Completely Bootstrapped Tokamak
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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
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 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
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 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 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].