Juno-UVS UV brightness profiles and derived quantities

FITS files containing time series of the ultraviolet brightness profiles for different wavelength ranges along Juno's magnetic footprint. Derived mean electron energies precipitating electron energy fluxes and Hall/Pedersen conductances are also provided, assuming a kappa energy distribution (kappa=2.5). The dataset covers the 69 first perijove sequences (no data was collected during PJ2). The time series are built upon calibrated data from the UVS instrument (Gladstone et al. 2017 doi:10.1007/s11214-014-0040-z). The magnetic field used for the magnetic mapping to 400 km above the 1-bar surface is JRM33+Con2020 (Connerney et al. 2020, 2022). For each quantity, there are 5 profiles, the first one is the profile at the magnetic footprint as prescribed by the model and the 4 others originate from profiles shifted 1000 km North, South, East and West of the magnetic field model prediction. Uncertainties and upper/lower values are provided. When missing (not-a-number values), the evaluated quantity should not be considered as reliable. The h2ly (155-162nm) brightness profile correction, as well as the colour ratio to energy conversion are from Vinesse et al. 2026 (DOI: 10.1051/0004-6361/202556908). The conductance profiles use conversions from Sicorello et al. 2025 (DOI: 10.1051/0004-6361/202556176 ).