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  <controlfield tag="001">8144</controlfield>
  <controlfield tag="005">20260722102846.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="a">10.3847/2041-8213/ae7d2e</subfield>
    <subfield code="2">DOI</subfield>
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  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">SCART-2026-0146</subfield>
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  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Guastavino, Sabrina</subfield>
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  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Validation of an Extreme-ultraviolet Desaturation Technique for the Atmospheric Imaging Assembly on Board the Solar Dynamics Observatory Using Observations from the Extreme Ultraviolet Imager on Board Solar Orbiter</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2026</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">High-dynamic-range imaging in the extreme-ultraviolet regime is frequently compromised by detector saturation and charge blooming during intense solar flares, preventing reliable photometry of flare cores. This study presents, for the first time, a direct validation of a sparsity-regularized inverse-diffraction desaturation algorithm applied to saturated images from the Atmospheric Imaging Assembly on the Solar Dynamics Observatory, using contemporaneous short-exposure, unsaturated observations from the Extreme Ultraviolet Imager on Solar Orbiter. The validation exploits a near-radial spacecraft alignment on 2024 March 19, when an M2.1 flare erupted in active region 13615. To obtain coregistered intensity maps, the data were processed with reprojection onto a common helioprojective grid, exposure-time normalization, light-travel-time correction, and field-of-view pointing refinement. Photometric comparisons were performed using peak-based statistics within a rigorously defined region of interest. Results show close morphological agreement and a temporally stable ratio between the desaturated and reference intensities through the impulsive and early decay phases. An early-phase discrepancy is observed and attributed to rapid subexposure evolution, sampling effects, and bandpass/response differences. These findings demonstrate that the desaturation procedure successfully recovers physically meaningful time-dependent core fluxes and, for the first time, provide independent empirical support for the use of desaturated archive frames in quantitative studies of large flares.</subfield>
  </datafield>
  <datafield tag="594" ind1=" " ind2=" ">
    <subfield code="a">STCE</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">Solar Orbiter</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">EUI</subfield>
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  <datafield tag="653" ind1="1" ind2=" ">
    <subfield code="a">flares</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Berghmans, David </subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Verbeeck, Cis</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Hofmeister, Stefan</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Kraaikamp, Emil</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Dickson, Ewan C. M. </subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Benvenuto, Federico</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Massa, Paolo</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Massone, Anna Maria</subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Piana, Michele</subfield>
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  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">The Astrophysical Journal Letters</subfield>
    <subfield code="v">1005</subfield>
    <subfield code="y">2026</subfield>
    <subfield code="n">2</subfield>
    <subfield code="c">id.L50</subfield>
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  <datafield tag="856" ind1="0" ind2=" ">
    <subfield code="f">david.berghmans@ksb-orb.be</subfield>
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  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">https://ui.adsabs.harvard.edu/abs/2026ApJ..1005L..50G/abstract</subfield>
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  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">https://iopscience.iop.org/article/10.3847/2041-8213/ae7d2e</subfield>
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    <subfield code="a">published in</subfield>
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    <subfield code="a">REFERD</subfield>
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