Fig. 6.

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Example of the dispersion relation of Langmuir waves driven by the bump-on-tail instability using Eq. (2). (a) The distribution function used to calculate the dispersion relation (black line). The vertical dashed black line shows the vph of the wave correspond to maximum growth. (b) Dispersion relation of Langmuir waves (black line) and associated growth rate (red line) shifted up in frequency by ωpe. The upper and lower dashed lines show the Doppler-shifted dispersion dispersion relation for k aligned and anti-aligned with s solar wind flow of 350 km s−1. The blue shaded region shows the expected range of k and frequencies for Langmuir waves.
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