Optically-Excited Waves in 3D Dusty Plasmas John Goree The University of Iowa.

Slides:



Advertisements
Similar presentations
Optical sources Lecture 5.
Advertisements

Waves 2 Sound and Light.
Rotating Wall/ Centrifugal Separation John Bollinger, NIST-Boulder Outline ● Penning-Malmberg trap – radial confinement due to angular momentum ● Methods.
Flinders University of South Australia Leon Mitchell Nathan Prior University of Sydney Brian James Alex Samarian Felix Cheung.
What are Waves? Building Science Champions. In thought On a separate sheet of paper, write a paragraph about how surfers are able to use waves for their.
Phys141 Principles of Physical Science Chapter 6 Waves Instructor: Li Ma Office: NBC 126 Phone: (713) Webpage:
Shock wave propagation across the column of dusted glow discharge in different gases. A.S.Baryshnikov, I.V.Basargin, M.V.Chistyakova Ioffe Physico-Technical.
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
Phonons in a 2D Yukawa triangular lattice: linear and nonlinear experiments Dept. of Physics and Astronomy, University of Iowa supported by DOE, NASA,
Chapter 4 Waves in Plasmas 4.1 Representation of Waves 4.2 Group velocity 4.3 Plasma Oscillations 4.4 Electron Plasma Waves 4.5 Sound Waves 4.6 Ion Waves.
F. Cheung, A. Samarian, B. James School of Physics, University of Sydney, NSW 2006, Australia.
Processing of dust particles in low-pressure plasmas G. Paeva, R.P. Dahiya*, E. Stoffels, W.W. Stoffels, G.M.W. Kroesen, Department of Physics, Eindhoven.
Physics of fusion power Lecture 11: Diagnostics / heating.
The Spatiotemporal Evolution of an RF Dusty Plasma: Comparison of Numerical Simulations and Experimental Measurements Steven Girshick, Adam Boies and Pulkit.
1 Sinusoidal Waves The waves produced in SHM are sinusoidal, i.e., they can be described by a sine or cosine function with appropriate amplitude, frequency,
Measurement of the Charge of a Particle in a Dusty Plasma Jerome Fung, Swarthmore College July 30, 2004.
Lecture 3: Laser Wake Field Acceleration (LWFA)
SPEC(troscopy) -Trap Outline of talk Introduction – motivation for two cross continent traps Imperial College Group – areas of interest and expertise SPECTRAP/SPECTRAP’
1.Today : Review of Science & technology of Light 2.Class #23 1.Invisibility: Is this possible? Yes!!! How it works & when we can buy our invisibility.
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.
ElectroMagnetic Radiation Spectrum The basics about light and waves.
F. Cheung, A. Samarian, W. Tsang, B. James School of Physics, University of Sydney, NSW 2006, Australia.
Waves.
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
Transverse optical mode in a 1-D Yukawa chain J. Goree, B. Liu & K. Avinash.
Consider a time dependent electric field E(t) acting on a metal. Take the case when the wavelength of the field is large compared to the electron mean.
Status of the advanced LIGO laser O. Puncken, L. Winkelmann, C. Veltkamp, B. Schulz, S. Wagner, P. Weßels, M. Frede, D. Kracht.
Electromagnetically Trapped Dusty Plasma Ring R. Sheldon, E. Thomas Jr, D. Gallagher, M. Adrian, M. Abbas, P. Craven & E. Reynolds Wheaton College / National.
Waves and solitons in complex plasma and the MPE - UoL team D. Samsonov The University of Liverpool, Liverpool, UK.
The Influence of the Return Current and the Electron Beam on the X-Ray Flare Spectra Elena Dzifčáková, Marian Karlický Astronomical Institute of the Academy.
1 Experiments on Shocks and Dust Structures in Dusty Plasmas Robert L. Merlino, Jonathon R. Heinrich, Su-Hyun Kim and John K. Meyer Department of Physics.
© 2004 Plano ISD, Plano, TX During every waking and sleeping moment of our lives, we are bombarded with of energy.
PHYS 430/603 material Laszlo Takacs UMBC Department of Physics
Dusty Plasmas I. what is a plasma? l 4 th state of matter (after solid, liquid and gas) l a plasma is: ionized gas which is macroscopically neutral exhibits.
Dusty Plasmas in the Laboratory and Space Bob Merlino April 2003 APS Meeting Philadelphia, PA.
Phonon spectrum measured in a 1D Yukawa chain John Goree & Bin Liu.
Complex Plasmas as a Model for the Quark-Gluon-Plasma Liquid
International Microgravity Plasma Facility John Goree The University of Iowa.
AFM. The cantilever holder The cantilever dimensions Tip position.
Plasmas. The “Fourth State” of the Matter The matter in “ordinary” conditions presents itself in three fundamental states of aggregation: solid, liquid.
Crystallisation Experiments with Complex Plasmas M. Rubin-Zuzic 1, G. E. Morfill 1, A. V. Ivlev 1, R. Pompl 1, B. A. Klumov 1, W. Bunk 1, H. M. Thomas.
Electron cloud in the wigglers of ILC Damping Rings L. Wang SLAC ILC Damping Rings R&D Workshop - ILCDR06 September 26-28, 2006 Cornell University.
Dusty plasmas in basic science, astronomy, industry & fusion John Goree The Univ. of Iowa.
Damping of the dust particle oscillations at very low neutral pressure M. Pustylnik, N. Ohno, S.Takamura, R. Smirnov.
Waves in a 2D Dusty Plasma Crystal
Energy  an object is said to have “energy” if the object has the ability to change its environment Two ways to transfer energy  1. through the application.
Transverse optical mode in a 1-D chain J. Goree, B. Liu & K. Avinash.
Phonons Packets of sound found present in the lattice as it vibrates … but the lattice vibration cannot be heard. Unlike static lattice model , which.
IMPACT Laboratory investigations of electrostatic dust lofting on comet and asteroid (airless bodies) surfaces Xu Wang Joseph Schwan, Hsiang-Wen Hsu, Mihály.
Waves in Plasma Very short course.
Waves Waves can transfer energy and information without a net motion of the medium through which they travel. They involve vibrations (oscillations) 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.
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.
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.
Waves S8P4 - Students will explore the wave nature of sound and electromagnetic radiation. a. Identify the characteristics of electromagnetic and mechanical.
Phonons Packets of sound found present in the lattice as it vibrates … but the lattice vibration cannot be heard. Unlike static lattice model , which.
Matter: States of Matter (Gas)
Compressional and Shear Wakes in a 2D Dusty Plasma Crystal V. Nosenko, J. Goree & Z.W. Ma Univ. of Iowa A. Piel Univ. of Kiel D. Dubin UCSD.
Types of Waves There are two ways we can group waves into different types based on the relationship of the wave to its medium mechanical electromagnetic.
Sound.
Participation IAP NAS of Ukraine in understanding of vacuum breakdown phenomena Iaroslava Profatilova, V.Baturin, O. Karpenko.
N. D’Angelo, B. Kustom, D. Susczynsky, S. Cartier, J. Willig
B. Liu, J. Goree, V. Nosenko, K. Avinash
Wakefield Accelerator
Introduction to Atmospheric Science at Arecibo Observatory
CESRTA Measurement of Electron Cloud Density by TE Wave and RFA
Confining instabilities in a complex plasma S. V. Vladimirov, A. A
UG: Describe the Nature of Electromagnetic Waves
Sound Vs. Light.
Longitudinal-particles move parallel to wave motion
Presentation transcript:

Optically-Excited Waves in 3D Dusty Plasmas John Goree The University of Iowa

plasma = electrons + ions What is a dusty plasma? Debye shielding small particle of solid matter becomes negatively charged absorbs electrons and ions

Solar system Rings of Saturn Comet tails Fundamental science Coulomb crystals Waves Manufacturing Particle contamination (Si wafer processing) Nanomaterial synthesis Who cares about dusty plasmas?

Forces Acting on a Particle Coulomb QE Other forces: Gas drag Ion drag Thermophoresis Radiation Pressure Gravity mg

Electrostatic trapping of particles Equipotential contours electrode positive potential electrode With gravity, particles sediment to high-field region  2-D layer Without gravity, particles fill 3-D volume QE mg

polymer microspheres 8  m diameter Particles separation a  0.5 mm charge Q  e

Same: Coulomb repulsion Crystals Different: Dusty plasma has much lower damping rate  wave propagation is easier Comparison to Colloidal Suspensions

2D physics: Ground-based 3D physics: Flight Experiments described in this talk

triangular lattice with hexagonal symmetry 2D lattice Yukawa inter-particle potential

Two modes in a lattice

Dispersion relations in 2D triangular lattice Wang et al. PRL 2001  =0,

Setup

scanning mirror Scanning mirror Ar laser beam

Longitudinal wave 4mm k Laser incident here f = 1.8 Hz

Random particle motion No Laser! = compression + shear 4mm Nunomura et al. PRL 2002

Phonon spectrum & sinusoidally-excited waves Nunomura et al. PRL 2002

Mach cones

Mach cone angle C = U Sin   U

Lateral wake Transverse Wake Ship’s wake

water  air Wake pattern is determined by dispersion relation Mach cone Lateral & transverse wakes Has both features: Mach Cone Lateral & transverse wakes plasma crystal

Mach cone excitation V/C L = 1.17

Mach cone + lateral wakes Nosenko et al. PRL 2002

3D physics Microgravity

Predecessor microgravity experiments Sounding rockets Morfill et al., PRL – 2002 ISS - PKE

PKE vacuum chamber Cameras for imaging particles Laser sheets for illuminating particles

imaging cameras cw Nd-YAG laser (manipulation) galvanometer scanning mirror diode laser (for imaging) shown in a mid-deck locker:plasma chamber & optics not shown: gas/vacuum, power, data Flight hardware concept for optically-excited waves in 3D dusty plasmas