日冕模型 corona model
- 在本文的模型中,采用了最新的色球-日冕过渡区的远紫外(EUV)资料;
In our model, we have used the latest EUV data on the chromosphere-corona transition region; - 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. - 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.
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