Relaxation Model for Extended Magnetohydrodynamics

Relaxation Model for Extended Magnetohydrodynamics
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Total Pages:
Release: 2011
Genre:
ISBN:

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It is shown that the two-fluid model under a generalized Ohm's law formulation and the resistive magnetohydrodynamics (MHD) can both be described as relaxation systems. In the relaxation model, the under-resolved stiff source terms constrain the dynamics of a set of hyperbolic equations to give the correct asymptotic solution. When applied to the collisional two-fluid model, the relaxation of fast time scales associated with displacement current and finite electron mass allows for a natural transition from a system where Ohm's law determines the current density to a system where Ohm's law determines the electric field. This result is used to derive novel algorithms, which allow for multiscale simulation of low and high frequency extended-MHD physics. This relaxation formulation offers an efficient way to implicitly advance the Hall term and naturally simulate a plasma-vacuum interface without invoking phenomenological models. The relaxation model is implemented as an extended-MHD code, which is used to analyze pulsed power loads such as wire arrays and ablating foils. Two-dimensional simulations of pulsed power loads are compared for extended-MHD and MHD. For these simulations, it is also shown that the relaxation model properly recovers the resistive-MHD limit.

Lectures in Magnetohydrodynamics

Lectures in Magnetohydrodynamics
Author: Dalton D. Schnack
Publisher: Springer
Total Pages: 317
Release: 2009-08-11
Genre: Science
ISBN: 3642006884

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Magnetohydrodynamics, or MHD, is a theoretical way of describing the statics and dynamics of electrically conducting uids. The most important of these uids occurring in both nature and the laboratory are ionized gases, called plasmas. These have the simultaneous properties of conducting electricity and being electrically charge neutral on almost all length scales. The study of these gases is called plasma physics. MHD is the poor cousin of plasma physics. It is the simplest theory of plasma dynamics. In most introductory courses, it is usually afforded a short chapter or lecture at most: Alfven ́ waves, the kink mode, and that is it. (Now, on to Landau damping!) In advanced plasma courses, such as those dealing with waves or kinetic theory, it is given an even more cursory treatment, a brief mention on the way to things more profound and interesting. (It is just MHD! Besides, real plasma phy- cists do kinetic theory!) Nonetheless, MHD is an indispensable tool in all applications of plasma physics.

Extended Magnetohydrodynamic Modeling of Plasma Relaxation Dynamics in the Reversed-field Pinch

Extended Magnetohydrodynamic Modeling of Plasma Relaxation Dynamics in the Reversed-field Pinch
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Publisher:
Total Pages: 0
Release: 2015
Genre:
ISBN:

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Nonlinear plasma relaxation dynamics in reversed-field pinch (RFP) conditions are investigated using extended magnetohydrodynamic modeling with the NIMROD code [Sovinec et. al. JCP 195 (2004)]. The computations display quasi-periodic relaxation events, consistent with the RFP sawtooth cycle. The first event occurs from a saturated single-helicity state and is not representative of the multi-helicity conditions in typical RFP discharges. The MHD and Hall dynamo electric fields cooperate during the initial relaxation, and the change in the plasma flow parallel to the magnetic field is in the direction of the Lorentz force density and opposite to the change in parallel current density. In subsequent events, the MHD dynamo relaxes the parallel current and is opposed by the Hall dynamo, which is smaller in magnitude. The associated Lorentz force density drives changes in flow that are in the same direction as the change in current, in agreement with experimental observations [Kuritsyn et. al. POP 055903 (2009)]. Changes in total momentum are due to viscous coupling to the wall; radial transport occurs through Maxwell stresses associated with current relaxation. The magnetic and hybrid helicity are well conserved relative to magnetic energy over the relaxation events. The helicities change by

Shock Study with an Extended-MHD Model Using a Positivity-preserving Semi-implicit Discontinuous Galerkin Scheme

Shock Study with an Extended-MHD Model Using a Positivity-preserving Semi-implicit Discontinuous Galerkin Scheme
Author: Xuan Zhao
Publisher:
Total Pages: 221
Release: 2015
Genre:
ISBN:

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A positivity-preserving discontinuous Galerkin (DG) scheme (Zhang, X. & Shu, C.W., J. Comp. Phys., 229(23), 8918-8934.) is used to solve the Extended Magnetohydrodynamics (XMHD) model, which is a two-fluid model expressed with a center-of-mass formulation. We prove that the DG scheme with a positivitypreserving limiter is stable for the system governed by the XMHD model or the resistive MHD model. We use the relaxation system formulation (Seyler, C.E., & Martin, M.R. Physics of Plasmas, 18, 012703.) for describing the XMHD model, and solve the equations using a split level implicit-explicit time advance scheme, stepping over the time step constraint imposed by the stiff source terms. The magnetic field is represented in an exact locally divergence-free form of DG (Li, F., & Shu, C.W. 22(1-3), 413-442.), which greatly improves the accuracy and stability of MHD simulations. As presently constructed, the method is able to handle a wide range of density variation, solve the XMHD model on MHD time scales, and provide greatly improved accuracy over a Finite Volume implementation of the same model. The extended-MHD code DG-PERSEUS, which is an implementation of this method on a 3D Cartesian coordinates, has been applied to the study of the magnetized shock in the context where a magnetized flow is interacting with a solid obstacle. Several physics issues are found to be associated with this problem, such as bow shock, reconnection, plasmoids, which have been studied. The inflow parameters, such as the magnetosonic mach number M f and the ratio of thermal pressure to magnetic pressure [beta] can significantly affect the physical structures of the flow-obstacle interaction, which can be used as a diagnostic tool for the flow. The Hall effect can also significantly influence the results. Interplanetary physics - the solar wind interacting with Mars - is also studied. Simulations are carried out to show that the interplanetary features (bow shock, reconnection) can also be achieved with laboratory parameters.

Lectures in Magnetohydrodynamics

Lectures in Magnetohydrodynamics
Author: Dalton D. Schnack
Publisher: Springer Science & Business Media
Total Pages: 317
Release: 2009-08-26
Genre: Science
ISBN: 3642006876

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Magnetohydrodynamics, or MHD, is a theoretical way of describing the statics and dynamics of electrically conducting uids. The most important of these uids occurring in both nature and the laboratory are ionized gases, called plasmas. These have the simultaneous properties of conducting electricity and being electrically charge neutral on almost all length scales. The study of these gases is called plasma physics. MHD is the poor cousin of plasma physics. It is the simplest theory of plasma dynamics. In most introductory courses, it is usually afforded a short chapter or lecture at most: Alfven ́ waves, the kink mode, and that is it. (Now, on to Landau damping!) In advanced plasma courses, such as those dealing with waves or kinetic theory, it is given an even more cursory treatment, a brief mention on the way to things more profound and interesting. (It is just MHD! Besides, real plasma phy- cists do kinetic theory!) Nonetheless, MHD is an indispensable tool in all applications of plasma physics.

Magnetohydrodynamics of Plasma Relaxation

Magnetohydrodynamics of Plasma Relaxation
Author: S. Ortolani
Publisher: World Scientific
Total Pages: 208
Release: 1993
Genre: Science
ISBN: 9789810208608

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This book gives a concise description of the phenomenon of plasma relaxation from the point of view of resistive magnetohydrodynamic (MHD) theory. Magnetized plasmas relax when they seek their natural state of lowest energy subject to certain topological constraints imposed by the magnetic field. Relaxation may be fast and dynamic or slow and gradual depending on the external environment in which the magnetoplasma system evolves. Relaxation occurs throughout the universe and may describe such diverse phenomena as dynamos, solar flares, and the operation of magnetic fusion energy experiments. This book concentrates on the dynamic, rather than variational aspects of relaxation. While the processes described are general, the book focuses on the reversed-field pinch experiment as a paradigm for plasma relaxation and dynamo action. Examples from other branches of plasma physics are also discussed. The authors draw upon their extensive experience in numerical and experimental studies of relaxation.

Development of a Multifluid Magnetohydrodynamic Model for Anisotropic, Partially Ionized Plasmas

Development of a Multifluid Magnetohydrodynamic Model for Anisotropic, Partially Ionized Plasmas
Author: Ken Miura
Publisher:
Total Pages: 0
Release: 2019
Genre:
ISBN:

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A multifluid magnetohydrodynamic (MHD) model based on an extended fluid dynamics description for each plasma species is proposed for the prediction of the flow and behaviour of fully and partially ionized non-equilibrium anisotropic plasmas. Two-(electrons and ions) and three-fluid (ions, electrons and neutrals) plasma models are described that both make use of a 10-moment or Gaussian anisotropic moment closure of the Boltzmann equation. The moment equations for each plasma species are fully coupled to the Maxwell's equations which govern electromagnetic wave propagation within the plasma and a Bhatnagar-Gross-Krook (BGK) relaxation time approximation is used to model non-equilibrium collisional processes between the plasma species. Chemical kinetic models are included to represent the partially ionized plasma processes. Unlike conventional MHD models, the proposed multi-species MHD model is capable of taking into account large temperature anisotropies and temperature differences between the electrons and ions, both of which can occur for low-density, high-temperature plasmas and/or strongly magnetized plasmas. A second-order Godunov-type finite-volume method is developed for the solution of the one- and two-dimensional forms of the multifluid plasma models, which includes temporal limiting in one-dimension and a parallel scheme utilizing a Newton-Krylov-Schwarz (NKS) implicit algorithm for the two-dimensional solution procedure. The numerical fluxes in the Godunov-type scheme are solved using HLLE and Godunov numerical flux functions. The two-dimensional solution procedure includes Generalized Lagrange Multiplier (GLM) and diffusive error correction schemes for the treatment of divergence errors associated with the electromagnetic field. An accuracy assessment is performed for the two-dimensional numerical solution procedure, demonstrating good convergence of solutions for a range of problems. The validated two-dimensional solution procedure for the multifluid MHD model is then applied to the solution of the well-known Geospace Environmental Modelling (GEM) challenge problem involving magnetic field reconnection and numerical results are compared to established solutions in the literature. Results of grid refinement and parametric studies for the GEM case are also described. The proposed multifluid MHD model is shown to recover known published results with relatively small computational effort and the potential of the proposed treatment for describing a range of non-equilibrium anisotropic plasma flows is demonstrated.

Center for Extended Magnetohydrodynamic Modeling Cooperative Agreement

Center for Extended Magnetohydrodynamic Modeling Cooperative Agreement
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Total Pages:
Release: 2008
Genre:
ISBN:

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The Center for Extended Magnetohydrodynamic Modeling (CEMM) is developing computer simulation models for predicting the behavior of magnetically confined plasmas. Over the first phase of support from the Department of Energy's Scientific Discovery through Advanced Computing (SciDAC) initiative, the focus has been on macroscopic dynamics that alter the confinement properties of magnetic field configurations. The ultimate objective is to provide computational capabilities to predict plasma behavior--not unlike computational weather prediction--to optimize performance and to increase the reliability of magnetic confinement for fusion energy. Numerical modeling aids theoretical research by solving complicated mathematical models of plasma behavior including strong nonlinear effects and the influences of geometrical shaping of actual experiments. The numerical modeling itself remains an area of active research, due to challenges associated with simulating multiple temporal and spatial scales. The research summarized in this report spans computational and physical topics associated with state of the art simulation of magnetized plasmas. The tasks performed for this grant are categorized according to whether they are primarily computational, algorithmic, or application-oriented in nature. All involve the development and use of the Non-Ideal Magnetohydrodynamics with Rotation, Open Discussion (NIMROD) code, which is described at http://nimrodteam.org. With respect to computation, we have tested and refined methods for solving the large algebraic systems of equations that result from our numerical approximations of the physical model. Collaboration with the Terascale Optimal PDE Solvers (TOPS) SciDAC center led us to the SuperLU_DIST software library [http://crd.lbl.gov/~xiaoye/SuperLU/] for solving large sparse matrices using direct methods on parallel computers. Switching to this solver library boosted NIMROD's performance by a factor of five in typical large nonlinear simulations, which has been publicized as a success story of SciDAC-fostered collaboration. Furthermore, the SuperLU software does not assume any mathematical symmetry, and its generality provides an important capability for extending the physical model beyond magnetohydrodynamics (MHD). With respect to algorithmic and model development, our most significant accomplishment is the development of a new method for solving plasma models that treat electrons as an independent plasma component. These 'two-fluid' models encompass MHD and add temporal and spatial scales that are beyond the response of the ion species. Implementation and testing of a previously published algorithm did not prove successful for NIMROD, and the new algorithm has since been devised, analyzed, and implemented. Two-fluid modeling, an important objective of the original NIMROD project, is now routine in 2D applications. Algorithmic components for 3D modeling are in place and tested; though, further computational work is still needed for efficiency. Other algorithmic work extends the ion-fluid stress tensor to include models for parallel and gyroviscous stresses. In addition, our hot-particle simulation capability received important refinements that permitted completion of a benchmark with the M3D code. A highlight of our applications work is the edge-localized mode (ELM) modeling, which was part of the first-ever computational Performance Target for the DOE Office of Fusion Energy Science, see http://www.science.doe.gov/ofes/performancetargets.shtml. Our efforts allowed MHD simulations to progress late into the nonlinear stage, where energy is conducted to the wall location. They also produced a two-fluid ELM simulation starting from experimental information and demonstrating critical drift effects that are characteristic of two-fluid physics. Another important application is the internal kink mode in a tokamak. Here, the primary purpose of the study has been to benchmark the two main code development lines of CEMM, NIMROD and M3D, on a relevant nonlinear problem. Results from the two codes show repeating nonlinear relaxation events driven by the kink mode over quantitatively comparable timescales. The work has launched a more comprehensive nonlinear benchmarking exercise, where realistic transport effects have an important role.

Monolithic Multigrid Methods for Two-dimensional Resistive Magnetohydrodynamics

Monolithic Multigrid Methods for Two-dimensional Resistive Magnetohydrodynamics
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Publisher:
Total Pages: 24
Release: 2016
Genre:
ISBN:

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Magnetohydrodynamic (MHD) representations are used to model a wide range of plasma physics applications and are characterized by a nonlinear system of partial differential equations that strongly couples a charged fluid with the evolution of electromagnetic fields. The resulting linear systems that arise from discretization and linearization of the nonlinear problem are generally difficult to solve. In this paper, we investigate multigrid preconditioners for this system. We consider two well-known multigrid relaxation methods for incompressible fluid dynamics: Braess--Sarazin relaxation and Vanka relaxation. We first extend these to the context of steady-state one-fluid viscoresistive MHD. Then we compare the two relaxation procedures within a multigrid-preconditioned GMRES method employed within Newton's method. To isolate the effects of the different relaxation methods, we use structured grids, inf-sup stable finite elements, and geometric interpolation. Furthermore, we present convergence and timing results for a two-dimensional, steady-state test problem.

Multi-scale Dynamical Processes in Space and Astrophysical Plasmas

Multi-scale Dynamical Processes in Space and Astrophysical Plasmas
Author: Manfred P. Leubner
Publisher: Springer Science & Business Media
Total Pages: 230
Release: 2012-08-01
Genre: Science
ISBN: 3642304419

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Magnetized plasmas in the universe exhibit complex dynamical behavior over a huge range of scales. The fundamental mechanisms of energy transport, redistribution and conversion occur at multiple scales. The driving mechanisms often include energy accumulation, free-energy-excited relaxation processes, dissipation and self-organization. The plasma processes associated with energy conversion, transport and self-organization, such as magnetic reconnection, instabilities, linear and nonlinear waves, wave-particle interactions, dynamo processes, turbulence, heating, diffusion and convection represent fundamental physical effects. They demonstrate similar dynamical behavior in near-Earth space, on the Sun, in the heliosphere and in astrophysical environments. 'Multi-scale Dynamical Processes in Space and Astrophysical Plasmas' presents the proceedings of the International Astrophysics Forum Alpbach 2011. The contributions discuss the latest advances in the exploration of dynamical behavior in space plasmas environments, including comprehensive approaches to theoretical, experimental and numerical aspects. The book will appeal to researchers and students in the fields of physics, space and astrophysics, solar physics, geophysics and planetary science.