Simultaneous multi-scale and multi-instrument observations of Saturn's aurorae during the 2013 observing campaign

On 21 April 2013, during a co-ordinated Saturn auroral observing campaign, the northern and southern poles of the planet were observed from the Earth using the NASA Infrared Telescope Facility (IRTF), Keck, and Hubble Space Telescope (HST) simultaneously with the Cassini infrared, visible, and ultraviolet remote sensing instruments. We present simultaneous multi-scale and multi-wavelength analysis of the morphology of auroral emissions at Saturn. The visible main auroral emission vary between similar to 2 and 10 kR on timescales of minutes and across spatial scales of down to similar to 14 km on the planet. The H-2 Far Ultraviolet (FUV) brightness varies by a factor of similar to 10, from similar to 4-40 kR, over timescales of 1 min and spatial scales of 720 km. H-3(+) infrared emissions vary less than the H-2 emissions, from similar to 5-10 mu W m(-2) sr(-1), over similar spatial scales (similar to 300 km) and timescales of a few seconds to a few hours. The fine-scale temporal and spatial features seen in the main oval show that complex structures are present even during quiet solar wind conditions. Diffuse ultraviolet emissions southward of the southern midnight main oval that are not seen in the infrared, implying a steep temperature gradient of similar to 50 K over 2-4 degrees latitude equatorward of the main oval. Dynamics on scales of similar to 100 km at the poles are revealed by lower spatial resolution observations, the morphologies of which are partly consistent with overlapping local-time fixed and co-rotating current systems. We also present the first direct comparison of simultaneous infrared, visible, and ultraviolet auroral emissions at Saturn. Finally, the main auroral emissions are found to be approximately co-located in the midnight sector, forming an arc with a width of similar to 0.5-1 degrees, at 72-74 degrees southern latitude, moving slightly equatorward with increasing local-time. (C) 2015 Elsevier Inc. All rights reserved.