论文标题
平面射频磁铁等离子体中的电子动力学:ii。通过2D3V粒子/蒙特卡洛代码研究的加热和能量机制
Electron dynamics in planar radio frequency magnetron plasmas: II. Heating and energization mechanisms studied via a 2d3v particle-in-cell/Monte Carlo code
论文作者
论文摘要
本工作使用(r,z)粒子中的粒子(PIC)模拟了典型的RF驱动的轴对称磁控管排放,研究了电子传输和加热机制。结果表明,对于被考虑的磁场拓扑,电子电流通过(r,z)平面的不同通道流动:``横向''一个,涉及赛道上方的电子磁性限制区(EMCR)的电流流动,而两个”“纵向”。电子沿着各种机制从这些通道沿电场中获得能量,这些机制与维持直流驱动的磁子的能量截然不同。纵向功率吸收涉及镜面效应加热(MEH),非线性电子共振加热(NERH),磁化弹跳加热(MBH)以及在鞘层界面处的双极野战场的加热。 MEH和MBH代表了以前文献中缺少的两种新机制。 MEH是由克服在不均匀磁场中产生的镜像所需的反向电场引起的,以确保电子向动力电极的足够通量,并且MBH与电子的可能性有关,可以通过电子从纵向通道中通过ARC样磁场连接的纵向通道中膨胀鞘进行多种反射。横向通道中的电子加热主要是由于赛道上方的EMCR中基本无碰撞的大厅加热引起的,从而产生了强大的EXB方位角漂移速度。后一种机制导致有效的电子能量,即,在非弹性范围内从电场到电子的能量转移。由于该机制通过该机制启用的主要电子种群长期限制在放电中,因此其对电离过程的贡献是主要的。
The present work investigates electron transport and heating mechanisms using an (r, z) particle-in-cell (PIC) simulation of a typical rf-driven axisymmetric magnetron discharge with a conducting target. It is shown that for the considered magnetic field topology the electron current flows through different channels in the (r, z) plane: a ``transverse'' one, which involves current flow through the electrons' magnetic confinement region (EMCR) above the racetrack, and two ''longitudinal'' ones. Electrons gain energy from the electric field along these channels following various mechanisms, which are rather distinct from those sustaining dc-powered magnetrons. The longitudinal power absorption involves mirror-effect heating (MEH), nonlinear electron resonance heating (NERH), magnetized bounce heating (MBH), and the heating by the ambipolar field at the sheath-presheath interface. The MEH and MBH represent two new mechanisms missing from the previous literature. The MEH is caused by a reversed electric field needed to overcome the mirror force generated in a nonuniform magnetic field to ensure sufficient flux of electrons to the powered electrode, and the MBH is related to a possibility for an electron to undergo multiple reflections from the expanding sheath in the longitudinal channels connected by the arc-like magnetic field. The electron heating in the transverse channel is caused mostly by the essentially collisionless Hall heating in the EMCR above the racetrack, generating a strong ExB azimuthal drift velocity. The latter mechanism results in an efficient electron energization, i.e., energy transfer from the electric field to electrons in the inelastic range. Since the main electron population energized by this mechanism remains confined within the discharge for a long time, its contribution to the ionization processes is dominant.