Stellarator Work

Total Page:16

File Type:pdf, Size:1020Kb

Stellarator Work Vision of the KSTAR Research in ITER Era Hyeon K. Park POSTECH on February 24, 2012 at KSTAR Conference Muju Korea Talk Why large scale clean energy source? The ultimate option – “Fusion Power” Progress in fusion energy development and role of the KSTAR research Brief background of the fusion energy research Paradigm change in fusion research in recent years: steady state capable fusion devices in Asia Role of KSTAR in ITER era and K-Demo International facility and physics basis for K-Demo New path of the fusion plasma research “New idea” and “new methodology” Past, present, and future of “We” (population and energy) A few Scenarios in energy world consumption rate Can we replace the fossil fuel? How and on what time scale? Global warming and CO2 emission CO2 concentration will trigger the global warming Argument is still controversial but there may be no turning point once it happens Needs a positive proof?? Reduction of CO2 is a good preventive measure but the cost is not cheap unless …….. Need a long term plan for a clean large scale energy including fuel cell The beginning of the fusion concept 1928 Concept of fusion reaction – energy radiated by stars [R. Atkinson & F.G. Houtermans, Physik, 54 (1929)] - J. Jeans was skeptical; A. Eddington retorted: “ I suggest he finds a hotter place” 1932: Fusion reactions discovered in laboratory by M. Oliphant - Lord Rutherford felt possibility of fusion power using beam-solid target approach “moonshine” 1935 Basic understanding of fusion reactions - tunneling through Coulomb barrier – G. Gamov et al. - Fusion requires high temperatures (Maxwellian) 1939 Fusion power cycle for the stars: H. Bethe - Nobel prize 1967 “for his theory of nuclear reactions, especially his discoveries concerning the energy production in stars” Early Years of Magnetic Confinement Fusion Research 1940s - Concept of using a magnetic field to confine a hot plasma for fusion 1947 - G.P. Thomson and P.C. Thonemann began classified investigations of toroidal “pinch” RF discharge, eventually leading to ZETA, a large pinch at UKAEA Harwell, England in 1956 1949 - R. Richter in Argentina claimed to have achieved controlled fusion – turns out to be bogus, but news piques interest of Lyman Spitzer at Princeton 1950 - Spitzer conceived “stellarator” (while on a ski lift) and makes proposal to AEC ($50k) - Project Matterhorn initiated at Princeton 1950s - Classified US Project Sherwood on controlled thermonuclear fusion 1958 - Magnetic fusion research declassified. US and others unveil results at 2nd UN Atoms for Peace Conference in Geneva Magnetic Fusion (closed traps):Tokamak B Plasma in a simple torus does not have an equilibrium Curvature and gradient in B cause single particles to drift vertically Charge separation at the edges produces a downward E field that drives outward drift of plasma Introduce rotational transform (helical twist) to field lines so TEXTOR (Torus-Experiment for Technology Oriented Research) drifts are compensated over several transits External windings, geometrical B modification v toroidal current in the plasma Bt B itself p major radius: 1.75 m minor radius: 0.50 m plasma current: 0.5 (0.8) MA toroidal field: 2.8 T pulse length: 10 sec In Stellarators, rotational transform is created by twisting the axis or external coils (or both) Hot plasma is confined by an intricate magnetic field Tokamak – external magnetic field and magnetic field by a driven plasma current Stellarator – magnetic field by complex external coils Large Helical Device (LHD), NIFS, Japan External diameter 13.5 m Plasma major radius 3.9 m Plasma minor radius 0.6 m Plasma volume 30 m3 Magnetic field 3 T Scientific break-even Three large tokamak era: non-steady state device based on Cu coils (pulse length is limited by the cooling system < ~ 20 sec.) Tokamak Fusion Test Reactor (USA) 1982-1997, Princeton Plasma Physics Laboratory, USA Fusion power yield: Q ~ 0.3 from D-T experiment Joint European Tokamak (EU):1983 – present, Culham, Oxfordshore, UK Fusion power yield: Q ~ 0.7 from D-T experiment JT-60U (Japan):1985 - present, Japan Atomic Energy Agency (JAEA), Japan Q~1.25 extrapolated from D-D experiment Internal view of Internal view of TFTR Internal view of JT60-U JET/plasma discharge ITER (Q=10) The goal is "to demonstrate the scientific and technological feasibility of fusion power for peaceful purposes". Demonstration of fusion power yield; Q (output power/input power) ~10 International consortium (Europe, Japan, Russia, Korea, China, and India) Total cost and beyond ~ $10 B for ~10 years and the next step is Demo Physics basis is empirical energy confinement scaling Current status of ITER project (2011) Construction is in progress at Cadarache, France ITER site Device PF coil facility Admin Fusion research history and the future JET (EU) ITER (Q~10, 2025) Advanced future reactor smaller and efficient Needs physics basis !! Future fusion reactor: rendering New fusion research facilities in Asia Steady state capable devices are critical for the physics and engineering basis for the fusion plasma research New superconducting tokamak devices are merging to Asian countries – Japan (LHD, JT-60SA), China (EAST), Korea (KSTAR) and India (SST) SST-1, India EAST, LHD, NIFS, Hefei, Japan China JT-60SA, JAEA, Japan KSTAR, NFRI, Korea Paradigm change in fusion research Critical mass in fusion effort is being established in Asia New steady state capable magnetic fusion devices are operated and/or being built in Asia (within two hour time zone) Number of Asian scientists in fusion science is ever increasing Engineering support in Asian sector is reliable and cost effective Asian Plasma Physics Organization will be effective for Sharing physics research burden (stability, transport, current drive, material test, advanced control, etc.) Sharing advanced technology and engineering development (advanced diagnostic system, material development, etc.) Sharing theoretical understanding and computational facility (modeling center for fusion research) Role of KSTAR and K-Demo 2009 2020 2040 Fast Track DEMO K-Demo (EU,CN,JP,KO,US) KSTAR It is a long Research term endeavor Device but It is our ultimate GOAL Two important roles of KSTAR International role - center for steady state physics research Human resource development for world wide fusion research Support ITER related physics issues National role - physics basis for K-Demo design K-Demo based on current ITER scaling is a challenge (size matters !!) Physics basis of the Transport and Stability for ITER size K-Demo New and high impact physics topics Redefine the conventional wisdoms What is the magic of the L/H/l/Q,.. scalings ? Suppression or mitigation of the harmful MHD instabilities Current drive and bootstrap current profile control What are the key physics parameters for compact reactor? Go with what you believe !! I am pretty tired. I think I’ll go home now What is the fundamentals of H-mode? L/H mode operation Circular plasma (limiter fueling and series of radial low resistors – L-mode Diverter plasmas (x-point DIII-D, R. Groebner, et al. fueling and series of high PPFC 44, 2002 resistors – H-mode Reduction of recycling with Li and core heating Energy and particle flux (in and out) – to guess the transport physics NSTX, M. Ono, et al. FED, 2010 What is the fundamentals of ITB? Super/RS/ERS mode operation Heavy recycling control (Li) and core heating profile - Source and Loss in power balance Energy and particle TFTR, Efthimion, et al. flux (in and out) at a flux surface is not known – measures only the difference JT-60U, Fujita, et al . PRL 1997 TFTR, D. Mansfield, et al. Phys. of Plasma. 1996 New idea and new methodology Remaining physics issues Stethoscope and engineering challenges require new path Physics - experimental verification of the hypothesis and assumptions is essential for the advancement Comprehensive visualization of magnetic reconnection process is an example Engineering – Discovery/ Invention of new materials to reduce the cost of the fusion reactor Magnetic resonance imaging Example: Classical sawtooth oscillation Sudden break up of a stable magnetic surface in a time scale much shorter than energy transport time Sawtooth oscillation is a magnetic self-organization via magnetic reconnection process H. Park (PRL, 2006) Simultaneous measurement (~400 channels) World first observation of core and edge MHD instabilities simultaneously Core – sawtooth Edge - ELMs In 2012, POSTECH will attempt world first 3-D measurement in fusion devices Two imaging systems separated on toroidal plane G. Yun (PRL, 2011) Summary Long but significant progress has been made in high temperature plasma research Progress is clear from the early skepticism of the star power to ITER Paradigm change in the fusion research is evident Two important roles of KSTAR International research device for ITER physics and human resource development Physics basis for K-Demo New path for advanced fusion reactor design “New Idea” and “New Methodology” are essential .
Recommended publications
  • Controlled Nuclear Fusion
    Controlled Nuclear Fusion HANNAH SILVER, SPENCER LUKE, PETER TING, ADAM BARRETT, TORY TILTON, GABE KARP, TIMOTHY BERWIND Nuclear Fusion Thermonuclear fusion is the process by which nuclei of low atomic weight such as hydrogen combine to form nuclei of higher atomic weight such as helium. two isotopes of hydrogen, deuterium (composed of a hydrogen nucleus containing one neutrons and one proton) and tritium (a hydrogen nucleus containing two neutrons and one proton), provide the most energetically favorable fusion reactants. in the fusion process, some of the mass of the original nuclei is lost and transformed to energy in the form of high-energy particles. energy from fusion reactions is the most basic form of energy in the universe; our sun and all other stars produce energy through thermonuclear fusion reactions. Nuclear Fusion Overview Two nuclei fuse together to form one larger nucleus Fusion occurs in the sun, supernovae explosion, and right after the big bang Occurs in the stars Initially, research failed Nuclear weapon research renewed interest The Science of Nuclear Fusion Fusion in stars is mostly of hydrogen (H1 & H2) Electrically charged hydrogen atoms repel each other. The heat from stars speeds up hydrogen atoms Nuclei move so fast, they push through the repulsive electric force Reaction creates radiant & thermal energy Controlled Fusion uses two main elements Deuterium is found in sea water and can be extracted using sea water Tritium can be made from lithium When the thermal energy output exceeds input, the equation is self-sustaining and called a thermonuclear reaction 1929 1939 1954 1976 1988 1993 2003 Prediction Quantitativ ZETA JET Project Japanese Princeton ITER using e=mc2, e theory Tokomak Generates that energy explaining 10 from fusion is fusion.
    [Show full text]
  • NEWSLETTER Issue No. 7 September 2017
    NEWSLETTER September 2017 Issue no. 7 Nuclear Industry Group Newsletter September 2017 Contents Notes from the Chair ................................................................................... 3 IOP Group Officers Forum .......................................................................... 4 NIG Committee Elections ............................................................................ 6 Nuclear Industry Group Career Contribution Prize 2017 .......................... 7 Event – Gen IV Reactors by Richard Stainsby (NNL) ................................ 8 Event – Nuclear Security by Robert Rodger (NNL) and Graham Urwin (RWM) ......................................................................................................... 12 Event – The UK’s Nuclear Future by Dame Sue Ion ................................ 13 Event – Regulatory Challenges for Nuclear New Build by Mike Finnerty. .................................................................................................................... 15 Event – European Nuclear Young Generation Forum ............................. 18 Event – Nuclear Fusion, 60 Years on from ZETA by Chris Warrick (UKAEA), Kate Lancaster (York Plasma Institute), David Kingham (Tokamak Energy) and Ian Chapman (UKAEA) ....................................... 19 IOP Materials and Characterisation Group Meetings .............................. 25 “Brexatom” – the implications of the withdrawal for the UK from the Euratom Treaty. ........................................................................................
    [Show full text]
  • The Economist's Free E-Mail Newsletters Twist and Shout and Alerts
    Log in Register My account Subscribe Digital & mobile Newsletters RSS Jobs Help Thursday September 1st 2011 Search World politics Business & finance Economics Science & technology Culture Blogs Debate & discuss Multimedia Print edition Fusion power Be the first to comment Print Next ITERation? E-mail Reprints & permissions Generating electricity by nuclear fusion has long looked like a chimera. A reactor being built in Germany may change that Advertisement Sep 3rd 2011 | from the print edition Like 3 7 Most commented Most recommended 1. China's military power: Modernisation in sheep's clothing 2. Charlemagne: Among the dinosaurs 3. Anti-corruption protests in India: No modern-day AS THE old joke has it, fusion is the power of the future—and always will be. The sales Mahatma pitch is irresistible: the principal fuel, a heavy isotope of hydrogen called deuterium, 4. German business and politics: Goodbye to Berlin can be extracted from water. In effect, therefore, it is in limitless supply. Nor, unlike 5. Libya: The birth of free Libya fusion’s cousin, nuclear fission, does the process produce much in the way of 6. Immigration: Let them come radioactive waste. It does not release carbon dioxide, either. Which all sounds too good 7. Climate science (II): Clouds in a jar to be true. And it is. For there is the little matter of building a reactor that can run for 8. Language learning: No, she's foreign! long enough to turn out a meaningful amount of electricity. Since the first attempt to do 9. Martin Luther King: A blockheaded memorial so, a machine called Zeta that was constructed in Britain in the 1950s, no one has even 10.
    [Show full text]
  • Nicholas Christofilos and the Astron Project in America's Fusion Program
    Elisheva Coleman May 4, 2004 Spring Junior Paper Advisor: Professor Mahoney Greek Fire: Nicholas Christofilos and the Astron Project in America’s Fusion Program This paper represents my own work in accordance with University regulations The author thanks the Program in Plasma Science and Technology and the Princeton Plasma Physics Laboratory for their support. Introduction The second largest building on the Lawrence Livermore National Laboratory’s campus today stands essentially abandoned, used as a warehouse for odds and ends. Concrete, starkly rectangular and nondescript, Building 431 was home for over a decade to the Astron machine, the testing device for a controlled fusion reactor scheme devised by a virtually unknown engineer-turned-physicist named Nicholas C. Christofilos. Building 431 was originally constructed in the late 1940s before the Lawrence laboratory even existed, for the Materials Testing Accelerator (MTA), the first experiment performed at the Livermore site.1 By the time the MTA was retired in 1955, the Livermore lab had grown up around it, a huge, nationally funded institution devoted to four projects: magnetic fusion, diagnostic weapon experiments, the design of thermonuclear weapons, and a basic physics program.2 When the MTA shut down, its building was turned over to the lab’s controlled fusion department. A number of fusion experiments were conducted within its walls, but from the early sixties onward Astron predominated, and in 1968 a major extension was added to the building to accommodate a revamped and enlarged Astron accelerator. As did much material within the national lab infrastructure, the building continued to be recycled. After Astron’s termination in 1973 the extension housed the Experimental Test Accelerator (ETA), a prototype for a huge linear induction accelerator, the type of accelerator first developed for Astron.
    [Show full text]
  • 1 Looking Back at Half a Century of Fusion Research Association Euratom-CEA, Centre De
    Looking Back at Half a Century of Fusion Research P. STOTT Association Euratom-CEA, Centre de Cadarache, 13108 Saint Paul lez Durance, France. This article gives a short overview of the origins of nuclear fusion and of its development as a potential source of terrestrial energy. 1 Introduction A hundred years ago, at the dawn of the twentieth century, physicists did not understand the source of the Sun‘s energy. Although classical physics had made major advances during the nineteenth century and many people thought that there was little of the physical sciences left to be discovered, they could not explain how the Sun could continue to radiate energy, apparently indefinitely. The law of energy conservation required that there must be an internal energy source equal to that radiated from the Sun‘s surface but the only substantial sources of energy known at that time were wood or coal. The mass of the Sun and the rate at which it radiated energy were known and it was easy to show that if the Sun had started off as a solid lump of coal it would have burnt out in a few thousand years. It was clear that this was much too shortœœthe Sun had to be older than the Earth and, although there was much controversy about the age of the Earth, it was clear that it had to be older than a few thousand years. The realization that the source of energy in the Sun and stars is due to nuclear fusion followed three main steps in the development of science.
    [Show full text]
  • Years of Fusion Research
    “50” Years of Fusion Research Dale Meade Fusion Innovation Research and Energy® Princeton, NJ Independent Activities Period (IAP) January 19, 2011 MIT PSFC Cambridge, MA 02139 1 FiFusion Fi FiPre Powers th thSe Sun “We nee d to see if we can mak e f usi on work .” John Holdren @MIT, April, 2009 3 Toroidal Magg(netic Confinement (1940s-earlyy) 50s) • 1940s - first ideas on using a magnetic field to confine a hot plasma for fusion. • 1947 Sir G.P. Thomson and P. C. Thonemann began classified investigations of toroidal “pinch” RF discharge, eventually lead to ZETA, a large pinch at Harwell, England 1956. • 1949 Richter in Argentina issues Press Release proclaiming fusion, turns out to be bogus, but news piques Spitzer’s interest. • 1950 Spitzer conceives stellarator while on a ski lift, and makes ppproposal to AEC ($50k )-initiates Project Matterhorn at Princeton. • 1950s Classified US Program on Controlled Thermonuclear Fusion (Project Sherwood) carried out until 1958 when magnetic fusion research was declassified. US and others unveil results at 2nd UN Atoms for Peace Conference in Geneva 1958. Fusion Leading to 1958 Geneva Meeting • A period of rapid progress in science and technology – N-weapons, N-submarine, Fission energy, Sputnik, transistor, .... • Controlled Thermonuclear Fusion had great potential – Much optimism in the early 1950s with expectation for a quick solution – Political support and pressure for quick results (but bud gets were low, $56M for 1951-1958) – Many very “innovative” approaches were put forward. – Early fusion reactor concepts - Tamm/Sakharov, Spitzer (Model D) very large. • Reality began to set in by the mid 1950s – Coll ectiv e eff ects - MHD instability ( 195 4), Bo hm d iffus io n was ubi qui tous – Meager plasma physics understanding led to trial and error approaches – A multitude of experiments were tried and ended up far from fusion conditions – Magnetic Fusion research in the U.S.
    [Show full text]
  • ITER Session at the IAEA Fusion Energy Conferencexa304 3
    ITER activities in 2003 is expected to be on the same level as in previous years, It was reported that the mandate of the Russian delegation to participate in the Negotiations in 2003 is expected to be approved soon by the Government. The RF delegation also reported that they had received informal enquiries from the Republic of Korea about possible participation in ITER. Dr. S. Matsuda, Moderator of the Fifth Meeting of the Negotiations Standing Sub-Group (NSSG-5, held in Rokkasho-mura on 7-9 October 2002) introduced the progress report of the NSSG. The delegations noted the progress report from the NSSG on the Joint Assessment of Specific Sites (JASS). The joint assessment of the Japanese site at Rokkasho-mura was conducted on 2-5 October 2002. This followed the assessment in September of the proposed Canadian site at Clarington. With the successful conduct of these two assessments, the JASS process is at the halfway mark. The last two site assessments will be carried out i] December at the two sites proposed by the European Union one at Cadar-ache in France and the other at Vandellos in Spain. It was agreed that the final report of the JASS would be presented at the Eighth Negotiations Meeting (N8), Significant progress was also made on a wide range of other issues, including matters such as the treaty to implement ITER (the Joint Implementation Agreement - JIA), procurement allocation and the intellectual property rights thait would accrue to participants in the project. The Negotiators agreed that the international organization responsible for implementing the project would be called the ITE-R International Fusion Energy Organization.
    [Show full text]
  • Sixty Years on from ZETA …
    Sixty years on from ZETA … Chris Warrick The Sun … What is powering it? Coal? Lifetime 3,000 years Gravitational Energy? Lifetime 30 million years – Herman Von Helmholtz, Lord Kelvin - mid 1800s The Sun … Suggested the Earth is at least 300 million years old – confirmed by geologists studying rock formations … The Sun … Albert Einstein (Theory of Special Relativity) and Becquerel / Curie’s work on radioactivity – suggested radioactive decay may be the answer … But the Sun comprises hydrogen … The Sun … Arthur Eddington proposed that fusion of hydrogen to make helium must be powering the Sun “If, indeed, the subatomic energy is being freely used to maintain their great furnaces, it seems to bring a little nearer to fulfilment our dream of controlling this latent power for the well-being of the human race – or for its suicide” Cambridge – 1930s Cockcroft Walton accelerator, Cavendish Laboratory, Cambridge. But huge energy losses and low collisionality Ernest Rutherford : “The energy produced by the breaking down of the atom is a very poor kind of thing . Anyone who expects a source of power from the transformation of these atoms is talking moonshine.” Oxford – 1940s Peter Thonemann – Clarendon Laboratory, Oxford. ‘Pinch’ experiment in glass, then copper tori. First real experiments in sustaining plasma and magnetically controlling them. Imperial College – 1940s George Thomson / Alan Ware – Imperial College London then Aldermaston. Also pinch experiments, but instabilities started to be observed – especially the rapidly growing kink instability. AERE Harwell Atomic Energy Research Establishment (AERE) Harwell – Hangar 7 picked up fusion research. Fusion is now classified. Kurchatov visit 1956 ZETA ZETA Zero Energy Thermonuclear Apparatus Pinch experiment – but with added toroidal field to help with instabilities and pulsed DC power supplies.
    [Show full text]
  • Plasma Physics and Controlled Fusion Research During Half a Century Bo Lehnert
    SE0100262 TRITA-A Report ISSN 1102-2051 VETENSKAP OCH ISRN KTH/ALF/--01/4--SE IONST KTH Plasma Physics and Controlled Fusion Research During Half a Century Bo Lehnert Research and Training programme on CONTROLLED THERMONUCLEAR FUSION AND PLASMA PHYSICS (Association EURATOM/NFR) FUSION PLASMA PHYSICS ALFV N LABORATORY ROYAL INSTITUTE OF TECHNOLOGY SE-100 44 STOCKHOLM SWEDEN PLEASE BE AWARE THAT ALL OF THE MISSING PAGES IN THIS DOCUMENT WERE ORIGINALLY BLANK TRITA-ALF-2001-04 ISRN KTH/ALF/--01/4--SE Plasma Physics and Controlled Fusion Research During Half a Century Bo Lehnert VETENSKAP OCH KONST Stockholm, June 2001 The Alfven Laboratory Division of Fusion Plasma Physics Royal Institute of Technology SE-100 44 Stockholm, Sweden (Association EURATOM/NFR) Printed by Alfven Laboratory Fusion Plasma Physics Division Royal Institute of Technology SE-100 44 Stockholm PLASMA PHYSICS AND CONTROLLED FUSION RESEARCH DURING HALF A CENTURY Bo Lehnert Alfven Laboratory, Royal Institute of Technology S-100 44 Stockholm, Sweden ABSTRACT A review is given on the historical development of research on plasma physics and controlled fusion. The potentialities are outlined for fusion of light atomic nuclei, with respect to the available energy resources and the environmental properties. Various approaches in the research on controlled fusion are further described, as well as the present state of investigation and future perspectives, being based on the use of a hot plasma in a fusion reactor. Special reference is given to the part of this work which has been conducted in Sweden, merely to identify its place within the general historical development. Considerable progress has been made in fusion research during the last decades.
    [Show full text]
  • Los Alamos National Laboratory
    Spotlight on National Labs Los Alamos National Laboratory Thom Mason, Director of Los Alamos National Laboratory Alan Carr, Historian of Los Alamos National Laboratory Leslie Sherrill, Group Leader, XTD-IDA (Integrated Design and Assessment) Alexis Trahan, Engineer, NEN-1 (Safeguards Science and Technology) Joetta Goda, Engineer, NEN-2 (Advanced Nuclear Technology) Dave Poston, Chief Reactor Designer, NEN-5 (Systems Design and Analysis) Moderator Nicholas Thompson, Engineer, NEN-2 (Advanced Nuclear Technology) May 6, 2020 ANS Spotlight on National Labs Los Alamos National Laboratory Thom Mason Director of LANL May 6, 2020 LA-UR-20-23309 75+ years serving the nation • In 1943, Los Alamos Laboratory was founded with a single, urgent purpose: build an atomic bomb • The future holds no shortage of national security threats, but there is no shortage of innovative ways to combat those threats • LANL leverages strategic nuclear deterrence to solve challenges to our nation’s security LANL’s national security focus means we are uniquely qualified to tackle big, novel problems such as COVID-19 Los Alamos National Laboratory 4/30/20 | 3 Our 12,866 employees rely on cutting-edge equipment and facilities to solve grand challenges on Earth and in space • 37.8 sq. mile campus (about the size of D.C.) • Flagship research facilities For plutonium, explosives, simulations, chemistry, and more, enabling work that’s impossible anywhere else • Much of our stockpile research is applied to complex challenges in: – Climate change – Vaccine development & epidemic
    [Show full text]
  • Nuclear Fusion Power – an Overview of History, Present and Future
    International Journal of Advanced Network, Monitoring and Controls Volume 04, No.04, 2019 Nuclear Fusion Power – An Overview of History, Present and Future Stewart C. Prager Department of Physics University of Wisconsin – Madison Madison, WI 53706, USA E-mail: [email protected] Summary—Fusion power offers the prospect of an allowing the nuclei to fuse together. Such conditions almost inexhaustible source of energy for future can occur when the temperature increases, causing the generations, but it also presents so far insurmountable ions to move faster and eventually reach speeds high engineering challenges. The fundamental challenge is to enough to bring the ions close enough together. The achieve a rate of heat emitted by a fusion plasma that nuclei can then fuse, causing a release of energy. exceeds the rate of energy injected into the plasma. The main hope is centered on tokamak reactors and II. FUSION TECHNOLOGY stellarators which confine deuterium-tritium plasma In the Sun, massive gravitational forces create the magnetically. right conditions for fusion, but on Earth they are much Keywords-Fusion Energy; Hydrogen Power; Nuclear Fusion harder to achieve. Fusion fuel – different isotopes of hydrogen – must be heated to extreme temperatures of I. INTRODUCTION the order of 50 million degrees Celsius, and must be Today, many countries take part in fusion research kept stable under intense pressure, hence dense enough to some extent, led by the European Union, the USA, and confined for long enough to allow the nuclei to Russia and Japan, with vigorous programs also fuse. The aim of the controlled fusion research underway in China, Brazil, Canada, and Korea.
    [Show full text]
  • Spitzer S 100Th: Founding PPPL & Pioneering Work in Fusion Energy
    (1) Spitzer’s 100th: Founding PPPL & Pioneering Work in Fusion Energy Greg Hammett (2) Some Stories From Working with Spitzer In the Early Years Russell Kulsrud Princeton Plasma Physics Laboratory Colloquium Dec. 4, 2013 These are shorter versions of talks we gave at the 100th Birthday Celebration for Lyman Spitzer, October 19-20, 2013, Peyton Hall, Princeton University, http://www.princeton.edu/astro/news-events/public-events/spitzer-100/ https://www.princeton.edu/research/news/features/a/?id=11377 Video of a longer talk by Kulsrud, “My Early Years Spent Working with Lyman Spitzer“: https://mediacentral.princeton.edu/id/1_1kil7s0p Thanks for slides: Dale Meade, Rob Goldston, Eleanor Starkman and PPPL photo archives, ... PPPL Historical Photos: https://www.dropbox.com/sh/tjv8lbx2844fxoa/FtubOdFWU2 June 19, 2014: added historical info. Jul 9, 2015: pointer to updated figure Lyman Spitzer Jr.’s 100th: Founding PPPL & Pioneering Work in Fusion Energy Outline: • Pictorial tour: from Spitzer’s early days, the Model-C stellarator (1960’s), to TFTR’s 10 megawatts of fusion & the Hubble Space Telescope (Dec. 9-10, 1993) • Russell Kulsrud: A few personal reflections on early days working with Lyman Spitzer. • The road ahead for fusion: – Interesting ideas being pursued in fusion, to improve confinement & reduce the cost of power plants I never officially met Prof. Spitzer, though I saw him at a few seminars. Heard many stories from Tom Stix, Russell Kulsrud, & others, learned from the insights in his book and his ideas in other books. 2 2 Lyman Spitzer, Jr. 1914-1997 Photo by Orren Jack Turner, from Biographical Memoirs V.
    [Show full text]