Abstract
A new analysis of the UV background radiation measurements obtained with the ELZ instrument on board the D2B-Aura satellite is performed at high galactic latitudes (|b| ⩾ 30°) in two bandpasses centered at 1690 Å and 2200 Å. Correlations of the UV brightnesses with dust tracers are found; the scattering phase function of dust can be derived. Among regions exhibiting a UV flux in excess over the average correlation, an insight is given on the Eridanus region known as a hot spot in soft X-rays.
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