Fusion Energy Science Opportunities in Emerging Concepts
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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. -
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. -
Plasma Physics Division Fachverband Plasmaphysik (P)
Hannover 2016 – P Overview Plasma Physics Division Fachverband Plasmaphysik (P) Navid Mahdizadeh ABB Switzerland Ltd Brown-Boveri-Strasse 5 CH-8050 Zürich [email protected] Overview of Invited Talks and Sessions (Lecture rooms b302 and b305; Poster Empore Lichthof) Invited Talks P 2.1 Mon 11:00–11:30 b305 Mid-infrared cavity enhanced absorption spectroscopy of gas and surface species — ∙Jean-Pierre van Helden, Norbert Lang, Andy Nave, Jürgen Röpcke P 3.1 Mon 14:30–15:00 b302 Advances in Laser Manipulation of Dusty Plasmas — ∙Jan Schablinski, Frank Wieben, Dietmar Block P 4.1 Mon 14:30–15:00 b305 Impact of electron attachment processes on nonthermal plasmas — ∙Jürgen Meichsner, Sebastian Nemschokmichal, Robert Tschiersch, Thomas Wegner P 6.1 Tue 11:00–11:30 b302 ns-Pulsed Micro-Plasmas at Atmospheric Pressures — ∙Uwe Czarnetzki P 7.1 Tue 11:00–11:30 b305 Erste Ergebnisse an Wendelstein 7-X — ∙Hans-Stephan Bosch, W7-X Team P 8.1 Tue 14:30–15:00 b302 Nanometer-scale characterization of laser-driven plasmas, compression, shocks and phase transitions, by coherent small angle x-ray scattering — ∙Thomas Kluge, Melanie Rödel, Alexander Pelka, Emma McBride, Luke Fletcher, Christian Rödel, Siegfried Glenzer, Michael Buss- mann, Ulrich Schramm, Thomas Cowan P 9.1 Tue 14:30–15:00 b305 Computer simulations of correlated fermions–from quantum plasmas to ultracold atoms and plasma-surface interaction — ∙Michael Bonitz P 13.1 Wed 11:00–11:30 b302 Power exhaust by impurity seeding in fusion reactors — ∙Matthias Bern- ert, Felix Reimold, Arne Kallenbach, Bruce Lipschultz, Ralph Dux, Marco Wischmeier, the ASDEX Upgrade team, the EUROfusion MST1 Team P 17.1 Wed 14:30–15:00 b305 Plasma measurement and control: challenges and recent advances — ∙Timo Gans P 21.1 Thu 11:00–11:30 b302 The behavior of helium in fusion plasmas — ∙Athina Kappatou, Rachael M. -
∫° Plasma Confinement in a Levitated Magnetic Dipole
Plasma Physics Reports, Vol. 23, No. 9, 1997, pp. 742–750. From Fizika Plazmy, Vol. 23, No. 9, 1997, pp. 801–810. Original English Text Copyright © 1997 by Kesner, Mauel. MAGNETIC CONFINEMENT SYSTEMS Plasma Confinement in a Levitated Magnetic Dipole J. Kesner* and M. Mauel** * Massachusetts Institute of Technology, Cambridge, Ma 02129 ** Columbia University, New York, N.Y. 10027 Received April 1, 1995 Abstract—Plasma confinement in the field of a levitated dipole offers many advantages for magnetic fusion. MHD stability is obtained from compressibility which utilizes the large flux tube expansion of a dipole field. Such a device could be high beta, steady state, and exhibit good confinement properties. The large flux expan- sion will ease the difficulty of the divertor design. The configuration is ideal for electron cyclotron heating and controlled convective flow patterns may provide a mechanism for fueling and ash removal. 1. INTRODUCTION tribution function, µ is the adiabatic invariant, µ = The dipole magnetic field is the simplest and most e⊥/2B, J is the parallel invariant, J = °∫v || dl and the flux, common magnetic field configuration in the universe. It ψ is the third adiabatic invariant. The frequencies that is the magnetic far-field of a single, circular current Ω correspond to these invariants are respectively c the loop, and it represents the dominate structure of the cyclotron frequency, ω , the bounce frequency and ω middle magnetospheres of magnetized planets and neu- b d tron stars. The use of a dipole magnetic field generated the curvature driven precessional drift frequency. Both by a levitated ring to confine a hot plasma for fusion of these conditions lead to dipole pressure profiles that scale with radius as r–20/3 while the adiabatic distribu- power generation was first considered by Akira Haseg- µ awa after participating in the Voyager 2 encounter with tion function, F( , J) also implies a density dependence ∝ –4 ∝ –8/3 Uranus [1]. -
Een Kernfusie Concept
Kernfusie Dr. Robert Bussard over kernfusie http://video.google.com/videoplay?docid=1996321846673788606# In de bovenstaande link geeft Robert Bussard een conferentie over alternatieve fusie energie waar hij zijn alternatieve opstelling “de polywell” verdedigt. Hoewel de benadering tot kernfusie in dit document geheel anders is, is het doel en sommige basisprincipes hetzelfde en had ik het zelf niet beter kunnen verwoorden. De opstelling De opstelling bestaat uit een sferische tank die doormiddel van een mechanisch systeem (fig1) wordt rondgedraaid, dit in twee dimensies. Het rondspinnen om twee assen van het lichaam zorgt ervoor dat deeltjes met de hoogste massadichtheid naar buiten worden geslingerd. De deeltjes met de laagste dichtheid worden hierdoor naar het center gedrukt. Als er dus bijvoorbeeld water in de sfeer bevindt, zal deze homogeen over de binnenkant van de sferische wand worden gedrukt. De lichtere, eventueel hetere deeltjes worden in het center gehouden. Warmteconvectie wordt hierdoor onderdrukt. Dit maakt dat het plasma geïsoleerd is zonder dat er een vacuüm kamer noodzakelijk is. Zoals bij een Tokamak, Stellator, Fusor of polywell wel het geval is. Hierdoor kan de druk in het plasma makkelijk opgevoerd worden zonder dat er super magneten voor noodzakelijk zijn, simpel weg door statische druk. Dit zou een drastisch verschil moeten maken in energiedichtheid. De opgewekte energie stijgt kwadratisch met De figuur 1: Het draaimechanisme de druk. Tevens kunnen er energieke geladen plasma deeltjes geïnjecteerd worden, wat bij magnetische opsluiting niet mogelijk is. sferische tank met daar rond het draaimechanisme bevindt zich in een tweede robuustere tank die bestand is tegen hoge druk. De vrijgekomen energie wordt afgevoerd voordat het de reactorwand bereikt evenals de 14Mev neutronen worden gemodereerd. -
Powerpoint Presentation: Fusion Energy: "Pipe Dream Or Panacea"
Fusion Energy: “Pipe Dream or Panacea” Mike Mauel Columbia University Energy Options & Paths to Climate Stabilization Aspen, 9 July 2003 Fusion Energy: “Pipe Dream or Panacea” “Promise, Progress, and the Challenge Ahead” Mike Mauel Columbia University Energy Options & Paths to Climate Stabilization Aspen, 9 July 2003 ~ OUTLINE ~ Fusion Primer Power Configurations Progress MFE Next Steps: Optimization and Burning Plasma “Fast Track” 35 Year Plan to enable Commercial Power References • Rose and Clark: Plasmas and Controlled Fusion (1961) • Sheffield: “The Physics of Magnetic Fusion Reactors,” RMP (1994) • Hawryluk: “Results from D-T Tokamak Confinement Experiments,” RMP (1998) • Example fusion resource development scenarios… • Schmidt, et al., “U.S. Fusion Future,” Fus. Tech. (2001) • Ongena and Van Oos, “Energy for future centuries. Will fusion be an inexhaustible, safe and clean energy source?” Fus. Sci. and Tech. (2002) • Report of the European Fusion “Fast Track”, D. King, et al. (2001) • Report of the U.S. DOE FESAC “A [35 Year] Plan to Develop Fusion Energy” (2003) • “The FIRE Place” http://fire.pppl.gov/ • Levitated Dipole Experiment http://www.psfc.mit.edu/ldx/ Why Fusion Energy Science? • for fundamental plasma physics and critical plasma technologies • for national defense • for fusion energy… • Inexhaustible: “unlimited” fuel and available to all nations; Low land-use costs • “Clean”: no greenhouse gases nor air pollution; Storage of short-lived radioactive components. • Safe: no catastrophic accidents; Low-risk for nuclear materials proliferation Today is an Exciting Time for Fusion Research • Tremendous progress in understanding how to confine & control high-temperature matter, e.g. • Suppression of some forms of turbulence • Control of some pressure-limiting instabilities • First light achieved at NIF • Negotiations well-along to start ITER construction: an international burning plasma experiment at the scale of a power plant. -
Minimization of Magnetic Forces on Stellarator Coils Arxiv:2103.13195
Minimization of magnetic forces on Stellarator coils R´emiRobin∗; 1 and Francesco Volpe †2 1 Laboratoire Jacques-Louis Lions, Sorbonne Universit´e 2Renaissance Fusion, https://stellarator.energy March 25, 2021 Abstract Magnetic confinement devices for nuclear fusion can be large and expensive. Compact stellarators are promising candidates for cost- reduction, but introduce new difficulties: confinement in smaller vol- umes requires higher magnetic field, which calls for higher coil-currents and ultimately causes higher Laplace forces on the coils - if everything else remains the same. This motivates the inclusion of force reduction in stellarator coil optimization. In the present paper we consider a coil winding surface, we prove that there is a natural and rigorous way to define the Laplace force (despite the magnetic field discontinuity across the current-sheet), we provide examples of cost associated (peak force, surface-integral of the force squared) and discuss easy generalizations to parallel and normal force-components, as these will be subject to different engineering constraints. Such costs can then be easily added arXiv:2103.13195v1 [math.OC] 24 Mar 2021 to the figure of merit in any multi-objective stellarator coil optimiza- tion code. We demonstrate this for a generalization of the REGCOIL code [1], which we rewrote in python, and provide numerical examples for the NCSX (now QUASAR) design. We present results for various definitions of the cost function, including peak force reductions by up to 40 %, and outline future work for further reduction. ∗[email protected] †[email protected] 1 1 Introduction Stellarators are non-axisymmetric toroidal devices that magnetically confine fusion plasmas [2]. -
Physics Research
TheT HE Plasma P LASMA Science S CIENCE && FusionF USION CenterC EN T ER • MMassachusettsASSACHUSE tt S I NSInstituteT I T U T E O Fof T ECHNOLOGYTechnology PHYSICS RESEARCH Understanding the basic physics of plasmas is necessary not only to advance fusion research, but to increase the physics-based foundations of plasma-related scientific disciplines and applications. embers of the Physics Re- search Division, including theoretical and experimen- Mtal plasma physicists, faculty mem- bers, graduate and undergraduate students and visiting collaborators, work together to better understand plasmas and to extend their uses. Research includes: ■ Laboratory experiments ■ Development of novel plasma diagnostics ■ Theory of magnetically confined fusion plasmas Photo by Paul Rivenberg Dr. Jan Egedal works atop the Versatile Toroidal Facility, a medium-sized tokamak currently ■ Nonlinear wave used to study magetic reconnection, a phenomenon observed in solar flares. propagation, turbulence In addition to basic plasma theory, waves to control pressure and current and chaos topics being pursued at the PSFC profiles in order to control instabilities ■ Space plasma physics include tokamak research on radio and achieve steady state operation in frequency heating and current drive, high pressure plasmas. ■ Plasma astrophysics core and edge transport and turbu- ■ Laser-plasma interactions lence, and magnetohydrodynamic and In the area of inertial confinement kinetic stability. This research sup- fusion (ICF), theorists study the ports the PSFC tokamak, Alcator C- ablation process, during which a Theoretical Plasma Physics Mod, and the Levitated Dipole Experi- plasma is created that causes nonlin- ment (LDX), as well as other such ear scattering of the laser light. This Using the fundamental laws of experiments around the world. -
Fusion Energy: Progress Towards an Unlimited Energy Source
Fusion Energy: Progress towards an Unlimited Energy Source Mike Mauel Columbia University http://www.columbia.edu/~mem4/ and Jefferson Science Fellow EEB/ESC/IEC 5 June 2007 Today is an Exciting Time for Fusion • Tremendous progress in understanding how to confine & control high-temperature matter • Experiments are extending the limits technology: superconductivity, lasers, heat sources, advanced materials, systems control, and computation,… • First light achieved at National Ignition Facility (NIF) • International community to build ITER: the first burning plasma experiment at the scale of a power plant & the world’s largest energy science partnership. Outline • Fusion Primer • Can fusion be “green” nuclear power? • Exciting Science and Experiments • ITER: Fusion at the scale of a power plant • Discussion and questions “Forces” of Nature Gravity Tidal Energy Electromagnetic/ Combustion, Batteries, “Everyday” Molecular Energy and Chemistry Weak/Radiation Geothermal Energy Fission, Fusion, and Solar Strong/Nuclear (including wind, hydro, …) Chemical vs. Nuclear Energy Density Why Fission is (Relatively) Easy to Do… • Nuclear force is very-short ranged. Must get very close! • Neutrons can easily split big, 92 protons positively-charged nuclei… 144 neutrons • Because neutrons are neutral! • Nucleons like to be paired (even numbers!) so certain nuclei are fissile: 233U, 235U, 239Pu Why Fusion is (Really, Really) Hard to Do… Deuterium Tritium • Nuclear force is very-short ranged. Must get very close! • Fusion requires close contact between light -
American Nuclear Society Fusion Energy Division December 2009 Newsletter
American Nuclear Society Fusion Energy Division December 2009 Newsletter Letter from the Chair Snead New ANS “Fusion” Fellows Uckan FED Slate of Candidates Najmabadi 19th ANS Topical Meeting on the Technology of Fusion Energy Najmabadi/Sharafat Call for Nominations: ANS-FED Awards Morley Fusion Award Recipients El-Guebaly News from Fusion Science and Technology Journal Uckan Ongoing Fusion Research: Recent Advances in High Temperature Superconductors Minervini Highlights of US Fusion-Fission Hybrid Workshop Freidberg International Activities: ITER Update Sauthoff Report on IAEA Technical Meetings on “First Generation of Fusion Power Plants: Design and Technology” and “Fusion Power Plant Safety” Mank/Kamendje Letter from the Chair, Lance Snead, Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN. As the subject of this letter I would like to bring the Fusion Energy Division (FED) membership up to speed on some of the metrics for our division. I am also happy to do so as the previous Chairs have made our division look quite good. For those of you who are not intimately plugged into the American Nuclear Society (ANS), the overall society membership has been remarkably constant over the 2000 decade with total membership of approximately 10,800. As can be seen from the figure below, the membership of the FED over that period has had a significant increase, for which the Division receives high marks. The ANS has recently invested great effort into evaluating the strength of each Division and has devised a set of metrics by which they can determine where improvements need to be made and which of the 22 Professional Divisions are becoming subcritical. -
Plans for Creation and Studies of Positron- Electron Plasmas in a Laboratory Magnetosphere
Plans for creation and studies of positron- electron plasmas in a laboratory magnetosphere Thomas Sunn Pedersen, for the APEX/PAX collaboration (next slide) Max Planck Institute for Plasma Physics, Greifswald and Garching, Germany The PairPlasma Team: A Positron-Electron plasma eXperiment (APEX) Positron Accumulation eXperiment (PAX) APEX – PAX team Max Planck Institute for Plasma Physics, IPP (Greifswald and Garching): T. Sunn Pedersen, H. Saitoh, E.V. Stenson, J. Horn-Stanja, U. Hergenhahn, S. Nissel M. Stoneking C. Surko L. Schweikhard C. Hugenschmidt Lawrence U., J. Danielson G. Marx Markus Singer WI, USA UC San Diego Martin Singer T. U. Munich CA, USA U. Greifswald Germany Germany Current financial support by the following entities Max Planck Deutsche Japan Society for National Institute 2 Society, Forschungs- the Promotion of for Fusion Science Germany gemeinschaft, Science Germany Japan Overview • Electron-positron (pair) plasmas and their importance around astrophysical objects • Some unique basic properties of pair plasmas • First pair plasma in the laboratory – Sarri group • Short-lived, unconfined, dense, hot pair plasma beam • Debye length and skin depth – two important scale lengths in a plasma • Our attempt to create small-Debye length, confined pair plasmas • The “grand” plan • How far we are • Summary Astrophysical relevance • Pair plasmas are created around compact, high-energy density astrophysical objects • Continuous sources include: • Accreting black holes • Magnetars • Pulsed or explosive sources include: – Magnetar flares – Cosmological gamma-ray bursts (GRB) • Copious pair creation can be thought of as a “breakdown of the vacuum” – Gamma-gamma (photon-photon) collisions – Gammas+ seed electrons+ strong magnetic fields: “pair cascade” • Conversion of matter- and charge-free space to highly conducting, matter-filled space – a pair plasma Inspired by and partly taken from talk by A. -
IAEA-F1-CN-69/ICP/09 (Final)
PLASMA CONFINEMENT IN A MAGNETIC DIPOLE* J. KESNER AND L. BROMBERG Plasma Science and Fusion Center MIT, Cambridge, MA 02139, USA D. GARNIER AND M. MAUEL Department of Applied Physics, Columbia University New York, NY 10027, USA Abstract A dipole fusion confinement device is stable to MHD interchange and ballooning modes when the pressure profile is sufficiently gentle. The plasma can be confined at high beta, is steady state and disruption free. Theory indicates that when the pressure gradient is sufficiently gentle to satisfy MHD requirements drift waves will also be stable. The dipole approach is particularly applicable for advanced fuels. A new experimental facility is presently being built to test the stability and transport properties of a dipole-confined plasma. 1. INTRODUCTION The dipole fusion concept was first proposed by Hasegawa [1, 2] who was motivated by observations of high β, energetic plasma within planetary magnetospheres. Active magneto- spheres, such as that surrounding Jupiter, can have plasma pressures exceeding the magnetic pressure, β > 1. A dipole fusion confinement device takes advantage of these properties by operating with plasma profiles that have sufficiently gentle gradients to be stable to interchange and ballooning modes at high beta. This stability derives from plasma compressibility. The dipole confinement concept is fundamentally different from other fusion concepts since the diamagnetic ω frequency, *, proportional to the radial gradient of plasma pressure, is small relative to the magnetic drift frequency, ωd, proportional to the radial gradient of the magnetic field. The ω ω ≤ condition */ d 2 characterizes a unique regime in magnetic plasma confinement. It corresponds to MHD stability and the possible elimination of drift wave instabilities [3].