{ "count": 741, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Solar+Activity%22", "previous": null, "results": [ { "id": 31375, "url": "https://svs.gsfc.nasa.gov/31375/", "result_type": "Visualization", "release_date": "2026-03-26T18:59:59-04:00", "title": "ISS views Aurora from the November 11-13, 2025 Geomagnetic Storm", "description": "This timelapse series of photos were taken from the ISS on November 12, 2026", "hits": 819 }, { "id": 31374, "url": "https://svs.gsfc.nasa.gov/31374/", "result_type": "Visualization", "release_date": "2026-03-26T10:59:59-04:00", "title": "Aurora Mosaic from the Geomagnetic Storm of November 11-13, 2025", "description": "A mosaic of Day/Night Band (DNB) images from the the Visible Infrared Imaging Radiometer (VIIRS) on the NOAA-20/JPSS-1 satellite showing a ring of bright auroral light extending south past 50N latitude.", "hits": 452 }, { "id": 40548, "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/", "result_type": "Gallery", "release_date": "2026-03-03T00:00:00-05:00", "title": "SOHO – Solar and Heliospheric Observatory", "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/", "hits": 500 }, { "id": 14972, "url": "https://svs.gsfc.nasa.gov/14972/", "result_type": "Produced Video", "release_date": "2026-02-27T12:00:00-05:00", "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] || ", "hits": 252 }, { "id": 14954, "url": "https://svs.gsfc.nasa.gov/14954/", "result_type": "Produced Video", "release_date": "2026-01-23T09:00:00-05:00", "title": "NASA's Illuminate Series (2026)", "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ", "hits": 341 }, { "id": 5503, "url": "https://svs.gsfc.nasa.gov/5503/", "result_type": "Visualization", "release_date": "2025-11-19T12:00:00-05:00", "title": "ESCAPADE Theoretical Flight Through Active Mars Magnetosphere", "description": "NASA's Escape and Plasma Acceleration Dynamics Explorers mission, or ESCAPADE, aims to study Mars' real-time response to the solar wind and how the Martian magnetosphere changes over time, helping us better understand Mars' climate history. In this data visualization, we use the September 13, 2017 solar storm that arrived at Mars as an example of a storm that the twin ESCAPADE spacecraft might study.", "hits": 396 }, { "id": 14927, "url": "https://svs.gsfc.nasa.gov/14927/", "result_type": "Produced Video", "release_date": "2025-11-19T10:00:00-05:00", "title": "The Sun Unleashes Six November X-class Flares", "description": "A blended composite image highlighting all six X-class flares from November 2025. The main image shows 131 Angstrom light, a subset of extreme ultraviolet light. The inset images show a variety of 131 and blends of 131, 171, and 304 Angstrom light. Credit: NASA/SDO/Scott Wiessinger || November_XFlares_All_6_Inset_Multi.jpg (7000x7000) [7.0 MB] || ", "hits": 295 }, { "id": 14907, "url": "https://svs.gsfc.nasa.gov/14907/", "result_type": "Produced Video", "release_date": "2025-09-30T14:00:00-04:00", "title": "What is space weather?", "description": "Though it is almost 100 million miles away from Earth, the Sun influences our daily lives in ways you may not realize.A farmer stops their planting operations due to poor GPS signal for their autonomous tractor. A power grid manager changes the configuration of their network to ensure a blackout doesn’t occur due to voltage instability. A pilot switches to back-up communication equipment due to loss of high-frequency radio. A commercial internet company providing service to the military must change the orbit of their spacecraft to avoid a collision due to increased atmospheric drag.These are a few examples of the ways the Sun influences our everyday lives. This is what we define as space weather – the conditions of the space environment driven by the Sun and its impacts on objects in the solar system. || ", "hits": 234 }, { "id": 14883, "url": "https://svs.gsfc.nasa.gov/14883/", "result_type": "Produced Video", "release_date": "2025-08-25T11:00:00-04:00", "title": "Mapping Stellar ‘Polka Dots’", "description": "Watch to learn how a new tool uses data from exoplanets, worlds beyond our solar system, to tell us about their polka-dotted stars.Credit: NASA’s Goddard Space Flight CenterMusic: “Whimsical Whirlwinds,” Claire Leona Batchelor [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Get the vertical version of this video [here](https://svs.gsfc.nasa.gov/14797/){target=_blank}. || PolkaDotStars_Thumbnail.jpg (1920x1080) [145.7 KB] || PolkaDotStars_Thumbnail_print.jpg (1024x576) [59.8 KB] || PolkaDotStars_Thumbnail_searchweb.png (320x180) [33.1 KB] || PolkaDotStars_Thumbnail_thm.png (80x40) [3.1 KB] || 14883_MappingStellarPolkaDots_Low.mp4 (1920x1080) [74.2 MB] || 14883_MappingStellarPolkaDots.mp4 (1920x1080) [262.9 MB] || MappingStellarPolkaDotsCaptions.en_US.srt [1.4 KB] || 14883_MappingStellarPolkaDots_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 125 }, { "id": 5375, "url": "https://svs.gsfc.nasa.gov/5375/", "result_type": "Visualization", "release_date": "2025-08-07T14:00:00-04:00", "title": "Carrington Class Coronal Mass Ejection - ENLIL Simulation of A Series of CMEs", "description": "A series of visualizations of the simulation of a series of CMEs between July 2012 and August 2012, including a carrington class coronal mass ejection that hit STEREO-A.", "hits": 310 }, { "id": 5567, "url": "https://svs.gsfc.nasa.gov/5567/", "result_type": "Visualization", "release_date": "2025-07-21T18:59:59-04:00", "title": "New Missions to L1", "description": "Three missions, Carruthers, IMAP and SWFO-L1 will be launched to the Sun-Earth Lagrange Point, L1.", "hits": 140 }, { "id": 5555, "url": "https://svs.gsfc.nasa.gov/5555/", "result_type": "Visualization", "release_date": "2025-07-15T10:00:00-04:00", "title": "TRACERS through Earth's Polar Cusps", "description": "Visualization of the orbit of the twin TRACERS (Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites) satellites that will explore the process of magnetic reconnection in Earth's polar regions and its effects on our atmosphere.", "hits": 183 }, { "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": 27 }, { "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": 32 }, { "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": 30 }, { "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": 48 }, { "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": 31 }, { "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": 17 }, { "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": 45 }, { "id": 5543, "url": "https://svs.gsfc.nasa.gov/5543/", "result_type": "Visualization", "release_date": "2025-06-11T10:00:00-04:00", "title": "Solar Magnetic Field - from Solar Minimum to Solar Maximum", "description": "Visualizations of the solar magnetic field evolution as a potential-field-source-surface model (PFSS) from solar minimum (2019) to solar maximum (2025).", "hits": 185 }, { "id": 20404, "url": "https://svs.gsfc.nasa.gov/20404/", "result_type": "Animation", "release_date": "2025-06-02T12:00:00-04:00", "title": "TRACERS Science Animations", "description": "The TRACERS, or the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 153 }, { "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": 23 }, { "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": 55 }, { "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": 13 }, { "id": 14829, "url": "https://svs.gsfc.nasa.gov/14829/", "result_type": "Produced Video", "release_date": "2025-04-25T10:00:00-04:00", "title": "TRACERS Thermal Vacuum Testing at Millennium Space Systems", "description": "NASA’s Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, or TRACERS, is embarking on its integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission. The TRACERS mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Below are clips of Millennium Space Systems’ team members conducting Thermal Vacuum (TVAC) testing at the Boeing Space Systems Laboratory in El Segundo, California.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 127 }, { "id": 14827, "url": "https://svs.gsfc.nasa.gov/14827/", "result_type": "Produced Video", "release_date": "2025-04-24T15:00:00-04:00", "title": "TRACERS Instrument Development & Testing at the University of Iowa", "description": "NASA’s Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, or TRACERS, is embarking on its integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission. The TRACERS mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Below are clips of TRACERS’ instrument design, build, and testing at the University of Iowa in Iowa City, Iowa.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 53 }, { "id": 14828, "url": "https://svs.gsfc.nasa.gov/14828/", "result_type": "Produced Video", "release_date": "2025-04-24T15:00:00-04:00", "title": "TRACERS Testing & Integration at Millennium Space Systems", "description": "NASA’s Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, or TRACERS, is embarking on its integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission. The TRACERS mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Below are clips of TRACERS’ testing and integration at the Millennium Space Systems Small Satellite Factory in El Segundo, California. Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 73 }, { "id": 40535, "url": "https://svs.gsfc.nasa.gov/gallery/tracers/", "result_type": "Gallery", "release_date": "2025-04-23T00:00:00-04:00", "title": "TRACERS – Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites", "description": "The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) helps understand magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when two magnetic fields, such as the Sun’s and Earth’s, intertwine and explosively realign. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth.\n\nTRACERS launched on July 23, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: https://science.nasa.gov/mission/tracers/", "hits": 184 }, { "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": 26 }, { "id": 5514, "url": "https://svs.gsfc.nasa.gov/5514/", "result_type": "Visualization", "release_date": "2025-04-07T09:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere for Fulldome", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents and magnetic fields combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 276 }, { "id": 5502, "url": "https://svs.gsfc.nasa.gov/5502/", "result_type": "Visualization", "release_date": "2025-04-07T00:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents (green colors) and magnetic fields (pink lines) combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 342 }, { "id": 14805, "url": "https://svs.gsfc.nasa.gov/14805/", "result_type": "Animation", "release_date": "2025-03-24T12:00:00-04:00", "title": "TRACERS Spacecraft Beauty Passes", "description": "The TRACERS, or the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ", "hits": 96 }, { "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": 21 }, { "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": 22 }, { "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": 28 }, { "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": 14 }, { "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": 8 }, { "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": 11 }, { "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": 17 }, { "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": 19 }, { "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": 17 }, { "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": 24 }, { "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": 18 }, { "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": 22 }, { "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": 23 }, { "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": 13 }, { "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": 18 }, { "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": 26 }, { "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": 17 }, { "id": 40532, "url": "https://svs.gsfc.nasa.gov/gallery/punch/", "result_type": "Gallery", "release_date": "2025-01-22T00:00:00-05:00", "title": "PUNCH – Polarimeter to Unify the Corona and Heliosphere", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in low Earth orbit capturing global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind, a stream of charged particles from the Sun that fills the solar system. By using PUNCH to image the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere — including the Sun, solar wind, and Earth — as a single connected system.\n\nPUNCH launched on March 11, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: science.nasa.gov/mission/punch", "hits": 225 }, { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "result_type": "Visualization", "release_date": "2024-12-12T12:00:00-05:00", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "hits": 297 }, { "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": 11 }, { "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": 7 }, { "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": 19 }, { "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": 27 }, { "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": 22 }, { "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": 21 }, { "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": 17 }, { "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": 16 }, { "id": 31324, "url": "https://svs.gsfc.nasa.gov/31324/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GMAO Band09 Obs Caribbean GMAO vs. GOES", "description": "GMAO Caribbean GOES vs GMAO || 3840x2160_16x9_30p [0 Item(s)] || GMAO Band09 Obs Caribbean GMAO vs. GOES ||", "hits": 16 }, { "id": 14706, "url": "https://svs.gsfc.nasa.gov/14706/", "result_type": "Produced Video", "release_date": "2024-11-08T13:00:00-05:00", "title": "NASA's Illuminate Series (2024)", "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ", "hits": 87 }, { "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": 24 }, { "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": 28 }, { "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": 31 }, { "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": 121 }, { "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": 62 }, { "id": 14685, "url": "https://svs.gsfc.nasa.gov/14685/", "result_type": "Produced Video", "release_date": "2024-10-15T15:00:00-04:00", "title": "What is Solar Maximum?", "description": "The Sun is stirring from its latest slumber. As sunspots and flares bubble from the Sun’s surface, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced on Tuesday, September 24, 2024, the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. || ", "hits": 321 }, { "id": 5344, "url": "https://svs.gsfc.nasa.gov/5344/", "result_type": "Visualization", "release_date": "2024-10-15T14:00:00-04:00", "title": "Solar Cycle 25 - the Solar Magnetic Field from Solar Minimum to Pole Flip", "description": "One advantage of long-lived missions like Solar Dynamics Observatory (SDO) is the ability to see slow but significant changes over long periods of time.This view from SDO's Helioseismic and Magnetic Imager (HMI) shows the evolution of sunspots on the solar disk starting from solar minimum (around December 2019) and into the maximum solar activity phase. The video ends in September 2024, however this maximum phase is expected to continue into 2025.", "hits": 561 }, { "id": 14683, "url": "https://svs.gsfc.nasa.gov/14683/", "result_type": "Produced Video", "release_date": "2024-10-15T13:30:00-04:00", "title": "NASA, NOAA Announce That the Sun Has Reached the Solar Maximum Period", "description": "In a teleconference with reporters on Tuesday, October 15, 2024, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South Poles swapping places every decade — and the Sun transitions from sluggish to active and stormy.During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity, such as the storm in May 2024, has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.Listen to the media telecon.Read NASA's article about the news. || ", "hits": 836 }, { "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": 25 }, { "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": 16 }, { "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": 8 }, { "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": 16 }, { "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": 11 }, { "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": 17 }, { "id": 14703, "url": "https://svs.gsfc.nasa.gov/14703/", "result_type": "Produced Video", "release_date": "2024-10-10T07:00:00-04:00", "title": "X1.8 Flare Erupts From Sun on October 8, 2024", "description": "NASA’s Solar Dynamics Observatory captured this imagery of an X1.8 solar flare – as seen in the bright flash in the center – on Oct. 08, 2024. The footage shows from 9:15 to 10:18 p.m. EDT in a blend of 171, 304, and 131 Angstrom light, subsets of extreme ultraviolet light. This cropped version is slowed to 1/3 speed. Credit: NASA/SDO || Video_Still.jpg (1920x1080) [570.8 KB] || Video_Still_searchweb.png (320x180) [106.4 KB] || Video_Still_thm.png (80x40) [7.7 KB] || SDO_10_09_24_X1pt8_131-171-304tpz.mp4 (1920x1080) [22.1 MB] || SDO_10_09_24_X1pt8_131-171-304tpz.mov (1920x1080) [154.8 MB] || ", "hits": 79 }, { "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": 17 }, { "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": 14 }, { "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": 19 }, { "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": 7 }, { "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": 8 }, { "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": 17 }, { "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": 4 }, { "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": 4 }, { "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": 18 }, { "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": 23 }, { "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": 14 }, { "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": 19 }, { "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": 17 }, { "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": 6 }, { "id": 40523, "url": "https://svs.gsfc.nasa.gov/gallery/escapade/", "result_type": "Gallery", "release_date": "2024-09-04T00:00:00-04:00", "title": "ESCAPADE – Escape and Plasma Acceleration and Dynamics Explorer", "description": "Using two identical spacecraft in orbit around Mars, the Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will investigate how a stream of charged particles from the Sun called the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE will use its twin orbiters to take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time. The data returned from ESCAPADE will provide new insight into the evolution of Mars’ climate, helping to understand how Mars began losing its atmosphere and water.\n\nESCAPADE launched on Nov. 13, 2025, from NASA’s Kennedy Space Center in Florida and is expected to reach Mars in September 2027.\n\nLearn more: https://science.nasa.gov/mission/escapade/ ", "hits": 300 }, { "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": 19 }, { "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": 17 } ] }