Table Top Plasma Experiments

Slides:



Advertisements
Similar presentations
H-mode characterization for dominant ECR heating and comparison to dominant NBI or ICR heating F. Sommer PhD thesis advisor: Dr. Jörg Stober Academic advisor:
Advertisements

Plasma Window Options and Opportunities for Inertial Fusion Applications Leslie Bromberg Ady Herskovitch* MIT Plasma Science and Fusion Center ARIES meeting.
A. Samarian, W. Tsang, J. Khachan, B. James Complex Plasma Laboratory School of Physics, University of Sydney, NSW 2006, Australia.
NASSP Self-study Review 0f Electrodynamics
Particle’s Dynamics in Dusty Plasma with Gradients of Dust Charges
Ion-Induced Instability of Diocotron Modes In Magnetized Electron Columns Andrey Kabantsev University of California at San Diego Physics Department Nonneutral.
Numerical investigations of a cylindrical Hall thruster K. Matyash, R. Schneider, O. Kalentev Greifswald University, Greifswald, D-17487, Germany Y. Raitses,
An electromagnetic wave with a peak magnetic field magnitude of 1
TEST GRAINS AS A NOVEL DIAGNOSTIC TOOL B.W. James, A.A. Samarian and W. Tsang School of Physics, University of Sydney NSW 2006, Australia
Cairo University Electrical Engineering – Faculty of Engineering Cyclotrons Yasser Nour El-Din Mohammed Group 2 - Accelerators and Applications Supervisors.
Max P. Katz, Wayne G. Roberge, & Glenn E. Ciolek Rensselaer Polytechnic Institute Department of Physics, Applied Physics and Astronomy.
EE 403 (or 503) Introduction to plasma Processing Fall 2011 Title of the project Your name.
Computational Modeling Capabilities for Neutral Gas Injection Wayne Scales and Joseph Wang Virginia Tech Center for Space Science and Engineering.
Simulations of Neutralized Drift Compression D. R. Welch, D. V. Rose Mission Research Corporation Albuquerque, NM S. S. Yu Lawrence Berkeley National.
THE WAFER- FOCUS RING GAP*
WAFER EDGE EFFECTS CONSIDERING ION INERTIA IN CAPACITIVELY COUPLED DISCHARGES* Natalia Yu. Babaeva and Mark J. Kushner Iowa State University Department.
STREAMER DYNAMICS IN A MEDIA CONTAINING DUST PARTICLES* Natalia Yu. Babaeva and Mark J. Kushner Iowa State University Department of Electrical and Computer.
Physics 1502: Lecture 6 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, solutions.
Plasma Kinetics around a Dust Grain in an Ion Flow N F Cramer and S V Vladimirov, School of Physics, University of Sydney, S A Maiorov, General Physics.
Remote Plasma Sputtering: Recent Developments in Understanding the Process S. Thornley, P. Hockley, M. Thwaites, J. Dutson Dr James Dutson Senior Development.
Physics of fusion power Lecture 7: particle motion.
Physics of Fusion power Lecture4 : Quasi-neutrality Force on the plasma.
Electricity, Electronics And Ham Radio “Kopertroniks” By Nick Guydosh 4/12/07.
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
Chapter 7 Electrodynamics
Electron interactions with CO 2 Bob Merlino Department of Physics and Astronomy The University of Iowa Iowa City, IA U. S. Department of Energy National.
1 ST workshop 2005 Numerical modeling and experimental study of ICR heating in the spherical tokamak Globus-M O.N.Shcherbinin, F.V.Chernyshev, V.V.Dyachenko,
Wave induced supersonic rotation in mirrors Abraham Fetterman and Nathaniel Fisch Princeton University.
1 Magnetism.. 2 Magnetic Fields  Magnetic fields are historically described in terms of their effect on electric charges. A moving electric charge, such.
Electromagnetically Trapped Dusty Plasma Ring R. Sheldon, E. Thomas Jr, D. Gallagher, M. Adrian, M. Abbas, P. Craven & E. Reynolds Wheaton College / National.
Excitation of ion temperature gradient and trapped electron modes in HL-2A tokamak The 3 th Annual Workshop on Fusion Simulation and Theory, Hefei, March.
Initial Exploration of HHFW Current Drive on NSTX J. Hosea, M. Bell, S. Bernabei, S. Kaye, B. LeBlanc, J. Menard, M. Ono C.K. Phillips, A. Rosenberg, J.R.
Yiting Zhangb, Mark Denninga, Randall S. Urdahla and Mark J. Kushnerb
Physics of fusion power Lecture 3: Lawson criterion / Approaches to fusion.
Dusty Plasmas in the Laboratory and Space Bob Merlino April 2003 APS Meeting Philadelphia, PA.
Complex Plasmas as a Model for the Quark-Gluon-Plasma Liquid
Ion Energy Distributions from a Permanent-Magnet Helicon Thruster Francis F. Chen, UCLA Low Temperature Plasma Physics Webinar, January 17, 2014.
RF simulation at ASIPP Bojiang DING Institute of Plasma Physics, Chinese Academy of Sciences Workshop on ITER Simulation, Beijing, May 15-19, 2006 ASIPP.
1 Non-neutral Plasma Shock HU Xiwei (胡希伟) 工 HU Xiwei (胡希伟) HE Yong (何勇) HE Yong (何勇) Hu Yemin (胡业民) Hu Yemin (胡业民) Huazhong University of Science and.
Electromagnetic Waves and Their Propagation Through the Atmosphere
Waves in a 2D Dusty Plasma Crystal
STUDIES OF NONLINEAR RESISTIVE AND EXTENDED MHD IN ADVANCED TOKAMAKS USING THE NIMROD CODE D. D. Schnack*, T. A. Gianakon**, S. E. Kruger*, and A. Tarditi*
Laboratory Study of Spiky Potential Structures Associated with Multi- Harmonic EIC Waves Robert L. Merlino and Su-Hyun Kim University of Iowa Guru Ganguli.
Book Reference : Pages To understand that the path of a charged particle in a magnetic field is circular 2.To equate the force due to the magnetic.
IPM EM Simulations 9 th DITANET Topical Workshop on Non-Invasive Beam Size Measurement for High Brightness Proton and Heavy Ion Accelerators April.
Fusion Technology Institute 4/5/2002HAPL1 Ion Driven Fireballs: Calculations and Experiments R.R. Peterson, G.A. Moses, and J.F. Santarius University of.
6E5  Dispersion relation of dust acoustic waves in a DC glow discharge plasma Bob Merlino, Ross Fisher, Univ. Iowa Ed Thomas, Jr. Auburn Univ. Work supported.
Alex Samarian Complex Plasma Laboratory School of Physics, University of Sydney, NSW 2006, Australia
Mach Cones in a 2D Dusty Plasma Crystal J. Goree Dept. of Physics and Astronomy, University of Iowa with results from V. Nosenko, Z. Ma, and D. Dubin Supported.
An Estimation of Critical Electron Density at Just Starting Breakdown in Gases Mase. H Professor Emeritus of Ibaraki University.
1 Observations of Linear and Nonlinear Dust Acoustic Waves* Bob Merlino, Jon Heinrich Su Hyun Kim and John Meyer Department of Physics and Astronomy The.
Copyright © by Holt, Rinehart and Winston. All rights reserved. ResourcesChapter menu Chapter 18 Electric Energy and Current Chapter 18.
1 Current State of Omegatron Analyzer in the HT-7 Tokamak HT-7 ASIPP Ling Bi-li a),Wang En-yao b),Gao wei a),Wan Bao-nian a),Li Jian-gang a) a) Institute.
Plan V. Rozhansky, E. Kaveeva St.Petersburg State Polytechnical University, , Polytechnicheskaya 29, St.Petersburg, Russia Poloidal and Toroidal.
WIDEROE ACCELERATOR CONCEPT (IN A BOTTLE) Stephen, Leon, Daichi, Stefan Presented by:
WIRELESS CHARGING Presented by: K.MAHESH (08T81A1236)
A Global Hybrid Simulation Study of the Solar Wind Interaction with the Moon David Schriver ESS 265 – June 2, 2005.
DC Sputtering Disadvantage #1 Low secondary electron yield
Multitube Helicon Source with Permanent Magnets
Participation IAP NAS of Ukraine in understanding of vacuum breakdown phenomena Iaroslava Profatilova, V.Baturin, O. Karpenko.
Electron Beam Welding Welding Technology/4.3 Electron Beam Welding.
SUPPRESSING NONLINEARLY-DRIVEN INHOMOGENEITIES IN HIGH FREQUENCY CCP’s
Atmosphere.
Section 1 Electric Potential
Strathclyde University, 3-8 September 2000
Influence of energetic ions on neoclassical tearing modes
DOE Plasma Science Center Control of Plasma Kinetics
1.6 Glow Discharges and Plasma
BOLTZMANN-FOKKER-PLANCK KINETIC SOLVER
Shukui Zhang, Matt Poelker, Marcy Stutzman
Presentation transcript:

Table Top Plasma Experiments LANL Critical Skills Program John Kline July 10, 2002 P-24 Plasma Physics

Outline Why build small experiments? Different Table Top Experiments Double Plasma Device Waves and Instabilities Non-Neutral Plasmas Malmburg Penning Traps RF Plasma Capacitively Coupled Inductively Coupled Helicon Plasmas Dusty Plasmas Planetary Rings Experiments Conclusions

Why build small plasma experiments? Needs: That is all you need. Costs: Every scientist knows that funding. Proof of Principle: A small experiment used to prove concepts before building full scale experiments can be limited.

Proof of Principle DIIID Tokamak in San Diego Operated by General Atomics

Proof of Principle These experiments study fusion directly These experiments study RF current drive at WVU

Proof of Principle Experiments The biggest draw back to small Proof of Principle experiments is scaling. Do the experiments scale up in size? Do the experiments scale up with the plasma parameters? DIIID Tokamak n ~ 1 x 1015 cm-3, Te ~ 5 keV, Ti ~ 15 keV WVU Tokamak n ~ 1 x 1013 cm-3, Te ~ 3-5 eV, Ti ~ 0.3- 1.0 eV

The Pickett’s Charge Plasma Device Double Plasma Device The Pickett’s Charge Plasma Device At Gettysburg College

Double Plasma Device Biasing Grid Antenna for launching waves Filament RF Power Supply Magnets

Double Plasma Device Plasma Parameters: Plasma Densities of n ~ 1 x 109 – 1 x 1010 cm-3 Electron Temperatures of Te ~ 1 – 3 eV Ion Temperatures of Ti ~ 0.2 – 0.3 eV Ar Fill Pressure of No ~ 1 x 10-5 – 5 x 10-4 Torr

Space Plasma Physics Plasma Physics: Chaos and Nonlinear Dynamics Potential Layers Waves and Instabilities Velocity Shear Driven Drift Waves Bo Velocity Gyro-orbit size Density Diamagnetic Current Radius

Non-Neutral Plasmas Most plasmas studied are quasi-neutral, i.e. ne ~Zni Small electric fields, perturbations, arise only at microscopic levels due to plasma waves. For Non-neutral plasmas, the plasma is made up of purely electrons or ions. This produces a net electric field in the plasma. Plasma parameters: Densities on the order of n ~ 1 x 106 – 1 x 109 cm-3 Temperatures of a few (1-2) eV Fill Pressures of < 1 x 10-6 Torr

Non-Neutral Plasmas Transport and Diffusion (neoclassical and classical) Vortex formation and Plasma Crystals Capturing of positrons and anti-protons Auto-resonance studies

Malmberg Penning Traps

Malmberg Penning Traps A) the outer cylindrical electrode, B) the inner cylindrical electrode, C) the grids, D) the annular collecting electrode and E) the filament.

Plasma Crystals

RF Plasma Discharge Radio Frequency plasma sources use high power AC sources to generate a plasma. There are three types of RF plasma sources: Capacitive, Inductive, and Helicon Research areas: Plasma Chemistry: For example control of N+, N2+, N, and N2; Break down of CH1 and CO2 Plasma Processing, both etching and deposition Waves and instabilities Textile processing Bacterial removal

RF Plasma Discharge Plasma Parameters: Typically operated at 13.56 MHz; Many different fill gases. Capacitive Density on order of n ~ 1 x 108 to 1 x 1010 cm-3 Electron Temperature Te ~ 3 eV Fill Pressure of No ~ 0.1 x 10-2 – 1.5 x 10-1 Torr Inductive Density on order of n ~ 1 x 109 to 1 x 1012 cm-3 Fill Pressure of No ~ 1 x 10-4 – 1 x 10-2 Torr (Atmospheric) Helicon Density on order of n ~ 1 x 1010 to 5 x 1013 cm-3 Electron Temperature Te ~ 3 - 5 eV Ion Temperature Ti ~ 0.05 – 1.0 eV

Capacitively Coupled Sources (GEC Reference Cell) Vacuum Chamber Matching Network RF Source Plasma Capacitor Plates

Inductively Coupled Sources Pyrex Chamber Matching Network RF Source Antenna Magnets (not required) Alternative Antenna

Inductively Coupled Sources

Inductively Coupled Sources

Helicon Sources Matching Network RF Source Antenna Magnets (required) Pyrex Chamber Matching Network RF Source Antenna Magnets (required)

Helicon Sources Magnetically enhanced RF Plasma source with driving frequency between the ion and electron cyclotron frequencies: ci <<  < < ce< pe. A helicon wave is “bounded” whistler, a right hand circularly polarized electromagnetic, wave. Wave propagation helps to enhance the density production. Developed in 1970 by Rod Boswell looking for left handed circularly polarized waves.

Helicon Sources

Dusty Plasma Experiments Because the presence of charged dust in plasma is relevant to environments ranging from industrial plasma process devices to the space plasma environment to the edges of fusion energy experiments, the study of dusty plasmas has recently become one of the fastest growing areas of plasma physics. A dusty plasma is created by adding small particles (~ 10 um) to a plasma. The dust particles become charged and change the plasma dynamics, as well as, create a dynamical system of their own.

Dusty Plasma Experiments Photomicrographs of a) glass microballoons and b) Minnesota Lunar Simulant (MLS-1), a simulated lunar soil. All samples were sieved to select a 53-63 micron grain size. The frames are approximately 200 microns square.

Planetary Rings Experiment

Planetary Rings Experiment A rotating magnet is used to generate a co-rotating electric field in the plasma. If a cloud of microparticles is suspended in the vicinity of the rotating magnet, the electric field can cause the cloud to become extended into a ring-like structure. Experiments will focus on studying the properties of driven and self-generated instabilities in the ring plane.

Saturn

Conclusions There are many interesting and scientifically significant plasma physics experiments that can be done on a table top. A well design and thought out experiment can be very productive. Other small plasma experiments: Glow discharge Arc discharge Hollow cathode Plasma gun Filament sources Atmospheric plasma jets: for welding, material sprays, and contamination cleanup

Cloud vs. Stream Velocities Comparison of particle speeds in the cloud and the stream. Particles in the stream have speeds, vst ~ 30 to 40 mm/s. Particles in the cloud have speeds up to vmax ~ 2 mm/s. Dust acoustic waves are also visible at the top of the cloud. (The stream velocity vectors are shown in 3/8th scale relative to the cloud velocity vectors.)