{ "count": 232, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Eruption%22", "previous": null, "results": [ { "id": 15041, "url": "https://svs.gsfc.nasa.gov/15041/", "result_type": "Produced Video", "release_date": "2026-05-20T09:00:00-04:00", "title": "NASA's Fermi Spies a Supercharged Supernova", "description": "Gamma rays detected by NASA’s Fermi Gamma-ray Space Telescope gave scientists a look under the hood of a rare supernova that produced much more light than normal.Credit: NASA’s Goddard Space Flight CenterMusic credits:\"Granular Game\" by John Bisset \"In The Zone\" by Daniel Migdal, Jonas Pomo\"Ornaments\" by Lisa Van Hal || Fermi_Spies_a_Supercharged_Supernova_Thumbnail.jpg (1280x720) [231.5 KB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.en_US.srt [2.2 KB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.en_US.vtt [2.1 KB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.webm (3840x2160) [34.1 MB] || 15041-_Fermi_Spies_a_Supercharged_Supernova.mp4 (3840x2160) [892.9 MB] || 15041-_Fermi_Spies_a_Supercharged_Supernova_ProRes.mov (3840x2160) [6.3 GB] || ", "hits": 365 }, { "id": 15005, "url": "https://svs.gsfc.nasa.gov/15005/", "result_type": "Visualization", "release_date": "2026-04-28T00:00:00-04:00", "title": "Mount Saint Helens Recovery", "description": "In 1980, Mount Saint Helens erupted and destroyed 230 square miles of forest in Washington State. This near-infrared time series follows the decades-long recovery of that scarred landscape. Volcanic ash and rock appear grey, while plant life appears bright red.", "hits": 37 }, { "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": 230 }, { "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": 40 }, { "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": 810 }, { "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": 223 }, { "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": 346 }, { "id": 31349, "url": "https://svs.gsfc.nasa.gov/31349/", "result_type": "Hyperwall Visual", "release_date": "2025-05-28T18:59:59-04:00", "title": "Juno images, 2024 - early 2025", "description": "Several recent images from the JunoCam and Jovian Infrared Auroral Mapper (JIRAM) instruments show volcanic hot spots on IO, polar storms and Jupiter's moon Amalthea.", "hits": 133 }, { "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": 79 }, { "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": 439 }, { "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": 70 }, { "id": 20393, "url": "https://svs.gsfc.nasa.gov/20393/", "result_type": "Animation", "release_date": "2024-11-04T11:00:00-05:00", "title": "T Coronae Borealis Nova Animations", "description": "Located 3,000 light-years away, T Coronae Borealis — T CrB for short — contains two stars that orbit each other: a red giant nearing the end of its life and an Earth-sized stellar remnant known as a white dwarf. The dwarf’s intense gravity rounds up some of the gas flowing off of the red giant, forming a flattened cloud of gas around the dwarf — an accretion disk. Gas in the disk gradually works its way inward, eventually flowing onto the white dwarf nestled at its center. Credit: NASA's Goddard Space Flight Center Conceptual Image LabAlt text: Animation showing the T CrB system || T_CrB_NOVA_SHOT_1_4k_30fps_ProRes.00300_print.jpg (1024x576) [91.6 KB] || T_CrB_NOVA_SHOT_1_4k_30fps_h264.mp4 (3840x2160) [18.1 MB] || T_CrB_Nova_S1 [0 Item(s)] || T_CrB_NOVA_SHOT_1_4k_30fps_ProRes.webm (3840x2160) [4.5 MB] || T_CrB_NOVA_SHOT_1_4k_30fps_ProRes.mov (3840x2160) [984.5 MB] || ", "hits": 664 }, { "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": 685 }, { "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": 17 }, { "id": 5334, "url": "https://svs.gsfc.nasa.gov/5334/", "result_type": "Visualization", "release_date": "2024-09-02T00:00:00-04:00", "title": "An M5.3 flare from Active Region 13738 - July 13, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13738 launches an M5.3 flare on July 13, 2024. For more details, see the Space Weather Database entry. There's also a nice eruption off the left limb.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 21 }, { "id": 14599, "url": "https://svs.gsfc.nasa.gov/14599/", "result_type": "Produced Video", "release_date": "2024-06-03T11:00:00-04:00", "title": "Sun Releases 50th X flare of Solar Cycle 25, Quickly Followed by Two More", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright eruption on the lower left – at 22:03 UTC on May 31, 2024. The image shows a blend of 131 Angstrom and 304 Angstrom light, subsets of extreme ultraviolet light. Credit: NASA/SDO || SDO_May31_2024_2204_131_304_2.jpg (4096x4096) [2.9 MB] || SDO_May31_2024_2204_131_304_2_searchweb.png (320x180) [83.2 KB] || SDO_May31_2024_2204_131_304_2_thm.png (80x40) [6.2 KB] || ", "hits": 274 }, { "id": 14597, "url": "https://svs.gsfc.nasa.gov/14597/", "result_type": "Produced Video", "release_date": "2024-05-28T16:00:00-04:00", "title": "Strong Solar Flare Erupts from Sun, May 27, 2024 and Another May 29th.", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare seen as the bright flash on the limb of the Sun on May 27, 2024, with an inset image of Earth for scale. The image shows a blend of 171 and 304 angstrom extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in red and yellow. Credit: NASA/SDO || SDO_May_27_Flare0700UT_171-304_EarthScale.jpg (1500x1500) [568.4 KB] || SDO_May_27_Flare0700UT_171-304_EarthScale_searchweb.png (320x180) [97.9 KB] || SDO_May_27_Flare0700UT_171-304_EarthScale_thm.png (80x40) [7.3 KB] || ", "hits": 355 }, { "id": 14592, "url": "https://svs.gsfc.nasa.gov/14592/", "result_type": "Produced Video", "release_date": "2024-05-14T00:00:00-04:00", "title": "Largest Flare yet from Solar Cycle 25", "description": "On May 14, 2024, the Sun emitted a strong solar flare. This solar flare is the largest of Solar Cycle 25 and is classified as an X8.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.A solar flare is an intense burst of radiation, or light, on the Sun. Flares are our solar system’s most powerful explosive events. Light only takes about 8 minutes to travel from the Sun to Earth, so that’s how long it would take the energy from a flare to reach our planet. Stronger solar flares — those rated class M5 or above — can have impacts on technology that depends on Earth’s ionosphere (our electrically charged upper atmosphere), like high-frequency radio used for navigation and GPS.NASA’s Solar Dynamics Observatory (SDO) captured these images of the flare, which peaked at 12:51 p.m. ET on May 14. The X8.7 flare appears on the lower right edge of the Sun. (A small eruption appears afterward in the upper left.) SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. Different wavelengths are shown in this video to highlight different features of the flare.Music credit: “Ethereal Mirrorscape” from the album Reflections written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || X8pt7_flare_May_14_2024.00_00_40_22.Still001.jpg (3840x2160) [3.0 MB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_print.jpg (1024x576) [342.3 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_searchweb.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_web.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_thm.png (80x40) [6.1 KB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.webm (3840x2160) [20.4 MB] || 14592_SDO_X8pt7_flare_May_14_2024_Good_Outro.mp4 (3840x2160) [175.9 MB] || 14592_SDO_X8pt7_flare_May_14_2024_YouTube_Outro.mp4 (3840x2160) [673.0 MB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.mov (3840x2160) [4.2 GB] || ", "hits": 539 }, { "id": 31277, "url": "https://svs.gsfc.nasa.gov/31277/", "result_type": "Hyperwall Visual", "release_date": "2024-04-12T00:00:00-04:00", "title": "Gravity waves from Hunga Tonga Eruption", "description": "Gravity waves caused by the Hunga Tonga-Hunga Ha′apai volcanic eruption can be seen in Geostationary satellite data by taking the difference between subsequent images. Global images are acquired every 10 minutes by the GOES and Himawari weather satellite imagers. Calculating the difference between two subsequent images reveals circular gravity waves spreading out from the eruption center. || ", "hits": 223 }, { "id": 5233, "url": "https://svs.gsfc.nasa.gov/5233/", "result_type": "Visualization", "release_date": "2024-03-26T00:00:00-04:00", "title": "X6.3 flare at Active Region 13590 - February 22, 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.And yet again, less than a day after it's X1.7 flare, Active Region 13590 tops off the day with an X6.3 eruption (largest so far this solar cycle) in the upper left quadrant. For details of this event, see the Space Weather database entry. For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 12 }, { "id": 5220, "url": "https://svs.gsfc.nasa.gov/5220/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "X3.3 flare at Active Region 13575 - February 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.Just days after an eruption, Active Region 13575, now carried by solar rotation just over the lower right limb of the solar disk, launches an X3.3 class flare. For details of this event, 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": 5224, "url": "https://svs.gsfc.nasa.gov/5224/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "M6.5 flare at Active Region 13576 - February 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.About a day after a previous M-class eruption, Active Region 13576 now launches another mid-range (M6.5 class) flare. For details of this event, see the Space Weather database entry. Near the end of this movie, we can see another lump of hot plasma erupting from the lower right from an active region now on the backside of the Sun from Earth.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": 13 }, { "id": 14531, "url": "https://svs.gsfc.nasa.gov/14531/", "result_type": "Produced Video", "release_date": "2024-02-20T10:00:00-05:00", "title": "February 16, 2024 X2.5 Solar Flare", "description": "NASA’s Solar Dynamics Observatory captured these images of a solar flare – as seen in the bright flash on the right of each image – on Feb. 16, 2024. The images show three subsets of extreme ultraviolet light that highlight the extremely hot material in flares and which are colorized in teal, gold, and red. Credit: NASA/SDO || Feb_16_Flare_Video_multi_still.jpg (1920x1080) [389.3 KB] || Feb_16_Flare_Video_multi_still_searchweb.png (320x180) [85.5 KB] || Feb_16_Flare_Video_multi_still_thm.png (80x40) [7.1 KB] || Feb_16_Flare_Video_multi.mp4 (1920x1080) [53.9 MB] || Feb_16_Flare_Video_multi.mov (1920x1080) [379.3 MB] || ", "hits": 103 }, { "id": 14479, "url": "https://svs.gsfc.nasa.gov/14479/", "result_type": "Produced Video", "release_date": "2024-02-09T11:00:00-05:00", "title": "Sun Releases X3.3 Flare on February 9, 2024", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the lower right – on Feb. 9, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona and the extremely hot material in flares, respectively. Credit: NASA/SDO || SDO_Feb_9_Flare1314UTC_131-171.jpg (4096x4096) [2.8 MB] || SDO_Feb_9_Flare1314UTC_131-171_searchweb.png (320x180) [102.5 KB] || SDO_Feb_9_Flare1314UTC_131-171_thm.png (80x40) [8.1 KB] || ", "hits": 93 }, { "id": 5205, "url": "https://svs.gsfc.nasa.gov/5205/", "result_type": "Visualization", "release_date": "2024-01-23T00:00:00-05:00", "title": "M6.3 & M6.9 'double' flares at Active Region 13514 - December 15, 2023", "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 13514 near the right limb of the solar disk does a 'double' eruption with two M6 class solar flares minutes apart. For details of this event, see the Space Weather database entry for M6.3 and Space Weather database entry for M6.9.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 10 }, { "id": 14498, "url": "https://svs.gsfc.nasa.gov/14498/", "result_type": "Produced Video", "release_date": "2024-01-11T11:05:00-05:00", "title": "Finding A New Galactic 'Fossil'", "description": "Some 5 million years ago, a black hole eruption in the galaxy NGC 4945 set off a star-formation frenzy and shot a vast cloud of gas into intergalactic space. Watch and learn how two X-ray telescopes revealed the story.Music Credits: Universal Production Music\"Planetary Horizons\" by Jia Lee\"Eyes Peeled\" by Bard\"Sprinkle of Mischief\" by Ash and HaroldWatch this video on the NASA Goddard YouTube channel.Credit: NASA’s Goddard Space Flight Center", "hits": 54 }, { "id": 5202, "url": "https://svs.gsfc.nasa.gov/5202/", "result_type": "Visualization", "release_date": "2023-12-22T00:00:00-05:00", "title": "M 5.4 flare at Active Region 13511 - December 8, 2023", "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 13511 near the lower right of the solar disk erupts with a class M5.4 flare. A particularly bright loop forms afterwards, apparently as part of the eruption. For details of this event, 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": 5201, "url": "https://svs.gsfc.nasa.gov/5201/", "result_type": "Visualization", "release_date": "2023-12-13T00:00:00-05:00", "title": "M 9.8 flare at Active Region 13500 - November 28, 2023", "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 13500 near the center of the solar disk erupts with a class M9.8 flare. A nice loop arcade forms, apparently as part of the eruption. For details of this event, see the Space Weather database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 12 }, { "id": 5159, "url": "https://svs.gsfc.nasa.gov/5159/", "result_type": "Visualization", "release_date": "2023-09-20T00:00:00-04:00", "title": "M 6.0 flare at Active Region 13413 - September 3, 2023", "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 13413 on the limb of the Sun erupts with mid-range flare exceeding M5 intensity. A nice loop arcade forms, apparently as part of the eruption. For details of this event, 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": 45 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 273 }, { "id": 40507, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Heliophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 164 }, { "id": 14317, "url": "https://svs.gsfc.nasa.gov/14317/", "result_type": "Produced Video", "release_date": "2023-03-28T13:50:00-04:00", "title": "NASA Missions Probe What May Be a 1-In-10,000-Year Gamma-ray Burst", "description": "The Hubble Space Telescope’s Wide Field Camera 3 revealed the infrared afterglow (circled) of the BOAT GRB and its host galaxy, seen nearly edge-on as a sliver of light extending to the burst's upper left. This animation flips between images taken on Nov. 8 and Dec. 4, 2022, one and two months after the eruption. Given its brightness, the burst’s afterglow may remain detectable by telescopes for several years. Each picture combines three near-infrared images taken at wavelengths from 1 to 1.5 microns and is 34 arcseconds across. Credit: NASA, ESA, CSA, STScI, A. Levan (Radboud University); Image Processing: Gladys Kober || GRB_WFC3IR1108+1204_circled.gif (512x512) [3.5 MB] || ", "hits": 342 }, { "id": 5082, "url": "https://svs.gsfc.nasa.gov/5082/", "result_type": "Visualization", "release_date": "2023-03-21T12:00:00-04:00", "title": "M 3.7 Flare and filament eruption at Active Region 13229 - February 24, 2023", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.A active region AR13229 near the center of the solar disk launches a mid-level M 3.7 class flare followed by a large filament eruption. The point-spread function correction (PSF) has been applied to all the imagery on this page.Event Description || ", "hits": 48 }, { "id": 40464, "url": "https://svs.gsfc.nasa.gov/gallery/cosmic-cycles1-the-sun/", "result_type": "Gallery", "release_date": "2023-03-21T00:00:00-04:00", "title": "Cosmic Cycles 1: The Sun", "description": "Born from a swirling cloud of dust and gas some 4.6 billion years ago, our Sun seethes and boils like a living thing. It is the very center of our solar system, and large enough to encompass 1.3 million Earths. Explosions flash on its surface in colors of light beyond human vision and enormous loops of plasma stretch into space. The Sun’s influence extends out beyond the planets, creating a protective cocoon within the galaxy.\n\nWant to know more?\nSDO Gallery SDO website NASA Heliophysics Home Page", "hits": 61 }, { "id": 14288, "url": "https://svs.gsfc.nasa.gov/14288/", "result_type": "Produced Video", "release_date": "2023-03-03T09:55:00-05:00", "title": "Hubble’s Inside The Image: V838 Mon", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the breathtaking image sequence of V838 Monocerotis (V838 Mon).Called a light echo, the expanding illumination of interstellar dust around the star has been revealing remarkable structures in the dusty cloud ever since the star suddenly brightened in January 2002. V838 Mon temporarily became 600,000 times brighter than our Sun, until it faded in April 2002. It was one of the brightest stars in the entire Milky Way. The reason for the eruption is still unclear.In this video, Dr. Padi Boyd explains this fascinating piece of history, teaching us some of the interesting science behind this famous Hubble image.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin FilmsVideo Credit:Hubble Space Telescope AnimationCredit: ESA/Hubble (M. Kornmesser & L. L. Christensen), A. Fujii, Robert Gendler, Digitized Sky Survey 2, Panther Observatory, Steve Cannistra, Michael Pierce, Robert Berrington (Indiana University), Nigel Sharp, Mark Hanna (NOAO)/WIYN/NSFMusic Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Moving Headlines” by Immersive Music (Via Shutterstock Music) || ", "hits": 64 }, { "id": 5077, "url": "https://svs.gsfc.nasa.gov/5077/", "result_type": "Visualization", "release_date": "2023-02-27T00:00:00-05:00", "title": "M1 Flare and Eruption on Solar Limb - February 7, 2023", "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 active region coming around the left limb of the sun launches a small M1 class flare and then an impressive flame-like eruption of solar material. The point-spread function correction (PSF) has been applied to all the imagery on this page. || ", "hits": 43 }, { "id": 5068, "url": "https://svs.gsfc.nasa.gov/5068/", "result_type": "Visualization", "release_date": "2023-02-10T00:00:00-05:00", "title": "Impressive solar filament eruption - January 20, 2023", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.A large solar filament hovers above the solar surface (lower right) for several hours before eventually launching into space. || ", "hits": 38 }, { "id": 14214, "url": "https://svs.gsfc.nasa.gov/14214/", "result_type": "Produced Video", "release_date": "2022-09-20T00:00:00-04:00", "title": "How NASA Sees the Life Cycle of Volcanic Island Hunga Tonga-Hunga Ha’apai", "description": "Complete transcript available. || HHTH_Final.00001_print.jpg (1024x576) [78.9 KB] || Thumbnail.png (2838x1588) [5.2 MB] || HHTH_Final.00001_searchweb.png (320x180) [66.5 KB] || HHTH_Final.00001_thm.png (80x40) [5.0 KB] || HHTH_Final.webm (1920x1080) [43.1 MB] || HHTH_Final.mp4 (1920x1080) [779.2 MB] || HHTH_Audio_otter_ai.en_US.srt [7.7 KB] || HHTH_Audio_otter_ai.en_US.vtt [7.7 KB] || ", "hits": 178 }, { "id": 5008, "url": "https://svs.gsfc.nasa.gov/5008/", "result_type": "Visualization", "release_date": "2022-08-19T00:00:00-04:00", "title": "A Peek from SDO: An Eruption on the Solar Limb", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.A large eruption occurs off the limb of the Sun (lower right) in this image sequence from May 2022. || ", "hits": 88 }, { "id": 14148, "url": "https://svs.gsfc.nasa.gov/14148/", "result_type": "Produced Video", "release_date": "2022-05-05T12:45:00-04:00", "title": "Magnetic Flip Drives Flare-Up of Monster Black Hole", "description": "Explore the unusual eruption of 1ES 1927+654, a galaxy located 236 million light-years away in the constellation Draco. A sudden reversal of the magnetic field around its million-solar-mass black hole may have triggered the outburst.Credit: NASA’s Goddard Space Flight Center Music: \"Water Dance\" and \"Alternate Worlds\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || ChangingLookAGN_Still1.jpg (1920x1080) [822.9 KB] || ChangingLookAGN_Still1_searchweb.png (320x180) [79.5 KB] || ChangingLookAGN_Still1_thm.png (80x40) [6.2 KB] || 14148_ChangingLook_AGN_1080.webm (1920x1080) [24.8 MB] || 14148_ChangingLook_AGN_Sub100MB.mp4 (1920x1080) [91.5 MB] || 14148_ChangingLook_AGN_1080.mp4 (1920x1080) [246.5 MB] || 14148_ChangingLook_AGN_Best_1080.mp4 (1920x1080) [534.7 MB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.srt [4.2 KB] || 14148_ChangingLook_AGN_SRT_Captions.en_US.vtt [4.3 KB] || 14148_ChangingLook_AGN_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 97 }, { "id": 14149, "url": "https://svs.gsfc.nasa.gov/14149/", "result_type": "Produced Video", "release_date": "2022-05-02T10:45:00-04:00", "title": "NASA's Black Hole Orrery", "description": "Learn more about the best-known black hole systems in our galaxy and its neighbor, the Large Magellanic Cloud. This visualization presents 22 X-ray binary systems that host confirmed black holes at the same scale, with their orbits sped up by about 22,000 times. The view of each system reflects how we see it from Earth. Star colors ranging from blue-white to reddish represent temperatures from 5 times hotter to 45% cooler than our Sun. In most of these systems, a stream of matter from the star forms an accretion disk around the black hole. In others, like the famous system called Cygnus X-1, the star produces a hefty outflow that is partly swept up by the black hole’s gravity to form the disk. The accretion disks use a different color scheme because they sport even higher temperatures than the stars. The largest disk shown, belonging to a binary called GRS 1915, spans a distance greater than that separating Mercury from our Sun. The black holes themselves are shown larger than in reality using spheres scaled to reflect their masses.Credit: NASA's Goddard Space Flight Center and Scientific Visualization StudioMusic: \"Event Horizon\" from Gravity. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Black_Hole_Orrery_Still.jpg (3840x2160) [321.9 KB] || Black_Hole_Orrery_Still_searchweb.png (320x180) [25.6 KB] || Black_Hole_Orrery_Still_thm.png (80x40) [4.1 KB] || 14149_Black_Hole_Orrery_FINAL_1080.mp4 (1920x1080) [118.8 MB] || 14149_Black_Hole_Orrery_FINAL_1080.webm (1920x1080) [12.4 MB] || 14149_Black_Hole_Orrery_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || 14149_Black_Hole_Orrery_FINAL_4k_Best.mp4 (3840x2160) [379.2 MB] || 14149_Black_Hole_Orrery_FINAL_4k.mp4 (3840x2160) [176.7 MB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.srt [1.9 KB] || 14149_Black_Hole_Orrery_SRT_Captions.en_US.vtt [1.9 KB] || ", "hits": 286 }, { "id": 14132, "url": "https://svs.gsfc.nasa.gov/14132/", "result_type": "Produced Video", "release_date": "2022-04-12T00:00:00-04:00", "title": "Black Hole Week: Black Hole GIFs", "description": "Black Hole WeekThis page provides social media assets used during previous celebrations of Black Hole Week. Join in! Below, you'll find many GIFs to use. || ", "hits": 540 }, { "id": 14126, "url": "https://svs.gsfc.nasa.gov/14126/", "result_type": "Produced Video", "release_date": "2022-04-01T00:00:00-04:00", "title": "SDO Video Toolkit", "description": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files || New_Trebuchet_mkII.00300_print.jpg (1024x576) [336.5 KB] || New_Trebuchet_mkII.00300_print_searchweb.png (320x180) [95.4 KB] || New_Trebuchet_mkII.00300_print_thm.png (80x40) [6.2 KB] || New_Trebuchet_mkII.mp4 (1920x1080) [32.4 MB] || New_Trebuchet_mkII.webm (1920x1080) [3.7 MB] || New_Trebuchet_mkII.mov (1920x1080) [443.3 MB] || New_Trebuchet_mkII.mp4.hwshow [115 bytes] || ", "hits": 626 }, { "id": 14084, "url": "https://svs.gsfc.nasa.gov/14084/", "result_type": "Produced Video", "release_date": "2022-02-22T15:00:00-05:00", "title": "NOAA and NASA Ready to Launch Crucial New Earth-Observing Satellite Live Shots", "description": "Quick link to EDITED B-ROLLQuick link to GOES-T resource pageQuick link to canned interview with NOAA GOES-R Program Chief of Staff Kevin Fryer || 32ABE9D9-BE05-487C-93CD-A1BA183FB9CE_1_105_c.jpeg (1399x561) [292.0 KB] || 32ABE9D9-BE05-487C-93CD-A1BA183FB9CE_1_105_c_print.jpg (1024x410) [166.8 KB] || 32ABE9D9-BE05-487C-93CD-A1BA183FB9CE_1_105_c_searchweb.png (320x180) [115.6 KB] || 32ABE9D9-BE05-487C-93CD-A1BA183FB9CE_1_105_c_thm.png (80x40) [8.5 KB] || ", "hits": 53 }, { "id": 13919, "url": "https://svs.gsfc.nasa.gov/13919/", "result_type": "Produced Video", "release_date": "2021-08-31T10:00:00-04:00", "title": "Landsat 9 L-16 Press Briefing Graphics", "description": "Officials from NASA and the U.S. Geological Survey (USGS) discussed the upcoming launch of the Landsat 9 satellite during a media briefing at 10 a.m. EDT Tuesday, Aug. 31.The Landsat 9 launch is targeted for no earlier than Thursday, Sept. 23, 2021.The media briefing will air live on NASA TV, the NASA app, and the agency’s website.Data from Landsat 9 will add to nearly 50 years of free and publicly available data from the Landsat program. The Landsat program is the longest-running enterprise for acquisition of satellite imagery of Earth. It is a joint NASA/USGS program. Researchers harmonize Landsat data to detect the footprint of human activities and measure the effects of climate change on land over decades.Once fully operational in orbit, Landsat 9 will replace Landsat 7 and join its sister satellite, Landsat 8, in continuing to collect data from across the planet every eight days. This calibrated data will continue the Landsat program’s critical role in monitoring land use and helping decision-makers manage essential resources including crops, water resources, and forests.Briefing participants, in speaking order, are:•Karen St. Germain, director of NASA's Earth Science Division•Del Jenstrom, Landsat 9 project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland•Jeff Masek, Landsat 9 project scientist at Goddard•David Applegate, acting director of USGS•Birgit Peterson, geographer at USGS•Inbal Becker-Reshef, director of NASA’s Harvest food security and agriculture program.NASA manages the Landsat 9 mission. Goddard teams also built and tested one of the two instruments on Landsat 9, the Thermal Infrared Sensor 2 (TIRS-2) instrument. TIRS-2 will use thermal imaging to make measurements that are used to calculate soil moisture and detect the health of plants.The USGS Earth Resources Observation and Science Center in Sioux Falls, South Dakota, will operate the mission and manage the ground system, including maintaining the Landsat archive. Ball Aerospace in Boulder, Colorado, built and tested the Operational Land Imager 2 (OLI-2) instrument, another imaging sensor that provides data in the visible, near infrared, and shortwave infrared portions of the spectrum. United Launch Alliance is the rocket provider for Landsat 9’s launch. Northrop Grumman in Gilbert, Arizona, built the Landsat 9 spacecraft, integrated it with instruments, and tested the observatory.For more information:Media AdvisoryLandsat Video Resourceshttps://landsat.gsfc.nasa.gov/https://www.usgs.gov/landsat || ", "hits": 39 }, { "id": 4909, "url": "https://svs.gsfc.nasa.gov/4909/", "result_type": "Visualization", "release_date": "2021-06-18T11:00:00-04:00", "title": "Monster Solar Filament Launch and CME", "description": "Launch of the filament at low cadence (36 seconds) as visible in the 304 Angstrom filter on SDO/AIA. || FilamentLaunch2012-Slow_304A_stand.HD1080i.00876_print.jpg (1024x576) [134.4 KB] || FilamentLaunch2012-Slow_304A_stand.HD1080i.00876_searchweb.png (320x180) [48.3 KB] || FilamentLaunch2012-Slow_304A_stand.HD1080i.00876_thm.png (80x40) [4.1 KB] || FilamentLaunch2012-Slow_304A (1920x1080) [0 Item(s)] || FilamentLaunch2012-Slow_304A_stand.HD1080i_p30.mp4 (1920x1080) [85.3 MB] || FilamentLaunch2012-Slow_304A_stand.HD1080i_p30.webm (1920x1080) [7.0 MB] || FilamentLaunch2012-Slow_304A.UHD (3840x2160) [0 Item(s)] || FilamentLaunch2012-Slow_304A_stand.UHD2160_p30.mp4 (3840x2160) [477.3 MB] || FilamentLaunch2012-Slow_304A_stand.HD1080i_p30.mp4.hwshow [212 bytes] || ", "hits": 141 }, { "id": 13869, "url": "https://svs.gsfc.nasa.gov/13869/", "result_type": "Produced Video", "release_date": "2021-06-07T15:00:00-04:00", "title": "The key to understanding solar explosions", "description": "Music credit: Universal Music Production“Early Birds,” Edwards Tschuggnall || ROSETTASTONE_THUMB.png (1920x1080) [1.0 MB] || ROSETTASTONE_THUMB_print.jpg (1024x576) [63.6 KB] || ROSETTASTONE_THUMB_searchweb.png (320x180) [56.1 KB] || ROSETTASTONE_THUMB_thm.png (80x40) [5.4 KB] || 0607_ROSETTASTONE_VIDEOFINAL.mp4 (1920x1080) [273.3 MB] || 0607_ROSETTASTONE_VIDEOFINAL.webm (1920x1080) [17.0 MB] || ROSETTASTONE_CAPTION.en_US.srt [2.5 KB] || ROSETTASTONE_CAPTION.en_US.vtt [2.5 KB] || ", "hits": 26 }, { "id": 4904, "url": "https://svs.gsfc.nasa.gov/4904/", "result_type": "Infographic", "release_date": "2021-04-28T00:00:00-04:00", "title": "Heliophysics Background Images for MS-Teams & PowerPoint", "description": "Upper atmosphere & ionosphere theme. || Helio_Teams_Bkgrd_1.jpg (1920x1080) [218.8 KB] || Helio_Teams_Bkgrd_1_with_Logos.png (1920x1080) [2.3 MB] || Helio_Teams_Bkgrd_1_with_Logos_and_Txt.png (1920x1080) [2.3 MB] || Helio_Teams_Bkgrd_1_print.jpg (1024x576) [151.3 KB] || Helio_Teams_Bkgrd_PPT_1.pptx [520.0 KB] || Six theme images for NASA Heliophysics - image, image+logos, image+logos+text, and PowerPoint files. Suitable as background images for MS-Teams and PowerPoint presentations. || ", "hits": 61 }, { "id": 4861, "url": "https://svs.gsfc.nasa.gov/4861/", "result_type": "Visualization", "release_date": "2021-03-17T00:00:00-04:00", "title": "Three years of SAGE III/ISS Stratospheric Aerosol Data", "description": "About three years of stratospheric aerosol data from SAGE III visualizing a zonal mean and measurements of various high aerosol events across the globe || sage3_final_full_60fps.7300_print.jpg (1024x576) [98.9 KB] || sage3_final_full_60fps.7300_searchweb.png (320x180) [57.4 KB] || sage3_final_full_60fps.7300_thm.png (80x40) [4.4 KB] || sage3_final_full_1080p59.94.webm (1920x1080) [25.5 MB] || orig (3840x2160) [1.0 MB] || sage3_final_full_1080p59.94.mp4 (1920x1080) [234.0 MB] || sage3_final_full_2160p59.94.mp4 (3840x2160) [1.0 GB] || ", "hits": 37 }, { "id": 20338, "url": "https://svs.gsfc.nasa.gov/20338/", "result_type": "Animation", "release_date": "2020-12-08T15:00:00-05:00", "title": "SunRISE Beauty Pass", "description": "A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events. || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_print.jpg (1024x576) [172.5 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_searchweb.png (320x180) [87.2 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.00240_thm.png (80x40) [5.9 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.mov (3840x2160) [695.8 MB] || SUNRISE-shot1_v06_4k_30fps_h264.mp4 (3840x2160) [13.7 MB] || SUNRISE-shot1_v06_4k (3840x2160) [32.0 KB] || SUNRISE-shot1_v06_4k_30fps_ProRes422.webm (3840x2160) [5.3 MB] || ", "hits": 71 }, { "id": 13778, "url": "https://svs.gsfc.nasa.gov/13778/", "result_type": "Produced Video", "release_date": "2020-12-03T17:00:00-05:00", "title": "Solar Activity Continues to Rise with 'Anemone' Eruption", "description": "Short video showing the solar flare and subsequent prominence eruption and \"arcade\" of loops.Credit: NASA/GSFC/SDOMusic: \"Beautiful Awesome\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Anemone_Eruption_131-171_Blend.jpg (1920x1080) [281.9 KB] || Anemone_Eruption_131-171_Blend_searchweb.png (180x320) [78.6 KB] || Anemone_Eruption_131-171_Blend_thm.png (80x40) [6.6 KB] || 13778_Anemone_Eruption_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 13778_Anemone_Eruption_Best_1080.mp4 (1920x1080) [718.2 MB] || 13778_Anemone_Eruption_1080.mp4 (1920x1080) [220.6 MB] || 13778_Anemone_Eruption_Best_1080.webm (1920x1080) [16.0 MB] || AnemoneEruption_SRT_Captions.en_US.srt [500 bytes] || AnemoneEruption_SRT_Captions.en_US.vtt [513 bytes] || ", "hits": 88 }, { "id": 13712, "url": "https://svs.gsfc.nasa.gov/13712/", "result_type": "Produced Video", "release_date": "2020-11-30T11:00:00-05:00", "title": "Landsat 9: Continuing the Legacy series", "description": "Five decades ago, NASA and the US Geological Society launched a satellite to monitor Earth’s land from space. It was the beginning of a legacy. The Apollo era had given us our first looks at Earth from space and inspired the idea of regularly collecting images of our planet. The first Landsat — originally known as the Earth Resources Technology Satellite, or ERTS — rocketed into space in 1972. Since then, there have been eight Landsats and we’re preparing to launch number nine.The Landsat legacy stretches far and wide. Using visible and infrared light, Landsat helps track the health of crops, shows ocean pollution, and tracks coral reefs, icebergs and more. Thanks to sensor that can record wavelengths beyond what we can see with our eyes, Landsat can record vital information about Earth's surface.Narrated by the actor Marc Evan Jackson, who played a Landsat scientist in the movie Kong: Skull Island (2017), this series of videos tells the story of Landsat 9. From the birth of the Landsat program to the present preparations for launching Landsat 9 and even a look to the future with Landsat NeXt. || ", "hits": 54 }, { "id": 13751, "url": "https://svs.gsfc.nasa.gov/13751/", "result_type": "Produced Video", "release_date": "2020-11-04T11:00:00-05:00", "title": "NASA Missions Team Up to Study Unique Magnetar Outburst", "description": "On April 28, space- and ground-based observatories detected powerful, simultaneous X-ray and radio bursts from a source in our galaxy. Watch to see how this unique event helps solve the longstanding puzzle of fast radio bursts observed in other galaxies.Credit: NASA's Goddard Space Flight CenterMusic: \"Jupiter's Eye\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Magnetar_FRB_Still.jpg (1920x1080) [535.5 KB] || Magnetar_FRB_Still_searchweb.png (320x180) [65.5 KB] || Magnetar_FRB_Still_thm.png (80x40) [4.8 KB] || 13751_Magnetar_FRB_Best_1080.webm (1920x1080) [25.7 MB] || 13751_Magnetar_FRB_1080.mp4 (1920x1080) [237.4 MB] || 13751_Magnetar_FRB_Best_1080.mp4 (1920x1080) [741.8 MB] || Fast_Radio_Burst_SRT_Captions.en_US.srt [4.5 KB] || Fast_Radio_Burst_SRT_Captions.en_US.vtt [4.5 KB] || 13751_Magnetar_FRB_ProRes_1920x1080_2997.mov (1920x1080) [3.2 GB] || ", "hits": 439 }, { "id": 13714, "url": "https://svs.gsfc.nasa.gov/13714/", "result_type": "Produced Video", "release_date": "2020-09-15T13:00:00-04:00", "title": "Solar Cycle 25 Is Here. NASA, NOAA Scientists Explain What This Means", "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.Click here for the NOAA press kit.Listen to the media telecon.Participants:• Lisa Upton, Co-chair, Solar Cycle 25 Prediction Panel; Solar Physicist, Space Systems Research Corporation• Doug Biesecker, Solar Physicist, NOAA’s Space Weather Prediction Center; Co-chair, Solar Cycle 25 Prediction Panel• Elsayed Talaat, Director, Office of Projects, Planning and Analysis; NOAA’s Satellite and Information Service • Lika Guhathakurta, Heliophysicist, Heliophysics Division, NASA Headquarters • Jake Bleacher, Chief Exploration Scientist, NASA Human Exploration and Operations Mission Directorate || ", "hits": 374 }, { "id": 13698, "url": "https://svs.gsfc.nasa.gov/13698/", "result_type": "Produced Video", "release_date": "2020-08-20T00:00:00-04:00", "title": "Small Flare Seen on the Sun, August 16, 2020", "description": "NASA’s Solar Dynamics Observatory observes the Aug. 16, 2020, B-class flare at 131, 171, and 193 angstroms. Credit: NASA/SDO || SDO_8-16-2020_Eruption_Triptych_ProRes_1080.00121_print.jpg (1024x576) [196.4 KB] || SDO_8-16-2020_Eruption_Triptych_ProRes_1080.00121_searchweb.png (320x180) [91.4 KB] || SDO_8-16-2020_Eruption_Triptych_ProRes_1080.00121_thm.png (80x40) [6.2 KB] || SDO_8-16-2020_Eruption_Triptych_ProRes_1080.mov (1920x1080) [129.8 MB] || SDO_8-16-2020_Eruption_Triptych_1080.mp4 (1920x1080) [10.1 MB] || SDO_8-16-2020_Eruption_Triptych_1080.webm (1920x1080) [1.0 MB] || ", "hits": 113 }, { "id": 20320, "url": "https://svs.gsfc.nasa.gov/20320/", "result_type": "Animation", "release_date": "2020-08-14T09:00:00-04:00", "title": "Solar Energetic Particles", "description": "The Sun goes through phases of strong activity, during which eruptions can occur. Such eruptions can have multiple components, including X rays, coronal mass ejection plasma, and solar energetic particles – bursts or events of fast-moving particles. These events can occur suddenly and have the potential to rapidly change the radiation environment of wide swaths of the inner solar system where they may create hazardous conditions. Not only are such conditions dangerous for humans in space, but the intense ionizing radiation can also affect the interior of spacecraft, including sensitive electronics. Solar energetic particles can reach all regions of near-Earth space, including the lunar surface, with the exception of low-altitude and low-latitude Earth orbit, where the Earth’s magnetic field is strong enough to form a protective barrier. || ", "hits": 299 }, { "id": 13614, "url": "https://svs.gsfc.nasa.gov/13614/", "result_type": "Produced Video", "release_date": "2020-05-18T11:00:00-04:00", "title": "40 Years of Forest Recovery", "description": "The long record of Landsat data (since 1972) is helping scientists Sean Healey and Zhiqiang Yang of the Rocky Mountain Research Station (U.S. Forest Service) study the long-term impact of the May 18, 1980, eruption of Mount St. Helens. With Landsat data for 8 years before the eruption, and 40 years since, they have calculated the percent tree cover for each year, watching as vegetation grows back.Music: The Waiting Room by Sam Dodson [PRS], published by Atmosphere Music Ltd [PRS]; Inner Strength by Brava [SGAE], Dsilence [SGAE], Input [SGAE] , Output [SGAE], published by El Murmullo Sarao [SGAE], Universal Sarao [SGAE], Some Assembly by Kyle Fredrickson [ASCAP] and Taylor Alexander Locke [BMI], published by Killer Tracks [BMI], Soundcast Music [SESAC], and Light From Dark by Adam Salkeld [PRS] and Neil Pollard [PRS], published by Atmosphere Music Ltd [PRS], all available from Universal Production Music.Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 13614_Mt_St_Helens_Landsat.png (1920x1080) [4.0 MB] || 13614_Mt_St_Helens_print.png (1920x1080) [3.5 MB] || 13614_Mt_St_Helens_print_print.jpg (1024x576) [287.9 KB] || 13614_Mt_St_Helens_print_searchweb.png (320x180) [106.3 KB] || 13614_Mt_St_Helens_print_thm.png (80x40) [7.4 KB] || 13614_Mt_St_Helens_prores.mov (1920x1080) [11.9 GB] || 13614_Mt_St_Helens_youtube.mp4 (1920x1080) [411.3 MB] || 13614_Mt_St_Helens_facebook.mp4 (1920x1080) [354.9 MB] || 13614_Mt_St_Helens_twitter.mp4 (1504x846) [139.3 MB] || 13614_Mt_St_Helens_youtube.webm (1920x1080) [47.9 MB] || 13614_Mt_St_Helens-captions.en_US.srt [8.6 KB] || 13614_Mt_St_Helens-captions.en_US.vtt [8.6 KB] || ", "hits": 54 }, { "id": 13578, "url": "https://svs.gsfc.nasa.gov/13578/", "result_type": "Produced Video", "release_date": "2020-04-13T11:00:00-04:00", "title": "NASA Missions Study a Nova's Shock Waves", "description": "NASA’s Fermi and NuSTAR space telescopes, together with another satellite named BRITE-Toronto, are providing new insights into a nova explosion that erupted in 2018. Detailed measurements of bright flares in the explosion clearly show that shock waves power most of the nova's visible light. Credit: NASA’s Goddard Space Flight CenterMusic: \"Scientist\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || novastill01.jpg (3840x2160) [1.1 MB] || novastill01_searchweb.png (320x180) [76.8 KB] || novastill01_thm.png (80x40) [6.7 KB] || 13578_Nova_Carinae_Best.webm (1920x1080) [13.8 MB] || novastill01.tif (3840x2160) [31.7 MB] || 13578_Nova_Carinae_SRT_Captions.en_US.srt [2.2 KB] || 13578_Nova_Carinae_SRT_Captions.en_US.vtt [2.2 KB] || 13578_Nova_Carinae_Best.mp4 (1920x1080) [319.4 MB] || 13578_Nova_Carinae_Good.mp4 (1920x1080) [129.0 MB] || 13578_Nova_Carinae_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 130 }, { "id": 31138, "url": "https://svs.gsfc.nasa.gov/31138/", "result_type": "Hyperwall Visual", "release_date": "2020-03-13T00:00:00-04:00", "title": "2019 AGU Hyperwall Presentations: Opening Night Talks and Data Visualization Winners", "description": "Opeing NASA AGU 2019 ExhibtThis video is also available on our YouTube channel. || Paula_Bontempi_SMD_open.00001_print.jpg (1024x576) [81.7 KB] || Paula_Bontempi_SMD_open.00001_searchweb.png (320x180) [65.9 KB] || Paula_Bontempi_SMD_open.00001_thm.png (80x40) [5.4 KB] || Paula_Bontempi_SMD_open.mp4 (1280x720) [87.8 MB] || Paula_Bontempi_SMD_open.webm (1280x720) [62.1 MB] || Paula_Bontempi_SMD_openCOR.en_US.srt [10.9 KB] || Paula_Bontempi_SMD_openCOR.en_US.vtt [10.9 KB] || ", "hits": 21 }, { "id": 13556, "url": "https://svs.gsfc.nasa.gov/13556/", "result_type": "Produced Video", "release_date": "2020-02-14T03:00:00-05:00", "title": "Astrophysics Valentines", "description": "Download our astrophysics-themed valentines! || Will you still love me tomorrow? Many cosmic couples, from binary stars to gravitationally bound galaxies, spend millions or even billions of years together — but some age more gracefully than others. Credit: NASA's Goddard Space Flight Center || LoveMeTomorrow.gif (540x304) [2.4 MB] || ", "hits": 139 }, { "id": 31106, "url": "https://svs.gsfc.nasa.gov/31106/", "result_type": "Hyperwall Visual", "release_date": "2020-02-12T00:00:00-05:00", "title": "Fires Light Up Mount Vesuvius", "description": "Wildfires on Mount Vesuvius || volcano-vesuvius_print.jpg (1024x576) [98.9 KB] || volcano-vesuvius.png (3840x2160) [3.5 MB] || volcano-vesuvius_searchweb.png (320x180) [66.4 KB] || volcano-vesuvius_thm.png (80x40) [5.3 KB] || fires-light-up-mount-vesuvius.hwshow [285 bytes] || ", "hits": 41 }, { "id": 13535, "url": "https://svs.gsfc.nasa.gov/13535/", "result_type": "Produced Video", "release_date": "2020-02-07T14:30:00-05:00", "title": "Solar Orbiter Science Press Briefing", "description": "NASA and the European Space Agency (ESA) will present Solar Orbiter, the ESA/NASA mission to the Sun, during a science press briefing on Friday, Feb. 7. 2020, at 2.30 p.m. EST. Solar Orbiter will observe the Sun with high spatial resolution telescopes and capture observations in the environment directly surrounding the spacecraft to create a one-of-a-kind picture of how the Sun can affect the space environment throughout our solar system. The spacecraft also will provide the first-ever images of the Sun’s poles and the never-before-observed magnetic environment there, which helps drive the Sun’s 11-year solar cycle and its periodic outpouring of solar storms.The teleconference audio will stream live at:https://www.nasa.gov/liveParticipants include:European Space Agency• Daniel Müller, Solar Orbiter Project Scientist• Günther Hasinger, Director of ScienceNASA• Nicky Fox, Heliophysics Division Director, NASA HQ• Thomas Zurbuchen, Associate Administrator for the Science Mission Directorate, NASA HQ || ", "hits": 56 }, { "id": 40409, "url": "https://svs.gsfc.nasa.gov/gallery/fermi-stills/", "result_type": "Gallery", "release_date": "2020-01-22T00:00:00-05:00", "title": "Fermi Stills", "description": "A collection of Fermi-related still images, illustrations, graphics and short clips.", "hits": 203 }, { "id": 13422, "url": "https://svs.gsfc.nasa.gov/13422/", "result_type": "Produced Video", "release_date": "2019-12-17T10:00:00-05:00", "title": "A New Kind of Explosion on the Sun", "description": "Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Credit: Light Hearted Angst by Dewey Dellay || ReconnThumb.jpg (1920x1080) [156.1 KB] || ReconnThumb_searchweb.png (320x180) [100.6 KB] || ReconnThumb_thm.png (80x40) [7.3 KB] || ForcedReconnV2_Twitter.mp4 (1920x1080) [29.6 MB] || ForcedReconnV2.webm (1920x1080) [14.8 MB] || ForcedReconnV2.mp4 (1920x1080) [134.9 MB] || ForcedReconnV2_FB.mp4 (1920x1080) [155.5 MB] || ForcedReconnV2_YouTube.mp4 (1920x1080) [207.3 MB] || ForcedReconnV2.en_US.srt [2.6 KB] || ForcedReconnV2.en_US.vtt [2.6 KB] || ForcedReconnV2.mov (1920x1080) [1.7 GB] || ", "hits": 76 }, { "id": 13494, "url": "https://svs.gsfc.nasa.gov/13494/", "result_type": "Produced Video", "release_date": "2019-12-11T13:00:00-05:00", "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission", "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ", "hits": 150 }, { "id": 13301, "url": "https://svs.gsfc.nasa.gov/13301/", "result_type": "Produced Video", "release_date": "2019-08-29T12:00:00-04:00", "title": "Photon Phriday", "description": "Photon Phriday is a weekly look at what ICESat-2 is measuring as it orbits the Earth. || ", "hits": 69 }, { "id": 13244, "url": "https://svs.gsfc.nasa.gov/13244/", "result_type": "Produced Video", "release_date": "2019-07-01T09:55:00-04:00", "title": "Hubble’s Brand New Image of Eta Carinae", "description": "In the mid-1800s, mariners sailing the southern seas navigated at night by a brilliant star in the constellation Carina. The star, named Eta Carinae, was the second brightest star in the sky for more than a decade. Those mariners could hardly have imagined that by the mid-1860s the brilliant orb would no longer be visible. Eta Carinae was enveloped by a cloud of dust ejected during a violent outburst named “The Great Eruption.” Because of Eta Carinae's violent history, astronomers have kept watch over its activities. Although Hubble has monitored the volatile superstar for 25 years, it still is uncovering new revelations. Using Hubble to map the ultraviolet-light glow of magnesium embedded in warm gas, astronomers were surprised to discover the gas in places they had not seen it before. For more information, visit https://nasa.gov/hubble Credit: NASA's Goddard Space Flight Center/Paul Morris.Music credits: \"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS]; Killer Tracks Production Music || ", "hits": 110 }, { "id": 30977, "url": "https://svs.gsfc.nasa.gov/30977/", "result_type": "Hyperwall Visual", "release_date": "2019-03-29T00:00:00-04:00", "title": "Nighttime Views of the 2018 Kilauea Eruption", "description": "An animation of Landsat-8 truecolor and nighttime imagery shows the prograssion of the East Rift Zone eruption. || kilauea_2018_east_rift_zone_20180712_print.jpg (1024x576) [70.6 KB] || kilauea_2018_east_rift_zone_20180712.png (3840x2160) [1.8 MB] || kilauea_2018_east_rift_zone_20180712_searchweb.png (320x180) [45.1 KB] || kilauea_2018_east_rift_zone_20180712_thm.png (80x40) [3.8 KB] || kilauea_2018_east_rift_zone_720p.mp4 (1280x720) [2.7 MB] || kilauea_2018_east_rift_zone_720p.webm (1280x720) [1.9 MB] || ", "hits": 85 }, { "id": 4726, "url": "https://svs.gsfc.nasa.gov/4726/", "result_type": "Visualization", "release_date": "2019-03-27T00:00:00-04:00", "title": "New Island forms in Tonga (Updated)", "description": "This visualization shows the evolution Tonga's new island between January 2015 and March 2018. || Tonga_evolutn.1300_print.jpg (1024x576) [129.1 KB] || Tonga_evolutn.1300_searchweb.png (320x180) [84.2 KB] || Tonga_evolutn.1300_web.png (320x180) [84.2 KB] || Tonga_evolutn_Wcredits_1080p30.mp4 (1920x1080) [43.0 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4 (1920x1080) [17.9 MB] || Tonga_evolutn_Wcredits_1080p30.webm (1920x1080) [5.8 MB] || Tonga_evolutn_Wcredits_2160p30_h265.mp4 (3840x2160) [50.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Tonga_evolutn_Wcredits_2160p30.mp4 (3840x2160) [140.4 MB] || Tonga_evolutn_Wcredits_1080p30_h265.mp4.hwshow || ", "hits": 194 }, { "id": 40359, "url": "https://svs.gsfc.nasa.gov/gallery/sdostillsand-graphics/", "result_type": "Gallery", "release_date": "2018-09-13T10:02:59-04:00", "title": "SDO: Stills and Graphics", "description": "No description available.", "hits": 186 }, { "id": 40361, "url": "https://svs.gsfc.nasa.gov/gallery/sdoproduced-videos/", "result_type": "Gallery", "release_date": "2018-09-13T10:02:58-04:00", "title": "SDO: Produced Videos", "description": "No description available.", "hits": 551 }, { "id": 40357, "url": "https://svs.gsfc.nasa.gov/gallery/sdo4k-content/", "result_type": "Gallery", "release_date": "2018-09-13T09:22:28-04:00", "title": "SDO: 4k Content", "description": "Since 2010, the Solar Dynamics Observatory has taken 60 million images of the sun and 2 comets. Here are a few of our favorites.", "hits": 492 }, { "id": 40360, "url": "https://svs.gsfc.nasa.gov/gallery/sdosolar-events/", "result_type": "Gallery", "release_date": "2018-09-13T09:22:27-04:00", "title": "SDO: Solar Events", "description": "No description available.", "hits": 629 }, { "id": 40358, "url": "https://svs.gsfc.nasa.gov/gallery/sdopresentation-resources/", "result_type": "Gallery", "release_date": "2018-09-07T00:00:00-04:00", "title": "SDO: Presentation Resources", "description": "No description available.", "hits": 54 }, { "id": 40355, "url": "https://svs.gsfc.nasa.gov/gallery/sdo/", "result_type": "Gallery", "release_date": "2018-08-31T00:00:00-04:00", "title": "SDO – Solar Dynamics Observatory", "description": "Since its launch on Feb. 11, 2010, the Solar Dynamics Observatory (SDO) has studied the solar atmosphere to help us understand the Sun’s influence on Earth. Every 12 seconds, SDO images the Sun in 10 wavelengths of ultraviolet light, each of which reveals different solar features. These images help us explain where the Sun's energy comes from, how the inside of the Sun works, and how the Sun’s atmosphere stores and releases energy in dramatic eruptions that can influence Earth.\n\nLearn more: https://science.nasa.gov/mission/sdo/", "hits": 901 }, { "id": 13028, "url": "https://svs.gsfc.nasa.gov/13028/", "result_type": "Produced Video", "release_date": "2018-08-08T00:00:00-04:00", "title": "Parker Solar Probe Media Telecons", "description": "This is a resource page for the media teleconferences on August 8, 2018. || ", "hits": 80 }, { "id": 12989, "url": "https://svs.gsfc.nasa.gov/12989/", "result_type": "Produced Video", "release_date": "2018-07-03T11:00:00-04:00", "title": "Superstar Eta Carinae Shoots Cosmic Rays", "description": "Zoom into Eta Carinae, where the outflows of two massive stars collide and shoot accelerated particles cosmic rays into space.Credit: NASA’s Goddard Space Flight Center Music: \"Expectant Aspect\" from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || Eta_Car_CR_Still.jpg (1920x1080) [307.1 KB] || Eta_Car_CR_Still_print.jpg (1024x576) [127.9 KB] || Eta_Car_CR_Still_searchweb.png (320x180) [98.2 KB] || Eta_Car_CR_Still_thm.png (80x40) [7.3 KB] || 12989_Eta_Car_CosmicRay_ProRes_1080.webm (1920x1080) [16.1 MB] || 12989_Eta_Car_CosmicRay_1080.m4v (1920x1080) [155.6 MB] || 12989_Eta_Car_CosmicRay_1080.mp4 (1920x1080) [234.6 MB] || 12989_Eta_Car_CosmicRay_1080p.mov (1920x1080) [311.6 MB] || 12989_Eta_Car_CosmicRay_SRT_Captions.en_US.srt [2.0 KB] || 12989_Eta_Car_CosmicRay_SRT_Captions.en_US.vtt [2.0 KB] || 12989_Eta_Car_CosmicRay_ProRes_1080.mov (1920x1080) [2.1 GB] || ", "hits": 90 }, { "id": 4659, "url": "https://svs.gsfc.nasa.gov/4659/", "result_type": "Visualization", "release_date": "2018-06-27T00:00:00-04:00", "title": "Incredible Solar Flare, Prominence Eruption and CME Event (hydrogen alpha filter)", "description": "This movie is generated from imagery collected by the NSO GONG network of solar observatories. It is not time-synchronized to the related observations by the Solar Dynamics Observatory (SDO). || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_print.jpg (1024x576) [25.1 KB] || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_searchweb.png (320x180) [20.9 KB] || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_thm.png (80x40) [2.3 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || BBSO_Halpha_2011JuneUh_HD1080i_p30.mp4 (1920x1080) [2.8 MB] || BBSO_Halpha_2011JuneUh_HD1080i_p30.webm (1920x1080) [1.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || BBSO_Halpha_2011JuneUh_2160p30.mp4 (3840x2160) [11.4 MB] || BBSO_Halpha_2011JuneUh_HD1080i_p30.mp4.hwshow [200 bytes] || ", "hits": 68 }, { "id": 4635, "url": "https://svs.gsfc.nasa.gov/4635/", "result_type": "Visualization", "release_date": "2018-06-15T11:00:00-04:00", "title": "Visualizations of Hunga Tonga Hunga Ha'apai and the Martian Landscape", "description": "In early 2015, a volcanic eruption in the Kingdom of Tonga created a new island informally known as Hunga Tonga Hunga Ha'apai (HTHH). The subsequent evolution of the new island was previously described in \"The Birth of a New Island\" available here. Below are additional visualizations, including an updated view of the island's appearance in March 2018 as well as some visualizations of the martian surface. Results of this study can enhance our understanding of numerous small volcanic landforms on Mars whose formation may have been in shallow-water environments during epochs when persistent surface water was present.The complete visualization of \"Using Earth to understand how water may have affected volcanoes on Mars\" is available here.Learn more about the evolution of Earth's newest island and how it could reveal new information about the presence of water on Mars: https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017GL076621 || ", "hits": 90 }, { "id": 30962, "url": "https://svs.gsfc.nasa.gov/30962/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "Sulfur Dioxide Leaks from Kilauea", "description": "This series of images, created using data from the Ozone Mapping Profiler Suite (OMPS) sensor on the Suomi National Polar-orbiting Partnership (NPP) satellite, shows elevated concentrations of sulfur dioxide from Hawaii's Kilauea volcano on May 5, 2018. || hawaii_omp_so2.png (1920x1080) [299.9 KB] || hawaii_omp_so2_print.jpg (1024x576) [49.1 KB] || hawaii_omp_so2_searchweb.png (320x180) [31.7 KB] || hawaii_omp_so2_thm.png (80x40) [3.7 KB] || sulfur-dioxide-leaks-from-kilauea-data.hwshow [290 bytes] || ", "hits": 41 }, { "id": 30963, "url": "https://svs.gsfc.nasa.gov/30963/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "Probing Kilauea’s Plume", "description": "These images, created using data from the Multi-angle Imaging Spectroradiometer (MISR) on Terra, show the height of the sulfur-rich plume from Hawaii's Kilauea on May 6, 2018. || probing_plume.png (1920x1080) [1.7 MB] || probing_plume_print.jpg (1024x576) [139.0 KB] || probing_plume_searchweb.png (320x180) [78.6 KB] || probing_plume_thm.png (80x40) [6.0 KB] || probing-kilaueas-plume.hwshow [272 bytes] || ", "hits": 24 }, { "id": 30964, "url": "https://svs.gsfc.nasa.gov/30964/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "Kilauea Continues to Erupt", "description": "On May 14, 2018, at 10:41 AM local time (20:41 Universal Time), the Operational Land Imager (OLI) on Landsat 8 acquired a natural-color image of Hawaii’s Kilauea volcano. || kilauea_continues_print.jpg (1024x682) [280.7 KB] || kilauea_continues.png (4860x3240) [26.3 MB] || kilauea_continues_searchweb.png (320x180) [123.7 KB] || kilauea_continues_thm.png (80x40) [8.0 KB] || kilauea-continues-to-erupt.hwshow [284 bytes] || ", "hits": 80 }, { "id": 30965, "url": "https://svs.gsfc.nasa.gov/30965/", "result_type": "Hyperwall Visual", "release_date": "2018-05-31T00:00:00-04:00", "title": "The Infrared Glow of Kilauea’s Lava Flows", "description": "The Operational Land Imager (OLI) on Landsat 8 acquired the data for this false-color view of the lava flow as it appeared on the night of May 23, 2018. || IR_leilani_print.jpg (1024x574) [95.3 KB] || IR_leilani.png (4104x2304) [3.5 MB] || IR_leilani_searchweb.png (320x180) [44.9 KB] || IR_leilani_thm.png (80x40) [2.7 KB] || the-infrared-glow-of-kilaueas-lava-flows.hwshow [284 bytes] || ", "hits": 54 }, { "id": 30973, "url": "https://svs.gsfc.nasa.gov/30973/", "result_type": "Hyperwall Visual", "release_date": "2018-05-27T00:00:00-04:00", "title": "Aoba (Ambae) Volcano Eruption, Vanuatu", "description": "Activity for Aoba (Ambae) volcano has increased in recent months and is now in a minor eruption state. A restricted area of risk which is 3km around the active vent has been established as the volcano began to become more active in March and early April 2018. At that time the volcano began to emit more and sustained volcanic ash or/ and gases. Vanuatu’s Council of Ministers has declared a state of emergency on Ambae due to the heavy ash fall which has contaminated water and food supplies for the island’s nearly 11,000 inhabitants, who are in the process of being evacuated from the island. || ", "hits": 152 }, { "id": 12890, "url": "https://svs.gsfc.nasa.gov/12890/", "result_type": "Produced Video", "release_date": "2018-03-09T10:00:00-05:00", "title": "Solar Highlights of 2018", "description": "3 NASA Satellite Recreate Solar Eruption in 3-DUsing data from three different satellites, scientists have developed new models that recreate, in 3-D, CMEs and shocks, separately. This movie illustrates the recreation of a CME and shock that erupted from the Sun on March 7, 2011. The pink lines show the CME structure and the yellow lines show the structure of the shock - a side effect of the CME that can spark space weather events around Earth.Scientists: Ryun Kwon (George Mason University), Angelos Vourlidas (The Johns Hopkins University Applied Physics Laboratory)Image credits: NASA’s Goddard Space Flight Center/GMU/APL/Joy NgWatch this video on the NASA.gov Video YouTube channel.Find this feature on NASA.gov. || 3DCME.00001_print.jpg (1024x576) [77.7 KB] || 3DCME.00001_searchweb.png (320x180) [52.1 KB] || 3DCME.00001_web.png (320x180) [52.1 KB] || 3DCME.00001_thm.png (80x40) [5.3 KB] || PRORES_B-ROLL_12890_3DCME_prores.mov (1280x720) [218.7 MB] || 3DCME_Prores.mov (1920x1080) [416.9 MB] || 3DCME.mp4 (1920x1080) [44.6 MB] || 12890_3DCME_appletv.m4v (1280x720) [24.5 MB] || NASA_TV_12890_3DCME.mpeg (1280x720) [102.5 MB] || LARGE_MP4_12890_3DCME_large.mp4 (1920x1080) [31.2 MB] || 3DCME.webm (1920x1080) [3.1 MB] || GSFC_20180309_CME_m12890_3DCME.en_US.vtt [64 bytes] || 12890_3DCME_ipod_sm.mp4 (320x240) [7.2 MB] || ", "hits": 32 }, { "id": 12542, "url": "https://svs.gsfc.nasa.gov/12542/", "result_type": "Produced Video", "release_date": "2018-01-08T12:00:00-05:00", "title": "CATS Eyes on the Atmosphere", "description": "See the atmosphere through CATS's eyes. || CATS_calbuco_09.3535_1024x576.jpg (1024x576) [67.5 KB] || CATS_calbuco_09.3535_print.jpg (1024x576) [74.0 KB] || CATS_calbuco_09.3535_searchweb.png (320x180) [40.5 KB] || CATS_calbuco_09.3535_thm.png (80x40) [3.4 KB] || CATS_calbuco_09.3535.tif (3840x2160) [5.4 MB] || ", "hits": 26 }, { "id": 12800, "url": "https://svs.gsfc.nasa.gov/12800/", "result_type": "Produced Video", "release_date": "2017-12-11T16:00:00-05:00", "title": "The Birth of a New Island: Press Materials", "description": "Music: Fountain by Mailcoat Sheppard; Data Visions by Pike; Guilty Curiosity by Brice Davoli; Concerning Nymphs by Hammond Roberts. Complete transcript available. || NewTongaIsland_Long_print.jpg (1024x573) [107.5 KB] || NewTongaIsland_Long.png (2552x1429) [3.6 MB] || NewTongaIsland_Long_searchweb.png (320x180) [99.0 KB] || NewTongaIsland_Long_thm.png (80x40) [7.8 KB] || FACEBOOK_720_NewTongaIsland_Long_facebook_720.webm (1280x720) [43.3 MB] || TWITTER_720_NewTongaIsland_Long_twitter_720.mp4 (1280x720) [96.7 MB] || NewTongaIsland_Long_large.mp4 (1920x1080) [404.5 MB] || FACEBOOK_720_NewTongaIsland_Long_facebook_720.mp4 (1280x720) [504.5 MB] || YOUTUBE_720_NewTongaIsland_Long_youtube_720.mp4 (1280x720) [660.6 MB] || YOUTUBE_1080_NewTongaIsland_Long_youtube_1080.mp4 (1920x1080) [694.2 MB] || TongaNewIslandCaptions.en_US.srt [7.9 KB] || TongaNewIslandCaptions.en_US.vtt [7.8 KB] || CH28_NewTongaIsland_Long_ch28.mov (1280x720) [3.7 GB] || NewTongaIsland_Long.mov (1920x1080) [10.5 GB] || ", "hits": 222 }, { "id": 4602, "url": "https://svs.gsfc.nasa.gov/4602/", "result_type": "Visualization", "release_date": "2017-12-11T10:00:00-05:00", "title": "New island forms in Tonga", "description": "This visualization shows the change in the island of Hunga Tonga Hunga Ha'apa between January 2015 and September 2017.This video is also available on our YouTube channel. || Tonga_v60_vis.0780_print.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_searchweb.png (320x180) [76.8 KB] || Tonga_v60_vis.0780_thm.png (80x40) [6.0 KB] || new_island_vis (1920x1080) [0 Item(s)] || Tonga_v60_vis_1080p30.mp4 (1920x1080) [33.3 MB] || Tonga_v60_vis_1080p30.webm (1920x1080) [5.1 MB] || Tonga_4k_final2_1080p30.mp4 (1920x1080) [34.3 MB] || new_island_vis (3840x2160) [0 Item(s)] || Tonga_4k_final2_2160p30.mp4 (3840x2160) [52.0 MB] || Tonga_v60_vis_1080p30.mp4.hwshow [187 bytes] || ", "hits": 110 }, { "id": 40339, "url": "https://svs.gsfc.nasa.gov/gallery/visualization-principles/", "result_type": "Gallery", "release_date": "2017-11-06T00:00:00-05:00", "title": "The Curious World of Scientific Visualization", "description": "Explore data brought to life by NASA’s artists and scientists\r\rData Brought to Life\rData is only as powerful as our ability to make sense of it. The right tools can help us find meaning in a trove of information and experience the wonder in it. When artists and scientists work in concert, they unearth stories within datasets and push the boundaries of knowledge. This collaboration is both a creative process and a mathematical one. Scientific visualization is not a mere translation of numbers into pictures: shapes and colors breathe life into real scientific data, allowing us to see patterns and complexities that were once invisible or unknown. The visualization itself becomes a vehicle for scientific inquiry, capturing the curiosity of both artist and scientist. When shared with the world, these data-driven artworks inspire as much as they educate and entertain. Scientific visualization reminds us of the beauty in understanding, and it is a means of discovery all its own. \r\rScientific Visualization at NASA\rAt NASA’s Goddard Space Flight Center, scientists work alongside a team of artists to extend their research into the visual space. The Scientific Visualization Studio creates animations and videos that showcase the latest discoveries in Earth and space sciences. These visualizations are both insightful tools for the NASA research community and accessible science stories designed to be enjoyed by people of all walks of life. As one of NASA’s leading outreach efforts, the Scientific Visualization Studio empowers scientists to share their work with as wide an audience as possible, in the most creative and engaging way possible. \r", "hits": 259 }, { "id": 12740, "url": "https://svs.gsfc.nasa.gov/12740/", "result_type": "Produced Video", "release_date": "2017-10-16T10:00:00-04:00", "title": "Doomed Neutron Stars Create Blast of Light and Gravitational Waves", "description": "This animation captures phenomena observed over the course of nine days following the neutron star merger known as GW170817, detected on Aug. 17, 2017. They include gravitational waves (pale arcs), a near-light-speed jet that produced gamma rays (magenta), expanding debris from a kilonova that produced ultraviolet (violet), optical and infrared (blue-white to red) emission, and, once the jet directed toward us expanded into our view from Earth, X-rays (blue). Credit: NASA's Goddard Space Flight Center/CI LabMusic: \"Exploding Skies\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Neutron_Star_Merger_Still_2_new_1080.png (1920x1080) [2.5 MB] || Neutron_Star_Merger_Still_2_new_1080.jpg (1920x1080) [167.3 KB] || Neutron_Star_Merger_Still_2_new_print.jpg (1024x576) [50.4 KB] || Neutron_Star_Merger_Still_2_new.png (3840x2160) [7.7 MB] || Neutron_Star_Merger_Still_2_new.jpg (3840x2160) [1.0 MB] || Neutron_Star_Merger_Still_2_new_thm.png (80x40) [4.4 KB] || Neutron_Star_Merger_Still_2_new_searchweb.png (320x180) [51.4 KB] || 12740_NS_Merger_Update_1080.m4v (1920x1080) [50.3 MB] || 12740_NS_Merger_Update_H264_1080.mp4 (1920x1080) [96.9 MB] || 12740_NS_Merger_Update_1080p.mov (1920x1080) [101.9 MB] || NS_Merger_SRT_Captions.en_US.srt [417 bytes] || NS_Merger_SRT_Captions.en_US.vtt [399 bytes] || 12740_NS_Merger_4k_Update.webm (3840x2160) [10.0 MB] || 12740_NS_Merger_4k_Update_H264.mp4 (3840x2160) [254.9 MB] || 12740_NS_Merger_4k_Update_H264.mov (3840x2160) [516.7 MB] || 12740_NS_Merger_4k_Update_ProRes_3840x2160_5994.mov (3840x2160) [5.1 GB] || 12740_NS_Merger_4k_Update_H264.hwshow [90 bytes] || ", "hits": 821 }, { "id": 30162, "url": "https://svs.gsfc.nasa.gov/30162/", "result_type": "Hyperwall Visual", "release_date": "2017-09-01T12:00:00-04:00", "title": "Devastation and Recovery of Mt. St. Helens", "description": "In the nearly four decades since the eruption (1980), Mt. St. Helens has given scientists an unprecedented opportunity to witness the steps through which life reclaims a devastated landscape. The scale of the eruption and the beginning of reclamation in the Mt. St. Helens blast zone are documented in this series of images between 1979 and 2017. The older images are false-color (vegetation is red). Not surprisingly, the first noticeable recovery (late 1980s) takes place in the northwestern quadrant of the blast zone, farthest from the volcano. It is another decade (late 1990s) before the terrain east of Spirit Lake is considerably greener. By the end of the series, the only area (beyond the slopes of the mountain itself) that remains conspicuously bare at the scale of these images is the Pumice Plain. || ", "hits": 74 }, { "id": 4352, "url": "https://svs.gsfc.nasa.gov/4352/", "result_type": "Visualization", "release_date": "2017-08-20T10:00:00-04:00", "title": "Incredible Solar Flare, Prominence Eruption and CME Event (SDO/HMI visible light)", "description": "These movies present the six hour interval around the event, a one minute per animation frame. || MonsterFilament_HMI_stand.HD1080i.00100_print.jpg (1024x576) [40.8 KB] || MonsterFilament_HMI_stand.HD1080i.00100_searchweb.png (320x180) [21.8 KB] || MonsterFilament_HMI_stand.HD1080i.00100_thm.png (80x40) [2.7 KB] || MonsterFilament_HMI_stand.HD1080i.00100_web.png (320x180) [21.8 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || MonsterFilament_HMI.HD1080i_p30.mp4 (1920x1080) [12.1 MB] || MonsterFilament_HMI.HD1080i_p30.webm (1920x1080) [1.2 MB] || MonsterFilament_HMI.HD1080i_p30.mp4.hwshow [197 bytes] || ", "hits": 114 }, { "id": 11797, "url": "https://svs.gsfc.nasa.gov/11797/", "result_type": "Produced Video", "release_date": "2017-08-11T10:00:00-04:00", "title": "Sun Shreds Its Own Eruption", "description": "Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music credit: Game Show Sphere 01 by by Anselm Kreuzer || fluxropethumb.jpg (1920x1080) [87.3 KB] || fluxropethumb_searchweb.png (320x180) [79.1 KB] || fluxropethumb_thm.png (80x40) [5.7 KB] || YOUTUBE_1080-11797_Shredding_a_Solar_EruptionV3_youtube_1080.mp4 (1920x1080) [193.2 MB] || APPLE_TV-11797_Shredding_a_Solar_EruptionV3_appletv.m4v (1280x720) [69.6 MB] || LARGE_MP4-11797_Shredding_a_Solar_EruptionV3_large.mp4 (1920x1080) [132.5 MB] || NASA_TV-11797_Shredding_a_Solar_EruptionV3.mpeg (1280x720) [440.3 MB] || YOUTUBE_HQ-11797_Shredding_a_Solar_EruptionV3_youtube_hq.mov (1920x1080) [808.6 MB] || PRORES_B-ROLL-11797_Shredding_a_Solar_EruptionV3_prores.mov (1280x720) [1.7 GB] || 11797_Shredding_a_Solar_EruptionV3.mov (1920x1080) [3.3 GB] || 11797_Shredding_a_Solar_EruptionV3.mp4 (1920x1080) [202.3 MB] || LARGE_MP4-11797_Shredding_a_Solar_EruptionV3_large.webm (1920x1080) [15.6 MB] || APPLE_TV-11797_Shredding_a_Solar_EruptionV3_appletv_subtitles.m4v (1280x720) [69.7 MB] || 11797_Shredding_a_Solar_EruptionV3.en_US.srt [2.2 KB] || 11797_Shredding_a_Solar_EruptionV3.en_US.vtt [2.2 KB] || NASA_PODCAST-11797_Shredding_a_Solar_EruptionV3_ipod_sm.mp4 (320x240) [20.9 MB] || ", "hits": 61 }, { "id": 12613, "url": "https://svs.gsfc.nasa.gov/12613/", "result_type": "Produced Video", "release_date": "2017-06-02T11:00:00-04:00", "title": "SDO 4k Slow-rotation Sun Resource Page", "description": "Still Image for page || SDO_Slow_Gallery.jpg (1920x1080) [235.4 KB] || SDO_Slow_Gallery_searchweb.png (320x180) [43.0 KB] || SDO_Slow_Gallery_thm.png (80x40) [3.6 KB] || ", "hits": 169 }, { "id": 12612, "url": "https://svs.gsfc.nasa.gov/12612/", "result_type": "Produced Video", "release_date": "2017-05-18T11:00:00-04:00", "title": "Landsat Tracks Mount St. Helens Recovery", "description": "In 1980, Mount St. Helens roared back into major activity with a massive eruption that leveled surrounding forest, blasted away over a thousand feet of the mountain's summit, and claimed 57 human lives.This short video shows the catastrophic eruption - and the amazing recovery of the surrounding ecosystem - through the eyes of the Landsat satellites, which have been imaging our planet for almost forty years. By observing red, near-infrared, and green wavelengths of light reflected off the surface, it is possible to distinguish healthy vegetation (in green) from bare ground (in magenta).Music: Running by Dirk Ehlert [BMI], Guillermo De La Barreda [BMI]Watch this video on the NASA Goddard YouTube channel. || 12612-Mt-St-Helens-timelapse-print.jpg (1920x1080) [2.3 MB] || 12612-Mt-St-Helens-timelapse-print_searchweb.png (320x180) [129.3 KB] || 12612-Mt-St-Helens-timelapse-print_thm.png (80x40) [7.7 KB] || 12612-Mt-St-Helens-timelapse_prores.mov (1280x720) [1.3 GB] || 12612-Mt-St-Helens-timelapse_large.mp4 (1920x1080) [95.7 MB] || 12612-Mt-St-Helens-timelapse_youtube_hq.mov (1920x1080) [407.5 MB] || 12612-Mt-St-Helens-timelapse_appletv.m4v (1280x720) [44.8 MB] || 12612-Mt-St-Helens-timelapse_.webm (960x540) [38.8 MB] || GSFC_20170518_MtStHelens_m12612_Timelapse.en_US.vtt [42 bytes] || 12612-Mt-St-Helens-timelapse_ipod_sm.mp4 (320x240) [15.5 MB] || ", "hits": 90 }, { "id": 12588, "url": "https://svs.gsfc.nasa.gov/12588/", "result_type": "Produced Video", "release_date": "2017-04-26T13:00:00-04:00", "title": "A Solar Eruption in 5 Steps", "description": "Music credit: Prism Mystery by Donn WilkersonComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || filament.thumb.jpg (1920x1080) [239.3 KB] || filament.thumb_print.jpg (1024x576) [176.5 KB] || filament.thumb_searchweb.png (320x180) [106.4 KB] || filament.thumb_web.png (320x180) [106.4 KB] || filament.thumb_thm.png (80x40) [7.0 KB] || 12588_Mechanisms_for_Solar_EruptionsV4.mov (1920x1080) [3.2 GB] || 12588_Mechanisms_for_Solar_EruptionsV4.webm (1920x1080) [10.2 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_appletv.m4v (1280x720) [63.8 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_large.mp4 (1920x1080) [114.5 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_youtube_hq.mov (1920x1080) [244.4 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_appletv_subtitles.m4v (1280x720) [63.8 MB] || 12588_Mechanisms_for_Solar_EruptionsV4.en_US.srt [1.2 KB] || 12588_Mechanisms_for_Solar_EruptionsV4.en_US.vtt [1.2 KB] || 12588MechanismsforSolarEruptionsV4_VX-281901_ipod_sm.mp4 (320x240) [17.5 MB] || ", "hits": 30 }, { "id": 40323, "url": "https://svs.gsfc.nasa.gov/gallery/applied-science/", "result_type": "Gallery", "release_date": "2017-03-30T00:00:00-04:00", "title": "Applied Science", "description": "Discovering innovative and practical uses of Earth observations\n\nappliedsciences.nasa.gov", "hits": 43 }, { "id": 12499, "url": "https://svs.gsfc.nasa.gov/12499/", "result_type": "Produced Video", "release_date": "2017-03-20T14:00:00-04:00", "title": "Swift Charts a Star's 'Death Spiral' into Black Hole", "description": "This animation illustrates how debris from a tidally disrupted star collides with itself, creating shock waves that emit ultraviolet and optical light far from the black hole. According to Swift observations of ASASSN-14li, these clumps took about a month to fall back to the black hole, where they produced changes in the X-ray emission that correlated with the earlier UV and optical changes.Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA.gov Video YouTube channel. || TD_Shocks_Still_print.jpg (1024x576) [115.2 KB] || TD_Shocks_Still.png (3840x2160) [32.6 MB] || TD_Shocks_Still.jpg (3840x2160) [922.7 KB] || TD_Shocks_Still_searchweb.png (320x180) [59.5 KB] || TD_Shocks_Still_thm.png (80x40) [4.8 KB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_1080.mov (1920x1080) [50.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_youtube_hq.mov (1920x1080) [25.7 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Good_1080.m4v (1920x1080) [44.4 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.m4v (960x540) [10.2 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_HD.wmv (1920x1080) [6.9 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_Compatible.webm (960x540) [3.8 MB] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_VX-280970_appletv_subtitles.m4v (1280x720) [25.2 MB] || 12499_Tidal_Disruption_SRT_Captions.en_US.srt [509 bytes] || 12499_Tidal_Disruption_SRT_Captions.en_US.vtt [522 bytes] || 12499_Tidal_Disruption_Shocks_at_Apocenter_FINAL_ProRes_1920x1080_2997.mov (1920x1080) [591.1 MB] || ", "hits": 175 }, { "id": 40317, "url": "https://svs.gsfc.nasa.gov/gallery/vcearth-video-wall/", "result_type": "Gallery", "release_date": "2017-02-02T00:00:00-05:00", "title": "VC Earth Video Wall", "description": "list of videos to display on video wall in Earth science exhibit at Goddard Visitor Center", "hits": 37 }, { "id": 12451, "url": "https://svs.gsfc.nasa.gov/12451/", "result_type": "Produced Video", "release_date": "2017-01-30T11:30:00-05:00", "title": "Fermi Sees Gamma Rays from Far Side Solar Flares", "description": "On three occasions, NASA's Fermi Gamma-ray Space Telescope has detected gamma rays from solar storms on the far side of the sun, emission the Earth-orbiting satellite shouldn't be able to detect. Particles accelerated by these eruptions somehow reach around to produce a gamma-ray glow on the side of the sun facing Earth and Fermi. Watch to learn more. Credit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available.This illustration shows large magnetic structures extending high above the sun from the active region hosting the Sept. 1, 2014, solar blast. Left: Scientists think particles accelerated at the leading edge of the event's coronal mass ejection followed magnetic lines high above the sun. Right: Some of the particles followed similar magnetic structures rooted in the Earth-facing side of the sun. They rained down on the sun and interacted with the solar surface, producing gamma rays (magenta). The solar images shown here come from (left) STEREO B and (right) NASA's Solar Dynamics Observatory. Credit: NASA/STEREO and NASA/SDO || STEREO-SDO_Fermi_Still.jpg (1920x1080) [433.9 KB] || STEREO-SDO_Fermi_Still_searchweb.png (320x180) [101.1 KB] || STEREO-SDO_Fermi_Still_thm.png (80x40) [7.7 KB] || 12451_Fermi_Farside_Flares_ProRes_1920x1080_2997.mov (1920x1080) [2.5 GB] || 12451_Fermi_Farside_Flares_FINAL_youtube_hq.mov (1920x1080) [1.2 GB] || 12451_Fermi_Farside_Flares-H264_1080.mov (1920x1080) [286.5 MB] || 12451_Fermi_Farside_Flares-H264_Good_1080.m4v (1920x1080) [190.5 MB] || 12451_Fermi_Farside_Flares_FINAL_appletv.m4v (1280x720) [100.4 MB] || 12451_Fermi_Farside_Flares-H264_Compatible.m4v (960x540) [74.4 MB] || 12451_Fermi_Farside_Flares_FINAL_appletv_subtitles.m4v (1280x720) [100.5 MB] || 12451_Fermi_Farside_Flares-H264_Compatible.webm (960x540) [20.5 MB] || 12451_Fermi_Farside_Flares_SRT_Captions.en_US.srt [3.3 KB] || 12451_Fermi_Farside_Flares_SRT_Captions.en_US.vtt [3.3 KB] || ", "hits": 57 } ] }