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AXISYMMETRIC SCATTERING OF p MODES BY THIN MAGNETIC TUBES

机译:薄磁管对p模式的轴对称散射

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We examine the scattering of acoustic p-mode waves from a thin magnetic fibril embedded in a gravitationally stratified atmosphere. The scattering is mediated through the excitation of slow sausage waves on the magnetic tube, and only the scattering of the monopole component of the wave field is considered. Since such tube waves are not confined by the acoustic cavity and may freely propagate along the field lines removing energy from the acoustic wave field, the excitation of fibril oscillations is a source of acoustic wave absorption as well as scattering. We compute the mode mixing that is achieved and the absorption coefficients and phase shifts. We find that for thin tubes the mode mixing is weak and the absorption coefficient is small and is a smooth function of frequency over the physically relevant band of observed frequencies. The prominent absorption resonances seen in previous studies of unstratified tubes are absent. Despite the relatively small absorption, the phase shift induced can be surprisingly large, reaching values as high as 15° for f modes. Further, the phase shift can be positive or negative depending on the incident mode order and the frequency.
机译:我们检查了嵌入在重力分层大气中的薄磁纤维的声p模波的散射。散射是通过磁管上的慢香肠波的激发来介导的,仅考虑波场的单极子分量的散射。由于这种管波不受声腔限制,而是可以沿磁力线自由传播,从而从声波场中去除能量,因此原纤维振荡的激发是声波吸收和散射的来源。我们计算实现的模式混合以及吸收系数和相移。我们发现,对于细管,模式混合很弱,吸收系数很小,并且是在观测频率的物理相关频带上频率的平滑函数。以前的未分层管研究中没有看到明显的吸收共振。尽管吸收量相对较小,但感应出的相移却可能非常大,对于f模式,其达到高达15°的值。此外,取决于入射模式顺序和频率,相移可以是正的或负的。

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