{ "count": 827, "next": "https://svs.gsfc.nasa.gov/api/search/?keywords=Sun-earth+Interactions&limit=100&offset=100", "previous": null, "results": [ { "id": 5647, "url": "https://svs.gsfc.nasa.gov/5647/", "result_type": "Visualization", "release_date": "2026-05-22T14:00:00-04:00", "title": "Map of the August 12, 2026, Total Solar Eclipse", "description": "On Wednesday, August 12, 2026, the Moon passes in front of the Sun, casting its shadow across a broad swath of Earth's northern hemisphere. Totality is visible in Spain and Iceland, while the rest of Europe and parts of North America and Africa experience a partial eclipse.", "hits": 5991 }, { "id": 5643, "url": "https://svs.gsfc.nasa.gov/5643/", "result_type": "Visualization", "release_date": "2026-05-12T12:00:00-04:00", "title": "The Ring Current in Earth's Magnetosphere", "description": "The ring current is a dynamic, doughnut-shaped region around Earth where charged particles flow in opposite directions along magnetic field lines, creating electrical currents. During a solar storm, changes in the ring current can lead to charge buildup on satellites, increased satellite drag, and magnetic fluctuations and induced currents on the ground that can affect pipelines and power lines.", "hits": 526 }, { "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": 364 }, { "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": 157 }, { "id": 14956, "url": "https://svs.gsfc.nasa.gov/14956/", "result_type": "Produced Video", "release_date": "2026-01-26T16:00:00-05:00", "title": "Space Weather Effects Animations", "description": "Solar flares, coronal mass ejections, solar particle events, and the solar wind form the recipe for space weather that affects life on Earth and astronauts in space. 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 it’s impacts on objects in the solar system. Learn more about space weather: https://science.nasa.gov/space-weather-2/ || ", "hits": 573 }, { "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": 212 }, { "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": 325 }, { "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": 443 }, { "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": 226 }, { "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": 465 }, { "id": 31354, "url": "https://svs.gsfc.nasa.gov/31354/", "result_type": "Animation", "release_date": "2025-06-13T16:19:00-04:00", "title": "PUNCH", "description": "NASA’s PUNCH Releases Its First Images of Huge Eruptions from Sun", "hits": 76 }, { "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": 28 }, { "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": 54 }, { "id": 5524, "url": "https://svs.gsfc.nasa.gov/5524/", "result_type": "Interactive", "release_date": "2025-05-22T08:00:59-04:00", "title": "\"Snap It!\" Solar Eclipse Photography Game", "description": "The Traveler needs your help! They have come to Earth to study an event we call a total solar eclipse. Can you help the Traveler snap photos of an eclipse?", "hits": 93 }, { "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": 21 }, { "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": 51 }, { "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": 128 }, { "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": 3003 }, { "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": 22 }, { "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": 36 }, { "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": 19 }, { "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": 31 }, { "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": 34 }, { "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": 21 }, { "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": 34 }, { "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": 28 }, { "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": 23 }, { "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": 25 }, { "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": 14 }, { "id": 5510, "url": "https://svs.gsfc.nasa.gov/5510/", "result_type": "Visualization", "release_date": "2025-02-25T17:10:00-05:00", "title": "Map of the March 29, 2025 Partial Solar Eclipse", "description": "On Saturday, March 29, 2025, the Moon passes in front of the Sun, casting its shadow across the Atlantic Ocean. Observers in Europe, western Africa, and eastern Canada are positioned to see a partial eclipse.", "hits": 389 }, { "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": 15 }, { "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": 31 }, { "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": 46 }, { "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": 75 }, { "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": 15 }, { "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": 26 }, { "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": 19 }, { "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": 39 }, { "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": 443 }, { "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": 18 }, { "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": 9 }, { "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": 27 }, { "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": 22 }, { "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": 30 }, { "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": 21 }, { "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": 15 }, { "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": 22 }, { "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": 28 }, { "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": 22 }, { "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": 16 }, { "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": 19 }, { "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": 86 }, { "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": 49 }, { "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": 396 }, { "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": 74 }, { "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": 20 }, { "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": 15 }, { "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": 27 }, { "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": 32 }, { "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": 41 }, { "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": 86 }, { "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": 21 }, { "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": 31 }, { "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": 32 }, { "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": 42 }, { "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": 11 }, { "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": 24 }, { "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": 16 }, { "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": 32 }, { "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": 12 }, { "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": 20 }, { "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": 140 }, { "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": 35 }, { "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": 46 }, { "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": 35 }, { "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": 18 }, { "id": 5378, "url": "https://svs.gsfc.nasa.gov/5378/", "result_type": "Visualization", "release_date": "2024-09-07T15:30:00-04:00", "title": "Map of the October 2, 2024 Annular Solar Eclipse", "description": "On Wednesday, October 2, 2024, the Moon passes in front of the Sun, casting its shadow across the Pacific Ocean. Observers on Rapa Nui (Easter Island) and in far southern Chile and Argentina are in the path of the annular eclipse. Hawai'i, parts of Antarctica, and the southern half of South America see a partial eclipse.", "hits": 191 }, { "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": 26 }, { "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": 24 }, { "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": 10 }, { "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": 25 }, { "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": 23 }, { "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": 14628, "url": "https://svs.gsfc.nasa.gov/14628/", "result_type": "Produced Video", "release_date": "2024-08-28T11:30:00-04:00", "title": "Discovering Earth’s Third Global Energy Field", "description": "High above the Earth’s North and South Poles, a steady stream of particles escapes from our atmosphere into space. Scientists call this mysterious outflow the “polar wind,” and for almost 60 years, spacecraft have been flying through it as scientists have theorized about its cause. The leading theory was that a planet-wide electric field was drawing those particles up into space. But this so-called ambipolar electric field, if it exists, is so weak that all attempts to measure it have failed – until now.In 2022, scientists traveled to Svalbard, a small archipelago in Norway, to launch a rocket in an attempt to measure Earth’s ambipolar electric field for the first time. This was NASA’s Endurance rocketship mission, and this is its story.To learn more, visit: https://science.nasa.gov/science-research/heliophysics/nasa-discovers-long-sought-global-electric-field-on-earth/ || ", "hits": 244 }, { "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": 20 }, { "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": 18 }, { "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": 26 }, { "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": 50 }, { "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": 35 }, { "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": 37 }, { "id": 5289, "url": "https://svs.gsfc.nasa.gov/5289/", "result_type": "Visualization", "release_date": "2024-07-09T00:00:00-04:00", "title": "An X5.8 flare 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.A hefty X5.8 flare erupts from Active Region 13664 on May 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": 49 }, { "id": 5291, "url": "https://svs.gsfc.nasa.gov/5291/", "result_type": "Visualization", "release_date": "2024-07-09T00:00:00-04:00", "title": "An X1.0 flare from Active Region 13664 - May 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.Another X-flare (X 1.0) flare erupts from Active Region 13664 near the lower right limb of the Sun. 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": 21 }, { "id": 5292, "url": "https://svs.gsfc.nasa.gov/5292/", "result_type": "Visualization", "release_date": "2024-07-09T00:00:00-04:00", "title": "An M6.6 flare from Active Region 13664 - May 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.An M6.6 flare fires with lots of action from the coronal loops from Active Region 13664 (lower right solar limb) on May 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": 27 }, { "id": 5284, "url": "https://svs.gsfc.nasa.gov/5284/", "result_type": "Visualization", "release_date": "2024-07-03T00:00:00-04:00", "title": "An X2.2 flare from Active Region 13664 - May 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 13664 (lower right quadrant of the solar disk) launches an X2.2 class solar flare on May 9, 2024. More details of this event can be found at 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": 26 }, { "id": 5285, "url": "https://svs.gsfc.nasa.gov/5285/", "result_type": "Visualization", "release_date": "2024-07-03T00:00:00-04:00", "title": "An X1.1 flare from Active Region 13664 - May 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 13664 (lower right quadrant of solar disk) again launches an X-flare (X1.1) and a stream of plasma. More details on the Space Weather database.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": 43 }, { "id": 5286, "url": "https://svs.gsfc.nasa.gov/5286/", "result_type": "Visualization", "release_date": "2024-07-03T00:00:00-04:00", "title": "An X3.9 flare from Active Region 13664 - May 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 13664 (lower right quadrant) continues its streak of bright flares launching a strong X-flare (X3.9) on May 10, 2024. More details at 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": 5287, "url": "https://svs.gsfc.nasa.gov/5287/", "result_type": "Visualization", "release_date": "2024-07-03T00:00:00-04:00", "title": "An M5.9 flare from Active Region 13664 - May 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 13664 (lower right quadrant) launches an M5.9 flare on May 10, 2024. More details at 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": 49 }, { "id": 5279, "url": "https://svs.gsfc.nasa.gov/5279/", "result_type": "Visualization", "release_date": "2024-07-02T00:00:00-04:00", "title": "Multiple large flares from Active Region 13663 - May 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.Near the close of May 4, 2024, Active region 13663 (upper right quadrant) launched a series of flares ranging from M7.4 to X1.3 over a period of about 12 hours.M9.0: 2024-05-04T23:48Z. Space Weather Database entryM8.4: 2024-05-05T01:27Z. Space Weather Database entryX1.3: 2024-05-05T06:01Z. Space Weather Database entryM7.4: 2024-05-05T10:00Z. Space Weather Database entryX1.2: 2024-05-05T11:54Z. Space Weather Database entryFor 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": 59 }, { "id": 5280, "url": "https://svs.gsfc.nasa.gov/5280/", "result_type": "Visualization", "release_date": "2024-07-02T00:00:00-04:00", "title": "An X4.5 flare from Active Region 13663 - May 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.Lots of coronal loop motion precedes the launch of an X4.5 flare from Active Region 13663 on May 6, 2024 (upper right quadrant). More details of this event can be found at 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": 37 } ] }