A possible origin of viscosity in Keplerian accretion disks due to secondary perturbation：Turbulent transport without magnetic fields 期刊界 All Journals 搜尽天下杂志传播学术成果专业期刊搜索期刊信息化学术搜索

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A possible origin of viscosity in Keplerian accretion disks due to secondary perturbation：Turbulent transport without magnetic fields

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关键词：	扰动模式湍流输送磁场耦合吸积盘开普勒粘度起源 Couette流动
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