PLASMA DIAGNOSTICS Carlos Silva

Slides:



Advertisements
Similar presentations
Dynamo Effects in Laboratory Plasmas S.C. Prager University of Wisconsin October, 2003.
Advertisements

Ion Heating and Velocity Fluctuation Measurements in MST Sanjay Gangadhara, Darren Craig, David Ennis, Gennady Fiskel and the MST team University of Wisconsin-Madison.
Examples of ITER CODAC requirements for diagnostics
NUCP 2371 Radiation Measurements II
Status and activity on LIF-technique development in NFI. I.Moskalenko, N.Molodtsov, D.Shcheglov.
The Amazing Spectral Line Begin. Table of Contents A light review Introduction to spectral lines What spectral lines can tell us.
Physics of fusion power
The Bases x-ray related physics
Introduction to Astrophysics Lecture 4: Light as particles.
Lectures in Plasma Physics
Electromagnetic Radiation
Spectroscopy. Spectroscopy is complex - but it can be very useful in helping understand how an object like a Star or active galaxy is producing light,
Laser Anemometry P M V Subbarao Professor Mechanical Engineering Department Creation of A Picture of Complex Turbulent Flows…..
Lecture 6.1 Lecture 6.1 ADVANCED PLASMA DIAGNOSTICTECHNIQUES Fri 23 May 2008, 1 pm LT5 Presented by Dr Ian Falconer Room.
Auroral dynamics EISCAT Svalbard Radar: field-aligned beam  complicated spatial structure (
Sub-THz Component of Large Solar Flares Emily Ulanski December 9, 2008 Plasma Physics and Magnetohydrodynamics.
Physics of fusion power Lecture 11: Diagnostics / heating.
Simulations of Neutralized Drift Compression D. R. Welch, D. V. Rose Mission Research Corporation Albuquerque, NM S. S. Yu Lawrence Berkeley National.
ISP Astronomy Gary D. Westfall1Lecture 6 The Nature of Light Light and other forms of radiation carry information to us from distance astronomical.
Physics of fusion power Lecture 10 : Running a discharge / diagnostics.
European Joint PhD Programme, Lisboa, Diagnostics of Fusion Plasmas Spectroscopy Ralph Dux.
Outline (HIBP) diagnostics in the MST-RFP Relationship of equilibrium potential measurements with plasma parameters Simulation with a finite-sized beam.
Electromagnetic Radiation & Electricity RTEC 111.
Physics of fusion power Lecture 7: particle motion.
© 2010 Pearson Education, Inc. Light and Matter: Reading Messages from the Cosmos.
Introduction to Plasma- Surface Interactions G M McCracken Hefei, October 2007.
Chapter 5 Diffusion and resistivity
Chapter 3 Light and Matter
Nils P. Basse Plasma Science and Fusion Center Massachusetts Institute of Technology Cambridge, MA USA ABB seminar November 7th, 2005 Measurements.
1 ECE 480 Wireless Systems Lecture 3 Propagation and Modulation of RF Waves.
A Singular Value Decomposition Method For Inverting Line Integrated Electron Density Measurements in Magnetically Confined Plasma Christopher Carey, The.
The principle of SAMI and some results in MAST 1. Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, Anhui, , China 2. Culham Centre.
PROTO-SPHERA Diagnostics PROTO-SPHERA WORKSHOP Frascati March 18-19, 2002.
How do we detect photons? Kensuke Okada RIKEN BNL Research Center April 20,
Plasma diagnostics using spectroscopic techniques
Plasmas. The “Fourth State” of the Matter The matter in “ordinary” conditions presents itself in three fundamental states of aggregation: solid, liquid.
Tunable, resonant heterodyne interferometer for neutral hydrogen measurements in tokamak plasmas * J.J. Moschella, R.C. Hazelton, M.D. Keitz, and C.C.
1 Nature of Light Wave Properties Light is a self- propagating electro- magnetic wave –A time-varying electric field makes a magnetic field –A time-varying.
Fyzika tokamaků1: Úvod, opakování1 Tokamak Physics Jan Mlynář 5. Electromagnetic radiation from tokamaks Introduction, EM waves, cyclotron radiation, bremsstrahlung,
Introduction to Plasma- Surface Interactions Lecture 3 Atomic and Molecular Processes.
SPECTROSCOPIC CONCEPTS BY Dr.JAGADEESH. INTRODUCTION SPECTROSCOPY: Study of interaction of matter with electromagnetic radiationelectromagnetic radiation.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Hybrid MHD-Gyrokinetic Simulations for Fusion Reseach G. Vlad, S. Briguglio, G. Fogaccia Associazione EURATOM-ENEA, Frascati, (Rome) Italy Introduction.
1 Introduction to Atomic Spectroscopy Lecture 10.
Spectroscopy and Atomic Structure Ch 04.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 2 Light and Matter.
A. Vaivads, M. André, S. Buchert, N. Cornilleau-Wehrlin, A. Eriksson, A. Fazakerley, Y. Khotyaintsev, B. Lavraud, C. Mouikis, T. Phan, B. N. Rogers, J.-E.
-Plasma can be produced when a laser ionizes gas molecules in a medium -Normally, ordinary gases are transparent to electromagnetic radiation. Why then.
Chemistry XXI Unit 2 How do we determine structure? The central goal of this unit is to help you develop ways of thinking that can be used to predict the.
Lecture 8 Optical depth.
Laboratory photo-ionized plasma David Yanuka. Introduction  Photo-ionized plasmas are common in astrophysical environments  Typically near strong sources.
1.1 What’s electromagnetic radiation
D-Alpha Fast-Ion Diagnostic: Recent Results from DIII-D W.W. Heidbrink, UC Irvine D-Alpha Diagnostic: Yadong Luo, K. Burrell, + Ion Cyclotron Heating:
بسمه تعالی Fast Imaging of turbulent plasmas in the GyM device D.Iraji, D.Ricci, G.Granucci, S.Garavaglia, A.Cremona IFP-CNR-Milan 7 th Workshop on Fusion.
Chapter 9 Stellar Atmospheres. Specific Intensity, I I ( or I ) is a vector (units: W m -2 Hz -1 sterad -1 )
Lecture 3. INTRODUCTION TO PLASMA PHYSICS
Hard X-rays from Superthermal Electrons in the HSX Stellarator Preliminary Examination for Ali E. Abdou Student at the Department of Engineering Physics.
Chapter 1: The Nature of Analytical Chemistry
NIMROD Simulations of a DIII-D Plasma Disruption S. Kruger, D. Schnack (SAIC) April 27, 2004 Sherwood Fusion Theory Meeting, Missoula, MT.
A Global Hybrid Simulation Study of the Solar Wind Interaction with the Moon David Schriver ESS 265 – June 2, 2005.
© 2017 Pearson Education, Inc.
The Solar System Lesson2 Q & A
Electromagnetic Energy
Catalin Teodorescu, William Young, Richard Ellis, Adil Hassam
Really Basic Optics Instrument Sample Sample Prep Instrument Out put
Introduction to Atmospheric Science at Arecibo Observatory
Interactions of Electromagnetic Radiation
Status of Equatorial CXRS System Development
Stars and Galaxies Lesson2 Q & A
Origin of Universe - Big Bang
Presentation transcript:

PLASMA DIAGNOSTICS Carlos Silva

Basic concepts The physical quantities are measured with instruments. The instrument should measure always the same value if they were perfectly accurate. In reality the instruments are not perfectly accurate, so the measure differs from the real value of the physical quantity . Measurement is the activity of comparing a number with a predefined pattern, involving the existence of measurement units. These units are essentially arbitrary; i.e. create and agree to use them. The basic units are the simple measurements of time, length, mass, temperature , amount of substance, electric current and light intensity. The derived units are comprised of basic units, e.g., velocity (m/s) or density (kg/m3) . By measuring is possible to express numerically qualities (quantify ) avoiding concepts like " big / small " , " strong / weak "

Diagnostics Plasma diagnostics are methods, techniques whose purpose is to deduce information about the plasma from practical observations of physical processes and their effects In general we do not have access to the physical quantity and we need to use models, theories, simulations to interpret the results. Main quantities of interest: Magnetic (Current, Flux loop, B-fields, magnetic configuration) Kinetic (Electron and ion temperature and density, pressure) Plasma composition (impurities, wall interaction)

What to measure Density of particles Temperature Potential, electric field, velocities, … Energy: joule (J) but often we use 1 eV = 1.6  10-19 J (energy gain by an electron in a potential difference of 1 volt) Temperature: kelvin (K) but often we use the equivalent in eV/k (Boltzmann constant) 1 eV/k = 1.6  10-19 J / 1.38  10-23 J/K = 11600 K 1 eV  11600 K

Diagnostic characteristics Ideal diagnostics should provide measurement of plasma quantities Direct and independent With good spatial and time resolution. With no perturbations (by the plasma and to the plasma) Real plasma diagnostics are Often indirect (need interpretation models as there is no direct access the physical quantity). The understanding of the associated physics process is required to interpret the results Often mutually dependent (need other plasma parameters) Spatial and time resolution dependent of the measurement technique Plasma perturbation and environment noise is an issue.

Complementarity of diagnostics Different techniques: Except for a few quantities each plasma parameter in general can be measured by more than one technique, often with different spatial and time resolution or with the use of different interpretation models. Compatibility of different measurements: Different diagnostics may give different values for the same parameter. Compatibility is related to the validity of the interpretation models and to the correct determination of measurement errors. Complementarity: The diagnostics operating in a plasma experimental must be seen as set of complementary techniques that operate all together to provide a reliable picture of the plasma.

Diagnostic characteristics Local measurements (electrical probes): can only be used in cold plasma. Remote measurements are required for hot plasmas. Some plasma parameters are difficult to measure (plasma characterization limited) There is a large variety of plasma diagnostics (hot and cold). The choice of the appropriated diagnostic toll depends on the plasma condition and budget. Required temporal and spatial resolution depends on the plasma parameters (ex. gradients)

Temporal / spatial resolution

Complexity of diagnostics Noisy environment poses strict requirements: electric and magnetic shielding. Careful signal grounding. Optical insulation in signal transmission sometimes necessary Accessibility: Limited accessibility to diagnostic equipment in large fusion machines Reliability: Long term survival of plasma facing components, damage by irradiation High degree of automatization of control/monitoring of diagnostic equipment and of data acquisition. Consequence: High complexity and high cost of diagnostic systems.

Accuracy vs Precision Real value may not be known Definition The degree of closeness to true value. The degree to which an instrument will repeat the same value. Measurements: Single Multiple measurements are needed Real value may not be known Do not mix up lack of precision with plasma fluctuations High accuracy Low precision High accuracy High precision Low accuracy Low precision

Scales: space In large fusion experiments the spatial scales vary by 6 orders of magnitude Debye length (< mm) Electron Larmor radius (< mm) Ion Larmor radius (mm) Turbulence scale (cm) Scale of the magnetic perturbations (cm) Gradients (cm – dimension of the experiment, m) Length along the magnetic field line (10-100 m)

Scales: time In large fusion experiments the temporal scales vary by 12 orders of magnitude Magnetic activity (0 – 1 MHz) Particles exchange with the wall (< Hz) Current diffusion (kHz -Hz) Magnetic equilibria, confinement ( kHz -Hz) Turbulence (1-200 kHz) Ion cyclotron frequency (> 10 MHz) Electron cyclotron frequency (10 GHz)

Diagnostic classification Plasma perturbation None: Spectroscopy, Magnetic probes Weak: Micro-waves, Lasers, particle beams Strong: Electric probes, particle beams Nature Electromagnetic: Electric and Magnetic probes Optics: Spectroscopy (visible, X-ray, ...), Interferometer Particles: Ion beams

Plasma Diagnostic Systems

Selected low temperature plasma diagnostics Diagnostic Measures Langmuir probes Plasma potential, electron temperature & density Magnetic diagnostics Plasma current, plasma waves, …. Spectroscopic Plasma composition, ion temperature & drift velocity, ……. Microwave diagnostics Plasma electron density, density profile, ….. Mass / energy analyser Identify species of ions, and measures their charge state and energy Laser diagnostics Density of various species in the plasma

Selected ITER diagnostics Diagnostic Measures Magnetic diagnostics Plasma current, position, shape, waves .. Spectroscopic & neutral Ion temperature, He & impurity particle analyser systems density, .......... Neutron diagnostics Fusion power, ion temperature profile, …. Microwave diagnostics Plasma position, shape, electron density, profile, ….. Optical/IR(infra-red) systems Electron density (Line-average & profile, electron temperature profile, …. Bolometric diagnostics Total radiated power, …. Plasma-facing components & Temperature of, and particle flux operational diagnostics to First Wall, ….. Neutral beam diagnostics Various parameters

Diagnostics overview

Lectures on: Electrical probes (Carlos Silva) Magnetic probes (Bernardo Carvalho) Particle beams (Artur Malaquias) Spectroscopy (Elena Tatarova) Reflectometry (M.E. Manso, MT5)

Electrical probes Conductor inserted into the plasma Simplest diagnostic Data interpretation complicated as probes perturb the plasma Limited to the plasma region were the probes can survive or do not perturb plasma Allows the determination of a large variety of plasma parameters (some of them only possible with probes) Potential and particle flux depends on plasma parameters

Langmuir probes I – V characteristic

Magnetic measurements Essential in magnetic confinement devices Plasma current, position, geometry, instabilities Sensor fluxo magnético Signal in the sensor Signal has to be integrated (hardware or software)

Magnetic measurements

Magnetic probes on ISTTOK

Magnetic probes

Particle beams Ions: Heavy elements (Xenon): Require large mass elements and low magnetic field. Larmor radius has the dimension of the device: The aim is to collect the ions after crossing the plasma. Information from the plasma parameters at the ionization location Neutral: Light elements (Lithium): The aim is to measure the ionization radiation. Neutral elements so not limited by B.

Heavy ion beam Larmor radius has the dimension of the device: the aim is to collect the ions after crossing the plasma. Information from the plasma parameters at the ionization location

Lithium beams Light elements (Lithium): The aim is to measure the ionization radiation. Neutral elements so not limited by B.

Plasma radiation Plasma radiation contains important information about the plasma properties. Plasma emits electromagnetic radiation due to different physics processes Complex spectra (continuum + spectral lines) from IR to X-ray

Plasma radiation Bremsstrahlung: Due to electron desacelaration in the ion field, used to measured the electron temperature Cyclotronic radiation: Due to rotation in the magnetic field ce  B  1/R (50 – 500 GHz)

Plasma radiation Spectral lines: Discrete radiation due to electron transition between energy atomic levels From visible to X-ray Broadening  Ti, Doppler shift  velocity Intensity = f(ni, n0, Te) Only high-Z elements emit X-rays ( keV, E ~ 13.6Z2 eV). Spectra: mix of continuum and lines Hot plasmas: Dominated by Bremsstrahlung (10 kev, Z~1) Low temperature plasmas: Spectral lines dominate (1 – 10 eV, Z > 1)

Spectral lines

Bolometer

Infra-red cameras

Infra-red cameras

Fast visible cameras Advantages: Large temporal and spatial resolution, plug-and-play Disadvantages: Expansive (100 k €), measurement not local (different average field lines, inversion necessary), difficult to extract plasma parameters Example: Photon ultima APX-RS 3,000 fps (1024 x 1024), 250,000 fps (64 x 64)

Fast visible cameras

Fast visible cameras Difficult to extract physical quantities. Possible to determine the speed, size and origin of the plasma structure (need the mapping of the field lines)

ISTTOK Database Support for Matlab (Octave), IDL, Matematica http://baco.ipfn.ist.utl.pt/jws/DataViewer.jnlp http://metis.ipfn.ist.utl.pt/CODAC/SDAS/Access http://metis.ipfn.ist.utl.pt/CODAC/SDAS/Codes