Low Beta Rigid Mode Stability Criterion for an Arbitrary Larmor Radius Plasma

Low Beta Rigid Mode Stability Criterion for an Arbitrary Larmor Radius Plasma

Low Beta Rigid Mode Stability Criterion for an Arbitrary Larmor Radius Plasma H. L. Berk and H. V. Wong Institute for Fusion Studies, The University o f Texas at Austin, Austin, Texas 78712 Z. Naturforsch. 42 a, 1208-1224 (1987); received May 25, 1987 Dedicated to Professor Dieter Pfirsch on his 60th Birthday The low beta flute axisymmetric dispersion relation for rigid displacement perturbation of plasma equilibria with arbitrary Larmor radius particles and field line radius of curvature large compared to the plasma radius is derived. The equilibrium particle orbits are characterized by two constants o f motion, energy and angular momentum, and a third adiabatic invariant derived from the rapid radial motion. The Vlasov equation is integrated, assuming that the mode frequency, axial “bounce” frequency, and particle drift frequency are small compared to the cyclotron frequency, and it is demonstrated that the plasma response to a rigid perturbation has a universal character independent of Larmor radius. As a result the interchange instability is the same as that predicted from conventional M H D theory. However, a new prediction, more optimistic than earlier work, is found for the low density threshold of systems like Migma, which are disc-shaped, that is, the axial extent Az is less than the radial extent r0. The stability criterion for negative field line curvature x 1 x\al^ 8 dh______ r ro ß/ 1 + 2 Z —--- j- Az co£jj where <ypj is the mean ion plasma frequency, £2, the ion cyclotron frequency,öh the hot particle to total ion particle ratio, x./r is the ratio of the field line curvature and the midplane radius, which in our model is treated as a constant over the entire plasma, ah is the Larmor radius of the 8 Az energetic species, Z is approximately given by an interpolation formula Z = —— I--- which Az Az I n r0 goes over to the correct limits if e ith e r-- > 1 o r --- 1. For Az/r0<^ 1, the stability criterion ''o r0 is determined by the total particle number. Whereas the older theory (Az/r0$> 1) predicted instability at about the densities achieved in actual M igm a experiments, the present theory (Az/r0 4 1) indicates that the experimental results are for plasmas with particle number below the interchange threshold. I. Introduction radius, for the response of an equilibrium con­ figuration to long wavelength rigid mode perturba­ Under a variety of conditions the linear response tions. The assumptions made in the calculation are of hot particles with arbitrary Larmor radius may that there is azimuthal symmetry in the equilib­ differ appreciably from the predictions of MHD rium, that the magnetic field curvature radius is theory [1-7]. There is a variety of concepts, such as large compared to the plasma radius and beta is astron [8, 9], Elmo Bumpy Torus [10], field reversedlow. Because of the last assumption, we shall neglect theta pinch [11], tokamaks containing hot particles the equilibrium induced magnetic fields and con­ [12], and Migma [13, 14] that hope to exploit suchsider only electrostatic perturbations. The self- an effect to achieve favorable containment. In this consistent description with equilibrium magnetic work we present a theory for arbitrary Larmor fields and electromagnetic perturbation will be reported in a later work, although preliminary results of the fully self-consistent calculation will be discussed in the summary. Reprint requests to Prof. Dr. H. L. Berk, Institute for Fusion Studies, The University of Texas, Austin, Texas The primary result of our calculation is that the 78712, USA. response to a rigid perturbation has a universal 0932-0784 / 87 / 1000-1208 $ 01.30/0. - Please order a reprint rather than making your own copy. Dieses Werk wurde im Jahr 2013 vom Verlag Zeitschrift für Naturforschung This work has been digitalized and published in 2013 by Verlag Zeitschrift in Zusammenarbeit mit der Max-Planck-Gesellschaft zur Förderung der für Naturforschung in cooperation with the Max Planck Society for the Wissenschaften e.V. digitalisiert und unter folgender Lizenz veröffentlicht: Advancement of Science under a Creative Commons Attribution Creative Commons Namensnennung 4.0 Lizenz. 4.0 International License. H. L. Berk and H. V. Wong • An Arbitrary Larmor Radius Plasma 1209 character [1, 15] independent of Larmor radius. As a discuss the consequences of the interchange instabil­ result the same interchange instability as predicted ity to the Migma concept. from conventional MHD theory is predicted. How­ In the summary we note that a rigid mode pertur­ ever, if the predicted M HD growth rate is less than bation can rigorously be chosen at sufficiently high the precessional frequency of the particles, stabiliza­ density. However, near the threshold density, the tion arises. Such stabilization can occur at low rigid mode eigenfunction cannot be rigorously densities,if the plasma frequency is appreciably less justified, and a modification of our threshold con­ than the ion cyclotron frequency [1] or if the ratio of ditions is to be expected. The method of obtaining hot particle density to cold particle density is the modification will be discussed elsewhere. sufficiently small [4], These stabilization mechan­ isms have been noted in small Larmor radius II. Equilibrium theories [1, 4], but we believe that this calculation is the first to rigorously demonstrate that the stability In cylindrically symmetric plasma equilibria criteria is independent of Larmor radius. where the current density J 0 is azimuthal, the The calculation is applied to the Migma con­ equilibrium vector potential A0 may be represented figuration, where the experimentally achieved in terms of the flux variable y/(r, z): equilibrium has an axial width, Lp, considerably less than the radial extent, Rp, which is of order two A0= if/VO Larmor radii. Because of the shape, the density where r, 0, z are the usual cylindrical coordinates. threshold for instability is shown to be larger by a The equilibrium magnetic field B is factor, Rp/Lp, than the case where Lp ^> R p, which is usually studied. The predicted particle number B = V(// x V#. ( 1) threshold is above the number of particles trapped The lines of force lie in surfaces of i// = constant and in the Migma experiment [14] and is therefore com­ 0 = constant. patible with experimental results, where the inter­ It is convenient to introduce a function /(r,z) so change mode has not been observed. that t//, 6, / form an othogonal set of curvilinear We expect the universality of the response of coordinates, where rigid modes to apply even in the finite beta fully electromagnetic case. Hence, if we apply known B = (2) results from small Larmor radius theory, we can so that / is determined by indicate the stability criteria for arbitrary beta. This 0/ rB2 n discussion will be given in the summary section. We V x B = - ; ee= 4 Joeee ■ also need to examine the validity of a rigid mode as oi// /. c an eigenfunction (see below). Note that The structure of the paper is as follows. In Sect. II 1 B Vi// = rB, |V0|=—, | Vzj =— . we discuss the equilibrium. In Sect. Ill we analyze r k the dispersion relation that is obtained for a rigid The equilibrium Hamiltonian for the particle displacement. The algebra needed to obtain the motion describing the particle dynamics in these formal response makes use of Hamiltonian pertur­ coordinates is bation theory. Use of a Hamiltonian formalism in the perturbation theory allows for a systematic analysis of complex configurations. Since we are ( 3 ) dealing with large orbits, and will need to find 2 M 2 Mr 2 M k ‘ adiabatic invariants in a non-conventional ordering, a Hamiltonian formalism is particularly useful [16]. where p v, pe, px are the particle momenta conjugate However, the details are somewhat involved, and as to (//, 0, /, and M the particle mass. The equations of a consequence we have included the algebraic motion are then as usual: reduction of the problem separately in Section IV. q j= dH /d p j, pi = — dH /d qj , In Sect. Ill the analysis of the electric field coupling for a disc-shaped plasma is presented. In Sect. V we qi=(if/,9,X), P i= (PV,P0 ,PX)- 1210 H. L. Berk and H. V. Wong • An Arbitrary Larmor Radius Plasma For example In this analysis we also treat x/r independent of position, which is a justified approximation if Bx (z) P¥ 6 . P e ~ ~ c y/ dr is quadratic in z2 and the mirror ratio sampled by p if/ r B + 2M dy/ M r: dij/ plasma particles is close to unity. P e - e-y III. Electrostatic m = 1 Flute Perturbation e d B 2 + - P\ c M r 2 2M dy/~? III. 1 General Description of Method of Solution We are interested in low beta mirror equilibrium of Dispersion Relation where the vacuum magnetic field may be approxi­ In order to describe the electrostatic dispersion mated by a near axis expansion of the vacuum field relation or the perturbed system, we examine the flux function yj\ structure of the variational quadratic form to the “2 response of a rigid displacement. This procedure uz = — Bo + B\ (z) — —3 —j B\(z) + ... can be justified as follows: Y 2 8 dr" (1) The electrostatic dispersion relation is valid Thus for the threshold of instability as it occurs at such low beta that magnetic perturbations, which B- — Bq + B\ — -—-—; B\ ... = B -- ---- r B primarily produce large positive energy perturba­ 4 dz 4 dz' tions, must be negligible in order to have instability. r d - (2) A symmetric quadratic form in the perturbed Br~~ 2 dz Bx' amplitude <p(r) = (p(y/, /) exp(/ / 9) and its adjoint <p+(r) = (p(y/, x) exp(— i 19) is known to exist, where The vacuum field curvature is the variation with respect to <p(y/, /) gives the exact r d 2 - Vy/ linear eigenmode equation [17-19].

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