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Abstract Uranus' magnetosphere presents a unique system to examine global magnetic reconnection processes due to its location far from the Sun. We assess reconnection effectiveness during Voyager 2's Uranus flyby, using a physics‐based analytical model to calculate reconnection voltages applied to the magnetopause. This assessment of reconnection conditions at Uranus uses real‐time varying solar wind conditions as opposed to steady conditions or parameter studies. Here we show that reconnection effectiveness varied considerably over the 2 weeks before Voyager 2 passed into the magnetosphere, with voltages fluctuating between ∼0 and 76 kV; peaking and then sharply dropping off shortly before Voyager 2's entry. Variability in the voltages was found to be strongly influenced by Uranus' extreme magnetic obliquity driving diurnal modulation. Furthermore, changes in solar wind conditions, in particular density and interplanetary magnetic field strength were found to drive additional variations which disrupts the expected ∼17‐hr periodicity of the voltages.
Zomerdijk-Russell et al. (Fri,) studied this question.