Andrew P. Ingersoll

TL;DR: In this paper, the authors presented well-calibrated, high-resolution maps of Saturn's thermal emission at 2.2-cm wavelength obtained by the Cassini RADAR radiometer through the Prime and Equinox Cassini missions, a period covering approximately 6 years.

TL;DR: Junocam will look for convective clouds and lightning in thunderstorms and derive the heights of the clouds and support Juno’s radiometer experiment by identifying any unusual atmospheric conditions such as hotspots.

TL;DR: In this paper, the effective temperature of Saturn from 30°S to 10°N is 96.5 ± 2.5 K. This value is 1.9 K higher than our preliminary estimate (Ingersoll et al., 1980).

TL;DR: The VLBI tracking experiment provided measurements of balloon positions and horizontal winds along their trajectories as mentioned in this paper, and the VEGA Balloons obtained in-situ measurements of pressure, temperature, vertical winds, cloud density, ambient illumination, and the frequency of lightning during their 48 hour flights in the Venus middle cloud layer.

TL;DR: In this paper, the authors detect visible lightning on the night side of Saturn in a broadband clear filter and the 2011 lightning is detected on the day side in blue wavelengths only, which leaves the lightning spectrum unknown.