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Дата последнего поиска статьи во внешних источниках: 3 июня 2020 г.
Аннотация:The study of the Galilean satellites can help clarify the structure of the magnetospheric magneticfield from observations of their projections along magnetic field lines in the atmosphere/ionosphere ofJupiter, where patches of auroras appear. UV auroras in projections on the ionosphere of Io, Europe andGanymede occur almost permanently, while the observation of the track of Callisto is difficult. One of the reasons is that the Callisto projection lies near or inside Jupiter’s bright main oval. Another reason is that Callisto is not constantly in the sub-Alfvénic flow of magnetospheric plasma. The interaction of Callisto with the magnetospheric plasma of the planet is an actual problem widely discussed in the literature, which sheds light on the key processes occurring in the Jovian system.