Auroral 3D structure retrieval from the Juno/UVS data

Open Access

Fig. 6

Maps of the inverse average energy for the kappa distribution case. These maps were obtained for the north (left panel) and south (right panel) auroral regions using the CR(E, θ) relationship and the CR observed during PJ11 (see Fig. 4). The iso-energy lines have the same values as in Fig. 5.

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