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    "title": "M7.4 flare from Active Region 13964 - January 17, 2025",
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    "release_date": "2025-02-20T14:00:00-05:00",
    "update_date": "2025-02-20T13:20:51.119327-05:00",
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    "main_credits": {
        "Visualizations by": [
            {
                "name": "Tom Bridgman",
                "employer": "Global Science and Technology, Inc."
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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>Active Region 13964 (in the upper right quadrant of the disk) launches an M7.4 flare followed by some complex post-flare evolution.  For more details, see the <a href=\"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/FLR/36446/2\" target=\"_blank\">Space Weather Database entry.</a><br><br>For more information on the classification of solar flares, see <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> or <a href=\"https://svs.gsfc.nasa.gov/10109\" target=\"_blank\">X-Class: A Guide to Solar Flares</a>. The point-spread function correction (PSF) has been applied to some of this imagery.",
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            "description": "<br><h2>What is the PSF (Point Spread-Function)?</h2>Many telescopes, especially reflecting telescopes such as the ones used on SDO (<a href=\"https://en.wikipedia.org/wiki/Reflecting_telescope\" target=\"_blank\">Wikipedia</a>), have internal structures that support various optical components. These components can result in incoming light being scattered to other parts of the image. This can appear in the image as a faint haze, brightening dark areas and dimming bright areas. The point-spread function (<a href=\"https://en.wikipedia.org/wiki/Point_spread_function\" target=\"_blank\">Wikipedia</a>) is a measure of how light that would normally be received by a single camera pixel, gets scattered onto other pixels. This is often seen as the \"spikes\" seen in images of bright stars. For SDO, it manifests as a double-X shape centered over a bright flare (see <a href=\"https://svs.gsfc.nasa.gov/11383\" target=\"_blank\">Sun Emits Third Solar Flare in Two Days</a>). The effect of this scattered light can be computed, and removed, by a process called deconvolution (<a href=\"https://en.wikipedia.org/wiki/Deconvolution\" target=\"_blank\">Wikipedia</a>). This is often a very compute-intensive process which can be sped up by using a computers graphics-processing unit (GPU) for the computation.",
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            "caption": "",
            "description": "Time slates for the multiple movies above, for custom compositing. Make sure to match the event and frame tag for the SDO frames you are using.",
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                        "filename": "AIA.0171A-Slates",
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            "role": "Visualizer",
            "people": [
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                    "name": "Tom Bridgman",
                    "employer": "Global Science and Technology, Inc."
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            ]
        },
        {
            "role": "Producer",
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                {
                    "name": "Scott Wiessinger",
                    "employer": "eMITS"
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        },
        {
            "role": "Technical support",
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                {
                    "name": "Laurence Schuler",
                    "employer": "ADNET Systems, Inc."
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            "organizations": [
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        "Coronal Mass Ejections",
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        "EUV Imaging",
        "Extreme Ultraviolet Imaging",
        "Heliophysics",
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        "Solar Active Regions",
        "Solar Activity",
        "Solar Cycle 25",
        "Solar Dynamics Observatory",
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        "Space Weather",
        "Sun-earth Interactions"
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    "recommended_pages": [],
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