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2019 | OriginalPaper | Chapter

4. Semi-empirical Model of Strong Evaporation

Author : Yuri B. Zudin

Published in: Non-equilibrium Evaporation and Condensation Processes

Publisher: Springer International Publishing

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Abstract

Knowledge of laws of strong evaporation is instrumental for the solution of a number of applied problems: the effect of laser radiation on materials [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 function of the distance to Sun, in a very substantial range and may reach very large values.

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previous chapter Approximate Kinetic Analysis of Strong Evaporation
next chapter Approximate Kinetic Analysis of Strong Condensation
Footnotes
1
For a gas discharge to the region of reduced pressure, the discontinuity surface is front of a rarefaction shock.
 
2
Strictly speaking, physically sensible on the CPS are the temperature \(T_{w}\) and density \(\rho_{w}\). The pressure \(p_{w}\) and velocity \(u_{w}\) are reference values.
 
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Metadata
Title
Semi-empirical Model of Strong Evaporation
Author
Yuri B. Zudin
Copyright Year
2019
Book
Non-equilibrium Evaporation and Condensation Processes

Print ISBN: 978-3-030-13814-1

Electronic ISBN: 978-3-030-13815-8

Copyright Year: 2019

DOI
https://doi.org/10.1007/978-3-030-13815-8_4

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