The present paper discusses the distortion of field lines in the co-rotation region of a star caused by a non-axisymmetrical magnetic field.
本文讨论了由于非轴对称磁场所引起的星体共转区中的磁力线变形。
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For co-rotation and counter-rotation in which the centrifugal force dominates the flow, the secondary flow in a rotating helical pipe has the same direction with that in a stationary one.