{ "count": 656, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=Corona", "previous": null, "results": [ { "id": 31381, "url": "https://svs.gsfc.nasa.gov/31381/", "result_type": "Hyperwall Visual", "release_date": "2026-03-31T11:51:59-04:00", "title": "NASA’S PUNCH Images Eruptions from the Sun", "description": "This video shows several coronal mass ejections (CMEs) erupting from the Sun’s surface from Oct. 21 to Nov. 12, 2025.", "hits": 651 }, { "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": 222 }, { "id": 40544, "url": "https://svs.gsfc.nasa.gov/gallery/hinode/", "result_type": "Gallery", "release_date": "2026-02-27T00:00:00-05:00", "title": "Hinode (Solar-B)", "description": "Hinode (Solar-B) is an international mission, led by the Japan Aerospace Exploration Agency (JAXA), to study the Sun. Hinode explores the magnetic fields of the Sun, from tracking their strength and direction on the solar surface, or photosphere, to decoding their role in heating and powering eruptions in the Sun’s outer atmosphere, or corona, to driving the constant outflow from the Sun, the solar wind. \n\nThe mission launched on Sept. 23, 2006, from Uchinoura Space Center in Japan aboard a JAXA M-V rocket.\n\nLearn more: https://science.nasa.gov/mission/hinode/", "hits": 61 }, { "id": 14973, "url": "https://svs.gsfc.nasa.gov/14973/", "result_type": "Produced Video", "release_date": "2026-02-17T10:00:00-05:00", "title": "Furious February Flares", "description": "In early February 2026, the Sun emitted more than 50 flares including several X-class events, which is the most intense category of solar flares. NASA’s Solar Dynamics Observatory watches the Sun 24/7 and captured these views of the Sun in multiple wavelengths of light.The Sun’s activity, which includes flares, follows an approximately 11-year cycle that creates periods of high and low activity. After reaching the current cycle’s most active phase in 2024 — known as solar maximum — the Sun remains in a heightened period of activity.For news of the recent flares: https://science.nasa.gov/blogs/solar-cycle-25/ || ", "hits": 238 }, { "id": 14964, "url": "https://svs.gsfc.nasa.gov/14964/", "result_type": "Produced Video", "release_date": "2026-02-05T13:00:00-05:00", "title": "Early February Flares 2026", "description": "So far, the Sun has emitted six X-class solar flares in the first four days of February. X-class flares are the most powerful. In this composite image, we've layered all six X-class flares onto the Sun at once, to show the active areas. The images come from the Solar Dynamics Observatory (SDO), which observes the Sun in different wavelengths, using filters that emphasize different characteristics. Flare #6, for example, shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares, which is colored in red and blue. The Sun’s magnetic field goes through a cycle, called the solar cycle, about every 11 years, with periods of more and less activity. The Sun reached its most active phase – solar maximum – in 2024, which means we’re still in a fairly active period of the cycle.For news of the recent flares: https://science.nasa.gov/blogs/solar-cycle-25/Image DescriptionComposite image of 6 X-class solar flares emitted in February. In the center, the Sun is a dark red globe with mottled darker and glowing orange spots. Just above the equator and to the left of center longitudinally, 2 bright white glowing spots are made of the combined 6 X-class flares emitted so far. Six squares pop out from the center Sun, with lines connecting to the spot on the composite Sun their flare is contributing. Along the top, the squares are labeled 2, 4 and 6. Each has a subset of the Sun seen in a different colored wavelength. Box 2 is a purple Sun with a pinkish flare, from Feb. 2, 2026. Box 4 is a golden Sun with a white flare from Feb. 2, 2026. Box 6 is a pink Sun with an orange flare from Feb. 4, 2026. Along the bottom, the boxes are labeled 1, 3 and 5. Box 1 has a turquoise Sun with a teal flare from Feb. 1, 2026. Box 3 has a yellow Sun with an orange flare from Feb. 2, 2026. Box 5 has a red Sun the same color as the center, with a white flare, from Feb. 3, 2026. || February_2026_X_Flares_SIX_FINAL.jpg (7000x7000) [5.3 MB] || ", "hits": 986 }, { "id": 5609, "url": "https://svs.gsfc.nasa.gov/5609/", "result_type": "Visualization", "release_date": "2026-01-26T05:00:00-05:00", "title": "Heliophysics Satellite Fleet - 2026", "description": "A tour of the NASA Heliophysics fleet from near-Earth satellites out to the Voyagers beyond the heliopause.", "hits": 861 }, { "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": 361 }, { "id": 14922, "url": "https://svs.gsfc.nasa.gov/14922/", "result_type": "Produced Video", "release_date": "2025-12-01T14:00:00-05:00", "title": "Anatomy of an Active Galactic Nucleus", "description": "An active galactic nucleus, or AGN, is a supermassive black hole at the center of a galaxy that is consuming surrounding matter. Although the black hole itself is not visible, the structures around it emit light across many wavelengths. The artist’s concepts here highlight distinct structures that can accompany an AGN — the photon ring, accretion disk, corona, dusty torus, and relativistic jets. || ", "hits": 1003 }, { "id": 14905, "url": "https://svs.gsfc.nasa.gov/14905/", "result_type": "Produced Video", "release_date": "2025-11-28T09:00:00-05:00", "title": "Black Hole Environments, Explained", "description": "If light can’t escape black holes, how do we know where they are? The regions around them tell an incredible story. From blazing coronas and swirling accretion disks to powerful jets that stretch millions of miles, these extreme environments reveal black holes' secrets and how these mysterious objects shape the universe.Join host Sophia Roberts as she talks with researchers Jenna Cann and Cecilia Chirenti at NASA Goddard about how scientists study these mysterious structures, the challenges of observing the unseeable, and the discoveries that continue to change our understanding of black holes.Credit: NASA’s Goddard Space Flight CenterMusic credits from Universal Production Music:\"Breaking the Barrier,\" David Bertrand Holland\"Dust Spirals,\" Alexandre Prodhomme\"Miniature Universe,\" Geoffrey Wilkinson\"Urban Decay,\" Sarah Natasha Penelope Warne\"Solar Plexus,\" Brandon Seliga\"Polygraph,\" Eric Chevalier\"The Mischief Makers,\" Joaquim Badia\"Maelstrom Dream,\" Lucie Rose\"The Truth Will Out,\" Chris Dony and Beth Perry || 14905_-_BHE_Thumbnail.jpg (1280x720) [947.8 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.srt [15.7 KB] || 14905_-_Black_Hole_Environments_Explained_Captions.en_US.vtt [14.8 KB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_1080.mp4 (1920x1080) [1.7 GB] || FINAL_-_14905_Black_Hole_Enviroments_Explained_4k.mp4 (3840x2160) [9.2 GB] || FINAL_-_14905_-_Black_Hole_Environments_Explained_ProRes.mov (3840x2160) [39.3 GB] || ", "hits": 207 }, { "id": 5577, "url": "https://svs.gsfc.nasa.gov/5577/", "result_type": "Animation", "release_date": "2025-11-20T09:00:00-05:00", "title": "SDO Sun This Week", "description": "This visualization shows SDO AIA-304 imagery from the past 7 days with a color table and image processing applied. Archive folders are provided in the Download menu.", "hits": 0 }, { "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": 279 }, { "id": 14920, "url": "https://svs.gsfc.nasa.gov/14920/", "result_type": "Produced Video", "release_date": "2025-11-13T12:00:00-05:00", "title": "Preparing for Martian Explorers: NASA's ESCAPADE Investigates Mars Space Weather", "description": "NASA’s new ESCAPADE mission is launching to Mars to help us better understand the Sun’s influence on Mars’ past and present. Its work could help protect future human explorers from potentially dangerous space weather when they set foot on the Red Planet.For the first time, the mission will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. Its observations will reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE orbiters build on earlier Mars missions, such as NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) orbiter. The MAVEN mission has one spacecraft that has been studying Mars’ atmospheric loss since arriving at the Red Planet in 2014.ESCAPADE is scheduled to launch no earlier than fall 2025 from Cape Canaveral Space Force Station Launch Complex 36 in Florida.Find out more about the ESCAPADE mission: https://science.nasa.gov/mission/escapade/ || ", "hits": 159 }, { "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": 250 }, { "id": 14885, "url": "https://svs.gsfc.nasa.gov/14885/", "result_type": "Produced Video", "release_date": "2025-09-12T06:00:00-04:00", "title": "NASA Interview Opportunity: Groundbreaking New NASA Mission Will Give Us The Most Detailed Look Yet At Our Solar System’s Shield", "description": "Scroll down page for associated cut b-roll and pre-recorded soundbites. || IMAP_banner.jpeg (1600x640) [185.0 KB] || IMAP_banner_print.jpg (1024x409) [110.6 KB] || IMAP_banner_searchweb.png (320x180) [73.1 KB] || IMAP_banner_thm.png (80x40) [6.7 KB] || ", "hits": 114 }, { "id": 14892, "url": "https://svs.gsfc.nasa.gov/14892/", "result_type": "Produced Video", "release_date": "2025-08-29T16:00:00-04:00", "title": "Solar Wind Animations", "description": "The Sun releases a constant stream of charged particles, called the solar wind. The solar wind originates in the outermost layer of the Sun’s atmosphere, the corona, when plasma is heated to a point that the Sun’s gravity can’t hold it down. When this plasma escapes – often reaching speeds of over one million miles per hour – it drags the Sun’s magnetic out across the solar system. When the solar wind encounters Earth, it is deflected by our planet's magnetic shield, causing most of the solar wind's energetic particles to flow around and beyond us. However, some of these high-energy particles can sneak past Earth’s natural magnetic defenses and produce hazardous conditions for satellites and astronauts, as well as power grids and infrastructure on Earth.Learn more about the solar wind: https://science.nasa.gov/sun/what-is-the-solar-wind/ || ", "hits": 920 }, { "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": 433 }, { "id": 14863, "url": "https://svs.gsfc.nasa.gov/14863/", "result_type": "Produced Video", "release_date": "2025-07-17T09:00:00-04:00", "title": "Quickshot: New NASA Mission Launching Soon To Study Earth’s Space Weather Shield", "description": "Scroll down page for advisory with suggested questions and anchor intro. You will also find the associated cut b-roll and pre-recorded soundbites below.Click here for more information about TRACERS || Live_Shot_Banner_TRACERS_final.jpg (1800x720) [256.8 KB] || Live_Shot_Banner_TRACERS_final_print.jpg (1024x409) [150.1 KB] || Live_Shot_Banner_TRACERS_final_searchweb.png (320x180) [82.8 KB] || Live_Shot_Banner_TRACERS_final_thm.png (80x40) [6.5 KB] || ", "hits": 124 }, { "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": 38 }, { "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": 36 }, { "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": 46 }, { "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": 57 }, { "id": 14865, "url": "https://svs.gsfc.nasa.gov/14865/", "result_type": "Produced Video", "release_date": "2025-07-10T14:00:00-04:00", "title": "The Closest Images Ever Taken of the Sun’s Atmosphere", "description": "On its record-breaking pass by the Sun in December 2024, NASA’s Parker Solar Probe captured stunning new images from within the Sun’s atmosphere. These newly released images — taken closer to the Sun than we’ve ever been before — are helping scientists better understand the Sun’s influence across the solar system, including events that can affect Earth.Parker Solar Probe started its closest approach to the Sun on Dec. 24, 2024, flying just 3.8 million miles from the solar surface. As it skimmed through the Sun’s outer atmosphere, called the corona, in the days around the perihelion, it collected data with an array of scientific instruments, including the Wide-Field Imager for Solar Probe, or WISPR.Learn more - https://science.nasa.gov/science-research/heliophysics/nasas-parker-solar-probe-snaps-closest-ever-images-to-sun/Find the latest WISPR imagery here. || ", "hits": 480 }, { "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": 34 }, { "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": 29 }, { "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": 57 }, { "id": 5534, "url": "https://svs.gsfc.nasa.gov/5534/", "result_type": "Visualization", "release_date": "2025-06-18T11:23:00-04:00", "title": "Parker Solar Probe - Extended Mission", "description": "After it's ultimate perihelion in December 2024, the Parker Solar Probe will continue it's orbits around the Sun. This visualization presents a projection of it's current orbit through 2029.", "hits": 935 }, { "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": 173 }, { "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": 65 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 514 }, { "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": 78 }, { "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": 17 }, { "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": 41 }, { "id": 14803, "url": "https://svs.gsfc.nasa.gov/14803/", "result_type": "Produced Video", "release_date": "2025-03-17T09:00:00-04:00", "title": "NASA’s SPHEREX and PUNCH Missions Launch from Vandenberg Space Force Base", "description": "Ignition, and liftoff! At 11:10 p.m. EDT (8:10 p.m. PDT) March 11, 2025, SpaceX’s Falcon 9 rocket blasted off from Vandenberg Space Force Base’s Space Launch Complex 4 East, carrying NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) and PUNCH (Polarimeter to Unify the Corona and Heliosphere) missions.SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) will orbit Earth for a two-year prime mission and create a three-dimensional map of the cosmos. This will help scientists answer major questions about what happened in the first second after the big bang, how galaxies form and evolve, and the origins and abundance of water and other key ingredients for life in our galaxy.Ride-sharing with SPHEREx was NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, which will study the outer portion of the Sun, the corona, to understand how solar wind forms.For more information on SPHEREx: nasa.gov/spherexFor more information on PUNCH: science.nasa.gov/mission/punch || ", "hits": 170 }, { "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": 24 }, { "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": 25 }, { "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": 23 }, { "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": 5 }, { "id": 5489, "url": "https://svs.gsfc.nasa.gov/5489/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X1.1 flare from Active Region 13936 - December 29, 2024", "description": "Active region 13936 (upper right quadrant) launches an X1.1 flare.", "hits": 10 }, { "id": 5484, "url": "https://svs.gsfc.nasa.gov/5484/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.4 flare from Active Region 13922 - December 10, 2024", "description": "Active region 13922 launches an M6.4 flare near the left limb of the Sun on December 10, 2024.", "hits": 29 }, { "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": 14 }, { "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": 19 }, { "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": 379 }, { "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": 11 }, { "id": 5496, "url": "https://svs.gsfc.nasa.gov/5496/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.7 flare from Active Region 13978 - January 31, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13978 launch an M6.7 flare on January 31, 2025.", "hits": 15 }, { "id": 5497, "url": "https://svs.gsfc.nasa.gov/5497/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M5.1 flare from Active Region 13977 - February 2, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13977 (in the upper center of the disk) launch an M5.1 flare and a filament of material on February 2, 2025.", "hits": 31 }, { "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": 29 }, { "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": 14 }, { "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": 21 }, { "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": 17 }, { "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": 15 }, { "id": 14784, "url": "https://svs.gsfc.nasa.gov/14784/", "result_type": "Produced Video", "release_date": "2025-02-13T14:00:00-05:00", "title": "PUNCH Mission Media Teleconference", "description": "NASA held a media teleconference at 2 p.m. EST on Tuesday, February 4, to share information about the agency’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, which is targeted to launch no earlier than Thursday, February 27, 2025.The agency’s PUNCH mission is a constellation of four small satellites. When they arrive in low Earth orbit, the satellites will make global, 3D observations of the Sun’s outer atmosphere, the corona, and help NASA learn how the mass and energy there become solar wind. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission will share a ride to space with NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) space telescope on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.The Southwest Research Institute in Boulder, Colorado, leads the PUNCH mission. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington.To learn more about PUNCH, please visit: nasa.gov/punch || ", "hits": 113 }, { "id": 14783, "url": "https://svs.gsfc.nasa.gov/14783/", "result_type": "Produced Video", "release_date": "2025-02-13T12:00:00-05:00", "title": "NASA Interview Opportunity: Two Missions, One Rocket: One Shared Goal", "description": "Assocated cut b-roll will be posted by 5 p.m. EST on Monday, Feb 24. || SPHEREx_PUNCH_Live_Shots_Banner.jpg (1800x720) [495.3 KB] || SPHEREx_PUNCH_Live_Shots_Banner_print.jpg (1024x409) [260.6 KB] || SPHEREx_PUNCH_Live_Shots_Banner_searchweb.png (320x180) [111.2 KB] || SPHEREx_PUNCH_Live_Shots_Banner_thm.png [8.0 KB] || ", "hits": 83 }, { "id": 14779, "url": "https://svs.gsfc.nasa.gov/14779/", "result_type": "Produced Video", "release_date": "2025-02-11T09:00:00-05:00", "title": "NASA's Illuminate Series (2025)", "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ", "hits": 226 }, { "id": 14773, "url": "https://svs.gsfc.nasa.gov/14773/", "result_type": "Produced Video", "release_date": "2025-02-04T10:00:00-05:00", "title": "NASA's PUNCH Mission", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun’s corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.Watch the video to learn how imaging the Sun’s corona and the solar wind together will help scientists better understand the entire inner heliosphere — Sun, solar wind, and Earth — as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate.For more information visit science.nasa.gov/mission/punch || ", "hits": 126 }, { "id": 14776, "url": "https://svs.gsfc.nasa.gov/14776/", "result_type": "Produced Video", "release_date": "2025-01-30T14:00:00-05:00", "title": "PUNCH Satellites Integration and Testing", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 95 }, { "id": 14771, "url": "https://svs.gsfc.nasa.gov/14771/", "result_type": "Produced Video", "release_date": "2025-01-24T14:00:00-05:00", "title": "PUNCH Instruments", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system. By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.Three of the PUNCH satellites will carry a Wide Field Imager (WFI), and the fourth will carry the Narrow Field Imager (NFI).The Narrow Field Imager (NFI)The Narrow Field Image (NFI) is a coronagraph, a type of device that blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. The coronagraph will have a similar field of view as the SOHO (Solar and Heliospheric Observatory) Large Angle and Spectrometric Coronagraph (LASCO) C3 field, from 6 to 32 solar radii on the sky, and it will view the corona in both polarized and unpolarized light.Wide Field Imager (WFI)The Wide Field Imager (WFI) is a heliospheric imager, a device that provides views from 18 to 180 solar radii (45 degrees) away from the Sun in the sky. Heliospheric imagers use an artificial “horizon” and deep baffles to view the very faint outermost portion of the solar corona and the solar wind itself. The instrument reduces direct sunlight by over 16 orders of magnitude, which is like the ratio between the mass of a human and the mass of a cold virus. The wide-field imaging optics are based on the design of the famous Nagler eyepieces, which are known among observational astronomers for their clarity, low distortion, wide field, and achromatic focus. Three of the PUNCH spacecraft will carry a WFI instrument. || ", "hits": 134 }, { "id": 14770, "url": "https://svs.gsfc.nasa.gov/14770/", "result_type": "Produced Video", "release_date": "2025-01-24T09:00:00-05:00", "title": "PUNCH Satellites Test Operations at Vandenberg Space Force Base", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 58 }, { "id": 14768, "url": "https://svs.gsfc.nasa.gov/14768/", "result_type": "Produced Video", "release_date": "2025-01-23T17:00:00-05:00", "title": "PUNCH Satellites Solar Array Deployment Test", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 112 }, { "id": 14767, "url": "https://svs.gsfc.nasa.gov/14767/", "result_type": "Produced Video", "release_date": "2025-01-23T16:00:00-05:00", "title": "PUNCH Satellites Arrival at Vandenberg Space Force Base", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 79 }, { "id": 14765, "url": "https://svs.gsfc.nasa.gov/14765/", "result_type": "Produced Video", "release_date": "2025-01-23T15:00:00-05:00", "title": "PUNCH Assembly and Testing", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.By imaging the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere – Sun, solar wind, and Earth – as a single connected system.The PUNCH mission is led by Southwest Research Institute’s office in Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate. || ", "hits": 107 }, { "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": 294 }, { "id": 14753, "url": "https://svs.gsfc.nasa.gov/14753/", "result_type": "Produced Video", "release_date": "2025-01-13T10:14:00-05:00", "title": "Astronomers Track Jet Launch, Fluctuating X-Rays from Brink of Active Black Hole", "description": "Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away.Credit: Pan-STARRSUnannotated versions available.Image description: On a mottled black background, soft circles ranging in color from blue-white to orange represent stars in our own galaxy. At center, to the right of a chain of three bluish stars, lies a softer white circle set within a grayish ellipse whose longest dimension is oriented vertically. This is 1ES 1927+654, circled in green in this image. || 1ES1927_PanSTARRS_1080_circ.jpg (1920x1080) [597.2 KB] || 1ES1927_PanSTARRS_1080.jpg (1920x1080) [591.5 KB] || 1ES1927_PanSTARRS_2160.jpg (3840x2160) [1.7 MB] || 1ES1927_PanSTARRS_1080_circ_searchweb.png (320x180) [87.7 KB] || 1ES1927_PanSTARRS_1080_circ_thm.png [8.9 KB] || ", "hits": 197 }, { "id": 14739, "url": "https://svs.gsfc.nasa.gov/14739/", "result_type": "Produced Video", "release_date": "2025-01-03T12:00:00-05:00", "title": "From the Moon, NASA’s LEXI Will Reveal Earth’s Magnetic Shield", "description": "NASA’s next mission to the Moon will carry an instrument called LEXI (the Lunar Environment Heliospheric X-ray Imager), which will provide the first-ever global view of the magnetic environment that shields Earth from solar radiation.From the surface of the Moon, LEXI will capture wide-field images of Earth's magnetic environment, or magnetosphere, in low-energy (or \"soft\") X-rays. LEXI will study changes in the magnetosphere and help us learn more about how it interacts with a stream of particles from the Sun called the solar wind, which can pose hazards for Artemis astronauts traveling to the Moon.Learn more about LEXI and its CLPS (Commercial Lunar Payload Services) flight to the Moon from Hyunju Connor, LEXI co-investigator at NASA’s Goddard Space Flight Center.More on LEXI: https://science.nasa.gov/science-research/heliophysics/nasas-lexi-will-provide-x-ray-vision-of-earths-magnetosphere/ || ", "hits": 180 }, { "id": 14744, "url": "https://svs.gsfc.nasa.gov/14744/", "result_type": "Produced Video", "release_date": "2025-01-03T00:00:00-05:00", "title": "GDC and DYNAMIC to Explore Earth’s Upper Atmosphere", "description": "Two upcoming missions, the Geospace Dynamics Constellation (GDC) and Dynamical Neutral Atmosphere-Ionosphere Coupling (DYNAMIC) will revolutionize our understanding of Earth’s upper atmosphere. This region includes Earth’s ionosphere, thermosphere, and mesosphere, and stretches from roughly 50 to 400 miles above Earth’s surface. Space weather disturbances can impact communications, navigation signals, and satellite orbits, and induce currents can trigger power outages on Earth — making the region a crucial area of study.GDC is a team of satellites that will study Earth’s upper atmosphere and provide the first direct global measurements of our planet’s dynamic and complex interface with the space environment. Working in tandem with the DYNAMIC spacecraft, scientists will be able paint a fuller picture of how energy transforms and travels throughout the upper atmosphere. GDC will fly at an altitude of 350-400 km.DYNAMIC is a pair of satellites that will work in tandem with GDC to study how changes in Earth’s lower atmosphere influence our planet’s upper atmosphere. Between the multiple spacecraft of GDC and DYNAMIC, simultaneous observations from different locations can give scientists a more complete picture of how atmospheric waves propagate up through this unique part of the atmosphere. DYNAMIC will fly at an altitude of 550-800 km. || ", "hits": 192 }, { "id": 14722, "url": "https://svs.gsfc.nasa.gov/14722/", "result_type": "Produced Video", "release_date": "2024-12-06T15:00:00-05:00", "title": "NASA Interview Opportunity: NASA Spacecraft Days Away From Historic Close Approach to the Sun", "description": "Scroll down the page for associated cut b-roll for the live shots and pre-recorded soundbites.Find out more about NASA's Parker Solar Probe here! nasa.gov/parker || Screenshot_2024-12-06_at_2.24.02 PM.png (1546x606) [1.9 MB] || Screenshot_2024-12-06_at_2.24.02 PM_print.jpg (1024x401) [195.3 KB] || Screenshot_2024-12-06_at_2.24.02 PM_searchweb.png (320x180) [128.7 KB] || Screenshot_2024-12-06_at_2.24.02 PM_thm.png (80x40) [12.2 KB] || ", "hits": 148 }, { "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": 13 }, { "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": 10 }, { "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": 20 }, { "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": 15 }, { "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": 16 }, { "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": 9 }, { "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": 7 }, { "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": 17 }, { "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": 21 }, { "id": 5428, "url": "https://svs.gsfc.nasa.gov/5428/", "result_type": "Visualization", "release_date": "2024-11-25T00:00:00-05:00", "title": "Parker Solar Probe Towards its Ultimate Perihelion", "description": "Parker Solar Probe is making its final planned orbits around the Sun.On Wednesday, November 6, 2024, NASA's Parker Solar Probe completed it's final Venus gravity assist maneuver, passing within 233 miles (376 kilometers) of Venus' surface. The flyby adjusted Parker's trajectory into its final orbital configuration, bringing the spacecraft to within an unprecedented 3.86 million miles from the solar surface on December 24, 2024. It will be the closest any human-made object has been to the Sun. || ", "hits": 512 }, { "id": 20392, "url": "https://svs.gsfc.nasa.gov/20392/", "result_type": "Animation", "release_date": "2024-11-12T14:00:00-05:00", "title": "Space Weather and NOAA's Space Weather Follow On at Lagrange point 1 (SWFO-L1)", "description": "NOAA and Impacts of Space Weather || SWFO_0924_2MinVer_HD_v02.01800_print.jpg (1024x576) [187.1 KB] || SWFO_0924_2MinVer_HD_v02.01800_searchweb.png (180x320) [89.8 KB] || SWFO_0924_2MinVer_HD_v02.01800_thm.png (80x40) [6.3 KB] || SWFO_0924_2MinVer_FHD_v02.mp4 (1920x1080) [159.2 MB] || SWFO_0924_2MinVer_HD_v02.mp4 (1280x720) [157.5 MB] || SWFO_0924_2MinVer_SD_v02.mp4 (852x480) [156.8 MB] || SWFO_0924_2MinVer_4k_v02.mp4 (3840x2160) [231.9 MB] || SWFO_0924_2MinVer_4k_v02.mov (3840x2160) [15.8 GB] || ", "hits": 130 }, { "id": 14714, "url": "https://svs.gsfc.nasa.gov/14714/", "result_type": "B-Roll", "release_date": "2024-11-06T10:00:00-05:00", "title": "CODEX Heads to the Space Station for Install", "description": "On Nov. 4, 2024, the Coronal Diagnostic Experiment (CODEX) launched to space aboard NASA’s SpaceX CRS-31 – a commercial resupply mission of an uncrewed Dragon spacecraft headed for the International Space Station. Liftoff occurred at 9:29 p.m. EST.CODEX is a solar coronagraph that will be installed on the Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun’s outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contributions from Italy’s National Institute for Astrophysics (INAF).To learn more about the experiment, visit: https://science.nasa.gov/mission/codex/ || ", "hits": 96 }, { "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": 40 }, { "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": 53 }, { "id": 14709, "url": "https://svs.gsfc.nasa.gov/14709/", "result_type": "Produced Video", "release_date": "2024-10-28T15:00:00-04:00", "title": "Sun Releases Strong Solar Flare on October 23, 2024", "description": "NASA’s Solar Dynamics Observatory captured this image of an X3.3 solar flare – as seen in the bright flash and loop on the left – on Oct. 23, 2024. The image shows a blend of 171 Angstrom, 304 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light. Credit: NASA/SDO || SDO_X3pt3_10-23-2024_0340_131-304-171.jpg (4096x4096) [4.7 MB] || SDO_X3pt3_10-23-2024_0340_131-304-171_searchweb.png (320x180) [104.1 KB] || SDO_X3pt3_10-23-2024_0340_131-304-171_thm.png (80x40) [7.2 KB] || ", "hits": 68 }, { "id": 14710, "url": "https://svs.gsfc.nasa.gov/14710/", "result_type": "Produced Video", "release_date": "2024-10-28T15:00:00-04:00", "title": "Sun Erupts with X-class flare on October 26, 2024", "description": "A sequence of October 26th's X1.8-class solar flare viewed in three different wavelengths of extreme ultraviolet light captured by NASA’ Solar Dynamics Observatory.AIA 171 (colorized here in gold) shows solar material at just over 1 million degrees Fahrenheit. AIA 131 (colorized here in teal) shows solar material at up to a blistering 18 million degrees Fahrenheit, AIA 304 (colorized here in red) shows material at around 100,000 degrees Fahrenheit.Credit:NASA/SDO || Oct_26_X1pt8_Flare_multi_big.jpg (5120x3072) [3.4 MB] || Oct_26_X1pt8_Flare_multi_big_searchweb.png (320x180) [95.8 KB] || Oct_26_X1pt8_Flare_multi_big_thm.png (80x40) [7.6 KB] || ", "hits": 88 }, { "id": 14704, "url": "https://svs.gsfc.nasa.gov/14704/", "result_type": "Produced Video", "release_date": "2024-10-23T06:00:00-04:00", "title": "NASA Interview Opportunity: Star light, star bright, check out the evening sky on your Halloween walk tonight", "description": "Scroll down the page to find b-roll for the live shots + a pre-recorded interview with Rebekah HounsellFor more information check out: @NASAUniverse on social media platforms and universe.nasa.gov online || T_CrB_banner_-_ENGLISH.png (1800x720) [1.8 MB] || T_CrB_banner_-_ENGLISH_print.jpg (1024x409) [109.8 KB] || T_CrB_banner_-_ENGLISH_searchweb.png (320x180) [80.0 KB] || T_CrB_banner_-_ENGLISH_thm.png (80x40) [7.0 KB] || ", "hits": 85 }, { "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": 83 }, { "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": 43 }, { "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": 26 }, { "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": 25 }, { "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": 23 }, { "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": 24 }, { "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": 35 }, { "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": 97 }, { "id": 14701, "url": "https://svs.gsfc.nasa.gov/14701/", "result_type": "Produced Video", "release_date": "2024-10-03T09:00:00-04:00", "title": "Sun Emits X9.0 Flare on October 3, 2024", "description": "Several video views of October 3rd's X9-class solar flare, the most powerful of this solar cycle, featuring two different wavelengths of extreme ultraviolet light captured by NASA’ Solar Dynamics Observatory. AIA 171 (colorized here in gold) shows solar material at just over 1 million degrees Fahrenheit. AIA 131 (colorized here in red) shows solar material at up to a blistering 18 million degrees Fahrenheit.Credit:NASA/SDO || X9_Flare_video_still.jpg (1920x1080) [416.4 KB] || 14701SDOX9FlareCaptions.en_US.srt [172 bytes] || 14701SDOX9FlareCaptions.en_US.vtt [174 bytes] || 14701_SDO_October032024_X9_Flare.mp4 (1920x1080) [124.7 MB] || 14701_SDO_October032024_X9_Flare_ProRes_1920x1080.mov (1920x1080) [881.1 MB] || ", "hits": 203 }, { "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": 35 }, { "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": 20 }, { "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": 30 } ] }