Test Cases for Grid-Based Direct Kinetic Modeling of Plasma Flows
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Verification of Gyrokinetic Codes: Theoretical Background & Numerical Implementations
N.Tronko 1, T.Goerler 2 , A.Bottino 2 , B.D.Scott 2, E.Sonnendrücker 1 Verification of Gyrokinetic codes: Theoretical background & Numerical implementations NumKin 2016, IRMA, Strasbourg, France 1 NMPP, Max Planck Institute für Plasmaphysik 2 TOK, Max Planck Institute für Plasmaphysik VeriGyro Project Participants Enabling Research Project on Verification of Gyrokinetic codes • Germany! Max Planck Insitute for Plasma Physics (Garching and Greifswald) • Switzerland SPC-EPFL, Lausanne • Finland! Aalto Univeristy • Great Britain University of Warwick • France CEA Cadarache, Université Paris IV, Rennes, Toulouse, Lorraine, Bretagne IRMA, Maison de la Simulation (Saclay) • USA Saint Michel’s College, VT NumKin 2016 VeriGyro Project @ IPP Garching Interdisciplinary Project in IPP Max Planck (Garching) NMPP Division (Numerical Methods for Plasma Physics) • Development and implementation of new algorithms for fusion and astrophysical plasma modeling • Development of libraries (i.e. Selalib) • Verification of existing codes • Participants: N. Tronko, E. Sonnendrücker Enabling Research Project VeriGyro TOK (Tokamak Theory) • Development of major codes • Plasma modeling and comparison with experimental results (ASDEX Upgrade) • Participants: T. Görler, A. Bottino, B. D. Scott NumKin 2016 VeriGyro Project: Motivation • Verification of Global (Electromagnetic) Gyrokinetic codes: Why? • Most popular tools for magnetised plasmas simulations: • Significant Development since last 10 years • Electrostatic gyrokinetic implementations : well established ! [Dimits -
1 the Derivation of Particle Monte Carlo Methods for Plasma Modeling
The derivation of Particle Monte Carlo methods for plasma modeling from transport equations. Savino Longo Dipartimento di Chimica dell'Università and CNR/IMIP, Via Orabona 4, 70126 Bari, Italy. e-mail: [email protected] Abstract: We analyze here in some detail, the derivation of the Particle and Monte Carlo methods of plasma simulation, such as Particle in Cell (PIC), Monte Carlo (MC) and Particle in Cell / Monte Carlo (PIC/MC) from formal manipulation of transport equations. Keywords: Charged Particle Transport, Boltzmann Equation, Monte Carlo Methods, Particle-in-Cell, Vlasov/Boltzmann equation 1 1.Introduction An accurate calculation of the velocity distribution of charged particles in non equilibrium plasmas is necessary in order to evaluate the rate at which collisional elementary processes take place in these media as well as their transport properties [1]. In doing so, one has to take into account the effect of inertia, scattering, externally applied and self-coherent fields, all affecting the particle transport. To this aim, different particle simulation techniques have been used extensively, as an alternative to the grid-based solution of transport equations [1] by finite differences or finite element techniques. To these belong the very well-know Test Particle Monte Carlo (TPMC, or simply Monte Carlo, MC [1]), the Particle in Cell (PIC [2,3]) and Particle in Cell / Monte Carlo methods (PIC/MC [4]). No explicit description of the methods will be given here because of their widespread application within the plasma modelling community, and we assume in the following that they are already known to the reader. -
A Truncation Error Analysis of Third-Order MUSCL Scheme for Nonlinear Conservation Laws
A Truncation Error Analysis of Third-Order MUSCL Scheme for Nonlinear Conservation Laws Hiroaki Nishikawa∗ National Institute of Aerospace, Hampton, VA 23666, USA Abstract This paper is a rebuttal to the claim found in the literature that the MUSCL scheme cannot be third-order accurate for nonlinear conservation laws. We provide a rigorous proof for third-order accuracy of the MUSCL scheme based on a careful and detailed truncation error analysis. Throughout the analysis, the distinction between the cell average and the point value will be strictly made for the numerical solution as well as for the target operator. It is shown that the average of the solutions reconstructed at a face by Van Leer’s κ-scheme recovers a cubic solution exactly with κ = 1/3, the same is true for the average of the nonlinear fluxes evaluated by the reconstructed solutions, and a dissipation term is already sufficiently small with a third-order truncation error. Finally, noting that the target spatial operator is a cell-averaged flux derivative, we prove that the leading truncation error of the MUSCL finite-volume scheme is third-order with κ = 1/3. The importance of the diffusion scheme is also discussed: third-order accuracy will be lost when the third-order MUSLC scheme is used with a wrong fourth-order diffusion scheme for convection-diffusion problems. Third-order accuracy is verified by thorough numerical experiments for both steady and unsteady problems. This paper is intended to serve as a reference to clarify confusions about third-order accuracy of the MUSCL scheme, as a guide to correctly analyze and verify the MUSCL scheme for nonlinear equations, and eventually as the basis for clarifying third-order unstructured-grid schemes in a subsequent paper. -
The QUICK Scheme Is a Third-Order Finite-Volume Scheme with Point
The QUICK Scheme is a Third-Order Finite-Volume Scheme with Point-Valued Numerical Solutions Hiroaki Nishikawa∗ National Institute of Aerospace, Hampton, VA 23666, USA June 30, 2020 Abstract In this paper, we resolve the ever-present confusion over the QUICK scheme: it is a second-order scheme or a third-order scheme. The QUICK scheme, as proposed in the original reference [B. P. Leonard, Comput. Methods. Appl. Mech. Eng., 19, (1979), 59-98], is a third-order (not second-order) finite-volume scheme for the integral form of a general nonlinear conservation law with point-valued solutions stored at cell centers as numerical solutions. Third-order accuracy is proved by a careful and detailed truncation error analysis and demonstrated by a series of thorough numerical tests. The QUICK scheme requires a careful spatial discretization of a time derivative to preserve third-order accuracy for unsteady problems. Two techniques are discussed, including the QUICKEST scheme of Leonard. Discussions are given on how the QUICK scheme is mistakenly found to be second-order accurate. This paper is intended to serve as a reference to clarify any confusion about third-order accuracy of the QUICK scheme and also as the basis for clarifying economical high-order unstructured- grid schemes as we will discuss in a subsequent paper. 1 Introduction This paper is a sequel to the previous paper [1], where we discussed the third-order MUSCL scheme. The main motivation behind this work is to clarify some economical high-order unstructured-grid finite-volume schemes used in practical computational fluid dynamics solvers but largely confused in their mechanisms to achieve third- and possibly higher-order accuracy (e.g., third-order U-MUSCL with κ =1/2 [2], κ =1/3 [3, 4], κ = 0 [5, 6]). -
Finite-Volume Simulations of Maxwell's Equations On
Finite-Volume Simulations of Maxwell's Equations on Unstructured Grids Ian Jeffrey PhD Thesis Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy Department of Electrical and Computer Engineering University of Manitoba Winnipeg, Manitoba, Canada Copyright c 2011 by Ian Jeffrey Abstract Herein a fully parallel, upwind and flux-split Finite-Volume Time-Domain (FVTD) numerical engine for solving Maxwell's Equations on unstructured grids is developed. The required background theory for solving Maxwell's Equations using FVTD is given in sufficient detail, including a description of both the temporal and spatial approx- imations used. The details of the local-time stepping strategy of Fumeaux et al. is included. A global mesh-truncation scheme using field integration over a Huygens' surface is also presented. The capabilities of the FVTD algorithm are augmented with thin-wire and subcell circuit models that permit very flexible and accurate simulations of circuit-driven wire structures. Numerical and experimental validation shows that the proposed models have a wide-range of applications. Specifically, it appears that the thin-wire and subcell circuit models may be very well suited to the simulation of radio-frequency coils used in magnetic resonance imaging systems. A parallelization scheme for the volumetric field solver, combined with the local-time stepping, global mesh-truncation and subcell models is developed that theoretically provides both linear time- and memory scaling in a distributed parallel environment. Finally, the FVTD code is converted to the frequency domain and the possibility of using different flux-reconstruction schemes to improve the iterative convergence of the Finite-Volume Frequency-Domain algorithm is investigated. -
Computational Plasma Physics
Computational plasma physics S. Possanner and E. Sonnendr¨ucker Max-Planck-Institut f¨urPlasmaphysik und Zentrum Mathematik, TU M¨unchen Lecture notes Sommersemester 2019 April 26, 2019 Contents 1 Introduction2 1.1 Scientific computing..........................2 1.2 Plasmas.................................4 1.3 Model equations.............................4 1.3.1 The N-body model.......................6 1.3.2 Kinetic models.........................7 1.3.3 Fluid models..........................9 1 Chapter 1 Introduction 1.1 Scientific computing Understanding an experiment in physics relies on a model which is generally a differential equation or a partial differential equation or a system involving many of these. In sufficiently simple cases analytical solutions of these models exist and then this can be used to predict the behaviour of a similar experiment. However in many cases, especially when the model is based on first principles, it is so complex that there is no analytical solution available. Then there are two options: the first is to simplify the model until it can be analytically solved, the second is to compute an approximate solution using a computer. In practice both are usually done, the simplified models being used to verify that the code is working properly. Due to the enormous development of computer resources in the last 50 years, quite realistic simulations of physical problems become now possible. A large amount of theoretical work in physics and related disciplines, in particular in plasma physics, now relies quite heavily on numerical simulation. Computational sciences have emerged next to theory and experiments as a third pillar in physics and engineering. Designing efficient, robust and accurate simulation codes is a challenging task that is at the interface of the application domain, plasma physics in our case, applied mathematics and computer science. -
Computational Modeling of Fully Ionized Magnetized Plasmas Using the fluid Approximationa…
PHYSICS OF PLASMAS 13, 058103 ͑2006͒ Computational modeling of fully ionized magnetized plasmas using the fluid approximationa… ͒ D. D. Schnackb Center for Energy and Space Science, Science Applications International Corporation, 10260 Campus Point Drive, San Diego, California 92121 D. C. Barnes Center for Integrated Plasma Studies, University of Colorado, 2000 Colorado Avenue, Boulder, Colorado 80309 D. P. Brennan General Atomics, P.O. Box 85608, San Diego, California 92186 C. C. Hegna Department of Engineering Physics, University of Wisconsin, 1500 Engineering Drive, Madison, Wisconsin 53706 E. Held Department of Physics, Utah State University, Logan, Utah 84322 C. C. Kim Department of Engineering Physics, University of Wisconsin, 1500 Engineering Drive, Madison, Wisconsin 53706 and Plasma Science and Innovation Center, University of Washington, P.O. Box 352250, Seattle, Washington 98195 S. E. Kruger TechX Corporation, 5621 Arapahoe Avenue, Suite A, Boulder, Colorado 80303 A. Y. Pankin Center for Energy and Space Science, Science Applications International Corporation, 10260 Campus Point Drive, San Diego, California 92121 C. R. Sovinec Department of Engineering Physics, University of Wisconsin, 1500 Engineering Drive, Madison, Wisconsin 53706 ͑Received 20 October 2005; accepted 6 January 2006; published online 11 May 2006͒ Strongly magnetized plasmas are rich in spatial and temporal scales, making a computational approach useful for studying these systems. The most accurate model of a magnetized plasma is based on a kinetic equation that describes the evolution of the distribution function for each species in six-dimensional phase space. High dimensionality renders this approach impractical for computations for long time scales. Fluid models are an approximation to the kinetic model. -
Méthode De Décomposition De Domaine Avec Adaptation De
UNIVERSIT E´ PARIS 13 No attribu´epar la biblioth`eque TH ESE` pour obtenir le grade de DOCTEUR DE L’UNIVERSIT E´ PARIS 13 Discipline: Math´ematiques Appliqu´ees Laboratoire d’accueil: ONERA - Le centre fran¸cais de recherche a´erospatiale Pr´esent´ee et soutenue publiquement le 19 d´ecembre 2014 par Oana Alexandra CIOBANU Titre M´ethode de d´ecomposition de domaine avec adaptation de maillage en espace-temps pour les ´equations d’Euler et de Navier–Stokes devant le jury compos´ede: Fran¸cois Dubois Rapporteur Laurence Halpern Directrice de th`ese Rapha`ele Herbin Rapporteure Xavier Juvigny Examinateur Olivier Lafitte Examinateur Juliette Ryan Encadrante UNIVERSITY PARIS 13 THESIS Presented for the degree of DOCTEUR DE L’UNIVERSIT E´ PARIS 13 In Applied Mathematics Hosting laboratory: ONERA - The French Aerospace Lab presented for public discussion on 19 decembre 2014 by Oana Alexandra CIOBANU Subject Adaptive Space-Time Domain Decomposition Methods for Euler and Navier–Stokes Equations Jury: Fran¸cois Dubois Reviewer Laurence Halpern Supervisor Rapha`ele Herbin Reviewer Xavier Juvigny Examiner Olivier Lafitte Examiner Juliette Ryan Supervisor newpage Remerciements Tout d’abord, je remercie grandement Juliette Ryan pour avoir accept´e d’ˆetre mon encad- rante de stage puis mon encadrante de th`ese. Pendant plus de trois ans, elle m’a fait d´ecouvrir mon m´etier de jeune chercheuse avec beaucoup de patience et de professionnalisme. Elle m’a soutenue, elle a ´et´ed’une disponibilit´eet d’une ´ecoute extraordinaires, tout en sachant ˆetre rigoureuse et exigeante avec moi comme avec elle-mˆeme. Humainement, j’ai beaucoup appr´eci´e la relation d’amiti´eque nous avons entretenue, le climat de confiance que nous avons maintenu et les discussions extra-math´ematiques que nous avons pu avoir et qui ont renforc´ele lien que nous avions. -
Particle-In-Cell Simulations of Highly Collisional Plasmas on the GPU in 1 and 2 Dimensions
Particle-In-Cell Simulations Of Highly Collisional Plasmas On The GPU In 1 And 2 Dimensions A thesis for the degree of PHILOSOPHIAE DOCTOR Presented to DUBLIN CITY UNIVERSITY By Nina Hanzlikova B.Sc. School of Physical Sciences Dublin City University Research Supervisor: Prof. Miles M. Turner March 2015 Declaration I hereby certify that this material, which I now submit for assessment on the programme of study leading to the award of Philosophiae Doctor is entirely my own work, and that I have exercised reasonable care to ensure that the work is original, and does not to the best of my knowledge breach any law of copyright, and has not been taken from the work of others save and to the extent that such work has been cited and acknowledged within the text of my work. Signed: ........................................................ Nina Hanzlikova ID No.: 56459501 Date: 27th December 2014 Contents List of Figures xii List of Symbols xiii 1 Introduction 1 1.1 Overview . 2 1.2 Plasma Fundamentals . 4 1.2.1 Debye Length . 4 1.2.2 Plasma Frequency . 5 1.2.3 Collisions . 7 1.2.4 Diffusion . 9 1.2.5 Plasma Sheath . 11 1.2.6 Driving Potential and Heating . 14 1.3 Atmospheric Pressure Plasmas . 15 1.3.1 Atmospheric Plasma Sources . 15 1.3.2 Atmospheric Plasma Characteristics . 16 ii CONTENTS 1.4 Plasma Modelling . 21 1.4.1 Particle Modelling . 22 1.4.2 Atmospheric Plasma Modelling . 23 1.5 Chapter Summary . 25 2 Introduction To High Performance Computing 27 2.1 Graphical Processing Unit (GPU) . -
Semiclassical Modeling of Multiparticle Quantum Mechanics
UNIVERSITY OF CALIFORNIA Los Angeles Semiclassical Modeling of Quantum-Mechanical Multiparticle Systems using Parallel Particle-In-Cell Methods A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Physics by Dean Edward Dauger 2001 © Copyright by Dean Edward Dauger 2001 To my parents, Alan and Marlene, who were always fully supportive of my work and my endeavors. And Charlie and Allegra, my cats. And to all those who have a vision, a dream of something new and inspiring, to express that Idea, limited only by its own conclusion if it has one. iii Contents I. Introduction A. Motivation ···················································································1 B. Existing Methods ···················································································6 C. Outline ···················································································8 D. Conventions ···················································································9 II. Theory A. The Approach ·················································································11 B. Feynman Path Integrals···············································································13 C. The Semiclassical Approximation·······························································18 D. Initial Position and Final Momentum·························································21 E. The Matrix ··················································································23 F. The Determinant -
A Comparison of High-Resolution, Finite-Volume, Adaptive±Stencil
Advances in Water Resources 24 (2001) 29±48 www.elsevier.com/locate/advwatres A comparison of high-resolution, ®nite-volume, adaptive±stencil schemes for simulating advective±dispersive transport Matthew W. Farthing, Cass T. Miller * Department of Environmental Sciences and Engineering, Center for the Advanced Study of the Environment, University of North Carolina, Chapel Hill, NC 27599-7400, USA Received 1 February 2000; received in revised form 8 May 2000; accepted 16 May 2000 Abstract We investigate a set of adaptive±stencil, ®nite-volume schemes used to capture sharp fronts and shocks in a wide range of ®elds. Our objective is to determine the most promising methods available from this set for solving sharp-front advective±dispersive transport problems. Schemes are evaluated for a range of initial conditions, and for Peclet and Courant numbers. Based upon results from this work, we identify the most promising schemes based on eciency and robustness. Ó 2000 Elsevier Science Ltd. All rights reserved. 1. Introduction ecient for solving relatively simple advective-domi- nated problems. These approaches, however, can pose The processes of solute and energy transport in nat- mass conservation problems, are not well suited for ural systems are most often described using an advec- problems with multiple sources and non-linear mass tive±dispersive equation (ADE) with additional terms transfer terms, and can be diusive and oscillatory for sources, reactions, and interphase exchange of mass [3,19,38,44]. or energy [34]. For many problems, especially those in- Over the last decade, simulators in the water re- volving multiple species, ADE solutions can be a sub- sources ®eld have employed so-called high-resolution stantial part of the computational eort involved for a methods more and more for discretizing the advective given ¯ow and transport simulator. -
New Roe Scheme for All Speed Flow
Role of Momentum Interpolation Mechanism of the Roe Scheme in Shock Instability Xiao-dong Ren1,2 Chun-wei Gu1 Xue-song Li1,* 1. Key Laboratory for Thermal Science and Power Engineering of Ministry of Education, Department of Thermal Engineering, Tsinghua University, Beijing 100084, PR China 2. Department of Mathematics, School of Science, Hong Kong University of Science and Technology, Hong Kong, China Abstract: The shock instability phenomenon is a famous problem for the shock-capturing scheme. By subdividing the numerical dissipation of the Roe scheme, the pressure-difference-driven modification for the cell face velocity is regarded as a version of the momentum interpolation method (MIM). The MIM is necessary for low Mach number flows to suppress the pressure checkerboard problem. Through the analysis and numerical tests, MIM has been discovered to have the most important function in shock instability. In fact, MIM should be completely removed for non-linear flows. However, unexpected MIM is activated on the cell face nearly parallel to the flow for high Mach number flows or low Mach number flows in shock. Therefore, the MIM should be kept for low Mach number flows and be completely removed for high Mach number flows and low Mach number flows in shock. For such conditions, two coefficients are designed on the basis of the local Mach number and a shock detector. The improved Roe scheme is then proposed. This scheme considers the requirement of MIM for incompressible and compressible flows and is validated for good performance of numerical tests. It is also proved that the acceptable result can be obtained with only Mach number coefficient for general practical computation.