8–12 Jul 2019
University of Milano-Bicocca UNIMIB
Europe/Rome timezone

P4.1051 Nonlinear MHD simulation of plasma termination events in stellarators

11 Jul 2019, 14:00
2h
Building U6 (University of Milano-Bicocca UNIMIB)

Building U6

University of Milano-Bicocca UNIMIB

Piazza dell’Ateneo Nuovo, 1 20126 Milan, Italy
MCF Poster P4

Speaker

Y. Suzuki (EPS 2019)

Description

See full abstract here
http://ocs.ciemat.es/EPS2019ABS/pdf/P4.1051.pdf

Nonlinear dynamics of plasma termination events in stellarators are studied using a 3D nonlinear MHD simulation code. In this study, two types of plasma termination events, which are MHD instabilities driven by the pressure gradient and plasma current, are studied, respectively. In the Large Helical Device (LHD) experiment, many MHD instabilities are observed. In particular, if the peaked pressure profile was sustained by the pellet injection, a collapse event, so-called the core density collapse (CDC), was happen. In nonlinear MHD simulations, it is expected the CDC is driven by the resistive ballooning mode [1]. Recently, a new imaging diagnostics of the two-dimensional soft-X ray arrays is installed in the LHD. Using the new diagnostics, perturbations localized at the outward of the torus. That is a characteristic of the ballooning mode. So, it seems the ballooning mode is observed in the LHD experiments. However, to interpret the experimental observation, we need to know what kind mode patterns should be observed. On the other hand, in Wendelstein 7-X (W7-X) experiment, collapse events simultaneously happened in the plasma core, if the strongly localized plasma current is driven in the plasma core. That expects a MHD event driven by the plasma current. But, we did not identify what kind mode makes the collapse event in such a case. In this study, we study 3D MHD equilibria with reconstructed pressure profile using a 3D MHD equilibrium code, which does not assume nested flux surfaces [2]. And then, we will study nonlinear MHD simulations based on the 3D MHD equilibrium with the magnetic island [3]. In this study, we note nonlinear saturation to compare with the experimental observation.

  1. N. Mizuguchi, et al., Nucl. Fusion 49 (2009) 095023 2. Y. Suzuki, et al., Nucl. Fusion. 46 (2006) L19 3. Y. Todo, et al., Plasma Fusion Res. 5 (2010) S2062

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