{
    "id": 5055,
    "url": "https://svs.gsfc.nasa.gov/5055/",
    "page_type": "Visualization",
    "title": "A Cluster of M-class solar flares from Active Region 13165",
    "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Here, Active Region 13165 (lower right of solar disk) fires of a cluster of M-class flares over a couple of days in mid-December 2022 (Solar Flares: What does it take to be X-class?).   The point-spread function correction (PSF) has been applied to all the imagery on this page.  An M6.3 flare erupts followed shortly by a smaller M3.2 flare. || ",
    "release_date": "2023-01-10T12:00:00-05:00",
    "update_date": "2023-05-03T11:43:46.936774-04:00",
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        "filename": "20221214_AR13165M06_AIA131_PSF_stamped.000222_print.jpg",
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        "alt_text": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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        "alt_text": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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    "main_credits": {
        "Visualizations by": [
            {
                "name": "Tom Bridgman",
                "employer": "Global Science and Technology, Inc."
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        ],
        "Produced by": [
            {
                "name": "Scott Wiessinger",
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    "progress": "Complete",
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            "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.<br><br>Here, Active Region 13165 (lower right of solar disk) fires of a cluster of M-class flares over a couple of days in mid-December 2022 (<a href=\"https://www.nasa.gov/mission_pages/sunearth/news/X-class-flares.html\" target=\"_blank\">Solar Flares: What does it take to be X-class?</a>).   The point-spread function correction (PSF) has been applied to all the imagery on this page.  An M6.3 flare erupts followed shortly by a smaller M3.2 flare. ",
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            "description": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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                        "alt_text": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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                        "alt_text": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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                        "alt_text": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005000/a005055/frames/4096x4096_1x1_30p/20221214_AR13165M06_AIA131-Frames.PSF_stamped/",
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                        "alt_text": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 131 angstrom filter.  The dark region around the central 'X' marking the flare is an artifact of the PSF correction.  'Flickering' in the images around the flare are created due to the 'flare mode' images which have a shorter exposure.  Normalizing the solar disk to the same brightness in these frames enhances the background noise off the solar disk.",
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            "description": " <br>The next day, December 15, 2022, an M5.7 flare erupts from the same active region. ",
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            "description": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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                        "alt_text": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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                        "alt_text": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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                        "alt_text": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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                        "alt_text": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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                        "alt_text": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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                        "alt_text": "An additional larger flare event (M5.7) of December 15, 2022, as seen in the SDO AIA 131 angstrom filter.",
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            "description": "  <br>In these examples of smaller flares, the flare is much more visible in the AIA 131 angstrom filter.  However, in the 171 angstrom  filter, the complex loop structure in the magnetic fields is more obvious ",
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            "description": "The double flare event (M6.3 & M 3.2) of December 14, 2022 as seen in the SDO AIA 171 angstrom filter. ",
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