# Chapter10 [186,16 KiB]

Past exam papers (c) Assume that the ion oscillations are so slow that the electrons remain in a MaxwellBoltzmann distribution. If eφ/kB Te 1, show that the perturbed charge density of the electrons is given by −(n0 e2 /kB Te )φ. (d) Use Poisson’s equation to deduce the following dispersion relation: k 2 = (n0 e2 /mi ε0 ω 2 )k 2 − n0 e2 /kB Te ε0 (e) Recast the dispersion relation in the following form: 2 ω 2 = ωpi /(1 + 1/k 2 λ2D ). Discuss the low and high-k limits and compare with the Bohm-Gross dispersion relation for electron plasma waves. Question 3 (10 marks) (a) Using the steady-state force balance equation (ignore the convective derivative) show that the particle ﬂux Γ = nu for electrons and singly charged ions in a fully ionized unmagnetized plasma is given by: Γj = nuj = ±µj nE − Dj ∇n with mobility µ =| q | /mν where ν is the electron-ion collision frequency and diﬀusion coeﬃcient D = kB T /mν. (b) Show that the diﬀusion coeﬃcient can be expressed as D ∼ λ2mfp /τ where λmfp is the mean free path between collisions and τ is the collision time. (c) Show that the plasma resistivity is given approximately by η = me ν/ne2 . (d) In the presence of a magnetic ﬁeld, the mean perpedicular velocity of particles across the ﬁeld is given by ∇n uE + uD u⊥ = ±µ⊥ E − D⊥ + n 1 + ν 2 /ωc2 with uE = E×B/B 2 , uD = −∇p×B/qnB 2 and where µ⊥ = µ/(1 + ωc2 τ 2 ) and D⊥ = D/(1 + ωc2 τ 2 ). Discuss the scaling with ν of each of the four terms in the expression for u⊥ . Question 4 (10 marks) (a) Show that the drift speed of a charge q in a toroidal magnetic ﬁeld can be written as vT = 2kB T /qBR where R is the radius of curvature of the ﬁeld. (Hint: Consider both gradient and curvature drifts) (b) Compute the value of vT for a plasma at a temperature of 10 keV, a magnetic ﬁeld strength of 2 T and a major radius R = 1 m. (c) Compute the time required by a charge to drift across a toroidal container of minor radius 1 m. (d) Suppose an electric ﬁeld is applied perpendicular to the plane of the torus. Describe what happens. Question 5 (10 marks) (a) Show that the MHD force balance equation ∇p = j×B requires both j and B to lie on surfaces of constant pressure. (b) Using Ampere’s law and MHD force balance, show that B2 ∇ p+ 2µ0 = 1 (B.∇)B µ0 and discuss the meaning of the various terms. (c) A straight current carrying plasma cylinder (linear pinch) is subject to a range of instabilities (sausage, kink etc.). These can be suppressed by providing an axial magnetic ﬁeld Bz that stiﬀens the plasma through the additional magnetic pressure Bz2 /2µ0 and tension against bending. Consider a local constriction dr in the radius r of the plasma column. Assuming that the longitudinal magnetic ﬂux Φ through the cross-section of the cylinder remains constant during the compression (dΦ = 0), show that the axial magnetic ﬁeld strength is increased by an amount dBz = −2Bz dr/r. (d) Show that the internal magnetic pressure increases by an amount dpz = Bz dBz /µ0 = −(2Bz2 /µ0 )dr/r. [The last step uses the result obtained in (c)]. (e) By Ampere’s law we have for the azimuthal ﬁeld component rBθ (r) = constant. Show that the change in azimuthal ﬁeld strength due the compression dr is dBθ = −Bθ dr/r and that the associated increase in external azimuthal magnetic pressure is dpθ = −(Bθ2 /µ0 )dr/r. (f) Show that the plasma column is stable against sausage distortion provided Bz2 > Bθ2 /2. Question 6 (10 marks) (a) Plot the wave phase velocity as a function of frequency for plasma waves propagating perpendicular to the magnetic ﬁeld B, identifying cutoﬀs and resonances for both ordinary and extraordinary modes. (b) Using the matrix form of the wave dispersion relation S − n2z −iD nx n z Ex iD S − n2x − n2z 0 Ey = 0 0 P − n2x Ez nx n z show that the polarization state for the extraordinary wave is given by Ex /Ey = iD/S. Using a diagram, show the relative orientations of B, k and E for this wave. Past exam papers THE AUSTRALIAN NATIONAL UNIVERSITY First Semester Examination 2000 PHYSICS C17 PLASMA PHYSICS Writing period 2 hours duration Study period 15 minutes duration Permitted materials: Calculators Attempt four questions. All are of equal value. Show all working and state and justify relevant assumptions. Question 1 (10 marks) Attempt three of the following. Answers for each should require at most half a page. (a) Discuss the relationship between the Boltzmann equation, the electron and ion equations of motion and the single ﬂuid force balance euqation. (b) Describe electric breakdown with reference to the parameter E/p and the role of secondary emission. (c) Discuss the physical meaning of the Boltzmann relation. Use diagrams to aid your explanation. (d) Discuss the origin of plasma diamagnetism and its implications for magnetic plasma conﬁnement. (e) Draw a Langmuir probe I-V characteristic indicating the saturation currents, plasma potential and ﬂoating potential. How can the characteristic be used to estimate temperature? (f) Describe Debye shielding and the relationship between the plasma frequency and Debye length. Question 2 (10 marks) (a) Consider two inﬁnite, perfectly conducting plates A1 and A2 occupying the planes y = 0 and y = d respectively. An electron enters the space between the plates through a small hole in plate A1 with initial velocity v towards plate A2 . A potential diﬀerence V between the plates is such as to decelerate the electron. What is the minimum potential diﬀerence to prevent the electron from reaching plate A2 . (b) Suppose the region between the plates is permeated by a uniform magnetic ﬁeld B parallel to the plate surfaces (imagine it as pointing into the page). A proton appears at the surface of plate A1 with zero initial velocity. As before, the potential V between the plates is such as to accelerate the proton towards plate A2 . What is the minimum value of the magnetic ﬁeld B necessary to prevent the proton from reaching plate B? Sketch what you think the proton trajectory might look like. (HINT: Energy considerations may be useful). Question 3 (10 marks) (a) Using the equilibrium force balance equation for electrons (assume ions are relatively immobile) show that the conductivity of an unmagnetized plasma is given by σ0 = ne2 me ν (10.4) (b) What is the dependence of the conductivity on electron temperature and density in the fully ionized case? (c) When the plasma is magnetized, the Ohm’s law for a given plasma species (electrons or ions) becomes j = σ0 (E + u×B) where j = nqu is the current density. Show that the familiar E×B drift is recovered when the collision frequency becomes very small. (d) If E is at an angle to B, there will be current ﬂow components both parallel and perpendicular to B, If ui is diﬀerent from ue , there is also a nett Hall current j ⊥ = en(ui⊥ − ue⊥ ) that ﬂows in the direction E×B. To conveniently describe all these currents, the Ohm’s ↔ law can equivalently be expressed by the tensor relation j = σ E with conductivity tensor given by σ⊥ −σH 0 ↔ σ⊥ 0 σ= (10.5) σH 0 0 σ where ν2 ν 2 + ωc2 ∓νωc = σ0 2 ν + ωc2 ne2 = σ0 = mν σ⊥ = σ0 σH σ Explain the collision frequency dependence of the perpendicular and Hall conductivities. Past exam4 papers Question (10 marks) Answer either part (a) or part (b) (a) Consider the two sets of long and straight current carrying conductors shown in confurations A and B of Figure 1. (i) Sketch the magnetic ﬁeld line conﬁguration for each case. (ii) Describe the particle guiding centre drifts in each case, with particular emphasis on the conservation of the ﬁrst adiabatic moment. (iii) Charge separation will occur due to the magnetic ﬁeld inhomogeneity. This in turn establishes an electric ﬁeld. Comment on the conﬁning properties (or otherwise) of this electric ﬁeld. Configuration A Configuration B Figure 10.1: Conductors marked with a cross carry current into the page (z direction), while the dots indicate current out of the page. (b) In a small experimental plasma device, a toroidal B-ﬁeld is produced by uniformly winding 120 turns of conductor around a toroidal vacuum vessel and passing a current of 250A through it. The major radius of the torus is 0.6m. A plasma is produced in hydrogen by a radiofrequency heating ﬁeld. The electrons and ions have Maxwellian velocity distribution functions at temperatures 80eV and 10eV respectively. The plasma density at the centre of the vessel is 1016 m−3 . (i) Use Ampere’s law around a toroidal loop linking the winding to calculate the vacuum ﬁeld on the axis of the torus. (ii) What is the ﬁeld on axis in the presence of the plasma? (iii) Calculate the total drift for both ions and electrons at the centre of the vessel and show the drifts on a sketch. (iv) Explain how these drifts are compensated when a toroidal current is induced to ﬂow. (v) The toroidal current produces a poloidal ﬁeld. The combined ﬁelds result in helical magnetic ﬁeld lines that encircle the torus axis. For particles not on the torus axis and which have a high parallel to perpendicular velocity ratio the projected guiding centre motion executes a rotation in the poloidal plane (a vertical cross-section of the torus) as it moves helically along a ﬁeld line. What happens to particles that have a high perpendicular to parallel velocity ratio? Question 5 (10 marks) There is a standard way to check the relative importance of terms in the single ﬂuid MHD equations. For space derivatives we choose a scale length L such that we can write ∂u/∂x ∼ u/L. Similarly we choose a time scale τ such that ∂u/∂t ∼ u/τ . So ∇×E = ∂B/∂t becomes E/L ∼ B/τ . Introduce velocity V = L/τ so that E ∼ BV . (a) Examine the single ﬂuid momentum equation. ρ ∂u = j×B − ∇p ∂t (10.6) Show that the terms are in the ratio nmi 2 V nme vthe : jB : τ L or 1 : 2 jBτ me vthe : nmi V mi V 2 (10.7) When the plasma is cold, show that this suggests V ∼ jBτ /nmi (b) Examine the generalized Ohm’s law: me ∂j 1 1 = E + u×B − j×B + ∇pe − ηj ne2 ∂t ne ne (10.8) Show that the terms are in the ratio 2 1 1 νei 1 vthe : 1 : 1 : : : 2 2 ωce ωci τ ωci τ ωce τ V ωce ωci τ (10.9) (c) Which terms of the Ohm’s law can be neglected if (i) τ 1/ωci (ii) τ ≈ 1/ωci (iii) τ ≈ 1/ωce (iv) τ 1/ωce When can the resistive term ηj be dropped? Question 6 (10 marks) Electromagnetic wave propagation in an unmagnetized plasma. Consider an electromagnetic wave propagating in an unbounded, unmagnetized uniform plasma of equilibrium density n0 . We assume the bulk plasma velocity is zero (v 0 = 0) but allow small drifts v1 to be induced by the one-dimensional harmonic electric ﬁeld perturbation E = E1 exp [i(kx − ωt)] that is transverse to the wave propagation direction. Past exam papers (a) Assuming the plasma is also cold (∇p = 0) and collisionless, show that the momentum equations for electrons and ions give n0 mi (−iωvi1 ) = n0 eE1 n0 me (−iωve1 ) = −n0 eE1 (b) The ion motions are small and can be neglected (why?). Show that the resulting current density ﬂowing in the plasma due to the imposed oscillating wave electric ﬁeld is given by j1 = en0 (vi1 − ve1 ) ≈ i n0 e2 E1 . me ω (10.10) (c) Associated with the ﬂuctuating current is a small magnetic ﬁeld oscillation which is given by Ampere’s law. Use the diﬀerential forms of Faraday’s law and Ampere’s law (Maxwell’s equations) to obtain the ﬁrst order equations kE1 = ωB1 and ikB1 = µ0 j1 − iωµ0 ε0 E1 linking B1 , E1 and j1 . (d) Use these relations to eliminate B1 and j1 to obtain the dispersion relation for plane electromagnetic waves propagating in a plasma: k2 = 2 ω 2 − ωpe c2 (10.11) (d) Sketch the dispersion relation and comment on the physical signiﬁcance of the dispersion near the region ω = ωpe . THE AUSTRALIAN NATIONAL UNIVERSITY First Semester Examination 2001 PHYSICS C17 PLASMA PHYSICS Writing period 2 hours duration Study period 15 minutes duration Permitted materials: Calculators Attempt four questions. All are of equal value. Show all working and state and justify relevant assumptions. Question 1 Attempt three of the following. Answers for each should require at most half a page. (a) Discuss the relationship between moments of the particle distribution function f and moments of the Boltzmann equation. Plot f (v) for a one dimensional drifting Maxwellian distribution, indicating pictorially the meaning of the three lowest order velocity moments. (b) Describe electric breakdown with reference to the parameter E/p and the role of secondary emission. (c) Discuss the physical meaning of the Boltzmann relation. Use diagrams to aid your explanation. (d) Discuss the origin of plasma diamagnetism and its implications for magnetic plasma conﬁnement. (e) Elaborate the role of Coulomb collisions for diﬀusion in a magnetized plasma. (f) Discuss magnetic mirrors with reference to the adiabatic invariance of the orbital magnetic moment µ. (g) Describe Debye shielding and the relationship between the plasma frequency and Debye length. Question 2 Consider an axisymmetric cylindrical plasma with E = Er̂, B = B ẑ and ∇pi = ∇pe = r̂∂p/∂r. If we negelct (v.∇)v, the steady state two-ﬂuid momentum-balance equations can be written in the form en(E + ui ×B) − ∇pi − e2 n2 η(ui − ue ) = 0 −en(E + ue ×B) − ∇pe + e2 n2 η(ui − ue ) = 0 (a) From the θ̂ components of these equations, show that uir = uer . Past examthe papers (b) From r̂ components, show that ujθ = uE + uDj (j = i, e). (c) Find an expression for uir showing that it does not depend on E. Question 3 The induced emf at the terminals of a wire loop that encircles a plasma measures the rate of change of magnetic ﬂux expelled by the plasma. You are given the following parameters: Vacuum magnetic ﬁeld strength - 1 Tesla Number of turns on the diamagnetic loop - N = 75 Radius of the loop - aL = 0.075m Plasma radius - a = .05m. Given the observed diamagnetic ﬂux loop signal shown below, calculate the plasma pressure as a function of time. If the temperature of the plasma is constant at 1 keV, what is the plasma density as a function of time? (HINT: use Faraday’s law relating the emf to the time derivative of the magnetic ﬂux) Volts 1.0 12 2 4 6 8 14 16 10 Time (µs) -1.0 Figure 10.2: Magnetic ﬂux loop signal as a function of time. Question 4 An inﬁnite straight wire carries a constant current I in the +z direction. At t = 0 an electron of small gyroradius is at z = 0 and r = r0 with v⊥0 = v0 (⊥ and refer to the direction relative to the magnetic ﬁeld.) (a) Calculate the magnitude and direction of the resulting guiding centre drift velocity. (b) Suppose the current increases slowly in time in such a way that a constant electric ﬁeld is induced in the ±z direction. Indicate on a diagram the relative directions of I, E, B and vE . (c) Do v⊥ and v increase, decrease or remain the same as the current increases? Explain your answer. Question 5 Magnetic pumping is a means of heating plasmas that is based on the constancy of the magnetic moment µ. Consider a magnetized plasma for which the magnetic ﬁeld strength is modulated in time according to (10.12) B = B0 (1 + cos ωt) 2 where ω ωc and 1. If U⊥ = mv⊥ /2 = (mvx2 + mvy2 )/2 is the particle perpendicular kinetic energy (electrons or ions) show that the kinetic energy is also modulated as U⊥ dB dU⊥ = . dt B dt We now allow for a collisional relaxation between the perpendicular (U⊥ ) and parallel (U ) kinetic energies modelled according to the coupled equations U⊥ dB U⊥ dU⊥ = −ν − U dt B dt 2 dU U⊥ = ν − U dt 2 where ν is the collision frequency. By suitably combining these equations, one can calculate the increment ∆U in total kinetic energy during a period ∆t = 2π/ω to obtain a nett heating rate ∆U 2 ω2ν U ≡ αU. = ∆t 6 9ν 2 /4 + ω 2 (10.13) This heating scheme is called collisional magnetic pumping. Comment on the physical reasons for the ν-dependence of α in the cases ω ν and ω ν. Assuming that the plasma is fully ionized (Coulomb collisions), and in the case ω ν, show that the heating rate ∆U/∆t decreases as the temperature increases. What would happen if the magnetic ﬁeld were oscillating at frequency ω = ωc ? Question 6 On a graph of wave frequency ω versus wavenumber k show the dispersion relations for the ion and electron acoustic waves, and a transverse electromagnetic wave (ω > ωpe ) propagating in an unmagnetized plasma. (HINT: Draw the ion and electron plasma frequencies and lines corresponding to the electron sound speed, the ion sound speed and the speed of light.) Past exam papers Consider the case of electron plasma oscillations in a uniform plasma of density n0 in the presence of a uniform steady magnetic ﬁeld B 0 = B0 k̂. We take the background electric ﬁeld to be zero (E 0 = 0) and assume the plasma is at rest u = 0. We shall consider longitudinal electron oscillations having k E 1 where we take the oscillating electric ﬁeld perturbation associated with the electron wave E 1 ≡ E î to be parallel to the x-axis. Replacing time derivatives by −iω and spatial gradients by ik, and ignoring pressure gradients and the convective term (u.∇)u, show that for small amplitude perturbations, the electron motion is governed by the linearized mass and momentum conservation equations and Maxwell’s equation: −iωn1 + n0 ikux = 0 −iωu = −e(E + u×B 0 ) ε0 ikE = −en1 . (10.14) (10.15) (10.16) Use Eq. (10.15) to show that the x component of the electron motion is given by ux = eE/iωm 1 − ωc2 /ω 2 (10.17) Substituting for ux from the continuity equation and eliminating the density perturbation using Eq. (10.16), obtain the dispersion relation for the longitudinal electron plasma oscillation transverse to B: (10.18) ω 2 = ωp2 + ωc2 . Why is the oscillation frequency greater than ωp ? By expressing the ratio ux /uy in terms of ω and ωc show that the electron trajectory is an ellipse elongated in the x direction. THE AUSTRALIAN NATIONAL UNIVERSITY First Semester Examination 2002 PHYSICS C17 PLASMA PHYSICS Writing period 2 hours duration Study period 15 minutes duration Permitted materials: Calculators Attempt four questions. All are of equal value. Show all working and state and justify relevant assumptions. Question 1 Discuss, using diagrams where appropriate, three of the following issues. Answers for each should require at most half a page. (a) Ambipolar diﬀusion in unmagnetized plasma. (b) Electric breakdown. Why is E/p important and what is the role of secondary emission? (c) The physics underlying the Boltzmann relation. (d) MHD waves that propagate perpendicular and parallel to B. (e) The resistivity of weakly and fully ionized unmagnetized plasmas. (f) Magnetic mirrors and the role of the invariance of the orbital magnetic moment µ. (g) Debye shielding and the relationship between the plasma frequency and Debye length. Question 2 (a) Explain using a diagram why the orbit of a particle gyrating in a magnetic ﬁeld is diamagnetic. (b) Given that the magnetic moment of a gyrating particle is µ=W⊥ /B where W⊥ is the kinetic energy of the motion perpendicular to the magnetic ﬁeld of strength B, ﬁnd an expression for the magnetic moment per unit volume M in a plasma with particle density n and temperature T immersed in a uniform magnetic ﬁeld. (c) Supposing the ﬁeld inside the plasma to be reduced compared with that outside the plasma B by µ0 M B, calculate the diﬀerence in magnetic pressure B 2 /2µ0 inside the plasma and conﬁrm that the total pressure is constant. Past exam papers (d) Describe in general terms what happens to maintain pressure balance as the plasma temperature is increased, keeping the total number of particles constant. Question 3 (a) With the aid of diagrams, explain why magnetic plasma conﬁnement is not possible in a purely toroidal magnetic ﬁeld. (b) The earth’s magnetic ﬁeld may be approximated as a magnetic dipole out to a few earth radii (RE = 6370km). The magnetic ﬁeld for a dipole can be written approximately as µ0 2M cos θ 4π r3 µ0 M sin θ = 4π r3 Br = (10.19) Bθ (10.20) where θ is the polar angle from the direction of the dipole moment vector, Br is the magnetic ﬁeld radial component and Bθ is the component orthogonal to Br . Using the fact that, at one of the magnetic poles (r = RE ) , the ﬁeld has a magnitude of 0.5 Gauss, calculate the earth’s dipole moment M . (c) Assuming an electron is constrained to move in the earth’s magnetic equatorial plane (v = 0), calculate the guiding centre drift velocity, and determine the time it takes to drift once around the earth at a radial distance r0 . What is the direction of drift. (d) Let there be an isotropic population of 1 eV protons and 30 keV electrons each with density n = 107 m−3 at r = 5RE in the equatorial plane. Compute the ring current density in A/m2 associated with the drift obtained in (c). (e) Now assume that the perpendicular kinetic energy equals the parallel kinetic energy at the magnetic equatorial plane. Qualitatively describe the motion of the electron guiding centre. Question 4 (a) Using the steady-state force balance equation (ignore the convective derivative) show that the particle ﬂux Γ = nu for electrons and singly charged ions in an unmagnetized plasma is given by: Γj = nuj = ±µj nE − Dj ∇n with mobility µ =| q | /mν where ν is the collision frequency and diﬀusion coeﬃcient D = kB T /mν. (b) Show that the diﬀusion coeﬃcient can be expressed as D ∼ λ2mfp /τ where λmfp is the mean free path between collisions and τ is the collision time. (c) Show that the plasma resistivity is given approximately by η = me ν/ne2 . (d) In a weakly ionized magnetoplasma, the mean perpendicular velocity of particles across the ﬁeld is given by uE + uD ∇n u⊥ = ±µ⊥ E − D⊥ + n 1 + ν 2 /ωc2 with uE = E×B/B 2 , uD = −∇p×B/qnB 2 and where µ⊥ = µ/(1 + ωc2 τ 2 ) and D⊥ = D/(1 + ωc2 τ 2 ). Discuss the physical origin of each of these terms and their behaviour in the limit of weak and strong magnetic ﬁelds. Question 5 (10 marks) The dispersion relation for low frequency magnetohydrodynamic waves in a magnetized plasma was derived in lectures as −ω 2 u1 + (VS2 + VA2 )(k.u1 )k + (k.V A )[(k.V A )u1 − (V A .u1 )k − (k.u1 )V A ] = 0 where u1 is the perturbed ﬂuid velocity, k is the propagataion wavevector and V A = B 0 /(µ0 ρ0 )1/2 is a velocity vector in the direction of the magnetic ﬁeld with magnitude equal to the Alfvén speed and VS is the sound speed. (a) Deduce the dispersion relations for waves propagating parallel to the magnetic ﬁeld and identify the wave modes. (b) Using ∂B 1 − ∇×(u1 ×B 0 ) = 0 ∂t E 1 + u1 ×B = 0 ∂ → −iω and ∇× → ik×, make a sketch and assuming plane wave propagation so that ∂t showing the relation between the perturbed quantities u1 , E 1 , B 1 and k and B 0 for the transverse wave propagating along B 0 . Question 6 (10 marks) Consider an electromagnetic wave propagating in an unbounded, em unmagnetized uniform plasma of equilibrium density n0 . We assume the bulk plasma velocity is zero (v 0 = 0) but allow small drifts v1 to be induced by the one-dimensional harmonic electric ﬁeld perturbation E = E1 exp [i(kx − ωt)] that is transverse to the wave propagation direction. (a) Assuming the plasma is also cold (∇p = 0) and collisionless, show that the momentum equations for electrons and ions give n0 mi (−iωvi1 ) = n0 eE1 n0 me (−iωve1 ) = −n0 eE1 (b) The ion motions are small and can be neglected. Show that the resulting current density ﬂowing in the plasma due to the imposed oscillating wave electric ﬁeld is given by j1 = en0 (vi1 − ve1 ) ≈ i n0 e2 E1 . me ω (10.21) Past exam papers (c) Associated with the ﬂuctuating current is a small magnetic ﬁeld oscillation which is given by Ampere’s law. Use the diﬀerential forms of Faraday’s law and Ampere’s law (Maxwell’s equations) to obtain the ﬁrst order equations kE1 = ωB1 and ikB1 = µ0 j1 − iωµ0 ε0 E1 linking B1 , E1 and j1 . (d) Use these relations to eliminate B1 and j1 to obtain the dispersion relation for plane electromagnetic waves propagating in a plasma: k2 = 2 ω 2 − ωpe c2 (10.22) (d) Sketch the dispersion relation and comment on the physical signiﬁcance of the dispersion near the region ω = ωpe . APPENDIX: A Glossary of Useful Formulae Chapter 1: Basic plasma phenomena ωpe = e2 ne ε0 m e λD = ε0 kB Te ne e2 3 ni Te2 −Ui exp 2.4 × ×1021 n ni kB T √ fpe 9 ne ( Hz) Chapter 2: Kinetic theory ∂f q +v.∇r .f + (E +v×B).∇v .f = ∂t m ∂f ∂t eφ ne = ne0 exp kB Te coll Γ = nv̄ λmfp = j = qnv̄ 2 p = nŪr 3 −mv 2 2 fM (v) = A exp( ) ) = A exp (−v 2 /vth 2kB T 1 Ūr (Maxwellian) ≡ EAv = kB T (1 − D) 2 1 eV 11, 600 K vrms = 3kB T m 2kB T m pj = nj kB Tj 1 nσ λmfp v ν = nσv 2qq0 b0 = 4πε0 mv 2 λD ln Λ = ln b0 τ= ei σcoulomb Z 2 e4 ln Λ 2πε20 m2e ve4 δEei ∼ vth = Pei = − 4Ee me mi me ne (ue − ui ) τei Chapter 2: Fluid and Maxwell’s equations σ = ni q i + n e q e j = ni qi ui + ne qe ue ∂nj + ∇.(nj uj ) = 0 ∂t ∂uj + (uj .∇)uj = qj nj (E + uj ×B) − ∇pj + Pcoll m j nj ∂t γ pj = Cj nj j σ ∇.E = ε0 ∂B ∇×E = − ∂t ∇.B = 0 Past exam papers ∇×B = µ0 j + µ0 ε0 ∂E ∂t Chapter 3: Gaseous Electronics Γj = nuj = ±µj nE − Dj ∇n |q | µ= mν kB T D= mν E = ηj νei me η= ne e2 √ Ze2 me ln Λ η √ 6 3πε20 (kB Te )3/2 5.2 × 10−5 Z ln Λ η = 3 2 Te(eV) I= 4 J= 9 I0 eαx (1 − γeαx ) 2e ε0 |φw |3/2 mi d2 uBohm = kB Te mi eφw 2πme 1 ≈ ln kB Te 2 mi 1 kB Te Isi n0 eA 2 mi Chapter 4: Single Particle Motions dv = q(E + v×B) dt |q|B ωc ≡ m v⊥ rL = ωc 2 mv⊥ µ= 2B E×B vE = B2 1 F ×B vF = q B2 mv2 Rc ×B vR = qB 2 R2 1 B×∇B v ∇B = ± v⊥ rL 2 B2 1 Ė vP = ωc B ↔ j =σ E F =m F = −µ∇ B 2 (K − µB) v = m 1/2 1 Bm = B0 sin2 θm q(r) = ↔ σ e= ine2 me ω ↔ dφ B0 rB0 = = dθ RBθ Bθ ω2 2 ω 2 − ωce iωce ω 2 2 ω − ωce 0 ε = ε0 −iωce ω 0 2 ω 2 − ωce 2 ω 0 2 ω 2 − ωce 0 1 ↔ i ↔ I + σ ε0 ω Chapter 5: Magnetized Plasmas u⊥ = E×B −∇p×B + B2 qnB 2 j D = (kB Ti + kB Te ) B×∇n B2 uE + uD ∇n + n 1 + ν 2 /ωc2 µ µ⊥ = 1 + ωc2 τ 2 u⊥ = ±µ⊥ E − D⊥ D⊥ = D 1 + ωc2 τ 2 ν2 ν 2 + ωc2 ∓νωc = σ0 2 ν + ωc2 ne2 = σ0 = mν σ⊥ = σ0 σH σ σ⊥ −σH 0 ↔ 0 σ= σH σ⊥ 0 0 σ D⊥ = η⊥ ns kB Ts B2 Chapter 5: Single Fluid Equations ∂u ∂t E + u×B ∂ρ + ∇.(ρu) ∂t ∂σ + ∇.j ∂t ρ = j×B − ∇p + ρg = ηj = 0 = 0 ∂B ∂t ∇×B = µ0 j p = Cnγ ∇×E = − Chapter 6: Magnetohydrodynamics B2 1 ∇ p+ = (B.∇)B 2µ0 µ0 η ∂B = ∇2 B + ∇×(u×B) ∂t µ0 RM = µ0 vL η Chapter 7, 8, 9: Waves vg = VA = B2 µ0 ρ ↔ dω dk n×(n×E)+ K .E = 0 /2 n= 1/2 γe kB Te + γi kB Ti VS = mi ω c vφ = = 2 k (1 − ωpe /ω 2 )1/2 2 ω 2 = ωpe + 3kB T 2 k m c k ω n =| n |= ck/ω = c/vφ S −iD 0 ↔ ↔ 0 K= /ε0 = iD S 0 0 P Past exam papers S = 1− i,e D = ± i,e P = 1− ωp2 ωc ω(ω 2 − ωc2 ) ωp2 i,e R L S D P ωp2 ω 2 − ωc2 ω2 = = = = S+D Right S−D Left (R + L)/2 Sum (R − L)/2 Diﬀ Plasma 2 P (n − L)(n2 − R) tan2 θ = 2 (n − P )(RL − n2 S) c2 vφ2 L =1− R 2 2 ωpi ωpe − ω(ω ± ωce ) ω(ω ∓ ωci ) 2 2 1/2 + 4ωpe ) /2 ω0L = −ωce + (ωce 2 2 1/2 + 4ωpe ) /2 ω0R = ωce + (ωce 2 2 c2 (ω 2 − ω0L )(ω 2 − ω0R ) n = 2 = vφ ω 2 (ω 2 − ωU2 H ) 2 2 2 1/2 ωU H = (ωpe + ωce ) ωLH ≈ (ωci ωce )1/2 n2 = 2 2 c2 (ω 2 − ω0L )(ω 2 − ω0R ) = 2 2 2 2 vφ ω (ω − ωU H ) Useful Mathematical Identities A.(B×C) = B.(C×A) = C.(A×B) (A×B)×C = B(C.A) − A(C.B) ∇.(φA) = A.∇φ + φ∇.A ∇×(φA) = ∇φ×A + φ∇×A A×(∇×B) = ∇(A.B) − (A.∇)B − (B.∇)A − B×(∇×A) 1 (A.∇)A = ∇( A2 ) − A×(∇×A) 2 ∇.(A×B) = B.(∇×A) − A.(∇×B) ∇×(A×B) = A(∇.B) − B(∇.A) + (B.∇)A − (A.∇)B ∇×(∇×A) = ∇(∇.A) − (∇.∇)A ∇×∇φ = 0 ∇.(∇×A) = 0 ∞ 1 v exp (−av )dv = 2 −∞ 2 2 π a3 Cylindrical coordinates ∇φ = ∂φ 1 ∂φ ∂φ r̂ + θ̂ + ẑ ∂r r ∂θ ∂z 1 ∂ ∂φ 1 ∂2φ ∂2φ r + 2 2 + 2 ∇ φ= r ∂r ∂r r ∂θ ∂z 2 ∇.A = 1 ∂ 1 ∂Aθ ∂Az (rAr ) + + r ∂r r ∂θ ∂z 1 ∂Az ∂Aθ ∂Ar ∂Az r̂ + ∇×A = − − r ∂θ ∂z ∂z ∂r 1 ∂Ar 1 ∂ + (rAθ ) − ẑ r ∂r r ∂θ Bibliography [1] R. D. Hazeltine and F. L. Waelbroeck, The Framework of Plasma Physics (Perseus Books, Reading, Massachusetts, 1998). [2] D. J. ROSE and M. CLARK, Plasmas and Controlled Fusion (John Wiley and Sons, New York, 1961). [3] J. A. ELLIOT, in Plasma Physics - An Introductory Course, edited by R. O. DENDY (Press Syndicate of the University of Cambridge, Cambridge, 1993), pp. 29–53. [4] F. F. CHEN, Introduction to Plasma Physics and Controlled Fusion (Plenum Press, New York, 1984), Vol. 1. [5] C. L. HEMENWAY, R. W. HENRY, and M. CAULTON, Physical Electronics (Wiley International, New York, 1967). [6] G. BEKEFI, Radiation Processes in Plasmas (John Wiley and Sons, New York, 1966). [7] J. A. BITTENCOURT, Fundamentals of Plasma Physics (Pergamon Press, New York, 1986). List of Figures 1.1 1.2 1.3 1.4 1.5 The electric ﬁeld applied between electrodes inserted into a plasma is screened by free charge carriers in the plasma. . . . . . . . . . . . . . . . . . . . . . . . . . . Electric ﬁeld generated by a line of charge . . . . . . . . . . . . . . . . . . . . . The ﬁgure shows regions of unbalanced charge and the resulting electric ﬁeld proﬁle that results. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Principle of the Mach Zehnder interferometer . . . . . . . . . . . . . . . . . . . Curve showing the dependence of the fractional ionization of a hydrogen (Ui =13.6 eV) as a function of temperature and number density. . . . . . . . . . . . . . . . . 8 . 10 . 11 . 12 . 14 1.6 Unless alternatives can be found, a serious shortfall in expendable energy reserves will be apparent by the middle of the next century. (reproduced from http://FusEdWeb.pppl.gov/) 1.7 The terrestrial fusion reaction is based on the fusion of deuterium and tritium with the release of a fast neutron and an alpha particle. (reproduced from http://FusEdWeb.pppl.gov/) 1.8 Comaprison of fuel needs and waste by-products for 1GW coal fired and fusion power plants. (reproduced from http://FusEdWeb.pppl.gov/) . . . . . . . . . . . . . . . . 18 The principal means for confining hot plasma are gravity (the sun), inertia (laser fusion) and using electric and magnetic fields (magnetic fusion). (reproduced from http://FusEdWeb.pppl.gov/ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 16 17 1.9 1.10 H-1NF. (a) Artist’s impression (the plasma is shown in red), (b) during construction and (c) coil support structure. . . . . . . . . . . . . . . . . . . . . . . . . . . 1.11 Computed magnetic surfaces (left) and surfaces measured using electron gun and fluorescent screen (right). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.12 Joint European Torus (JET) tokamak. (a) CAD view and (b) inside the vacuum vessel. From JET promotional material. . . . . . . . . . . . . . . . . . . . . . . . 1.13 Large Helical Device (LHD) heliotron. . . . . . . . . . . . . . . . . . . . . . . . . 1.14 Coil system and vacuum vessel for the Wendelstein 7-X (W 7-X) modular helias. . 1.15 Coil system and plasma of the H-1NF ﬂexible heliac. Key: PFC: poloidal ﬁeld coil, HCW: helical control winding, TFC: toroidal ﬁeld coil, VFC: vertical ﬁeld coil. 1.16 Plasma and coil system for the Heliotron-E torsatron. . . . . . . . . . . . . . . . . 2.1 2.2 2.3 2.4 Left: A conﬁguration space volume element dr = dxdydz at spatial position r. Right: The equivalent velocity space element. Together these two elements constitute a volume element dV = drdv at position (r, v) in phase space. . . . . Evolution of phase space volume element under collisions . . . . . . . . . . . . . Examples of velocity distribution functions . . . . . . . . . . . . . . . . . . . . . Imaginary box containing plasma at temperature T . . . . . . . . . . . . . . . . . . . . 21 22 25 26 26 27 27 30 33 36 39 2.5 Electrostatic Coulomb potential and Debye potential as a function of distance from a test charge Q. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.6 The contributions (i) and (ii) noted in the text [3] . . . . . . . . . . . . . . . . . 2.7 Diagram showing the electron potential energy −eφ in an electron plasma wave. Regions labelled A accelerate the electron while in B, the electron is decelerated [3]. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.8 Particles moving from the left and impinging on a gas undergo collisions. . . . . 2.9 The trajectory taken by an electron as it makes a glancing impact with a massive test charge Q . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2.10 Collison between ion and electron in centre of mass frame. . . . . . . . . . . . . 2.11 The electron impact ionization cross-section for hydrogen as a function of electron energy. Note the turn-on at 13.6 eV. [2] . . . . . . . . . . . . . . . . . . . . . . . 2.12 Electron secondary emission for normal incidence on a typical metal surface [2] 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 3.9 3.10 3.11 3.12 3.13 3.14 4.1 4.2 4.3 4.4 Illustrating the Boltzmann relation. Because of the pressure gradient, fast mobile electrons move away, leaving ions behind. The nett positive charge generates an electric ﬁeld. The force F e opposes the pressure gardient force F p .[4] . . . . . . Schematic diagram showing plasma in a container of length 2L with particle density vanishing at the wall. [4] . . . . . . . . . . . . . . . . . . . . . . . . . . . . High spatial frequency features are quickly washed out by diﬀusion as the plasma density relaxes towards its lowest order proﬁle.[4] . . . . . . . . . . . . . . . . . Elastic collision cross-section of electrons in Ne, A, Kr and Xe.[2] . . . . . . . . Drift velocity of electrons in hydrogen and deuterium.[2] . . . . . . . . . . . . . The ionization coeﬃcient α/p for hydrogen. Note the exponential behaviour.[2] . An electron avalanche as a function of time.[5] . . . . . . . . . . . . . . . . . . . (a) Paschen’s curve showing breakdown voltage as a function of the product pd. (b) A plot of plasma current versus applied voltage. Note the dramatic increase at the onset of breakdown. [5] . . . . . . . . . . . . . . . . . . . . . . . . . . . . (a) The plasma potential distribution for a plasma conﬁned electrostatically and (b) the corresponding density distribution of ions and electrons. The ion density is higher than electrons near the wall due to the negative electric ﬁeld established there by the escaping electron ﬂux. . . . . . . . . . . . . . . . . . . . . . . . . . The structure of the potential distribution near the plasma boundary. . . . . . Potential variation in the wall edge of the sheath compared with that for uniform and point like charge distributions. . . . . . . . . . . . . . . . . . . . . . . . . . Schematic diagram showing the potential drops around the plasma circuit. . . . The Langmuir probe I − V characteristic showing the electron and ion contributions and the plasma. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . The circuit shows the typical measurement arrangement using Langmuir probes. The probe bias is adjusted using the variable resistor. . . . . . . . . . . . . . . . Electrons and ions spiral about the lines of force. The ions are left-handed and electrons right. The magnetic ﬁeld is taken out of the page . . . . . . . . . . . . When immersed in orthogonal electric and magnetic ﬁelds, electrons and ions drift in the same direction and at the same velocity. . . . . . . . . . . . . . . . . . . . The orbit in 3-D for a charged particle in uniform electric and magnetic ﬁelds. . The cylindrical plasma rotates azimuthally as a result of the radial electric and axial magnetic ﬁelds. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44 . 46 . 48 . 50 . 51 . 53 . 56 . 57 . 66 . 70 . . . . . 73 74 75 76 77 . 77 . 78 . 80 . 82 . 84 . 85 . 86 . 90 . 91 . 93 . 94 LIST FIGURES 4.5 OF When the electric ﬁeld is changed at time t = 0, ions and electrons suﬀer an additional displacement as shown. The eﬀect is opposite for each species. . . . . . 94 4.6 The decomposition of E ⊥ into left and right handed components. . . . . . . . . . 97 4.7 When the magnetic ﬁeld changes in time, the induced electric ﬁeld does work on the cyclotron orbit. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102 4.8 The grad B drift is caused by the spatial inhomogeneity of B. It is in opposite directions for electrons and ions but of same magnitude. . . . . . . . . . . . . . . 103 4.9 The curvature drift arises due to the bending of lines of force. Again this force depends on the sign of the charge. . . . . . . . . . . . . . . . . . . . . . . . . . . . 105 4.10 The grad B drift for a cylindrical ﬁeld. . . . . . . . . . . . . . . . . . . . . . . . . 106 4.11 Schematic diagram showing lines of force in a magnetic mirror device. . . . . . . . 106 4.12 Top:The ﬂux linked by the particle orbit remains constant as the particle moves into regions of higher ﬁeld. The particle is reﬂected at the point where v = 0. Bottom: Showing plasma conﬁned by magnetic mirror . . . . . . . . . . . . . . . 109 4.13 Particles having velocities in the loss cone are preferentially lost . . . . . . . . . . 110 4.14 The grad B drift separates vertically the electrons and ions. The resulting electric ﬁeld and E/B drift pushes the plasma outwards. . . . . . . . . . . . . . . . . . . . 111 4.15 A helical twist (rotational transform) of the toroidal lines of force is introduced with the induction of toroidal current in the tokamak. Electrons follow the magnetic lines toroidally and short out the charge separation caused by the grad B drift. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111 4.16 Diagram showing toridal magnetic geometry . . . . . . . . . . . . . . . . . . . . . 112 4.17 Top: Schematic diagram of trajectory of “banana orbit” in a tokamak ﬁeld. Bottom: The projection of passing and banana-trapped orbits onto the poloidal plane. 116 5.1 5.2 5.3 5.4 5.5 6.1 6.2 6.3 Left: Diamagnetic current ﬂow in a plasma cylinder. Right: more ions moving downwards than upwards gives rise to a ﬂuid drift perpendicular to both the density gradient and B. However, the guiding centres remain stationary. . . . . Schematic showing the parallel and perpendicular electron and ion ﬂuxes for a magnetized plasma . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Top: The directions of current ﬂow and their associated conductivities in a weaklyionized magnetoplasma. Bottom: The collision frequency dependence of the perpendicular conductivty. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Left: Schematic showing particle displacements in direct Coulomb collisions between like species in a magnetized plasma. Right: Collisons between unlike particles eﬀectively displace guiding centres. . . . . . . . . . . . . . . . . . . . . . . . The theoretical perpendicular diﬀusion coeﬃcient versus collision frequency for a tokamak. The region of enhanced diﬀusion occurs in the so called ”plateau” regime centered about the particle bounce frequency in the magnetic mirrors. . . . 121 . 124 . 126 . 131 . 132 In a cylindrical magnetized plasma column, the pressure gradient is supported by the diamagnetic current j. In time, however, the gradient is dissipated through radial diﬀusion u⊥ = ur . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 136 In a tokamak, the equilibrium current density and magnetic ﬁeld lie in nested surfaces of constant pressure. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 136 The plasma thermal pressure gradient is exactly balanced by a radial variation in the magnetic pressure. This variation is generated by diamagnetic currents that ﬂow azimuthally. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138 6.4 6.5 6.6 6.7 6.8 6.9 7.1 7.2 7.3 7.4 7.5 7.6 7.7 7.8 8.1 8.2 8.3 8.4 9.1 9.2 9.3 9.4 9.5 The magnetic lines of force for wires carrying parallel currents. . . . . . . . . . . The geometric interpretation of the magnetic tension due to curvature of lines of force. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . An unmagnetized linear pinch showing sausage instability. . . . . . . . . . . . . The kinking of a plasma column under magnetic forces. . . . . . . . . . . . . . . Left:The ﬂux through surface S as it is convected with plasma velocity u remains constant in time. Right: showing the area element dA swept out by the plasma motion. Note that this area vanishes when u is parallel to the circumferential element d. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Showing the process of magnetic reconnection. . . . . . . . . . . . . . . . . . . . The phase and group velocities of a wave can be determined from its dispersion relation. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Torisonal Alfvén waves in a compressible conducting MHD ﬂuid propagating along the lines of force. The ﬂuid motion and magnetic perturbations are normal to the ﬁeld lines. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Longitudinal sound waves propagate along the magnetic ﬁeld lines in a compressible conducting magnetoﬂuid. . . . . . . . . . . . . . . . . . . . . . . . . . . . . The magnetoacoustic wave propagates perpendicularly to B compressing and releasing both the lines of force and the conducting ﬂuid which is tied to the ﬁeld. The perturbed components associated with the compressional magnetoacoustic wave propagating perpendicular to B 0 . . . . . . . . . . . . . . . . . . . . . . . The perturbed components associated with the torsional or shear wave propagating along B 0 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . The perturbed components associated with the torsional wave in a cylindrical plasma column . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Wave normal diagrams for the fast, slow and pure Alfvén waves for (a) VA > VS and (b) VA < VS . The length of the radius from the origin to a point on the associated closed curve is proportional to the wave phase velocity . . . . . . . . The longitudinal and transverse electric ﬁeld perturbations for waves in a cold electron plasma are decoupled . . . . . . . . . . . . . . . . . . . . . . . . . . . . Phase velocity versus oscillation frequency for the transverse electron plasma wave. Note reciprocal behaviour of vg and vφ and the region of nonpropagation. . . . . The form of the complex wavenumber for transverse electron plasma waves. . . . Dispersion relations for the three wave modes supported in an isotropic (unmagnetized) warm plasma. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . The geometry for analysis of plane waves in cold magnetized plasma. . . . . . . (a) Near a cutoﬀ, the wave ﬁeld swells, the wavelength increases and the wave is ultimately reﬂected. (b) near a resonance, the waveﬁeld diminishes, the wavelength decreases and the wave enrgy is absorbed. . . . . . . . . . . . . . . . . . . . . . A plot of wave phase velocity versus frequency for waves propagating parallel to the magnetic ﬁeld for a cold plasma. . . . . . . . . . . . . . . . . . . . . . . . . The principle of Faraday rotation for an initially plane polarized wave propagating parallel to the magnetic ﬁeld. . . . . . . . . . . . . . . . . . . . . . . . . . . . . The ordinary wave is a transverse electromagnetic wave having its electric vector parallel to B. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138 . 139 . 140 . 140 . 142 . 145 . 149 . 151 . 152 . 153 . 156 . 157 . 157 . 159 . 162 . 164 . 165 . 168 . 172 . 175 . 176 . 177 . 178 LIST FIGURES 9.6 OF The relationship between the propagation vector, magnetic ﬁeld and wave components for the extraordinary wave. The wave exhibits an electric ﬁeld in the direction of motion and so is partly electrostatic in character. . . . . . . . . . . . . 179 9.7 A plot of wave phase velocity versus frequency for waves propagating perpendicular to the magnetic ﬁeld for a cold plasma. . . . . . . . . . . . . . . . . . . . . . . . . 181 10.1 Conductors marked with a cross carry current into the page (z direction), while the dots indicate current out of the page. . . . . . . . . . . . . . . . . . . . . . . . 205 10.2 Magnetic ﬂux loop signal as a function of time. . . . . . . . . . . . . . . . . . . . 209 Index adiabatic changes, 58 adiabatic invariants, 85 ambipolar diﬀusion coeﬃcient, 69 ambipolar electric ﬁeld, 68 anomalous diﬀusion, 129 average velocity, 32 banana orbit, 113 Bohm diﬀusion coeﬃcient, 129 Bohm sheath criterion, 79 Bohm speed, 79 Bohm-Gross dispersion relation, 44 Boltzmann factor, 77 relation, 64 Boltzmann factor, 40 Boltzmann relation, 39 breakdown, 71–75 Child-Langmuir Law, 80 collision frequency, 48 collision time, 48 collisions, 47–55 Coulomb, 48, 129 cross section, 48 electron-ion, 58 electron-neutral, 72 fusion, 52 mean free path, 47 conductivity tensor, 123 conductivity tensor, 97 conﬁguration space, 28 convective derivative, 30 Coulomb collisions, 48–52 force, 48 current density, 66 diamagnetic, 102, 118, 133 Hall, 128 ion saturation, 82 polarization, 93 current density, 33 cyclotron frequency, 15, 86 Debye length, 12 Debye shielding, 40 Debye shielding, 11 diamagnetic current, 117 diamagnetic drift, 118 diamagnetism, 87, 135 dielectric low frequency susceptibility, 93 susceptibility, 168 tensor, 124 dielectric tensor, 98 diﬀusion, 67–70 ambipolar, 121, 128 Fick’s law, 65, 128 fully ionized, magnetized, 128 neoclassical, 130 perpendicular, 120 resistive, 140–143 diﬀusion coeﬃcient, 65 dispersion electron plasma waves, 44 extraordinary wave, 175 ion acoustic wave, 154 left hand em wave, 172 magnetoacoustic wave, 152 ordinary wave, 175 right hand em wave, 172 torsional Alfvén wave, 154 dispersion relation Alfvén waves, 152 cold magnetized plasma, 171 distribution average, 32 distribution function, 28 electric sheath, 76, 80 INDEX electromagnetic waves, 145 electron plasma waves, 42 sound speed, 165 electron plasma frequency, 10 electron saturation current, 83 electrostatic waves, 145 equation of continuity, 56 equation of motion, 57 equation of state, 58 Faraday rotation, 175 ﬂuid equations, 32 generalized Ohm’s law, 127 group velocity, 147 guiding centre, 85 H-1 heliac, 16 Hall current, 122 heating ohmic, 67, 142 ideal MHD equations, 133 inelastic collisions, 47 interferometry, 11 ion saturation current, 82 ionization electron impact, 54 photo, 53 isothermal, 59 kink instability, 138 Landau damping, 42 Langmuir probes, 81–83 Larmor radius, 87 light scattering, 13, 52 Lorentz equation, 85 loss cone, 106 lower hybrid frequency, 178 magnetic diﬀusion, 140–143 dipole moment, 100 ﬂux, frozen-in, 140 islands, 143 mirror ratio, 106 pressure, 135 reconnection, 143 tension, 135 magnetic ﬂux surface, 18 magnetic mirrors, 104 magnetic Reynold’s number, 141 magnetohydrodynamics, 125 Maxwell-Boltzmann distribution, 35 mean free path, 48 mean speed, 38 mobility perpendicular, 120 mobility, 65 mobility tensor, 96 neoclassical diﬀusion, 113 nuclear fusion, 52 particle ﬂux, 33 particle number density, 32 Paschen’s law, 75 passing particles, 110 phase space, 28, 29 phase velocity, 146 phasor, 146 photo-ionization, 70 plasma approximation, 60 conﬁnement, 15 convection, 139 heating, 14 oscillations, 161 potential, 81 stability, 137, 143 plasma parameter, 9 plasma sound speed, 165 polarization left handed, 96 right handed, 96 polarization current, 91 Poynting ﬂux, 161 pre-sheath, 79 pressure, 37, 57 pressure tensor, 33 radiative recombination, 70 random particle ﬂux, 38 ratio of speciﬁc heats, 59, 164 recombination, 70 refractive index, 168 resistivity, 66 rms thermal speed, 34 rotational transform, 108, 111 safety factor, 111 Saha equation, 13 sausage instability, 138 secondary emission, 54 sheath, 76 single ﬂuid equations, 125, 127 speed mean v, 38 rms vrms , 34, 36 thermal vth , 35 stellarator, 111 Stellarators, 16 superposition, 146 thermal equilibrium, 29, 35 tokamak, 108 tokamak, 16 upper-hybrid frequency, 177 velocity drift curvature v R , 102 E/B v E , 90 Grad B v ∇B , 102 polarization v P , 93 toroidal, 107 group, 147 phase, 146 velocity moments, 32 velocity space, 28 Vlasov, 30 Vlasov equation, 42 wave Alfvén, 153 cutoﬀ, 162, 172 electron plasma, 42 extraordinary, 176 ion acoustic, 148, 153 left hand, 171 magnetoacoustic, 150, 152 ordinary, 176 resonance, 172 right hand, 171 sound, 148 torsional Alfvén, 148 Whistler, 174 wave normal, 156 wave:ion acoustic, 149 winding number, 111 zeroth order velocity moment, 32

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