General Plasma Physics I Notes AST 551

Total Page:16

File Type:pdf, Size:1020Kb

General Plasma Physics I Notes AST 551 General Plasma Physics I Notes AST 551 Nick McGreivy Princeton University Fall 2017 1 Contents 0 Introduction5 1 Basics7 1.1 Finals words before the onslaught of equations . .8 1.1.1 Logical framework of Plasma Physics . .9 1.2 Plasma Oscillations . 10 1.3 Debye Shielding . 13 1.4 Collisions in Plasmas . 17 1.5 Plasma Length and Time Scales . 21 2 Single Particle Motion 24 2.1 Guiding Center Drifts . 24 2.1.1 E Cross B Drift . 25 2.1.2 Grad-B drift . 29 2.1.3 Curvature Drift . 31 2.1.4 Polarization Drift . 35 2.1.5 Magnetization Drift and Magnetization Current . 37 2.1.6 Drift Currents . 38 2.2 Adiabatic Invariants . 40 2.2.1 First Adiabatic Invariant µ ................. 44 2.2.2 Second Adiabatic Invariant J ................ 46 2.3 Mirror Machine . 46 2.4 Isorotation Theorem . 48 2.4.1 Magnetic Surfaces . 49 2.4.2 Proof of Iso-rotation Theorem . 50 3 Kinetic Theory 54 3.1 Klimantovich Equation . 57 3.2 Vlasov Equation . 60 3.2.1 Some facts about f . 62 3.2.2 Properties of Collisionless Vlasov-Maxwell Equations . 63 3.2.3 Entropy of a distribution function . 64 3.3 Collisions in the Vlasov Description . 66 3.3.1 Heuristic Estimate of Collision Operator . 66 3.3.2 Strongly and Weakly Coupled Plasmas . 67 3.3.3 Properties of Collision Operator . 68 3.3.4 Examples of Collision Operators . 69 3.4 Lorentz Collision Operator . 70 3.4.1 Lorentz Conductivity . 72 4 Fluid and MHD Equations 74 4.1 Deriving Fluid Equations . 75 4.1.1 Continuity Equation . 77 4.1.2 Momentum Equation . 78 2 4.1.3 Energy Equation . 81 4.1.4 Closure of Fluid Equations . 85 4.1.5 Summary of Assumptions Made in Fluid Model . 89 4.2 Deriving MHD Equations . 91 4.2.1 Asymptotic Assumptions in MHD . 91 4.2.2 MHD Continuity Equation . 92 4.2.3 MHD Momentum Equation . 92 4.2.4 MHD Ohm's Law . 93 4.2.5 MHD Energy Equation . 94 4.2.6 Information Content of the MHD Equations . 96 4.2.7 Summary of Assumptions Made in MHD . 97 4.3 Deriving Ideal MHD . 98 4.3.1 High Collisionality . 99 4.3.2 Small Gyroradius . 101 4.3.3 Low Resistivity . 101 4.3.4 Ideal MHD Momentum Equation . 102 4.3.5 Ideal MHD Ohm's Law . 103 4.3.6 Ideal MHD Energy Equation . 103 4.3.7 Summary of Assumptions Made in Ideal MHD . 106 4.3.8 The Electric Field in Ideal MHD . 107 4.4 MHD Equilibrium . 108 5 Waves in Plasmas 110 5.1 Kinetic Description of Waves . 111 5.1.1 Langmuir Wave . 115 5.1.2 Ion Acoustic Wave . 116 5.1.3 Isothermal Electrostatic Waves Don't Exist . 119 5.2 Plasma Waves in the Fluid Description . 119 5.2.1 Revisiting Plasma Oscillations . 119 5.2.2 Langmuir Waves and Ion Acoustic Waves with the Fluid Model . 123 5.2.3 Electromagnetic Plasma Waves . 128 5.3 MHD Waves . 131 5.3.1 Intermediate Wave . 134 5.3.2 Slow and Fast Waves . 137 5.4 Streaming Instability . 139 5.4.1 Electron-Positron Streaming Instability . 142 5.4.2 Electron-Ion Streaming Instability . 144 5.4.3 An Apparent Contradiction . 146 6 Landau Damping 148 6.1 Fundamentals of Complex Analysis . 148 6.1.1 Integrals of Analytic Functions in the Complex Plane . 148 6.1.2 Integrals of Non-Analytic Functions in the Complex Plane 150 6.1.3 Laplace Transforms . 151 6.1.4 Analytic Continuation . 154 3 6.2 Fourier Transform in Space, Laplace Transform in Time . 156 6.3 Landau Contours and All That Jazz . 159 4 0 Introduction These notes are intended to summarize and explain the topics discussed during class in the Fall 2017 section of AST551, General Plasma Physics I. I have written these notes primarily as a learning experience. I find that in order to learn something, I need to explain it to someone else. I also need to focus on the details of the subject, going through each step in detail. You will see that I try not to skip steps as much as possible. I've found that with many of the plasma physics books I've looked at, I understand the math and the derivations, but walk away without an understanding of the physics. My goal with these notes is for that not to be the case, both for me and for the reader. I have done my best to not only include the math, but to do my best to explain the physics behind the math, opting for wordiness over brevity. If I can't explain something simply, it's because I don't understand it well enough. Although my original intention was to cover only the topics covered in class, I ultimately decided that there are a few topics not covered in class which I would have liked to learn during GPP1. To a first-order approximation, however, these notes cover the topics from class. I've divided the notes into 6 chapters, not necessarily correlated with the order the topics were covered in class. The first chapter covers the most basic topics in plasma physics, including plasma oscillations, Debye shielding, space-time scales, and a bit on collisions. The second chapter covers single particle motion, including particle drifts, adiabatic invariants, mirror machines, and the iso-rotation theorem. The third chapter introduces kinetic theory, the Vlasov equation and discuss collision operators. The fourth chapter derives fluid equations, MHD, and ideal MHD. Chapter 5 covers some fundamental waves in plasmas, from kinetic, fluid, and MHD perspectives. Chapter 6 covers Landau damping, to the extent it was covered in class. So far, the best resource I have found for learning introductory plasma physics is Paul Bellan's book, Fundamentals of Plasma Physics. Every deriva- tion is done step-by-step in great detail, so that the reader is not lost, and each concept is explained thoroughly and usually with good physical insight. The downside of the book is that it is quite long.1 Everything Professor Bhatachar- jee does is exceptional,2 and his textbook Introduction to Plasma Physics with Space, Laboratory, and Astrophysical Applications is no exception. His book covers many of the same topics covered in these notes, plus many more. It would be a good reference book for this course, and less time and algebra in- tensive than Bellan. It's a great reference book for GPP2. Physics of Fully Ionized Plasmas by Lyman Spitzer is a really old, fairly short book, with an old-fashioned take to the fundamentals of plasmas. Sam Cohen once told me it's the only book I need to read to understand plasma physics. I don't believe him. 1After writing these notes summarizing the topics covered in class, I've realized that the first 5 chapters of Bellan's book are remarkably similar to the 6 chapters of these notes. What that suggests to me is that the topics covered in this course haven't changed all that much since fall of 1970 when Bellan, now a professor at Caltech, took the course. 2Except perhaps ping pong. 5 Introduction to Plasma Physics and Controlled Fusion by Francis Chen is often referenced as a good book for beginning students - however, I think the level is appropriate for an undergraduate starting a summer of research into plasma physics, not for a graduate student concentrating in plasma physics. These books have all been helpful for me in reviewing this material. However, I should give a big thanks to the professors for this course, Nat Fisch and Hong Qin, for not only teaching me this material but generously answering my questions as I've tried to figure this stuff out. Among the many things I know very little about, one is what one should do to prepare oneself to be a plasma physicist. However, I do know that the process of writing these notes has been enormously helpful to me in understanding this material. My hope is that these notes might also be useful for other students as they take AST551 or prepare for generals. These notes will be more useful if they do not contains errors or typos, so if you are reading these notes and find a typo or error, no matter how small, please let me know so I can fix it. You can reach me at [email protected]. Speaking of generals, I've attached a picture with the cover of the a previous written section of the generals exam. Of the 360 points in the written section of this generals exam, 50 of the points come directly from this course. Everything on the test, with the exception of the applied math section, builds upon or asks directly about the introductory material covered in this course. I think it's important we learn it, and learn it well. To put it another way - you can't learn how to dance unless you know how to move your hips. Let's boogie. 6 1 Basics It's unbelievable how much you don't know about the game you've been playing all your life. Mickey Mantle Greg Hammett imbued us first-year students with three pieces of wisdom during the first lecture for GPP1 way back in September. I figure I should pass that advice on. The first piece of advice is to remember how fortunate we are to be at this wonderful university, and to make the most of this experience.
Recommended publications
  • Chapter 4 SINGLE PARTICLE MOTIONS
    Chapter 4 SINGLE PARTICLE MOTIONS 4.1 Introduction We wish now to consider the effects of magnetic fields on plasma behaviour. Especially in high temperature plasma, where collisions are rare, it is important to study the single particle motions as governed by the Lorentz force in order to understand particle confinement. Unfortunately, only for the simplest geometries can exact solutions for the force equation be obtained. For example, in a constant and uniform magnetic field we find that a charged particle spirals in a helix about the line of force. This helix, however, defines a fundamental time unit – the cyclotron frequency ωc and a fundamental distance scale – the Larmor radius rL. For inhomogeneous and time varying fields whose length L and time ω scales are large compared with ωc and rL it is often possible to expand the orbit equations in rL/L and ω/ωc. In this “drift”, guiding centre or “adiabatic” approximation, the motion is decomposed into the local helical gyration together with an equation of motion for the instantaneous centre of this gyration (the guiding centre). It is found that certain adiabatic invariants of the motion greatly facilitate understanding of the motion in complex spatio-temporal fields. We commence this chapter with an analysis of particle motions in uniform and time-invariant fields. This is followed by an analysis of time-varying electric and magnetic fields and finally inhomogeneous fields. 4.2 Constant and Uniform Fields The equation of motion is the Lorentz equation dv F = m = q(E + v×B) (4.1) dt 88 4.2.1 Electric field only In this case the particle velocity increases linearly with time (i.e.
    [Show full text]
  • Plasma Oscillation in Semiconductor Superlattice Structure
    Memoirs of the Faculty of Engineering,Okayama University,Vol.23, No, I, November 1988 Plasma Oscillation in Semiconductor Superlattice Structure Hiroo Totsuji* and Makoto Takei* (Received September 30, 1988) Abstract The statistical properties of two-dimensional systems of charges in semiconductor superlattices are analyzed and the dispersion relation of the plasma oscillation is ealculated. The possibility to excite these oscillations by applying the electric field parallel to the structure is discussed. ]. Introduction The layered structure of semiconductors with thickness of the order of lO-6 cm or less is called semiconductor superlattice. The superlattice was first proposed by Esaki and Tsu [11 as a structure which has a Brillouin zone of reduced size and therefore allows to apply the negative mass part of the band structure to electronic devices through conduction of carriers perpendicular to the structure. The superlattice has been realized by subsequent developments of technologies such as molecular beam epitaxy (MBE) and metal-organic chemical vapor deposition (MOCVD) in fabricating controlled fine structures. At the same time, many interesting and useful physical phenomena related to the parallel conduction have also been revealed in addition to the parallel conduction. From the view point of application to devices, the enhancement of the carrier mobility due to separation of channels from Ionized impurities may be one of the most important progresses. Some high speed devices are based on this technique. The superlattlce structure
    [Show full text]
  • Particle Motion
    Physics of fusion power Lecture 5: particle motion Gyro motion The Lorentz force leads to a gyration of the particles around the magnetic field We will write the motion as The Lorentz force leads to a gyration of the charged particles Parallel and rapid gyro-motion around the field line Typical values For 10 keV and B = 5T. The Larmor radius of the Deuterium ions is around 4 mm for the electrons around 0.07 mm Note that the alpha particles have an energy of 3.5 MeV and consequently a Larmor radius of 5.4 cm Typical values of the cyclotron frequency are 80 MHz for Hydrogen and 130 GHz for the electrons Often the frequency is much larger than that of the physics processes of interest. One can average over time One can not however neglect the finite Larmor radius since it lead to specific effects (although it is small) Additional Force F Consider now a finite additional force F For the parallel motion this leads to a trivial acceleration Perpendicular motion: The equation above is a linear ordinary differential equation for the velocity. The gyro-motion is the homogeneous solution. The inhomogeneous solution Drift velocity Inhomogeneous solution Solution of the equation Physical picture of the drift The force accelerates the particle leading to a higher velocity The higher velocity however means a larger Larmor radius The circular orbit no longer closes on itself A drift results. Physics picture behind the drift velocity FxB Electric field Using the formula And the force due to the electric field One directly obtains the so-called ExB velocity Note this drift is independent of the charge as well as the mass of the particles Electric field that depends on time If the electric field depends on time, an additional drift appears Polarization drift.
    [Show full text]
  • 10. Collisions • Use Conservation of Momentum and Energy and The
    10. Collisions • Use conservation of momentum and energy and the center of mass to understand collisions between two objects. • During a collision, two or more objects exert a force on one another for a short time: -F(t) F(t) Before During After • It is not necessary for the objects to touch during a collision, e.g. an asteroid flied by the earth is considered a collision because its path is changed due to the gravitational attraction of the earth. One can still use conservation of momentum and energy to analyze the collision. Impulse: During a collision, the objects exert a force on one another. This force may be complicated and change with time. However, from Newton's 3rd Law, the two objects must exert an equal and opposite force on one another. F(t) t ti tf Dt From Newton'sr 2nd Law: dp r = F (t) dt r r dp = F (t)dt r r r r tf p f - pi = Dp = ò F (t)dt ti The change in the momentum is defined as the impulse of the collision. • Impulse is a vector quantity. Impulse-Linear Momentum Theorem: In a collision, the impulse on an object is equal to the change in momentum: r r J = Dp Conservation of Linear Momentum: In a system of two or more particles that are colliding, the forces that these objects exert on one another are internal forces. These internal forces cannot change the momentum of the system. Only an external force can change the momentum. The linear momentum of a closed isolated system is conserved during a collision of objects within the system.
    [Show full text]
  • Carbon Fiber Skeleton/Silver Nanowires Composites with Tunable Negative
    EPJ Appl. Metamat. 8, 1 (2021) © Y. An et al., published by EDP Sciences, 2021 https://doi.org/10.1051/epjam/2020019 Available online at: epjam.edp-open.org Metamaterial Research Updates from China RESEARCH ARTICLE Carbon fiber skeleton/silver nanowires composites with tunable negative permittivity behavior Yan An1, Jinyuan Qin1, Kai Sun1,*, Jiahong Tian1, Zhongyang Wang2,*, Yaman Zhao1, Xiaofeng Li1, and Runhua Fan1 1 College of Ocean Science and Engineering, Shanghai Maritime University, Shanghai 201306, PR China 2 State Key Lab of Metal Matrix Composites, School of Materials Science and Engineering, Shanghai Jiao Tong University, Shanghai 200240, PR China Received: 13 November 2020 / Accepted: 25 December 2020 Abstract. With the development of periodic metamaterials, more attention has been paid to negative permittivity behavior due to great potential applications. In this paper, silver nanowires (AgNWs) were introduced to the porous carbon fibers (CFS) by an impregnation process to prepare CFS/AgNWs composites with different content of AgNWs and the dielectric property was investigated. With the formation of conductive network, the Drude-like negative permittivity was observed in CFS/AgNWs composites. With the increase of AgNWs, the connectivity of conductive network became enhanced, the conductivity gradually increases, and the absolute value of the negative dielectric constant also increases to 8.9 Â 104, which was ascribed to the enhancement of electron density of the composite material. Further investigation revealed that the inductive characteristic was responsible for the negative permittivity. Keywords: Negative permittivity / metacomposites / plasma oscillation / inductive characteristic 1 Introduction capacitors [10,11]. The electromagnetic metamaterials have a great value in the fields of wireless communication In the past decades, electromagnetic metamaterials with [12], electromagnetic absorption [13] and shielding [14], etc.
    [Show full text]
  • Lecture 7: Moments of the Boltzmann Equation
    !"#$%&'()%"*#%*+,-./-*+01.2(.*3+456789* !"#$%&"'()'*+,"-$.'+/'0+1$2,3--4513.+6'78%39+-' Dr. Peter T. Gallagher Astrophysics Research Group Trinity College Dublin :2;$-$(01*%<*=,-./-*=0;"%/;"-* !"#$%#&!'()*%()#& +,)-"(./#012"(& 4,$50,671*)& 9*"5:%#))& 3*1*)& 87)21*)& ;<7#1*)& 3*%()5$&*=&9*"5:%#))& ;<7#1*)& +,)-"(&>7,?& 37"1/"(&& 3@4& >7,?$& >%/;"#.*%<*?%,#@/-""AB,-.%C*DE'-)%"* o Under certain assumptions not necessary to obtain actual distribution function if only interested in the macroscopic values. o Instead of solving Boltzmann or Vlasov equation for distribution function and integrating, can take integrals over collisional Boltzmann-Vlasov equation and solve for the quantities of interest. "f q "f & "f ) +v #$f + [E +(v % B)]# = ( + "t m "v ' "t *coll (7.1) o Called “taking the moments of the Boltzmann-Vlasov equation” . ! o Resulting equations known as the macroscopic transport equations, and form the foundation of plasma fluid theory. o Results in derivation of the equations of magnetohydrodynamics (MHD). F;$%#0A%$&;$*>%/;"#G*H%")"'2#1*DE'-)%"* o Lowest order moment obtained by integrating Eqn. 7.1: "f q "f ' "f * # dv + # v $%fdv + # [E +(v & B)]$ dv = # ) , dv "t m "v ( "t +coll The first term gives "f " "n o # dv = # fdv = (7.2) "t "t "t ! o Since v and r are independent, v is not effected by gradient operator: ! $ v " #fdv = # " $ vfdv o From before, the first order moment of distribution function is ! 1 u = " vf (r,v,t)dv n therefore, $ v " #fdv = # "(nu) (7.3) ! ! F;$%#0A%$&;$*>%/;"#G*H%")"'2#1*DE'-)%"* o For the third term, consider E and B separately. E term vanishes as #f # $ E " dv = $ "( fE)dv = $ fE "dS = 0 (7.4a) #v #v using Gauss’ Divergence Theorem in velocity space.
    [Show full text]
  • Free Electron Lasers and High-Energy Electron Cooling*
    FREE ELECTRON LASERS AND HIGH-ENERGY ELECTRON COOLING* Vladimir N. Litvinenko, BNL, Upton, Long Island, NY, USA# Yaroslav S. Derbenev, TJNAF, Newport News, VA, USA) Abstract The main figure of merit of any collider is its average Cooling intense high-energy hadron beams remains a luminosity, i.e., its average productivity for an appropriate major challenge in modern accelerator physics. branch of physics. Cooling hadron beams at top energy Synchrotron radiation of such beams is too feeble to may further this productivity. provide significant cooling: even in the Large Hadron For a round beam, typical for hadron colliders, the Collider (LHC) with 7 TeV protons, the longitudinal luminosity is given by a simple expression: ' * damping time is about thirteen hours. Decrements of N1N2 & s traditional electron cooling decrease rapidly as the high L = fc * % h) * , (1) 4"# $ ( # + power of beam energy, and an effective electron cooling of protons or antiprotons at energies above 100 GeV where N1, N2 are the number of particles per bunch, fc is seems unlikely. Traditional stochastic cooling still cannot their collision frequency, !* is the transverse !-function catch up with the challenge of cooling high-intensity at the collision point, " is the transverse emittance of the bunched proton beams - to be effective, its bandwidth b!ea m, #s is the bunch length, and h ! 1 is a coefficient must be increased by about two orders-of-magnitude. accounting for the so-called hourglass effect [1]: Two techniques offering the potential to cool high- " 1/ x 2 h(x) = e erfc(1/ x). energy hadron beams are optical stochastic cooling (OSC) x and coherent electron cooling (CEC) – the latter is the The hourglass effect is caused by variations in the beam’s 2 focus of this paper.
    [Show full text]
  • Law of Conversation of Energy
    Law of Conservation of Mass: "In any kind of physical or chemical process, mass is neither created nor destroyed - the mass before the process equals the mass after the process." - the total mass of the system does not change, the total mass of the products of a chemical reaction is always the same as the total mass of the original materials. "Physics for scientists and engineers," 4th edition, Vol.1, Raymond A. Serway, Saunders College Publishing, 1996. Ex. 1) When wood burns, mass seems to disappear because some of the products of reaction are gases; if the mass of the original wood is added to the mass of the oxygen that combined with it and if the mass of the resulting ash is added to the mass o the gaseous products, the two sums will turn out exactly equal. 2) Iron increases in weight on rusting because it combines with gases from the air, and the increase in weight is exactly equal to the weight of gas consumed. Out of thousands of reactions that have been tested with accurate chemical balances, no deviation from the law has ever been found. Law of Conversation of Energy: The total energy of a closed system is constant. Matter is neither created nor destroyed – total mass of reactants equals total mass of products You can calculate the change of temp by simply understanding that energy and the mass is conserved - it means that we added the two heat quantities together we can calculate the change of temperature by using the law or measure change of temp and show the conservation of energy E1 + E2 = E3 -> E(universe) = E(System) + E(Surroundings) M1 + M2 = M3 Is T1 + T2 = unknown (No, no law of conservation of temperature, so we have to use the concept of conservation of energy) Total amount of thermal energy in beaker of water in absolute terms as opposed to differential terms (reference point is 0 degrees Kelvin) Knowns: M1, M2, T1, T2 (Kelvin) When add the two together, want to know what T3 and M3 are going to be.
    [Show full text]
  • The Vlasov-Poisson System and the Boltzmann Equation
    DISCRETE AND CONTINUOUS Website: http://AIMsciences.org DYNAMICAL SYSTEMS Volume 8, Number 2, April 2002 pp. 361–380 AN INTRODUCTION TO KINETIC EQUATIONS: THE VLASOV-POISSON SYSTEM AND THE BOLTZMANN EQUATION JEAN DOLBEAULT Abstract. The purpose of kinetic equations is the description of dilute par- ticle gases at an intermediate scale between the microscopic scale and the hydrodynamical scale. By dilute gases, one has to understand a system with a large number of particles, for which a description of the position and of the velocity of each particle is irrelevant, but for which the decription cannot be reduced to the computation of an average velocity at any time t ∈ R and any d position x ∈ R : one wants to take into account more than one possible veloc- ity at each point, and the description has therefore to be done at the level of the phase space – at a statistical level – by a distribution function f(t, x, v) This course is intended to make an introductory review of the literature on kinetic equations. Only the most important ideas of the proofs will be given. The two main examples we shall use are the Vlasov-Poisson system and the Boltzmann equation in the whole space. 1. Introduction. 1.1. The distribution function. The main object of kinetic theory is the distri- bution function f(t, x, v) which is a nonnegative function depending on the time: t ∈ R, the position: x ∈ Rd, the velocity: v ∈ Rd or the impulsion ξ). A basic 1 d d requirement is that f(t, ., .) belongs to Lloc (R × R ) and from a physical point of view f(t, x, v) dxdv represents “the probability of finding particles in an element of volume dxdv, at time t, at the point (x, v) in the (one-particle) phase space”.
    [Show full text]
  • Microwave Power Coupling with Electron Cyclotron Resonance Plasma Using Langmuir Probe
    PRAMANA c Indian Academy of Sciences Vol. 81, No. 1 — journal of July 2013 physics pp. 157–167 Microwave power coupling with electron cyclotron resonance plasma using Langmuir probe SKJAIN∗, V K SENECHA, P A NAIK, P R HANNURKAR and S C JOSHI Raja Ramanna Centre for Advanced Technology, Indore 452 013, India ∗Corresponding author. E-mail: [email protected] MS received 14 April 2012; revised 16 January 2013; accepted 26 February 2013 Abstract. Electron cyclotron resonance (ECR) plasma was produced at 2.45 GHz using 200– 750 W microwave power. The plasma was produced from argon gas at a pressure of 2 × 10−4 mbar. Three water-cooled solenoid coils were used to satisfy the ECR resonant conditions inside the plasma chamber. The basic parameters of plasma, such as electron density, electron temperature, floating potential, and plasma potential, were evaluated using the current–voltage curve using a Langmuir probe. The effect of microwave power coupling to the plasma was studied by varying the microwave power. It was observed that the optimum coupling to the plasma was obtained for ∼ 600 W microwave power with an average electron density of ∼ 6 × 1011 cm−3 and average electron temperature of ∼ 9eV. Keywords. Electron cyclotron resonance plasma, Langmuir probe, electron density, electron temperature. PACS Nos 52.50.Dg; 52.70.–m; 52.50.Sw 1. Introduction The electron cyclotron resonance (ECR) plasma is an established source for delivering high current, high brightness, stable ion beam, with significantly higher lifetime of the source. Such a source has been widely used for producing singly and multiply charged ion beams of low to high Z elements [1–3], for research in materials sciences, atomic and molecular physics, and as an accelerator injector [4,5].
    [Show full text]
  • Plasma Diagnostics Lecture.Key
    LA3NET School | Salamanca, Spain | October 1st, 2014 Advanced diagnostics Plasma density profile measurements and synchronisation of lasers to accelerators J. Osterhoff and L. Schaper Deutsches Elektronen-Synchrotron DESY Outline > Importance of the plasma density profile > Measurement techniques > Interferometry > Absorption spectroscopy > Rayleigh scattering > Raman scattering > Laser induced fluorescence > Synchronisation of lasers to accelerators > Summary Jens Osterhoff | plasma.desy.de | LA3NET School, Salamanca | Oct 1, 2014 | Page 002 Access to novel in-plasma beam-generation techniques requires control over plasma profile in LWFA/PWFA > Density down-ramp injection J. Grebenyuk et al., NIM A 740, 246 (2014) IB & 1kA > Laser-induced ionization injection (Trojan Horse injection) B. Hidding et al., Physical Review Letters 108, 035001 (2012) IB & 5kA > Beam-induced ionization injection A. Martinez de la Ossa et al., NIM A 740, 231 (2014) IB & 7.5kA > Wakefield-induced ionization injection A. Martinez de la Ossa et al., Physical Review Letters 111, 245003 (2013) IB & 10 kA Jens Osterhoff | plasma.desy.de | LA3NET School, Salamanca | Oct 1, 2014 | Page 003 Access to novel in-plasma beam-generation techniques requires control over plasma profile in LWFA/PWFA > Density down-ramp injection J. Grebenyuk et al., NIM A 740, 246 (2014) n0 = 1.2 x 1018 cm-3 IB & 1kA > Laser-induced ionization injection (Trojan Horse injection) B. Hidding et al., Physical Review Letters 108, 035001 (2012) Driver: Eb = 1 GeV, Ib = 10 kA, Qb = 574 pC σz = 7 μm, σx,y = 4 μm, εx,y = 1 μm IB & 5kA injection > Beam-induced ionization injection A. Martinez de la Ossa et al., NIM A 740, 231 (2014) acceleration IB & 7.5kA > Wakefield-induced ionization injection A.
    [Show full text]
  • [Insert Your Title Here]
    Laboratory Investigation of the Dynamics of Shear Flows in a Plasma Boundary Layer by Ami Marie DuBois A dissertation submitted to the Graduate Faculty of Auburn University in partial fulfillment of the requirements for the Degree of Doctor of Philosophy Auburn, Alabama December 14, 2013 Copyright 2013 by Ami Marie DuBois Approved by Edward Thomas, Jr., Chair, Professor of Physics William Amatucci, Staff Scientist at Naval Research Laboratory Uwe Konopka, Professor of Physics David Maurer, Professor of Physics Abstract The laboratory experiments presented in this dissertation investigate a regime of instabilities that occur when a highly localized, radial electric field oriented perpendicular to a uniform background magnetic field gives rise to an azimuthal velocity shear profile at the boundary between two interpenetrating plasmas. This investigation is motivated by theoretical predictions which state that plasmas are unstable to transverse and parallel inhomogeneous sheared flows over a very broad frequency range. Shear driven instabilities are commonly observed in the near-Earth space environment when boundary layers, such as the magnetopause and the plasma sheet boundary layer, are compressed by intense solar storms. When the shear scale length is much less than the ion gyro- radius, but greater than the electron gyro-radius, the electrons are magnetized in the shear layer, but the ions are effectively un-magnetized. The resulting shear driven instability, the electron-ion hybrid instability, is investigated in a new interpenetrating plasma configuration in the Auburn Linear EXperiment for Instability Studied (ALEXIS) in the absence of a magnetic field aligned current. In order to truly understand the dynamics at magnetospheric boundary layers, the EIH instability is studied in the presence of a density gradient located at the boundary layer between two plasmas.
    [Show full text]