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Endogenous and asymmetric magnetic reconnection with associated processes of relevance to fusion burning plasmas

机译:内源性和不对称磁重联,与与聚变燃烧等离子体有关的相关过程

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An endogenous magnetic reconnection process is characterized by a driving factor that lays within the layer where a drastic change of magnetic field topology occurs. This kind of process is shown to take place in the presence of an electron temperature gradient in a well-confined plasma where, referring to quasi-collisionless regimes, the resulting electron temperature fluctuations can be anisotropic. Then a class of (radially) localized reconnecting modes is identified. These involve a transverse generated field (B) over tilde (x) of odd parity (as a function of the radial variable), and have finite (phase) velocities of propagation contrary to commonly considered reconnecting modes. The widths of the relevant reconnection layers remain significant even when large macroscopic distances are considered. Given that there are plasmas in the Universe with considerable electron thermal energy contents, these features can be relied upon in order to produce magnetic field generation, or conversion of magnetic energy into particle energy when the coupling of the localized odd modes to extended even modes can be significant. In any case, the resulting magnetic islands are not symmetric. With their excitation these modes can extract momentum from the main body of the plasma column which should recoil in the opposite direction. The excitation of antisymmetric endogenous modes is shown to be relevant to the electron temperature heating due to the reaction products in a fusion burning plasma as, in this case, the longitudinal thermal conductivity on selected rational magnetic surfaces can be decreased, relative to its collisional value, by the effects of reconnection. This kind of steepening is proposed to have a role in enhancing the growth rate of the instability involved in disruption events of the plasma column. The best agreement between theory and experiments concerning the onset of magnetic reconnection is (probably) represented by the theory of the internal kink mode. The observed accelerated reconnection rate following the onset is suggested as being explained by the formation of a relatively large magnetic island with a local steepening of the electron temperature gradient. A new kind of odd 'thermonuclear heating' mode associated with symmetric reconnection is identified.
机译:内源性磁重连接过程的特征在于,驱动因子位于发生磁场拓扑急剧变化的层中。此类过程显示为在电子空间梯度有限的等离子体中发生,在这种情况下,参照准无碰撞状态,所产生的电子温度波动可以是各向异性的。然后,识别一类(径向)本地化的重新连接模式。这些涉及奇偶校验的代字号(x)上的横向生成场(B)(作为径向变量的函数),并且与通常考虑的重新连接模式相反,具有有限的(相位)传播速度。即使考虑到较大的宏观距离,相关的重新连接层的宽度仍保持显着。假设宇宙中存在具有相当大的电子热能含量的等离子体,则可以依靠这些特征来产生磁场,或者当局部奇数模与扩展偶数模的耦合可以时,将磁能转换为粒子能。有意义。在任何情况下,所得的磁岛都不对称。借助它们的激发,这些模式可以从等离子柱的主体中提取动量,该动量应沿相反的方向反冲。由于在聚变燃烧等离子体中的反应产物,反对称内生模式的激发与电子温度加热有关,因为在这种情况下,相对于其碰撞值,可以降低所选有理磁性表面上的纵向热导率,受重新连接的影响。提出这种陡峭化具有提高等离子体柱破坏事件所涉及的不稳定性的增长速率的作用。关于内部磁扭折模式的理论(可能)代表了关于磁重新连接发生的理论与实验之间的最佳一致性。建议在发生之后观察到加速的重新连接速率,这是由于形成了一个相对较大的磁岛而使电子温度梯度局部变陡而解释的。确定了一种与对称重新连接相关的新型奇数“热核”加热模式。

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