momentum equation which leads to a nonzero correlation with the magnetic field. Finally, the applicati on to energy convergence in solar wind turbulence is discussed.
DOI:
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发表时间:
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期刊:
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影响因子:
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作者:
M. Schrinner;K. R. Adler;D. Schmitt;M. Rheinhardt;U. Christensen
通讯作者:
M. Schrinner;K. R. Adler;D. Schmitt;M. Rheinhardt;U. Christensen
DOI:
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发表时间:
2007
期刊:
影响因子:
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作者:
Masaki Yoshida;Akira Kageyama;陰山 聡(招待講演);陰山聡;陰山 聡(招待講演);陰山聡;Akira Kageyama (Invited Talk);陰山 聡(招待講演);陰山聡;Akira Kageyama (Invited Talk);陰山 聡(招待講演);陰山聡;陰山 聡(招待講演);N.Ohno;大野 暢亮;M.Furuichi;Akira Kageyama (Invited talk);Akira Kageyama;陰山聡(招待講演);陰山聡(招待講演);Akira Kageyama (Invited talk);Akira Kageyama (Invited talk);Akira Kageyama;Akira Kageyama;宮腰 剛広;宮腰 剛広;陰山 聡;陰山聡(招待講演);Akira Kageyama (Invited lecture)
通讯作者:
Akira Kageyama (Invited lecture)