Dusty plasmas with magnetized dust

Slides:



Advertisements
Similar presentations
INFLUENCE OF RAMSAUER EFFECT ON BOUNDED PLASMAS IN MAGNETIC FIELDS N. Sternberg and C. Sataline, Clark University, Worcester, MA, USA V. Godyak, RF Plasma.
Advertisements

Alex.A. Samarian and Brian.W. James School of Physics, University of Sydney, NSW 2006, Australia Sheath edge location The charge of dust particles in sheath.
Methanol maser polarization in W3(OH) Lisa Harvey-Smith Collaborators: Vlemmings, Cohen, Soria-Ruiz Joint Institute for VLBI in Europe.
Resonance Capture generalization to non- adiabatic regime Observatoire de Cote d’Azur, Jan 2007 Alice Quillen University of Rochester.
Plasmas in Space: From the Surface of the Sun to the Orbit of the Earth Steven R. Spangler, University of Iowa Division of Plasma Physics, American Physical.
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
F. Cheung, A. Samarian, B. James School of Physics, University of Sydney, NSW 2006, Australia.
Max P. Katz, Wayne G. Roberge, & Glenn E. Ciolek Rensselaer Polytechnic Institute Department of Physics, Applied Physics and Astronomy.
Physics of fusion power
Dusty Plasmas M. Coppins M. Bacharis C. Willis T. Zimmermann J. Allen Z. Ehsan.
The Magnetic Field The force on a charge q moving with a velocity The magnitude of the force.
The Martian Ionosphere in Regions of Crustal Magnetic Fields Paul Withers, Michael Mendillo, Dave Hinson DPS 2004, Louisville, Kentucky,
The Magnetized Dusty Plasma Experiment (MDPX)
A Critical Role for Viscosity in the Radio Mode AGN Feedback Cycle Paul Nulsen Harvard-Smithsonian Center for Astrophysics 2014 July 9X-ray View of Galaxy.
F. Cheung, A. Samarian, W. Tsang, B. James School of Physics, University of Sydney, NSW 2006, Australia.
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
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.
Table Top Plasma Experiments
Electromagnetically Trapped Dusty Plasma Ring R. Sheldon, E. Thomas Jr, D. Gallagher, M. Adrian, M. Abbas, P. Craven & E. Reynolds Wheaton College / National.
Computational Astrophysics: Magnetic Fields and Charged Particle Dynamics 11-dec-2008.
TITLE: Scaling of the far SOL turbulence as a function of (1), the average density keeping other plasma parameters constant. (3), the plasma current keeping.
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
9 May MESSENGER First Flyby Magnetospheric Results J. A. Slavin and the MESSENGER Team BepiColombo SERENA Team Meeting Santa Fe, New Mexico 11 May.
Types of Waves and Their Properties. Transverse Waves Particles vibrate at right angles to the direction the wave is traveling Transverse Waves Particles.
The Propagation of Electromagnetic Wave in Atmospheric Pressure Plasma Zhonghe Jiang XiWei Hu Shu Zhang Minghai Liu Huazhong University of Science & Technology.
The propagation of a microwave in an atmospheric pressure plasma layer: 1 and 2 dimensional numerical solutions Conference on Computation Physics-2006.
THE IOWA IQ-2 Q MACHINE. Schematic diagram of IQ-2 HP-E HP-W Pumping system 30 cm 198 cm 60 cm 63.5 mm 50 cm.
Two problems with gas discharges 1.Anomalous skin depth in ICPs 2.Electron diffusion across magnetic fields Problem 1: Density does not peak near the.
Physics of fusion power Lecture 12: Diagnostics / heating.
Laboratory Study of Spiky Potential Structures Associated with Multi- Harmonic EIC Waves Robert L. Merlino and Su-Hyun Kim University of Iowa Guru Ganguli.
Coulomb fission of a charged dust cloud in an afterglow plasma*
R. L. Merlino, J. R. Heinrich, and S.-H. Kim University of Iowa
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.
“Ambipolar Diffusion” and Magnetic Reconnection Tsap Yu. T
1 The effect of negative ions on the charging of dust in a plasma Bob Merlino and Su-Hyun Kim The University of Iowa Supported by The U. S. Dept. of Energy.
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
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.
Narrow plasma & electron injection simulations for the AWAKE experiment A. Petrenko, K. Lotov, October 11,
Multitube Helicon Source with Permanent Magnets
Faraday Rotation as a Diagnostic of Cosmic Magnetic Fields
Main Scientific Challenge of this research area
Microwave Plasma Discharge and Its Applications
Field-Particle Correlation Experiments on DIII-D Frontiers Science Proposal Under weakly collisional conditions, collisionless interactions between electromagnetic.
Introduction to Plasma Physics and Plasma-based Acceleration
Magnetism Magnetism Lecture 15 Today Magnetic Fields
Single particle motion and trapped particles
N. D’Angelo, B. Kustom, D. Susczynsky, S. Cartier, J. Willig
Inside Jupiter and Saturn
DOE Plasma Science Center Control of Plasma Kinetics
Exam 1 Results Sores are curved: Score based out of 98 total points
Electromagnetic Radiation
B. Liu, J. Goree, V. Nosenko, K. Avinash
Wakefield Accelerator
Stern-Gerlach experiment
Electromagnetic Spectrum
LASER-COLLISION INDUCED FLUORESCENCE IN ARGON DISCHARGES
M4 m4 WHAT IS A TOKAMAK? Graphic: EUROfusion, Reinald Fenke, CC BY 4.0,
New Diagnostic for Electric Field
A beam of particles, all with the same momentum but with a variety of masses and charges, enters a region of uniform magnetic field, as shown in the picture.
Ion Motion Through an RFQ
Topic links activity Physics A
Types of Waves.
How fast does sound travel through a solid, liquid and gas?
Rectangular Waveguide
How fast does sound travel through a solid, liquid and gas?
Selection of dust particles in the self-organized dust structures
Resonance Capture generalization to non-adiabatic regime
Superconducting Magnets
Presentation transcript:

Dusty plasmas with magnetized dust Auburn University  October 19, 2009 Dusty plasmas with magnetized dust Bob Merlino University of Iowa Full text available at: http://www.physics.uiowa.edu/~rmerlino/Dusty%20Plasmas.htm

Why? New dusty plasma physics to study Astrophysical and planetary dusty plasmas have magnetized dust Much theoretical work on waves in magnetized dusty plasmas has been done

Criteria for magnetized dust 1. dust gyroradius << transverse plasma dimension 2. dust gyrofrequency >> dust-neutral collision frequency

Magnetic field strength vs. device size Criteria can be satisfied with high B and moderate size device, or Moderate B and very large device Cost trade-off ??

Dust size consideration Both criteria are satisfied more easily with small dust grains But, grains that are too small are not easily imaged Another issue  diagnostics ??

Plasma source considerations Not easy to make uniform and stable plasmas in high B fields Discharge sources require neutral gas, and the dust-neutral collision frequency ~ pressure Probably need plasma source that operates at pressures below 10-5 torr

Parameter scalings (a = dust radius)

Dust gyroradius vs. B

questions Should the particles be large enough to be imaged? How will we diagnose this dusty plasma? What type of plasma source should be used? What dusty plasma physics should be studied