Topics in Magnetohydrodynamic Topology, Reconnection and Stability Theory, David MacTaggart; Andrew Hillier
Автор: Dieter Biskamp Название: Magnetohydrodynamic turbulence ISBN: 052105253X ISBN-13(EAN): 9780521052535 Издательство: Cambridge Academ Рейтинг: Цена: 7445.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This book presents an introduction to, and state-of-the-art account of, magnetohydrodynamic (MHD) turbulence. Applications to three topics from astrophysics are considered: the solar wind, accretion disks, and the interstellar medium. Suitable for graduate students and researchers working in turbulence theory, plasma physics and astrophysics.
Автор: McGuire Fay Название: Magnetohydrodynamics Handbook ISBN: 1632383101 ISBN-13(EAN): 9781632383105 Издательство: Неизвестно Цена: 17702.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This thesis presents an accurate and advanced numerical methodology to remedy difficulties such as direct numerical simulation of magnetohydrodynamic (MHD) flow in computational fluid dynamics (CFD), grid generation processes in tokamak fusion facilities, and the coupling between the surface tension force and Lorentz force in the metallurgical industry. In addition, on the basis of the numerical platform it establishes, it also investigates selected interesting topics, e.g. single bubble motion under the influence of either vertical or horizontal magnetic fields. Furthermore, it confirms the relation between the bubble’s path instability and wake instability, and observes the anisotropic (isotropic) effect of the vertical (horizontal) magnetic field on the vortex structures, which determines the dynamic behavior of the rising bubble. The direct numerical simulation of magnetohydrodynamic (MHD) flows has proven difficult in the field of computational fluid dynamic (CFD) research, because it not only concerns the coupling of the equations governing the electromagnetic field and the fluid motion, but also calls for suitable numerical methods for computing the electromagnetic field. In tokamak fusion facilities, where the MHD effect is significant and the flow domain is complex, the process of grid generation requires considerable time and effort. Moreover, in the metallurgical industry, where multiphase MHD flows are usually encountered, the coupling between the surface tension force and Lorentz force adds to the difficulty of deriving direct numerical simulations.
Описание: The book presents an advanced but accessible overview of some of the most important sub-branches of magnetohydrodynamics (MHD): stability theory, magnetic topology, relaxation theory and magnetic reconnection.
Описание: Selected Papers of the PAMIR Conference held in Aussois, France, 22-26 September, 1997
Автор: A. Yoshizawa Название: Hydrodynamic and Magnetohydrodynamic Turbulent Flows ISBN: 9048150906 ISBN-13(EAN): 9789048150908 Издательство: Springer Рейтинг: Цена: 28732.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: TUrbulence modeling encounters mixed evaluation concerning its impor- tance. The estrangement between the physics community and the turbulence modeling is further enhanced by the fact that the latter is founded on a weak theoretical basis, compared with the study of small-scale turbulence.
Автор: Davidson Название: Introduction to Magnetohydrodynamics ISBN: 131661302X ISBN-13(EAN): 9781316613023 Издательство: Cambridge Academ Рейтинг: Цена: 8870.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: A comprehensive textbook which prioritises physical ideas over mathematical detail. This new edition offers additional coverage of planetary dynamos, astrophysical applications and fusion plasma magnetohydrodynamics. An ideal companion for both undergraduates and postgraduates in physics, applied mathematics or engineering.
Описание: This monograph set presents a consistent and self-contained framework of stochastic dynamic systems with maximal possible completeness. This approach offers a possibility of both obtaining exact solutions to stochastic problems for a number of models of fluctuating parameters and constructing various asymptotic buildings.
Описание: 1 Introduction.- Part I Hydrodynamical Phenomena in Astrophysical Objects.- 2 Basic Equations for Hydrodynamics.- 3 Astrophysical Fluid Flows.- 4 Wave Phenomena in Astrophysical Objects.- 5 Convection and Related Topics.- 6 Dynamical Instability and Dynamical Excitation of Oscillations.- 7 Instabilities due to Dissipative Processes I (Secular Instability).- 8 Overstability due to Dissipative Processes II: Excitation of Oscillations.- 9 General Relativistic Hydrodynamics.- Part II Magnetohydrodynamical Phenomena in Astrophysical Objects.- 10 Derivation of Magnetohydrodynamical Equations from Boltzmann Equation.- 11 MHD Equations and Basic Characteristics of Magnetic Fields.- 12 Astrophysical MHD Flows.- 13 Waves and Shocks in Magnetohydrodynamical Fluids.- 14 Astrophysical Dynamo.- 15 General Stability Theorem for MHD Systems.- 16 Instabilities Related to Magnetic Fields.- 17 Important Non-Ideal MHD Processes.- 18 Relativistic Magnetohydrodynamics.- Part III Astrophysical Radiation Hydrodynamics.- 19 Basic Concepts of Radiative Fluids.- 20 Basic Equations for Radiative Transfer.- 21 Basic Equations for Radiation Hydrodynamics.- 22 Astrophysical RHD Flows.- 23 Wave and Instability in Radiative Fluids.- 24 Relativistic Radiative Transfer.- 25 Relativistic Radiation Hydrodynamics .- 26 General Relativistic Radiation Hydrodynamics.
Описание: Turbulence and magnetic fields are ubiquitous in the Universe. Their importance to astronomy cannot be overestimated. The theoretical advancements in magnetohydrodynamic (MHD) turbulence achieved during the past two decades have significantly influenced many fields of astronomy. This book provides predictive theories of the magnetic field generation by turbulence and the dissipation of MHD turbulence.These fundamental non-linear problems were believed to be tractable only numerically. This book provides complete analytical descriptions in quantitative agreement with existing numerics, as well as theoretical predictions in physical regimes still unreachable by simulations, and explanations of various related observations. It also discusses and promotes the astrophysical applications of MHD turbulence theories, including (i) the particle acceleration and radiation in high-energy phenomena, e.g., Gamma-Ray Bursts, supernova remnants, cosmic rays; (ii) interstellar density fluctuations and the effect on observations, e.g., Faraday rotation, scattering measurements of Galactic and extragalactic radio sources; (iii) density and magnetic field structure in molecular clouds toward star formation. In closing, this book demonstrates the key role of MHD turbulence in connecting diverse astrophysical processes and unraveling long-standing astrophysical problems, as foreseen by Chandrasekhar, a founder of modern astrophysics.
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