DCON for SPEC - PPPL
Transcript of DCON for SPEC - PPPL
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 0
DCON for SPEC
Alan H. GlasserFusion Theory & Computation, Inc.
Presented atPrinceton Plasma Physics Laboratory
Princeton, NJ February 12, 2020
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 1
Ideal MHD Stability CriteriaØ Bernstein, Frieman, Kruskal & Kulsrud (1958) derived an ideal MHD potential energy
functional dW[x(x)]. They showed that a static equilibrium is unstable iff there is a perturbation x(x) that makes dW < 0.
Ø Newcomb (1960) applied this to a cylindrical plasma. He derived a 2nd-order Euler-Lagrange equation, (f x’)’ – g x = 0, and showed that there is a x(r) that makes dW < 0 iff the solution x(r) changes sign between singular points, where f = 0. This criterion is limited to fixed-boundary modes.
Ø PEST, ERATO, GATO, CAS3D, TERPSICHORE (1975++) expansion in basis functions, large matrix eigenvalue problem.
Ø Glasser (2016) generalized Newcomb’s criterion to axisymmetric toroidal plasmas, with x(r)replaced by a vector X(y) of complex Fourier coefficients of coupled poloidal harmonics mand a 2Mth order ODE. Implemented in the DCON code.
Ø A simple procedure extends this to free-boundary modes, with a vacuum region surrounding the plasma.
Ø The present work further generalizes this to a nonaxisymmetric plasma with stellarator symmetry, coupling multiple toroidal harmonics n = n0 + k*l, with l the number of stellarator field periods and k any integer. Formulated for SPEC equilibrium.
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 2
Stellarator Equilibrium CodesØ VMEC• Developed by Steve Hirshman et al, ORNL.• Imposes nested toroidal flux surfaces on equilibrium, not true energy minimum.• Radial finite differences equally space in toroidal magnetic flux.• Problems: very coarse near magnetic axis, fails to ensure div B = 0.
Ø SPEC• S.R. Hudson, R.L. Dewar et al., “Computation of multi-region relaxed
magnetohydrodynamic equilibria,” Phys. Plasmas 19, 112502 (2012).• Infinitesimal interfaces with finite pressure discontinuities,
[[p+B^2/2]] = 0, Bnormal = 0.• Volumes between interfaces where B may be stochastic.• All plasma confinement is localized to infinitesimal interfaces.• Radial discretization uses Chebyshev polynomials. • Regularization near coordinate axis.• Solves for vector potential A rather than magnetic field B, ensures div B = 0
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 3
SPEC Interfaces at Four Toroidal Locations
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 4
Outline of Stability Calculation, 1
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 5
Outline of Stability Calculation, 2
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 6
SPEC Equilibrium Description
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 7
Perturbations
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 8
Fourier Representation
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 9
Ideal MHD Energy Principle Volumes Between Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 10
Metric Tensor
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 11
Coefficient Matrices
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 12
Elimination of as
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 13
Euler-Lagrange Equation Volumes Between Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 14
Generalized Newcomb Criterion Volumes Between Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 15
Straight Fieldline CoordinatesLayers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 16
Transformation of Fourier Series
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 17
Equilibrium Magnetic Field Layers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 18
Equilibrium Current and Pressure Layers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 19
Perturbations Layers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 20
Fourier Representation and Ordering Assumptions
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 21
Current and Pressure Terms
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 22
Ideal MHD Energy PrincipleLayers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 23
Euler-Lagrange EquationLayers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 24
Coefficient Matrices
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 25
Generalized Newcomb Criterion Layers Inside Interfaces
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 26
Summary of Stability ProcedureØ Read equilibrium data.
Ø Compute Fourier expansion of metric tensor, fit to complex cubic splines.
Ø Compute coefficients of Euler-Lagrange equations in each interface and volume.
Ø Initialize in first volume near magnetic axis.
Ø Integrate Euler-Lagrange equations across each region, initializing from previous region.
Ø Monitor critical determinant DC(s), generalized Newcomb criterion; change of sign indicates fixed-boundary instability.
Ø If no change of sign, then construct plasma response matric WP, vacuum response matrix WV, total response matrix WT = WP + WV. Negative eigenvalues determine free-boundary instability.
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Glasser, DCON for SPEC, PPPL, February 12, 2020, Slide 27
Conclusions and Future WorkØ The generalized Newcomb criterion has been derived for fixed-boundary ideal MHD
perturbations of SPEC equilibria. The procedure consists of integrating the Euler-Lagrange Equation across each interval, matching the solutions across boundaries, and monitoring the criterion DC for change of sign.
Ø Following discussions with Stuart Hudson and Adelle Wright, ideal MHD stability is a necessary but not sufficient condition for SPEC equilibria. There is an energy principle for MRxMHD equilibria, Eq. (11) of S. R. Hudson, R. L. Dewar, G. Dennis, M. J. Hole, M. McGann, G. von Nessi, and S. Lazerson Phys. Plasmas 19, 112502 (2012). The Newcomb criterion can be extended to treat this energy principle.
Ø Experience with DCON for Tokamaks indicates that this method provides much faster and more accurate determination of stability than PEST-like codes, which compute the full ideal MHD spectrum.
Ø Implementation is under development.
Ø DCON for SPEC can be extended to treat free-boundary stability. This will require a Green’s function computation of perturbed vacuum energy, equivalent to Morrell Chance’s axisymmetric VACUUM code and Peter Merkel’s nonaxisymmetric code.