Tokamak and Stellarator Require Doubly Connected Blanket => Very

Total Page:16

File Type:pdf, Size:1020Kb

Tokamak and Stellarator Require Doubly Connected Blanket => Very Tokamak and Stellarator require doubly connected blanket => Very complex & large systems Tokamak Stellarator Tokamak and Stellarator require doubly connected blanket => Very complex & large systems Tokamak Stellarator Study of Magnetic Reconnection and Merging of Compact Toroids Russell Kulsrud and Masaaki Yamada Norman Rostoker Memorial Symposium August 24, 2015 Magnetic Reconnection Experiment Magnetic reconnection = Fundamental Process Local view of reconnection: filed line reconnection=> Topology Change Conversion of magnetic energy to particle heating and acceleration How do we study magnetic reconnection in dedicated lab experiments? 1. We create a proto-typical reconnection layer in a controlled manner and study the fundamental plasma dynamics 2. Cross-validation of experiment and numerical modeling The primary issues/questions; • Why does reconnection occur so fast? • Dynamics of electrons and ions • How does local reconnection determine global phenomena? • How is magnetic energy converted to plasma flows and thermal energy? Experimental Setup and Formation of Current Sheet Experimentally measured flux evolution 13 -3 ne= 1-10 x10 cm , Te~5-15 eV, B~100-500 G, Local Reconnection Physics 1. MHD analysis 2. Two-fluid analysis Particle dynamics of the two-fluid reconnection layer Normalized with Erec +Vin × Brec = 0 Hall term Electron inertia Electron Ideal MHD region term pressure term B (G) Y 44 42 Ion Flow 40 Electron Flow 40 Separatrix 20 38 Magnetic Field Line R (cm) 0 36 Electron Diffusion Region −20 34 Ion Diffusion Region 32 −40 −9 −6 −3 0 3 6 9 Z (cm) MRX with fine probe arrays Linear probe arrays • Five fine structure probe arrays with resolution up to ∆x= 2.5 mm in radial direction are placed with separation of ∆z= 2-3 cm Evolution of magnetic field lines during reconnection in MRX e Measured region Experimental Setup for Energetics Study Magnetic Probe Array Equilibrium Field Coil Magnetic Field Lines 3 7 . 5 c m Flux Core R Current Sheet Y Z • Helium discharge 13 3 • ne: 2-8×10 /cm • Te~Ti: 6-15eV • λmfp,e ≥ c/ωpi > δCS (~2cm) • No guide field. • IDSP to measure Ti Electron dynamics and strong electron heating observed in the broad exhaust region of MRX AB3−D View of Fig.a Z (cm) ABMagnetic Field Lines and Electron Flow Vectors 3−D View of Fig.a Z (cm) Magnetic Field Lines and Electron Flow Vectors 0 0 j = Curl B, V = j /ne 44 5 5 e e 44 10 10 15 15 45 4242 45 4040 40 40 3838 R (cm)R (cm) R (cm) R (cm) 3636 35 35 3434 30 −305 −5 3232 0 0 5 5 10 10 Y (cm)Y (cm) 0 0 5 5 10 10 15 15 Z (cm)Z (cm) CDCDT (eV)T (eV) 3 3 2−D2− ElectronD Electron Temperature Temperature Profile Profile e e j ⋅E Profilej E Profile (W/cm(W/cm) ) e e 12 12 - Electron gain energy mostly near the 4242 42 42 11 11 150 150 X-point. 4040 40 40 10 10 100 100 - The energy transported via heat 3838 38 38 9 9 conduction R (cm) R (cm) R (cm) R (cm) 50 3636 36 36 50 8 8 3434 34 34 0 7 7 0 3232 32 32 6 6 0 0 5 5 10 10 15 15 0 0 5 5 10 10 15 15 Z (cm)Z (cm) Z (cm)Z (cm) Ion acceleration and heating in the reconnection layer Ion heating is attributed to re-magnetization of accelerated ions We note collisions play a role in ion heating in the exhaust Inventory of Energy Magnetic energy inflow rate! 1.0±0.1! Magnetic energy Energy deposition Energy deposition outflow rate! rate to electrons! rate to ions! 0.49±0.05! 0.18±0.04! 0.37±0.07! MHD Change of Change of flow component! thermal energy! energy! 0.22±0.02! 0.14±0.05! 0.07±0.02! Hall-field Energy loss rate Change of component! (Conduction, thermal energy! radiation) 0.27±0.03! radiation) 0.17±0.05! 0.08±0.04! Energy loss rate (Conduction, neutrals) ≤ 0.16! Nature Communications (2014) Energy conversion during magnetic reconnection - Significant particle heating and acceleration observed in reconnection events in the magnetosphere, solar flares and laboratory experiments. - It is generally difficult to identify the inventory and partitioning of energy - Our findings on energy partitioning in a reconnection layer is remarkably consistent with the recent space results J. Eastwood et al, 2013 Summary of findings on MRX reconnection research MRX has been very productive; 15 plus PRL, Science, Nature papers et al. • Verified experimentally the two-fluid (collision-less) reconnection physics – Verification of Hall effects – Validation and verification of numerical simulation codes – Identification electron diffusion layer => NASA’s MMS Project • Identified the in-plane electric field which plays a key role for ion acceleration and heating – Ions are accelerated electrostatically near the separatrices. – Ions are heated downstream by re-magnetization and collisions. • Conversion magnetic energy and partitioning is quantitatively analyzed in the reconnection layer - Substantial component of outgoing magnetic energy (~ 50%) - 50+% of incoming magnetic energy goes to plasma particles 2/3: to ions 1/3: to electrons SPIRIT (Self-organized Plasma by Induction, Reconnection, Injection Techniques) Attempts for simpler reactor core design => Compact Toroid Reactor Core Spherical Torus Spheromak Field Reversed Configuration SPIRIT Concepts (1997 -) “Self-organized Plasma with Induction, Reconnection, and Injection Techniques” • Formation of FRC by reconnection of spheromaks • Sustained FRC plasmas with the use of inductive drive • Sustainment of FRC by 10-20 kV NB Injection • <=> N. Rostoker <=> TAE Spheromak Merging Experiments in MRX (Toroidal Energy => Plasma Kinetic Energy) Plasma Initiation Spheromak Formation (1) - + Speromak Merging Final CT (1) Spheromak Merging Experiments in U. Tokyo (Toroidal Energy => Plasma Kinetic Energy) TS-3; Yamada et al PRL (1990) Ono et al PRL(1996) Norman’s 70 year Symposium (1995) Strong ion heating occurs while toroidal field is annihilated Strongest ion Temperature Rise During Merging Phase (285µs-300µs) Strong Elimination of Toroidal Field Energy During Merging (285µs-300µs) Spheromak Merging is provide a promising option for the TAE project CT Sustainment Campaign on MRX • 68 turn Ohmic solenoid, Inconel liner • Three capacitor banks for 4 coils (TF, PF, SF, Ohmic) New 2D Probe Array Surface Voltage Current Density Trapped Flux Solenoid Current (V) (A/m2) (mWb) (kA) MoreFlux, Drive Generates Inductive Longer Sustainment Longer Input Powers: Input Powers: OH Voltages OH Voltages 300-800kW 300-800kW 5kV-9kV 5kV-9kV Ohmic Sustainment for ~300µs Demonstrated 275 µs 325 µs 375 µs 450 µs 550 µs Summary Notes 1) Compact toroid plasma concept to achieve a small, simple, high efficiency, and economical reactor core. • Simple geometry • High power density • High beta ( FRC has highest equilibrium beta) • Can lead to advanced fuel reactor (P-B11, D-He3) 2) Major challenges remain: • Obtain good confinement of plasma • Control of magnetic self-organization 3) To understand magnetic reconnection is a key 4) TAE is in the forefront to solve these major issues => M. Binderbauer’s talk .
Recommended publications
  • Scientists Propose Source of Unexplained Solar Jets 8 July 2021, by Raphael Rosen
    Scientists propose source of unexplained solar jets 8 July 2021, by Raphael Rosen was an undergraduate at Princeton University. He currently is a doctoral student in the Nuclear Engineering and Radiological Sciences department at the University of Michigan. Large coronal jets, though originating 93 million miles away on the sun, can affect us here on Earth. The jets can contribute to outpourings of particles known as the solar wind that can strike our planet's outer atmosphere and interfere with communications satellites and power grids. Smaller jets, which are studied at PPPL, also contribute to the solar wind, and along with bursts of X-ray light can help heat the corona. Any insights into how the jets form could help scientists to predict their occurrence and prepare Earth for their impact. Graduate student Joshua Latham with computer- generated images of magnetic field lines and plasma on The simulations indicate that a dome-shaped the sun. Credit: Elle Starkman magnetic structure forms on the sun's surface prior to the coronal jets. Then, magnetic field lines at the bottom of the structure detach from the solar surface in a process known as magnetic Nothing seems more familiar than the sun in the reconnection, the breaking apart and violent sky. But mysterious swirls, jets, and flashes of reconnection of magnetic fields that occurs powerful light that scientists cannot explain occur throughout the universe. in the sun's outer atmosphere all the time. Now, researchers at the U.S. Department of Energy's Now the dome begins to tilt. As it does so, the top (DOE) Princeton Plasma Physics Laboratory magnetic field lines touch the surrounding lines and (PPPL) have gained insight into these puzzling create another round of reconnection.
    [Show full text]
  • MRX Research in the Context of Princeton Max-Planck Collaboration
    MRX research in the context of Princeton Max-Planck collaboration Masaaki Yamada Princeton Plasma Physics laboratory Princeton University January 14, 2013 With MRX Staff: H. Ji, R. Kulsrud, E. Lawrence, T. Tharp + Graduate students Magnetic Reconnection • Topological rearrangement of magnetic field lines! • Magnetic energy => Kinetic energy! • Key to stellar flares, coronal heating, particle acceleration, star formation, energy loss in lab plasmas! Before reconnection After reconnection Outline! !Magnetic reconnection! – Leading issue in space, astro- and fusion plasma physics" –! A major question was: Why does it occur so fast?" –! New question: How does energy flow from magnetic field to plasmas?" •! Generation of a reconnection layer on MRX => Local analysis" •! Two fluid physics analysis! Recent Emphasis:! •! Energy conversion processes from B2 to ions and electrons! •! A new series of experimental campaign and the recent results! –! Plasma jog experiment: Addresses heating and acceleration of ions and electrons" –! Guide field effects on two-fluid reconnection" –! Reconnection in partially ionized plasmas" –! Solar flare relevant plasma arcs" Plans for Princeton-MPPC collaboration! Magnetic Reconnection Experiment Primary objectives of MRX is to create a proto-typical reconnection layer and study it experimentally with cross- validation with numerical simulations Experimentally measured flux evolution! 13 -3 ne= 1-10 x10 cm , ! Te~5-15 eV, ! B~100-500 G, ! S < 1000! Reconnection layer Profile changes with Collisionality: Experimentally measured field line features in MRX •! Manifestation of Hall effects •! Electrons would pull magnetic field lines with their flow Two-fluid physics dictates reconnection layer dynamics (a) (b) R •! Out of plane magnetic field is generated during reconnection. •! Electron acceleration and heating with mirror- Plasma Electron Outflow trapped electrons.
    [Show full text]
  • Frontiers in Plasma Physics Research: a Fifty-Year Perspective from 1958 to 2008-Ronald C
    • At the Forefront of Plasma Physics Publishing for 50 Years - with the launch of Physics of Fluids in 1958, AlP has been publishing ar In« the finest research in plasma physics. By the early 1980s it had St t 5 become apparent that with the total number of plasma physics­ related articles published in the journal- afigure then approaching 5,000 - asecond editor would be needed to oversee contributions in this field. And indeed in 1982 Fred L. Ribe and Andreas Acrivos were tapped to replace the retiring Fran~ois Frenkiel, Physics of Fluids' founding editor. Dr. Ribe assumed the role of editor for the plasma physics component of the journal and Dr. Acrivos took on the fluid Editor Ronald C. Davidson dynamics papers. This was the beginning of an evolution that would see Physics of Fluids Resident Associate Editor split into Physics of Fluids A and B in 1989, and culminate in the launch of Physics of Stewart J. Zweben Plasmas in 1994. Assistant Editor Sandra L. Schmidt Today, Physics of Plasmas continues to deliver forefront research of the very Assistant to the Editor highest quality, with a breadth of coverage no other international journal can match. Pick Laura F. Wright up any issue and you'll discover authoritative coverage in areas including solar flares, thin Board of Associate Editors, 2008 film growth, magnetically and inertially confined plasmas, and so many more. Roderick W. Boswell, Australian National University Now, to commemorate the publication of some of the most authoritative and Jack W. Connor, Culham Laboratory Michael P. Desjarlais, Sandia National groundbreaking papers in plasma physics over the past 50 years, AlP has put together Laboratory this booklet listing many of these noteworthy articles.
    [Show full text]
  • Structure of the Electron Diffusion Region in Magnetic Reconnection with Small Guide Fields
    Structure of the electron diffusion region in magnetic reconnection with small guide fields MASSA0HU- by Jonathan Ng JAN I Submitted to the Department of Physics in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 2012 @ Jonathan Ng, MMXII. All rights reserved. The author hereby grants to MIT permission to reproduce and distribute publicly paper and electronic copies of this thesis document in whole or in part. Author ............ Department of Physics May 11, 2012 / / Certified by..... *2) Jan Egedal-Pedersen Associate Professor of Physics Thesis Supervisor Accepted by ...... .............. ........ ............. ... Nergis Mavalvala Senior Thesis Coordinator, Department of Physics 2 Structure of the electron diffusion region in magnetic reconnection with small guide fields by Jonathan Ng Submitted to the Department of Physics on May 11, 2012, in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics Abstract Observations in the Earth's magnetotail and kinetic simulations of magnetic reconnec- tion have shown high electron pressure anisotropy in the inflow of electron diffusion regions. This anisotropy has been accurately accounted for in a new fluid closure for collisionless reconnection. By tracing electron orbits in the fields taken from particle-in-cell simulations, the electron distribution function in the diffusion region is reconstructed at enhanced resolutions. For antiparallel reconnection, this reveals its highly structured nature, with striations corresponding to the number of times an electron has been reflected within the region, and exposes the origin of gradients in the electron pressure tensor important for momentum balance. The addition of a guide field changes the nature of the electron distributions, and the differences are accounted for by studying the motion of single particles in the field geometry.
    [Show full text]
  • Physicist Masaaki Yamada Wins 2015 James Clerk Maxwell Prize In
    PRINCETON PLASMA PHYSICS LABORATORY A Collaborative National Center for Fusion & Plasma Research WEEKLY October 26, 2015 Calendar of Events Physicist Masaaki Yamada wins WEDNESDAY, OCT. 28 PPPL Colloquium 2015 James Clerk Maxwell Prize 4:15 p.m. u MBG Auditorium Seeing the Big Bang More Clearly: The Evolution of Observational in Plasma Physics Techniques in CMB Studies By Raphael Rosen Dr. Bruce Partridge, Haverford College asaaki Yamada, a Distinguished THURSDAY, OCT. 29 M Laboratory Research Fellow at PPPL, PPPL Benefits Fair has won the 2015 James Clerk Maxwell 10 a.m.–2 p.m. Prize in Plasma Physics. The award from the American Physical Society (APS) Division of Plasma Physics recognized Yamada for UPCOMING “fundamental experimental studies of mag- NOV. 3–6 netic reconnection relevant to space, astro- physical and fusion plasmas, and for pio- 18th International Spherical Torus Workshop neering contributions to the field of labora- Princeton University tory plasma astrophysics.” Yamada will receive the award at the 57th FRIDAY, NOV. 6 annual meeting of the APS Division of Public Tour Plasma Physics in Savannah, Georgia, in 10 a.m. November, and will present a plenary talk [email protected] to the session. “I am quite honored and pleased to be recognized,” said Yamada, the PPPL Colloquium 2:15 p.m. u MBG Auditorium principal investigator for PPPL’s Magnetic Masaaki Yamada Technical Aspects of the Iran Reconnection Experiment (MRX), the Nuclear Deal world’s leading laboratory facility for studying reconnection—an astrophysical pro- Professor Robert Goldston, cess that gives rise to solar flares, the northern lights, and geomagnetic storms.
    [Show full text]
  • Particle Heating and Energy Partition in Reconnection with a Guide Field
    ABSTRACT Title of dissertation: PARTICLE HEATING AND ENERGY PARTITION IN RECONNECTION WITH A GUIDE FIELD Qile Zhang Doctor of Philosophy, 2019 Dissertation directed by: Professor James Drake Department of Physics Kinetic Riemann simulations have been completed to explore particle heating during reconnection with a guide field in the low-beta environment of the inner helio- sphere and the solar corona. The reconnection exhaust is bounded by two rotational discontinuities (RDs) with two slow shocks (SSs) that form within the exhaust as in magnetohydrodynamic (MHD) models. At the RDs, ions are accelerated by the magnetic field tension to drive the reconnection outflow as well as flows in the out- of-plane direction. The out-of-plane flows stream toward the midplane and meet to drive the SSs. The turbulence at the SSs is weak so the shocks are laminar and pro- duce little dissipation, which differs greatly from the MHD treatment. Downstream of the SSs the counter-streaming ion beams lead to higher density and therefore to a positive potential between the SSs that confines the downstream electrons to maintain charge neutrality. The potential accelerates electrons from upstream of the SSs to downstream and traps a small fraction but only produces modest electron heating. In the low-beta limit the released magnetic energy is split between bulk flow and ion heating with little energy going to electrons. To firmly establish the laminar nature of reconnection exhausts, we explore the role of instabilities and turbulence in the dynamics. Two-dimensional recon- nection and Riemann simulations reveal that the exhaust develops large-amplitude striations resulting from electron-beam-driven ion cyclotron waves.
    [Show full text]
  • Landon Bevier (U. of Washington), Advised by Dr. Masaaki Yamada (PPPL)
    Preliminary Study of Coronal Jets due to Spheromak Tilt Instability Landon Bevier (U. of Washington), advised by Dr. Masaaki Yamada (PPPL) Abstract Methods Findings Activity in the solar corona such as flares, coronal mass ejections, and coronal jets are driven by the release of energy through • Over 400 shots were taken for this experiment under a Stability: magnetic reconnection events. Understanding the mechanism(s) variety of settings. 푎 • The Alfvén time defined as 휏퐴 = = 4휇푠, was used to behind coronal jets has been long sought-after in solar and space • The three main categories used to assess these shots were 푣퐴 physics. We propose coronal jets could be modeled by embedding formation mechanics, magnetics/camera correlation, and normalize the time scales of this experiment. a hemispherical spheromak-like closed field structure inside a large stability. • 푣퐴 = 100푘푚/푠 [3] is the Alfvén speed and 푎 = 0.4푚 is a scale open field. In the boundary between these structures, current character length in the system chosen to be the major radius filaments form then undergo a reconnection event linking them to of the plasma. the open field lines, thereby allowing the filaments to become a Figure 4: (a) Image of MRX. (b) Cross-section of MRX showing coil plasma jet1. It is postulated that this reconnection event may be geometry, probe array, and typical reconnection region. related to the global reconnection which occurs during the spheromak tilt instability. This paper explores the results from a • This preliminary experiment was conducted to provide preliminary experiment done on the Magnetic Reconnection proof of concept that MRX could be used to form a stable Experiment (MRX) in which a spheromak is formed inside of an spheromak.
    [Show full text]
  • On Kinetic Dissipation in Collisionless Turbulent Plasmas
    ON KINETIC DISSIPATION IN COLLISIONLESS TURBULENT PLASMAS by Tulasi Nandan Parashar A dissertation submitted to the Faculty of the University of Delaware in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics Spring 2011 c 2011 Tulasi Nandan Parashar All Rights Reserved ON KINETIC DISSIPATION IN COLLISIONLESS TURBULENT PLASMAS by Tulasi Nandan Parashar Approved: George Hadjipanayis, Ph.D. Chair of the Department of Physics & Astronomy Approved: George Watson, Ph.D. Dean of the College of Arts & Sciences Approved: Charles G. Riordan, Ph.D. Vice Provost for Graduate and Professional Education I certify that I have read this dissertation and that in my opinion it meets the academic and professional standard required by the University as a dissertation for the degree of Doctor of Philosophy. Signed: Michael A Shay, Ph.D. Professor in charge of dissertation I certify that I have read this dissertation and that in my opinion it meets the academic and professional standard required by the University as a dissertation for the degree of Doctor of Philosophy. Signed: William H Matthaeus, Ph.D. Member of dissertation committee I certify that I have read this dissertation and that in my opinion it meets the academic and professional standard required by the University as a dissertation for the degree of Doctor of Philosophy. Signed: Dermott Mullan, Ph.D. Member of dissertation committee I certify that I have read this dissertation and that in my opinion it meets the academic and professional standard required by the University as a dissertation for the degree of Doctor of Philosophy.
    [Show full text]
  • 13Th International Congress on Plasma Physics (ICPP 2006) BOOK
    UA061408 13th International Congress on Plasma Physics (ICPP 2006) Bogolyubov Institute for Theoretical Physics of the National Academy of Sciences of Ukraine May 22-26, 2006 BOOK OF ABSTRACTS Part I. Sections A, B, C KIEV 2006 13th International Congress on Plasma Physics (ICPP 2006) Bogolyubov Institute for Theoretical Physics of the National Academy of Sciences of Ukraine May 22-26, 2006 BOOK OF ABSTRACTS Part I. Sections A, B, C KIEV 2006 Preface The 13th International Congress on Plasma Physics (ICPP 2006) is hosted, on behalf of the National Academy of Sciences of Ukraine, by the Bogolyubov Institute for Theoretical Physics (BITP). The Congress is held in the Institute of International Relations of the Shevchenko National University of Kiev. Five main topics are covered: A. Fundamental Problems of Plasma Physics B. Fusion Plasmas C. Plasmas in Astrophysics and Space Physics D. Plasmas in Applications and Technologies E. Complex Plasmas The discussions are held in the traditional ICPP format: 5 plenary sessions (9 Invited Plenary Talks, 45 min. each) 10 review sessions (32 Invited Topical Talks, 30 min. each) 12 oral sessions (60 oral presentations, 20 min. each) 3 poster sessions The Book of Abstracts contains the abstracts of invited and contributed papers. Full texts of the Invited Papers will be published as a special issue of Plasma Physics and Controlled Fusion. A copy will be sent to each registered participant. Four-page texts of contributed papers will be published in electronic (CD) form and posted on the Congress Website. The structure of the Book of Abstracts follows the format of the Congress.
    [Show full text]
  • Table of Contents (Online)
    NEWSPAPER 78 PHYSICAL REVIEW LETTERS Contents VOLUME 78, NUMBER 16 21 April 1997 General Physics Three-Particle Entanglements from Two Entangled Pairs ................................................................. 3031 Anton Zeilinger, Michael A. Horne, Harald Weinfurter, and Marek Zukowski˙ Barrier Tunneling and Reflection in the Time and Energy Domains: The Battle of the Exponentials . .................. 3035 N. T. Maitra and E. J. Heller Steady State and Dynamics of Driven Diffusive Systems with Quenched Disorder . ................................... 3039 Goutam Tripathy and Mustansir Barma Gravitation and Astrophysics Indication of Anisotropy in Electromagnetic Propagation over Cosmological Distances .................................. 3043 Borge Nodland and John P. Ralston Preliminary Results of a Determination of the Newtonian Constant of Gravitation: A Test of the Kuroda Hypothesis 3047 Charles H. Bagley and Gabriel G. Luther General Relativity in Terms of Dirac Eigenvalues . ...................................................................... 3051 Giovanni Landi and Carlo Rovelli Elementary Particles and Fields CODEN: PRLTAO 78 (16), 3031–3227 (21 April 1997) New Signature for Gauge Mediated Supersymmetry Breaking ........................................................... 3055 D. A. Dicus, B. Dutta, and S. Nandi Calculation of Hadron Form Factors from Euclidean Dyson-Schwinger Equations ....................................... 3059 M. Burkardt, M. R. Frank, and K. L. Mitchell Wide Scalar Neutrino Resonance and bb Production
    [Show full text]
  • PSI 2018 Conference Experts Guide Booklet
    Need an Expert? Whether you’re reporting on fusion energy or plasma science, or have questions about physics, chances are we have an expert you can interview. See inside for details on renowned experts at the Princeton Plasma Physics Laboratory, a national laboratory managed by Princeton University for the U.S. Department of Energy’s Office of Science. Atiba Brereton Expert Topics: Diagnostic equipment, Computer aided design (CAD), Fusion energy Atiba Brereton is a diagnostic engineer who con- tributes to the design, fabrication, and installation of various types of diagnostic equipment on PPPL’s National Spherical Torus Experiment-Upgrade (NSTX-U). He has worked on several diagnostics such as SPRED (Survey, Poor Resolution, Extended Domain), a spectrometer that will be used Fusion. Energy. Plasma. Physics. to measure impurities in the divertor of the tokamak, and FIReTIP Tokamaks. Stellarators. Radioactivity. (Far InfraRed Tangential Interferometer/Polarimeter), which will be used to monitor plasma density. He is also a popular PPPL tour Nanotechnology. Astrophysics. guide and a frequent volunteer with the Offi ce of Communications Computational simulations. and Public Outreach. Vacuum technology. Materials science. Electronics. STEM education. These are some of the areas of expertise of sta at the Ahmed Diallo Princeton Plasma Physics Laboratory. PPPL is devoted to Expert Topics: Laser diagnostics, Plasma physics creating new knowledge about the physics of plasmas Ahmed Diallo is leader of the pedestal structure — hot, charged gases that make up the fourth state of and control topical science group of the National matter — and to developing practical solutions for the Spherical Torus Experiment-Upgrade (NSTX-U) and creation of controlled fusion energy.
    [Show full text]
  • Past Colloquium Speakers
    Past Colloquium Speakers 2007/2008 Alain Herve “Experience Gained from the Construction, Test, and Operation of the Large 4-Tesla Superconducting Coil for the CMS Experiment at CERN” Former Technical Coordinator of the CMS Experiment, CERN, Geneva, Switzerland Erik Winfree “Programming the DNA World” Associate Professor, California Institute of Technology, Computer Science & Computation and Neural science, Pasadena, CA John Sheffield “What About Fusion Reactors?” Senior Fellow, University of Tennessee, Institute for a Secure and Sustainable Environment, Knoxville, TN Ian Dobson “Cascading Failure, the Risk of Large Blackouts, Criticality, and Self-Organization” Professor, University of Wisconsin Madison, Department of Electrical & Computer Engineering, Madison, WI Edward W. Felten “Electronic Voting: Danger and Opportunity” Professor, Princeton University, Computer Science and Public Affairs Sergey Macheret “Weakly Ionized Plasmas for Aerospace Applications” Senior Staff Aeronautical Engineer, Revolutionary Technology Programs, Lockheed Martin, Palmdale, CA Stewart Prager “The Reversed Field Pinch: Progress from Fusion to Astrophysics” Professor, University of Wisconsin Madison, Department of Physics, Madison, WI Peter Barker “Controlling the Motion of Atoms and Molecules with Intense Optical Fields” Professor, Department of Physics and Astronomy, University College – London, U.K. Michael A. Liebreman “Nanoelectronics and Plasma Processing—the Next Fifteen Years and Beyond” Professor, University of California Berkeley, Department of Engineering
    [Show full text]