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  <controlfield tag="001">6307</controlfield>
  <controlfield tag="005">20230201145008.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="a">https://doi.org/10.1051/0004-6361/202243257</subfield>
    <subfield code="2">DOI</subfield>
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  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">SCART-2023-0104</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Alipour, N.</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Automatic detection of small-scale EUV brightenings observed by the Solar Orbiter/EUI</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2022</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">Context. 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 km) from a sequence of 50 High Resolution EUV telescope (HRIEUV) 174 Å images. From 21 near co-temporal AIA images covering the same field of view as EUI, we found 1131 campfires, 58% of which were also detected in HRIEUV images. In contrast, about 16% of campfires recognized in HRIEUV were detected by AIA. We obtain a campfire birthrate of 2 × 10−16 m−2 s−1. About 40% of campfires show a duration longer than 5 s, having been observed in at least two HRIEUV images. We find that 27% of campfires were found in coronal bright points and the remaining 73% have occurred out of coronal bright points. We detected 23 EUI campfires with a duration greater than 245 s. We found that about 80% of campfires are formed at supergranular boundaries, and the features with the highest total intensities are generated at network junctions and intense H I Lyman-α emission regions observed by EUI/HRILya. The probability distribution functions for the total intensity, peak intensity, and projected area of campfires follow a power law behavior with absolute indices between 2 and 3. This self-similar behavior is a possible signature of self-organization, or even self-organized criticality, in the campfire formation process.</subfield>
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  <datafield tag="594" ind1=" " ind2=" ">
    <subfield code="a">STCE</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Safari, H.</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Verbeeck, C.</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Berghmans, D.</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">ManyOtherAuthors, X.</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Dolla, L.</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Gissot, S.</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Zhukov, A. N.</subfield>
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  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Astronomy &amp; Astrophysics</subfield>
    <subfield code="v">663</subfield>
    <subfield code="y">2022</subfield>
    <subfield code="c">A128</subfield>
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  <datafield tag="856" ind1="0" ind2=" ">
    <subfield code="f">david.berghmans@observatoire.be</subfield>
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  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">https://www.aanda.org/articles/aa/full_html/2022/07/aa43257-22/aa43257-22.html</subfield>
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  <datafield tag="905" ind1=" " ind2=" ">
    <subfield code="a">published in</subfield>
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    <subfield code="a">REFERD</subfield>
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