Multi-wavelength Observations of Jupiters Northern Circumpolar Cyclones

Juno arrived at Jupiter in 2016 and was inserted into a polar orbit with its closest approach (perijove) near Jupiters equator. One of Junos first major discoveries was the existence of circumpolar cyclones covering both of Jupiters poles. Over the course of Junos prime and extended missions, the line of apsides of the orbit has experienced a constant northward migration due to Jupiters asymmetric gravity field. One result of this migration is the lowering the spacecrafts altitude over Jupiters north pole. Recently, the altitude over the north pole has reduced sufficiently to allow Junos microwave radiometer (MWR) to resolve Jupiters circumpolar cyclones. The observations provide new insights into how the circumpolar cyclones evolve with depth. We will present results from multi-wavelength observations of Jupiters polar cyclones including visible light images (JunoCam), the infrared images (JIRAM) and microwave images (MWR). The combined data set reveals information on how the circumpolar cyclones compare and evolve with depth.