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20–23 Jul 2020
WebEx Meeting
Europe/Vienna timezone

Overview of the Radiated Fraction and Radiation Asymmetries Following Shattered Pellet Injection

Not scheduled
25m
WebEx Meeting

WebEx Meeting

Invited Mitigation

Speaker

Ryan Sweeney (Massachusetts Institute of Technology)

Description

During shattered pellet injection (SPI) shutdowns in ITER, a high fraction of the plasma thermal energy must be radiated with a moderate degree of uniformity to avoid damages to the divertor and the first wall such as melting. DIII-D, J-TEXT, JET, and KSTAR now operate SPI systems and studies have begun to assess these requirements. For studies of gross dependencies of the radiation efficiency, the radiation is often assumed axisymmetric and is measured in one toroidal location by approximately calibrated fast diodes, or by metal foil bolometers that integrate over the entire disruption and require subtraction of the radiated magnetic energy. Both approaches find increasing radiation as the injected neon quantity is increased until a saturation is observed at ~10 Pa$\cdot$m$^3$ in DIII-D [D. Shiraki et al., Phys. Plasmas 23 (2016)] and ~50 Pa$\cdot$m$^3$ in JET, in approximate agreement with the scaling $N_{\mathrm{Ne}} \propto (W_{\mathrm{th}}V/a)^{0.5}$. Unfortunately, the assumed axisymmetric radiated fraction $\langle f_{\mathrm{rad}} \rangle$ in JET decreases as the plasma thermal fraction $f_{\mathrm{th}}$ increases, similar to massive gas injection [M. Lehnen et al., NF 53 (2013)], and suggests that the ITER divertor will melt even with mitigation [$\langle f_{\mathrm{rad}} \rangle = \langle W_{\mathrm{rad}} \rangle /(W_{\mathrm{th}} + W_{\mathrm{mag}} – W_{\mathrm{coupled}})$ where $\langle W_{\mathrm{rad}} \rangle$ is the assumed axisymmetric radiated energy, $W_{\mathrm{th}}$ and $W_{\mathrm{mag}}$ are the thermal and magnetic energies, and $W_{\mathrm{coupled}}$ is the magnetic energy coupled to the vessel]. However, an asymmetry in the radiation is measured that shows positive correlations with $f_{\mathrm{th}}$ and the injected neon quantity, invalidating the axisymmetric assumption at high $f_{\mathrm{th}}$, and possibly resolving the radiation shortfall. Work towards a full 3D treatment of the radiated power is ongoing. Asymmetries are explored further by varying the toroidal phase of an applied $n=1$ field and measurements show that the radiation asymmetries at least partially track the phase-locked magnetohydrodynamic (MHD) modes. Localized wall heating near the SPI port in DIII-D is measured with infrared cameras, and work continues to quantify the radiation peaking consistent with this hot spot. The JOREK, M3D-C1, and NIMROD nonlinear MHD codes can be used to better understand the asymmetries, and present simulations show qualitative agreement with experiment.

Member State or International Organization United States of America
Affiliation Plasma Science and Fusion Center, Massachusetts Institute of Technology, 167 Albany St, Cambridge, MA 02139, USA

Primary authors

Ryan Sweeney (Massachusetts Institute of Technology) Larry R. Baylor (Oak Ridge National Laboratory) Daniele Bonfiglio (Consorzio RFX, Padova, Italy) Mr Douglas Craven (UKAEA/CCFE) Nicholas Eidietis (General Atomics) Robert Granetz (MIT) Valentina Huber (Forschungszentrum Jülich GmbH, Supercomputing Centre, 52425 Jülich, Germany) Emmanuel Joffrin (CEA/IRFM) Eric M. Hollmann (University of California San Diego) Stefan Jachmich (ITER Organization) Jayhyun Kim (National Fusion Research Institute) Damian King (UKAEA/CCFE ) Michael Lehnen (ITER Organization) Dr Jack Lovell (UKAEA/CCFE) Costanza Maggi (CCFE) Dr Alan Peacock (UKAEA/CCFE) Roger Raman (University of Washington) Cedric Reux (CEA, IRFM, F-13108 Saint Paul-lez-Durance, France.) Dr Umar Sheikh (EPFL-SPC) Daisuke Shiraki (Oak Ridge National Laboratory) Dr Scott Silburn (UKAEA/CCFE) You Li (Huazhong University of Science and Technology) Dr James Wilson (UKAEA/CCFE) JET Contributors (See the author list of “Overview of the JET preparation for Deuterium-Tritium Operation” by E. Joffrin et al. to be published in Nuclear Fusion Special issue: overview and summary reports from the 27th Fusion Energy Conference (Ahmedabad, India, 22-27 October 2018)) DIII-D Team KSTAR Team

Presentation materials