Random density fluctuations convert beam-driven Langmuir/Z waves into Z-mode radiation at constant frequency, producing polarization ratios up to F~1 and setting a threshold Delta_N ~ 3(v_T/v_b)^2 for diagnosing solar wind density turbulence.
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Polarization ratios of turbulent Langmuir/$\mathcal{Z}$-mode waves generated by electron beams in magnetized solar wind plasmas
Random density fluctuations convert beam-driven Langmuir/Z waves into Z-mode radiation at constant frequency, producing polarization ratios up to F~1 and setting a threshold Delta_N ~ 3(v_T/v_b)^2 for diagnosing solar wind density turbulence.