the numerical construction of stellarator equilibria and

28
The Numerical Construction of Stellarator Equilibria and Coil Design. 1 S. R. Hudson, R. L. Dewar, M. J. Hole, J. Loizu, C. Zhu, A. Cerfon et al. Simons Foundation Meeting, 2019 1. This talk shall outline the mathematical and numerical construction of a magnetically confined plasma in force balance with a magnetic field produced by external currents (coils). 2. The plasma equilibrium is an appropriately constrained minimum of the plasma energy functional. A restriction upon the boundary conditions is required to avoid non-physical, non-tractable solutions. 3. The coil geometry is obtained by minimizing an error functional that quantifies how well the coils provide the magnetic field required to hold the plasma in equilibrium.

Upload: others

Post on 08-Feb-2022

3 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: The Numerical Construction of Stellarator Equilibria and

The Numerical Construction of Stellarator Equilibria and Coil Design.

1

S. R. Hudson, R. L. Dewar, M. J. Hole, J. Loizu, C. Zhu, A. Cerfon et al. Simons Foundation Meeting, 2019

1. This talk shall outline the mathematical and numerical construction of a magnetically confined plasma in force balance with a magnetic field produced by external currents (coils).

2. The plasma equilibrium is an appropriately constrained minimum of the plasma energy functional. A restriction upon the boundary conditions is required to avoid non-physical, non-tractable solutions.

3. The coil geometry is obtained by minimizing an error functional that quantifies how well the coils provide the magnetic field required to hold the plasma in equilibrium.

Page 2: The Numerical Construction of Stellarator Equilibria and

Confinement of Charged Particles in Toroidal Magnetic Fields, and Fusion Energy.

2

φ

θ

Page 3: The Numerical Construction of Stellarator Equilibria and

Magneto-hydro-dynamic (MHD) Equilibria Are Minima of the Thermal + Magnetic Energy Functional.

3 Bernstein, Freiman, Kruskal & Kulsrud, Phys. Fluids (1958), https://doi.org/10.1098/rspa.1958.0023

Page 4: The Numerical Construction of Stellarator Equilibria and

Restricting Attention to “Ideal” Variations, We Can Derive the Euler Lagrange Equation.

4

Page 5: The Numerical Construction of Stellarator Equilibria and

But, in Ideal MHD, Pressure Gradients Near Rational Surfaces Create Non-Physical Current Densities.

5

Page 6: The Numerical Construction of Stellarator Equilibria and

The δ-function Current Densities Are Consistent with Assumption of Infinite Conductivity.

6

Page 7: The Numerical Construction of Stellarator Equilibria and

But, Cross-Sectional Surfaces Exist Through Which the Pressure-Driven “1/x” Current is Infinite.

7

Page 8: The Numerical Construction of Stellarator Equilibria and

And, in Ideal MHD, Perturbation Theory Breaks Down Near Rational Surfaces.

8 Rosenbluth, Dagazian & Rutherford (1975)

Page 9: The Numerical Construction of Stellarator Equilibria and

Helicity is a Measure of the Global “Inter-linked-ness” of the Magnetic Field.

9 Berger, PPCF (1999)

Page 10: The Numerical Construction of Stellarator Equilibria and

“Taylor” Relaxation Allows for a Less-Restrictive Class of Variations in the Pressure and Magnetic Field.

10

Page 11: The Numerical Construction of Stellarator Equilibria and

Extension to Multi-Region Relaxed MHD Equilibria. Theoretical Model by Courant Institute, ANU & PPPL.

pres

sure

radial coordinate

Stepped-pressure profile

Bruno & Laurence, (1996); S.R. Hudson, R.L. Dewar et al., (2012)

Page 12: The Numerical Construction of Stellarator Equilibria and

Numerical Method Uses Global Coordinates and a Mixed Chebyshev Fourier Representation.

R

Z

12

Page 13: The Numerical Construction of Stellarator Equilibria and

Given the Beltrami Fields in Each Volume, Then Adjust Geometry of Interfaces to Balance Force.

13

Page 14: The Numerical Construction of Stellarator Equilibria and

When Using Toroidal Coordinates, The Singularity at the Origin Requires Some Care.

R

Z

14

Page 15: The Numerical Construction of Stellarator Equilibria and

By Exploiting An Integral Representation for Maxwell’s Equations, Can Convert Problem to Surface Integrals.

15

Page 16: The Numerical Construction of Stellarator Equilibria and

Given Boundary Conditions, Can Solve for Unknowns.

16

Page 17: The Numerical Construction of Stellarator Equilibria and

A Free-Boundary Equilibrium Must Be Supported By An Externally-Generated Magnetic Field.

17

Page 18: The Numerical Construction of Stellarator Equilibria and

Can Generalize Stepped Pressure to Smooth Pressure By Expanding the Ideal Interfaces to Ideal Regions.

18

MHD Equilib.

Page 19: The Numerical Construction of Stellarator Equilibria and

rota

tiona

l tr

ansf

orm

pr

essu

re

Mixed Ideal-Relaxed MHD Allows Continuous Pressure. Can Approximate “Fractal Staircase” Pressure Profiles.

19 S.R. Hudson & B. Kraus, J. Plasma Phys., 83, 715830403 (2017)

radial coordinate = toroidal flux

Page 20: The Numerical Construction of Stellarator Equilibria and

A Set of External Current-Carrying Coils Provides the Required External Magnetic Field.

20

Page 21: The Numerical Construction of Stellarator Equilibria and

The Geometry of a Set of Discrete Coils is Determined Numerically.

21

Page 22: The Numerical Construction of Stellarator Equilibria and

The Equilibrium and the Coil Geometry Depend on B.n. Can Optimize Plasma Performance And Coil Complexity.

22

Page 23: The Numerical Construction of Stellarator Equilibria and

Summary

23

1. This talk outlined the mathematical/numerical construction of a magnetically confined plasma in force balance with a magnetic field produced by external currents (coils).

2. The plasma equilibrium is an appropriately constrained minimum of the plasma energy functional. A restriction upon the allowed variations is required to avoid non-physical, non-tractable solutions.

3. The coil geometry is obtained by minimizing an error functional that quantifies how well the coils provide the magnetic field required to hold the plasma in equilibrium.

Page 24: The Numerical Construction of Stellarator Equilibria and

24

Page 25: The Numerical Construction of Stellarator Equilibria and

The Equilibrium and Coil Geometry can be Computed Simultaneously Within the Plasma Optimization

Page 26: The Numerical Construction of Stellarator Equilibria and

Can Simplify the Coils Under the Constraint of Conserved Plasma Properties.

26

Page 27: The Numerical Construction of Stellarator Equilibria and

27

Page 28: The Numerical Construction of Stellarator Equilibria and

The Quadratic-Flux is an Analytic Function of the Surface.

28