更新马戈进展

S. Garanin, V. Mamyshev, V. B. Yakubov
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引用次数: 7

摘要

该研究领域在俄罗斯被称为MAGO(俄语缩写为磁内爆),在美国被称为MTF(磁化靶聚变),是主要CTF方法(磁约束系统和惯性约束聚变)的替代方案。MAGO/MTF方法包括两个阶段:首先产生适合进一步压缩的磁化热等离子体(磁场~0.1 mg,具有闭合场线配置;等离子体密度~10 cm-3,温度-300 eV,杂质含量少,因为杂质会造成辐射损失)。2. 然后利用强大的驱动器(如爆炸磁发生器、肌电图)对等离子体进行准绝热压缩(速度约为1cm /mus),并使其参数达到符合劳森准则的值。这里有必要提供~10-5 s的等离子体寿命。为了实现这一方法,必须结合两个基本要素:热磁等离子体产生系统和高能压缩系统。在MAGO腔室中,制备出了高度5- 8cm、外半径6- 10cm、内半径0.9-1.2 cm的圆柱形DT等离子体,其参数为:平均密度8ldr10 cm-3,平均温度200-250 eV,等离子体中特征方位磁场~0.15 MG。在VNIIEF/LANL联合实验hel1中,获得了在压缩阶段达到点火所需参数(~25 MJ能量,~0.8 cm/mus速度)的衬里。用与hel1实验参数相近的直线压缩纯等离子体的内径和二维计算表明,在这种情况下可以产生符合Lawson准则特征的等离子体。然而,在x射线二极管的初步加热实验中获得的数据表明,等离子体寿命~2-3 μ s,不足以保证在压缩中点火。计算和实验结果表明,杂质对等离子体的污染和杂质对等离子体的辐照是导致MAGO等离子体冷却的重要机制。等离子体污染可能是由于等离子体与绝缘体蒸气混合(可由//推力放电产生)和等离子体冲刷壁材造成的。在MAGO腔室的等离子体压缩过程中,从腔室壁上冲出的质量可能比预热阶段的质量还要大。因此,在MAGO室中进行DT等离子体压缩实验时,应使用轻质材料(碳、铍或锂作壁,氧化铍、碳化硼、氮化硼作绝缘体)。使用轻质材料作为腔壁和绝缘体可以增加等离子体的寿命,使等离子体适合于衬里等离子体实验。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Update on Mago Progress
The research area known as MAGO (Russian abbreviation for magnetic implosion) in Russia and as MTF (Magnetized Target Fusion) in the United States is an alternative to the main CTF approaches (magnetic confinement systems and inertial confinement fusion). The MAGO/MTF approach consists of two phases: 1. First magnetized hot plasma is produced suitable for further compression (with magnetic field ~0.1 MGs having a closed field line configuration; the plasma is of density ~10 cm-3, temperature -300 eV, and small impurity content, as impurities can contribute to the losses caused by radiation). 2. Then the plasma is compressed in the quasi-adiabatic manner by liners (at velocities on the order of 1 cm/mus) using powerful drivers (e. g., explosive magnetic generators, EMG) and its parameters are brought to the ones meeting the Lawson criterion. Here it is necessary to provide the plasma lifetime of ~10-5 s . To implement this approach, it is necessary to combine two essential elements: hot magnetized plasma generation system and highly energetic compression system. In the MAGO chambers, DT plasma of the following parameters has been produced in a cylindrical bulk with 5-8 cm height, 6-10 cm outer radius, and 0.9-1.2 cm inner radius: average density 8ldr10 cm-3 , average temperature 200-250 eV , characteristic azimuthal magnetic field in the plasma ~0.15 MG . In the joint VNIIEF/LANL experiment HEL-1 a liner with the parameters (~25 MJ energy, ~0.8 cm/mus velocity) necessary to reach ignition at compression stage was obtained. As ID and 2D computations of pure plasma compression by a liner with the parameters close to those in the experiment HEL-1 show, the plasma with the characteristics corresponding to the Lawson criterion can be produced in this case. However, the data obtained in preliminary heating experiments using X-ray diodes, suggests ~2-3 mus plasma lifetime, which is insufficient to ensure the ignition in compression. Basing on the computed and experimental data one can conclude that the most important mechanism that contributes to MAGO plasma cooling is contamination of the plasma with impurities and it's cooling due to irradiation on impurities. This plasma contamination can result from the plasma mixing with the insulator vapors (which can be produced from //-pushed discharge) and wall material washout by the plasma. During the plasma compression in the MAGO chamber the mass washed out from the chamber walls can be even larger than that at the preheating phase. So light materials (carbon, beryllium or lithium for walls, beryllium oxide, boron carbide, boron nitride for insulator) should be used in experiments on DT plasma compression in the MAGO chamber. Using light materials for the chamber walls and insulator can increase the plasma lifetime and make the plasma suitable for the liner-plasma experiments.
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