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772 PESlC FIG. 5. Real and imaginary parts of NL0 versus x for uc(O)/u = 0.625, w 2 p{0)ta 2 c{0) = 0.6, c/v,(O) = 8, c/vs(O) = 4, u = 0, 0,- = 60° and several values of-q. that propagating in the direction of increasing magnetic field the X-mode reaches the right hand cut-off at x = 0.34. Here complete first pass absorption can be obtained at koa = 2 x 10 4 . It should be noted that in high density plasmas the absorption efficiency improves significantly with the increase of both the tail and bulk electron temperatures. The effect of the streaming electron motion on the absorption at downshifted frequencies depends strongly on u/vs and the sign of N|. For No > 0 and u < vs(0) it is relatively weak. However, for Nf < 0 the presence of a current carrying tail causes an increase of Im N±x along with a broadening of the absorption profile. It turns out that in these wave launching conditions the streaming electron motion enhances substantially the wave absorption at downshifted frequencies. For instance, for the parameters of Fig. 4 and at N[ = -0.5 and u/vs(0) = 1, the X-mode is absorbed completely in one pass through a plasma with koa = 3.5 x 10 3 . In this case the power deposition profile has a broad maximum which takes place at x = 0.7, i.e. at v,/c = 0.23. 4. ORDINARY MODE In general, the spatial damping of the O-mode around the SECH is much weaker than the X-mode damping [4]. This conclusion can be further verified in Fig. 5, where we show the variation of the real and the imaginary part of the perpendicular wave refractive index of the O-mode with x for Bt = 60°. The other parameters are the same as in Fig. 2. We see that the presence of superthermal electrons slightly enlarges the thermal absorption profile. The normalized optical thickness of the Omode has a stronger temperature dependence than that of the X-mode [4]. This sug-
IAEA-CN-50/E-IV-ll 773 gests that in very high temperature, large plasmas, complete first pass absorption at large frequency downshifts can be achieved. 5. CONCLUSIONS We have investigated the propagation and absorption of electromagnetic waves in a weakly relativistic Maxwellian plasma in the presence of a non-drifting or current carrying superthermal tail, with the main objective of clarifying whether the frequency requirements of the SECH plasma heating can be reduced. The results obtained indicate that in the range of bulk electron temperatures T = 1-4 keV, > X-waves whose frequency is significantly lower than the central SECH frequency, w < 2coc(0)/(l + A" 1 ), produce good power deposition profiles in large plasmas. In small and medium size plasmas (koa < 10 3 ), moderate frequency downshifts of the X- or O-mode are more effective in heating the central plasma region. Both the non-drifting and current carrying (at Nf < 0) superthermal tails substantially improve the wave absorption efficiency at downshifted frequencies. Higher electron temperatures allow the use of waves with larger frequency downshifts in medium size plasmas as well as an effective optimization of the power deposition. REFERENCES [1] MAZZUCATO, E., FIDONE, I., GIRUZZI, G., KRIVENSKI, V., Electron cyclotron heating at down-shifted frequencies in existing tokamak devices, Nucl. Fusion 26 (1986) 3-9. [2] FIDONE, I., GIRUZZI, G., MAZZUCATO, E., Electron cyclotron heating of a tokamak reactor at downshifted frequencies, Phys. Fluids 28 5 (1985) 1224. [3] BORNATICI, M., RUFFINA, U., "Electron cyclotron absorption at downshifted frequencies in presence of a superthermal tail", Controlled Fusion and Plasma Physics (Proc. 14th Eur. Conf. Madrid, 1987), Vol. HD, Part II, European Physical Society (1987) 890. [4] PESIC, S., Wave-plasma interaction near the second electron cyclotron harmonic, Phys. Fluids 31 1 (1988) 115. [5] SHKAROFSKY, I.P., Dielectric tensor in Vlasov plasmas near cyclotron harmonics, Phys. Fluids 9 3 (1966) 561.
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The cover picture shows the inside
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AFGHANISTAN ALBANIA ALGERIA ARGENTI
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PLASMA PHYSICS AND CONTROLLED NUCLE
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EDITORIAL NOTE The Proceedings have
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A. Kaminaga, T. Kaneko, T. Kato, M.
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Improved confinement regimes with O
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Tokamak with strong magnetic field
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Resonant island divertor experiment
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Particle removal capabilities of th
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Inside launch electron cyclotron he
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T. Hjima, S. Ishida, K. Itami, T. I
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T. Yamauchi, I. Nakazawa, K. Hasega
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ARTSIMOVICH MEMORIAL LECTURE C. MAI
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IAEA-CN-50/A-0 5 ceptible to fast r
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IAEA-CN-50/A-0 7 fusion power plant
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FIRST EXPERIMENTS IN TORE SUPRA EQU
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IAEA-CN-50/A-I-1 11 Supra is the fi
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IAEA-CN-50/A-I-1 13 poloidal field
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nee id interfere >res an j-> 1 O E
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i I •O OJ) — '5 c IS 2 HI 1ZI _
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5.' ' *[Wbl t. 3. 2. 1. _ _ X IAEA-
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nl 30 .29 .28 .27 26 .25 .24 .23 22
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IAEA-CN-50/A-I-1 However, reasonabl
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IAEA-CN-50/A-I-1 25 will make it po
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IAEA-CN-50/A-I-2 AN OVERVIEW OF TFT
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IAEA-CN-50/A-I-2 29 inner belt limi
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IAEA-CN-50/A-I-2 31 0 10 20 TOTAL P
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5 DC LU LU 3 - 1 - Q Q A 1 A IAEA-C
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IAEA-CN-50/A-I-2 35 The question ar
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0.20 0.15 0.10 Rp= 2.45 m a = 0.79
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: . • • 1 IAEA-CN-50/A-I-2 39 1
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LATEST JET RESULTS AND FUTURE PROSP
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Parameter Plasma major radius (Ro)
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1500 IAEA-CN-50/A-I-3 45 2 4 I, (MA
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IAEA-CN-50/A-I-3 47 3.0 3.5 Major r
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I 15 10 5 0 IAEA-CN-50/A-I-3 49 V \
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IAEA-CN-50/A-I-3 51 Magnetic measur
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0.8 0.6 IAEA-CN-50/A-I-3 53 -0.2 12
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10 0.5 Pulse No: 15376 n(He')/ne=1.
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IAEA-CN-50/A-I-3 57 5 10 15 [Pt-dW/
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10 E X 4 H-mode y 0.2 0.4 0.6 0.8 1
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IAEA-CN-50/A-I-3 61 where V is the
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IAEA-CN-50/A-I-3 63 confinement deg
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IAEA-CN-50/A-I-3 65 References [1 ]
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68 JT-60 TEAM T. TANAKA, Y. TANAKA,
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Ip = 3.2 MA lp = 2.7 MA JT-60TEAM R
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72 JT-60TEAM E5695 0 1 2 3 4 5 6 7
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74 JT-60TEAM 3 : LIH *3.1HA 2.8HA A
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76 JT-60TEAM 4.5 5.0 5.5 6.0 6.5 7.
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78 JT-60TEAM 250 "(a) 200 150 50 n
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80 JT-60 TEAM The further developme
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STABILITY OF HIGH BETA DISCHARGES I
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IAEA-CN-50/A-II-l 85 a typical plas
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0.5- 0- 0.8- 0.4- 0.0- IAEA-CN-50/A
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IAEA-CN-50/A-IM 89 absence of the l
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s.o • .5 (a) IAEA-CN-50/A-II-l 91
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IAEA-CN-50/A-II-l 93 stability limi
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IAEA-CN-50/A-II-l 95 [6] STAMBAUGH,
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98 OKABAYASHI et al. PBX-M maximall
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100 1 .0 .6 .0 -.2 -.4 -.6 1.11 CO
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102 0.5 OKABAYASHI et al. Indentati
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104 OKABAYASHI et al. 40 30 I I I I
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106 OKABAYASHI et al. §1 •a J i
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108 OKABAYASHI et al. -2 1 • •
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MHD ACTIVITIES AND RELATED IMPURITY
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0.5 IAEA-CN-50/A-H-3 113 FIG. 1. St
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0) a. II E IAEA-CN-50/A-H-3 115 1 1
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IAEA-CN-50/A-II-3 117 These observa
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6. CONCLUSIONS IAEA-CN-50/A-II-3 11
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122 GAO et al. With hydrogen plasma
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124 GAO et al. P—3.0 r—8.5 SHOT
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126 GAO et al. a) M >
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128 GAO et al. 0.6 0.3 0.0 50 100 r
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SUPERLOW DENSITY EXPERIMENT ON HT-6
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IAEA-CN-50/A-n-S-l 133 (b) Hard X-r
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IAEA-CN-SO/A-n-5-l 135 0 0.2 0.4 0:
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IAEA-CN-50/A-D-5-2 INVESTIGATION OF
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0.14 0.10 0.09 0.08 0.05 0.04 0.03
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TABLE I. REDUCTION OF Xe (m 2 -s')
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IAEA-CN-50/A-II-5-2 143 (3) The lin
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146 FUSSMANN et al. Abstract IMPROV
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148 FUSSMANN et al. 150- 100- 50- 0
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150 FUSSMANN et al. UJ 100- 50- + 2
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152 FUSSMANN et al. In both regimes
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154 FUSSMANN et al. reduced. With c
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156 FUSSMANN et al. and consequentl
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THE JET H-MODE AT HIGH CURRENT AND
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IAEA-CN-50/A-IH-2 achieve an H-mode
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6.0 40 2.0 (a) 0l=. 5.0 (c) 0 Pulse
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IAEA-CN-50/A-III-2 165 reduced in t
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IAEA-CN-50/A-HI-2 167 near the firs
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IAEA-CN-50/A-III-2 169 plasmas with
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I 3s H-mode 8
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IAEA-CN-50/A-HI-2 173 The steep tem
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IAEA-CN-50/A-III-2 175 available),
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IAEA-CN-50/A-III-2 177 (xi0 19 m 3
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IAEA-CN-50/A-III-2 179 APPENDIX I T
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IAEA-CN-50/A-IH-2 181 [16] Bishop,
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184 ZARNSTORFT et al. Abstract TRAN
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186 ZARNSTORFF et al. X-ray spectro
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188 ZARNSTORFF et al. 8 CM e CM E 2
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190 ZARNSTORFF et al. 1.5 2.0 2.5 n
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IAEA-CN-50/A-III-4 ENERGY CONFINEME
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o O •
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0.3 0.2- 0.1- 0.0 0.8 0.6 0.4 0.2 0
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00 d f CM I- CQ i o o o IAEA-CN-50/
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E m F LU LJU Z o N_ CE UU o / UJ q
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IAEA-CN-50/A-m-4 203 The TB values
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IAEA-CN-50/A-HM 205 [7] OHYABU, N.,
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208 SUZUKI et al. favourable in a c
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210 SUZUKI etal. As the neutral bea
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212 SUZUKI et al. 3. FOUR-PELLET IN
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HEATING OF PEAKED DENSITY PROFILES
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Yd o g a> - c 4 _n ...— 0) n 12 t
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1.3 I" 1 |03 C 0.5 i: 12 8 4 n - Te
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IAEA-CN-50/A-IV-l 221 1 2 3 Q,_-2ff
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2 q(o) 1- 10 1 U • O • IAEA-CN-
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0.3 f0.2 1 5" 0.1 IAEA-CN-50/A-IV-l
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IAEA-CN-50/A-IV-l 227 APPENDIX I TH
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IAEA-CN-50/A-IV-2 PELLET INJECTION
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3 - 2 - 1 - IAEA-CN-50/A-IV-2 231 1
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0 FIG. 4. ONI O £ at o ID c IC 15
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IAEA-CN-50/A-IV-2 0.35 MW 2.6 MW Ga
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IAEA-CN-50/A-IV-2 237 finement. The
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240 AZIZOV et al. TABLE I. TSP PARA
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242 AZIZOV et al. 65 75 85 95 105 1
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244 AZIZOV et al. 30 40 50 60 Ip =
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HIGH TEMPERATURE EXPERIMENTS AND FU
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IAEA-CN-50/A-IV-4 249 FIG. 1. Data
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P ICRHV 2 IAEA-CN-50/A-IV-4 251 FIG
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IAEA-CN-SO/AIV-4 253 FIG. 4. (a) Di
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IAEA-CN-50/A-IV-4 255 The fusion pe
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258 STRACHAN et al. - Z - 1, Steady
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260 STRACHAN et al. 10' 10' Classic
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262 STRACHAN et al. _ 1 s 10* I : 1
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ENERGY CONFINEMENT WITH AUXILIARY H
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E6950(Bi=4.0T) E6956(Bt = 2.7T) °4
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E7558 • IMPROVED 5 6 TIME (S) IAE
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7.0 E - 1 0.0 7.0 0.0 =— \ n; - T
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IAEA-CN-50/A-V-1 273 [9] SHIMOMURA,
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276 ASHRAF et al. However, the conv
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278
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280 ASHRAF et al. Modulation amplit
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282 KIMet al. (a) (b) 410 420 TIME
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284 KIM et al. (b) o 3
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286 KIM et ah In summary, we observ
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288 KAWAHATA et al. TEXT tokamak, t
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290 KAWAHATA et al. ^ 30 °- S-200.
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292 KAWAHATA et al. 0 6 12 18 24 ra
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294 WOOTTON et al. 1. Particle tran
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296 10' N 10° E gio- 1 O (a) 10" 0
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298 WOOTTON et al. ne=3xl0 19 m- 3
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300 ZURRO et al. FIG. 1. Variation
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302 ZURRO et al. Mo) 6 (10"cm- 3 )
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304 ZURRO et al. -140 50 100 f(kHz)
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TRANSPORT STUDIES ON TFTR UTILIZING
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IAEA-CN-50/A-V-4 309 uses the TRANS
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5 g 30 20 < 2.0 Q § 1.0 i 0.5 10 1
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IAEA-CN-50/A-V-4 313 the laser-blow
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IAEA-CN-S0/A-V-4 315 on working gas
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I0 7 ! 10' 1.8 IAEA-CN-50/A-V-4 317
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IAEA-CN-50/A-V-4 319 The difference
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IAEA-CN-50/A-V-4 321 [12] RADEZTSKY
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324 DONNE et al. E CO o FIG. 1. Sho
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326 DONNE et al. 350 300 250 200 15
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328 DONNE et al. 1.0 0.8 - 0.6 - t
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RECENT TEXTOR RESULTS TEXTOR TEAM (
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IAEA-CN-50/A-VI-l 333 line-radiatio
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IAEA-CN-50/A-VI-l 335 These measure
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q(r] 3- 2- 1- - IAEA-CN-50/A-VI-l 3
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IAEA-CN-50/A-VI-l 339 FIG. 4. Sawto
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IAEA-CN-S0/A-VI-2-1 RESONANT ISLAND
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IAEA-CN-50/A-VI-2-1 343 • «• >
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IAEA-CN-50/A-VI-2-1 345 tons. This
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348 EVANS et al. JIPP T-IIU ( minor
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350 EVANS et al. FIG. 3. High speed
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352 EVANS et al. REFERENCES [1] KAR
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354 BAKOS et al. The radiation of t
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356 BAKOS et al. < + s 5 2 1 5 2 10
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358 BAKOS et al. REFERENCES [1] BAK
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360 STfiCKEL et al. A quantitative
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362 STOCKEL et al. This and other f
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364 STOCKEL et al. 15 I 10 "" 5 0 (
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GLOBAL POWER BALANCE AND LOCAL HEAT
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0.5 1 r. (s> Goldston IAEA-CN-50/A-
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IAEA-CN-50/A-VH-l 371 Separate Elec
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IAEA-CN-50/A-VII-l 373 4. SIMULATIO
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6. CONCLUSIONS IAEA-CN-50/A-VII-l 3
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SAWTOOTH ACTIVITY AND CURRENT DENSI
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-0.6 (keV) 6.6 6.4 6.2 6.0 5.8 IAEA
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IAEA-CN-50/A-VII-2 381 #15697 . 0 1
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IAEA-CN-50/A-VII-2 383 radius. In a
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IAEA-CN-50/A-VH-2 385 [11] Goldston
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388 NAGAYAMA et al. of the magnetic
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390 NAGAYAMA et al. RECONNECTION RE
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392 NAGAYAMA et al. m/n=2/1 island
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STABILITY OF TFTR PLASMAS IAEA-CN-5
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IAEA-CN-50/A-VII-4 397 the electron
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9 8 — 7 6 5 4 - 3 2 X • * • i
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0.5 ' 0.4 0.3 - 3 0.2 0.1 - 0 —r"
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0.4 0.3 0.2 0.1 n IAEA-CN-50/A-VH-4
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Ip(MA) 0.85 0.89 0.9 0.9 1.4 IAEA-C
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IAEA-CN-50/A-VH-4 407 ACKNOWLEDGMEN
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410 AGIM et al. , , , , I , , , .,
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412 AGIM et al. to diminish and the
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414 AGIM et al. Hence, the preventi
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416 MAUELetal. Small tokamak plasma
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418 MAUELetal. 3. Mode structure of
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420 100- 350 MAUEL et al. RAOIUS (c
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STUDY OF PLASMA MHD STABILITY IN T-
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1.5 _ 1.0 >
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20 £ 15 - " 10 II 5 5 — ECH IAEA
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200 - IAEA-CN-S0/A-Vn-7 429 I I I I
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60 40 20 n / l IAEA-CN-S0/A-VII-7 4
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LU 30 - 20 - 10 - IAEA-CN-50/A-V1I-
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as if 200 - 100 -- 20 - I 10 - 15
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RELAXATION OF q PROFILE IN A HIGH B
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0 0.5 1.0 IAEA-CN-50/A-VII-8 439 .
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0 6 12 (Wall) r(cm) IAEA-CN-50/A-VH
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5. CONCLUSIONS IAEA-CN-50/A-VH-8 44
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446 HENDERetal. An alternative meth
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448 HENDER et al. and Jdriven(max)
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450 HENDER et al. TJ :? Island V 6
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IAEA-CN-50/A-VII-10 PARTICLE REMOVA
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IAEA-CN-50/A-VH-10 455 3. POLOIDAL
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X > o S 6 U- 2- 0 160 • 80 0 1 0.
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IAEA-CN-S0/A-VH-10 459 between scoo
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THE ROLE OF LIMITERS AND WALLS IN I
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Shine through IAEA-CN-50/A-VH-ll 46
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3 01 £ "c t=! o E c 12 10 8 6 4 2
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THE PLASMA BOUNDARY IN JET IAEA-CN-
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o x CO o 3.0 2.0 .2-0.5 'in c 0.3 1
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1 10" IAEA-CN-50/A-VI1-12 LCFS LCFS
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o •£ 0.15 'o = 0.05 C O J3 o 0.0
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IAEA-CN-50/A-VIM2 475 densities, bu
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478 LEONOV et al. 2. INSTALLATION A
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480 LEONOV et al. &r (cm) 0.2 -0.2
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482 LEONOV et al. Uo, at constant p
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484 CHEETHAM et al. We present simu
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486 CHEETHAM et al. 0 20 40 60 30 1
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488 CHEETHAM et al. o LU 3.0 2.8
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490 CHEETHAM et al. sior CO 111 c o
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492 CHEETHAM et al. reported from o
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IAEA-CN-S0/A-Vn-15 EXPERIMENTAL RES
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IAEA-CN-50/A-VII-15 497 800 (a) _ -
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IAEA-CN-50/A-VII-15 499 formation.
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300 4X10' 3 - IAEA-CN-50/A-VII-15 5
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CONCLUSION IAEA-CN-50/A-VU-1S 503 W
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506 KIKUCH1 et al. 1. INTRODUCTION
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508 KIKUCHI et al. 1.0 o.s 1 — -
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510 KIKUCHIetal. REFERENCES [1] ZAR
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STUDY OF DENSITY LIMIT AND LOW q(aL
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IAEA-CN-50/E-I-l-l 515 1 2 3 4 5 ne
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/ / IAEA-CN-50/E-I-l-l 517 / / / /
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(J n 3 o ? 2 i o ' 1 IAEA-CN-50/E-M
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0.03 - 0.02 - 0.01 - IAEA-CN-50/E-I
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CO u CO "o IC 7 - 6 — 5 - 4 - 3 1
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IAEA-CN-50/E-I-l-l REFERENCES 52 5
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528 PRATER et al. 1. INTRODUCTION E
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530 PRATER et al. 0.8 0.6 0.4 0.2 n
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532 PRATER et al. 1.5 x 10 19 m~ 3
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534 PRATER et al. 10 1 0.75 0.25 0.
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536 PRATER et al. added to 1.25 MW
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538 PRATER et al. 2.0 1.5 1.0 0.5 /
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INSIDE LAUNCH ELECTRON CYCLOTRON HE
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0-20 0-15 a CO. 0-10 0-05 0-0 5S g.
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IAEA-CN-50/E-I-3 545 0.25 • (a) 1
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IAEA-CN-50/E-I-3 547 A/3 deduced fr
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IAEA-CN-50/E-I-3 549 ECRH phases as
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552 MOTOJIMA et al. ICRF and plasma
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554 MOTOJIMA et al. (a) 0.6SneS0.9x
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556 MOTOJIMA et al. 0 20 W 60 80 10
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558 5 4 3 2 1 0 60 40 20 0 la) cuto
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560 MOTOJIMA et al. 3 0.005 0 0.2 0
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RF CURRENT DRIVE AND MHD INSTABILIT
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IAEA-CN-50/E-I-5 565 80 PEC
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of x o o i L_ t IAEA-CN-50/E-I-5 56
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IAEA-CN-50/E-I-5 569 FIG. 5. Contou
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HEATING AND CONFINEMENT STUDIES WIT
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R 6 IAEA-CN-50/E-IM 0.5 10 1.5 Ne(r
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IAEA-CN-50/E-II-l FIG. 3. Total rad
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IAEA-CN-50/E-II-l 577 1.0 2.0 Time
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IAEA-CN-50/E-II-l 579 TABLE I. SUMM
Page 607 and 608:
6. SAWTOOTH BEHAVIOUR IAEA-CN-50/E-
Page 609 and 610:
IAEA-CN-50/E-II-2 LONG PULSE HIGH P
Page 611 and 612:
IAEA-CN-50/E-II-2 585 23996 2 3 0 U
Page 613 and 614:
IAEA-CN-50/E-II-2 587 TABLE I. a) C
Page 615 and 616:
t a ce> 03 E cs o. otal 100 90 80 7
Page 617 and 618:
IAEA-CN-50/E-H-2 591 and confinemen
Page 619 and 620:
IAEA-CN-50/E-n-3 EXPERIMENTAL AND T
Page 621 and 622:
§ 1PUTUDE ( $ #•14613 200 (a) 18
Page 623 and 624:
IAEA-CN-50/E-II-3 597 The results o
Page 625 and 626:
to V. (a)' • \ \ \ \ \ \ w \'\ \\
Page 627 and 628:
IAEA-CN-50/E-II-3 601 cccurs progre
Page 629:
IAEA-CN-50/E-II-3 603 [5] CAMPBELL,
Page 632 and 633:
606 FUJII et al. 1. INTRODUCTION Se
Page 634 and 635:
608 140 " (0,0) PIC= l~ 3 MW 120 '
Page 636 and 637:
610 FUJII et al. ACKNOWLEDGEMENTS T
Page 638 and 639:
612 BATCHELOR et al. resolves this
Page 640 and 641:
614 BATCHELOR et al. •J5 1
Page 642 and 643:
616 BATCHELOR et al. to match asymp
Page 644 and 645:
618 BATCHELOR et al. of T, R, and C
Page 646 and 647:
620 BATCHELOR et al. [3] SMITHE, D.
Page 648 and 649:
622 USHIGUSA et al. 1. INTRODUCTION
Page 650 and 651:
624 USHIGUSA et al. at f = 1.74 GHz
Page 652 and 653:
626 USHIGUSA et al. BT (T) (ms) ao
Page 654 and 655:
628 USHIGUSA et al. [2] JT-60 TEAM,
Page 656 and 657:
630 ITOH et al. , Breakdown 20 40 6
Page 658 and 659:
632 ITOH et al. 1.0 20 30 40 50 60
Page 660 and 661:
634 ITOH et al. 30 |20 a "" 10 n H=
Page 662 and 663:
636 ITOH et al. REFERENCES [1] ITOH
Page 664 and 665:
638 ALLADIO et al. generation of hi
Page 666 and 667:
640 ALLADIO et al. 4 T (keV) 3 2 -
Page 668 and 669:
642 ALLADIO et al. 3 ID 10 2 10' 10
Page 671 and 672:
IAEA-CN-50/E-ID-4 LOWER HYBRID WAVE
Page 673 and 674:
1000 - 500 1001— o — 2 35 IAEA-
Page 675 and 676:
10 10* 10 10 IAEA-CN-50/E-HI-4 649
Page 677 and 678:
IAEA-CN-50/E-III-4 651 density of t
Page 679 and 680:
IAEA-CN-50/E-IU-4 653 I I I I I I F
Page 681 and 682:
CURRENT DRIVE AND CONFINEMENT OF AN
Page 683 and 684:
1.0 -0.5 o - - 4.0 IAEA-CN-50/E-III
Page 685 and 686:
IAEA-CN-50/E-III-5 659 TABLE I. SUM
Page 687 and 688:
IAEA-CN-SO/E-in-S 661 0.4 RADIUS (m
Page 689 and 690:
10' Convection Dominates IAEA-CN-50
Page 691 and 692:
IAEA-CN-50/E-III-5 665 versus unbal
Page 693:
IAEA-CN-50/E-III-5 667 [11] ZARNSTO
Page 696 and 697:
670 SIMONEN et al. Neutral beam cur
Page 698 and 699:
672 SIMONEN et al. 1.6 2.0 FIG. 3.
Page 700 and 701:
674 SIMONEN et al. MHD modes, obser
Page 702 and 703:
676 SIMONEN et al. toroidal drift o
Page 704 and 705:
678 SIMONEN et al. occurs near the
Page 707 and 708:
NEW CURRENT DRIVE AND CONFINEMENT T
Page 709 and 710:
IAEA-CN-50/E-III-7 683 is typically
Page 711 and 712:
IAEA-CN-S0/E-III-7 685 plasma beta
Page 713 and 714:
IAEA-CN-50/E-III-7 687 The equilibr
Page 715:
IAEA-CN-50/E-III-7 689 [8] McGUIRE,
Page 718 and 719:
692 100 a 10- 0.1 WILSON et al. •
Page 720 and 721:
694 WILSON et al. 3. Plasma Heating
Page 722 and 723:
696 WILSON et al. I 3 i - • / Tim
Page 725 and 726:
INVESTIGATION OF ICRH ON THE TUMAN-
Page 727 and 728:
~x o X •9to 12 1 11 10 180 s - 12
Page 729 and 730:
400 - 300 - 200 - I 100 - 35 / 1 ,
Page 731 and 732:
5 - IAEA-CN-50/E-IV-2 r (cm) FIG. 7
Page 733 and 734:
IAEA-CN-50/E-IV-3 CONVERSION AND CY
Page 735 and 736:
IAEA-CN-50/E-IV-3 709 bution, e(j,
Page 737 and 738:
IAEA-CN-S0/E-IV-3 711 FIG. 3. kxPd
Page 739 and 740:
IAEA-CN-50/E-IV-3 713 3. NON-LOCAL
Page 741 and 742:
x exp | ds" ' u ' x -oosgn u d fiV2
Page 743 and 744:
IAEA-CN-50/E-IV-3 717 x If {sin i [
Page 745:
IAEA-CN-5O/E-IV-3 719 2. A non-loca
Page 748 and 749: 722 MOREAU et al. =t _» Here, K is
Page 750 and 751: 724 MOREAU et al. FIG. 1. Modulus o
Page 752 and 753: 726 MOREAU et al. REFERENCES [1] MA
Page 754 and 755: 728 YASAKA et al. 2. EFFICIENT PLAS
Page 756 and 757: 730 YASAKA et al. '£ 1 0.5 0 4 Pne
Page 758 and 759: 732 YASAKA et al. WT-3 1 2 Q,f C 10
Page 760 and 761: 734 invi p o p p •^ CJ -^ o IO o
Page 762 and 763: 736 YAMAMOTO et al. (A) OJ — o (A
Page 764 and 765: 738 YAMAMOTO et al. of Tsx =1.5 keV
Page 766 and 767: 740 PEREVERZEV current drive produc
Page 768 and 769: 742 PEREVERZEV 300 - - 150 ne (10 1
Page 770 and 771: 744 PEREVERZEV 0.2- -0.2- 0.1X10 19
Page 772 and 773: 746 PEREVERZEV The dependences of l
Page 774 and 775: 748 PORKOLAB et al. ASPECT RATIO FI
Page 776 and 777: 750 PORKOLAB et al. 1.0 _, 0.8 1 0.
Page 778 and 779: 752 PORKOLAB et al. X D E o Q_ 1.8
Page 780 and 781: 754 LUO et al. - o £ 3 §. II Ml "
Page 782 and 783: 756 LUO et al. 20 10 ATe ( 1 m11 1
Page 785 and 786: IAEA-CN-50/E-IV-10 MICROWAVE HEATIN
Page 787 and 788: n MCPAT _ Analysis IAEA-CN-50/E-IV-
Page 789 and 790: IAEA-CN-50/E-IV-10 763 3. QUASI-LIN
Page 791 and 792: IAEA-CN-50/E-IV-10 765 In the limit
Page 793 and 794: IAEA-CN-50/E-IV-ll SECOND ELECTRON
Page 795 and 796: IAEA-CN-50/E-IV-ll 769 FIG. ]. Real
Page 797: -0.2 IAEA-CN-50/E-IV-ll 771 FIG. 3.
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