Abstract
The NOT Program, in which the present JT-60U is being modified into a superconducting coil machine, is discussed under nationwide collaboration in Japan. Its mission is to establish high-beta steady-state operation for DEMO and to contribute to ITER. NCT is designed to have potential to investigate such research.
| Original language | English |
|---|---|
| Pages (from-to) | S428-S432 |
| Journal | Journal of the Korean Physical Society |
| Volume | 49 |
| Issue number | SUPPL. 1 |
| Publication status | Published - Dec 2006 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)
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In: Journal of the Korean Physical Society, Vol. 49, No. SUPPL. 1, 12.2006, p. S428-S432.
Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - Overview of national centralized tokamak program - Mission, design and strategy to contribute to ITER and DEMO
AU - Ninomiya, H.
AU - Akiba, M.
AU - Fujii, T.
AU - Fujita, T.
AU - Fujiwara, M.
AU - Hamamatsu, K.
AU - Hayashi, N.
AU - Hosogane, N.
AU - Ikeda, Y.
AU - Inoue, N.
AU - Kamada, Y.
AU - Kawashima, H.
AU - Kikuchi, M.
AU - Kizu, K.
AU - Kubo, H.
AU - Kudo, Y.
AU - Kurihara, K.
AU - Kurita, G.
AU - Kuriyama, M.
AU - Masaki, K.
AU - Matsukawa, M.
AU - Miura, Y.
AU - Miya, N.
AU - Morioka, A.
AU - Okuno, K.
AU - Sakurai, S.
AU - Suzuki, T.
AU - Takahashi, H.
AU - Takechi, M.
AU - Tamai, H.
AU - Tsuchiya, K.
AU - Yamamoto, T.
AU - Azechi, H.
AU - Horiike, H.
AU - Miura, Y. M.
AU - Hashizume, H.
AU - Ichimura, M.
AU - Imai, T.
AU - Yatsu, K.
AU - Ida, K.
AU - Nishimura, A.
AU - Sagara, A.
AU - Kimura, A.
AU - Matsuoka, M.
AU - Itoh, S.
AU - Nakamura, K.
AU - Sakamoto, M.
AU - Sato, K.
AU - Shimizu, A.
AU - Yoshida, N.
AU - Okano, K.
AU - Shimada, R.
AU - Tsutsui, H.
AU - Takase, Y.
AU - Tanaka, S.
AU - Uesugi, Y.
N1 - Funding Information: We would like to thank the referee, Preben Grosbøl, for excellent comments that improved the clarity of this paper. AGK, AAH, and LVB acknowledge the hospitality of the Institut d'Astrophysique de Paris (France) during their stay as visiting scientists supported by the Programme Visiteurs Extérieurs (PVE). This work was supported by the RA MES State Committee of Science, in the frames of the research project number 15T-1C129. This work was made possible in part by a research grant from the Armenian National Science and Education Fund (ANSEF) based in New York, USA. V.A. acknowledges the support from Fundação para a Ciência e Tecnologia (FCT) through Investigador FCT contract nr. IF/00849/2015/CP1273/CT0003 and the support from FCT through national funds and by FEDER through COMPETE2020 by the grant PTDC/FIS-AST/7073/2014 & POCI-01-0145-FEDER-016880. Funding for the SDSS-IV has been provided by the Alfred P. Sloan Foundation, the US Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org. SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center forAstrophysics, Instituto de Astrofísica deCanarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPAGarching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University ofVirginia, University ofWashington, University ofWisconsin, Vanderbilt University, and Yale University Funding Information: We would like to thank the referee, Preben Grosbøl, for excellent comments that improved the clarity of this paper. AGK, AAH, and LVB acknowledge the hospitality of the Institut d’Astrophysique de Paris (France) during their stay as visiting scientists supported by the Programme Visiteurs Extérieurs (PVE). This work was supported by the RA MES State Committee of Science, in the frames of the research project number 15T–1C129. This work was made possible in part by a research grant from the Armenian National Science and Education Fund (ANSEF) based in New York, USA. V.A. acknowledges the support from Fundac¸ão para a Ciência e Tecnologia (FCT) through Investigador FCT contract nr. IF/00849/2015/CP1273/CT0003 and the support from FCT through national funds and by FEDER through COMPETE2020 by the grant PTDC/FIS-AST/7073/2014 & POCI-01-0145-FEDER-016880. Funding for the SDSS-IV has been provided by the Alfred P. Sloan Foundation, the US Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org. SDSS–IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofísica de Ca-narias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astro-physik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.
PY - 2006/12
Y1 - 2006/12
N2 - The NOT Program, in which the present JT-60U is being modified into a superconducting coil machine, is discussed under nationwide collaboration in Japan. Its mission is to establish high-beta steady-state operation for DEMO and to contribute to ITER. NCT is designed to have potential to investigate such research.
AB - The NOT Program, in which the present JT-60U is being modified into a superconducting coil machine, is discussed under nationwide collaboration in Japan. Its mission is to establish high-beta steady-state operation for DEMO and to contribute to ITER. NCT is designed to have potential to investigate such research.
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UR - http://www.scopus.com/inward/citedby.url?scp=33846370517&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:33846370517
SN - 0374-4884
VL - 49
SP - S428-S432
JO - Journal of the Korean Physical Society
JF - Journal of the Korean Physical Society
IS - SUPPL. 1
ER -