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    "title": "A Peek from SDO: An Eruption on the Solar Limb",
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                "employer": "Global Science and Technology, Inc."
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                        "filename": "AIA304-Frames.PSF",
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            "description": "<br><h3>What is the PSF (Point Spread-Function)?</h3><br>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.<br>",
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            "description": "Time-stamp slates for these frames.",
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                {
                    "name": "Tom Bridgman",
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        },
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                {
                    "name": "Laurence Schuler",
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            "type": "Other",
            "organizations": [
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            "url": "http://jsoc.stanford.edu/",
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            "id": 14163,
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            "page_type": "Produced Video",
            "title": "Sun Produces Sparkling Flare on May 19, 2022",
            "description": "Video of the May 19th M5.6 solar flare captured by SDO in 171 angstrom light.  This view shows the full solar disk and an inset focusing on the region where the flare occured.Credit: NASA/GSFC/SDO || May_19_Flare_inset_video_STILL.jpg (1920x1080) [397.3 KB] || May_19_Flare_inset_video_STILL_searchweb.png (320x180) [87.4 KB] || May_19_Flare_inset_video_STILL_thm.png (80x40) [7.5 KB] || May_19_M5pt6_Flare_171_inset_video_1.mp4 (1920x1080) [49.7 MB] || May_19_M5pt6_Flare_171_inset_video_1.webm (1920x1080) [1.8 MB] || May_19_M5pt6_Flare_171_inset_ProRes_1920x1080.mov (1920x1080) [278.1 MB] || ",
            "release_date": "2022-05-26T00:00:00-04:00",
            "update_date": "2023-05-03T11:44:09.017741-04:00",
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                "media_type": "Image",
                "alt_text": "Video of the May 19th M5.6 solar flare captured by SDO in 171 angstrom light.  This view shows the full solar disk and an inset focusing on the region where the flare occured.Credit: NASA/GSFC/SDO",
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