By Edited by Pietro VINCENZINI World Academy of Ceramics and National Research Council, Italy Co-edited by Hua-Tay LIN, Oak Ridge National Laboratory, USA Kevin FOX, Savannah River National Laboratory, USA
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Additional resources for 5th FORUM ON NEW MATERIALS PART B Proceedings of the 5th Forum on New Materials, part of CIMTEC 2010-12 th International Ceramics Congress and 5th Forum on New Materials Montecatini Terme, Italy, June 13-18, 2010
H. Jones, L. Giancarli, A. Hasegawa, Y. Katoh, A. Kohyama, B. L. J. Weber, Journal of Nuclear Materials 307–311 (2002) 1057–1072  A. Hasegawa, A. H. L. Snead, B. Riccardi, P. Fenici, Journal of Nuclear Materials 283±287 (2000) 128±137  B. Riccardi, L. Giancarli, A. Hasegawa, Y. Katoh, A. H. L. H. L. Snead, A. Kohyama, P. Fenici, Fusion Engineering and Design 41(1998)15-24  T. Nozawa, T. Hinoki, Y. Katoh, A. Kohyama, J. Nucl. Mater. 307-311 (2002) 1173-1177  L. El-Guebaly, ARIES II/IV Report, to be published  H.
2. Microstructure of V-4Cr-4Ti (NIFS-HEAT-2) as a function of re-heating temperature following annealing for precipitate dissolution (1373K, 1 hour). (a) 873K, (b) 973K, (c) 1073K, (d) 1173K, (e) 1273K and (f) 1373K for 1 hour. 220 Vickers Vicker's Hardness hardness (Hv) (Hv) r The manufacturing of V-4Cr-4Ti alloy (NIFS-HEAT-2) products in the Japanese program proceeded with (1) ingot fabrication, (2) hot forging, (3) hot and cold rolling and (4) thermal annealing [5,6]. The last process is known to influence strongly the properties of the products.
The annealing for precipitate dissolution followed by re-heating for re-precipitation was investigated for the purpose of strengthening the alloy . Fig. 3 shows Vickers hardness with the time of re-heating at 873K following the dissolution annealing at 1373K for 1 hour. The investigation selected the re-heating time of 20 hours as the standard heat treatment for strengthening. Results of TEM observation after re-heating at 873K for 20 hours are shown in Fig. 4. No precipitate image was observed with the conventional bright field imaging and weak-beam dark field (WBDF) imaging with the g vector of .