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Generalized dispersive Alfven waves

机译:广义色散Alfven波

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Generalized dispersion relations for Alfven waves are derived, accounting for arbitrary values of omega/omega (ci), k perpendicular to rho (i), and k perpendicular to lambda (e): where omega (omega (ci)) is the wave (ion gyro) frequency k(perpendicular to) = 2 pi/lambda (perpendicular to) the perpendicular (to the external magnetic field line) wavenumber and rho (i)(lambda (e)) the ion gyroradius (electron skin depth). Our dispersion relations are appropriate for deducing the relationships of the dispersive (inertial and kinetic) Alfven waves with other plasma modes. The present results can be considered as a prerequisite for understanding some salient features of the broadband eleetromagnetic/electrostatic waves that are frequently observed by the Freja and FAST spacecraft in the auroral zone of the Earth's ionosphere. [References: 20]
机译:推导了Alfven波的广义色散关系,说明了omega / omega(ci),垂直于rho(i)的k和垂直于lambda(e)的k的任意值:其中omega(omega(ci))是波(离子陀螺仪的频率k(垂直于)= 2 pi / lambda(垂直于)(垂直于(外部磁场线))波数,rho(i)(λ)(e)离子陀螺仪半径(电子趋肤深度)。我们的色散关系适用于推导色散(惯性和动力学)Alfven波与其他等离子体模式的关系。当前的结果可以被认为是了解宽带电磁场/静电波的一些显着特征的前提,这些特征通常是在地球电离层极光区的Freja和FAST航天器经常观察到的。 [参考:20]

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