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            "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on theupper left – on Feb. 21, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona and the extremely hot material in flares, respectively. Cropped to highlight the flaring region. Credit: NASA/SDO",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the upper right – on Feb. 21, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona, tinted yellow, and the extremely hot material in flares, tinted blue, respectively. Credit: NASA/SDO",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the upper right – on Feb. 21, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona, tinted yellow, and the extremely hot material in flares, tinted blue, respectively. A scale image of Earth is added to show the size of the flaring region. Credit: NASA/SDO",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the upper left – on Feb. 21, 2024. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares, and which is colorized in teal. Credit: NASA/SDO",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of the Sun on Feb. 21, 2024. The image shows a subset of extreme ultraviolet light that highlights the loops of hot plasma in the solar corona, and which is colorized in yellow. Credit: NASA/SDO",
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            "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the upper right – on Feb. 21, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona, tinted yellow, and the extremely hot material in flares, tinted blue, respectively. Credit: NASA/SDO",
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                        "alt_text": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the upper right – on Feb. 21, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona, tinted yellow, and the extremely hot material in flares, tinted blue, respectively. Credit: NASA/SDO",
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            "description": "See [https://blogs.nasa.gov/solarcycle25/2024/02/22/sun-releases-two-strong-flares/](https://blogs.nasa.gov/solarcycle25/2024/02/22/sun-releases-two-strong-flares/)",
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        {
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            "page_type": "Produced Video",
            "title": "NASA's SDO Captures a February Solar Flare Triple Play",
            "description": "The Solar Dynamics Observatory (SDO) spotted three X-class flares on the Sun between February 21 and 22, 2024.  Watch this video to see what those events looked like in several wavelengths of extreme ultraviolet light that SDO captures. The video opens with quick shots of the three flares in different wavelength blends.  The first is a blend of 131 and 171-angstrom-light imagery, the second is 171 and 304, and the last is 171 and 1600.  Each wavelength highlights different temperature plasma and reveals different layers and features of the Sun. 131 angstrom light shows both the extremely hot plasma of flares (6-10 million Kelvin) and cooler plasma (400,000 Kelvin).  Credit: NASA's Goddard Space Flight Center/SDOMusic: \"Serene Reverie\" from the album Reflections.  Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || February_Triple_Play_Still_print.jpg (1024x576) [166.0 KB] || February_Triple_Play_Still.jpg (3840x2160) [2.1 MB] || February_Triple_Play_Still_searchweb.png (320x180) [100.7 KB] || February_Triple_Play_Still_thm.png (80x40) [8.0 KB] || 14536_FebruaryXFlareTriplePlay_1080.webm (1920x1080) [26.0 MB] || Flare_Triple_Play_Captions.en_US.srt [811 bytes] || Flare_Triple_Play_Captions.en_US.vtt [772 bytes] || 14536_FebruaryXFlareTriplePlay_1080.mp4 (1920x1080) [405.7 MB] || 14536_FebruaryXFlareTriplePlay_1080_small.mp4 (1920x1080) [166.7 MB] || 14536_FebruaryXFlareTriplePlay_ProRes_3840x2160.mov (3840x2160) [14.2 GB] || 14536_FebruaryXFlareTriplePlay_4k_25mbps.mp4 (3840x2160) [670.9 MB] || 14536_FebruaryXFlareTriplePlay_4k_50mbps.mp4 (3840x2160) [1.3 GB] || ",
            "release_date": "2024-02-26T14:45:00-05:00",
            "update_date": "2024-02-26T10:29:40.486688-05:00",
            "main_image": {
                "id": 1089561,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014536/February_Triple_Play_Still_print.jpg",
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                "media_type": "Image",
                "alt_text": "The Solar Dynamics Observatory (SDO) spotted three X-class flares on the Sun between February 21 and 22, 2024.  Watch this video to see what those events looked like in several wavelengths of extreme ultraviolet light that SDO captures. The video opens with quick shots of the three flares in different wavelength blends.  The first is a blend of 131 and 171-angstrom-light imagery, the second is 171 and 304, and the last is 171 and 1600.  Each wavelength highlights different temperature plasma and reveals different layers and features of the Sun. 131 angstrom light shows both the extremely hot plasma of flares (6-10 million Kelvin) and cooler plasma (400,000 Kelvin).  Credit: NASA's Goddard Space Flight Center/SDOMusic: \"Serene Reverie\" from the album Reflections.  Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.",
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