提出了一种基于沸腾表面微结构分析的预测核态沸腾中汽化核心密度的方法。
A method has been presented to predict the nucleation site density in nucleate boiling based on the investigation of the microstructure of boiling surface.
通过对沸腾表面微结构进行分析，沸腾表面上具备贮藏气体条件的凹坑被识别出来，并且得到一个这些具备贮藏气体条件凹坑的开口半径的数据集合。
Through the investigation, the gas trapping cavities on boiling surface are identified and a data set of the mouth diameters of gas trapping cavities is got.
由于温度较高，必须有足够的云彩才能防止星球表面的水分不会出现沸腾。
With the high temperatures, there must be sufficient cloud cover to keep any water on the surface from boiling.
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