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1)  Temperature fluctuation
温度涨落
2)  Density fluctuation
密度涨落
1.
Motion equation of density fluctuation in the nuclear reaction in stellar core;
星核反应密度涨落运动方程
2.
The dependence of the mass distribution of fragments, density fluctuation and the MLE on temperature has been studied for nuclear systems 124 Sn an.
应用量子分子动力学模型 ,从原子核发生碎化时的碎块质量分布、密度涨落以及混沌动力学中描述混沌程度的最大Lyapunov指数等 3个方面 ,对原子核的液气相变及其在临界点附近的行为进行较为全面的探讨 。
3.
The liquid superheat limit and vapor subcooling limit in homogeneous nucleation are determined in the present paper by using density fluctuation theory of statistical thermodynamics.
应用统计热力学巨正则系综的密度涨落理论 ,提出了确定均质沸腾中液体极限过热度和均质凝结中蒸汽极限过冷度的方法。
3)  intensity fluctuation
强度涨落
4)  fluctuation scaling
涨落尺度
5)  concentration fluctuation
浓度涨落
6)  width fluctuation correction
带宽度涨落
1.
The interaction reaction data of the neutron with Tin have been calculated by the optical model(OPM), HauserFeshbach theory with width fluctuation correction(WHF) and evaporation model including preequilibrium emission(PEM) in the energy range of incident neutron between 1 to 20 MeV.
对天然锡中子反应的实验数据进行评价,并用光学模型(OPM)、带宽度涨落修正的豪泽-费许巴哈理论(WHF)以及平衡前发射的蒸发模型(PEM),计算了入射能量为1~20MeV的中子与锡核相互作用的反应数据。
2.
The reaction data of neutron with titanium have been calculated by means of the optical model, the Hauser Feshbach theory with width fluctuation correction and the evaporation model including the preequilibrium emission in the energy range from 1 to 20 MeV.
采用光学模型(OPM)、带宽度涨落修正的豪泽-费许巴哈理论(WHF)和包括平衡前发射在内的蒸发模型(PEM),计算了入射能量为1~20MeV的中子和天然钛的反应数据。
补充资料:铂电阻温度表(见电阻温度表)


铂电阻温度表(见电阻温度表)


表。bod旧nZu wendubiao铂电阻温度表见电阻温
说明:补充资料仅用于学习参考,请勿用于其它任何用途。
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