Skewness and kurtosis of solar wind proton distribution functions: The normal inverse-Gaussian model and its implications

Open Access

Fig. 2.

PAS and MAG observations (19/03/2022). From top to bottom: (a) Time/energy ion spectrogram (500 eV–4 keV, unit: s⁻¹ cm⁻² sr⁻¹ keV⁻¹). (b) and (c): Proton density and temperature. (d): Pressure – parallel in red, perpendicular in blue and green. (e)–(g): Magnetic and velocity field components in RTN frame. The vertical lines show the selected times.

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