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Fig. 4

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Surface reflectance maps of Ganymede in the following six spectral intervals: [150 nm, 160 nm], [160 nm, 170 nm], [170 nm, 175 nm], [175 nm, 185 nm],[185 nm, 195 nm], and [195 nm, 205 nm]. The reflectance was obtained by fitting the reflected solar continuum, using spectra extracted from the Juno/UVS spectral cube, spatially convolved with a latitude-longitude window of 10° × 10°. These maps complete the reflectance map in the [140 nm, 150 nm] interval shown in Fig. 3, and allow us to analyze the UV reflectance on the Ganymede surface spectrally and spatially.

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