Radiated energy fraction of SPI-induced disruptions at ASDEX Upgrade
Paul Heinrich (1, 2), Gergely Papp (1), Stefan Jachmich (3), Javier, Artola (3), Matthias Bernert (1), Pascal de Marn\'e (1), Mathias Dibon (3),, Ralph Dux (1), Thomas Eberl (1), J\"org Hobirk (1), Michael Lehnen (1),, Tobias Peherstorfer (4), Nina Schwarz (3), Umar Sheikh (5)

TL;DR
This study investigates how different pellet compositions and shattering methods in SPI disrupt plasma at ASDEX Upgrade, revealing neon content and pellet size as key factors influencing radiated energy and disruption thresholds.
Contribution
It provides new experimental data on SPI-induced disruptions, highlighting the effects of neon content, pellet size, and shatter head design on radiated energy fraction and disruption thresholds.
Findings
Neon content in pellets strongly affects radiated energy fraction.
Larger and faster fragments increase radiated energy for neon content below 1.25%.
Disruption threshold for 100% D₂ pellets is around 10²² molecules.
Abstract
Future large tokamaks will operate at high plasma currents and high stored plasma energies. To ensure machine protection in case of a sudden loss of plasma confinement (major disruption), a large fraction of the magnetic and thermal energy must be radiated to reduce thermal loads. The disruption mitigation system for ITER is based on massive material injection in the form of shattered pellet injection (SPI). To support ITER, a versatile SPI system was installed at the tokamak ASDEX Upgrade (AUG). The AUG SPI features three independent pellet generation cells and guide tubes, and each was equipped with different shatter heads for the 2022 experimental campaign. We dedicated over 200 plasma discharges to the study of SPI plasma termination, and in this manuscript report on the results of bolometry (total radiation) analysis. The amount of neon inside the pellets is the dominant factor…
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Taxonomy
TopicsParticle Detector Development and Performance · Magnetic confinement fusion research · Ionosphere and magnetosphere dynamics
