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JOREK simulations of the X-point radiator formation and its movement in ASDEX Upgrade

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Abstract
Future large-scale magnetic confinement fusion reactors require operational regimes that can avoid extreme heat fluxes onto the plasma-facing components. One promising regime is the X-point radiator (XPR), which relies on a highly radiative, cold, and dense plasma volume forming above the X-point, and which can be accessed via impurity seeding. Experimentally, the height of the XPR can be controlled by adjusting the seeding rate and heating power. This contribution presents axisymmetric (2D) simulations of the XPR regime in ASDEX Upgrade using the nonlinear MHD code JOREK extended with a kinetic particle framework for the main species neutrals and nitrogen impurities. With the time-dependent simulations, the progression from attached divertors to a complete detachment with the XPR formation is shown, highlighting the effects of the neutrals and impurities separately. Amid this progression, the formation and the loss of the high-field-side high-density are observed. After the XPR is well-formed at the height of 6.8 cm, the fueling and seeding rates are adjusted so that the XPR remains stationary. From the stationary case, the seeding rate is then changed to see how the XPR location reacts. By increasing and decreasing the seeding rate, the XPR responds by moving upward and downward, respectively. These simulations show JOREK's capability of simulating time-varying XPR, which will provide a baseline for the transition to 3D simulations, so the MHD activities and their interaction with the XPR can be studied.
Year of Publication
2026
Journal
Physics of Plasmas
Volume
33
Issue
5
Number of Pages
052508
Date Published
2026-05-01
DOI
PId
1f4087097b7214330ba2f26d47233eac
Label
OA
Journal Article
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Citation
Liang, Y. C., Cathey, A., Hoelzl, M., Korving, S., Szucs, M., Pan, O., … Team, A. U. (2026). JOREK simulations of the X-point radiator formation and its movement in ASDEX Upgrade. Physics of Plasmas, 33(5), 052508. https://doi.org/10.1063/5.0326876 (Original work published)