NEGATIVE ION PLASMAS Professor Robert L. Merlino Department of Physics & Astronomy University of Iowa Plasma Physics Seminar, April 23, 2007.

Slides:



Advertisements
Similar presentations
Anomalous Ion Heating Status and Research Plan
Advertisements

Physics of fusion power
Ion-Induced Instability of Diocotron Modes In Magnetized Electron Columns Andrey Kabantsev University of California at San Diego Physics Department Nonneutral.
Introduction to Plasma-Surface Interactions Lecture 6 Divertors.
1 Ionospheres of the Terrestrial Planets Stan Solomon High Altitude Observatory National Center for Atmospheric Research
Lectures in Plasma Physics
Session A Wrap Up. He Abundance J. Kasper Helium abundance variation over the solar cycle, latitude and with solar wind speed Slow solar wind appears.
Lecture 6 nitrogen and ozone photochemistry Regions of Light Absorption of Solar Radiation.
L.B. Begrambekov Plasma Physics Department, Moscow Engineering and Physics Institute, Moscow, Russia Peculiarities, Sources and Driving Forces of.
Fusion Physics - Energy Boon or Nuclear Gloom? David Schilter and Shivani Sharma.
POLYMERISATION PROCESSES IN LOW-PRESSURE FLUOROCARBON PLASMAS
EE 403 (or 503) Introduction to plasma Processing Fall 2011 Title of the project Your name.
Lecture 25 Practice problems Boltzmann Statistics, Maxwell speed distribution Fermi-Dirac distribution, Degenerate Fermi gas Bose-Einstein distribution,
The star we see but seldom notice
5. Simplified Transport Equations We want to derive two fundamental transport properties, diffusion and viscosity. Unable to handle the 13-moment system.
Surface and volume production of negative ions in a low-pressure plasma E. Stoffels, W.W. Stoffels, V.M. Kroutilina*, H.-E. Wagner* and J. Meichsner*,
METO 637 LESSON 3. Photochemical Change A quantum of radiative energy is called a photon, and is given the symbol h Hence in a chemical equation we.
Magnetosphere-Ionosphere Coupling through Plasma Turbulence at High- Latitude E-Region Electrojet Y. Dimant and M. Oppenheim Tuesday, April 13, 2010 Center.
Lecture 10 Energy production. Summary We have now established three important equations: Hydrostatic equilibrium: Mass conservation: Equation of state:
The Classification of Stellar Spectra
the Ionosphere as a Plasma
Salamanca.ppt, © Thomas Schwarz-Selinger, 03. Juni 2008 G. S. Oehrlein*, T. Schwarz-Selinger, K. Schmid, M. Schlüter and W. Jacob Interaction of Deuterium.
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.
The Sun Earth Science - Mr. Gallagher. The Sun is the Earth's nearest star. Similar to most typical stars, it is a large ball of hot electrically charged.
SCATTERING OF RADIATION Scattering depends completely on properties of incident radiation field, e.g intensity, frequency distribution (thermal emission.
Collisions and transport phenomena Collisions in partly and fully ionized plasmas Typical collision parameters Conductivity and transport coefficients.
AS 4002 Star Formation & Plasma Astrophysics Supercritical clouds Rapid contraction. Fragmentation into subregions –Also supercritical if size R ≥ clump.
The SUN.
Negative Ions in IEC Devices David R. Boris 2009 US-Japan IEC Workshop 12 th October, 2009 This work performed at The University of Wisconsin Fusion Technology.
Why plasma processing? (1) UCLA Accurate etching of fine features.
Hiden Analytical Excellence in plasma diagnostics An Introduction to the Hiden EQP Excellence in Plasma Diagnostics An Introduction to the Hiden EQP
Dusty Plasmas in the Laboratory and Space Bob Merlino April 2003 APS Meeting Philadelphia, PA.
Plasmas. The “Fourth State” of the Matter The matter in “ordinary” conditions presents itself in three fundamental states of aggregation: solid, liquid.
Atoms in stellar atmospheres are excited and ionized primarily by collisions between atoms/ions/electrons (along with a small contribution from the absorption.
M. Ichimura, Y. Yamaguchi, R. Ikezoe, Y. Imai, T. Murakami,
Introduction to Space Weather Jie Zhang CSI 662 / PHYS 660 Spring, 2012 Copyright © Ionosphere II: Radio Waves April 12, 2012.
Solar Properties Has more than 99% the mass of our solar system Has more than 99% the mass of our solar system Diameter: 1,390,000 km Diameter: 1,390,000.
CCFE is the fusion research arm of the United Kingdom Atomic Energy Authority Beam Species Measurements on the MAST NBI system Brendan Crowley Thanks to.
Physics of fusion power Lecture 12: Diagnostics / heating.
Energy “The energy of the mind is the essence of life” Aristotle. “If you want to find the secrets of the universe, think in terms of energy, frequency.
THE ATMOSPHERE (chapter 24.1)
-Plasma can be produced when a laser ionizes gas molecules in a medium -Normally, ordinary gases are transparent to electromagnetic radiation. Why then.
NEGATIVE ION PLASMAS Professor Robert L. Merlino Department of Physics & Astronomy University of Iowa Plasma Physics Seminar, April 23, 2007.
Laboratory Study of Spiky Potential Structures Associated with Multi- Harmonic EIC Waves Robert L. Merlino and Su-Hyun Kim University of Iowa Guru Ganguli.
Lecture 8 Optical depth.
ESS 200C Lecture 13 The Earth’s Ionosphere
Etching: Wet and Dry Physical or Chemical.
The Sun By: JGilliam The Sun’s CompositionIdentifying Stars Composition ▪ Hydrogen and Helium together make up 99% of the sun’s mass. ▪ 75% of the sun’s.
1 Charging of Dust in a Plasma with Negative Ions Su-Hyun Kim and Bob Merlino The University of Iowa Supported by DOE 11 th Workshop on the Physics of.
Özkan ŞAHİN & Tadeusz KOWALSKI Uludağ University, Physics Department, Bursa – TURKEY Faculty of Physics and Applied Computer Science, AGH University of.
An Estimation of Critical Electron Density at Just Starting Breakdown in Gases Mase. H Professor Emeritus of Ibaraki University.
Large Area Plasma Processing System (LAPPS) R. F. Fernsler, W. M. Manheimer, R. A. Meger, D. P. Murphy, D. Leonhardt, R. E. Pechacek, S. G. Walton and.
1 NSTX EXPERIMENTAL PROPOSAL - OP-XP-712 Title: HHFW Power Balance Optimization at High B Field J. Hosea, R. Bell, S. Bernabei, L. Delgado-Aparicio, S.
Many mass spectra are observed in addition to those of nitrogen (28amu) and benzene (78amu) molecules between 1 and 80amu, when the discharge is not generated.
Influence of pulse parameters and cathodic cage size on plasma nitriding DEPARTMENT OF PHYSICS QUAID-I-AZAM UNIVERSITY ISLAMABAD, PAKISTAN Prof.
Introduction to Plasma Physics and Plasma-based Acceleration
The Solar System Lesson2 Q & A
Seok-geun Lee, Young-hwa An, Y.S. Hwang
DOE Plasma Science Center Control of Plasma Kinetics
N. D’Angelo, B. Kustom, D. Susczynsky, S. Cartier, J. Willig
Lecture 25 Practice problems
Fusion vs Fission Fission Fusion Division of an atom’s nucleus
Presented by Jim Garver, K7YO for Ken Neubeck, WB2AMU
Stars and Galaxies Lesson2 Q & A
Atmosphere 11-1.
Earth’s Ionosphere Lecture 13
Ionosphere References: Prolss: Chap. 4, P (main)
1.6 Glow Discharges and Plasma
LECTURE II: ELEMENTARY PROCESSES IN IONIZED GASES
The Centre of the Solar System Earth Science 11
Presentation transcript:

NEGATIVE ION PLASMAS Professor Robert L. Merlino Department of Physics & Astronomy University of Iowa Plasma Physics Seminar, April 23, 2007

negative ion plasma a plasma containing electrons, positive ions and negative ions a fraction of the electrons are attached to negative ions characterized by the parameter p = n  / n + the % of negative ions in the plasma occur naturally in space and astrophysics and can be produced in the lab

OUTLINE I.Introduction A. the chemical physics of negative ion formation B. examples of negative ion plasmas (1)neutral beam sources (2)photosphere of the Sun (3)D region of the ionosphere (4)plasma processing reactors

II. Production of negative ion plasmas A.Q machine B.electron attachment cross sections C. Langmuir probe measurements D. comparison of SF 6 and C 7 F 14 results III. Waves in negative ion plasmas A.ion acoustic waves B. electrostatic ion cyclotron waves

The chemical physics of negative ions A) Negative ion formation mechanisms: ( molecule XYZ ) attachment autoionization radiative stabilization IVR dissociative attachment

B) Negative ion destruction mechanisms mutual neutralization photodetactment collisional detachment

The negative hydrogen ion H  one of the most important negative ions in the universe! It exists, electron affinity (binding energy of the extra electron) = 0.75 eV why does it exist? first electron in H only partially shields the nuclear charge QM calculations confirm this responsible for most of the continuum opacity of the photosphere

Negative ion sources for neutral beam systems magnetically confined fusion plasmas are heated by neutral beam injection (150 keV D + ) cannot accelerate neutral atoms accelerate H + then neutralize by charge exchange  inefficient at >100 keV however, with H -, the neutralization efficiency remains high out to 500 keV. now use negative-ion based neutral beam systems capable of producing multiampere beams of H and D negative ions

H  in the photosphere photosphere - what you see when you look at the sun about 400 km thick, cool ~ 4400K – 5800K, mostly H remarkably opaque at infrared and shorter wavelengths most H in ground state and thus does not contribute much to absorption need 13.6 eV (121.6 nm) to get H in first excited state about one in 10 7 H’s are H –, and need only 0.75 eV to remove extra electron  1653 nm (Saha relation) so H – can account for absorption down to very long wavelengths negative H makes photosphere as opaque as a dense object, therefore it radiates like a blackbody

negative ions in the earth’s ionosphere negative ions (O 2 –) are generally present in the lower ionosphere (D region) 60 – 90 km they may play a role in the creation and destruction of the ozone layer observed at 76 km in the polar region Data from rocket borne instruments

Effect of rocket exhaust on the ionospheric plasma artificially induced airglow caused by Challenger engine burn on 29 July 1985

electron depletion experiments in space electron density changes recorded on a Langmuir probe onboard a rocket payload when 30 kg (10 26 molecules) of CF 3 Br) triflouromethyl bromide (was released at 309 km. in less than 0.1 sec, the electron density was reduced from 10 5 cm -3 to less than 15 cm -3 CF 3 Br + e–  Br – + CF 3 time (sec) electrondensity electricfield mV/m cm -3

negative ions in plasma processing Plasma Assisted Chemical Vapor Deposition (PECVD) systems use silane (SiH 4 ) for deposition of amorphous silicon (a-Si:H) for solar cell fabrication positive and negative ions are formed: SiH 4 + e –  SiH H + 2e – (dissociative ionization ) SiH 4 + e –  SiH 3 – + H ( dissociative attachment) chemical reactions among the various species then lead to the formation of bigger particles (nm) which are deposited on a substrate as a thin film. A typical rf processing reactor in which reactive radicals, positive and negative ions, neutrals and molecules are produced when a glow discharge is formed by a continuous flow of feed gas.

Interest in negative ion plasmas much or ordinary plasma behavior is dominated by the fact that m e << m + but in a negative ion plasma we have n e << n +, so the plasma has m –  m + electron induced ambipolar fields no longer dominate shielding of low frequency electric fields by electrons is less important effect on low frequency plasma waves due to the quasineutrality condition n + = n e + n –

e.g. sheaths in a plasma typically v e,th >> v +,th  electrons leave first plasma potential adjusts to maintain quiasi-neutrality  SHEATH plasma potential sheaths position

Production of negative ion plasmas introduce an electronegative gas into a plasma, e.g., SF 6 attachment cross sections are highly energy dependent F is highly corrosive

Q machine SF 6 grid for launching IA waves K + or Cs + plasmas, nearly fully ionized T e = T +  0.2 eV n + ~ 10 8 – cm -3

IQ-3

Attachment cross sections Low energy cross sections SF 6  sulfur hexafluoride C 7 F 14  perfluoromethylcyclohexane

reduction in the electron density as the SF 6 pressure is increased the Langmuir probe is used to observe the reduction in electron density the negative ion contribution to the probe current is much smaller than the electron current since m – >> m e the reduction in electron current can be used to estimate n – /n +

comparison of results in SF 6 and C 7 F 14 in C 7 F 14 can achieve n e /n + < 10 –3

Langmuir probe floating potential V I VpVp VfVf

Ion acoustic waves in a negative ion plasma An e – / + ion plasma supports low frequency (f << f p+ ) ion sound waves in the same way that a gas supports ordinary sound waves the ions provide the inertia for the wave and the electrons the pressure which is communicated to the ions via the electric field a negative ion plasma supports 2 ion acoustic modes – a ‘slow’ mode and a ‘fast’ mode.

Ion acoustic waves in a negative ion plasma p = Fast Mode Slow Mode Notice that for the fast mode, the phase speed is >> ion thermal speed for large values of the negative ion percentage  this reduces, considerably the effects of ion Landau damping on the wave.

IAW in plasma with negative ions Phase velocity wave damping

electrostatic ion cyclotron (EIC) waves in a plasma with negative ions EIC waves are fundamental low frequency (ion) modes of a magnetized plasma they propagate nearly  to B, but with a finite the mode frequency is just above the ion- cyclotron frequency,  c+ : it is excited by an electron drift v ed ~ (10-20) v +,th along the magnetic field the critical electron drift speed needed to excite the mode is reduced in a negative ion plasma

you cannot draw a dc current in a magnetized plasma 100  s electron current

EIC modes in a plasma with K + ions, electrons and C 7 F 14 – Negative ion EIC mode can be used as a diagnostic for the relative concentration of the negative ion. T e = T + = 0.2 eV, T - = 0.03 eV

Power spectra of EIC modes in a plasma with C 7 F 14 No C 7 F 14 with C 7 F FREQUENCY (kHz) POWER SPECTRA OF EIC MODES B = 0.36 T P(C 7 F 14 ) = 0 B = 0.36 T P(C 7 F 14 ) = 6  Torr f o,– f 1,– f o, + f 1, + f o, + f 1, + 10 dB Frequency (kHz)

C 7 F 14 mode frequencies vs. B

At three minutes and four seconds after 2 AM on the 6th of May this year, the time and date will be 02:03:04 05/06/07. This will never happen again.