{
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    "title": "A Busy Day of flares at Active Region 13615 - March 28, 2024",
    "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.Multiple M-class and an X-class flares erupt from Active Region AR 13615 on March 28, 2024.  For more details, see the Space Weather Database:  M7.0, M6.1, M9.7, X1.1.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ",
    "release_date": "2024-05-13T00:00:00-04:00",
    "update_date": "2024-05-06T14:23:28.805198-04:00",
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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>Multiple M-class and an X-class flares erupt from Active Region AR 13615 on March 28, 2024.  For more details, see the Space Weather Database:  <a href=\"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/FLR/29824/2\" target=\"_blank\">M7.0</a>, <a href=\"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/FLR/29828/2\" target=\"_blank\">M6.1</a>, <a href=\"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/FLR/29833/2\" target=\"_blank\">M9.7</a>, <a href=\"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/FLR/29836/2\" target=\"_blank\">X1.1</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 all this imagery.<br>",
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            "description": "<br><br><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.<br>",
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            "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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                        "alt_text": "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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                        "pixels": 97280
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                },
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                        "filename": "AIA131-Slates",
                        "media_type": "Frames",
                        "alt_text": "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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                },
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                        "media_type": "Frames",
                        "alt_text": "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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                        "height": 0,
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                },
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                        "filename": "AIA171-Slates",
                        "media_type": "Frames",
                        "alt_text": "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.",
                        "width": 0,
                        "height": 0,
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                    }
                }
            ],
            "extra_data": {}
        }
    ],
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        {
            "role": "Visualizer",
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                    "name": "Tom Bridgman",
                    "employer": "Global Science and Technology, Inc."
                }
            ]
        },
        {
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            "people": [
                {
                    "name": "Scott Wiessinger",
                    "employer": "KBR Wyle Services, LLC"
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            ]
        },
        {
            "role": "Technical support",
            "people": [
                {
                    "name": "Laurence Schuler",
                    "employer": "ADNET Systems, Inc."
                },
                {
                    "name": "Ian Jones",
                    "employer": "ADNET Systems, Inc."
                }
            ]
        }
    ],
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    "datasets": [
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            "name": "304 Filter",
            "common_name": "AIA 304",
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            "sensor": "AIA",
            "type": "Other",
            "organizations": [
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            "credit": "",
            "url": "http://jsoc.stanford.edu/",
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        },
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            "organizations": [
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            "credit": "",
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            "date_range": "2024-03-28T05:00:00 TAI to 2024-03-29T01:00:00 TAI"
        },
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            "organizations": [
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            "credit": "",
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        }
    ],
    "nasa_science_categories": [
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    ],
    "keywords": [
        "Corona",
        "Earth Science",
        "EUV Imaging",
        "Extreme Ultraviolet Imaging",
        "Heliophysics",
        "Point-Spread-Function (PSF)",
        "SDO",
        "Solar Active Regions",
        "Solar Activity",
        "Solar Cycle 25",
        "Solar Dynamics Observatory",
        "Solar Flares",
        "Space Weather",
        "Sun-earth Interactions"
    ],
    "recommended_pages": [],
    "related": [],
    "sources": [],
    "products": [],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}