Deriving the bulk properties of solar wind electrons observed by Solar Orbiter - A preliminary study of electron plasma thermodynamics

Solar Orbiter First Results (Cruise Phase)

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Fig. 4.

2D cuts of the model distribution function shown in Fig. 3, constructed in the instrument frame. Left: distribution function f at u_z = 0 km s⁻¹ as a function of u_x and u_y. Middle: f at u_y = 0 km s⁻¹ as a function of u_x and u_z. Right: f at u_x = 0 km s⁻¹ and as a function of u_y and u_z.

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