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Christmas Night
Twas the night before Christmas when all through the houseNo electrons were flowing through even my mouse.
All devices were plugged in by the chimney with careWith the hope that St. Nikola Tesla would share.
R.J. Hawryluk, D. Mueller, J. Hosea, C.W. Barnes1,M. Beer, M.G. Bell, R. Bell, H. Biglari, M. Bitter, R. Boivin2, N.L. Bretz, R. Budny, C.E. Bush3, L. Chen, C.Z. Cheng, S. Cowley, D.S. Dairow, P.C. Efthimion, R.J. Fonck4, E. Fredrickson, H.P. Furth, G. Greene, B. Grek, L.R. Grisham, G. Hammett, W. Heidbrink5, K.W. Hill, D. Hoffman3, R.A. Hulse, H. Hsuan, A. Janos, D.L. Jassby, F.C. Jobes, D.W. Johnson, L.C. Johnson, J. Kamperschroer, J. Kesner2, C.K. Phillips, S.J. Kilpatrick, H. Kugel, P.H. LaMarche, B. LeBlanc, D.M. Manos, D.K. Mansfield, E. S. Marmar2, E. Mazzucato, M.P. McCarthy, J. Machuzak2, M. Mauel6, D.C McCune, K.M. McGuire, S.S. Medley, D.R. Mikkelsen D. Monticello, Y. Nagayama7, G.A. Navratil6, R. Nazikian, D.K. Owens, H. Park, W. Park, S. Paul, F. Perkins, S. Pitcher8, D. Rasmussen3, M.H. Redi, G. Rewoldt, D. Roberts4, A.L. Roquemore, S. Sabbagh6, G. Schilling, J. Schivell, G.L. Schmidt, S.D. Scott, J. Snipes2, J. Stevens, B.C. Stratton, J.D. Strachan,W. Stodiek, E. Synakowski, W. Tang, G. Taylor, J. Terry2, J.R. Timberlake, H.H. Towner M. Ulrickson, S. von Goeler, R. Wieland, J.R. Wilson, K.L. Wong, P. Woskov2, M. Yamada, K.M. Young, M.C. Zamstorff, S.J. Zweben
Fusion Science and Technology | Volume 21 | Number 3 | May 1992 | Pages 1324-1331
Magnetic and Inertial Fusion Experiment | doi.org/10.13182/FST92-A29907
Articles are hosted by Taylor and Francis Online.
Recent research on TFTR has emphasized optimization of performance in deuterium plasmas, transport studies and studies of energetic ion and fusion product physics in preparation for the D-T experiments that will commence in July of 1993. TFTR has achieved full hardware design parameters, and the best TFTR discharges in deuterium are projected to QDT of 0.3 to 0.5. The physics phenomena that will be studied during the D-T phase will include: tritium particle confinement and fueling, ICRF heating with tritium, species scaling with tritium, collective alpha-particle instabilities, alpha heating of the plasma and helium ash buildup. It is important for the fusion program that these physics issues be addressed to identify regimes of benign alpha behavior, and to develop techniques to actively stabilize or control instabilities driver by collective alpha effects.