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Reassessment of tritium content in CFC tiles exposed to the JET D-T campaign in 1997

Likonen, J. ; Bekris, N. 1; Coad, J. P.; Ayres, C.; Gotts, N.; Jepu, I.; Zayachuk, Y.; Widdowson, A.; Wilson, I.; Catarino, N.; de Alves, E.
1 Institut für Astroteilchenphysik (IAP), Karlsruher Institut für Technologie (KIT)

Abstract:

In 2019 two MkIIA divertor tiles (6IN3 and 4BN4) exposed during DTE1 were retrieved at CCFE for Thermal Desorption Spectroscopy (TDS) and pyrolysis analyses. A set of samples were prepared using a coring technique. The highest tritium (T) inventories were found in the shadowed corner of the inner divertor due to asymmetric deposition. TDS analyses indicated that T is desorbed at rather high temperatures with maximum release peaks at ∼590 and 820 °C. A few samples were reannealed at 850 °C using the same heating procedure and it turned out that a further ∼40–50 % of T was still released indicating that the annealing procedure used does not empty the sample completely. Pyrolysis results for thin disks cut from the surface of the tile were somewhat higher than the corresponding TDS results. T amounts were also investigated as a function of depth from the tile surface up to a depth of ∼4.5 mm and T was detected at these depths. Comparison was also made with old results obtained with the pyrolysis technique and a PIN-diode method a few years after the DTE1 experiment, allowing for the natural decay and off-gassing of T. Our results agree within a factor of ∼3 with these results.


Verlagsausgabe §
DOI: 10.5445/IR/1000153597
Veröffentlicht am 04.01.2023
Cover der Publikation
Zugehörige Institution(en) am KIT Institut für Astroteilchenphysik (IAP)
Publikationstyp Zeitschriftenaufsatz
Publikationsjahr 2022
Sprache Englisch
Identifikator ISSN: 2352-1791
KITopen-ID: 1000153597
HGF-Programm 51.13.01 (POF IV, LK 01) Neutrinophysik und Dunkle Materie
Erschienen in Nuclear Materials and Energy
Verlag Elsevier
Band 33
Seiten Art.Nr. 101312
Vorab online veröffentlicht am 19.11.2022
Nachgewiesen in Scopus
Dimensions
Web of Science
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