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pro vyhledávání: '"W. Gasparino"'
Autor:
H. Wolff, A. Dodhy, G. Cattanei, S. Geissler, E. Würsching, A. A. Borschegovsky, S. A. Malygin, H. Verbeek, H. Ringler, F. Sardei, N. Ruhs, P. Pech, H. Niedermeyer, F. Karger, M. Endler, U. Wenzel, R. Burhenn, A. Rudjy, H. Maassberg, S. Sattler, H. J. Hartfuss, G. A. Müller, J. V. Hofmann, J. Baldzuhn, Frank Schneider, R. Jaenicke, M. Tutter, G. Kuehner, T. Geist, G. Herre, D. Zimmermann, H. Kroiss, O. Heinrich, L. Giannone, V. I. Malygin, M. Kick, Ulrich Stroth, T. Ott, V. Erckmann, D. Hildebrandt, D. Dorst, M. Zippe, U. Gasparino, R. Brakel, E. Speth, C. Mahn, K. McCormick, G. Siller, Friedrich E. Wagner, P. Grigull, W. Kasparek, W. Gasparino, J. Saffert, K. Engelhardt, V. I. Ilin, P. G. Schüller, A. Weller, H. P. Penningsfeld, Ulrich Schneider, V. I. Kurbatov, A. Elsner, W. Ohlendorf, H. Hacker, E. Unger
Publikováno v:
Fusion Engineering and Design. 26:141-152
Electron cyclotron resonance heating (ECRH) at the W7-AS stellarator is performed two systems of comparable heating power at 70 GHz (0.8 MW, 3 s) and 140 GHz (0.9 MW, 0.4 s). Experiments with 140 GHz open a new parameter window with high density oper