Calculation of continuum damping of Alfv\'en eigenmodes in 2D and 3D cases
G.W. Bowden, M.J. Hole, A. K\"onies

TL;DR
This paper presents a computationally efficient method using complex contours to calculate continuum damping of shear Alfvén eigenmodes in 2D and 3D plasma configurations, including stellarators, with applications to various magnetic confinement devices.
Contribution
It introduces the first application of the complex contour method to fully three-dimensional stellarator equilibria for calculating continuum damping.
Findings
Continuum damping depends on coupling to multiple harmonics.
Method reduces computational resolution requirements.
First 3D stellarator eigenmode damping calculations.
Abstract
In ideal MHD, shear Alfv\'{e}n eigenmodes may experience dissipationless damping due to resonant interaction with the shear Alfv\'{e}n continuum. This continuum damping can make a significant contribution to the overall growth/decay rate of shear Alfv\'{e}n eigenmodes, with consequent implications for fast ion transport. One method for calculating continuum damping is to solve the MHD eigenvalue problem over a suitable contour in the complex plane, thereby satisfying the causality condition. Such an approach can be implemented in three-dimensional ideal MHD codes which use the Galerkin method. Analytic functions can be fitted to numerical data for equilibrium quantities in order to determine the value of these quantities along the complex contour. This approach requires less resolution than the established technique of calculating damping as resistivity vanishes and is thus more…
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Taxonomy
TopicsMagnetic confinement fusion research · Seismic Imaging and Inversion Techniques · Geomagnetism and Paleomagnetism Studies
