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Credit: NASA/SDO", "items": [ { "id": 427180, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1092027, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014588/SDO_131_May-9-2024_0918UTC_X2_labeled.jpg", "filename": "SDO_131_May-9-2024_0918UTC_X2_labeled.jpg", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured this image of an X2.2 solar flare – as seen in the bright flash in the lower center – on May 9, 2024. The image shows 131 Angstrom light, a subset of extreme ultraviolet light, colorized red. Credit: NASA/SDO", "width": 4096, "height": 4096, "pixels": 16777216 } }, { "id": 427182, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1092039, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014588/SDO_131_May-9-2024_0918UTC_X2.png", "filename": "SDO_131_May-9-2024_0918UTC_X2.png", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured this image of an X2.2 solar flare – as seen in the bright flash in the lower center – on May 9, 2024. The image shows 131 Angstrom light, a subset of extreme ultraviolet light, colorized red. Credit: NASA/SDO", "width": 4096, "height": 4096, "pixels": 16777216 } } ], "extra_data": {} }, { "id": 374184, "url": "https://svs.gsfc.nasa.gov/14588/#media_group_374184", "widget": "Single image", "title": "", "caption": "", "description": "NASA’s Solar Dynamics Observatory captured this image of an X3.9 flare on May 10, 2024. The image shows a blend of 171 and 131 Angstrom light, subsets of extreme ultraviolet light.
Credit: NASA/SDO", "items": [ { "id": 427185, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1092091, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014588/SDO_X3pt9_Flare_May_10_2024_131-171.jpg", "filename": "SDO_X3pt9_Flare_May_10_2024_131-171.jpg", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured this image of an X3.9 flare on May 10, 2024. The image shows a blend of 171 and 131 Angstrom light, subsets of extreme ultraviolet light. Credit: NASA/SDO", "width": 4096, "height": 4096, "pixels": 16777216 } } ], "extra_data": {} }, { "id": 374185, "url": "https://svs.gsfc.nasa.gov/14588/#media_group_374185", "widget": "Single image", "title": "", "caption": "", "description": "NASA’s Solar Dynamics Observatory captured this image of an X3.9 flare on May 10, 2024. The image shows a blend of 171 and 131 Angstrom light, subsets of extreme ultraviolet light.
Credit: NASA/SDO", "items": [ { "id": 427187, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 1092093, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014588/SDO_X3pt9_Flare_May_10_2024_131-171_crop.jpg", "filename": "SDO_X3pt9_Flare_May_10_2024_131-171_crop.jpg", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured this image of an X3.9 flare on May 10, 2024. The image shows a blend of 171 and 131 Angstrom light, subsets of extreme ultraviolet light. Credit: NASA/SDO", "width": 1920, "height": 1920, "pixels": 3686400 } } ], "extra_data": {} }, { "id": 374186, "url": "https://svs.gsfc.nasa.gov/14588/#media_group_374186", "widget": "Single image", "title": "", "caption": "", "description": "NASA’s Solar Dynamics Observatory captured this image of an X3.9 flare on May 10, 2024. The image shows a blend of AIA 1600 Angstrom light and HMI Continuum.
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This region, along with another called AR 13663, was responsible for the majority of strong solar flares from May 3 through May 9.Watch this video on the NASA Goddard YouTube channel.Music credit: \"Collab Alert\" by Ellis Kent [PRS] from Universal Production Music || Thumbnail02.jpg (1280x720) [818.1 KB] || 14593_X-ClassFlaresDominateSunInMay_1080_YouTube.mp4 (1920x1080) [221.9 MB] || XClassFlares.en_US.srt [1.4 KB] || XClassFlares.en_US.vtt [1.3 KB] || 14593_X-ClassFlaresDominateSunInMay_4K_Facebook.mp4 (3840x2160) [328.8 MB] || 14593_X-ClassFlaresDominateSunInMay_4K_YouTube.mp4 (3840x2160) [539.4 MB] || 14593_X-ClassFlaresDominateSunInMay_4K_ProRes_.mov (3840x2160) [7.2 GB] || ", "release_date": "2024-05-16T10:00:00-04:00", "update_date": "2024-11-25T12:03:01.031406-05:00", "main_image": { "id": 1092366, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014593/JHV_2024-05-15_11.22.12-0001.png", "filename": "JHV_2024-05-15_11.22.12-0001.png", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the right – on May 15, 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", "width": 2048, "height": 2048, "pixels": 4194304 } }, { "id": 14592, "url": "https://svs.gsfc.nasa.gov/14592/", "page_type": "Produced Video", "title": "Largest Flare yet from Solar Cycle 25", "description": "On May 14, 2024, the Sun emitted a strong solar flare. This solar flare is the largest of Solar Cycle 25 and is classified as an X8.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.A solar flare is an intense burst of radiation, or light, on the Sun. Flares are our solar system’s most powerful explosive events. Light only takes about 8 minutes to travel from the Sun to Earth, so that’s how long it would take the energy from a flare to reach our planet. Stronger solar flares — those rated class M5 or above — can have impacts on technology that depends on Earth’s ionosphere (our electrically charged upper atmosphere), like high-frequency radio used for navigation and GPS.NASA’s Solar Dynamics Observatory (SDO) captured these images of the flare, which peaked at 12:51 p.m. ET on May 14. The X8.7 flare appears on the lower right edge of the Sun. (A small eruption appears afterward in the upper left.) SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. Different wavelengths are shown in this video to highlight different features of the flare.Music credit: “Ethereal Mirrorscape” from the album Reflections written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || X8pt7_flare_May_14_2024.00_00_40_22.Still001.jpg (3840x2160) [3.0 MB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_print.jpg (1024x576) [342.3 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_searchweb.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_web.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_thm.png (80x40) [6.1 KB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.webm (3840x2160) [20.4 MB] || 14592_SDO_X8pt7_flare_May_14_2024_Good_Outro.mp4 (3840x2160) [175.9 MB] || 14592_SDO_X8pt7_flare_May_14_2024_YouTube_Outro.mp4 (3840x2160) [673.0 MB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.mov (3840x2160) [4.2 GB] || ", "release_date": "2024-05-14T00:00:00-04:00", "update_date": "2025-03-09T23:18:57.886911-04:00", "main_image": { "id": 1092219, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014592/X8pt7_Flare_1651_May_14_2024_131-193-304_crop.jpg", "filename": "X8pt7_Flare_1651_May_14_2024_131-193-304_crop.jpg", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the right – on May 14, 2024. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in red and yellow. Credit: NASA/SDO", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 14589, "url": "https://svs.gsfc.nasa.gov/14589/", "page_type": "Produced Video", "title": "Continued Strong Solar Flare Activity: May 10-14, 2024", "description": "NASA’s Solar Dynamics Observatory captured images of the two solar flares on May 10 and May 11, 2024. The flares are classified as X5.8 and X1.5-class flares, respectively. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares created from a mixture of SDO’s AIA 193, 171 and 131 channels. Available with EDT and UTC time labels as well as unlabeled.Credit: NASA/SDO || May_11_side-by-side_EDT.jpg (2160x1080) [595.7 KB] || May_11_side-by-side_UTC.jpg (2160x1080) [595.3 KB] || May_11_side-by-side_no_text.jpg (2160x1080) [584.2 KB] || May_11_side-by-side_no_text_searchweb.png (320x180) [98.4 KB] || May_11_side-by-side_no_text_thm.png (80x40) [7.6 KB] || ", "release_date": "2024-05-11T10:00:00-04:00", "update_date": "2024-05-14T11:49:57.095798-04:00", "main_image": { "id": 1092154, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014589/May_11_side-by-side_no_text_searchweb.png", "filename": "May_11_side-by-side_no_text_searchweb.png", "media_type": "Image", "alt_text": "NASA’s Solar Dynamics Observatory captured images of the two solar flares on May 10 and May 11, 2024. The flares are classified as X5.8 and X1.5-class flares, respectively. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares created from a mixture of SDO’s AIA 193, 171 and 131 channels. Available with EDT and UTC time labels as well as unlabeled.Credit: NASA/SDO", "width": 320, "height": 180, "pixels": 57600 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }