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Fine Structure of the Emission Spectra of a Relativistic Cherenkov Plasma Maser

机译:相对论的契伦科夫等离子体Maser的发射光谱的精细结构

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摘要

The evolution of the emission spectrum of a relativistic Cherenkov plasma maser is studied both experimentally and numerically. The frequency range of emission is 1.5-6 GHz at a power level of 50 MW and pulse duration of up to 500 ns. It is shown that the relativistic Cherenkov plasma maser is capable of producing both broadband (with a spectrum width of ~1 GHz) and narrowband (≈40 Mhz) microwave pulses with a tunable mean frequency. Calculations by linear theory and numerical simulations provide a satisfactory explanation of the specific features and the time evolution of the spectra observed. It is suggest that the plasma nonlinearity is responsible for the experimentally observed shortening of the microwave pulses and the broadening of the emission spectrum.
机译:通过实验和数值研究了相对论的契伦科夫等离子体激射器的发射光谱的演化。发射的频率范围是1.5-6 GHz,功率水平为50 MW,脉冲持续时间最长为500 ns。结果表明,相对论的切伦科夫等离子体激射器能够产生具有可调平均频率的宽带(频谱宽度约为1 GHz)和窄带(≈40 Mhz)微波脉冲。通过线性理论和数值模拟进行的计算为观察到的光谱的特定特征和时间演化提供了令人满意的解释。提示等离子体非线性是实验观察到的微波脉冲缩短和发射光谱变宽的原因。

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