Breu, C.; Peter, H.; Solanki, S. K.; Cameron, R.; De Moortel, I.: Non-thermal broadening of coronal lines in a 3D MHD loop model. Monthly Notices of the Royal Astronomical Society 530, pp. 2361 - 2377 (2024)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.