Mechanics of turbulence of multicomponent gases - Info and Reading Options
By Mikhail I͡Akovlevich Marov

"Mechanics of turbulence of multicomponent gases" was published by Kluwer Academic Publishers in 2001 - Dordrecht, it has 375 pages and the language of the book is English.
“Mechanics of turbulence of multicomponent gases” Metadata:
- Title: ➤ Mechanics of turbulence of multicomponent gases
- Author: Mikhail I͡Akovlevich Marov
- Language: English
- Number of Pages: 375
- Publisher: Kluwer Academic Publishers
- Publish Date: 2001
- Publish Location: Dordrecht
“Mechanics of turbulence of multicomponent gases” Subjects and Themes:
- Subjects: ➤ Atmospheres - Turbulence - Rarefied gas dynamics - Planets - Thermodynamics - Meteorology - Physics - Astronomy - Mathematical physics - Planets, atmospheres - Gas dynamics - Mechanics, Fluids, Thermodynamics - Meteorology/Climatology - Mathematical and Computational Physics
Edition Specifications:
- Pagination: xiii, 375 p. :
Edition Identifiers:
- The Open Library ID: OL18173095M - OL12341256W
- Online Computer Library Center (OCLC) ID: 48045877
- Library of Congress Control Number (LCCN): 2001050301
- ISBN-10: 1402001037
- All ISBNs: 1402001037
AI-generated Review of “Mechanics of turbulence of multicomponent gases”:
"Mechanics of turbulence of multicomponent gases" Description:
The Open Library:
This book develops a new mathematical approach for modelling multicomponent gas turbulence that adequately describes the combined processes of dynamics and heat and mass transfer when chemical kinetics and turbulent mixing are equally important. The developed models include the evolutionary transfer equations for the single-point second correlation moments of turbulent fluctuations of thermohydrodynamical parameters. The phenomenological approach to the closure problem in hydrodynamic equations of mean motion at the level of the first order moments is based on the thermodynamics of irreversible processes and enables defining relationships in a more general form as compared to those conventionally deduced using the mixing path concept. Based on the developed approach, turbulent exchange factors for a planetary upper atmosphere are evaluated, and a turbulent model of a protoplanetary accretion gas-dust disk involving heat and mass transfer and coagulation is also considered.
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