Observations with Solar Orbiter/EUI reveal fast (500 to 2200 km/s), weakly damped, quasi-periodic 2-minute intensity disturbances in the upper parts of non-flaring active-region coronal loops.
The red line indicates the location of the sub-slit where F14 is detected
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Fast and periodic propagating disturbances along coronal loops detected with EUI on board Solar Orbiter
Observations with Solar Orbiter/EUI reveal fast (500 to 2200 km/s), weakly damped, quasi-periodic 2-minute intensity disturbances in the upper parts of non-flaring active-region coronal loops.