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Effective Length of a Receiving Antenna in a Streaming Plasma

机译:流等离子体中接收天线的有效长度

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摘要

The root-mean-square (r.m.s) voltage induced on a receiving dipole antenna by incident potential waves in a streaming otherwise isotropic plasma in the resonance frequency band is calculated. The open-circuit voltage on antenna terminals is the product of the wave electric field strength at the receiving point and the effective length of the receiving antenna$L_eff$. The effective length differs substantially from that in a non-streaming plasma for waves propagating downstream at frequencies close to the plasma frequency. The case of stream velocity lower than the electron thermal velocity is considered, which is of interest for wave measurements in the solar wind. We discuss some implications for relevant experiments in space plasmas, namely the appearance of narrowband lines in the spectra around local plasma frequency observed in the solar wind. The possible exaggeration of plasma wave amplitudes in conventional interpretations of measurements is pointed out.
机译:计算在谐振频带中流动的各向同性等离子体中入射电势波在入射偶极子天线上感应出的均方根(r.m.s)均方根电压。天线端子上的开路电压是接收点处的波电场强度与接收天线的有效长度$ L_eff $的乘积。对于在接近等离子体频率的频率向下游传播的波,有效长度与非流动等离子体的有效长度大不相同。考虑流速度低于电子热速度的情况,这对于太阳风中的波测量很重要。我们讨论了空间等离子体相关实验的一些含义,即在太阳风中观察到的局部等离子体频率附近的光谱中出现了窄带线。指出了在传统的测量解释中等离子波幅度的可能夸大。

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