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RISS 인기검색어
- 검색키워드
- 저자 : BERGH S. VAN DEN (검색결과 3 건)
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Van Den Berghe, S.,Lemoine, P. Korean Nuclear Society 2014 Nuclear Engineering and Technology Vol.46 No.2
This review aims to provide a synthesis of the knowledge generated and the lessons learned in roughly 15 years of UMo dispersion fuel R&D in Europe through a series of irradiation experiments. A lot of irradiations were also performed outside of Europe, particularly in the USA, Russia, Canada, Korea and Argentina. In addition, a large number of out-of-pile investigations were done throughout the world, providing support to the understanding of the phenomena governing the UMo behaviour in pile. However, the focus of this article will be on the irradiations and Post-Irradiation Examination (PIE) results obtained in European experiments. The introduction of the article provides a historic overview of the evolution and progress in the high density UMo dispersion fuel development. The ensuing sections then provide further details on the various phases of the development, from the UMo dispersion in a pure Al matrix through the addition of Si to the matrix to address the interaction layer formation and finally to the more advanced solutions to the excessive swelling encountered in various experiments. This review was based only on published results or results that are currently in the process of being published.
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S. Van den Berghe,LEMOINE 한국원자력학회 2014 Nuclear Engineering and Technology Vol.46 No.2
This review aims to provide a synthesis of the knowledge generated and the lessons learned in roughly 15 years of UModispersion fuel R&D in Europe through a series of irradiation experiments. A lot of irradiations were also performed outside ofEurope, particularly in the USA, Russia, Canada, Korea and Argentina. In addition, a large number of out-of-pileinvestigations were done throughout the world, providing support to the understanding of the phenomena governing the UMobehaviour in pile. However, the focus of this article will be on the irradiations and Post-Irradiation Examination (PIE) resultsobtained in European experiments. The introduction of the article provides a historic overview of the evolution and progress in the high density UModispersion fuel development. The ensuing sections then provide further details on the various phases of the development, fromthe UMo dispersion in a pure Al matrix through the addition of Si to the matrix to address the interaction layer formation andfinally to the more advanced solutions to the excessive swelling encountered in various experiments. This review was based only on published results or results that are currently in the process of being published.
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HESSER J. E.,STETSON P. B.,HARRISM W. E.,BOLTE M.,SMECKER-HANE T. A.,VANDENBERG D. A.,BELL R. A.,BOND H. E.,BERGH S. VAN DEN,MCCLURE R. D.,FAHLMAN G. G.,RICHER H. B. The Korean Astronomical Society 1996 Journal of The Korean Astronomical Society Vol.29 No.suppl1
We review observational evidence bearing on the formation of a prototypical large spiral galaxy, the Milky Way. New ground- and space-based studies of globular star clusters and dwarf spheroidal galaxies provide a wealth of information to constrain theories of galaxy formation. It appears likely that the Milky Way formed by an combination of rapid, dissipative collapse and mergers, but the relative contributions of these two mechanisms remain controversial. New evidence, however, indicates that initial star and star cluster formation occurred simultaneously over a volume that presently extends to twice the distance of the Magellanic Clouds.
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