Shear instability of differential rotation in stars

Shear instability of differential rotation in stars
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恒星差分旋转的剪切不稳定性

DOI:
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发表时间:
1980
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影响因子:
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通讯作者:
M. Watson
M. Watson
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文献类型:
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作者:
M. Watson

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本文研究了差动旋转星星的二维(水平)剪切不稳定性。研究了太阳型自转规律。当赤道角速度与两极角速度相差29%时,赤道加速度不稳定。
Abstract The two-dimensional (horizontal) shear instability of a differentially rotating star is examined. A solar-type rotation law is investigated. and it is found that for equatorial accelerations there is instability when there is a difference of 29% between the angular velocity of the equator and the poles.