The authors review the original mixing length theory and give a set of modified mixing length formula.

作者对此提出了质疑，并提出了一种修正的混合长公式。

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Basee on the mixing-length theory of convection, macroscopical stress of the turbulence is used in hydrostatics equation of the stellar structural and evolutionary model.

以恒星结构与演化理论中常用的混合程理论为基础，将湍流作用表现出来的宏观应力引入恒星结构与演化模型中的流体静力学平衡方程。

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