Turbulence and self-organization : modeling astrophysical objects
This book focuses on the development of continuum models of natural turbulent media. It provides a theoretical approach to the solutions of different problems related to the formation, structure and evolution of astrophysical and geophysical objects. A stochastic modeling approach is used in the mat...
Enregistré dans:
| Auteurs principaux: | , |
|---|---|
| Format: | Livre numérique |
| Sprog: | Anglais |
| Udgivet: |
New York, NY :
Springer New York
[20..].
Cham : Springer Nature |
| Udgivelse: | 1st ed. 2013. |
| Serier: | Astrophysics and Space Science Library
389 |
| Online adgang: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Kommentar: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Turbulence and self-organization, modeling astrophysical objects, Mikhail Ya Marov, Aleksander V. Kolesnichenko, 2013, New York, Springer, 1 vol. (XXVIII-657 p.), Astrophysics and space science library, 978-1-4614-5154-9 |
Indholdsfortegnelse:
- Turbulent Chaos and Self-organization in Space and Natural Environments Basics of Mathematical Modeling of Reactive Gas Mixtures Closed System of Hydrodynamic Equations for the Description of Turbulent Motion of Multicomponent Media Differential Models of Closure of the Averaged Hydrodynamic Equations for the Turbulent Chemically-active Continuous Medium.-Stochastic-thermodynamic Modeling of the Developed Structural Turbulence Self-organization of the Developed Turbulence and Mechanisms of Coherent Structure Formation Basics of Heterogeneous Mechanics with Applications to Accretion Discs Influence of Hydrodynamic Spirality on Turbulence Evolution in the Accretion Disc Thermodynamic Model of Magnetohydrodynamic (MGD) Turbulence and Some Application to the Accretion Discs