Observations of whistler mode waves by Solar Orbiter’s RPW Low Frequency Receiver (LFR): In-flight performance and first results

Solar Orbiter First Results (Cruise Phase)

Open Access

Fig. 2.

Components and amplitude of the DC magnetic field (B₀) measured by the MAG instrument (Horbury et al. 2020), and the electron plasma density (n₀) as estimated by the RPW instrument suite from the spacecraft potential measurement (Khotyaintsev et al. 2021) for the same time interval as in Fig. 1.

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