Abstract
Numerical MHD simulations are used to gain insight into how sawteeth are affected by three-dimensional shaping from the Compact Toroidal Hybrid (CTH) stellarator field. CTH is a small stellarator-tokamak hybrid and sawteeth are sometimes seen on soft x-ray signals when operating with tokamak like profiles. We use NIMROD to compute numerical solutions having repeated sawtooth relaxations for a sequence of configurations with increasing helical stellarator field strength. The experimentally observed trend of the sawtooth period decreasing as the helical field strength is increased is recovered in the simulations. Careful attention to numerical convergence was required to obtain the results, and these considerations may be relevant to simulations of other phenomena in devices with non-axisymmetric plasmas such as perturbed tokamaks, RFPs, and stellarators.
Original language | English |
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Article number | 092513 |
Journal | Physics of Plasmas |
Volume | 23 |
Issue number | 9 |
DOIs | |
State | Published - Sep 1 2016 |
Externally published | Yes |
Funding
This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. This work was supported by the U.S. DOE Grant Nos. DE-FG-02-00ER54610 and DE-FG-02-03ER54692.
Funders | Funder number |
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DOE Office of Science | |
U.S. DOE | DE-FG-02-00ER54610, DE-FG-02-03ER54692 |
U.S. Department of Energy | DE-AC02-05CH11231 |
Office of Science |