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Fig. 14.

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Summary figure of the properties extracted from the whistlers detected in the DFB cross-spectra for PSP encounter 1. Wave frequency vs. solar distance. Each dot represents a wave packet in the spectra, with their WNA color-coded, their relative amplitude constraining the size of the dot, and the absence of collocation with |B| dip resulting in an empty dot. The two gray lines indicate 20% of the electron-cyclotron frequency fce and the lower-hybrid frequency flh, from November 1, 2018, until November 11, 2018. As seen in Sect. 4.1, most of the whistlers are detected from November 1 to November 5. The second part of these gray lines (the outbound phase of the encounter) are thus relevant for very few events.

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