{ "count": 367, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Spectrum%22", "previous": null, "results": [ { "id": 31376, "url": "https://svs.gsfc.nasa.gov/31376/", "result_type": "Hyperwall Visual", "release_date": "2026-03-30T12:00:00-04:00", "title": "SPHEREx All Sky Map 2025", "description": "Two passes of an all-sky mosaic image from NASAs SPHEREx space telescope, the first showing dust and gas and the second showing stars and galaxies.", "hits": 470 }, { "id": 14968, "url": "https://svs.gsfc.nasa.gov/14968/", "result_type": "Produced Video", "release_date": "2026-03-25T12:00:00-04:00", "title": "XRISM Clocks Hot Wind of Galaxy M82", "description": "The Resolve instrument aboard the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft captured data revealing the velocity of the hot wind at the center of starburst galaxy M82. The energy range of iron emission lines show that the gas moves around 2 million miles (about 3 million kilometers) per hour. Inset: XRISM Xtend instrument’s image of M82.Credit: NASA’s Goddard Space Flight Center, JAXA/NASA, XRISM Collaboration et al. 2026Alt text: Spectrum and image of galaxy M82Image description: This image is labeled, “XRISM Resolve Measures the Hot Wind of Starburst Galaxy M82.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 2 to 9. The left side is labeled “X-ray brightness.” A squiggly white line starts near the bottom of the left side. Several peaks are labeled, including silicon, sulfur, argon, and calcium. Four peaks are identified as iron. In the upper right corner, a small inset shows an image that looks like a purple pansy with a yellow center. || v3_XRISM_Resolve_M82.jpg (4412x2993) [2.6 MB] || v3_XRISM_Resolve_M82_searchweb.png (320x180) [46.6 KB] || v3_XRISM_Resolve_M82_thm.png (80x40) [4.6 KB] || ", "hits": 712 }, { "id": 14966, "url": "https://svs.gsfc.nasa.gov/14966/", "result_type": "Produced Video", "release_date": "2026-02-14T00:00:00-05:00", "title": "SPHEREx Spacecraft and Observing Animations", "description": "SPHEREx is a small, highly-capable astronomy satellite mission that will map out the entire sky in 102 colors of infrared light from its vantage point in a low-Earth orbit. The spacecraft bus is powered by Sun-facing, rectangular solar panels.The white, conical Sun shield keeps the inner telescope components at a cool temperature that enables the detectors to operate with high sensitivity. The Sun shields are faded out at the end of the sequence to provide an unobstructed view of the telescope components.Credit: NASA/JPL-CaltechWatch this video on the JPLraw YouTube channel.JPL Page || SPHEREx_SurveyAnimationShot1_Stlll.jpg (3840x2160) [658.9 KB] || SPHEREx_SurveyAnimationShot1_Stlll_searchweb.png (320x180) [63.1 KB] || SPHEREx_SurveyAnimationShot1_Stlll_thm.png (80x40) [4.5 KB] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_ProRes422.mov (1920x1080) [703.6 MB] || SPHEREx_Shot1_Caption.en_US.srt [49 bytes] || SPHEREx_Shot1_Caption.en_US.vtt [59 bytes] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_4K.mp4 (3840x2160) [154.7 MB] || SPHEREx_SpacecraftAnimation_01_R27_TwoTurns_SpaceBackg_ProRes422_4K.mov (3840x2160) [2.0 GB] || ", "hits": 234 }, { "id": 14946, "url": "https://svs.gsfc.nasa.gov/14946/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Viewing an Exoplanet Transmission Spectrum", "description": "When planets orbiting distant stars are aligned just right, a host star's light can pass through its planet's atmosphere before reaching our telescopes. This alters the light, and by analyzing its spectrum, astronomers can find out what the planet’s atmosphere is made of. This animation is a quick visual representation of that process. || ", "hits": 363 }, { "id": 14947, "url": "https://svs.gsfc.nasa.gov/14947/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Webb Spectrum and Image Animations", "description": "These are animated versions of James Webb Space Telescope imagery and spectra. The spectra visualizations were created by the Space Telescope Science Institute and then animated at NASA's Goddard Space Flight Center. || ", "hits": 459 }, { "id": 14916, "url": "https://svs.gsfc.nasa.gov/14916/", "result_type": "Produced Video", "release_date": "2025-12-08T09:30:00-05:00", "title": "Black Hole Eats Star: The Longest GRB Ever Seen", "description": "Unusually long gamma-ray bursts require more exotic origins than typical GRBs. This animation illustrates one proposed explanation for GRB 250702B — the merger of a stellar-mass black hole with its stellar companion. As the black hole makes its last few orbits, it pulls large amounts of gas from the star. At some point in this process, the system begins to shine brightly in X-rays. Then, as the black hole enters the main body of the star, it rapidly consumes stellar matter, blasting gamma-ray jets (magenta) outward and causing the star to explode. Credit: NASA/LSU/Brian MonroeWatch this video on the NASA.gov Video YouTube channel. || Longest_GRB_Animation_Still.jpg (1920x1080) [296.0 KB] || Longest_GRB_Animation_Still_searchweb.png (320x180) [63.7 KB] || Longest_GRB_Animation_Still_thm.png (80x40) [5.5 KB] || NASA_GRB_Sequence_Final_v01.mp4 (1920x1080) [134.3 MB] || Longest_GRB_Animation_Captions.en_US.srt [1.2 KB] || Longest_GRB_Animation_Captions.en_US.vtt [1.2 KB] || NASA_GRB_Sequence_Final_v01.mov (1920x1080) [1.2 GB] || ", "hits": 603 }, { "id": 14871, "url": "https://svs.gsfc.nasa.gov/14871/", "result_type": "Produced Video", "release_date": "2025-07-24T09:55:00-04:00", "title": "Hubble Catches Intermediate-Sized Black Hole", "description": "NASA's Hubble Space Telescope revealed that most galaxies have supermassive black holes at their centers, but there's a mysterious middle category that's been nearly impossible to find: intermediate mass black holes. These elusive objects only are incredibly difficult to detect.Hubble and NASA's Chandra X-ray Observatory teamed up to study one of these rare items in galaxy NGC 6099. Chandra detected scorching X-rays at three million degrees while Hubble revealed an incredibly dense cluster of stars packed together, creating the perfect feeding ground for a hungry black hole.This discovery shows how different space telescopes working together across multiple wavelengths can unveil the complete story of these cosmic phenomena, helping us understand the full spectrum of black holes shaping our universe.For more information, visit science.nasa.gov/mission/hubbleCredit: NASA's Goddard Space Flight Center Paul Morris: Lead ProducerMusic Credit:\"Float On\" by Layla Pavey [PRS] and Samuel John Chase [PRS] via Zone Music Ltd [PRS] and Universal Production Music || ", "hits": 59 }, { "id": 14866, "url": "https://svs.gsfc.nasa.gov/14866/", "result_type": "Produced Video", "release_date": "2025-07-15T00:00:00-04:00", "title": "Cosmic Desktop & Phone Wallpapers", "description": "We can’t clean up your messy desktop, but we can provide a bit of beauty from the universe to act as a backdrop to it. Here you’ll find a collection of images from across the universe. Download these phone and desktop wallpapers for your screens. ||", "hits": 31825 }, { "id": 5560, "url": "https://svs.gsfc.nasa.gov/5560/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "M8.4 flare from Active Region 14114 - June 15, 2025", "description": "M8.4 flare from Active Region 14114 - June 15, 2025", "hits": 25 }, { "id": 5561, "url": "https://svs.gsfc.nasa.gov/5561/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "M6.3 flare from Active Region 14114 - June 16, 2025", "description": "M6.3 flare from Active Region 14114 - June 16, 2025", "hits": 30 }, { "id": 5562, "url": "https://svs.gsfc.nasa.gov/5562/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "X1.2 flare from Active Region 14114 - June 17, 2025", "description": "X1.2 flare from Active Region 14114 - June 17, 2025", "hits": 24 }, { "id": 5564, "url": "https://svs.gsfc.nasa.gov/5564/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "An X1.9 flare from AR 14114 - June 19, 2025", "description": "An X1.9 flare from AR 14114 on June 19, 2025.", "hits": 56 }, { "id": 5559, "url": "https://svs.gsfc.nasa.gov/5559/", "result_type": "Visualization", "release_date": "2025-07-10T10:00:00-04:00", "title": "M6.8 flare from Active Region 14105 - June 14, 2025", "description": "M6.8 flare from Active Region 14105 - June 14, 2025", "hits": 29 }, { "id": 5550, "url": "https://svs.gsfc.nasa.gov/5550/", "result_type": "Visualization", "release_date": "2025-07-09T10:00:00-04:00", "title": "M8.9 flare from Active Region 14098 - May 25, 2025", "description": "M8.9 flare from Active Region 14098 - May 25, 2025", "hits": 24 }, { "id": 5551, "url": "https://svs.gsfc.nasa.gov/5551/", "result_type": "Visualization", "release_date": "2025-07-09T10:00:00-04:00", "title": "M8.1 flare from Active Region 14100 - May 30, 2025", "description": "Solar active region 14100 launches an M8.1 flare on May 30, 2025.", "hits": 21 }, { "id": 5549, "url": "https://svs.gsfc.nasa.gov/5549/", "result_type": "Visualization", "release_date": "2025-06-25T10:00:00-04:00", "title": "X1.1 flare from Active Region 14098 - May 25, 2025", "description": "X1.1 flare from Active Region 14098 - May 25, 2025", "hits": 47 }, { "id": 31345, "url": "https://svs.gsfc.nasa.gov/31345/", "result_type": "Visualization", "release_date": "2025-06-11T18:59:59-04:00", "title": "One Year of PACE OCI Chlorophyll", "description": "The Ocean Color Instrument (OCI) on the Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite is a spectrometer designed to identify and quantify phytoplankton. This is a year-long visualization of the level 3 mapped chlorophyll data.", "hits": 147 }, { "id": 14857, "url": "https://svs.gsfc.nasa.gov/14857/", "result_type": "Produced Video", "release_date": "2025-06-11T14:10:00-04:00", "title": "NASA’s Webb Reveals Galaxy Population Driving Cosmic Renovation", "description": "Symbols mark the locations of young, low-mass galaxies bursting with new stars when the universe was about 800 million years old. Using a filter sensitive to such galaxies, NASA’s James Webb Space Telescope imaged them with the help of a natural gravitational lens created by the massive galaxy cluster Abell 2744. In all, 83 young galaxies were found, but only the 20 shown here (white diamonds) were selected for deeper study. The inset zooms into one of the galaxies. Credit: NASA/ESA/CSA/Bezanson et al. 2024 and Wold et al. 2025Alt text: Animation showing the locations of young, low-mass, starburst galaxies around galaxy cluster Abell 2744.Image description:White and yellow galaxies of various sizes and shapes appear against the blackness of space. Two bright stars in our own galaxy display prominent six-spike diffraction patterns with bluish rays, visible at center left and lower left. Then 20 white diamonds sweep across the image. One diamond enlarges to reveal an image of a young, low-mass, star-forming galaxy. It looks like a green oval against a red and green checked background. The enlarged image then shrinks back, and the diamonds sweep away. The sequence loops. || Pandora_stamp_60pct.gif (600x600) [961.0 KB] || ", "hits": 270 }, { "id": 31353, "url": "https://svs.gsfc.nasa.gov/31353/", "result_type": "Animation", "release_date": "2025-06-09T18:59:59-04:00", "title": "Supermassive Black Holes", "description": "In this video NuSTAR (Nuclear Spectroscopic Telescope Array) lead scientist Peter Boorman explains how the NuSTAR penetrates thick gas and dust to reveal black holes that other telescopes can’t see. \r\n\r\nThis video was prepared for use on the NASA Hyperwall from content originally published at [https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/](https://www.jpl.nasa.gov/videos/using-x-ray-eyes-to-find-hidden-black-holes-nasas-nustar-mission/)", "hits": 269 }, { "id": 5541, "url": "https://svs.gsfc.nasa.gov/5541/", "result_type": "Visualization", "release_date": "2025-05-28T18:59:59-04:00", "title": "X1.2 flare from Active Region 14086 - May 13, 2025", "description": "X1.2 flare from Active Region 14086 - May 13, 2025", "hits": 26 }, { "id": 5542, "url": "https://svs.gsfc.nasa.gov/5542/", "result_type": "Visualization", "release_date": "2025-05-28T06:59:59-04:00", "title": "X2.7 and more flares from Active Region 14087 - May 14, 2025", "description": "An X 2.7 flare from Active region 14087 and a couple more, May 14, 2025, as seen by Solar Dynamics Observatory (SDO).", "hits": 16 }, { "id": 5407, "url": "https://svs.gsfc.nasa.gov/5407/", "result_type": "Visualization", "release_date": "2025-05-28T00:00:00-04:00", "title": "Solar Loops and Eruptions - October 8, 2024", "description": "A fourteen hour continuous observation of the Sun, showing the variety of eruptions.", "hits": 56 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 486 }, { "id": 5527, "url": "https://svs.gsfc.nasa.gov/5527/", "result_type": "Visualization", "release_date": "2025-05-22T00:00:00-04:00", "title": "M5.6 flare from Active Region 14046 - April 1, 2025 - No foolin'!", "description": "Active Region 14046 launches an M5.6 flare on April 1, 2025.", "hits": 10 }, { "id": 5526, "url": "https://svs.gsfc.nasa.gov/5526/", "result_type": "Visualization", "release_date": "2025-04-14T00:00:00-04:00", "title": "X1.1 flare from Active Region 14046 - March 28, 2025", "description": "Active region 14046 (on the left limb of the Sun) launches an X1.1 flare and a significant amount of plasma.", "hits": 27 }, { "id": 5482, "url": "https://svs.gsfc.nasa.gov/5482/", "result_type": "Visualization", "release_date": "2025-03-17T00:00:00-04:00", "title": "An M9.4 flare from Active Region 13910 - November 25, 2024", "description": "As solar rotation carries it over the left limb of the Sun, Active Region 13910 launches an M9.4 flare.", "hits": 20 }, { "id": 14796, "url": "https://svs.gsfc.nasa.gov/14796/", "result_type": "Produced Video", "release_date": "2025-03-14T12:00:00-04:00", "title": "Beyond the Visible: Landsat Next’s New Spectral Bands", "description": "Landsat Next takes Earth observation beyond the visible, unlocking new insights to protect our planet like never before. || LNext_Spectral_Thumb.png (1920x1080) [1.4 MB] || LNext_Spectral_Thumb_print.jpg (1024x576) [136.3 KB] || LNext_Spectral_Thumb_searchweb.png (320x180) [81.4 KB] || LNext_Spectral_Thumb_thm.png [7.0 KB] || NASA_LNextSpectral_Final_REV.webm (1920x1080) [66.0 MB] || NASA_LNextSpectral.en_US.vtt [14.2 KB] || NASA_LNextSpectral.en_US.srt [14.3 KB] || NASA_LNextSpectral_Final_REV.mp4 (1920x1080) [1.2 GB] || ", "hits": 47 }, { "id": 5513, "url": "https://svs.gsfc.nasa.gov/5513/", "result_type": "Visualization", "release_date": "2025-03-12T00:00:00-04:00", "title": "X2.0 flare from Active Region 14001 - February 23, 2025", "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.Just before rotating over the right solar limb, active region 14001 launches an X2.0 flare. For more details see the Space Weather database entry.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 some of this imagery. || ", "hits": 15 }, { "id": 5488, "url": "https://svs.gsfc.nasa.gov/5488/", "result_type": "Visualization", "release_date": "2025-03-05T08:02:00-05:00", "title": "An M7.1 flare from Active Region 13936 - December 29, 2024", "description": "Active Region 13936 launches an M7.1 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 21 }, { "id": 5483, "url": "https://svs.gsfc.nasa.gov/5483/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X2.2 flare from Active Region 13912 - December 8, 2024", "description": "Active region 13912 launches an X2.2 flare near the right limb on December 8, 2024.", "hits": 22 }, { "id": 5486, "url": "https://svs.gsfc.nasa.gov/5486/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M8.9 flare from Active Region 13932 - December 23, 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.Active region 13932 (in the lower left quadrant) launches an M8.9 flare on December 23. 2024. Some filaments of plasma launch from the site after the flare. For more details, see the Space Weather Database entry.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 some of this imagery. || ", "hits": 17 }, { "id": 5487, "url": "https://svs.gsfc.nasa.gov/5487/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M7.4 flare from Active Region 13938 - December 26, 2024", "description": "Active region 13938 (upper left quadrant) launches an M7.4 flare.", "hits": 6 }, { "id": 5489, "url": "https://svs.gsfc.nasa.gov/5489/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X1.1 flare from Active Region 13936 - December 29, 2024", "description": "Active region 13936 (upper right quadrant) launches an X1.1 flare.", "hits": 10 }, { "id": 5484, "url": "https://svs.gsfc.nasa.gov/5484/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.4 flare from Active Region 13922 - December 10, 2024", "description": "Active region 13922 launches an M6.4 flare near the left limb of the Sun on December 10, 2024.", "hits": 25 }, { "id": 5485, "url": "https://svs.gsfc.nasa.gov/5485/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.7 flare from Active Region 13912 - December 11, 2024", "description": "Active region 13912 on the right limb of the Sun launches an M6.7 flare on December 11, 2024.", "hits": 16 }, { "id": 5500, "url": "https://svs.gsfc.nasa.gov/5500/", "result_type": "Visualization", "release_date": "2025-03-03T00:00:00-05:00", "title": "M7.6 flare from Active Region 13981 - February 6, 2025", "description": "Active Region 13981 (in the upper right quadrant of the disk) launches an M7.6 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 16 }, { "id": 5501, "url": "https://svs.gsfc.nasa.gov/5501/", "result_type": "Visualization", "release_date": "2025-03-03T00:00:00-05:00", "title": "M7.5 flare from Active Region 13981 - February 7, 2025", "description": "Active Region 13981 (in the upper right quadrant of the disk) launches an M7.5 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 12 }, { "id": 5495, "url": "https://svs.gsfc.nasa.gov/5495/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M7.4 flare from Active Region 13964 - January 17, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13964 (in the upper right quadrant of the disk) launch an M7.4 flare followed by some complex post-flare evolution.", "hits": 10 }, { "id": 5496, "url": "https://svs.gsfc.nasa.gov/5496/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.7 flare from Active Region 13978 - January 31, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13978 launch an M6.7 flare on January 31, 2025.", "hits": 15 }, { "id": 5497, "url": "https://svs.gsfc.nasa.gov/5497/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M5.1 flare from Active Region 13977 - February 2, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13977 (in the upper center of the disk) launch an M5.1 flare and a filament of material on February 2, 2025.", "hits": 18 }, { "id": 5498, "url": "https://svs.gsfc.nasa.gov/5498/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M8.8 flare from Active Region 13981 - February 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13981 launch an M8.8 flare early February 3, 2025 (a smaller M3.1 fires off near the same location about two hours later). The Earth eclipses the view from SDO as the video ends.", "hits": 20 }, { "id": 5499, "url": "https://svs.gsfc.nasa.gov/5499/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.1 flare from Active Region 13981 - February 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13981 launching an M6.1 flare on February 3, 2025.", "hits": 10 }, { "id": 5494, "url": "https://svs.gsfc.nasa.gov/5494/", "result_type": "Visualization", "release_date": "2025-02-20T00:00:00-05:00", "title": "X1.8 flare from Active Region 13947 - January 4, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13947 launch an X1.8 flare on January 4, 2025.", "hits": 20 }, { "id": 5492, "url": "https://svs.gsfc.nasa.gov/5492/", "result_type": "Visualization", "release_date": "2025-02-19T00:00:00-05:00", "title": "X1.2 flare from Active Region 13947 - January 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes active region 13947 launch an X1.2 flare on January 3, 2025.", "hits": 20 }, { "id": 5493, "url": "https://svs.gsfc.nasa.gov/5493/", "result_type": "Visualization", "release_date": "2025-02-19T00:00:00-05:00", "title": "X1.1 and M- flares from Active Region 13947 - January 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13947 launch an X1.1 flare followed by a couple of M-class flares on January 3-4 of 2025.", "hits": 19 }, { "id": 14754, "url": "https://svs.gsfc.nasa.gov/14754/", "result_type": "Produced Video", "release_date": "2025-01-16T10:14:00-05:00", "title": "NASA’s Pandora Mission Closer To Probing Alien Atmospheres", "description": "Basic overview of NASA's Pandora mission, which will revolutionize the study of exoplanet atmospheres.", "hits": 125 }, { "id": 5430, "url": "https://svs.gsfc.nasa.gov/5430/", "result_type": "Visualization", "release_date": "2024-12-02T00:00:00-05:00", "title": "An M9.4 flare from Active Region 13889 and more - November 10, 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.Active region 13889 launches an M9.4 flare on November 10, 2024. For more details, see the Space Weather Database entry.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 some of this imagery. || ", "hits": 7 }, { "id": 5426, "url": "https://svs.gsfc.nasa.gov/5426/", "result_type": "Visualization", "release_date": "2024-11-29T00:00:00-05:00", "title": "An M5.5 flare from Active Region 13883 - November 4, 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.Active region 13883 launched an M5.5 flare on November 4, 2024. For more details, see the Space Weather Database entry.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 some of this imagery. || ", "hits": 5 }, { "id": 5427, "url": "https://svs.gsfc.nasa.gov/5427/", "result_type": "Visualization", "release_date": "2024-11-29T00:00:00-05:00", "title": "An X2.3 flare from Active Region 13878 and more - November 6, 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.Active Region 13878 launches an X2.3 flare, between a couple of M5+ flares, on November 6, 2024. For more details, see the Space Weather Database for the entries M 5.8 (peek at 2024-11-06T08:50), X2.3 (peak at 2024-11-06T13:40) and M5.3 (peak at 2024-11-06T14:38).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 some of this imagery. || ", "hits": 18 }, { "id": 5411, "url": "https://svs.gsfc.nasa.gov/5411/", "result_type": "Visualization", "release_date": "2024-11-28T00:00:00-05:00", "title": "An M6.5 flare from Active Region 13854 - October 19, 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.In a last flash before rotating over the limb, active region 13854 launches an M6.5 flare on October 19, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 14 }, { "id": 5403, "url": "https://svs.gsfc.nasa.gov/5403/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 flare from Active Region 13848 - October 9, 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.Active Region 13848 launches an X1.8 flare on October 9, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 34 }, { "id": 5406, "url": "https://svs.gsfc.nasa.gov/5406/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.7 flare from Active Region 13842 - October 9, 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.In a last flash before rotating over the limb, active region 13842 launches an M7.7 flare on October 9, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 12 }, { "id": 5413, "url": "https://svs.gsfc.nasa.gov/5413/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 & M9.5 flare from Active Region 13873 - October 26, 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.Double flares launch from the same active region (AR 13873) less than an hour apart. For more details, see the Space Weather Database entry for M9.5 @ 2024-10-26T06:23 TAI and X1.8 @ 2024-10-26T07:19 TAI.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 some of this imagery. || ", "hits": 17 }, { "id": 5420, "url": "https://svs.gsfc.nasa.gov/5420/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.2 flare from Active Region 13878 - October 30,2024", "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.Active Region 13878 launches an M7.2 flare. For more details, see the Space Weather Database entry.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 some of this imagery. || ", "hits": 4 }, { "id": 5421, "url": "https://svs.gsfc.nasa.gov/5421/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X2.0 and M9.4 flare from Active Region 13878 - October 31, 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.Active Region 13878 presents a 'double whammy' of two strong flares (X 2.0 and M9.4) only about 30 minutes apart. For more details, see the Space Weather Database entries for X2.0 (peak @ 2024-10-31T21:20) and M9.4 (peak @ 2024-10-31T21:54).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 some of this imagery. || ", "hits": 8 }, { "id": 5412, "url": "https://svs.gsfc.nasa.gov/5412/", "result_type": "Visualization", "release_date": "2024-11-26T00:00:00-05:00", "title": "An X3.3 flare from Active Region 13869 - October 24, 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.Active region 13869 launches an X3.3 flare on October 24, 2024. For more details, see the Space Weather Database entry.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 some of this imagery. || ", "hits": 15 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 655 }, { "id": 14650, "url": "https://svs.gsfc.nasa.gov/14650/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Infrared Detector and Spectrometer", "description": "EXCITE (EXoplanet Climate Infrared TElescope) is designed to study atmospheres around exoplanets, or worlds beyond our solar system, during long-duration scientific balloon trips over Antarctica.These images, taken in July 2024, show Peter Nagler and Nat DeNigris preparing EXCITE’s infrared detector and installing it into the mission’s spectrometer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. At the time, the EXCITE team was gearing up for a test flight in Fort Sumner, New Mexico. || ", "hits": 42 }, { "id": 14715, "url": "https://svs.gsfc.nasa.gov/14715/", "result_type": "Produced Video", "release_date": "2024-11-18T00:00:00-05:00", "title": "COBE Celebrates 35th Launch Anniversary", "description": "Technicians work on the COBE (Cosmic Background Explorer) spacecraft in a clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The mission launched into an Earth orbit in 1989 to make an all-sky map of the cosmic microwave background, the oldest light in the universe. The conical silver shield protects the scientific instruments from direct radiation from the Sun and Earth, isolates them from radio-frequency interference from the spacecraft transmitters and terrestrial sources, and provides thermal isolation for a dewar containing liquid helium coolant.Credit: NASA/COBE Science Team || COBE_in_gfsc_clean_room_1.jpg (1629x1600) [552.8 KB] || ", "hits": 212 }, { "id": 5402, "url": "https://svs.gsfc.nasa.gov/5402/", "result_type": "Visualization", "release_date": "2024-11-05T00:00:00-05:00", "title": "An X2.1 and X1.0 flare from Active Region 13842 - October 7, 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.Active region 13842 launches an X2.1, followed less than 30 minutes later by an X1.0 flare on October 7, 2024. For more details, see the Space Weather Database for the X2.1 flare and the X1.0 flare.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. || ", "hits": 22 }, { "id": 5399, "url": "https://svs.gsfc.nasa.gov/5399/", "result_type": "Visualization", "release_date": "2024-11-04T00:00:00-05:00", "title": "An M6.7 flare from Active Region 13843 - October 3, 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.", "hits": 23 }, { "id": 5398, "url": "https://svs.gsfc.nasa.gov/5398/", "result_type": "Visualization", "release_date": "2024-10-30T00:00:00-04:00", "title": "An X9.0 flare from Active Region 13842 - October 3, 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.", "hits": 41 }, { "id": 14704, "url": "https://svs.gsfc.nasa.gov/14704/", "result_type": "Produced Video", "release_date": "2024-10-23T06:00:00-04:00", "title": "NASA Interview Opportunity: Star light, star bright, check out the evening sky on your Halloween walk tonight", "description": "Scroll down the page to find b-roll for the live shots + a pre-recorded interview with Rebekah HounsellFor more information check out: @NASAUniverse on social media platforms and universe.nasa.gov online || T_CrB_banner_-_ENGLISH.png (1800x720) [1.8 MB] || T_CrB_banner_-_ENGLISH_print.jpg (1024x409) [109.8 KB] || T_CrB_banner_-_ENGLISH_searchweb.png (320x180) [80.0 KB] || T_CrB_banner_-_ENGLISH_thm.png (80x40) [7.0 KB] || ", "hits": 70 }, { "id": 31319, "url": "https://svs.gsfc.nasa.gov/31319/", "result_type": "Hyperwall Visual", "release_date": "2024-10-23T00:00:00-04:00", "title": "2025 NASA Science Calendar", "description": "Images from the 2025 NASA Science Calendar", "hits": 124 }, { "id": 5397, "url": "https://svs.gsfc.nasa.gov/5397/", "result_type": "Visualization", "release_date": "2024-10-17T00:00:00-04:00", "title": "An X7.1 flare from Active Region 13842 - October 1, 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.Active Region AR 13842 launches an X7.1 flare on October 1, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 72 }, { "id": 5396, "url": "https://svs.gsfc.nasa.gov/5396/", "result_type": "Visualization", "release_date": "2024-10-15T00:00:00-04:00", "title": "An M7.6 flare from Active Region 13842 - September 30, 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.An M7.6 flare fires off from Active Region 13842 on September 30, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 27 }, { "id": 5370, "url": "https://svs.gsfc.nasa.gov/5370/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An M5.1 flare from Active Region 13800 - August 23, 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.Active Region AR 13800 launches an M5.1 flare on August 23, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 14 }, { "id": 5385, "url": "https://svs.gsfc.nasa.gov/5385/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An M5.0 flare from Active Region 13811 - September 11, 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.Active Region AR 13811 launches an M5.0 flare on September 11, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 20 }, { "id": 5386, "url": "https://svs.gsfc.nasa.gov/5386/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An X1.3 flare from Active Region 13825 - and later an M6.8 - September 12, 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.Active Region AR 13825 launches an X1.3 flare on the lower left limb on September 12, 2024. Later, an M6.8 (14:43 TAI) erupts on the right limb. For more details, see the Space Weather Database for X1.3 and M6.8. An additional small filament eruption occurs near the center of the disk about 17:24 TAI.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. || ", "hits": 24 }, { "id": 5387, "url": "https://svs.gsfc.nasa.gov/5387/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An M5.4 flare from Active Region 13811 - September 13, 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.Framed by a set of large coronal loops, active Region AR 13811 launches an M5.4 flare on September 13, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 22 }, { "id": 5388, "url": "https://svs.gsfc.nasa.gov/5388/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An X4.5 flare from Active Region 13825 - September 14, 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.", "hits": 28 }, { "id": 5359, "url": "https://svs.gsfc.nasa.gov/5359/", "result_type": "Visualization", "release_date": "2024-10-03T00:00:00-04:00", "title": "An M5.3 flare from Active Region 13780 - August 10, 2024", "description": "Active Region AR 13780 launches an M5.3 flare on August 10, 2024. For more details, see the Space Weather Database entry.", "hits": 23 }, { "id": 5367, "url": "https://svs.gsfc.nasa.gov/5367/", "result_type": "Visualization", "release_date": "2024-10-03T00:00:00-04:00", "title": "An X1.1 flare from Active Region 13784 - August 14, 2024", "description": "Active Region AR 13784 launches an X1.1 flare on August 14, 2024.", "hits": 11 }, { "id": 5346, "url": "https://svs.gsfc.nasa.gov/5346/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An X1.5 flare from Active Region 13764 - July 29, 2024", "description": "Active Region AR 13764 launches an X1.5 flare on July 29, 2024. A small M1 erupts later in the lower right quadrant (05:20 TAI). Then the 'curtain' falls as Earth eclipses. SDO's geosynchronous orbit around Earth enables the Sun to occasionally be eclipsed by Earth (Eclipse Season Starts for NASA's SDO).", "hits": 28 }, { "id": 5347, "url": "https://svs.gsfc.nasa.gov/5347/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An M8.7 flare from Active Region 13762 and more - July 29, 2024", "description": "Active Region AR 13762 launches an M8.7 flare on July 29, 2024. A smaller M4.2 flare fires shortly thereafter (14:42 TAI) on the left limb. For more details, see the Space Weather Database entry for M8.7 and M4.2.", "hits": 6 }, { "id": 5355, "url": "https://svs.gsfc.nasa.gov/5355/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An X1.7 flare from Active Region 13765 and some extra energetic activity - August 5, 2024", "description": "Active Region AR 13765 launches an X1.7 flare on August 5, 2024 on the rightmost part of the solar limb. Shortly thereafter, an X1.1 flare launches near the left limb from AR 13780. For more details, see the Space Weather Database entry for X1.7 and X1.1. Towards the end of this visualization, around 18:35 TAI, a bright filament launches near the center of the disk.", "hits": 9 }, { "id": 5356, "url": "https://svs.gsfc.nasa.gov/5356/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An M6.1 flare from Active Region 13780 - August 5, 2024", "description": "Active Region AR 13780 launches an M6.1 flare on August 5, 2024. Shortly thereafter, the Earth eclipses the Sun in the view from SDO.", "hits": 10 }, { "id": 5357, "url": "https://svs.gsfc.nasa.gov/5357/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An M5.0 flare from Active Region 13777 - August 7, 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.Active Region AR 13777 near the center of the solar disk launches an impressive M5.0 flare on August 7, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 9 }, { "id": 5358, "url": "https://svs.gsfc.nasa.gov/5358/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An X1.3 flare from Active Region 13777 - August 8, 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.Active Region AR 13777 launches a larger flare, an X1.3, on August 8, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 31 }, { "id": 5368, "url": "https://svs.gsfc.nasa.gov/5368/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An M5.3 flare from Active Region 13790 - August 14, 2024", "description": "Active Region AR 13790 launches an M5.3 flare on August 14, 2024.", "hits": 9 }, { "id": 5369, "url": "https://svs.gsfc.nasa.gov/5369/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An M5.1 flare from Active Region 13796 - August 21, 2024", "description": "Active Region AR 13796 launches an M5.1 flare on August 21, 2024.", "hits": 7 }, { "id": 5353, "url": "https://svs.gsfc.nasa.gov/5353/", "result_type": "Visualization", "release_date": "2024-09-12T00:00:00-04:00", "title": "An M7.4 flare from Active Region 13768 - August 2, 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.Active Region AR 13768 launches an M7.4 flare on August 2, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 12 }, { "id": 5354, "url": "https://svs.gsfc.nasa.gov/5354/", "result_type": "Visualization", "release_date": "2024-09-12T00:00:00-04:00", "title": "An M7.3 flare from Active Region 13775 - August 3, 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.Active Region AR 13775 launches an M7.3 flare on August 3, 2024 and later AR13781 launched an M5.4 flare. For more details, see for M7.3 and for M5.4.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. || ", "hits": 17 }, { "id": 5349, "url": "https://svs.gsfc.nasa.gov/5349/", "result_type": "Visualization", "release_date": "2024-09-11T00:00:00-04:00", "title": "An M9.4 flare from Active Region 13772 - July 30, 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.Minutes after a small (M1.9) flare erupts in the lower right quadrant of the disk (19:20 TAI), Active Region AR 13772 launches an M9.4 flare (19:38 TAI) on July 30, 2024.", "hits": 15 }, { "id": 5351, "url": "https://svs.gsfc.nasa.gov/5351/", "result_type": "Visualization", "release_date": "2024-09-11T00:00:00-04:00", "title": "An M6.0 flare from Active Region 13772 (and an M5.3 from AR 13768) - July 31, 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.Active Region AR 13772 continues its launches of M-flares with an M6.0 flare on July 31, 2024. Later (18:05TAI), an M5.3 flare launches from AR13768. For more details, see M 6.0 and M5.3.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. || ", "hits": 14 }, { "id": 5352, "url": "https://svs.gsfc.nasa.gov/5352/", "result_type": "Visualization", "release_date": "2024-09-11T00:00:00-04:00", "title": "Multiple M-flares and an Earth Eclipse - August 1, 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.Active Region AR 13773 launches an M6.3 flare (right lower quadrant) followed by an Earth eclipse, after which AR 13768 launches an M8.2 flare on August 1, 2024.", "hits": 14 }, { "id": 5348, "url": "https://svs.gsfc.nasa.gov/5348/", "result_type": "Visualization", "release_date": "2024-09-10T00:00:00-04:00", "title": "An M6.4 flare from Active Region 13772 - July 29, 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.Active Region AR 13772 launches an M6.4 flare on July 29, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 9 }, { "id": 5330, "url": "https://svs.gsfc.nasa.gov/5330/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "A rapid-fire M7.8 and M9.9 flare from Active Region 13766 - July 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.Active Region AR 13766 launches a M7.8 flare followed shortly after by an M9.9 flare on July 28, 2024. For more details, see the respective Space Weather database entries (M7.8 and M9.9).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. || ", "hits": 16 }, { "id": 5334, "url": "https://svs.gsfc.nasa.gov/5334/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "An M5.3 flare from Active Region 13738 - July 13, 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.Active Region AR 13738 launches an M5.3 flare on July 13, 2024. For more details, see the Space Weather Database entry. There's also a nice eruption off the left limb.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. || ", "hits": 15 }, { "id": 5335, "url": "https://svs.gsfc.nasa.gov/5335/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "An M5, then an X1.2 flare erupt from Active Region 13738 - July 13-14, 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.Active Region AR 13738 launches an M5 flare, followed by a larger X1.2 flare, on July 13-14, 2024. For more details, see the Space Weather Database entries M5 and X1.2 entries.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. || ", "hits": 6 }, { "id": 5336, "url": "https://svs.gsfc.nasa.gov/5336/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "An X1.9 flare from Active Region 13738 - July 16, 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.Active Region AR 13738 launches an X1.9 flare on July 16, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 5 }, { "id": 5337, "url": "https://svs.gsfc.nasa.gov/5337/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "An M5.0 flare from Active Region 13743 - and an Earth Eclipse - July 17, 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.Active Region AR 13743 launches an M5.0 flare on July 17, 2024. Moments later, the Sun was eclipsed by Earth from SDO so we don't get to enjoy much of the post-flare evolution. SDO's geosynchronous orbit around Earth enables the Sun to occasionally be eclipsed by Earth (Eclipse Season Starts for NASA's SDO). For more details, see the Space Weather Database entry.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. || ", "hits": 16 }, { "id": 5345, "url": "https://svs.gsfc.nasa.gov/5345/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "Another Double-Flare Event: M7.7 flare from Active Region 13762 (and a little M2.6 from AR 13737) - July 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.Active Region AR 13762 launches an M7.7 flare on July 28, 2024. A smaller M2.6 flare fires from a nearby active region in the lower left quadrant at about 12:50TAI. For more details, see the Space Weather Database entry.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. || ", "hits": 14 }, { "id": 14634, "url": "https://svs.gsfc.nasa.gov/14634/", "result_type": "Produced Video", "release_date": "2024-07-25T14:00:00-04:00", "title": "Fermi Finds Novel Feature in BOAT Gamma-Ray Burst", "description": "The brightest gamma-ray burst yet recorded gave scientists a new high-energy feature to study. Learn what NASA’s Fermi mission saw, and what this feature may be telling us about the burst’s light-speed jets. Credit: NASA's Goddard Space Flight CenterMusic: “Tides,” Jon Cotton [PRS] and Ben Niblett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Distant_GRB_still.jpg (3840x2160) [2.5 MB] || 14634_Fermi_GRB_Emission_Line_Under100.mp4 (1920x1080) [90.7 MB] || 14634_Fermi_GRB_Emission_Line_Best.mp4 (1920x1080) [422.0 MB] || 14634FermiGRBEmissionLine_Captions.en_US.srt [4.4 KB] || 14634FermiGRBEmissionLine_Captions.en_US.vtt [4.2 KB] || 14634_Fermi_GRB_Emission_Line_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || ", "hits": 133 }, { "id": 5317, "url": "https://svs.gsfc.nasa.gov/5317/", "result_type": "Visualization", "release_date": "2024-07-22T00:00:00-04:00", "title": "An X1.5 flare from Active Region 13697 - June 10, 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.Active Region AR 13697 launches an X1.5 flare on June 10, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 16 }, { "id": 5318, "url": "https://svs.gsfc.nasa.gov/5318/", "result_type": "Visualization", "release_date": "2024-07-22T00:00:00-04:00", "title": "An M9.5 flare from Active Region 13697 - June 10, 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.Active Region AR 13697 launches an M9.5 flare on June 10, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 12 }, { "id": 5323, "url": "https://svs.gsfc.nasa.gov/5323/", "result_type": "Visualization", "release_date": "2024-07-22T00:00:00-04:00", "title": "An M5.7 flare from Active Region 13719 - June 20, 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.Active Region AR 13719 launches an M5.7 flare on June 20, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 15 }, { "id": 5324, "url": "https://svs.gsfc.nasa.gov/5324/", "result_type": "Visualization", "release_date": "2024-07-22T00:00:00-04:00", "title": "An M9.3 flare from Active Region 13723 - June 23, 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.Active Region AR 13723 launches an M9.3 flare on June 23, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 44 }, { "id": 5293, "url": "https://svs.gsfc.nasa.gov/5293/", "result_type": "Visualization", "release_date": "2024-07-10T00:00:00-04:00", "title": "An X1.7 flare from Active Region 13664 - May 14, 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.An X1.7 flare erupts at the right solar limb from Active Region 13664 on May 14, 2024. For more details, see the Space Weather Database entry.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. || ", "hits": 28 }, { "id": 5288, "url": "https://svs.gsfc.nasa.gov/5288/", "result_type": "Visualization", "release_date": "2024-07-09T00:00:00-04:00", "title": "An X1.5 flare and more from Active Region 13664 - May 11, 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.An X1.5 flare erupts from Active Region 13664 (lower right quadrant) on May 11, 2024. Less than four hours later, a smaller M8.8 flare erupts from the same region. For more details, see the Space Weather Database for the X1.5 and M8.8 entries. A large filament is also forming on the lower right solar limb.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. || ", "hits": 71 } ] }