The limits for the heat loads on the DEMO first wall are significantly stricter compared to those of ITER due to cooling and breeding blanket requirements. Fast particles in the form of NBI ions can escape the confinement due to magnetic perturbations and produce a significant power load on the first wall. In this contribution, we use the fast ion orbit-following code ASCOT to study NBI losses under the effects of 3D magnetic perturbations, including toroidal field ripple and ferritic inserts. The losses were found to not endanger the integrity of the wall, with loads remaining below 40 kW/m2 even with unmitigated ripple, and losses did not increase above 2.5 % even with 16 toroidal field coils. Ionization in the scrape-off layer was not found to increase the losses significantly for realistic density profiles, and the design of the wall allows for some flexibility in the distance between the plasma and the first wall tiles.

Sensitivity of fast ion losses to magnetic perturbations in the European DEMO

Vincenzi P;Agostinetti P;
2019

Abstract

The limits for the heat loads on the DEMO first wall are significantly stricter compared to those of ITER due to cooling and breeding blanket requirements. Fast particles in the form of NBI ions can escape the confinement due to magnetic perturbations and produce a significant power load on the first wall. In this contribution, we use the fast ion orbit-following code ASCOT to study NBI losses under the effects of 3D magnetic perturbations, including toroidal field ripple and ferritic inserts. The losses were found to not endanger the integrity of the wall, with loads remaining below 40 kW/m2 even with unmitigated ripple, and losses did not increase above 2.5 % even with 16 toroidal field coils. Ionization in the scrape-off layer was not found to increase the losses significantly for realistic density profiles, and the design of the wall allows for some flexibility in the distance between the plasma and the first wall tiles.
2019
Istituto gas ionizzati - IGI - Sede Padova
Inglese
146
1615
1619
5
https://www.sciencedirect.com/science/article/pii/S0920379619303229
Sì, ma tipo non specificato
Magnetic field effects
Breeding blankets
Ions
Wave plasma interactions
Available online 5 April 2019 / E-ISSN: 1873-7196 / http://www.scopus.com/record/display.url?eid=2-s2.0-85063758452&origin=inward / This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under grant agreement No 633053. This work was partially funded by the Academy of Finland project No. 259675, and has also received funding from Tekes - the Finnish Funding Agency for Innovation under the FinnFusion Consortium. The work was carried out using the HELIOS supercomputer system at International Fusion Energy Research Centre, Aomori, Japan, under the Broader Approach collaboration between Euratom and Japan, implemented by Fusion for Energy and JAEA. Part of the work was carried out on the EUROfusion High Performance Computer (Marconi-Fusion). The supercomputing resources of CSC - IT center for science were utilised in the studies. Some of the calculations were performed using computer resources within the Aalto University School of Science "Science-IT" project.
1
info:eu-repo/semantics/article
262
Varje, J.; KurkiSuonio, T.; Snicker, A.; Särkimäki, K.; Vincenzi, P.; Agostinetti, P.; Fable, E.; Sonato, P.; Villone, F.
01 Contributo su Rivista::01.01 Articolo in rivista
none
   EU Fusion for ITER Applications
   EUFORIA
   FP7
   211804

   Implementation of activities described in the Roadmap to Fusion during Horizon 2020 through a Joint programme of the members of the EUROfusion consortium
   EUROfusion
   H2020
   633053
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/367838
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