{ "count": 788, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Cycle%22", "previous": null, "results": [ { "id": 14992, "url": "https://svs.gsfc.nasa.gov/14992/", "result_type": "Animation", "release_date": "2026-03-24T15:00:00-04:00", "title": "Lunar Near and Far Side Phases", "description": "These animations illustrate opposite lunar phases on the near and far sides of the Moon.", "hits": 6579 }, { "id": 40548, "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/", "result_type": "Gallery", "release_date": "2026-03-03T00:00:00-05:00", "title": "SOHO – Solar and Heliospheric Observatory", "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/", "hits": 500 }, { "id": 40549, "url": "https://svs.gsfc.nasa.gov/gallery/interstellar-boundary-explorer-ibex/", "result_type": "Gallery", "release_date": "2026-03-02T00:00:00-05:00", "title": "IBEX – Interstellar Boundary Explorer", "description": "The Interstellar Boundary Explorer (IBEX) is a NASA spacecraft studying how our heliosphere — the protective bubble surrounding the Sun and planets that is inflated by a constant stream of solar particles — interacts with interstellar space. IBEX created the first maps showing the interactions at that border, and how they change over time due to variations in the Sun’s activity. IBEX studies the heliosphere’s boundaries by measuring a type of uncharged particle called energetic neutral atoms.\n\nIBEX launched on Oct. 19, 2008, from the Ronald Reagan Ballistic Missile Defense Test Site, in the Republic of the Marshall Islands. \n\nLearn more: https://science.nasa.gov/mission/ibex/", "hits": 225 }, { "id": 31365, "url": "https://svs.gsfc.nasa.gov/31365/", "result_type": "Visualization", "release_date": "2026-03-01T18:59:59-05:00", "title": "The Earth System Science Spheres", "description": "A rotating sphere shows data from recent satellites representing four of the five science spheres: Atmosphere, Biosphere, Geosphere, and Hydrosphere.", "hits": 1372 }, { "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": 373 }, { "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": 779 }, { "id": 5587, "url": "https://svs.gsfc.nasa.gov/5587/", "result_type": "Visualization", "release_date": "2025-12-11T12:00:00-05:00", "title": "Moon Phase and Libration, 2026", "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.", "hits": 7694 }, { "id": 5588, "url": "https://svs.gsfc.nasa.gov/5588/", "result_type": "Visualization", "release_date": "2025-12-11T12:00:00-05:00", "title": "Moon Phase and Libration, 2026 South Up", "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.", "hits": 796 }, { "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": 14898, "url": "https://svs.gsfc.nasa.gov/14898/", "result_type": "Produced Video", "release_date": "2025-09-15T15:00:00-04:00", "title": "Our Home In Space Series", "description": "The heliosphere, the massive bubble created by our Sun, is like our “house” in space. It shelters us from harsh weather outside and regulates the environment inside. Without our heliosphere, Earth may never have developed life at all. But there’s a lot we still don’t know about our cosmic home. How big is it, and what is it shaped like? How does it compare to the “houses” created by other stars? A new NASA mission will soon unlock answers to these questions and more. Launching as early as Sept. 23, NASA’s Interstellar Mapping and Acceleration Probe will help us construct the “blueprints” or our home in space. This three-part series explores how we learn about our heliosphere, how it protects us, and how it advances the search for life elsewhere in the Universe. || ", "hits": 154 }, { "id": 14883, "url": "https://svs.gsfc.nasa.gov/14883/", "result_type": "Produced Video", "release_date": "2025-08-25T11:00:00-04:00", "title": "Mapping Stellar ‘Polka Dots’", "description": "Watch to learn how a new tool uses data from exoplanets, worlds beyond our solar system, to tell us about their polka-dotted stars.Credit: NASA’s Goddard Space Flight CenterMusic: “Whimsical Whirlwinds,” Claire Leona Batchelor [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Get the vertical version of this video [here](https://svs.gsfc.nasa.gov/14797/){target=_blank}. || PolkaDotStars_Thumbnail.jpg (1920x1080) [145.7 KB] || PolkaDotStars_Thumbnail_print.jpg (1024x576) [59.8 KB] || PolkaDotStars_Thumbnail_searchweb.png (320x180) [33.1 KB] || PolkaDotStars_Thumbnail_thm.png (80x40) [3.1 KB] || 14883_MappingStellarPolkaDots_Low.mp4 (1920x1080) [74.2 MB] || 14883_MappingStellarPolkaDots.mp4 (1920x1080) [262.9 MB] || MappingStellarPolkaDotsCaptions.en_US.srt [1.4 KB] || 14883_MappingStellarPolkaDots_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 125 }, { "id": 20409, "url": "https://svs.gsfc.nasa.gov/20409/", "result_type": "Animation", "release_date": "2025-08-22T09:00:00-04:00", "title": "The Heliosphere and Galactic Cosmic Rays", "description": "Surrounding our solar system is a giant protective bubble created by particles and magnetic fields from the Sun called the heliosphere. Every 11 years, the Sun’s activity ramps up and down in what’s known as the solar cycle. As the Sun reaches its peak activity level, called solar maximum, the heliosphere expands. During this time, the heliosphere’s protective shield is strengthened by the increase in particles and magnetic fields from the Sun. As a result, fewer damaging particles from the galaxy, such as galactic cosmic rays, are able to penetrate into the heliosphere. As the Sun ramps down into a low level of activity, called solar minimum, the heliosphere shrinks and more cosmic rays are able to enter the heliosphere. || ", "hits": 446 }, { "id": 40543, "url": "https://svs.gsfc.nasa.gov/gallery/imap/", "result_type": "Gallery", "release_date": "2025-08-20T00:00:00-04:00", "title": "IMAP – Interstellar Mapping and Acceleration Probe", "description": "NASA's Interstellar Mapping and Acceleration Probe (IMAP) maps the boundaries of the heliosphere — the protective bubble surrounding the Sun and planets that is inflated by the constant stream of particles from the Sun called the solar wind. As a modern-day celestial cartographer, IMAP also explores and charts the vast range of particles in interplanetary space, helping to investigate important issues in heliophysics, the field studying the Sun and its sphere of influence. IMAP provides near-real-time information about the solar wind to provide advanced space weather warnings from its location at Lagrange point 1, one million miles from Earth toward the Sun.\n\nThe mission launched on Sept. 24, 2025, from NASA’s Kennedy Space Center in Florida.\n\nLearn more: https://science.nasa.gov/mission/imap/", "hits": 397 }, { "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": 78 }, { "id": 5560, "url": "https://svs.gsfc.nasa.gov/5560/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "M8.4 flare from Active Region 14114 - June 15, 2025", "description": "M8.4 flare from Active Region 14114 - June 15, 2025", "hits": 27 }, { "id": 5561, "url": "https://svs.gsfc.nasa.gov/5561/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "M6.3 flare from Active Region 14114 - June 16, 2025", "description": "M6.3 flare from Active Region 14114 - June 16, 2025", "hits": 32 }, { "id": 5562, "url": "https://svs.gsfc.nasa.gov/5562/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "X1.2 flare from Active Region 14114 - June 17, 2025", "description": "X1.2 flare from Active Region 14114 - June 17, 2025", "hits": 30 }, { "id": 5564, "url": "https://svs.gsfc.nasa.gov/5564/", "result_type": "Visualization", "release_date": "2025-07-14T10:00:00-04:00", "title": "An X1.9 flare from AR 14114 - June 19, 2025", "description": "An X1.9 flare from AR 14114 on June 19, 2025.", "hits": 48 }, { "id": 5559, "url": "https://svs.gsfc.nasa.gov/5559/", "result_type": "Visualization", "release_date": "2025-07-10T10:00:00-04:00", "title": "M6.8 flare from Active Region 14105 - June 14, 2025", "description": "M6.8 flare from Active Region 14105 - June 14, 2025", "hits": 31 }, { "id": 5550, "url": "https://svs.gsfc.nasa.gov/5550/", "result_type": "Visualization", "release_date": "2025-07-09T10:00:00-04:00", "title": "M8.9 flare from Active Region 14098 - May 25, 2025", "description": "M8.9 flare from Active Region 14098 - May 25, 2025", "hits": 24 }, { "id": 5551, "url": "https://svs.gsfc.nasa.gov/5551/", "result_type": "Visualization", "release_date": "2025-07-09T10:00:00-04:00", "title": "M8.1 flare from Active Region 14100 - May 30, 2025", "description": "Solar active region 14100 launches an M8.1 flare on May 30, 2025.", "hits": 17 }, { "id": 5565, "url": "https://svs.gsfc.nasa.gov/5565/", "result_type": "Visualization", "release_date": "2025-06-26T00:00:00-04:00", "title": "Water Cycle Extremes 2002-2024: Droughts and Pluvials", "description": "In a study of 20 years of data from the NASA/German GRACE and GRACE-FO satellites, NASA scientists confirmed that major droughts and pluvials — periods of excessive precipitation and water storage on the landscape — have been occurring more often. They also found that the worldwide intensity of these extreme wet and dry events – a metric that combines extent, duration, and severity — is closely linked to global warming.", "hits": 412 }, { "id": 5549, "url": "https://svs.gsfc.nasa.gov/5549/", "result_type": "Visualization", "release_date": "2025-06-25T10:00:00-04:00", "title": "X1.1 flare from Active Region 14098 - May 25, 2025", "description": "X1.1 flare from Active Region 14098 - May 25, 2025", "hits": 45 }, { "id": 31345, "url": "https://svs.gsfc.nasa.gov/31345/", "result_type": "Visualization", "release_date": "2025-06-11T18:59:59-04:00", "title": "One Year of PACE OCI Chlorophyll", "description": "The Ocean Color Instrument (OCI) on the Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite is a spectrometer designed to identify and quantify phytoplankton. This is a year-long visualization of the level 3 mapped chlorophyll data.", "hits": 120 }, { "id": 5541, "url": "https://svs.gsfc.nasa.gov/5541/", "result_type": "Visualization", "release_date": "2025-05-28T18:59:59-04:00", "title": "X1.2 flare from Active Region 14086 - May 13, 2025", "description": "X1.2 flare from Active Region 14086 - May 13, 2025", "hits": 30 }, { "id": 5542, "url": "https://svs.gsfc.nasa.gov/5542/", "result_type": "Visualization", "release_date": "2025-05-28T06:59:59-04:00", "title": "X2.7 and more flares from Active Region 14087 - May 14, 2025", "description": "An X 2.7 flare from Active region 14087 and a couple more, May 14, 2025, as seen by Solar Dynamics Observatory (SDO).", "hits": 23 }, { "id": 5407, "url": "https://svs.gsfc.nasa.gov/5407/", "result_type": "Visualization", "release_date": "2025-05-28T00:00:00-04:00", "title": "Solar Loops and Eruptions - October 8, 2024", "description": "A fourteen hour continuous observation of the Sun, showing the variety of eruptions.", "hits": 55 }, { "id": 5527, "url": "https://svs.gsfc.nasa.gov/5527/", "result_type": "Visualization", "release_date": "2025-05-22T00:00:00-04:00", "title": "M5.6 flare from Active Region 14046 - April 1, 2025 - No foolin'!", "description": "Active Region 14046 launches an M5.6 flare on April 1, 2025.", "hits": 13 }, { "id": 5477, "url": "https://svs.gsfc.nasa.gov/5477/", "result_type": "Visualization", "release_date": "2025-05-16T13:00:00-04:00", "title": "SOS - Day/Night cycle with Blue Marble and Black Marble Nightlights", "description": "This animation shows daylight and nighttime cycles of Earth over a three-day period in 2024 as the planet spins on it’s axis.", "hits": 1183 }, { "id": 5530, "url": "https://svs.gsfc.nasa.gov/5530/", "result_type": "Visualization", "release_date": "2025-05-14T08:00:59-04:00", "title": "Webb Confirms Seasonal Variations in Titan Climate Model", "description": "This global circulation model simulates a year of weather on Titan, depicting seasonal variations in wind currents, methane cloud cover, and sunlight over the course of a Saturn year (approximately 29.5 Earth years). New observations from the James Webb Science Telescope confirm this seasonal variation.", "hits": 181 }, { "id": 14819, "url": "https://svs.gsfc.nasa.gov/14819/", "result_type": "Produced Video", "release_date": "2025-05-06T10:45:00-04:00", "title": "NASA's NICER Studies Recurring Cosmic Crashes", "description": "Watch how astronomers used data from NASA’s NICER (Neutron star Interior Composition Explorer) to study a mysterious cosmic phenomenon called a quasi-periodic eruption, or QPE.Credit: NASA’s Goddard Space Flight CenterMusic: \"Superluminal\" by Lee Groves [PRS] and Peter Geogre Marett [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_thumbnail_NICER_QPE.jpg (1280x720) [225.7 KB] || YTframe_thumbnail_NICER_QPE_searchweb.png (320x180) [95.5 KB] || YTframe_thumbnail_NICER_QPE_thm.png [8.7 KB] || 14819_NICER_QPE_Good.mp4 (1920x1080) [70.6 MB] || 14819_NICER_QPE_Best.mp4 (1920x1080) [172.3 MB] || 14819_NICER_QPE_Captions.en_US.srt [2.8 KB] || 14819_NICER_QPE_Captions.en_US.vtt [2.7 KB] || 14819_NICER_QPE_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || ", "hits": 140 }, { "id": 40535, "url": "https://svs.gsfc.nasa.gov/gallery/tracers/", "result_type": "Gallery", "release_date": "2025-04-23T00:00:00-04:00", "title": "TRACERS – Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites", "description": "The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) helps understand magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when two magnetic fields, such as the Sun’s and Earth’s, intertwine and explosively realign. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth.\n\nTRACERS launched on July 23, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: https://science.nasa.gov/mission/tracers/", "hits": 184 }, { "id": 5526, "url": "https://svs.gsfc.nasa.gov/5526/", "result_type": "Visualization", "release_date": "2025-04-14T00:00:00-04:00", "title": "X1.1 flare from Active Region 14046 - March 28, 2025", "description": "Active region 14046 (on the left limb of the Sun) launches an X1.1 flare and a significant amount of plasma.", "hits": 26 }, { "id": 5482, "url": "https://svs.gsfc.nasa.gov/5482/", "result_type": "Visualization", "release_date": "2025-03-17T00:00:00-04:00", "title": "An M9.4 flare from Active Region 13910 - November 25, 2024", "description": "As solar rotation carries it over the left limb of the Sun, Active Region 13910 launches an M9.4 flare.", "hits": 21 }, { "id": 5513, "url": "https://svs.gsfc.nasa.gov/5513/", "result_type": "Visualization", "release_date": "2025-03-12T00:00:00-04:00", "title": "X2.0 flare from Active Region 14001 - February 23, 2025", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Just before rotating over the right solar limb, active region 14001 launches an X2.0 flare. For more details see the Space Weather database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 22 }, { "id": 5517, "url": "https://svs.gsfc.nasa.gov/5517/", "result_type": "Visualization", "release_date": "2025-03-12T00:00:00-04:00", "title": "Antarctic Sea Ice Minimum, 2025", "description": "Antarctic sea ice minimum extent, March 1 2025 || antarctic_sea_ice_min_2025_print.jpg (1024x576) [79.2 KB] || antarctic_sea_ice_min_2025.png (3840x2160) [2.8 MB] || ", "hits": 239 }, { "id": 5488, "url": "https://svs.gsfc.nasa.gov/5488/", "result_type": "Visualization", "release_date": "2025-03-05T08:02:00-05:00", "title": "An M7.1 flare from Active Region 13936 - December 29, 2024", "description": "Active Region 13936 launches an M7.1 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 21 }, { "id": 5483, "url": "https://svs.gsfc.nasa.gov/5483/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X2.2 flare from Active Region 13912 - December 8, 2024", "description": "Active region 13912 launches an X2.2 flare near the right limb on December 8, 2024.", "hits": 28 }, { "id": 5486, "url": "https://svs.gsfc.nasa.gov/5486/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M8.9 flare from Active Region 13932 - December 23, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13932 (in the lower left quadrant) launches an M8.9 flare on December 23. 2024. Some filaments of plasma launch from the site after the flare. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 14 }, { "id": 5487, "url": "https://svs.gsfc.nasa.gov/5487/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M7.4 flare from Active Region 13938 - December 26, 2024", "description": "Active region 13938 (upper left quadrant) launches an M7.4 flare.", "hits": 8 }, { "id": 5489, "url": "https://svs.gsfc.nasa.gov/5489/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X1.1 flare from Active Region 13936 - December 29, 2024", "description": "Active region 13936 (upper right quadrant) launches an X1.1 flare.", "hits": 11 }, { "id": 5484, "url": "https://svs.gsfc.nasa.gov/5484/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.4 flare from Active Region 13922 - December 10, 2024", "description": "Active region 13922 launches an M6.4 flare near the left limb of the Sun on December 10, 2024.", "hits": 17 }, { "id": 5485, "url": "https://svs.gsfc.nasa.gov/5485/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.7 flare from Active Region 13912 - December 11, 2024", "description": "Active region 13912 on the right limb of the Sun launches an M6.7 flare on December 11, 2024.", "hits": 19 }, { "id": 5500, "url": "https://svs.gsfc.nasa.gov/5500/", "result_type": "Visualization", "release_date": "2025-03-03T00:00:00-05:00", "title": "M7.6 flare from Active Region 13981 - February 6, 2025", "description": "Active Region 13981 (in the upper right quadrant of the disk) launches an M7.6 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 17 }, { "id": 5501, "url": "https://svs.gsfc.nasa.gov/5501/", "result_type": "Visualization", "release_date": "2025-03-03T00:00:00-05:00", "title": "M7.5 flare from Active Region 13981 - February 7, 2025", "description": "Active Region 13981 (in the upper right quadrant of the disk) launches an M7.5 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 24 }, { "id": 5495, "url": "https://svs.gsfc.nasa.gov/5495/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M7.4 flare from Active Region 13964 - January 17, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13964 (in the upper right quadrant of the disk) launch an M7.4 flare followed by some complex post-flare evolution.", "hits": 10 }, { "id": 5496, "url": "https://svs.gsfc.nasa.gov/5496/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.7 flare from Active Region 13978 - January 31, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13978 launch an M6.7 flare on January 31, 2025.", "hits": 18 }, { "id": 5497, "url": "https://svs.gsfc.nasa.gov/5497/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M5.1 flare from Active Region 13977 - February 2, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13977 (in the upper center of the disk) launch an M5.1 flare and a filament of material on February 2, 2025.", "hits": 22 }, { "id": 5498, "url": "https://svs.gsfc.nasa.gov/5498/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M8.8 flare from Active Region 13981 - February 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13981 launch an M8.8 flare early February 3, 2025 (a smaller M3.1 fires off near the same location about two hours later). The Earth eclipses the view from SDO as the video ends.", "hits": 23 }, { "id": 5499, "url": "https://svs.gsfc.nasa.gov/5499/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.1 flare from Active Region 13981 - February 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13981 launching an M6.1 flare on February 3, 2025.", "hits": 13 }, { "id": 5494, "url": "https://svs.gsfc.nasa.gov/5494/", "result_type": "Visualization", "release_date": "2025-02-20T00:00:00-05:00", "title": "X1.8 flare from Active Region 13947 - January 4, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13947 launch an X1.8 flare on January 4, 2025.", "hits": 18 }, { "id": 5492, "url": "https://svs.gsfc.nasa.gov/5492/", "result_type": "Visualization", "release_date": "2025-02-19T00:00:00-05:00", "title": "X1.2 flare from Active Region 13947 - January 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes active region 13947 launch an X1.2 flare on January 3, 2025.", "hits": 26 }, { "id": 5493, "url": "https://svs.gsfc.nasa.gov/5493/", "result_type": "Visualization", "release_date": "2025-02-19T00:00:00-05:00", "title": "X1.1 and M- flares from Active Region 13947 - January 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13947 launch an X1.1 flare followed by a couple of M-class flares on January 3-4 of 2025.", "hits": 17 }, { "id": 5442, "url": "https://svs.gsfc.nasa.gov/5442/", "result_type": "Visualization", "release_date": "2025-01-29T12:00:00-05:00", "title": "Water Cycle Nonstationarity", "description": "The global water cycle is undergoing unprecedented shifts from climate change, intensified by human water and land management practices. These changes are evident in phenomena such as depleted groundwater, earlier snowmelt, and erratic fluctuations in floods and drought occurrences. To better understand these changes in terrestrial water storage, scientists have integrated multiple remote sensing datasets with NASA’s advanced land surface model through data assimilation, creating a global water storage reanalysis dataset. The results capture the complex patterns of global water cycle shifts in response to both climate and human activities. Using this new integrated dataset, scientists use statistical methods (time series analysis) to identify trends (TR), seasonal shifts (SS), and changes in extreme events (EFR), ultimately developing an index, the “Nonstationarity Index,” (NSI) that quantifies the degree of nonstationarity within the global water system. || ", "hits": 30 }, { "id": 5444, "url": "https://svs.gsfc.nasa.gov/5444/", "result_type": "Visualization", "release_date": "2025-01-29T12:00:00-05:00", "title": "Terrestrial Water Storage: Regional Views 2003 - 2019", "description": "The global terrestrial water storage dataset is created using the NASA Land Information System modeling framework to merge land surface model simulations with observations from satellites through data assimilation. The team uses the Noah-MP land surface model and assimilates soil moisture from the European Space Agency’s Climate Change Initiative Program (ESA CCI), leaf area index from the Moderate Resolution Imaging Spectroradiometer (MODIS), and terrestrial water storage anomalies from the Gravity Recovery and Climate Experiment and the follow-on missions (GRACE/GRACE-FO). For more information, please visit our data description page at NASA VEDA dashboard. || ", "hits": 32 }, { "id": 14774, "url": "https://svs.gsfc.nasa.gov/14774/", "result_type": "Produced Video", "release_date": "2025-01-29T11:00:00-05:00", "title": "NASA Finds Ingredients of Life in Fragments of Lost World", "description": "Scientists studying the Bennu samples have discovered evidence of a wet, salty environment from 4.5 billion years ago that created the molecular building blocks of life.Complete transcript available.Universal Production Music: “Future Tense” by Gresby Race Nash [PRS]; “Take Off” by Nicholas Smith [PRS]; “Big Decision” by Gresby Race Nash [PRS]; “Waiting for the Answer” by Gresby Race Nash [PRS]Watch this video on the NASA Goddard YouTube channel. || 14774-Bennu-Organics-Thumbnail-V4_print.jpg (1024x576) [395.9 KB] || 14774-Bennu-Organics-Thumbnail-V4.jpg (1280x720) [1.2 MB] || 14774-Bennu-Organics-Thumbnail-V4.png (1280x720) [1.8 MB] || 14774-Bennu-Organics-Thumbnail-V4_searchweb.png (320x180) [120.2 KB] || 14774-Bennu-Organics-Thumbnail-V4_thm.png [8.3 KB] || 14774_OSIRIS-REx_Bennu_Organics_720.mp4 (1280x720) [66.1 MB] || 14774_OSIRIS-REx_Bennu_Organics_1080.mp4 (1920x1080) [370.5 MB] || BennuOrganicsCaptions.en_US.srt [6.4 KB] || BennuOrganicsCaptions.en_US.vtt [6.0 KB] || 14774_OSIRIS-REx_Bennu_Organics_4K.mp4 (3840x2160) [2.3 GB] || 14774_OSIRIS-REx_Bennu_Organics_ProRes.mov (3840x2160) [14.5 GB] || ", "hits": 382 }, { "id": 5478, "url": "https://svs.gsfc.nasa.gov/5478/", "result_type": "Visualization", "release_date": "2025-01-23T00:00:00-05:00", "title": "Science On a Sphere: IMERG Daily Precipitation Climatology (2001 - 2022)", "description": "IMERG daily climatology || IMERGdaily30_raw_v07.00001.edgefix_print.jpg (1024x512) [190.5 KB] || IMERGdaily30_raw_v07.00001.edgefix_searchweb.png (320x180) [95.5 KB] || IMERGdaily30_raw_v07.00416.edgefix_2048p30.mp4 (4096x2048) [78.3 MB] || 4096x2048_2x1_30p (4096x2048) [501 Item(s)] || IMERGdaily30_raw_v07.00001.edgefix_thm.png [7.4 KB] ||", "hits": 53 }, { "id": 40532, "url": "https://svs.gsfc.nasa.gov/gallery/punch/", "result_type": "Gallery", "release_date": "2025-01-22T00:00:00-05:00", "title": "PUNCH – Polarimeter to Unify the Corona and Heliosphere", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in low Earth orbit capturing global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind, a stream of charged particles from the Sun that fills the solar system. By using PUNCH to image the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere — including the Sun, solar wind, and Earth — as a single connected system.\n\nPUNCH launched on March 11, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: science.nasa.gov/mission/punch", "hits": 225 }, { "id": 5474, "url": "https://svs.gsfc.nasa.gov/5474/", "result_type": "Visualization", "release_date": "2025-01-20T00:00:00-05:00", "title": "Science On a Sphere: 4 Years of Biosphere", "description": "Biosphere data processed for display on Science On a Sphere (SOS)", "hits": 50 }, { "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": 177 }, { "id": 14736, "url": "https://svs.gsfc.nasa.gov/14736/", "result_type": "Produced Video", "release_date": "2024-12-16T09:00:00-05:00", "title": "NASA's #3point8 Challenge", "description": "On Dec. 24, 2024, NASA's Parker Solar Probe will fly approximately 3.8 million miles from the solar surface — the closest solar approach in history — while traveling about 430,000 miles per hour — the fastest any human-made object ever has traveled.To celebrate, join Parker's journey with a digital quest of your own: Each day from Dec. 17 - 24, 2024, we're hiding a new custom \"3.8\" digital sticker on a secret NASA webpage. Solve our puzzles to find them! || ", "hits": 94 }, { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "result_type": "Visualization", "release_date": "2024-12-12T12:00:00-05:00", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "hits": 297 }, { "id": 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": 143 }, { "id": 40529, "url": "https://svs.gsfc.nasa.gov/gallery/air-quality-dashboard/", "result_type": "Gallery", "release_date": "2024-12-04T00:00:00-05:00", "title": "Air Quality Dashboard", "description": "NASA's fleet of Earth observing satellites monitor our planet's oceans, biosphere, and atmosphere. Instruments onboard satellites observe air pollutants around the world. The data collected are used by air quality experts and researchers studying the impact of air pollution on human health.\n\n\n\n\n\n\n\n", "hits": 114 }, { "id": 5430, "url": "https://svs.gsfc.nasa.gov/5430/", "result_type": "Visualization", "release_date": "2024-12-02T00:00:00-05:00", "title": "An M9.4 flare from Active Region 13889 and more - November 10, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13889 launches an M9.4 flare on November 10, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 11 }, { "id": 5426, "url": "https://svs.gsfc.nasa.gov/5426/", "result_type": "Visualization", "release_date": "2024-11-29T00:00:00-05:00", "title": "An M5.5 flare from Active Region 13883 - November 4, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13883 launched an M5.5 flare on November 4, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 7 }, { "id": 5427, "url": "https://svs.gsfc.nasa.gov/5427/", "result_type": "Visualization", "release_date": "2024-11-29T00:00:00-05:00", "title": "An X2.3 flare from Active Region 13878 and more - November 6, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 launches an X2.3 flare, between a couple of M5+ flares, on November 6, 2024. For more details, see the Space Weather Database for the entries M 5.8 (peek at 2024-11-06T08:50), X2.3 (peak at 2024-11-06T13:40) and M5.3 (peak at 2024-11-06T14:38).For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 19 }, { "id": 5411, "url": "https://svs.gsfc.nasa.gov/5411/", "result_type": "Visualization", "release_date": "2024-11-28T00:00:00-05:00", "title": "An M6.5 flare from Active Region 13854 - October 19, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.In a last flash before rotating over the limb, active region 13854 launches an M6.5 flare on October 19, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 14 }, { "id": 5403, "url": "https://svs.gsfc.nasa.gov/5403/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 flare from Active Region 13848 - October 9, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13848 launches an X1.8 flare on October 9, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 27 }, { "id": 5406, "url": "https://svs.gsfc.nasa.gov/5406/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.7 flare from Active Region 13842 - October 9, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.In a last flash before rotating over the limb, active region 13842 launches an M7.7 flare on October 9, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 22 }, { "id": 5413, "url": "https://svs.gsfc.nasa.gov/5413/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 & M9.5 flare from Active Region 13873 - October 26, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Double flares launch from the same active region (AR 13873) less than an hour apart. For more details, see the Space Weather Database entry for M9.5 @ 2024-10-26T06:23 TAI and X1.8 @ 2024-10-26T07:19 TAI.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 21 }, { "id": 5420, "url": "https://svs.gsfc.nasa.gov/5420/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.2 flare from Active Region 13878 - October 30,2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 launches an M7.2 flare. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 17 }, { "id": 5421, "url": "https://svs.gsfc.nasa.gov/5421/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X2.0 and M9.4 flare from Active Region 13878 - October 31, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 presents a 'double whammy' of two strong flares (X 2.0 and M9.4) only about 30 minutes apart. For more details, see the Space Weather Database entries for X2.0 (peak @ 2024-10-31T21:20) and M9.4 (peak @ 2024-10-31T21:54).For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 8 }, { "id": 5412, "url": "https://svs.gsfc.nasa.gov/5412/", "result_type": "Visualization", "release_date": "2024-11-26T00:00:00-05:00", "title": "An X3.3 flare from Active Region 13869 - October 24, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13869 launches an X3.3 flare on October 24, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 16 }, { "id": 5415, "url": "https://svs.gsfc.nasa.gov/5415/", "result_type": "Visualization", "release_date": "2024-11-22T09:00:00-05:00", "title": "Moon Phase and Libration, 2025", "description": "The geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2025, at hourly intervals.", "hits": 4546 }, { "id": 5416, "url": "https://svs.gsfc.nasa.gov/5416/", "result_type": "Visualization", "release_date": "2024-11-22T09:00:00-05:00", "title": "Moon Phase and Libration, 2025 South Up", "description": " || The data in the table for all of 2025 can be downloaded as a JSON file or as a text file. || ", "hits": 573 }, { "id": 31326, "url": "https://svs.gsfc.nasa.gov/31326/", "result_type": "Hyperwall Visual", "release_date": "2024-11-18T00:00:00-05:00", "title": "GMAO South American Wild Fires", "description": "GMAO South American Wild Fires || 3840x2160_16x9_30p [0 Item(s)] || GMAO SOuth American Wild Fires ||", "hits": 19 }, { "id": 14706, "url": "https://svs.gsfc.nasa.gov/14706/", "result_type": "Produced Video", "release_date": "2024-11-08T13:00:00-05:00", "title": "NASA's Illuminate Series (2024)", "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ", "hits": 87 }, { "id": 5402, "url": "https://svs.gsfc.nasa.gov/5402/", "result_type": "Visualization", "release_date": "2024-11-05T00:00:00-05:00", "title": "An X2.1 and X1.0 flare from Active Region 13842 - October 7, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13842 launches an X2.1, followed less than 30 minutes later by an X1.0 flare on October 7, 2024. For more details, see the Space Weather Database for the X2.1 flare and the X1.0 flare.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 24 }, { "id": 5399, "url": "https://svs.gsfc.nasa.gov/5399/", "result_type": "Visualization", "release_date": "2024-11-04T00:00:00-05:00", "title": "An M6.7 flare from Active Region 13843 - October 3, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.", "hits": 28 }, { "id": 5398, "url": "https://svs.gsfc.nasa.gov/5398/", "result_type": "Visualization", "release_date": "2024-10-30T00:00:00-04:00", "title": "An X9.0 flare from Active Region 13842 - October 3, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.", "hits": 31 }, { "id": 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": 77 }, { "id": 5397, "url": "https://svs.gsfc.nasa.gov/5397/", "result_type": "Visualization", "release_date": "2024-10-17T00:00:00-04:00", "title": "An X7.1 flare from Active Region 13842 - October 1, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13842 launches an X7.1 flare on October 1, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 62 }, { "id": 5409, "url": "https://svs.gsfc.nasa.gov/5409/", "result_type": "Visualization", "release_date": "2024-10-17T00:00:00-04:00", "title": "Slow Reveal Graphs: Water Cycle Extremes", "description": "In a study of 20 years of data from the NASA/German GRACE and GRACE-FO satellites, NASA scientists confirmed that major droughts and pluvials — periods of excessive precipitation and water storage on the landscape — have been occurring more often. They also found that the worldwide intensity of these extreme wet and dry events – a metric that combines extent, duration, and severity — is closely linked to global warming.", "hits": 53 }, { "id": 14685, "url": "https://svs.gsfc.nasa.gov/14685/", "result_type": "Produced Video", "release_date": "2024-10-15T15:00:00-04:00", "title": "What is Solar Maximum?", "description": "The Sun is stirring from its latest slumber. As sunspots and flares bubble from the Sun’s surface, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced on Tuesday, September 24, 2024, the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. || ", "hits": 321 }, { "id": 5344, "url": "https://svs.gsfc.nasa.gov/5344/", "result_type": "Visualization", "release_date": "2024-10-15T14:00:00-04:00", "title": "Solar Cycle 25 - the Solar Magnetic Field from Solar Minimum to Pole Flip", "description": "One advantage of long-lived missions like Solar Dynamics Observatory (SDO) is the ability to see slow but significant changes over long periods of time.This view from SDO's Helioseismic and Magnetic Imager (HMI) shows the evolution of sunspots on the solar disk starting from solar minimum (around December 2019) and into the maximum solar activity phase. The video ends in September 2024, however this maximum phase is expected to continue into 2025.", "hits": 561 }, { "id": 14683, "url": "https://svs.gsfc.nasa.gov/14683/", "result_type": "Produced Video", "release_date": "2024-10-15T13:30:00-04:00", "title": "NASA, NOAA Announce That the Sun Has Reached the Solar Maximum Period", "description": "In a teleconference with reporters on Tuesday, October 15, 2024, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South Poles swapping places every decade — and the Sun transitions from sluggish to active and stormy.During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity, such as the storm in May 2024, has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.Listen to the media telecon.Read NASA's article about the news. || ", "hits": 836 }, { "id": 5396, "url": "https://svs.gsfc.nasa.gov/5396/", "result_type": "Visualization", "release_date": "2024-10-15T00:00:00-04:00", "title": "An M7.6 flare from Active Region 13842 - September 30, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.An M7.6 flare fires off from Active Region 13842 on September 30, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 25 }, { "id": 5370, "url": "https://svs.gsfc.nasa.gov/5370/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An M5.1 flare from Active Region 13800 - August 23, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13800 launches an M5.1 flare on August 23, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 16 }, { "id": 5385, "url": "https://svs.gsfc.nasa.gov/5385/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An M5.0 flare from Active Region 13811 - September 11, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13811 launches an M5.0 flare on September 11, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 8 }, { "id": 5386, "url": "https://svs.gsfc.nasa.gov/5386/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An X1.3 flare from Active Region 13825 - and later an M6.8 - September 12, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13825 launches an X1.3 flare on the lower left limb on September 12, 2024. Later, an M6.8 (14:43 TAI) erupts on the right limb. For more details, see the Space Weather Database for X1.3 and M6.8. An additional small filament eruption occurs near the center of the disk about 17:24 TAI.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 16 }, { "id": 5387, "url": "https://svs.gsfc.nasa.gov/5387/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An M5.4 flare from Active Region 13811 - September 13, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Framed by a set of large coronal loops, active Region AR 13811 launches an M5.4 flare on September 13, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 11 }, { "id": 5388, "url": "https://svs.gsfc.nasa.gov/5388/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An X4.5 flare from Active Region 13825 - September 14, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.", "hits": 17 }, { "id": 5401, "url": "https://svs.gsfc.nasa.gov/5401/", "result_type": "Visualization", "release_date": "2024-10-08T00:00:00-04:00", "title": "Powerful Hurricane Milton forms in the Gulf of Mexico, sweeps into Florida", "description": "Example composite showing how all the below animations can be combined into one long segment showing the lifecycle of Hurricane Milton through the eyes of GPM beginning October 6 ending October 9, 2024. || milton_lifecycle.00001_print.jpg (1024x576) [236.4 KB] || milton_lifecycle.mp4 (1920x1080) [287.6 MB] ||", "hits": 94 }, { "id": 5333, "url": "https://svs.gsfc.nasa.gov/5333/", "result_type": "Visualization", "release_date": "2024-10-07T09:00:00-04:00", "title": "DYAMOND Global Carbon Dioxide for Fulldome", "description": "Global CO2 ppm for January-March of 2020. This camera move orbits the Earth from a distance. || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k.00200_print.jpg (1024x1024) [19.8 KB] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k.00200_searchweb.png (320x180) [5.4 KB] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k.00200_web.png (320x320) [6.0 KB] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k.00200_thm.png (80x40) [751 bytes] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome_2048p30_h264.mp4 (2048x2048) [2.2 MB] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k [0 Item(s)] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k_4096p30_h265.mp4 (4096x4096) [9.0 MB] || dyamondPointCloud_12-4-2023b_dyamond_co2_anim_globe_orbit_dome4k_4096p30_h265.mp4.hwshow || ", "hits": 158 }, { "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": 175 }, { "id": 5359, "url": "https://svs.gsfc.nasa.gov/5359/", "result_type": "Visualization", "release_date": "2024-10-03T00:00:00-04:00", "title": "An M5.3 flare from Active Region 13780 - August 10, 2024", "description": "Active Region AR 13780 launches an M5.3 flare on August 10, 2024. For more details, see the Space Weather Database entry.", "hits": 17 }, { "id": 5367, "url": "https://svs.gsfc.nasa.gov/5367/", "result_type": "Visualization", "release_date": "2024-10-03T00:00:00-04:00", "title": "An X1.1 flare from Active Region 13784 - August 14, 2024", "description": "Active Region AR 13784 launches an X1.1 flare on August 14, 2024.", "hits": 14 }, { "id": 5346, "url": "https://svs.gsfc.nasa.gov/5346/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An X1.5 flare from Active Region 13764 - July 29, 2024", "description": "Active Region AR 13764 launches an X1.5 flare on July 29, 2024. A small M1 erupts later in the lower right quadrant (05:20 TAI). Then the 'curtain' falls as Earth eclipses. SDO's geosynchronous orbit around Earth enables the Sun to occasionally be eclipsed by Earth (Eclipse Season Starts for NASA's SDO).", "hits": 19 }, { "id": 5347, "url": "https://svs.gsfc.nasa.gov/5347/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An M8.7 flare from Active Region 13762 and more - July 29, 2024", "description": "Active Region AR 13762 launches an M8.7 flare on July 29, 2024. A smaller M4.2 flare fires shortly thereafter (14:42 TAI) on the left limb. For more details, see the Space Weather Database entry for M8.7 and M4.2.", "hits": 7 } ] }