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Internal magnetic fluctuations and electron heat transport in the Tore Supra tokamak: Observation by cross-polarization scattering

L. Colas, X.L. Zou, M. Paume, J.M. Chareau, L. Guiziou, G.T. Hoang, Y. Michelot, D. Grésillon1998年被引用 53Nuclear FusionIF 3出版社

Magnetic fluctuations (radial size ≈ 5 mm) are measured by a cross polarization scattering (CPS) diagnostic in Tore Supra. In the scenario O + → X, only the poloidal component of the magnetic fluctuations is measured, while both the radial and the poloidal component are measured in the scenario X + → O. These fluctuations are investigated quantitatively in the ohmic and low confinement regimes over a wide range of plasma currents, densities and additional heating powers. At the same time, the electron heat diffusivities expected from these fluctuations are compared with those obtained by profile analysis. Three main results are obtained: (a) The radial profile of the poloidal magnetic fluctuations in the gradient region (0.3 < r/a < 0.7) is established from these measurements. The magnetic fluctuation levels are found to increase towards the plasma edge, and this feature is compatible with that of electron heat diffusivity. (b) A strong correlation between the measured magnetic turbulence and the local temperature gradient is observed during the additional heating. (c) The local electron heat diffusivity induced by magnetic fluctuations is estimated using the non-collisional quasi-linear formula χmage = πqRvth(δBr/B)2, where the radial component of the magnetic turbulence is assumed to be of the same order as the poloidal component. Both the order of magnitude and the parametric dependence of χmage show similarities with electron diffusivities determined by transport analysis. In particular, a threshold is observed for the dependence of fluctuation induced heat fluxes on the local temperature gradient, which is close to the critical gradient observed for the measured heat fluxes.

日本語訳

磁気揺動(半径方向サイズ ≈ 5 mm)は、Tore Supraにおいて偏光散乱(CPS)診断法により測定される。シナリオO → Xでは、磁気揺動のポロイダル成分のみが測定され、シナリオX → Oでは、半径方向成分とポロイダル成分の両方が測定される。これらの揺動は、オーミックおよび低閉じ込め領域において、広範囲のプラズマ電流、密度、追加加熱パワーにわたって定量的に調査される。同時に、これらの揺動から予想される電子熱拡散係数は、プロファイル解析から得られる値と比較される。主な結果は以下の3点である:(a) 勾配領域(0.3 < r/a < 0.7)におけるポロイダル磁気揺動の半径方向プロファイルが確立された。磁気揺動レベルはプラズマ端に向かって増加し、この特徴は電子熱拡散係数の挙動と整合する。(b) 追加加熱中には、測定された磁気乱流と局所温度勾配の間に強い相関が観測される。(c) 磁気揺動によって誘起される局所電子熱拡散係数は、非衝突準線形式 χmage = πqRvth(δBr/B)2 を用いて推定される。ここで、磁気乱流の半径方向成分はポロイダル成分と同程度であると仮定される。χmage のオーダーおよびパラメータ依存性は、輸送解析から決定される電子拡散係数と類似性を示す。特に、揺動誘起熱流束の局所温度勾配に対する依存性には閾値が観測され、これは測定された熱流束で見られる臨界勾配に近い値である。

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Tore SupraHeat transportMagnetic fluctuationsElectron heat transport
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