Plasma Physics and Fusion Energy
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Magnetohydrodynamics - Overview
Center for Turbulence Research 361 Proceedings of the Summer Program 2006 Magnetohydrodynamics - overview Magnetohydrodynamics (MHD) is the study of the interaction of electrically conduct- ing fluids and electromagnetic forces. MHD problems arise in a wide variety of situations ranging from the explanation of the origin of Earth's magnetic field and the prediction of space weather to the damping of turbulent fluctuations in semiconductor melts dur- ing crystal growth and even the measurement of the flow rates of beverages in the food industry. The description of MHD flows involves both the equations of fluid dynamics - the Navier-Stokes equations - and the equations of electrodynamics - Maxwell's equa- tions - which are mutually coupled through the Lorentz force and Ohm's law for moving electrical conductors. Given the vast range of Reynolds numbers and magnetic Reynolds numbers characterising astrophysical, geophysical, and industrial MHD problems it is not feasible to devise an all-encompassing numerical code for the simulation of all MHD flows. The challenge in MHD is rather to combine a judicious application of analytical tools for the derivation of simplified equations with accurate numerical algorithms for the solution of the resulting mathematical models. The 2006 summer program provided a unique opportunity for scientists and engineers working in different sub-disciplines of MHD to interact with each other and benefit from the numerical capabilities available at the Center for Turbulence Research. In materials processing such as the growth of semiconductor crystals or the continuous casting of steel turbulent flows are often undesirable. The application of steady magnetic fields provides a convenient means for the contactless damping of turbulent fluctuations and for the laminarisation of flows. -
Superconducting Magnets Research for a Viable US Fusion Program Joseph V
Superconducting Magnets Research for a Viable US Fusion Program Joseph V. Minervini1, Leslie Bromberg1, Peter J. Lee2, David C. Larbalestier2, Introduction Magnet systems are the ultimate enabling technology for magnetic confinement fusion devices. Powerful magnetic fields are required for confinement of the plasma, and, depending on the magnetic configuration, dc and/or pulsed magnetic fields are required for plasma initiation, ohmic heating, inductive current drive, plasma shaping, equilibrium and stability control. Almost all design concepts for power producing commercial fusion reactors rely on superconducting magnets for efficient and reliable production of these magnetic fields. Future superconducting magnets for fusion applications require improvements in materials, components, and configurations to significantly enhance the feasibility and practicality of fusion reactors as an energy source. A demonstration of large-scale demountable High Temperature Superconducting (HTS) magnets could revolutionize fusion energy development, dramatically reducing program cost and development time. Background OFES established and maintained a robust magnet technology development for several decades. Until the end of the ITER EDA (1998), the magnet technology R&D program was arguably the most successful of all enabling magnet technology programs. Most of the laboratories and universities performing superconducting magnet R&D had robust programs. A major milestone was the first (and only) successful operation of the massive superconducting magnet system for MFTF-B at LLNL in 1986. The high point was the successful completion (1999) and operation (2000) of the ITER CS Model Coil (CSMC). Since that time, funding for the development of superconducting magnets and almost all other enabling technologies has been on a steady decline, leading to the proposed magnet technology budget for FY 2013 of $765,000 or 0.19% of the total fusion budget. -
10. Collisions • Use Conservation of Momentum and Energy and The
10. Collisions • Use conservation of momentum and energy and the center of mass to understand collisions between two objects. • During a collision, two or more objects exert a force on one another for a short time: -F(t) F(t) Before During After • It is not necessary for the objects to touch during a collision, e.g. an asteroid flied by the earth is considered a collision because its path is changed due to the gravitational attraction of the earth. One can still use conservation of momentum and energy to analyze the collision. Impulse: During a collision, the objects exert a force on one another. This force may be complicated and change with time. However, from Newton's 3rd Law, the two objects must exert an equal and opposite force on one another. F(t) t ti tf Dt From Newton'sr 2nd Law: dp r = F (t) dt r r dp = F (t)dt r r r r tf p f - pi = Dp = ò F (t)dt ti The change in the momentum is defined as the impulse of the collision. • Impulse is a vector quantity. Impulse-Linear Momentum Theorem: In a collision, the impulse on an object is equal to the change in momentum: r r J = Dp Conservation of Linear Momentum: In a system of two or more particles that are colliding, the forces that these objects exert on one another are internal forces. These internal forces cannot change the momentum of the system. Only an external force can change the momentum. The linear momentum of a closed isolated system is conserved during a collision of objects within the system. -
ERC Implementing Arrangements Call for Expression of Interest 2017
ERC Implementing Arrangements Call for Expression of Interest 2017 Project ID: Project Acronym: Evaluation Panel: 681178 G-EDIT LS1 Principal Investigator: Dr Mariusz Nowacki Host Institution: Universitat Bern - CH Mechanisms of RNA-guided genome editing in eukaryotes The goal of this project is to contribute to our understanding of RNA-mediated epigenetic mechanisms of genome regulation in eukaryotes. Ciliated protozoa offer a fantastic opportunity to investigate the complex process of trans-generational programming of chromosomal rearrangements, which is thought to serve as a form of immune defense against invasive DNA. Developmental processes in ciliates include extensive rearrangements of the germline DNA, including elimination of transposons and the precise excision of numerous single-copy elements derived from transposons. This process is considered to be maternally controlled because the maternal genome provides essential information in the form of RNA that determines the offspring's genome content and organization. This programmed DNA subtraction, the so-called ‘RNA scanning’ process, is mediated by trans-generational comparison between the germline and the maternal somatic genome. One of the most intriguing questions is how a complex population of small RNAs representing the entire germline genome can be compared to the entire rearranged maternal genome, resulting in the efficient selection of germline-specific RNAs, which are able to target DNA deletions in the developing genome. All this occurs in a very short time and involves a massively coordinated transport of all the components between three types of nuclei. This project focuses on characterizing the molecular machinery that can orchestrate the massive genome rearrangements in ciliates through nucleic acids and protein interactions. -
Inertial Electrostatic Confinement Fusor Cody Boyd Virginia Commonwealth University
Virginia Commonwealth University VCU Scholars Compass Capstone Design Expo Posters College of Engineering 2015 Inertial Electrostatic Confinement Fusor Cody Boyd Virginia Commonwealth University Brian Hortelano Virginia Commonwealth University Yonathan Kassaye Virginia Commonwealth University See next page for additional authors Follow this and additional works at: https://scholarscompass.vcu.edu/capstone Part of the Engineering Commons © The Author(s) Downloaded from https://scholarscompass.vcu.edu/capstone/40 This Poster is brought to you for free and open access by the College of Engineering at VCU Scholars Compass. It has been accepted for inclusion in Capstone Design Expo Posters by an authorized administrator of VCU Scholars Compass. For more information, please contact [email protected]. Authors Cody Boyd, Brian Hortelano, Yonathan Kassaye, Dimitris Killinger, Adam Stanfield, Jordan Stark, Thomas Veilleux, and Nick Reuter This poster is available at VCU Scholars Compass: https://scholarscompass.vcu.edu/capstone/40 Team Members: Cody Boyd, Brian Hortelano, Yonathan Kassaye, Dimitris Killinger, Adam Stanfield, Jordan Stark, Thomas Veilleux Inertial Electrostatic Faculty Advisor: Dr. Sama Bilbao Y Leon, Mr. James G. Miller Sponsor: Confinement Fusor Dominion Virginia Power What is Fusion? Shielding Computational Modeling Because the D-D fusion reaction One of the potential uses of the fusor will be to results in the production of neutrons irradiate materials and see how they behave after and X-rays, shielding is necessary to certain levels of both fast and thermal neutron protect users from the radiation exposure. To reduce the amount of time and produced by the fusor. A Monte Carlo resources spent testing, a computational model n-Particle (MCNP) model was using XOOPIC, a particle interaction software, developed to calculate the necessary was developed to model the fusor. -
AST242 LECTURE NOTES PART 3 Contents 1. Viscous Flows 2 1.1. the Velocity Gradient Tensor 2 1.2. Viscous Stress Tensor 3 1.3. Na
AST242 LECTURE NOTES PART 3 Contents 1. Viscous flows 2 1.1. The velocity gradient tensor 2 1.2. Viscous stress tensor 3 1.3. Navier Stokes equation { diffusion 5 1.4. Viscosity to order of magnitude 6 1.5. Example using the viscous stress tensor: The force on a moving plate 6 1.6. Example using the Navier Stokes equation { Poiseuille flow or Flow in a capillary 7 1.7. Viscous Energy Dissipation 8 2. The Accretion disk 10 2.1. Accretion to order of magnitude 14 2.2. Hydrostatic equilibrium for an accretion disk 15 2.3. Shakura and Sunyaev's α-disk 17 2.4. Reynolds Number 17 2.5. Circumstellar disk heated by stellar radiation 18 2.6. Viscous Energy Dissipation 20 2.7. Accretion Luminosity 21 3. Vorticity and Rotation 24 3.1. Helmholtz Equation 25 3.2. Rate of Change of a vector element that is moving with the fluid 26 3.3. Kelvin Circulation Theorem 28 3.4. Vortex lines and vortex tubes 30 3.5. Vortex stretching and angular momentum 32 3.6. Bernoulli's constant in a wake 33 3.7. Diffusion of vorticity 34 3.8. Potential Flow and d'Alembert's paradox 34 3.9. Burger's vortex 36 4. Rotating Flows 38 4.1. Coriolis Force 38 4.2. Rossby and Ekman numbers 39 4.3. Geostrophic flows and the Taylor Proudman theorem 39 4.4. Two dimensional flows on the surface of a planet 41 1 2 AST242 LECTURE NOTES PART 3 4.5. Thermal winds? 42 5. -
Energy Literacy Essential Principles and Fundamental Concepts for Energy Education
Energy Literacy Essential Principles and Fundamental Concepts for Energy Education A Framework for Energy Education for Learners of All Ages About This Guide Energy Literacy: Essential Principles and Intended use of this document as a guide includes, Fundamental Concepts for Energy Education but is not limited to, formal and informal energy presents energy concepts that, if understood and education, standards development, curriculum applied, will help individuals and communities design, assessment development, make informed energy decisions. and educator trainings. Energy is an inherently interdisciplinary topic. Development of this guide began at a workshop Concepts fundamental to understanding energy sponsored by the Department of Energy (DOE) arise in nearly all, if not all, academic disciplines. and the American Association for the Advancement This guide is intended to be used across of Science (AAAS) in the fall of 2010. Multiple disciplines. Both an integrated and systems-based federal agencies, non-governmental organizations, approach to understanding energy are strongly and numerous individuals contributed to the encouraged. development through an extensive review and comment process. Discussion and information Energy Literacy: Essential Principles and gathered at AAAS, WestEd, and DOE-sponsored Fundamental Concepts for Energy Education Energy Literacy workshops in the spring of 2011 identifies seven Essential Principles and a set of contributed substantially to the refinement of Fundamental Concepts to support each principle. the guide. This guide does not seek to identify all areas of energy understanding, but rather to focus on those To download this guide and related documents, that are essential for all citizens. The Fundamental visit www.globalchange.gov. Concepts have been drawn, in part, from existing education standards and benchmarks. -
Law of Conversation of Energy
Law of Conservation of Mass: "In any kind of physical or chemical process, mass is neither created nor destroyed - the mass before the process equals the mass after the process." - the total mass of the system does not change, the total mass of the products of a chemical reaction is always the same as the total mass of the original materials. "Physics for scientists and engineers," 4th edition, Vol.1, Raymond A. Serway, Saunders College Publishing, 1996. Ex. 1) When wood burns, mass seems to disappear because some of the products of reaction are gases; if the mass of the original wood is added to the mass of the oxygen that combined with it and if the mass of the resulting ash is added to the mass o the gaseous products, the two sums will turn out exactly equal. 2) Iron increases in weight on rusting because it combines with gases from the air, and the increase in weight is exactly equal to the weight of gas consumed. Out of thousands of reactions that have been tested with accurate chemical balances, no deviation from the law has ever been found. Law of Conversation of Energy: The total energy of a closed system is constant. Matter is neither created nor destroyed – total mass of reactants equals total mass of products You can calculate the change of temp by simply understanding that energy and the mass is conserved - it means that we added the two heat quantities together we can calculate the change of temperature by using the law or measure change of temp and show the conservation of energy E1 + E2 = E3 -> E(universe) = E(System) + E(Surroundings) M1 + M2 = M3 Is T1 + T2 = unknown (No, no law of conservation of temperature, so we have to use the concept of conservation of energy) Total amount of thermal energy in beaker of water in absolute terms as opposed to differential terms (reference point is 0 degrees Kelvin) Knowns: M1, M2, T1, T2 (Kelvin) When add the two together, want to know what T3 and M3 are going to be. -
A Mathematical Introduction to Magnetohydrodynamics
Typeset in LATEX 2" July 26, 2017 A Mathematical Introduction to Magnetohydrodynamics Omar Maj Max Planck Institute for Plasma Physics, D-85748 Garching, Germany. e-mail: [email protected] 1 Contents Preamble 3 1 Basic elements of fluid dynamics 4 1.1 Kinematics of fluids. .4 1.2 Lagrangian trajectories and flow of a vector field. .5 1.3 Deformation tensor and vorticity. 14 1.4 Advective derivative and Reynolds transport theorem. 17 1.5 Dynamics of fluids. 20 1.6 Relation to kinetic theory and closure. 24 1.7 Incompressible flows . 32 1.8 Equations of state, isentropic flows and vorticity. 34 1.9 Effects of Euler-type nonlinearities. 35 2 Basic elements of classical electrodynamics 39 2.1 Maxwell's equations. 39 2.2 Lorentz force and motion of an electrically charged particle. 52 2.3 Basic mathematical results for electrodynamics. 57 3 From multi-fluid models to magnetohydrodynamics 69 3.1 A model for multiple electrically charged fluids. 69 3.2 Quasi-neutral limit. 74 3.3 From multi-fluid to a single-fluid model. 82 3.4 The Ohm's law for an electron-ion plasma. 86 3.5 The equations of magnetohydrodynamics. 90 4 Conservation laws in magnetohydrodynamics 95 4.1 Global conservation laws in resistive MHD. 95 4.2 Global conservation laws in ideal MHD. 98 4.3 Frozen-in law. 100 4.4 Flux conservation. 105 4.5 Topology of the magnetic field. 109 4.6 Analogy with the vorticity of isentropic flows. 117 5 Basic processes in magnetohydrodynamics 119 5.1 Linear MHD waves. -
Fusion Energy Science Opportunities in Emerging Concepts
Fusion Energy Science Opportunities in Emerging Concepts Los Alamos National Laboratory Report -- LA-UR-99-5052 D. C. Barnes Los Alamos National Laboratory For the Emerging Concepts Working Group Convenors: J. Hammer Lawrence Livermore National Laboratory A. Hassam University of Maryland D. Hill Lawrence Livermore National Laboratory A. Hoffman University of Washington B. Hooper Lawrence Livermore National Laboratory J. Kesner Massachusetts Institute of Technology G. Miley University of Illinois J. Perkins Lawrence Livermore National Laboratory D. Ryutov Lawrence Livermore National Laboratory J. Sarff University of Wisconsin R. E. Siemon Los Alamos National Laboratory J. Slough University of Washington M. Yamada Princeton Plasma Physics Laboratory I. Introduction The development of fusion energy represents one of the few long-term (multi-century time scale) options for providing the energy needs of modern (or postmodern) society. Progress to date, in parameters measuring the quality of confinement, for example, has been nothing short of stellar. While significant uncertainties in both physics and (particularly) technology remain, it is widely believed that a fusion reactor based on the tokamak could be developed within one or two decades. It is also widely held that such a reactor could not compete economically in the projected energy market. A more accurate statement of projected economic viability is that the uncertainty in achieving commercial success is sufficient that the large development costs required for such a program are not justified at this time. While technical progress has been spectacular, schedule estimates for achieving particular milestones along the path of fusion research and development have proven notoriously inaccurate. This inaccuracy reflects two facts. -
Analysis of Equilibrium and Topology of Tokamak Plasmas
ANALYSIS OF EQUILIBRIUM AND TOPOLOGY OF TOKAMAK PLASMAS Boudewijn Philip van Millig ANALYSIS OF EQUILIBRIUM AND TOPOLOGY OF TOKAMAK PLASMAS BOUDEWHN PHILIP VAN MILUGEN Cover picture: Frequency analysis of the signal of a magnetic pick-up coil. Frequency increases upward and time increases towards the right. Bright colours indicate high spectral power. An MHD mode is seen whose frequency decreases prior to a disruption (see Chapter 5). II ANALYSIS OF EQUILIBRIUM AND TOPOLOGY OF TOKAMAK PLASMAS ANALYSE VAN EVENWICHT EN TOPOLOGIE VAN TOKAMAK PLASMAS (MET EEN SAMENVATTING IN HET NEDERLANDS) PROEFSCHRIFT TER VERKRUGING VAN DE GRAAD VAN DOCTOR IN DE WISKUNDE EN NATUURWETENSCHAPPEN AAN DE RUKSUNIVERSITEIT TE UTRECHT, OP GEZAG VAN DE RECTOR MAGNIFICUS PROF. DR. J.A. VAN GINKEL, VOLGENS BESLUTT VAN HET COLLEGE VAN DECANEN IN HET OPENBAAR TE VERDEDIGEN OP WOENSDAG 20 NOVEMBER 1991 DES NAMIDDAGS TE 2.30 UUR DOOR BOUDEWUN PHILIP VAN MILLIGEN GEBOREN OP 25 AUGUSTUS 1964 TE VUGHT DRUKKERU ELINKWIJK - UTRECHT m PROMOTOR: PROF. DR. F.C. SCHULLER CO-PROMOTOR: DR. N.J. LOPES CARDOZO The work described in this thesis was performed as part of the research programme of the 'Stichting voor Fundamenteel Onderzoek der Materie' (FOM) with financial support from the 'Nederlandse Organisatie voor Wetenschappelijk Onderzoek' (NWO) and EURATOM, and was carried out at the FOM-Instituut voor Plasmafysica te Nieuwegein, the Max-Planck-Institut fur Plasmaphysik, Garching bei Munchen, Deutschland, and the JET Joint Undertaking, Abingdon, United Kingdom. IV iEstos Bretones -
Stability Study of the Cylindrical Tokamak--Thomas Scaffidi(2011)
Ecole´ normale sup erieure´ Princeton Plasma Physics Laboratory Stage long de recherche, FIP M1 Second semestre 2010-2011 Stability study of the cylindrical tokamak Etude´ de stabilit´edu tokamak cylindrique Author: Supervisor: Thomas Scaffidi Prof. Stephen C. Jardin Abstract Une des instabilit´es les plus probl´ematiques dans les plasmas de tokamak est appel´ee tearing mode . Elle est g´en´er´ee par les gradients de courant et de pression et implique une reconfiguration du champ magn´etique et du champ de vitesse localis´ee dans une fine r´egion autour d’une surface magn´etique r´esonante. Alors que les lignes de champ magn´etique sont `al’´equilibre situ´ees sur des surfaces toriques concentriques, l’instabilit´econduit `ala formation d’ˆıles magn´etiques dans lesquelles les lignes de champ passent d’un tube de flux `al’autre, rendant possible un trans- port thermique radial important et donc cr´eant une perte de confinement. Pour qu’il puisse y avoir une reconfiguration du champ magn´etique, il faut inclure la r´esistivit´edu plasma dans le mod`ele, et nous r´esolvons donc les ´equations de la magn´etohydrodynamique (MHD) r´esistive. On s’int´eresse `ala stabilit´ede configurations d’´equilibre vis-`a-vis de ces instabilit´es dans un syst`eme `ala g´eom´etrie simplifi´ee appel´ele tokamak cylindrique. L’´etude est `ala fois analytique et num´erique. La solution analytique est r´ealis´ee par une m´ethode de type “couche limite” qui tire profit de l’´etroitesse de la zone o`ula reconfiguration a lieu.