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    "title": "Furious February Flares",
    "description": "In early February 2026, the Sun emitted more than 50 flares including several X-class events, which is the most intense category of solar flares.  NASA’s Solar Dynamics Observatory watches the Sun 24/7 and captured these views of the Sun in multiple wavelengths of light.The Sun’s activity, which includes flares, follows an approximately 11-year cycle that creates periods of high and low activity. After reaching the current cycle’s most active phase in 2024 — known as solar maximum —  the Sun remains in a heightened period of activity.For news of the recent flares: https://science.nasa.gov/blogs/solar-cycle-25/ || ",
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            "description": "In early February 2026, the Sun emitted more than 50 flares including several X-class events, which is the most intense category of solar flares.  NASA’s Solar Dynamics Observatory watches the Sun 24/7 and captured these views of the Sun in multiple wavelengths of light.<br><br>The Sun’s activity, which includes flares, follows an approximately 11-year cycle that creates periods of high and low activity. After reaching the current cycle’s most active phase in 2024 — known as solar maximum —  the Sun remains in a heightened period of activity.<br><br>For news of the recent flares: <a href=\"https://science.nasa.gov/blogs/solar-cycle-25/\">https://science.nasa.gov/blogs/solar-cycle-25/</a>",
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            "description": "<p><b>Watch this video on the <a href=\"https://youtu.be/gp7KmJXf2EQ\" target=\"_blank\" >NASA Goddard YouTube channel</a>.</b><p><p><p>Music credit: “Gravity” by Cy Samuels [PRS] via Universal Production Music <p><p><p><a href=\"/vis/a010000/a014900/a014973/script_39098_00.html\">Complete transcript</a> available.</p>",
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            "people": [
                {
                    "name": "AJ Christensen",
                    "employer": "ADNET Systems, Inc."
                }
            ]
        }
    ],
    "missions": [
        "SDO"
    ],
    "series": [],
    "tapes": [],
    "papers": [],
    "datasets": [],
    "nasa_science_categories": [
        "Sun"
    ],
    "keywords": [
        "flare",
        "SDO",
        "Solar Dynamics Observatory"
    ],
    "recommended_pages": [],
    "related": [
        {
            "id": 14972,
            "url": "https://svs.gsfc.nasa.gov/14972/",
            "page_type": "Produced Video",
            "title": "See the Sun's Active Region: The Source of the Early-February Flares",
            "description": "This video condenses nine days of solar activity into 12 minutes, playing 1,080 times faster than real time. NASA's Goddard Space Flight Center/SDO. Music Credit: “Atomic Drift,” “Echoes of the Unknown,” and “Particle Reverie” from the album Molecular Echoes. Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Active_Region-STILL.jpg (1920x1080) [239.1 KB] || Active_Region-STILL_searchweb.png (320x180) [72.9 KB] || Active_Region-STILL_thm.png (80x40) [5.9 KB] || 14972ActiveRegionLongCaptions.en_US.srt [162 bytes] || 14972ActiveRegionLongCaptions.en_US.vtt [164 bytes] || 14972_Active_Region_Long_Good.mp4 (1920x1080) [1.3 GB] || 14972_Active_Region_Long_Better.mp4 (1920x1080) [2.1 GB] || 14972_Active_Region_Long_YouTube.mp4 (1920x1080) [4.2 GB] || 14972_Active_Region_Long_ProRes_1920x1080_2997.mov (1920x1080) [11.5 GB] || ",
            "release_date": "2026-02-27T12:00:00-05:00",
            "update_date": "2026-02-27T07:42:21-05:00",
            "main_image": {
                "id": 1202156,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014900/a014972/Active_Region-STILL.jpg",
                "filename": "Active_Region-STILL.jpg",
                "media_type": "Image",
                "alt_text": "This video condenses nine days of solar activity into 12 minutes, playing 1,080 times faster than real time. NASA's Goddard Space Flight Center/SDO. Music Credit: “Atomic Drift,” “Echoes of the Unknown,” and “Particle Reverie” from the album Molecular Echoes. Written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        },
        {
            "id": 14964,
            "url": "https://svs.gsfc.nasa.gov/14964/",
            "page_type": "Produced Video",
            "title": "Early February Flares 2026",
            "description": "So far, the Sun has emitted six X-class solar flares in the first four days of February. X-class flares are the most powerful.  In this composite image, we've layered all six X-class flares onto the Sun at once, to show the active areas. The images come from the Solar Dynamics Observatory (SDO), which observes the Sun in different wavelengths, using filters that emphasize different characteristics. Flare #6, for example, shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares, which is colored in red and blue. The Sun’s magnetic field goes through a cycle, called the solar cycle, about every 11 years, with periods of more and less activity. The Sun reached its most active phase – solar maximum – in 2024, which means we’re still in a fairly active period of the cycle.For news of the recent flares: https://science.nasa.gov/blogs/solar-cycle-25/Image DescriptionComposite image of 6 X-class solar flares emitted in February. In the center, the Sun is a dark red globe with mottled darker and glowing orange spots. Just above the equator and to the left of center longitudinally, 2 bright white glowing spots are made of the combined 6 X-class flares emitted so far. Six squares pop out from the center Sun, with lines connecting to the spot on the composite Sun their flare is contributing. Along the top, the squares are labeled 2, 4 and 6. Each has a subset of the Sun seen in a different colored wavelength. Box 2 is a purple Sun with a pinkish flare, from Feb. 2, 2026. Box 4 is a golden Sun with a white flare from Feb. 2, 2026. Box 6 is a pink Sun with an orange flare from Feb. 4, 2026. Along the bottom, the boxes are labeled 1, 3 and 5. Box 1 has a turquoise Sun with a teal flare from Feb. 1, 2026. Box 3 has a yellow Sun with an orange flare from Feb. 2, 2026. Box 5 has a red Sun the same color as the center, with a white flare, from Feb. 3, 2026. || February_2026_X_Flares_SIX_FINAL.jpg (7000x7000) [5.3 MB] || ",
            "release_date": "2026-02-05T13:00:00-05:00",
            "update_date": "2026-02-09T16:36:55-05:00",
            "main_image": {
                "id": 1201856,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014900/a014964/SDO_02-03-26_131.00001_print.jpg",
                "filename": "SDO_02-03-26_131.00001_print.jpg",
                "media_type": "Image",
                "alt_text": "NASA’s Solar Dynamics Observatory captured this video of an X1.5 solar flare – as seen in the bright eruption on the upper left — at 14:15 UTC on Februrary 3, 2026. The image shows 131 Angstrom light, a subset of extreme ultraviolet light. Credit: NASA/SDO",
                "width": 1024,
                "height": 868,
                "pixels": 888832
            }
        }
    ],
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