The Jupiter Icy moons Explorer (JUICE), scheduled to launch in 2022, has among its instruments a radiometer called the Submillimeter Wave Instrument (SWI). This instrument is being built at the Max Plank Institute für Sonnensystemforschung in Göttingen, Germany. Here, they are building and testing several ground-based radiometers to serve as calibration standards for the SWI. During the summer, I helped to implement real-time forward modelling into the python firmware for these radiometers. I used the Atmospheric Radiative Transfer Simulator (ARTS) to run the retrievals, along with the Typhon software package, and was able to implement real-time forward modelling for four different spectrometers in the calibration lab.
Getting Under Europa’s Skin
Tracing Formation and Evolution of Outer Solar System Bodies Through Stable Isotopes and Noble Gas Abundances
Photosynthesis, a Planetary Revolution
Xenon: King of the Gases