本文采用非径向磁流管位形的假设，计算了太阳冕洞网络部分的色球-日冕过渡区的能量平衡模型。
Energy balance models of the chromosphere-corona transition region are computed for a segment of coronal hole assuming a nonradial magnetic field geometry.
在日冕和非日冕两种模型下，分别求解了电离速率方程。
Using model of coronal and non-coronal radiation, ionization rate equation has been solved respectively.
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