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Propagation of plasma beams across the magnetic field

机译:等离子体束在磁场中的传播

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Abstract: Beams of charge- and current-neutralized plasma will cross a transverse-magnetic field by a combination of collective-plasma processes. These processes were studied for a high-to-low beta ($beta $EQV plasma energy density/magnetic field energy density) hydrogen-plasma beam injected into a vacuum transverse magnetic field with nominal parameters: $Tau$-i$/ $APEQ 1 eV, $Tau$-e$/ $APEQ 5 eV, n $LSEQ 10$+14$/ cm$+$MIN@3$/, v$-i$/ $LSEQ 9 x 10$+6$/ cm/s, t$-pulse$/ $LS 70 $mu@s, $Beta$-z$/ $LSEQ 300 G. Plasma characteristics were measured for a wide beam, a/$-$Rho@(i)$/ $LSEQ 35, and a downstream distance, x $LSEQ 300 $-$Rho@(i)$/, where a is the beam radius, x is the downstream distance, and $-$Rho@(i)$/ is the ion gyroradius. A brief state of initial diamagnetic propagation is observed, followed by a rapid transition to $E@x$B propagation. $E@x$B propagation is accompanied by beam compression transverse to $B with as much as a factor of four increase in density and a slight drift of the beam in the ion Lorentz force direction. As the magnetic field increases, the observed magnetization time decreases from that calculated using classical Spitzer conductivity, approaching an order of magnitude. This rapid magnetization can be accounted for using classical Hall conductivity, rather than invoking anomalous processes or instabilities to calculate the magnetization time.!
机译:摘要:电荷和电流中和的等离子体束将通过集合等离子体过程的组合横穿横向磁场。对这些过程进行了研究,以从高到低的beta($ beta $ EQV等离子能量密度/磁场能量密度)氢等离子束注入真空横向磁场,其标称参数为:$ Tau $ -i $ / $ APEQ 1 eV,$ Tau $ -e $ / $ APEQ 5 eV,n $ LSEQ 10 $ + 14 $ / cm $ + $ MIN @ 3 $ /,v $ -i $ / $ LSEQ 9 x 10 $ + 6 $ / cm / s,t $ -pulse $ / $ LS 70 $ mu @ s,$ Beta-z $ / $ LSEQ 300 G.测量宽光束的等离子体特性,a / $-Rho @(i)$ / $ LSEQ 35和下游距离x $ LSEQ 300 $-$ Rho @(i)$ /,其中a是波束半径,x是下游距离,$-$ Rho @(i)$ /是离子陀螺半径。观察到初始反磁传播的简要状态,然后迅速过渡到$ E @ x $ B传播。 $ E @ x $ B传播伴随着横向于$ B的束压缩,密度增加了四倍,并且束在离子洛伦兹力方向上发生了轻微的漂移。随着磁场的增加,观察到的磁化时间会比使用经典Spitzer电导率计算的时间缩短,接近一个数量级。可以使用经典的霍尔电导率来解决这种快速的磁化问题,而不是调用异常过程或不稳定性来计算磁化时间。

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