Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 6.

Similar to Fig. 1 but for the arch filament system taken on 2022 March 17. The magnetogram is saturated at ±150 G. The arrows indicate the event shown in Fig. 7. The time difference of the EUI 174 Å images to obtain (b) is 15 s. An animation is available online.

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.