Electrostatic Double Layer in Dusty Plasma. Department of Physics, Kohat University of Science and Technology.

Slides:



Advertisements
Similar presentations
P.W. Terry K.W. Smith University of Wisconsin-Madison Outline
Advertisements

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.
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
Non-Resonant Quasilinear Theory Non-Resonant Theory.
“Physics at the End of the Galactic Cosmic-Ray Spectrum” Aspen, CO 4/28/05 Diffusive Shock Acceleration of High-Energy Cosmic Rays The origin of the very-highest-energy.
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.
Univ. Madeira Dept. Física Universidade da Madeira Departamento de Física COST 529 Meeting Eindhoven, March 31st, 2006 project Modes of current transfer.
Modeling Generation and Nonlinear Evolution of VLF Waves for Space Applications W.A. Scales Center of Space Science and Engineering Research Virginia Tech.
NUMERICAL INVESTIGATION OF WAVE EFFECTS IN HIGH-FREQUENCY CAPACITIVELY COUPLED PLASMAS* Yang Yang and Mark J. Kushner Department of Electrical and Computer.
High-Mach Number Relativistic Ion Acoustic Shocks J. Fahlen and W.B. Mori University of California, Los Angeles.
Chapter 3.1 Weakly Nonlinear Wave Theory for Periodic Waves (Stokes Expansion)  Introduction The solution for Stokes waves is valid in deep or intermediate.
Halliday/Resnick/Walker Fundamentals of Physics 8th edition
Buneman and Ion Two-Stream Instabilities in the Foot Region of Collisionless Shocks Fumio Takahara with Yutaka Ohira (Osaka University) Oct. 6, 2008 at.
Introducing Some Basic Concepts Linear Theories of Waves (Vanishingly) small perturbations Particle orbits are not affected by waves. Dispersion.
Boundaries in the auroral region --- Small scale density cavities and associated processes --- Vincent Génot (CESR/CNRS) C. Chaston (SSL) P. Louarn (CESR/CNRS)
Lecture 3: Laser Wake Field Acceleration (LWFA)
Lectures 11-12: Gravity waves Linear equations Plane waves on deep water Waves at an interface Waves on shallower water.
5. Simplified Transport Equations We want to derive two fundamental transport properties, diffusion and viscosity. Unable to handle the 13-moment system.
Physics of fusion power Lecture 2: Lawson criterion / some plasma physics.
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.
Ch 9 pages ; Lecture 21 – Schrodinger’s equation.
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
Chapter 5 Diffusion and resistivity
ENE 311 Lecture 2. Diffusion Process The drift current is the transport of carriers when an electric field is applied. There is another important carrier.
Speed-Current Relation in Lightning Return Strokes Ryan Evans, Student - Mostafa Hemmati, Advisor Department of Physical Sciences Arkansas Tech University.
Large-amplitude oscillations in a Townsend discharge in low- current limit Vladimir Khudik, Alex Shvydky (Plasma Dynamics Corp., MI) Abstract We have developed.
Modelling of the Effects of Return Current in Flares Michal Varady 1,2 1 Astronomical Institute of the Academy of Sciences of the Czech Republic 2 J.E.
ACKNOWLEDGMENTS This research was supported by the National Science Foundation of China (NSFC) under grants , , , the Specialized.
Average Lifetime Atoms stay in an excited level only for a short time (about 10-8 [sec]), and then they return to a lower energy level by spontaneous emission.
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.
TO THE POSSIBILITY OF STUDY OF THE EXTERNAL SOLAR WIND THIN STRUCTURE IN DECAMETER RADIO WAVES Marina Olyak Institute of Radio Astronomy, 4 Chervonopraporna,
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.
Typical Mean Dynamic Balances in Estuaries Along-Estuary Component 1. Barotropic pressure gradient vs. friction Steady state, linear motion, no rotation,
Stephan I. Tzenov STFC Daresbury Laboratory,
Double RF system at IUCF Shaoheng Wang 06/15/04. Contents 1.Introduction of Double RF System 2.Phase modulation  Single cavity case  Double cavity case.
M. Onofri, F. Malara, P. Veltri Compressible magnetohydrodynamics simulations of the RFP with anisotropic thermal conductivity Dipartimento di Fisica,
Lecture 21-22: Sound Waves in Fluids Sound in ideal fluid Sound in real fluid. Attenuation of the sound waves 1.
Norhayati Soin 06 KEEE 4426 WEEK 3/2 20/01/2006 KEEE 4426 VLSI WEEK 4 CHAPTER 1 MOS Capacitors (PART 3) CHAPTER MOS Capacitance.
Particle Acceleration by Relativistic Collisionless Shocks in Electron-Positron Plasmas Graduate school of science, Osaka University Kentaro Nagata.
Passage of magnetostatic waves through the lattice on the basis of the magnon crystal. Performed by Lanina Mariya, III year student, Faculty of Nonlinear.
Lecture 3. Full statistical description of the system of N particles is given by the many particle distribution function: in the phase space of 6N dimensions.
Waves in Plasma Very short course.
Numerical simulations of wave/particle interactions in inhomogeneous auroral plasmas Vincent Génot (IRAP/UPS/CNRS, Toulouse) F. Mottez (LUTH/CNRS, Meudon)
Superconductivity and Superfluidity Landau Theory of Phase Transitions Lecture 5 As a reminder of Landau theory, take the example of a ferromagnetic to.
Generation of anomalously energetic suprathermal electrons by an electron beam interacting with a nonuniform plasma Dmytro Sydorenko University of Alberta,
A Global Hybrid Simulation Study of the Solar Wind Interaction with the Moon David Schriver ESS 265 – June 2, 2005.
Saturation Roi Levy. Motivation To show the deference between linear and non linear spectroscopy To understand how saturation spectroscopy is been applied.
Introduction to Plasma Physics and Plasma-based Acceleration
Chapter 4 Fluid Mechanics Frank White
The London-London equation
A.S. Lidvansky, M.N. Khaerdinov, N.S. Khaerdinov
Chapter 3 Plasma as fluids
Huishan Cai, Jintao Cao, Ding Li
101° Congresso della societa italiana fisica
Nonequilibrium statistical mechanics of electrons in a diode
UNIT - 4 HEAT TRANSFER.
Kinetic Theory.
Chapter 25 Electric Potential.
The propagation of waves in an inhomogeneous medium
ESS 154/200C Lecture 19 Waves in Plasmas 2
paraxial approximation
Two-fluid Collisionless MHD
Strathclyde University, 3-8 September 2000
Physics of fusion power
Coronal Loop Oscillations observed by TRACE
Chapter 25 - Summary Electric Potential.
LECTURE I: SINGLE-PARTICLE MOTIONS IN ELECTRIC AND MAGNETIC FIELDS
Electron Acoustic Waves in Pure Ion Plasmas F. Anderegg C. F
K. A. Goodrich, R. E. Ergun, S. J. Schwartz, L. B
Two-fluid Collisionless MHD
Presentation transcript:

Electrostatic Double Layer in Dusty Plasma. Ghafran Khan, Zahid Kumail and Younas Khan Department of Physics, Kohat University of Science and Technology (KUST), Kohat, Pakistan Supervisor : Dr.Muhammad Adnan Khalil

Contents Motivation Model Equation Dispersion Relations Nonlinear Structures Conclusion

"Cairns et al. (1995) describe the distribution for non-thermal electrons to study the ion acoustic solitary structures observed by the FREJA satellite. FREJA and VIKING satellite both observe the electric field in space plasma which suggest that they are mostly likely electrostatic in nature [Dovner et al., 1994]. There are basically two types of density structure observed by these satellite. the FREJA satellite observe density known as lower-hybrid cavitons, the first observation of lower hybrid cavities in the auroral zone were reported by Vego at al [1992]. Similar structure have also been observed by VIKING satellite [Bostrom et al.,1988, Bostrom 1992] without associated lower hybrid waves. Maxwell distribution cannot gives the solution to the upper and lower cavities occur in the electrostatic waves. In 1995 R.A. Cairns propose theoretical explanation of these structure which he take to be a large amplitude of ion sound waves. He show that in the presence of a distribution of electron which is non-thermal, with an excess of energetic particles the nature of ion sound solitary structures changes and that is possible to obtain the solution with density depletions and dimensions roughly agreement with those observed freja and Viking satellite. Motivation

Cairns et al. (1995.) describe the distribution for non- thermal electrons. FREJA and VIKING satellite both observe the electric field in space plasma which suggest that they are mostly likely electrostatic in nature. FREJA satellite observe density known as lower- hybrid cavitons. VIKING satellite also observed similar structure without associated lower hybrid waves. Maxwell distribution cannot gives the solution to the upper and lower cavities occur in the electrostatic waves. Motivation GEOPHYSICAL RESEARCH LETTERS, VOL 22,NO 20, PAGES , OCTOBER 15, 1995

Maxwellian distribution In any system, a particle will have a wide range of energy, Graph shows the maxwell-boltzmann distributions having number of particles each having a particular energies. Most particles having a moderate energies Some particles having high energies A few particles have very low energies f(v) Graph rep M.D of a system

Non-thermal distribution Non-thermal distribution of electron which include the population of energetic (fast) as employed by cairns et al where is the parameter determining the number of energetic (non-thermal) electron present in model. The value of is always less then one. If is equall to zero then it recover Maxwell distribution of electron. Ref: Geophysical research letters. Vol.22.No.20.Pages October (A)(A)

Maxwell and non-thermal Graph

Comparison between Our and Samiran Ghosh work Our Work Electron, Ions, Dust plasma Ions are inertial and mobile Electron are massless and mobile Dust particle are stationary Electrostatic structure Non-thermal distribution More realistic Ref : Eur. Phys. J. Appl. Phys. 33, 199–203 (2006) Electron, Ions, Dust plasma Ions are inertial and mobile Electron are massless and mobile Dust particle are stationary Electrostatic structure Maxwellian distribution Less realistic S.Ghosh

History of Double layer Double layers were described in 1929 by the plasma pioneer and Nobel laureate Irving Langmuir. Another Nobel laureate, Hannes Alfvén, described a double layer as, “… a plasma formation by which a plasma — in the physical meaning of this word — protects itself from the environment. It is analogous to a cell wall by which a plasma. In the biological meaning of this word “protects” itself from the environment.”

Double Layer A double layer is structure in plasma consist of two parallel layer with opposite electrical charge. The sheet of charge cause strong electric field and correspondingly sharp change in voltage across the double layer. Ions and electrons which enter the double layer is accelerated, decelerated or reflected by the electric field. Double layer which may be curved rather than flat. Double layer are found in discharge tube to space plasma. Double layer are very thin, with widths ranging from a few millimetres to the thousand of kilometres.

Model Equations Three component dusty plasma

Normalized Equations Normalized Parameter t→ X →

We use the Fourier analysis for the small amplitude of wave Fourier Analysis: Reductive perturbation: method is used when one cannot deal the equations with full nonlinearity and weak nonlinearity are assumed in the system. The stretched variables in space and time are defined and slow time variations are induced by the nonlinearity of the system. Non-Linear Dynamics in Plasma Linear and Non-linear dynamic

Dispersion Relations Charge Neutrality condition Ion Temperature Ratio Dispersion for Maxwell distribution of electron by (samiran Ghosh) Maxwell distribution

Derivation of mKdV equation In order to find the nonlinear mKdV equation for one dimensional electrostatic waves in a unmagnatized dusty plasma having a non-thermal electrons, the stretching of independent variables is given by We use the standard reductive perturbation method (RPM) to solve the set of nonlinear equations.The perturbed quantities in terms of ε can be expanded. A B

Derivation of mKdV equation We introduce (A) and (B) in Normalized equation and equate the term of O(ε²), O(ε³) and O(ε ⁴ ) Similarly for Poisson equation The term is given by (C) (D) (E) (F)

The phase velocity is given by The (D) and (F) combine to give mKdV equation Dispersion in system

Solution of Double Layer (2) where Sagdeev potential V(ψ) is given by (3) (4) (5)

Solution of Double Layer Applying the first two boundary conditions of (5), we obtain : (6) Using (6), the expression of V(ψ) can be rewritten as, The double layer solution of equation (7)

where Δ is the thickness of the double layer. It should be noted from above equations (6,7) that for the existence of a double layer, we must have Solution of Double Layer as for ion acoustic wave in dusty plasma always β>0 (Eq.2). Also the nature of double layer i.e. whether the system will support a compressive or rarefactive double layer depends on the sign of the coefficient of quadratic nonlinear term α ₁. It follows from (6) that a compressive double or rarefactive double layer exists according as

Non-Thermal and maxwellian Graph

Conclusion We show that the potential difference between double layer is broader and is more realistic to the experimental observation.

Acknowledgement ….