How rare are counter Evershed flows?
J. Sebasti\'an Castellanos Dur\'an, Andreas Lagg, Sami K., Solanki

TL;DR
This study investigates the frequency, lifetime, and conditions of counter Evershed flows in sunspot penumbrae, revealing they are more common than previously thought but often underreported due to observational limitations.
Contribution
It provides the first comprehensive statistical analysis of counter Evershed flows using continuous space-based observations, highlighting their prevalence and characteristics.
Findings
CEFs occur in 83.5% of active regions.
Median lifetime of CEFs is approximately 10.6 hours.
Two populations of CEFs are identified based on association with light bridges.
Abstract
One of the main characteristics of the penumbra of sunspots is the radially outward-directed Evershed flow. Only recently have penumbral regions been reported with similar characteristics to normal penumbral filaments, but with an opposite direction of the flow. Such flows directed towards the umbra are known as counter Evershed flows (CEFs). We aim to determine the frequency of occurrence of CEFs in active regions (ARs) and to characterize their lifetime and the prevailing conditions in the ARs. We analysed the continuum images, Dopplergrams, and magnetograms recorded by SDO/HMI of 97 ARs that appeared from 2011 to 2017. We followed the ARs for days on average. We found 384 CEFs in total, with a median value of 6 CEFs per AR. CEFs are a rather common feature, they occur in 83.5% of all ARs regardless of the magnetic complexity of the AR. However, CEFs were observed on…
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