Fig. 2.
Examples of the geometry involved in the modelling of the Io-controlled emissions of Jupiter. The emission depends on the relative position of Io, Jupiter, and the observer, in particular on the jovigraphic longitude of the observer (λCML, i.e. the central meridian longitude) and that of the active field line which can differ from that of Io (λIo) by a lead angle (δλ).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.