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Francis F. Chen Third Edition - Eprints STTA Yogyakarta

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The publisher, authors and editors are confident in assuming that the advice and information in this book is believed to be true and correct at the date of publication. Plasma physics has grown so much that it's tempting to include everything that's new, but I haven't.

Occurrence of Plasmas in Nature

The natural occurrence of plasmas at high temperatures is the reason for the term "fourth state of matter". The equilibrium ion fraction should therefore decrease with ni; and this is the reason for the factor ni1 on the right-hand side of Eq.

Definition of Plasma

We must now define "quasi-neutral" and "collective behavior." The meaning of quasi-neutrality will be clarified in Sect. By "collective behavior" we mean movements that depend not only on local conditions, but also on the state of the plasma in distant regions.

Fig. 1.1 Illustrating the long range of electrostatic forces in a plasma
Fig. 1.1 Illustrating the long range of electrostatic forces in a plasma

Concept of Temperature

Because TandEava are so closely related, it is common practice in plasma physics to represent temperatures in units of energy. To avoid confusion about the number of dimensions involved, not Eav but the energy corresponding to KT is used to denote temperature.

Debye Shielding

Potentials of the order KT/ecan leak into the plasma and cause finite electric fields to exist. Fortunately, this region does not contribute much to the thickness of the cloud (called a sheath) because the potential drops off very quickly there.

Fig. 1.4 Potential distribution near a grid in a plasma
Fig. 1.4 Potential distribution near a grid in a plasma

The Plasma Parameter

Criteria for Plasmas

For the case of an infinite, transparent grid charged at a potential ϕ, show that the shielding distance is approximately given by. The space between them is uniformly filled by a gas with a density of charge particles. a) Using Poisson's equation, show that the potential distribution between the plates is.

Applications of Plasma Physics

  • Gas Discharges (Gaseous Electronics)
  • Controlled Thermonuclear Fusion
  • Space Physics
  • Modern Astrophysics
  • MHD Energy Conversion and Ion Propulsion
  • Solid State Plasmas
  • Gas Lasers
  • Particle Accelerators
  • Industrial Plasmas
  • Atmospheric Plasmas

Another important application of plasma physics is the study of Earth's environment in space. The solar wind blows the Earth's magnetic field into a long tail on the night side of the Earth.

Fig. 1.5 Principle of the MHD generator
Fig. 1.5 Principle of the MHD generator

Introduction

Finite E

In the first half cycle of the ion's orbit in Fig.2.2, it gains energy from the electric field and increases inv⊥and thus inrL. For particles with the same speed but different masses, the lighter one will have a smaller rL and thus drift less per cycle.

Fig. 2.2 Particle drifts in crossed electric and magnetic fields
Fig. 2.2 Particle drifts in crossed electric and magnetic fields

Gravitational Field

Approximate the right half of the orbit through a semicircle corresponding to the ion energy after acceleration through the E-field, and the left half through a semicircle corresponding to the energy after deceleration. If Bi is in the +z direction and E is the electrostatic field due to the charge of the beam, calculate the magnitude and direction of the EB drift at r¼a (see Fig.P2.7).

Nonuniform B Field

Curved B: Curvature Drift

If Bis is high enough in the "throat" of the mirror, v eventually becomes zero; and the particle is "bounced" back to the weak field region. A further example of the mirror effect is the confinement of particles in the Van Allen belts.

Fig. 2.8 A plasma trapped between magnetic mirrors
Fig. 2.8 A plasma trapped between magnetic mirrors

Nonuniform E Field

If the electric field is weak, we can use, as an approximation, the unperturbed orbit to estimate Ex(x). If there is a feedback mechanism that causes the second electric field to enhance the first, it grows infinitely and the plasma is unstable.

Time-Varying E Field

If we now make the assumption that Changes slowly, so thatω2ω2c, then Eq. 2.64) is the approximate solution to Eq. Since vpi is in opposite directions for ions and electrons, there is a polarization current; forZ¼1, that is.

Time-Varying B Field

If an E field is suddenly applied, the first thing the ion does is move in the E direction. Since the plasma is diamagnetic, we have B·dS<0 for ions and >0 for electrons.

Summary of Guiding Center Drifts

Adiabatic Invariants

The First Adiabatic Invariant, μ

In particular, a particle that makes a collision during the compression phase can transfer part of its gyration energy to energy, and this is not taken out again in the expansion phase. Since the B-field vanishes at the center of symmetry, ωci is zero there; andμ is not conserved.

Fig. 2.14 Plasma confinement in a cusped magnetic field
Fig. 2.14 Plasma confinement in a cusped magnetic field

The Second Adiabatic Invariant, J

This cannot happen if J is conserved. J determines the length of the line between the breakpoints, and no line has the same length between points with the same jBj. When taking the integral vkδs between the turning points, it may happen that the turning points on δs0 do not coincide with the intersections of the perpendicular planes (Fig. 2.17).

Fig. 2.17 Proof of the invariance of J
Fig. 2.17 Proof of the invariance of J

The Third Adiabatic Invariant, Ф

The magnetic field in the center of the room is 1 T, and you can make a large aspect ratio (Ra) approximation where necessary. At t¼0 an electron of small gyroradius is at z¼0 and r¼r0 with v⊥0¼vk0·(⊥and refers to the direction relative to the magnetic field.) (a) Calculate the magnitude and direction of the resulting center of conduction.

Introduction

  • Maxwell ’ s Equations
  • Classical Treatment of Magnetic Materials
  • Classical Treatment of Dielectrics
  • The Dielectric Constant of a Plasma

Note that we used E and B in the vacuum equations instead of their counterparts Dan and H, which are related by the constants ε0 and μ0. In the vacuum equation (3.1) we must include both the bound charge and the free charge: .

The Fluid Equation of Motion

  • The Convective Derivative
  • The Stress Tensor
  • Collisions
  • Comparison with Ordinary Hydrodynamics
  • Equation of Continuity
  • Equation of State
  • The Complete Set of Fluid Equations

Then all the particles in the fluid element move together and the average velocity u of the particles in the element is equal to the individual velocity of the particles v. The answer is guarded yes and the reasons for this will tell us the limitations of fluid theory.

Fig. 3.2 Direction of the salinity gradient at the mouth of a river
Fig. 3.2 Direction of the salinity gradient at the mouth of a river

Fluid Drifts Perpendicular to B

B2 ð3:69Þ In the particle image one would not expect to measure a current if the conduction centers are not drifting. In the presence of a density gradient, the density of conducting centers is not the same as the density of particles.

Fig. 3.4 Diamagnetic drifts in a cylindrical plasma
Fig. 3.4 Diamagnetic drifts in a cylindrical plasma

Fluid Drifts Parallel to B

The latter is the Boltzmann relation, Eq. b) Show that the plasma rotates as a solid body. Since the plasma is quasi-neutral, the gradient exists for both the electron and ion liquids.

The Plasma Approximation

Of course, if only one species can move and the other cannot follow, such as in high-frequency electron waves, then the plasma approximation is not valid and must be found from Maxwell's equations rather than from the ion and electron equations of motion. We will return to the question of the validity of the plasma approximation when we come to the theory of ion waves.

Representation of Waves

Ifω/kis is positive, the wave moves to the right; that is, xincreases in increments to keep kxωtconstant. The phaseδ can be recovered from Ec, since Re Ec ¼Ecosδ and Im Ec ¼Esinδ; so that.

Group Velocity

Plasma Oscillations

Either traveling waves or standing waves can be created, as in the case of a stretched rope. Note that the time patterns can be obtained by translating the x-patterns in the right direction, as if the wave were passing a fixed observer.

Fig. 4.3 Synthesis of a wave from an assembly of independent oscillators
Fig. 4.3 Synthesis of a wave from an assembly of independent oscillators

Electron Plasma Waves

The accumulation of electrons was not realized in the plasma, but in the oscillating coils at the ends of the plasma column. When the oscillator frequency ω varies, the graph of the dispersion curve (ω/ωp)2vs.ka is obtained, while the radius of the column (Fig. 4.10).

Fig. 4.7 Square of the observed frequency vs. plasma density, which is generally proportional to the discharge current.
Fig. 4.7 Square of the observed frequency vs. plasma density, which is generally proportional to the discharge current.

Sound Waves

Ion Waves

In ion acoustic waves, the other species (namely electrons) is far from fixed; in fact, electrons are pulled along with the ions and tend to shield electric fields created by the bundling of ions. First, the ion thermal motions spread out the ions; this effect gives rise to the second term in the square root of Eq.

Validity of the Plasma Approximation

This is the same as we obtained earlier (Eq. 4.41)) except for the factor 1þk2 λ2D: Our assumptions have given rise to an error of the order k2λ2D¼ð2πλD=λÞ2: Since λD is very small in most experiments, the plasma approximation is invalid everywhere a thin layer, called a mantle (chap.8), a few λDs in thickness, next to a wall.

Comparison of Ion and Electron Waves

The slopes of such lines give the phase velocities plotted in Figure 4.17 for the two masses and different plasma densities n0. The constancy of υs with ωenn0 is shown experimentally, and the two sets of points for K and Cs plasmas show the correct dependence on M.

Fig. 4.14 Q-machine experiment to detect ion waves. [From N. Rynn and N. D ’ Angelo, Rev
Fig. 4.14 Q-machine experiment to detect ion waves. [From N. Rynn and N. D ’ Angelo, Rev

Electrostatic Electron Oscillations Perpendicular to B

The existence of the upper hybrid frequency has been experimentally verified by microwave transmission through a magnetic field. One is like the plasma swing and the other is like the top hybrid swing, but both will be modified by the propagation angle.

diagram for these two waves for fixed k x , where k x /k z ¼ tan θ . Because of the symmetry of Eq
diagram for these two waves for fixed k x , where k x /k z ¼ tan θ . Because of the symmetry of Eq

Electrostatic Ion Waves Perpendicular to B

Electrostatic ion cyclotron waves were first observed by Motley and D'Angelo, again in the aQ-machine (Figure 4.24). In this experiment, the k2v2s term was small compared to the Ω2c term, and the measured frequencies were only slightly above Ωc.

The Lower Hybrid Frequency

If we had used Poisson's equation instead of the plasma approximation, we would have obtained In many low-density plasmas the latter term actually dominates because the plasma approximation is not valid when the Debye length is not negligibly small.

We see that the vacuum relation Eq. 4.76) is modified by a termω2 reminiscent of plasma oscillations. For densities greater than this, Eq. 4.85) cannot be fulfilled for any area and the wave cannot propagate.

Fig. 4.26 Dispersion relation for electromagnetic waves in a plasma with no dc magnetic field
Fig. 4.26 Dispersion relation for electromagnetic waves in a plasma with no dc magnetic field

Experimental Applications

Part of the signal goes to the detector through the "reference leg". The other part is sent through the plasma with horn antennas. Perhaps the best known effect of the plasma cutoff is its application to shortwave radio communications.

Fig. 4.30 A plasma lens has unusual optical properties, since the index of refraction is less than unity
Fig. 4.30 A plasma lens has unusual optical properties, since the index of refraction is less than unity

Electromagnetic Waves Perpendicular to B 0

In plasma physics, it makes more sense to let the "ordinary" wave be the one unaffected by the magnetic field.

Fig. 4.34 An ordinary wave launched from a waveguide antenna toward a magnetized plasma column
Fig. 4.34 An ordinary wave launched from a waveguide antenna toward a magnetized plasma column

¼0 ð4:102Þ Since the coefficientAisω2ω2h;whereωhis is the upper hybrid frequency given by Eq. 4.60), the condition AD¼BC can be written.

Cutoffs and Resonances

The boundary values ​​of the extraordinary wave are found by setting k equal to zero in Eq. Instead of the usual ω–k diagram, it is more illuminating to give a graph of phase velocity versus frequency; or, more precisely, a graph ofω2/c2k2¼1/n~2vs.ω(Fig. 4.36).

Fig. 4.36 The dispersion of the extraordinary wave, as seen from the behavior of the phase velocity with frequency
Fig. 4.36 The dispersion of the extraordinary wave, as seen from the behavior of the phase velocity with frequency

Electromagnetic Waves Parallel to B 0

For the R wave, k becomes infinite at ω¼ωc; the wave is then in resonance with the cyclotron motion of the electrons. The Lwave, on the other hand, has no cyclotron resonance with the electrons because it rotates in the opposite direction.

Experimental Consequences .1 The Whistler Mode.1 The Whistler Mode

Faraday Rotation

Show that there is no Faraday rotation in a positronium plasma (equal number of positrons and electrons). Show that the Faraday angle of rotation, in degrees, of a linearly polarized transverse wave propagating along B0 is given by.

Fig. 4.44 After traversing the plasma, the L wave is advanced in phase relative to the R wave, and the plane of polarization is rotated
Fig. 4.44 After traversing the plasma, the L wave is advanced in phase relative to the R wave, and the plane of polarization is rotated

Hydromagnetic Waves

As we saw before, ε is much larger than unity for most laboratory plasmas, and Eq. ð Þ1=2 ð4:125Þ These hydromagnetic waves move along B0 at a constant velocity vA, called the Alfve´n velocity:. vAB. At the point shown, By is in the positive y-direction, so, according to Eq. 4.128), Exists in the positivex direction ifω/kis in this direction.

Fig. 4.46 Relation among the oscillating quantities in an Alfve´n wave and the (exaggerated) distortion of the lines of force
Fig. 4.46 Relation among the oscillating quantities in an Alfve´n wave and the (exaggerated) distortion of the lines of force

Magnetosonic Waves

It is an acoustic wave in which compressions and rarefactions are produced not by motions along E but by EB motions along E. The phase velocity of the magnetosonic mode is almost always greater than vA; for this reason, it is often simply called "fast".

Summary of Elementary Plasma Waves

Nevertheless, it is a very useful set of equations to consider as a frame of reference for discussing more complex wave motions. Often a complex situation can be understood as a modification or superposition of these basic modes of oscillation.

The CMA Diagram

The upper regions of the CMA diagram correspond to ω ωc: the low-frequency ion waves are found here. The Appleton-Hartree dispersion relation for high-frequency electromagnetic waves propagating at an angle θ to the magnetic field is .

4.34. Figure P4.34 shows a far-infrared laser operating at λ ¼ 337 μ m. When B 0 ¼ 0, this radiation easily penetrates the plasma whenever ω p is less than ω , or n < n c ¼ 10 22 m 3
4.34. Figure P4.34 shows a far-infrared laser operating at λ ¼ 337 μ m. When B 0 ¼ 0, this radiation easily penetrates the plasma whenever ω p is less than ω , or n < n c ¼ 10 22 m 3

Diffusion and Mobility in Weakly Ionized Gases

Collision Parameters

The probability of loss of momentum can be expressed in terms of the equivalent cross section σ the atoms would have if they were perfect absorbers of momentum. The atoms are thought to be opaque spheres with a cross-sectional areaσ; that is, an electron each time.

Fig. 5.2 Illustration of the definition of cross section
Fig. 5.2 Illustration of the definition of cross section

Diffusion Parameters

If a current Γ of electrons is incident on the plate, the current that appears on the other side is Γ0 ¼Γð1nnσdxÞ. Due to the possibility of organized motions (plasma waves), the plasma can spread out in a way that is not truly random.

Decay of a Plasma by Diffusion .1 Ambipolar Diffusion.1Ambipolar Diffusion

Diffusion in a Slab

This is called the lowest diffusion mode. The density distribution is a cosine, and the peak density decays exponentially with time. Substituting this into the diffusion equation (5.17), we see that each cosine term yields a relation of the form

Fig. 5.3 Density of a plasma at various times as it decays by diffusion to the walls
Fig. 5.3 Density of a plasma at various times as it decays by diffusion to the walls

Diffusion in a Cylinder

Higher diffusion modes with more than one maximum in the cylinder will be given in terms of higher-order Bessel functions, in direct analogy with the plate geometry example.

Steady State Solutions

Constant Ionization Function

Plane Source

Line Source

Recombination

When the density is high, recombination, which is proportional ton2, is dominant, and the density decays reciprocally. After the density reaches a low value, diffusion becomes dominant, and the decay is henceforth exponential.

Diffusion Across a Magnetic Field

Ambipolar Diffusion Across B

However, this electric field can be short-circuited by an imbalance of the fluxes along B. In short plasma columns with the field lines terminating on conducting plates, one would expect the ambipolar electric field to be short-circuited.

Experimental Checks

Furthermore, the response depends sensitively on the boundary conditions at the ends of the field lines. The theory correctly predicted the value of Bc. The wave, in the form of a helical distortion of the plasma column, was later seen directly in an experiment by Allen, Paulikas, and Pyle at Berkeley.

Fig. 5.15 The normalized longitudinal electric field measured as a function of B at two different pressures.
Fig. 5.15 The normalized longitudinal electric field measured as a function of B at two different pressures.

Collisions in Fully Ionized Plasmas

  • Plasma Resistivity
  • Mechanics of Coulomb Collisions
  • Physical Meaning of η
  • Numerical Values of η
  • Pulsed Currents

This force is felt when the electron is near the ion; this time is approx. The factor 2.0 comes from the difference in the weighting of the different velocities in the electron distribution.

Fig. 5.16 Shift of guiding centers of two like particles making a 90  collision
Fig. 5.16 Shift of guiding centers of two like particles making a 90 collision

The Single-Fluid MHD Equations

A less obvious equation is obtained by a different linear combination of the equations of the two fluids. 5.82) with M and subtract the latter from the former. EþvB¼ηj ð5:91Þ The continuity equations for massρ and chargeσ are easily obtained from the sum and difference of the continuity equations of ions and electrons.

Diffusion of Fully Ionized Plasmas

First, D⊥ is not a constant in a fully ionized gas; it is proportional tons. This is because the density of scattering centers is determined not by the neutral atomic density, but by the plasma density itself. Finally, we would like to point out that there is no transverse mobility in a fully ionized gas.

Solutions of the Diffusion Equation

Time Dependence

Time-Independent Solutions

Bohm Diffusion and Neoclassical Diffusion

Suppose that the plasma in a fusion reactor is in the form of a cylinder with a diameter of 1.2 m and a length of 100 m. The increasing magnetic field inside the coil induces a surface current in the highly conductive plasma.

Fig. 5.20 Summary of confinement time measurements taken on various types of discharges in the Model C Stellarator, showing adherence to the Bohm diffusion law (Courtesy of D
Fig. 5.20 Summary of confinement time measurements taken on various types of discharges in the Model C Stellarator, showing adherence to the Bohm diffusion law (Courtesy of D

Introduction

Hydromagnetic Equilibrium

Gambar

Fig. 1.1 Illustrating the long range of electrostatic forces in a plasma
Fig. 2.11 Drift of a gyrating particle in a nonuniform electric field
Fig. 2.14 Plasma confinement in a cusped magnetic field
Fig. 2.15 A particle bouncing between turning points a and b in a magnetic field
+7

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