This work reports on the investigation of Eurofer-97 erosion behaviour when exposed to the deuterium plasma of the linear device GyM. The erosion dependence of Eurofer-97 on the deuterium ion fluence, 1025 m-2, and temperature of the samples, T = 600 K and 990 K, was addressed. A bias voltage of -200 V was applied to GyM sample holder during the experiments. Samples were deeply characterised by: profilometry, scanning electron microscopy, atomic force microscopy, energy-dispersive X-ray spectroscopy, time-of-flight secondary ion mass spectrometry, Rutherford backscattering spectroscopy and particle-induced X-ray emission. The behaviour of Eurofer-97 erosion rate with the ion fluence strictly depends upon temperature. At 600 K, it was 0.14 nm/s after 4.7 × 1024 m-2, then decreased, reaching a steady state value of 0.01 nm/s from 8.0 × 1024 m-2. At 990 K instead, the erosion rate was roughly constant around 0.019 nm/s for 1025 m-2. The value at 2.35 × 1025 m-2 was slightly lower. The erosion rate at 990 K was greater than that at 600 K for every ion fluence. Microscopy and surface analysis techniques showed that Eurofer-97 erosion rate dependence on at 600 K was primarily determined by the preferential sputtering of iron and other mid-Z elements of the alloy, leading to a surface rich in W and Ta difficult to be sputtered. The erosion behaviour at 990 K was dominated by the morphology dynamics, instead. The different properties of the morphology developed at the two temperatures can explain the higher erosion rate at 990 K for all the ion fluences.
Study the erosion of Eurofer-97 steel with the linear plasma device GyM
Uccello A.; Ghezzi F.; Kovac J.; Ekar J.; Filipic T.; Bogdanovic Radovic I.; Dellasega D.; Mellera V.; Pedroni M.; Ricci D.; GyM Team
Related products
-
The astrophysical journal. Letters (Print) 912 (2), pp. L21-1 - L21-8 Year: 2021 DOI: 10.3847/2041-8213/abf7d1
Evolution of Solar Wind Turbulence from 0.1 to 1 au during the First Parker Solar Probe-Solar Orbiter Radial Alignment
Telloni, Daniele; Sorriso-Valvo, Luca; Woodham, Lloyd D.; Panasenco, Olga; Velli, Marco; Carbone, Francesco; Zank, Gary P.; Bruno, Roberto; Perrone, Denise; Nakanotani, Masaru; Shi, Chen; D’Amicis, Raffaella; De Marco, Rossana; Jagarlamudi, Vamsee K.; Steinvall, Konrad; Marino, Raffaele; Adhikari, Laxman; Zhao, Lingling; Liang, Haoming; Tenerani, Anna; Laker, Ronan; Horbury, Timothy S.; Bale, Stuart D.; Pulupa, Marc; Malaspina, David M.; Macdowall, Robert J.; Goetz, Keith; De Wit, Thierry Dudok; Harvey, Peter R.; Kasper, Justin C.; Korreck, Kelly E.; Larson, Davin; Case, Anthony W.; Stevens, Michael L.; Whittlesey, Phyllis; Livi, Roberto; Owen, Christopher J.; Livi, Stefano; Louarn, Philippe; Antonucci, Ester; Romoli, Marco; O’Brien, Helen; Evans, Vincent; Angelini, Virginia
-
The astrophysical journal. Letters (Online) 919 (2), pp. L30-1 - L30-8 Year: 2021 DOI: 10.3847/2041-8213/ac26c5
Turbulent Cascade and Energy Transfer Rate in a Solar Coronal Mass Ejection
Sorriso-Valvo, Luca; Yordanova, Emiliya; Dimmock, Andrew P.; Telloni, Daniele
-
Nuclear fusion 61 (7), pp. 076012-1 - 076012-14 Year: 2021 DOI: 10.1088/1741-4326/abfb13
H-mode plasmas in the pre-fusion power operation 1 phase of the ITER research plan
Loarte A.; Polevoi A.R.; Schneider M.; Pinches S.D.; Fable E.; Militello Asp E.; Baranov Y.; Casson F.; Corrigan G.; Garzotti L.; Harting D.; Knight P.; Koechl F.; Parail V.; Farina D.; Figini L.; Nordman H.; Strand P.; Sartori R.
-
Nuclear fusion 61 (7), pp. 076013-1 - 076013-15 Year: 2021 DOI: 10.1088/1741-4326/abfcdf
Prediction of temperature barriers in weakly collisional plasmas by a Lagrangian coherent structures computational tool
Di Giannatale G.; Bonfiglio D.; Cappello S.; Chacon L.; Veranda M.
English
Italiano