International audienceContext. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are essential to the investigation of the physical processes heating the corona. Aims. We detected small-scale brightenings, termed campfires, using their morphological and intensity structures as observed in coronal EUV imaging observations for statistical analysis. Methods. We applied a method based on Zernike moments and a support vector machine (SVM) classifier to automatically identify and track campfires observed by Solar Orbiter/Extreme Ultraviolet Imager (EUI) and Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA). Results. This method detected 8678 campfires (with length scales between 400 km and 4000 k...
Context. Localised transient EUV brightenings, sometimes named ‘campfires’, occur throughout the qui...
The quiet solar corona consists of myriads of loop-like features, with magnetic fields originating f...
Brightenings observed in solar extreme-ultraviolet images are generally interpreted as signatures of...
Context. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are esse...
Context. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are esse...
International audienceContext. The heating of the solar corona by small heating events requires an i...
Context. The three-dimensional fine structure of the solar atmosphere is still not fully understood ...
12 pages, 14 figuresThe goal of this paper is to study the smallest brightening events observed in t...
The High Resolution Imager (HRIEUV) telescope of the Extreme Ultraviolet Imager (EUI) instrument onb...
Context. The smallest extreme-ultraviolet (EUV) brightening events that were detected so far, called...
The High Resolution Imager (HRIEUV) telescope of the Extreme Ultraviolet Imager (EUI) instrument onb...
Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter have cha...
Context. Localised transient EUV brightenings, sometimes named ‘campfires’, occur throughout the qui...
The quiet solar corona consists of myriads of loop-like features, with magnetic fields originating f...
Brightenings observed in solar extreme-ultraviolet images are generally interpreted as signatures of...
Context. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are esse...
Context. Accurate detections of frequent small-scale extreme ultraviolet (EUV) brightenings are esse...
International audienceContext. The heating of the solar corona by small heating events requires an i...
Context. The three-dimensional fine structure of the solar atmosphere is still not fully understood ...
12 pages, 14 figuresThe goal of this paper is to study the smallest brightening events observed in t...
The High Resolution Imager (HRIEUV) telescope of the Extreme Ultraviolet Imager (EUI) instrument onb...
Context. The smallest extreme-ultraviolet (EUV) brightening events that were detected so far, called...
The High Resolution Imager (HRIEUV) telescope of the Extreme Ultraviolet Imager (EUI) instrument onb...
Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter have cha...
Context. Localised transient EUV brightenings, sometimes named ‘campfires’, occur throughout the qui...
The quiet solar corona consists of myriads of loop-like features, with magnetic fields originating f...
Brightenings observed in solar extreme-ultraviolet images are generally interpreted as signatures of...