Integrated UV emissions in the [155 nm, 162 nm] range rescaled by a factor of 8.1 to obtain a map of the total unabsorbed emissions from Jupiter’s auroral regions observed during PJ11 in the SIII Jovicentric reference frame. The red arrowed lines represent the solar longitude progression during the observation. The iso-brightening contours have the following values: [1, 10, 100, 500, 1000, 2000] in kR.