2022
DOI: 10.1088/1741-4326/ac55ba
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Non-axisymmetric MHD simulations of the current quench phase of ITER mitigated disruptions

Abstract: Non-axisymmetric simulations of the current quench phase of ITER disruptions are key to predict asymmetric forces acting into the ITER wall. We present for the first time such simulations for ITER mitigated disruptions at realistic Lundquist numbers. For these strongly mitigated disruptions, we find that the edge safety factor remains above 2 and the maximal integral horizontal forces remain below 1 MN. The maximal integral vertical force is found to be 13 MN and arises in a time scale given by the resistive w… Show more

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Cited by 25 publications
(23 citation statements)
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“…2021; Artola et al. 2022), the deep plasma core tends to be a region where flux surfaces are not completely destroyed, or are broken up only for a very short period within the thermal quench. This may be related to the typically low magnetic shear in the deep core, which does not favour island overlap.…”
Section: Resultsmentioning
confidence: 99%
“…2021; Artola et al. 2022), the deep plasma core tends to be a region where flux surfaces are not completely destroyed, or are broken up only for a very short period within the thermal quench. This may be related to the typically low magnetic shear in the deep core, which does not favour island overlap.…”
Section: Resultsmentioning
confidence: 99%
“…Initially there is no transport as the flux surfaces are intact, but between 10 -12 ms (when the mode energies peak, see Fig. 4 in [10]) the stochastic field region expands until it penetrates almost the whole plasma. This is the beginning of the stochastic phase; also here the confinement volume begins to shrink due to plasma moving vertically into the wall.…”
Section: Resultsmentioning
confidence: 99%
“…Because the Hamiltonian motion is dominant and the effect of the radiation reaction force is comparable to the Coulomb collisions, we resolve to use the Euler method for solving Eq. (10). For consistency the guiding-center radiation reaction force is also solved with the Euler method in this work.…”
Section: Radiation Reaction Forcementioning
confidence: 99%
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