Progress in Turbulence and Wind Energy IV, Martin Oberlack; Joachim Peinke; Alessandro Talame

Автор: Sagaut Pierre
Название: Multiscale and Multiresolution Approaches in Turbulence
ISBN: 1848169868 ISBN-13(EAN): 9781848169869
Издательство: World Scientific Publishing
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Описание: Aims to provide the reader with a general presentation of multiscale/multiresolution approaches in turbulent flow simulations. In this book, all modern approaches (LES, hybrid RANS/LES, DES, SAS) are discussed and recast in a global comprehensive framework.

Автор: M. M. Stanisic
Название: The Mathematical Theory of Turbulence
ISBN: 0387966854 ISBN-13(EAN): 9780387966854
Издательство: Springer
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Описание: "I do not think at all that I am able to present here any procedure of investiga- tion that was not perceived long ago by all men of talent;

Автор: Shrira Victor
Название: Advances in Wave Turbulence
ISBN: 9814366935 ISBN-13(EAN): 9789814366939
Издательство: World Scientific Publishing
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Описание: Wave or weak turbulence is a branch of science concerned with the evolution of random wave fields of all kinds and on all scales, from waves in galaxies to capillary waves on water surface, from waves in nonlinear optics to quantum fluids. This title presents the advances in wave turbulence.

Автор: Michel Stanislas; Javier Jimenez; Ivan Marusic
Название: Progress in Wall Turbulence: Understanding and Modeling
ISBN: 9400733992 ISBN-13(EAN): 9789400733992
Издательство: Springer
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Описание: With contributions from leading researchers in the field, and including recent breakthrough work, this collection of recent results on near wall turbulence includes theory, new experiments, DNS, and modeling with RANS, LES and Low Order Dynamical Systems.

Автор: Roberto Bruno; Vincenzo Carbone
Название: Turbulence in the Solar Wind
ISBN: 331943439X ISBN-13(EAN): 9783319434391
Издательство: Springer
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Описание: This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence.This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfv?nic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere.The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yaglom’s law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating.Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context.