Fig. 6
Download original image
Results from radiative transfer modelling for Voyager 2 base atmosphere and 1998 observing conditions. Left column: modelled original (above) and attenuated by FG IPH and EEH (below) Lyα line-integrated intensities from Uranus’ atmosphere. Right column: line-resolved intensities for the radial pixels from the respective images in the left column. The Lyα lines are represented in Earth’s frame. All Doppler shifts are properly accounted for calculating the attenuation.
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.