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Radiation resistance of a short dipole immersed in a cold magnetoionic medium

机译:浸入冷磁离子介质中的短偶极子的抗辐射性

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摘要

Electromagnetic radiation from sources immersed in a cold magnetoplasma is analyzed by the use of ‘principal-polarized’ wave coordinates; and the wave fields, the mean complex radiated power, and the Poynting vector are systematically expressed in terms of ‘polarized' wave modes. For each polarized wave mode, the medium is effectively isotropic, since the Fourier-transformed wave equation for each principal mode is decoupled and is similar to the one obtained from the usual scalar Helmholtz operator. In application of the theory, consideration is made of the radiation resistance of a linear electric antenna of moderate length oriented both parallel and perpendicular to the static magnetic field. Approximate closed form expressions for the radiation resistance are obtained for the VLF frequency range by using a plasma model appropriate to the magnetosphere. These approximate closed form expressions are compared with the results obtained previously by other workers using a quasi-static approximation, and it is shown that excellent agreement exists between the two methods of analysis. It is concluded that the quasi-static approximation can accurately predict the radiation resistance of a linear antenna in the magnetosphere, given certain moderate restrictions on the antenna length.
机译:通过使用“主极化”波坐标来分析浸没在冷磁等离子体中的辐射源产生的电磁辐射;波场,平均复数辐射功率和坡印廷矢量都用“极化”波模来系统表示。对于每个极化波模式,介质都是有效各向同性的,因为每个主模式的傅立叶变换波动方程都是解耦的,并且与从通常的标量亥姆霍兹算子获得的方程相似。在该理论的应用中,考虑了平行于和垂直于静磁场的中等长度的线性电天线的辐射电阻。通过使用适合磁层的等离子体模型,可以在VLF频率范围内获得辐射强度的近似封闭形式。这些近似闭合形式的表达式与其他工人先前使用准静态近似得到的结果进行了比较,结果表明两种分析方法之间存在极好的一致性。结论是,在天线长度受到一定程度的适度限制的情况下,准静态近似可以准确预测磁层中线性天线的辐射电阻。

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