P. Miles

TL;DR: A huge planetary-scale disturbance in the highest-speed Jovian jet at latitude 235°N was first observed in October 2016 during the Juno perijove-2 approach.

TL;DR: In this paper, the authors observed a cloud system on the south side of the planet Neptune, which was first observed in January 2015 and nearly continuously from July to December 2015 in observations with telescopes in the 2-10m class and in images from amateur astronomers.

TL;DR: In this paper, the authors presented the first extensive analysis of the morphology and motions of the Venusian clouds at lower latitudes with 900-nm images from the IR1 camera onboard Akatsuki, and showed that the middle clouds exhibit hemispherical asymmetries every 4-5 days, sharp discontinuities in elongated "hook-like" stripes, and large contrasts associated with large changes in the optical thickness.

TL;DR: In this paper, the lower clouds follow a regular cycle punctuated by a sharp discontinuity or disruption with potential implications to Venus's general circulation and thermal structure, which exhibits a westward rotation period of $\sim$4.9 days faster than winds at this level.

TL;DR: In this paper, the lower clouds follow a regular cycle punctuated by a sharp discontinuity or disruption with potential implications to Venus's general circulation and thermal structure, which exhibits a westward rotation period of $\sim$4.9 days faster than winds at this level.