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2019 | OriginalPaper | Buchkapitel

4. Semi-empirical Model of Strong Evaporation

verfasst von : Yuri B. Zudin

Erschienen in: Non-equilibrium Evaporation and Condensation Processes

Verlag: 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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Vorheriges Kapitel Approximate Kinetic Analysis of Strong Evaporation

Nächstes Kapitel Approximate Kinetic Analysis of Strong Condensation

For a gas discharge to the region of reduced pressure, the discontinuity surface is front of a rarefaction shock.

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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Titel: Semi-empirical Model of Strong Evaporation
verfasst von: Yuri B. Zudin
Verlag: Springer International Publishing
Buch: Non-equilibrium Evaporation and Condensation Processes
Print ISBN: 978-3-030-13814-1

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

Copyright-Jahr: 2019
DOI: https://doi.org/10.1007/978-3-030-13815-8_4

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