Convection in Rotating Fluids
แแแ. 2012 ยท Fluid Mechanics and Its Applications แฌแแแแ 29 ยท Springer Science & Business Media
แแแฌแแแแ
232
แแแแ แแ
reportแ แแแขแแแแแแ แแ แแแแแฎแแแแแแ แแแฃแแแกแขแฃแ แแแแแแ ย แจแแแขแงแแแ แแแขแ
แแ แแแฌแแแแแก แจแแกแแฎแแ
Spatial inhomogeneity of heating of fluids in the gravity field is the cause of all motions in nature: in the atmosphere and the oceans on Earth, in astrophysical and planetary objects. All natural objects rotate and convective motions in rotating fluids are of interest in many geophysical and astrophysical phenomena. In many industrial applications, too (crystal growth, semiconductor manufacturing), heating and rotation are the main mechanisms defining the structure and quality of the material.
Depending on the geometry of the systems and the mutual orientation of temperature and gravity field, a variety of phenomena will arise in rotating fluids, such as regular and oscillating waves, intensive solitary vortices and regular vortex grids, interacting vortices and turbulent mixing. In this book the authors elucidate the physical essence of these phenomena, determining and classifying flow regimes in the space of similarity numbers. The theoretical and computational results are presented only when the results help to explain basic qualitative motion characteristics.
The book will be of interest to researchers and graduate students in fluid mechanics, meteorology, oceanography and astrophysics, crystallography, heat and mass transfer.
Depending on the geometry of the systems and the mutual orientation of temperature and gravity field, a variety of phenomena will arise in rotating fluids, such as regular and oscillating waves, intensive solitary vortices and regular vortex grids, interacting vortices and turbulent mixing. In this book the authors elucidate the physical essence of these phenomena, determining and classifying flow regimes in the space of similarity numbers. The theoretical and computational results are presented only when the results help to explain basic qualitative motion characteristics.
The book will be of interest to researchers and graduate students in fluid mechanics, meteorology, oceanography and astrophysics, crystallography, heat and mass transfer.
แจแแแคแแกแแ แแก แแแฌแแแแ
แแแแแฎแแ แแ แแฅแแแแ แแแ แ.
แแแคแแ แแแชแแ แฌแแแแแฎแแแกแแแ แแแแแแจแแ แแแแ
แกแแแ แขแคแแแแแ แแ แขแแแแแขแแแ
แแแแแแกแขแแแแ แแ Google Play Books แแแ Android แแ iPad/iPhone แแแฌแงแแแแแแแแแแกแแแแก. แแก แแแขแแแแขแฃแ แแ แแแแแฎแแ แชแแแแแแก แกแแแฅแ แแแแแแชแแแก แแฅแแแแก แแแแแ แแจแแแ แแ แกแแจแฃแแแแแแก แแแแชแแแ, แฌแแแแแแฎแแ แกแแกแฃแ แแแแ แแแแขแแแขแ แแแแแกแแแแ แแแแแแแก, แ แแแแ แช แแแแแแ, แแกแ แฎแแแแแ แแจแ แ แแแแแจแ.
แแแแขแแแแแ แแ แแแแแแฃแขแแ แแแ
Google Play-แจแ แจแแซแแแแแ แแฃแแแแฌแแแแแแแก แแแกแแแแ แแฅแแแแ แแแแแแฃแขแแ แแก แแแ-แแ แแฃแแแ แแก แแแแแงแแแแแแ แจแแแแซแแแแ.
แแแฌแแแแแแฎแแแแแแ แแ แกแฎแแ แแแฌแงแแแแแแแแแ
แแแแฅแขแ แแแฃแแ แแแแแแก แแแฌแงแแแแแแแแแแ แฌแแกแแแแแฎแแ, แ แแแแ แแชแแ Kobo eReaders, แแฅแแแ แฃแแแ แฉแแแแขแแแ แแแ แคแแแแ แแ แแแแแแขแแแแ แแแ แแฅแแแแก แแแฌแงแแแแแแแแจแ. แแแฎแแแ แแแแก แชแแแขแ แแก แแแขแแแฃแ แ แแแกแขแ แฃแฅแชแแแแแก แแแฎแแแแแ แแแแแแขแแแแ แคแแแแแแ แแฎแแ แแแญแแ แแ แแแฌแแแแแแฎแแแแแแแ.
