Re-analysis of Uranus Data from Voyager 2 Plasma Science Experiment

Both Voyager 1 and 2 are equipped with Plasma Science (PLS) instruments: four Faraday cups that measure the properties (density, temperature and flow) of low energy ions and electrons. During the Voyagers journey towards the interstellar space and the flybys from the gas giants PLS gave us the first in-situ data of the solar wind in such great distances, the magnetospheric plasma properties at the gas giants, and the extent of our heliosphere along with the conditions of the interstellar medium. Voyager was particularly important for the study of the gas giants, as it was the first time we had in-situ plasma measurements from inside the magnetospheres, and PLS helped in studying not only the morphology of the magnetosphere, but also the plasma sources, dynamics, interaction with the moons, and ultimately its interaction with the solar wind plasma. Jupiter and Saturn were visited from both Voyager 1 and 2, but only Voyager 2 visited Uranus and Neptune. The PLS data for Jupiter have been re-calibrated and archived by Bagenal+ [2017], Dougherty+ [2017], and Bodisch+ [2017]. They also developed an IDL package, VIPER (Voyager Ion PLS Experiment Response) for their analysis. For this work we re-analyzing the Voyager PLS data for Uranus and in this poster we present our methodology, the adaptation of VIPER for the Uranian conditions and the results of the re-analysis.