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  • 1
    Online Resource
    Online Resource
    Milton :Taylor & Francis Group,
    Keywords: Plasma turbulence. ; Electronic books.
    Description / Table of Contents: Plasma and Fluid Turbulence: Theory and Modelling explains modelling methodologies in depth with regard to turbulence phenomena and turbulent transport both in fluids and plasmas. Special attention is paid to structural formation and transitions. In this detailed book, the authors examine the underlying ideas describing turbulence, turbulent transport, and structural transitions in plasmas and fluids. By comparing and contrasting turbulence in fluids and plasmas, they demonstrate the basic physical principles common to fluids and plasmas while also highlighting particular differences. The book also discusses the application of these ideas to neutral fluids.
    Type of Medium: Online Resource
    Pages: 1 online resource (480 pages)
    Edition: 1st ed.
    ISBN: 9781420033694
    DDC: 530.4/4
    Language: English
    Note: Cover -- Half Title -- Title Page -- Copyright Page -- Dedication -- Table of Contents -- Preface -- Acknowledgments -- PART I: GENERAL INTRODUCTION -- 1: Introductory Remarks -- 2: Structure Formation in Fluids and Plasmas -- 2.1 Flow in a Pipe -- 2.1.1 Enhancement of Mixing Effects Due to Turbulence -- 2.1.2 Mean-Flow Structure Formation in Pipe Flows -- 2.2 Magnetic-Field Generation by Turbulent Motion -- 2.3 Collimation of Jets -- 2.4 Magnetic Confinement of Plasmas -- 2.4.1 Magnetic Confinement and Toroidal Plasmas -- 2.4.2 Flows in Toroidal Plasmas -- 2.4.3 Topological Change of Magnetic Surfaces -- 2.5 Nonlinearity in Transport and Structural Transition -- 2.5.1 Nonlinear Gradient-Flux Relation -- 2.5.2 Bifurcation in Flow -- 2.5.3 Bifurcation in Structural Formation -- References -- PART II: FLUID TURBULENCE -- Nomenclature -- 3: Fundamentals of Fluid Turbulence -- 3.1 Fundamental Equations -- 3.2 Averaging Procedures -- 3.3 Ensemble-Mean Equations -- 3.3.1 Mean-Field Equations -- 3.3.2 Turbulence Equations -- 3.4 Homogeneous Turbulence -- 3.4.1 Fundamental Concepts -- 3.4.2 Kolmogorov's Scaling Law -- 3.4.3 Failure of Kolmogorov's Scaling -- 3.4.4 Two-Dimensional Turbulence -- 3.5 Production and Diffusion Characteristics of Turbulent Energy -- References -- 4: Heuristic Turbulence Modelling -- 4.1 Approaches to Turbulence -- 4.2 Algebraic Turbulence Modelling -- 4.2.1 Modelling of Reynolds Stress -- 4.2.2 Modelling of Heat Flux -- 4.2.3 Modelling of Turbulence Equations -- 4.2.4 The Simplest Algebraic Model -- 4.2.5 Investigation into Some Representative Turbulent Flows -- 4.3 Second-Order Modelling -- 4.3.1 Modelling of Pressure-Strain Term -- 4.3.2 Modelling of Dissipation and Transport Terms -- 4.3.3 The Simplest Second-Order Model and its Relationship with a Higher-Order Algebraic Model -- 4.4 A Variational-Method Model. , 4.4.1 Helicity and Vortical-Structure Persistence -- 4.4.2 Derivation of the Vorticity Equation Using the Variational Method -- 4.4.3 Analysis of Swirling Pipe Flow -- 4.4.4 Swirl Effect on Reynolds Stress -- 4.5 Subgrid-Scale Modelling -- 4.5.1 Filtering Procedure -- 4.5.2 Filtered Equations -- 4.5.3 Fixed-Parameter Modelling -- 4.5.4 Dynamic Model -- References -- 5: Statistical Theory of Fluid Turbulence -- 5.1 Mathematical Methods Necessary for Turbulence Theory -- 5.1.1 Partial Summation of Infinite Series -- 5.1.2 Gaussian Distribution Function -- 5.1.3 Solution of Differential Equation Using Method of Partial Summation -- 5.2 Theoretical Approach to Inhomogeneous Turbulence -- 5.2.1 Perturbational Method to Turbulence -- 5.2.2 Introduction of Green's Function -- 5.2.3 Statistical Evaluation of Reynolds Stress -- 5.3 Contributions to Turbulence Modelling -- 5.3.1 Modelling of the Turbulent-Energy Equation -- 5.3.2 Modelling of the Mach-Number Effect -- References -- PART III: MAGNETOHYDRODYNAMIC TURBULENCE: DYNAMO -- Nomenclature -- 6: Fundamentals of Mean-Field Theory of Dynamo -- 6.1 One-Fluid Magnetohydrodynamic Approximation -- 6.1.1 Fundamental Equations -- 6.1.2 Nondimensional Parameters Characterizing Flows -- 6.1.3 Elsasser's Variables and Conservation Properties -- 6.2 Cowling's Anti-Dynamo Theorem -- 6.3 Mean-Field Equations -- 6.4 Turbulence Equations -- References -- 7: Theoretical Estimate of Turbulence Effects on Magnetic-Field Equations -- 7.1 Kinematic Method -- 7.1.1 Introduction of Two Scales and Scale-Parameter Expansion -- 7.1.2 Evaluation of Turbulent Electromotive Force -- 7.1.3 Evaluation of Reynolds Stress -- 7.2 Counter-Kinematic Method -- 7.2.1 Scale-Parameter Expansion -- 7.2.2 Evaluation of Turbulent Electromotive Force -- 7.2.3 Evaluation of Reynolds Stress. , 7.3 Discussions on Dynamo Effects from Kinematic and Counter-Kinematic Methods -- 7.3.1 Mathematical Features of Obtained Expressions -- 7.3.2 Physical Meanings of Obtained Expressions -- 7.4 Magnetohydrodynamic Method -- 7.4.1 Elsasser's Variables and Two-Scale Description -- 7.4.2 Perturbational Solution -- 7.4.3 Evaluation of Elsasser's Reynolds Stress -- 7.4.4 Comparison with Kinematic and Counter-Kinematic Methods -- References -- 8: One-Point Dynamo Modelling with Emphasis on Self-Consistency -- 8.1 Necessity and Significance of One-Point Modelling -- 8.2 Modelling Policy and Procedures -- 8.3 Summary of Dynamo Model -- 8.3.1 System of Model Equations -- 8.3.2 Model Constants -- 8.3.3 Remarks on Characteristic Time Scales -- References -- 9: Typical Magnetic-Field Generation Processes -- 9.1 Dominant-Helicity Dynamo -- 9.1.1 Convection Columns and Helicity -- 9.1.2 Mean-Field Equations -- 9.1.3 Turbulence Equations -- 9.2 Dominant/Cross-Helicity State -- 9.2.1 Mean-Field Equations -- 9.2.2 Turbulence Equations -- 9.3 Traditional Kinematic Dynamos -- 9.3.1 Alpha-Alpha Dynamo -- 9.3.2 Alpha-Omega Dynamo -- References -- 10: Application to Astro/Geophysical and Fusion Dynamos -- 10.1 Solar Magnetic Fields -- 10.1.1 Sunspot's Magnetic Field -- 10.1.2 Relationship of Sunspot's Polarity with Polar Field -- 10.1.3 Lorentz Force and Meridional Flow -- 10.1.4 Mean-Field-Theory Interpretation of Polarity Reversal -- 10.2 Geomagnetic Fields -- 10.2.1 Computer Simulation of Geodynamo -- 10.2.2 Saturation of Generated Magnetic Field -- 10.2.3 Frame-Rotation Effect on Magnetic Field -- 10.3 Collimation of Accretion-Disc Jets -- 10.3.1 Computer Simulation and Mean-Field Theory -- 10.3.2 Driving Force of Bipolar Jets -- 10.3.3 Collimation Mechanism Due to Magnetic Effect -- 10.3.4 Sustainment of Turbulent State. , 10.3.5 Physical Interpretation of Jet Collimation -- 10.4 Reversed-Field Pinches of Plasmas -- 10.4.1 Magnetic Plasma Confinement in a Torus -- 10.4.2 Derivation of Force-Free Field by Mean-Field Theory -- 10.4.3 Derivation of Force-Free Field by Variational Method -- 10.5 Plasma Rotation in Tokamaks -- 10.6 Transport Suppression Due to Electric-Field Effects -- 10.6.1 Equations with Electric-Field Effects Supplemented -- 10.6.2 Analysis of Turbulent Transport Rate of Thermal Energy -- 10.6.3 Effect of Radial Electric Field on Thermal-Energy Transport -- References -- PART IV: PLASMA TURBULENCE -- Nomenclature -- 11: Equations for Plasmas -- 11.1 Fluid Equations -- 11.2 Reduced Set of Equations -- 11.2.1 Yagi-Horton Equations -- 11.2.2 Hasegawa-Mima Equation -- 11.2.3 Hasegawa-Wakatani Equations -- 11.2.4 Reduced MHD Equations -- 11.3 Reduced Set of Equations and Conservation Property -- 11.3.1 Hasegawa-Mima Equation -- 11.3.2 Three-Field Equations -- 11.3.3 Yagi-Horton Equations -- 11.3.4 Dissipation and Transport Fiux -- 11.4 Kinetic Equation -- 11.4.1 Vlasov Equation -- 11.4.2 Gyro-Averaged Equations -- Appendix 11A Relations in Thermodynamics and Mean-Field Equation -- References -- 12: Inhomogeneity and Modes in Plasmas -- 12.1 Linear Mode -- 12.1.1 Dispersion Relation -- 12.1.2 Vlasov Equation and Linear Dielectric Tensor -- 12.2 Examples of Modes -- 12.2.1 Ion Sound Wave, Drift Wave and Convective Cell -- 12.2.2 Shear Alfven Wave and Drift Alfven Mode -- 12.2.3 Interchange Mode -- 12.2.4 Ion Temperature Gradient Mode -- 12.2.5 Dissipative Drift Mode -- 12.3 Weak Turbulence Theory -- 12.3.1 Ansatz of Weak Turbulence -- 12.3.2 Wave Kinetic Equation -- 12.3.3 Integral, Lyapunov Function and Thermodynamics -- 12.4 Transport Matrix and Symmetry -- Appendix 12A Quasilinear Theory of Transport -- References -- 13: Inhomogeneous Strong Turbulence. , 13.1 Regime of Strong Plasma Turbulence -- 13.2 Concepts to Describe Inhomogeneous Turbulent Plasmas -- 13.2.1 Gradients (Magnetic Surface, Shear, etc.) -- 13.2.2 Mode, Wave, and Vortex -- 13.2.3 Propagating Solitary Structure -- 13.2.4 Convective Cell, Zonal Flow and Streamer -- 13.2.5 Reconnection, Island Overlapping, Braiding, and Mixing -- 13.2.6 Plume and Avalanche (Time Intermittence) -- 13.2.7 Clumps -- 13.3 Microscale and Mesoscale Structures and Competition -- Appendix 13A Clumps -- References -- 14: Method for Strong Turbulence I. Renormalization and Statistical Method -- 14.1 Resonance Broadening and Renormalization in the Kinetic Propagator -- 14.1.1 Renormalization of the Propagator -- 14.1.2 Strong Turbulence Limit and Fluid Model -- 14.1.3 Strong Turbulence Limit and Kubo Number -- 14.2 Nonlinear Response in Fluid-Like Equations -- 14.2.1 Short-Wavelength Fluctuations -- 14.2.2 Rapidly-Changing, Long-Wavelength Components -- 14.2.3 Static but Sheared Flow -- 14.2.4 On Rigorous Upper Bound -- 14.3 Renormalization in a Reduced Set of (Fluid-Like) Equations -- 14.4 Randomness and the Statistical Picture -- 14.4.1 Estimate of Random Source Term -- 14.4.2 Dynamical Equations for Correlation Functions -- 14.4.3 Langevin Equations -- 14.4.4 Example of Three-Field Model -- 14.5 Fokker-Planck Equation -- 14.5.1 Projected Variable -- 14.5.2 Fokker-Planck Equation -- 14.5.3 Equilibrium Probability Density Function -- 14.5.4 H-Theorem -- 14.5.5 Tail in Probability Density -- 14.6 Memory Effects and Non-Markovian Property -- Appendix 14A Rigorous Upper Bounds for Transport -- References -- 15: Methods for Strong Turbulence II. Scale Invariance Method -- 15.1 Fluid Models -- 15.1.1 Reynolds Number and Drag -- 15.1.2 Spectrum -- 15.2 Plasma Models -- 15.2.1 Transport Coefficient -- 15.2.2 Spectrum -- References. , 16: Methods for Strong Turbulence III. Model Based on Reduced Variables.
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  • 2
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 79 (1996), S. 5452-5452 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Cubic Laves phase alloy YFe2 forms four types of hydrides, YFe2Hx: β1, β2 (hexagonal) of 1.2〈x〈1.6, γ (hexagonal) of 2.8〈x〈3.45, and δ (orthorhombic) of 3.7〈x. The β1 and β2 hydrides are formed in the hydrogen absorption below and above 500 K. The deuterides YFe2Dx have been prepared by deuterium absorption at various temperatures for YFe2 powders of diameters less than 0.3 mm. The formed samples are mixtures of main and extra deuteride phases. The x-ray and magnetization measurements in a magnetic field of 10.6 kOe showed five types of ferromagnetic deuterides with Curie temperatures of about 100 K (δ1), 300 K (δ2), 380 K (γ), 300–380 K (β1), and 540 K (amorphous). The extrapolated values of magnetization at 0 K are 3.5μB/YFe2Dx. The crystal structures are as follows: δ1, hexagonal, a=0.57 nm, c=2.74 nm; δ2, cubic, a=0.79 nm; γ, hexagonal, a=0.56 nm, c=2.63 nm; and β, hexagonal (a=0.53 nm, c=0.87 nm)–(a=0.51 nm, c=0.82 nm). © 1996 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 78 (1995), S. 30-38 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Theoretical analysis of the output performance of a transverse discharge pumped neon Penning laser (585.3 nm) using a mixture of Ne/H2 is described. The validity of the kinetic model is confirmed by comparing the results to the experimental discharge and laser performance. It is theoretically shown that the optimum mixing ratio of the Ne/H2 mixture is 1:2.5, and the optimum operating pressure is about 56 Torr. The model also predicts that the intrinsic efficiency reaches a peak of 8.5×10−6 at an excitation rate of 0.5 MW/cm3 under the optimum mixing ratio and operating pressure conditions. At excitation rates in excess of 0.5 MW/cm3 the laser output power is slowly increasing and then saturates due to electron collisional quenching of the upper laser level. The laser power extraction is increased by laser injection seeding in order to rapidly build up the lasing. The improved intrinsic efficiency is about two times higher than without the injection seeding. The improved specific laser output is 8 W/cm3, therefore, a discharge volume of 125 cm3 will be able to generate the peak laser power reaching 1 kW. This power value is sufficient to obtain the same treatment effect as the gold vapor laser used in photodynamic therapy. Moreover, by fitting this model to the experimental results of the laser output energy with a Ne/D2 mixture, it is shown that the Penning ionization rate constant of H2 is larger than that of D2. © 1995 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 75 (1994), S. 2115-2118 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Interfilament contact in Nb3Sn wires made by the internal-tin-diffusion process causes excess hysteresis loss beyond the intrinsic magnetic hysteresis loss of the filaments. In analogy with eddy-current and proximity-effect coupling losses, the excess contact loss can be reduced by decreasing the twist-pitch length of the filaments in the wire. One consequence of interfilament contact is that volume magnetization measurements are strongly dependent on sample length below about one twist pitch. We define a characteristic length whose reciprocal is equal to the sum of the reciprocals of the sample length and the twist pitch. Hysteresis loss is a universal function of characteristic length for different sample lengths and twist pitches. We discuss several experimental parameters for the magnetic determination of hysteresis loss.
    Type of Medium: Electronic Resource
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  • 5
    ISSN: 1520-4995
    Source: ACS Legacy Archives
    Topics: Biology , Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 63 (1988), S. 2167-2170 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The measurements of ρn (the normal state resistivity), Tc, Hc2, and (dHc2/dt)T=Tc have been made for bronze-processed Nb3Sn wires with addition of Ti to the Cu-Sn matrix in order to study the mechanism of Hc2 enhancement due to the addition of Ti. The coefficient of electron specific heat, γ, has been derived by two independent methods: one using the Ginzburg–Landau–Abrikosov–Gor'kov (GLAG) theory and the measured values of ρn, Tc, and (dHc2/dT)T=Tc, and the other using the Kramer pinning theory and the gradient of J1/2cH1/4 -H curves. The ratios of γ/γ0 which have been derived by these two methods are in good agreement with each other. (γ0 is the value of γ for the specimen to which Ti is not added.) The upper critical fields given by the GLAG theory, H@B|c2 and Hc2, at 0 K increase rapidly with Ti concentration in the Nb3Sn layer up to 2 at. % and decrease slightly above 2 at. %. The rapid increase in ρnγTc caused by the addition of Ti is sufficient to explain the enhancement in Hc2, and among ρn, γ and Tc, only ρn shows a significant increase with increasing amounts of additional Ti, indicating that the main reason for the Hc2 enhancement is the increase in ρn.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 68 (1990), S. 2164-2167 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The growth process in the initial stage of growth of Ge films on (811)Si substrate surfaces by GeH4 source molecular-beam epitaxy has been studied by in situ reflection high-energy electron diffraction observation. It has been found that a strained film by the monolayer overgrowth mode is formed initially with an epitaxial relationship of the parallel orientation, and that plate-shaped Ge islands with (811) facets are grown early in the growth, but that the predominant facet changes to {311} and the (100) planes with further growth. These growth processes are similar to those of Ge films on (100)Si surfaces reported previously. It is concluded that Ge islands with {811} facets are energetically stable in the initial stage of the island growth on the (811)Si surfaces as well as on the (100)Si surfaces.
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  • 8
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Magnetization and Mössbauer measurements were performed for PuNi3 type alloys Y(Fe1−xCox)2.9 and their hydrides. The composition dependencies of magnetization, Curie temperature, and average hyperfine field of 57Fe in the alloys show a maximum near x=0.5, and those in hydrides decrease with increasing x. This behavior suggests that the magnetic moments of iron and cobalt are nearly the same, except for cobalt rich alloys. Numerical fitting using a Stoner theory with a parabolic band was performed. It was assumed that the alloys and hydrides are ferromagnets of 3d-band-hole with incomplete saturation. It was shown that both the exchange energy kθ and Fermi energy ε0 decrease with substitution of cobalt for iron, and that the difference in the composition dependencies of kθ/ε0 in alloys and hydrides leads to different composition dependencies of the magnetization and Curie temperature. It was shown that ε0 and kθ decrease with hydrogenation, but kθ/ε0 increases to lead magnetization increase only in YFe3. © 1997 American Institute of Physics.
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  • 9
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 85 (1999), S. 8193-8198 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: We report on calculations of the anisotropy of the electron Hall mobility and its temperature dependence in n-type 6H–SiC. The model is based on the conduction band structure determined recently by a first-principle calculation. It provides explicit and easy to use analytical expressions for both drift and Hall mobilities. The calculation of the Hall mobility based on our model agrees very well with experimentally determined anisotropic Hall mobility in 6H–SiC. © 1999 American Institute of Physics.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Physics of Plasmas 5 (1998), S. 4121-4123 
    ISSN: 1089-7674
    Source: AIP Digital Archive
    Topics: Physics
    Notes: The solitary structure solution of the radial electric field Er in the tokamak plasmas is obtained. It is shown to be stable under an external power supply, like a biased electrode at the edge. The radial gradient is governed by the ion viscosity and the nonlinearlity of the perpendicular conductivity. The radial structure of Er and reduction of turbulent transport, which belong to key issues of the high confinement mode (H-Mode) [F. Wagner et al., Phys. Rev. Lett. 49, 1408 (1982)], are self-consistently determined. A bifurcation from a radially-uniform one to a solitary one occurs at a certain applied voltage, and a hysteresis is associated. © 1998 American Institute of Physics.
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