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Titlebook: Non-equilibrium Evaporation and Condensation Processes; Analytical Solutions Yuri B. Zudin Book 20192nd edition Springer Nature Switzerland

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31#
發(fā)表于 2025-3-26 21:33:49 | 只看該作者
2192-4732 analysis of hydrodynamical characteristics of thin films.Wri.This monograph is focused mostly on the exposition of analytical methods for the solution of problems of strong phase change. A new theoretical model is proved useful in describing, with acceptable accuracy, problems of strong evaporation
32#
發(fā)表于 2025-3-27 04:56:27 | 只看該作者
Semi-empirical Model of Strong Evaporation,amental problem of simulation of the inner cometary atmosphere. According to the modern view [3], the intensity of icy cometary nucleus varies, as a function of the distance to Sun, in a very substantial range and may reach very large values.
33#
發(fā)表于 2025-3-27 07:42:35 | 只看該作者
Flow Around a Cylinder (Vapor Condensation),lm is determined by the interaction between the gravity forces (the driving force) and the viscous friction on the wall. The analytical solution to this problem was obtained in 1916 in fundamental studies by Nusselt [3, 4].
34#
發(fā)表于 2025-3-27 11:08:07 | 只看該作者
35#
發(fā)表于 2025-3-27 16:01:20 | 只看該作者
Concept of Pseudo-Boiling,of enhancing the initial vapor parameters in the 1960s. SCFs are considered as promising coolants due to their specific properties, and at present SCP power units play the key role in heat power engineering of advanced countries.
36#
發(fā)表于 2025-3-27 21:40:24 | 只看該作者
Binary Schemes of Vapor Bubble Growth,the general laws governing the influence of various parameters. The basis of the physical modeling of the process of boiling is an idealized problem on a spherically symmetric growth of a vapor bubble in an infinite volume of a uniformly superheated liquid [2].
37#
發(fā)表于 2025-3-28 01:22:21 | 只看該作者
38#
發(fā)表于 2025-3-28 05:27:25 | 只看該作者
39#
發(fā)表于 2025-3-28 09:40:55 | 只看該作者
40#
發(fā)表于 2025-3-28 11:55:25 | 只看該作者
Semi-empirical Model of Strong Evaporation,1], calculation of the parameters of discharge into vacuum of a flashing coolant [2], etc. Strong evaporation also plays an important role in the fundamental problem of simulation of the inner cometary atmosphere. According to the modern view [3], the intensity of icy cometary nucleus varies, as a f
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