Physics of fusion power Lecture 7: particle motion.

Slides:



Advertisements
Similar presentations
Physics of fusion power
Advertisements

Basic Plasma Physics Principles Gordon Emslie Oklahoma State University.
Physics of fusion power Lecture 4: Cylindrical concepts.
MHD Concepts and Equations Handout – Walk-through.
AS 4002 Star Formation & Plasma Astrophysics BACKGROUND: Maxwell’s Equations (mks) H (the magnetic field) and D (the electric displacement) to eliminate.
Physics of Fusion Lecture 1: The basics Lecturer: A.G. Peeters.
Single particle motion and trapped particles
Fall 2008Physics 231Lecture 7-1 Magnetic Forces. Fall 2008Physics 231Lecture 7-2 Magnetic Forces Charged particles experience an electric force when in.
Physics of fusion power Lecture 6: Conserved quantities / Mirror device / tokamak.
Wednesday, Oct. 26, 2005PHYS , Fall 2005 Dr. Jaehoon Yu 1 PHYS 1444 – Section 003 Lecture #16 Wednesday, Oct. 26, 2005 Dr. Jaehoon Yu Charged Particle.
Charged Particles in Electric and Magnetic Fields Motion of charged particles Lorentz Force Examples: cyclotron, mass spectrometer.
Plasma Astrophysics Chapter 2: Single Particle Motion Yosuke Mizuno Institute of Astronomy National Tsing-Hua University.
February 16, 2010 Potential Difference and Electric Potential.
Fluid equations, magnetohydrodynamics Multi-fluid theory Equation of state Single-fluid theory Generalised Ohm‘s law Magnetic tension and plasma beta Stationarity.
Physics of fusion power
Physics of fusion power
Physics of fusion power Lecture 4: Cylindrical concepts.
Halliday/Resnick/Walker Fundamentals of Physics 8th edition
Physics of fusion power Lecture 8: Conserved quantities / mirror / tokamak.
Physics of Fusion power Lecture3 : Force on the plasma / Virial theorem.
Physics of fusion power
DEPARTMENT OF PHYSICS AND ASTRONOMY PA113/Unit 3 Electricity and Magnetism Course PA113 – Unit 3.
Physics of fusion power Lecture 8 : The tokamak continued.
Physics of fusion power Lecture 14: Collisions / Transport.
Physics of fusion power Lecture 10 : Running a discharge / diagnostics.
Physics of Fusion power Lecture 7: Stellarator / Tokamak.
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.
Announcements WebAssign HW Set 5 due October 10
Physics of fusion power
Physics of fusion power Lecture 2: Lawson criterion / Approaches to fusion.
Chapter 28 Magnetic Fields Key contents Magnetic fields and the Lorentz force The Hall effect Magnetic force on current The magnetic dipole moment.
Physics of Fusion power Lecture4 : Quasi-neutrality Force on the plasma.
ELECTRICITY & MAGNETISM (Fall 2011) LECTURE # 4 BY MOEEN GHIYAS.
Chapter 5 Diffusion and resistivity
Neoclassical Transport
Announcements WebAssign HW Set 6 due this Friday Problems cover material from Chapters 19 Prof. Kumar tea and cookies today from 5 – 6 pm in room 2165.
Lecture 16 Magnetic Fields& Force
ASEN 5335 Aerospace Environments -- Radiation Belts1 The Radiation Belts A radiation belt is a population of energetic particles stably-trapped by the.
Physics of fusion power Lecture 10: tokamak – continued.
PLASMA HEATING AND HOT ION SUSTAINING IN MIRROR BASED HYBRIDS
Computational Model of Energetic Particle Fluxes in the Magnetosphere Computer Systems Yu (Evans) Xiang Mentor: Dr. John Guillory, George Mason.
Wednesday, Sept. 7, 2005PHYS , Fall 2005 Dr. Jaehoon Yu 1 PHYS 1444 – Section 003 Lecture #3 Monday, Sept. 7, 2005 Dr. Jaehoon Yu Motion of a.
Motion in a constant uniform magnetic field Section 21.
Plasmas. The “Fourth State” of the Matter The matter in “ordinary” conditions presents itself in three fundamental states of aggregation: solid, liquid.
Announcements WebAssign HW Set 5 due October 10 Problems cover material from Chapters 18 HW set 6 due on October 17 (Chapter 19) Prof. Kumar tea and cookies.
Physics of fusion power Lecture 9 : The tokamak continued.
Physics of fusion power Lecture 12: Diagnostics / heating.
Wednesday, Sep. 14, PHYS Dr. Andrew Brandt PHYS 1444 – Section 04 Lecture #5 Chapter 21: E-field examples Chapter 22: Gauss’ Law Examples.
Tuesday March 29, PHYS Dr. Andrew Brandt PHYS 1444 – Section 02 Lecture #15 Tuesday Mar Dr. Andrew Brandt HW7 Ch 27 is due Fri.
Electric Field.
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.
Wednesday, Feb. 8, 2012PHYS , Spring 2012 Dr. Jaehoon Yu 1 PHYS 1444 – Section 004 Lecture #7 Wednesday, Feb. 8, 2012 Dr. Alden Stradeling Chapter.
Superconductivity and Superfluidity Landau Theory of Phase Transitions Lecture 5 As a reminder of Landau theory, take the example of a ferromagnetic to.
Introduction to Plasma Physics and Plasma-based Acceleration
Introduction to Plasma Physics and Plasma-based Acceleration
Particle in uniform B-field
Equilibrium and Stability
An overview of turbulent transport in tokamaks
Physics of fusion power
Larmor Orbits The general solution of the harmonic oscillator equation
Single particle motion and trapped particles
Chapter 3 Plasma as fluids
Charged Particles in Electric and Magnetic Fields
ESS 154/200C Lecture 19 Waves in Plasmas 2
Physics of fusion power
Earth’s Ionosphere Lecture 13
Lesson 3 Forces and Fields
LECTURE I: SINGLE-PARTICLE MOTIONS IN ELECTRIC AND MAGNETIC FIELDS
PHYS 1444 – Section 003 Lecture #3
Presentation transcript:

Physics of fusion power Lecture 7: particle motion

Gyro motion The Lorentz force leads to a gyration of the particles around the magnetic field We will write the motion as The Lorentz force leads to a gyration of the charged particles around the field line Parallel and rapid gyro-motion

Typical values For 10 keV and B = 5T. The Larmor radius of the Deuterium ions is around 4 mm for the electrons around 0.07 mm Note that the alpha particles have an energy of 3.5 MeV and consequently a Larmor radius of 5.4 cm Typical values of the cyclotron frequency are 80 MHz for Hydrogen and 130 GHz for the electrons Often the frequency is much larger than that of the physics processes of interest. One can average over time One can not necessarily neglect the finite (but small) Larmor radius since it leads to important effects.

Additional Force F Consider now a finite additional force F For the parallel motion this leads to a trivial acceleration Perpendicular motion: The equation above is a linear ordinary differential equation for the velocity. The gyro-motion is the homogeneous solution. The inhomogeneous solution

Drift velocity Inhomogeneous solution Solution of the equation

Physical picture of the drift The force accelerates the particle leading to a higher velocity The higher velocity however means a larger Larmor radius The circular orbit no longer closes on itself A drift results. Physics picture behind the drift velocity

Electric field Using the formula And the force due to the electric field One directly obtains the so-called ExB velocity Note this drift is independent of the charge as well as the mass of the particles

Electric field that depends on time If the electric field depends on time, an additional drift appears Polarization drift. Note this drift is proportional to the mass and therefore much larger for the ions compared with the electrons

Consequences of the drifts Assume a Force F on each ion in the x-direction Electrons are stationary Drawing of the slab of plasma with a force F on the ions in the x-direction

Drift leads to charge separation The drift of the ions leads to charge separation. A small charge separation will lead to a large electric field, i.e. a build up of an electric field can be expected This would lead to a polarization drift Quasi-neutrality Drawing of the slab of plasma with a force F on the ions in the x-direction

Electric field evolution The polarization drift balances the drift due to the force The plasma remains quasi- neutral, and the electric field can be calculated from the polarization drift Drawing of the slab of plasma with a force F on the ions in the x-direction

The next drift : The ExB velocity The electric field evolution leads to an ExB velocity Substituting the electric field

The ExB velocity Satisfies the equation Chain. Force leads to drift. Polarization drift balances the drift and leads to electric field, ExB velocity is in the direction of the force Motion due to the ExB velocity

Meaning of the drifts In a homogeneous plasma Free motion along the field line Fast gyration around the field lines ExB drift velocity. Provides for a motion of the plasma as a whole (no difference between electrons and ions) Polarization drift. Allows for the calculation of the electric field evolution under the quasi- neutrality assumption. Provides for momentum conservation.

Inhomogeneous magnetic fields When the magnetic field strength is a function of position the Lorentz force varies over the orbit Taking two points A and B Drawing of the Grad-B force

Inhomogeneous magnetic field Force due to magnetic field gradient is directed such that the particle tries to escape the magnetic field Leads to the grad-B drift

Curvature drift A particle moving along a curved field line experiences a centrifugal force For a low beta plasma Centrifugal force due to the motion along a curved magnetic field

Drifts due to the inhomogeneous field The drifts due to the inhomogeneous field (curvature and grad-B) The drift due to the magnetic field in homogeneity is in general much smaller than the thermal velocity Scales as 1/L where L is the scale length of the magnetic field Scales as  v

All together …. Parallel motion Gyration ExB drift Pololarization drift Grad-B and curvature drift

Conserved quantities In the absence of an electric field Perpendicular energy is conserved And consequently the total energy is conserved

More tricky ….. Consider a changing magnetic field. An electric field is generated Integrating over the area of the Larmor orbit

Acceleration Derive a second equation for the integral of the electric field from Solve through the inner product with the velocity Integrate towards time

Acceleration Integrate in time Note the integration has the opposite orientation compared with the one from Maxwell equation. One is minus the other

Magnetic moment is conserved The equation The magnetic moment is a conserved quantity

Flux conservation The magnetic moment is conserved Calculate the flux through the gyro-orbit Drawing of the ring current of a particle in a magnetic field. The ring will conserve the flux which is related to the magnetic moment

The mirror Theta pinch has end losses But one could use the mirror force to confine particles The mirror has a low B field in the centre and a high field near the coils Particles moving from the centre outward experience a force in the opposite direction Drawing the mirror concept and the motion of a particle in the field (in red)

Mirror configuration From magnetic moment conservation follows the perpendicular energy Energy conservation then dictates that the parallel velocity must decrease Particle moving from A to B

Bouncing condition Assume the particle moving from A to B is reflected in the point B Zero because the particle is reflected

The first key problem of the mirror Only part of the particles are confined (Collisional scattering in the loss region will lead to a rapid loss of the particles from the device)

Second key problem of the mirror The rapid loss of particles makes that the distribution of particles in velocity space is far from the Maxwell of thermodynamic equilibrium The ‘population inversion’ can drive all kinds of kinetic instabilities