Completely Bootstrapped Tokamak

Total Page:16

File Type:pdf, Size:1020Kb

Load more

W&M ScholarWorks Dissertations, Theses, and Masters Projects Theses, Dissertations, & Master Projects 1991 Completely bootstrapped tokamak Richard Henry Weening College of William & Mary - Arts & Sciences Follow this and additional works at: https://scholarworks.wm.edu/etd Part of the Plasma and Beam Physics Commons Recommended Citation Weening, Richard Henry, "Completely bootstrapped tokamak" (1991). Dissertations, Theses, and Masters Projects. Paper 1539623812. https://dx.doi.org/doi:10.21220/s2-2nck-2c81 This Dissertation is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Dissertations, Theses, and Masters Projects by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand corner and continuing from left to right in equal sections with small overlaps. Each original is also photographed in one exposure and is included in reduced form at the back of the book. Photographs included in the original manuscript have been reproduced xerographically in this copy. Higher quality 6" x 9" black and white photographic prints are available for any photographs or illustrations appearing in this copy for an additional charge. Contact UMI directly to order. University Microfilms International A Bell & Howell Information Company 300 North Zeeb Road. Ann Arbor, Ml 48106-1346 USA 313/761-4700 800/521-0600 ------------------------~ Order Number 9219102 Completely bootstrapped tokamak Weening, Richard Henry, Ph.D. The College of William and Mary, 1991 UMI 300 N. ZeebRd. Ann Arbor, MI 48106 --------------------------- COMPLETELY BOOTSTRAPPED TOKAMAK A Dissertation Presented to The Faculty of the Department of Physics The College of William and Mary in Virginia In Partial Fulfillment Of the Requirements for the Degree of Doctor of Philosophy by Richard H. Weening 1991 This dissertation is submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy Richard H. Weening Approved, November 1991 & A - . __________ Allen H. Boozer - l l . 6 ^ — Roy L. Champion Alkesh Punjabi Department of Mathematics Hangpfon University i"A V ^/ 'h / ^------- ' George T. Rublein Department of Mathematics Eugene R. T^py ______________ SlA^U. ______________L George M. Vahala ii It is not your obligation to complete the work of perfecting the world, but you are not free to desist from it either. - RABB! TARFON, Ethics of the Fathers ^ But all things very clear are as difficult as rare. - BARUCH SPINOZA, ETHIC God is inexorable in offering His gifts. He only gave me the stubbornness o f a mule. No! - He also gave me a keen sense of smell. - ALBERT EINSTEIN iii TABLE OF CONTENTS PREFACE....................................................................................................Vi ACKNOWLEDGEMENTS......................................................................... Viii LIST OF TABLES.....................................................................................xi LIST OF FIGURES..................................................................................xii ABSTRACT...............................................................................................xiv CHAPTER I. INTRODUCTION Section I-A. Thermonuclear Fusion ............................................2 Section 1-B. Magnetic Confinement .............................................8 Section I-C. Tokamaks .................................................................. 16 Section I-D. Tokamak Current ...................................................29 CHAPTER II. GENERALIZED OHM’S LAW Section II-A. MHD Theory .............................................................35 Section I I-B. Kinetic Theory ............................ 44 Section II-C. Fluid Equations ................................. 51 CHAPTER III. MAGNETIC FIELDS Section 11 I-A. Canonical Coordinates .......................................59 Section III-B. Magnetic Coordinates ........................................ 65 Section III-C. Magnetic Diffusion Equation ............................71 CHAPTER IV. TEARING MODES Section IV-A. Ideal MHD ...............................................................81 Section IV-B. Magnetic Topology .............................................. 91 iv Section IV-C. Tokamak Plasma Stability .............................I ll Section IV-D. Magnetic Island Growth .................................126 CHAPTER V. MEAN-FIELD THEORY Section V-A. Magnetic Helicity ...............................................133 Section V-B. Mean-field Ohm's Law ......................................144 Section V-C. Current Viscosity ..............................................152 CHAPTER VI. BOOTSTRAP EFFECT Section VI-A. Neo-classical Transport ................................ 162 Section VI-B. Current Amplification ....................................169 CHAPTER VII. NUMERICAL METHODS Section VII-A. Scaled Model Equations .................................178 Section VII-B. Poloidal Flux Evolution ..................................182 Section VII-C. Delta Prime Analysis ....................................198 CHAPTER VIII. INDUCTIVELY DRIVEN TOKAMAK Section VIII-A. Tokamak Temperature Profile ..................207 Section VIII-B. MHD-Stable Regime of the Tokamak . .218 CHAPTER IX. COMPLETELY BOOTSTRAPPED TOKAMAK Section IX-A. Tokamak Pressure Profile .............................237 Sec. IX-B. Self-maintenance of the Tokamak Current . .245 CHAPTER X. CONCLUSION Section X-A. Plasma Theory and Experiment ....................256 BIBLIOGRAPHY.....................................................................................261 VITA.......................................................................................................265 v PREFACE This is a dissertation about the leading fusion plasma confinement configuration, the tokamak. The problem we examine here is a fundamental one: How can one efficiently maintain the tokamak toroidal current in the steady-state? As will be seen later, this question is of great practical importance if one considers using the tokamak as a fusion reactor. The theoretical tools used to analyze our problem are fairly sophisticated ones. That is, we employ a new theoretical approach based on a magnetic helicity conserving mean-field Ohm’s law. Unfortunately, helicity is a very abstract topological concept. Nevertheless, an attempt has been made throughout the work to motivate theoretical arguments by physical rather than abstract considerations. The main accomplishment of this work is that, for the first time, a self-consistent mean-field helicity transport model for the tokamak has been successfully implemented on the computer. Two kinds of numerical simulations are accomplished: (1) simulations of inductively driven tokamaks and (2) simulations of completely bootstrapped tokamaks. The inductively driven tokamak simulations are compared with experimental results from the present generation of tokamak devices. The completely bootstrapped tokamak simulations are of great interest, since they suggest that an intrinsic tokamak steady-state can be obtained from the bootstrap current amplification effect alone. The organization of the dissertation is as follows. First, the Introduction has been written so that it is accessible to all readers and places our research within the context of the magnetic fusion program. Chapters II, III, and IV contain materials of a preliminary or background nature which describe the plasma Ohm's law, magnetohydrodynamics (MHD), representations of magnetic fields, tearing modes, and some tokamak physics. Reading these preliminary chapters will be vi particularly worthwhile for those uninitiated in plasma theory or those who want an in-depth view of our work. The reader who already possesses some knowledge of plasma physics may wish to move directly to chapters V and VI. which emphasize our mean-field theoretical approach. Chapter VII describes the numerical methods we have developed for the computer simulations which implement our mean-field theory. The results of the simulations are given in two chapters. Chapter VIII gives the results of simulations involving inductively driven tokamaks. Chapter IX analyzes the possiblity of the self-maintenance of the tokamak current by performing simulations of completely bootstrapped tokamaks. Finally, some concluding remarks are given in chapter X. vii ACKNOWLEDGEMENTS I would like to acknowledge and thank some of the many wonderful people who have helped make my graduate school career at William and Mary so enjoyable. First, I want to thank former Physics
Recommended publications
  • Subcritical Onset of Plasma Fluctuations and Magnetic Self-Organization in a Line-Tied Screw Pinch

    Subcritical Onset of Plasma Fluctuations and Magnetic Self-Organization in a Line-Tied Screw Pinch

    Subcritical Onset of Plasma Fluctuations and Magnetic Self-Organization in a Line-Tied Screw Pinch by Matthew Irvin Brookhart A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy (Physics) at the UNIVERSITY OF WISCONSIN-MADISON 2015 Date of final oral examination: 5/15/2015 The dissertation is approved by the following members of the Final Oral Committee: Cary Forest, Professor, Physics Ellen Zweibel, Professor, Astronomy John Sarff, Professor, Physics Jan Egedal, Associate Professor, Physics Chris Hegna, Professor, Nuclear Engineering and Engineering Physics UMI Number: 3703728 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. UMI 3703728 Published by ProQuest LLC (2015). Copyright in the Dissertation held by the Author. Microform Edition © ProQuest LLC. All rights reserved. This work is protected against unauthorized copying under Title 17, United States Code ProQuest LLC. 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, MI 48106 - 1346 i Subcritical Onset of Plasma Fluctuations and Magnetic Self-Organization in a Line-Tied Screw Pinch Matthew Irvin Brookhart Abstract The line-tied screw pinch is an important model for solar plasma and has been studied the- oretically and numerically for decades. Often these theoretical models used current profiles and equilibria that are difficult to make using inductive techniques conventionally used for creating pinch plasmas.
  • Study of Three-Dimensional Magnetic Reconnection Phenomena in the Experiment PROTO-SPHERA

    Study of Three-Dimensional Magnetic Reconnection Phenomena in the Experiment PROTO-SPHERA

    Macroarea di Scienze MM FF NN Corso di Laurea in Fisica Master Thesis Study of three-dimensional Magnetic Reconnection Phenomena in the experiment PROTO-SPHERA Student: Supervisor: Samanta Macera Prof. Marco Tavani Co-Supervisor: Dott. Franco Alladio Academic Year 2019/2020 Contents Introduction 4 1 Magnetic Reconnection 6 1.1 General theory of reconnection . 6 1.2 Steady state reconnection . 9 1.3 Fast Magnetic Reconnection . 14 1.4 Collisionless reconnection . 17 1.5 Three-dimensional reconnection . 24 1.6 Magnetic Reconnection in Astrophysics . 27 2 Laboratory Plasma 34 2.1 Experimental setup to study reconnection . 34 2.1.1 Magnetic Confinement . 35 2.1.2 Tokamak . 39 2.1.3 Reversed Field Pinch (RFP) and Spheromak . 41 2.2 Magnetic Reconnection and kink instability . 43 2.3 Experimental evidence of reconnection . 46 3 PROTO-SPHERA 51 3.1 From the screw pinch to the spherical torus . 54 3.1.1 Phase 1.0 . 55 3.1.2 Phase 1.25 (January 2018 - September 2019) . 57 3.1.3 Phase 1.5 (September 2019 - December 2021) . 58 3.1.4 The role of magnetic reconnection . 59 3.1.5 Towards phase 2.0 and beyond . 59 4 Data Analysis 63 4.1 Hall sensor . 63 4.2 Langmuir probe . 64 4.3 Fast cameras . 66 4.4 Fast camera image analysis . 68 4.5 Cross Correlations analysis . 74 4.6 Plasma phenomenology . 81 2 Conclusions 85 Bibliography 89 Ringraziamenti Introduction In the last eighty years, a lot of efforts have been made in Plasma Physics in order to understand magnetic reconnection, which is a physical process consisting of a topological rearrangement of magnetic field lines in a plasma.
  • TH/P9-29 Two-Fluid and Resistive Nonlinear Simulations of Tokamak

    TH/P9-29 Two-Fluid and Resistive Nonlinear Simulations of Tokamak

    TH/P9-29 Two-Fluid and Resistive Nonlinear Simulations of Tokamak Equilibrium, Stability, and Reconnection S. Jardin 1), C. Sovinec 2), J. Breslau 1), N. Ferraro 1), S. Hudson 1), J. King 2) , S. Kruger 4) J. Ramos 3), D. Schnack 2) 1) Princeton University Plasma Physics Laboratory 2) University of Wisconsin 3) Plasma Science and Fusion Center, Massachusetts Institute of Technology 4) Tech-X Corporation, Boulder CO e-mail contact of main author: [email protected] Abstract. The NIMROD and M3D / M3D-C1 codes now each have both a resistive MHD and a two-fluid (2F) capability including gyroviscosity and Hall terms. We describe: (1) a nonlinear 3D verification test in the resistive MHD regime in which the two codes are in detailed agreement , (2) new studies that illuminate the effect of two-fluid physics on spontaneous rotation in tokamaks, (3) studies of nonlinear reconnection in regimes of relevance to fusion plasmas with peak nonlinear reconnection rates that are essentially independent of the resistivity, and (4) linear two-fluid tearing mode calculations including electron mass that agree with analytic studies over a wide range of parameter regimes. 1. Introduction The SciDAC1 Center for Extended Magnetohydrodynamic Modeling (CEMM2) develops advanced computational models for the macroscopic dynamics of fusion-grade plasmas and implements these on some of the world’s most powerful computers. The center is built around the 3D nonlinear simulation codes NIMROD[1] and M3D[2]. A new variant of M3D, called M3D-C1 [3], uses a split-implicit time advance applied to high order finite elements with C1 continuity.
  • MHD Turbulence Generation, Interaction with the Internal Kink and Sheared Flows A

    MHD Turbulence Generation, Interaction with the Internal Kink and Sheared Flows A

    TH/P3-3 High-m Multiple Tearing Modes in Tokamaks: MHD Turbulence Generation, Interaction with the Internal Kink and Sheared Flows A. Bierwage 1)∗, S. Benkadda 2), M. Wakatani 1)†, S. Hamaguchi 3), Q. Yu 4) 1) Graduate School of Energy Science, Kyoto University, Uji, Kyoto, Japan 2) Equipe Dynamique des Syst`emes Complexes, UMR 6633 CNRS-Universit´e de Provence, Marseille, France 3) Center for Atomic and Molecular Technologies, Osaka University, Suita, Osaka, Japan 4) Max-Planck-Institut f¨ur Plasmaphysik, Euratom Association, Garching, Germany e-mail contact of main author: [email protected] Abstract. Linear instability and nonlinear dynamics of multiple tearing modes (MTMs) are studied with a reduced magnetohydrodynamic (RMHD) model of a large-aspect-ratio tokamak plasma in the limit of zero pressure. When low-order rational surfaces (such as those for q = 1 or 2 with q being the safety factor) are in close proximity, tearing modes on the rational surfaces are strongly coupled and exhibit a broad spectrum of positive growth rates with dominant mode numbers around mpeak ∼ 10. It is shown that collisionless double tearing modes (DTMs) due to electron inertia also have similar linear stability characteristics. Nonlinear dynamics associated with fast growing high-m MTMs can affect the evolution of low-m modes. For example, resistive q = 1 triple tearing modes (TTMs) generate MHD turbulence in a disrupted annular ring and the turbulence can impede the growth of an internal kink mode at a finite amplitude. Possible interactions between MTMs and sheared zonal flow are also discussed. 1.
  • Effects of Plasmoid Formation on Sawtooth Process in a Tokamak

    Effects of Plasmoid Formation on Sawtooth Process in a Tokamak

    Effects of Plasmoid Formation on Sawtooth Process in a Tokamak A. Ali1,2 and P. Zhu1,3,4,a 1CAS Key Laboratory of Geospace Environment and Department of Engineering and Applied Physics, University of Science and Technology of China, Hefei 230026, China 2 National Tokamak Fusion Program, Islamabad 3329, Pakistan 3KTX Laboratory and Department of Engineering and Applied Physics, University of Science and Technology of China, Hefei 230026, China 4Department of Engineering Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA For realistic values of Lundquist number in tokamak plasmas, the 1/1 magnetic island leads to the formation of secondary thin current sheet, which breaks up into a chain of small magnetic islands, called plasmoids. The role of plasmoid dynamics during the sawtooth reconnection process in fusion plasmas remains an unresolved issue. In this study, systematic simulations are performed to investigate the resistive internal kink mode using the full resistive MHD equations implemented in the NIMROD code in a simplified tokamak geometry. For Lundquist number 푆 ≥ 1.6×10, secondary current sheet is found to be unstable to plasmoids during the nonlinear resistive kink mode evolution with a critical aspect ratio of the current sheet of ~70. The merging of small plasmoids leads to the formation of a monster plasmoid that can significantly affect the primary island evolution. This may provide an explanation for the partial reconnection observed in sawtooth experiments. Keywords: tokamak, sawteeth oscillations, internal kink mode, plasmoids, partial reconnection a) E-mail address for corresponding author: [email protected] 1 I. Introduction Sawtooth crash is a typical example of fast magnetic reconnection observed in tokamak plasmas when the value of safety factor 푞 becomes less than one on the magnetic axis.
  • Direct Prediction of Nonlinear Tearing Mode Saturation Using a Variational Principle

    Direct Prediction of Nonlinear Tearing Mode Saturation Using a Variational Principle

    Direct prediction of nonlinear tearing mode saturation using a variational principle J. Loizu1, Y.-M. Huang2, S. R. Hudson2, A. Baillod1, A. Kumar3, and Z. Qu3 1 Ecole´ Polytechnique F´ed´erale de Lausanne, Swiss Plasma Center, CH-1015 Lausanne, Switzerland 2 Princeton Plasma Physics Laboratory, PO Box 451, Princeton NJ 08543, USA 3 Mathematical Sciences Institute, the Australian National University, Canberra ACT 2601, Australia∗ (Dated: June 8, 2020) It is shown that the variational principle of multi-region relaxed magnetohydrodynamics (MRxMHD) can be used to predict the stability and nonlinear saturation of tearing modes in strong guide field configurations without resolving the dynamics and without explicit dependence on the plasma resistivity. While the magnetic helicity is not a good invariant for tearing modes, we show that the saturated tearing mode can be obtained as an MRxMHD state of a priori unknown helicity by appropriately constraining the current profile. The predicted saturated island width in a tearing-unstable force-free slab equilibrium is shown to reproduce the theoretical scaling at small values of ∆0 and the scaling obtained from resistive MHD simulations at large ∆0. Magnetic reconnection is a ubiquitous phenomenon in very fact that a saturated state can be reached proves the the Universe that exhibits fast conversion of tremendous existence of a nearby, generally three-dimensional MHD amounts of magnetic energy into kinetic energy. It is ob- equilibrium. These observations raise the question: is served in solar eruptive flares [1, 2] and in the interaction there a variational principle that would allow direct cal- between the solar wind and the Earth's magnetic field [3].