T. Obiki, T. Mizuuchi, F. Sano, H. Okada,
K. Nagasaki, K. Hanatani, Y. Ijiri, T. Senju,
K. Yaguchi, K. Toshi, K. Sakamoto, T. Hamada,
H. Funaba
Institute of Advanced Energy, Kyoto University, Uji, Japan
K. Kondo, S. Besshou, H. Zushi, M. Wakatani,
Y. Nakamura, M. Nakasuga
Graduate School of Energy Science, Kyoto University, Uji, Japan
V. V. Chechkin, V. S. Voitsenya
Institute of Plasma Physics, National Science Center
``Kharkov Institute of Physics and Technology'', Kharkov, Ukraine
K. Ida, S. Sudo, M. Sato, S. Kobayashi
National Institute for Fusion Science, Toki, Japan
Interdisciplinary Graduate School of Engineering Science,
Kyushu University, Kasuga, Japan
K. Matsuo
Faculty of Engineering, Fukuoka Institute of Technology,
Fukuoka, Japan
Abstract. The effects of the plasma profile on the global energy confinement
have been studied in Heliotron E with special regard to differences between
heating methods (ECH, NBI, and NBI + ECH). With high power NBI, peaked
Ti and peaked
ne profiles (
Ti(0)/Ti 2.7,
ne(0)/ne 4.5) were simultaneously archieved under low recycling conditions. A
peaked
ne profile (
ne(0)/ne 2.5) could lead to the high
Ti mode where the ion heat
transport in the central region is substantially reduced. By changing the ECH
launching condition (on-axis, off-axis and toroidally oblique injection), the
peakedness of the
Te profile could be controlled in the range
1.3 Te(0)/Te 4.5. A peaked
Te- and flat
ne-profile (
3.5 Te(0)/Te,
ne(0)/ne 1.8) was brought about by the well focused on-axis
ECH. The ECH plasma with peaked
Te profile has higher stored
energy than that with a moderately peaked
Te profile for the same
injected ECH power and the same density region. The global energy confinement
time normalized by the LHD scaling,
/, showed
ne(0)/ne dependance for the low
Ti mode NMI plasmas. For the high
Ti mode, the
ne(0)/ne dependance of the
/ was
weak. These findings suggest that the LHD scaling should be modified to scale
the global energy confinement of the helical plasmas in a wide range of
ne(0)/ne.
IAEA 2001