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Almost-invariant surfaces for magnetic field-line flows

Published online by Cambridge University Press:  13 March 2009

S. R. Hudson
Affiliation:
Department of Theoretical Physics and Plasma Research Laboratory, Research School of Physical Sciences and Engineering, The Australian National University, Canberra ACT 0200, Australia†
R. L. Dewar
Affiliation:
Department of Theoretical Physics and Plasma Research Laboratory, Research School of Physical Sciences and Engineering, The Australian National University, Canberra ACT 0200, Australia†

Abstract

Two approaches to defining almost-invariant surfaces for magnetic fields with imperfect magnetic surfaces are compared. Both methods are based on treating magnetic field-line flow as a 1½-dimensional Hamiltonian (or Lagrangian) dynamical system. In the quadratic-flux minimizing surface approach, the integral of the square of the action gradient over the toroidal and poloidal angles is minimized, while in the ghost surface approach a gradient flow between a minimax and an action-minimizing orbit is used. In both cases the almost-invariant surface is constructed as a family of periodic pseudo-orbits, and consequently it has a rational rotational transform. The construction of quadratic-flux minimizing surfaces is simple, and easily implemented using a new magnetic field-line tracing method. The construction of ghost surfaces requires the representation of a pseudo field line as an (in principle) infinite-dimensional vector and also is inherently slow for systems near integrability. As a test problem the magnetic field-line Hamiltonian is constructed analytically for a topologically toroidal, non-integrable ABC-flow model, and both types of almost-invariant surface are constructed numerically.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1996

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References

REFERENCES

Angenent, S. & GoléC., 1991 Lamination by ghost circles. Technical Report, Forschungsinstitut für Mathematik, ETH, Zürich.Google Scholar
Arrowsmith, D.K. & Place, C.M. 1991 An Introduction to Dynamical Systems. Cambridge University Press.Google Scholar
Boozer, A.H. 1982 Establishment of magnetic coordinates for given magnetic field. Phys. Fluids 25, 520.CrossRefGoogle Scholar
Boozer, A.N. 1983 Evaluation of the structure of ergodic fields. Phys. Fluids 26, 1288.CrossRefGoogle Scholar
Cary, J.R. & Hanson, J.D. 1986 Stochasticity reduction. Phys. Fluids 29, 2464.CrossRefGoogle Scholar
Cary, J.R. & Littlejohn, R.G. 1983 Noncanonical Hamiltonian mechanics and its application to magnetic field line flow. Ann. Phys. (NY) 151, 1.CrossRefGoogle Scholar
Davidson, M.Dewar, R.L., Gardner, H.J. & Howard, J. 1995 Hamiltonian maps for Heliac magnetic islands. Aust. J. Phys. 48, 871.CrossRefGoogle Scholar
Dewar, R.L. & Khorev, A.B. 1995 Rational quadratic-flux minimizing circles for areapreserving twist maps. Physica D85, 66.Google Scholar
Dewar, R.L. & Meiss, J.D. 1992 Flux-minimizing curves for teversible area-preserving maps. Physica D57, 476.Google Scholar
Dewar, R.L., Hudson, S.R. & Price, P. 1994 Almost invariant manitbids for divergence free fields. Phys. Left. 194A, 49.CrossRefGoogle Scholar
D'haeseleer, W.D., Hitchon, W.N.G., Callen, J.D. & Shohet, J.L. 1983 Flux Coordinaics and Magnetic Field Structure. Springer-Verlag, Berlin.Google Scholar
Goldstein, H. 1980 Classical Mechanics, 2nd edn.Addison-Wesley, Reading, MA.Google Scholar
Golé, C. 1992 Partition by ghost circles. J. Differential Eqns 97, 140.CrossRefGoogle Scholar
Greene, J.M. 1979 A method for determining a stochastic transition. J. Math. Phys. 20, 1183.CrossRefGoogle Scholar
Greenside, H.S., Reiman, A.N., & Salas, A. 1989 Convergence properties of a nonvariational 3D MHD code. J. Comput. Phys. 81, 102.CrossRefGoogle Scholar
Hanson, J.D. 1994 Correcting small magnetic field non-axisymmetries. Nucl. Fusion 34, 441.CrossRefGoogle Scholar
Hanson, J.D. & Cary, J.R. 1984 Elimination of stochasticity in stellarators. Phys. Fluids 27, 767.CrossRefGoogle Scholar
Hayashi, T., Sato, T., Gardner, H.J. & Meiss, J.D. 1995 Evolution of magnetic islands in a Heliac. Phys. Plasmas 2, 752.CrossRefGoogle Scholar
Hirshman, S.P. & Betancourt, O. 1991 Preconditioned descent algorithm for rapid calculations of magnetohydrodynamic equilibria. J. Comput. Phys. 96, 99.CrossRefGoogle Scholar
Howard, J.E. & Humphreys, J. 1995 Nonmonotonic twist maps. Physica D80, 256.Google Scholar
Kaasalainen, M. & Binney, J. 1994 Construction of invariant tori and integrable Hamiltonians. Phys. Rev. Lett. 73, 2377.CrossRefGoogle ScholarPubMed
Lichtenberg, A.J. & Lieberman, M.A. 1992 Regular and Chaotic Dynamics, 2nd edn.Springer-Verlag, New York.CrossRefGoogle Scholar
MacKay, R.S. & Muldoon, M.R. 1993 Diffusing through spectres: ridge curves, ghost circles and a partition of phase space. Phys. Lett. 178A, 245.CrossRefGoogle Scholar
Meiss, J.D. 1992 Symplectic maps, variational principles and transport. Rev. Mod. Phys. 64, 362.CrossRefGoogle Scholar
Meiss, J.D. & Hazeltine, R.D. 1990 Canonical coordinates for guiding center particles. Phys. Fluids B2, 2563.CrossRefGoogle Scholar
Press, W. H., Flannery, B. P., Teukolsky, S. A., & Vetterling, W. T. 1983 Numerical Recipes in Fortran. Cambridge University Press.Google Scholar
Reiman, A. & Pomphrey, N. 1991 Computation of magnetic coordinates and action angle coordinates. J Comput. Phys. 94, 225.CrossRefGoogle Scholar
Yoshida, Z. 1994 A remark on the Hamiltonian form of the magnetic-field-line equations. Phys. Plasmas 1, 208.CrossRefGoogle Scholar