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Effect of β and collisionality on the vacuum magnetic field islands in stellarators

L. Garcia, B.A. Carreras, V.E. Lynch, M. Wakatani2003年被引用 9Nuclear FusionIF 3出版社

The resistive pressure gradient driven instability model is used to study the effect of plasma on a vacuum magnetic field island. Conditions under which the magnetic island is amplified or reduced have been identified. Starting with a set of reference parameters, we have varied these parameters by increasing either the density or the electron temperature. These scans lead to very different results. When β increases because of the increase in density, so does the island width. However, in cases in which β is increased by increasing the electron temperature, we observe a decrease in the island width. The main mechanism for island reduction seems to be the generation of strong sheared flow associated with the magnetic island. These results seem to reflect some observations in the Large Helical Device.

日本語訳

抵抗性圧力勾配駆動不安定性モデルを用いて、真空磁場島に対するプラズマの効果を調べた。磁気島が増幅または低減される条件を特定した。一連の基準パラメータから出発し、密度または電子温度のいずれかを増加させることによってこれらのパラメータを変化させた。これらの走査は非常に異なる結果をもたらす。密度の増加によりβが増加すると、島幅も増加する。しかしながら、電子温度を上げることによってβが増加する場合には、島幅の減少が観測される。島の低減の主なメカニズムは、磁気島に関連する強いシアー流の生成であると思われる。これらの結果は、大型ヘリカル装置におけるいくつかの観測結果を反映していると思われる。

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lhd中精度(概要文一致)

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StellaratorCollisionality
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