Laser Fusion: the First Ten Years 1962-1972
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Eyes for Gamma Rays” Though the Major Peaks Suggest a Periodic- Whether These Are Truly Gamma-Ray Bursts for a Description of This System)
sion of regularity and slow evolution in the They suggested that examination of the Vela exe-atmospheric nuclear detonation. Surpris- universe persisted into the 1960s. data might disclose evidence of bursts of ingly, however, the survey soon revealed that The feeling that transient cosmic events gamma rays at times close to the appearance the gamma-ray instruments on widely sepa- were rare was certainly prevalent in 1959 of supernovae. Such searches were con- rated satellites had sometimes responded when summit meetings were being held be- ducted; however, no distinctive signals were almost identically. Some of these events were tween England, the United States, and found. attributable to solar flare activity. However, Russia to discuss a nuclear test-ban treaty. On the other hand, there was evidence of one particularly distinctive event was dis- One key issue was the ability to detect treaty variability that had been ignored. For exam- covered for which a solar origin seemed violations unambiguously. A leading ple, the earliest x-ray data from small rocket inconsistent. Fortunately, the characteristics proposal for the detection of exo-at- probes and from satellites were often found of this event did not at all resemble those of a mospheric nuclear explosions was the use of to disagree significantly. The quality of the nuclear detonation, and thus the event did satellites with instruments that included de- data, rather than actual variations in the not create concern of a possible test-ban tectors sensitive to the gamma rays emitted sources, was suspected as the reason for treaty violation. by the explosion as well as those emitted these discrepancies. -
Weapons-Test Connection by Roger C
COMMENT The Weapons-Test Connection by Roger C. Eckhardt t the test ban summit meetings in 1959, Stirling Colgate from the gamma-ray detectors were searched for enhanced signals in watched the attention of the delegates drifting off the the vicinity of the times of reported supernovae in distant galaxies. technical discussion onto thoughts of wine and women. When these searches proved fruitless, the idea that an unknown and A He refocused their attention with one abrupt question: startlingly different phenomenon might be hiding in the data could Would the gamma rays from a supernova trigger the detectors in the not be examined with high priority by the people involved. During the proposed test-surveillance satellites? With this question, Colgate ten-year span they, instead, pursued an answer to a broader version connected the political goal of test surveillance with the scientific goal of Colgate’s original query: Could a natural background event mimic of understanding cosmic phenomena. In the satellite detection of the signal of an exe-atmospheric weapons test? Although this gamma rays this connection has persisted now for two decades. question was directed primarily toward the political goal, the natural However, it has been perceived in different ways with different scientific drive to eliminate even minor doubts resulted eventually in a consequences by different groups of people. surprise—the discovery of gamma-ray bursts. In truth, the time span At one extreme is the opinion represented by the National was due, not to classification, but to the fact that gamma-ray bursts Enquirer story that claimed gamma-ray bursts were evidence of were totally unexpected. -
Long Path Laser Spectroscopy of Weak
LONG PATH LASER SPECTROSCOPY OF WEAK SPECTRAL TRANSITIONS IN PLASMAS A Thesis Submitted for the Degree of DOCTOR OF PHILOSOPHY In the UNIVERSITY OF LONDON By MARK PHILIP SYDNEY NIGHTINGALE The Blackett Laboratory Imperial College of Science and Technology London SW7 2BZ LONG PATH LASER SPECTROSCOPY OF WEAK SPECTRAL TRANSITIONS IN PLASMAS By MARK PHILIP SYDNEY NIGHTINGALE ABSTRACT There has been much interest recently in spectral lineshapes, especially in plasmas where charge particle broadening is important. For the accurate measurement of such profiles, absorption spectroscopy offers distinct advantages over other techniques but requires the use of long optical paths (several metres or more) since, typically, plasma opacities are extremely low. A z-pinch plasma device has been used to generate a 10 metre long plasma column and optical paths in this plasma exceeding one kilometre have been achieved by the use of a multipassed CW dye laser system. Such paths allow both the accurate measurement of allowed line profiles over five orders of magnitude of absorption, and also provide the means of measuring weak features such as forbidden lines or continua. Full electron density diagnostics have been performed using interferometry (over twenty-one metre paths) and these show considerable density oscillations during the plasma recombination phase whose origins and effects might have considerable importance in the use of plasmas as spectroscopic sources. Results are presented for several long path absorption and 3 1 interferometric experiments. In Helium the 2p P - 3d 'D forbidden intercombination satellite on the 5876 A line-wing is fully resolved providing evidence as to its origin. -
The Proceedings of the 1St International Workshop O Laboratory Astrophysics Experiments with Large Lasers
CONF-960297— The Proceedings of the 1st International Workshop o Laboratory Astrophysics Experiments with Large Lasers B. A. Remington W.H. Goldstein August 9,1996 DISCLAIMER This document was prepared as an account of work sponsored by an agency of the United States Government Neither die United States Government nor the University of California nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any infonriation,apparatas,prodnc^orprocessdisdosed,ori«presentsthatitsnsewonldnotinfrmgeprivatelyownedright8. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement; recommendation, or favoring by the United States Government or the University of California. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Govenunent or the University of California, and shall notbe used for advertising or product endorsement purposes. This report has been reproduced directly from the best available copy. Available to DOE and DOE contractors from the Office of Scientific and Technical Information P.O. Box 62, Oak Ridge, TN 37831 Prices available from (615) 576-8401, FTS 626-8401 Available to the public from the National Technical Information Service US. Department of Commerce 5285 Port Royal Rcu, Springfield, VA 22161 WorkperfonnedundertheatispicesoftheU^.Departmentof Energy by IawrenceLivennoreNationalLaboratory-under Contract W-7405-Eng-48. DISCLAIMER Portions of this document may be illegible in electronic image products. Images are produced from the best available original document Contents Conference Photo i Title Page ii Scientific Committee/ Organizing Committee iii Preface iv-v Summary vi-xi I. -
Signature Redacted %
EXAMINATION OF THE UNITED STATES DOMESTIC FUSION PROGRAM ARCHW.$ By MASS ACHUSETTS INSTITUTE Lauren A. Merriman I OF IECHNOLOLGY MAY U6 2015 SUBMITTED TO THE DEPARTMENT OF NUCLEAR SCIENCE AND ENGINEERING I LIBR ARIES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF BACHELOR OF SCIENCE IN NUCLEAR SCIENCE AND ENGINEERING AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY FEBRUARY 2015 Lauren A. Merriman. All Rights Reserved. - The author hereby grants to MIT permission to reproduce and to distribute publicly Paper and electronic copies of this thesis document in whole or in part. Signature of Author:_ Signature redacted %. Lauren A. Merriman Department of Nuclear Science and Engineering May 22, 2014 Signature redacted Certified by:. Dennis Whyte Professor of Nuclear Science and Engineering I'l f 'A Thesis Supervisor Signature redacted Accepted by: Richard K. Lester Professor and Head of the Department of Nuclear Science and Engineering 1 EXAMINATION OF THE UNITED STATES DOMESTIC FUSION PROGRAM By Lauren A. Merriman Submitted to the Department of Nuclear Science and Engineering on May 22, 2014 In Partial Fulfillment of the Requirements for the Degree of Bachelor of Science in Nuclear Science and Engineering ABSTRACT Fusion has been "forty years away", that is, forty years to implementation, ever since the idea of harnessing energy from a fusion reactor was conceived in the 1950s. In reality, however, it has yet to become a viable energy source. Fusion's promise and failure are both investigated by reviewing the history of the United States domestic fusion program and comparing technological forecasting by fusion scientists, fusion program budget plans, and fusion program budget history. -
The Oppenheimer Years 1943-1945 6
" . .When you come right down to it the reason that we did this job is because it was an organic necessity. If you are a scientist you cannot stop such a thing . You believe that it is good to find out how the world works . [and] to turn over to mankind at large the greatest possible power to control the world and to deal with it according to its lights and its values. " . I think it is true to say that atomic weapons are a peril which affect everyone in the world, and in that sense a completely common problem . I think that in order to handle this common problem there must be a complete sense of community responsibility. " . The one point I want to hammer home is what an enormous change in spirit is involved. There are things which we hold very dear, and I think rightly hold very dear; I would say that the word democracy perhaps stood for some of them as well as any other word. There are many parts of the world in which there is no democracy . And when I speak of a new spirit in international affairs I mean that even to these deepest of things which we cherish, and for which Americans have been willing to die—and certainly most of us would be willing to die—even in these deepest things, we realize that there is something more profound than that; namely the common bond with other men everywhere . .“ J. Robert Oppenheimer speech to the Association of Los Alamos Scientists Los Alamos November 2, 1945 Excerpts from a speech to the Association of Los Alamos Scientists in Los Alamos, New Mexico, on November 2, 1945. -
Cover and Contents
All the animal species surrounding the AIDS virus (center) are targets of AIDS-like diseases. The slow viruses, or Ientiviruses, responsible for these diseases attack the cells of the host’s immune system. In the background are T4 cells, the primary target of the AIDS virus. The cells are stained with toluidine blue to identify nucleoproteins. The black dots, produced by radioactive probes, show the location of viral RNA in these infected cells. hy AIDS research at Los outlines the basic dynamics governing models are sadly lacking and often hard Alamos? In 1981 when the the epidemic in the United States. The to collect. Moreover, some data that wfirst AIDS cases were pub- model is based on two unique features have been collected are unavailable. licized, Stirling Colgate, a physicist of the AIDS case data from the Centers Seeing this deficiency, the Los Alamos at Los Alamos, was among those who for Disease Control (CDC). First, the group suggested in a commentary in Na- foresaw that a disease that undermines number of AIDS cases has not grown ture that a national database of complete the human immune system and is trans- exponentially with time (as happens and unfiltered information from diverse mitted through sexual contact could ex- when all members of a population are sources be established and made avail- pand into a worldwide pandemic. The equally at risk) but rather as the cube able to researchers and health officials threat seemed to him nearly as serious of time. Steady cubic growth between involved in surveying and forecasting as the threat of nuclear war, requiring 1982 and 1987 has occurred not only the course of the AIDS epidemic. -
PROTO-SPHERA Confines Axisymmetric Plasma Tori in Absence of Any Toroidal Magnet and Just in Presence of a Static Poloidal Magnetic Field
PROTO-SPHERA confines axisymmetric plasma tori in absence of any toroidal magnet and just in presence of a static poloidal magnetic field FSN Department, CR-ENEA Frascati Franco Alladio, Paolo Micozzi, Fabrizio Andreoli, Gerarda Apruzzese, Luca Boncagni, Paolo Buratti, Fabio Crescenzi, Ocleto D’Arcangelo, Giuseppe Galatola Teka, Edmondo Giovannozzi, Andrea Luigi Grosso, Matteo Iafrati, Alessandro Lampasi, Violeta Lazic, Simone Magagnino, Valerio Piergotti, Mario Pillon, Selanna Roccella, Giuliano Rocchi, Alessandro Sibio, Benedetto Tilia, Onofrio Tudisco, Alessandro Mancusoretired , Vincenzo Zanzaretired FSN Department, CR-ENEA Frascati and CREATE Consortium Giuseppe Maffia, Brunello Tirozzi, PlasmaTech Spin-off of Pisa University Francesco Giammanco, Paolo Marsili Pisa University Danilo Giulietti Nature Physics (2018) 1 Abstract The PROTO-SPHERA experiment, using DC helicity injection driven by a voltage applied between electrodes, has formed and sustained up to ½ sec magnetically confined current carrying tori in presence of a pre-existing axisymmetric configuration of magnetostatic poloidal field only and in absence of any doubly connected toroidal magnet. This result provides the first hints that future Fusion machines could be built with permanent magnets only. The relevance of a magnetic confinement machine built by axisymmetric permanent magnets only The use of permanent magnets in toroidal plasma confinement would be paramount for simplifying the design and the complexity of a Controlled Fusion rector based upon magnetic confinement. It would remove any direct dissipation connected with currents flowing inside the magnetic field coils and would even have great advantages with respect to superconducting coils, which share with permanent magnets the absence of ohmic dissipation but require a sophisticated cryogenic system; such a system entails a number of other thermal dissipations, in order to maintain the superconducting coils at the required low temperature conditions. -
A Brief History of the Co-Evolution of Supernova Theory with Neutrino Physics
A Brief History of the Co-evolution of Supernova Theory with Neutrino Physics Adam Burrows Department of Astrophysical Sciences, Princeton University, Princeton, NJ USA 08544 The histories of core-collapse supernova theory and of neutrino physics have paralleled one another for more than seventy years. Almost every development in neutrino physics necessi- tated modifications in supernova models. What has emerged is a complex and rich dynamical scenario for stellar death that is being progressively better tested by increasingly sophisiti- cated computer simulations. Though there is still much to learn about the agency and details of supernova explosions, whatever final theory emerges will have the neutrino at its core. I summarize in this brief contribution some of the salient developments in neutrino physics as they related to supernova theory, while avoiding any attempt to review the hundreds of pivotal papers that have pushed supernova theory forward. My goal has been merely to highlight the debt of supernova astrophysics to neutrino physics. 1 Introduction The theory of the violent deaths of massive stars in what are called supernova explosions has a long pedigree that spans more than half a century, has engaged hundreds of researchers, and has proven more elusive than anticipated. However, with the advent of numerically and physically sophisticated codes with which to simulate the onset of explosion in three spatial dimensions, the theoretical community now seems to be zeroing in on the mechanism of explosion. Central to this emerging theory are the neutrinos of all species produced copiously at the high densities and temperatures achieved during and after the collapse of the unstable Chandrasekhar core created in the center of the massive star at the end of its life. -
Colgate Paramp” • Talk Overview: – Introduction to the Colgate Paramp Story
A Meeting to Celebrate the 70th Birthday of Miller Goss Radio Astronomy & the ISM May 18-20th, 2011 Durango, Colorado The Colggpate Paramp & Its Impac t on Ra dio A st ronomy Bob Hayward Senior Engineer NRAO – Socorro, NM In Co llab orati on with The Man of th e Hour Himself Miller Goss 1 Setting the Scene A Letter Printed in Science Magazine , Jan 1972 2 One of the over 2000 MAR Western Electric Preamplifiers (dl(Model GF-40096) which came to be known as the “Colgate Paramp” • Talk Overview: – Introduction to the Colgate Paramp story. – Where did the ~2000 paramps come from? – What was Stirling Colgate’s interest in them? – Where did the 280 paramps go and what were they used for? – What happened to the rest of the paramps? – AkAcknow ldledgemen ts: • Doyle Piland (WSMR Archivist) • Bruce Blevins, Steve Hunyady & Joe Martinec (former NMT students) • Paul Krehbiel, John Reiche & Bill Winn (NMT) • Vestal Fulp & Bob Gamboa (former MAR-I employees) • Stirling Colgate (LANL & NMT) 3 Nike-X Prototype Multifunction Array Radar (MAR-I) The large dome was Hanger Runway 120 ft in diameter & 45 ft high. Most of the 195 x 155 ft structure is underground and extends 42 ft below the surface. It had 2 floors Test Aircraft Radar underground and 2 floors in each of Instrumentation Radar the domes. It had a total interior floor space of R-2 Rx Array (Blank) 90,000 sq ft. T-1 Tx Dome & Array Western Electric T-2 Tx Dome (Blank) (WECo) was the R-1 Rx Array primary contractor while Bell Labs was responsible for the overall design . -
Frontiers in High Energy Density Physics
FRONTIERS IN High Energy Density THE X-GAMES OF Physics CONTEMPORARY SCIENCE Committee on High Energy Density Plasma Physics Plasma Science Committee Board on Physics and Astronomy Division on Engineering and Physical Sciences THE NATIONAL ACADEMIES PRESS Washington, D.C. www.nap.edu THE NATIONAL ACADEMIES PRESS 500 Fifth Street, N.W. Washington, DC 20001 NOTICE: The project that is the subject of this report was approved by the Governing Board of the National Research Council, whose members are drawn from the councils of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. The members of the committee responsible for the report were chosen for their special competences and with regard for appropriate balance. This project was supported by the Department of Energy under Award No. DE-FG20- 00ER54612. Any opinions, findings, conclusions, or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the sponsors. Front Cover: Background image: Hubble Space Telescope image of the Cygnus Loop—the shock wave from a 20,000-year-old supernova in the constellation of Cygnus. Courtesy of NASA. Inset images: the Z-Machine, courtesy of Sandia National Laboratories; the OMEGA laser, courtesy of the Laboratory for Laser Energetics, University of Rochester; and results from the first gold-on-gold collision experiments at the Relativisitic Heavy Ion Collider, courtesy of Brookhaven National Laboratory. Back Cover: The target chamber at the National Ignition Facility, courtesy of Lawrence Livermore National Laboratory; and three-dimensional PIC simulation of a plasma wakefield accelerator, courtesy of R. -
Meren´I Magnetických Pol´I Na Základe Deflexe Rychlých Iont˚U V Z
Cesk´evysok´euˇcen´ıtechnick´evˇ Praze Fakulta jadern´aa fyzik´alnˇeinˇzen´yrsk´a Katedra fyziky Obor: Fyzik´aln´ıinˇzen´yrstv´ı Zamˇeˇren´ı:Fyzika a technika termojadern´ef´uze Mˇeˇren´ımagnetick´ych pol´ına z´akladˇedeflexe rychl´ych iont˚uv z-pinˇc´ıch Measurement of magnetic fields on the basis of fast ion deflectometry in z-pinches V´yzkumn´y´ukol Vypracoval: Bc. Vojtˇech Munzar Vedouc´ıpr´ace: doc. Ing. Daniel Kl´ırPh.D. Rok: 2015 Pˇredsv´az´an´ımm´ıstot´ehlestr´anky vloˇz´ıtezad´an´ıpr´ace s podpisem dˇekana (bude to jedin´yoboustrann´ylist ve Vaˇs´ıpr´aci)!!!! Prohl´aˇsen´ı Prohlaˇsuji,ˇzejsem tuto pr´aci vypracoval samostatnˇea pouˇziljsem pouze podklady uveden´ev pˇriloˇzen´emseznamu. Nem´amz´avaˇzn´yd˚uvod proti uˇzit´ıtohoto d´ılave smyslu §60 z´akona ˇc.121/200Sb.o pr´avuautorsk´em,o pr´avech souvisej´ıc´ıch s pr´avem autorsk´yma o zmˇenˇenˇekter´ych z´akon˚u(autorsk´yz´akon). ........................................ V Praze dne .................... Bc. Vojtˇech Munzar Podˇekov´an´ı Pˇredevˇs´ımbych chtˇelpodˇekovat m´emu vedouc´ımu doc. Ing. Danielu Kl´ırovi, Ph.D. a Ing. Jakubu Urbanovi, Ph.D. a Ing. Karlu Rez´aˇcovi,Ph.D.ˇ za cenn´ekonzultace. Bc. Vojtˇech Munzar N´azevpr´ace: Mˇeˇren´ımagnetick´ych pol´ına z´akladˇedeflexe rychl´ych iont˚uv z-pinˇc´ıch Autor: Bc. Vojtˇech Munzar Obor: Fyzik´aln´ıinˇzen´yrstv´ı Druh pr´ace: V´yzkumn´y´ukol Vedouc´ıpr´ace: doc. Ing. Daniel Kl´ırPh.D. FEL CVUTˇ Abstrakt: T´ematemt´etopr´aceje protonov´adeflektometrie pro mˇeˇren´ırychle se mˇen´ıc´ıch elektrick´ych a magnetick´ych pol´ıv Z-pinˇc´ıch.