Snapshot captured in the survey mode by the Solar Orbiter instrument RPW, on 2022 September 22, at 13:52:28 UT. (a) Waveform of the two electric field components E_z (blue) and E_y (red), in the SRF frame. (b) Hodograms E_y(E_z) calculated within equidistant time windows of 0.7 ms. (c)–(d) Wavelet spectrograms of the electric energy ∣E(f, t)∣² = ∣E_y(f, t)∣² + ∣E_z(f, t)∣² in the high- and low-frequency ranges, i.e., 45 ≤ f ≤ 48 kHz and f ≤ 1 kHz, respectively. (e) Wavelet spectrogram of the magnetic energy ∣B(f, t)∣², in the same frequency range as (c). (c)–(e) The color bars are in logarithmic scales. (f)–(i) Power spectra of the field components E_z (blue), E_y (red), and cB (green), respectively. Zoomed-in views are presented, in logarithmic and linear scales, in the ranges of 44 ≤ f ≤ 48 kHz ((g), (h)) and f ≤ 1 kHz (i). The black curve in (i) represents the spectrum of ∣E∣². The dashed vertical lines correspond to peaks at f₃ ≃ 45.74 kHz and f₁ ≃ 46.04 kHz (g)–(h), and at ﹩{f}_{1}^{{\prime} }\simeq 0.3﹩ kHz (i). Spectra in (f)–(i) are calculated in the time interval of 2 ≤ t ≤ 22 ms.