Multiscale views of an Alfvénic slow solar wind: 3D velocity distribution functions observed by the Proton-Alpha Sensor of Solar Orbiter

Solar Orbiter First Results (Cruise Phase)

Open Access

Fig. 1.

PAS and MAG observations from 14/07 10:00 to 15/07 6:00. From top to bottom: (a) Time/energy spectrogram of ion flux, from 500 eV to 1.7 keV (unit: part. s⁻¹ cm⁻² sr⁻¹ keV⁻¹); (b and c): proton density and temperature; (d–f): magnetic and velocity field components in RTN frame. In (d), |B| (in black) is also presented.

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