{ "count": 51, "next": null, "previous": null, "results": [ { "id": 5407, "url": "https://svs.gsfc.nasa.gov/5407/", "result_type": "Visualization", "release_date": "2025-05-28T00:00:00-04:00", "title": "Solar Loops and Eruptions - October 8, 2024", "description": "A fourteen hour continuous observation of the Sun, showing the variety of eruptions.", "hits": 55 }, { "id": 5486, "url": "https://svs.gsfc.nasa.gov/5486/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M8.9 flare from Active Region 13932 - December 23, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13932 (in the lower left quadrant) launches an M8.9 flare on December 23. 2024. Some filaments of plasma launch from the site after the flare. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 14 }, { "id": 5497, "url": "https://svs.gsfc.nasa.gov/5497/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M5.1 flare from Active Region 13977 - February 2, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13977 (in the upper center of the disk) launch an M5.1 flare and a filament of material on February 2, 2025.", "hits": 22 }, { "id": 5494, "url": "https://svs.gsfc.nasa.gov/5494/", "result_type": "Visualization", "release_date": "2025-02-20T00:00:00-05:00", "title": "X1.8 flare from Active Region 13947 - January 4, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13947 launch an X1.8 flare on January 4, 2025.", "hits": 18 }, { "id": 5386, "url": "https://svs.gsfc.nasa.gov/5386/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An X1.3 flare from Active Region 13825 - and later an M6.8 - September 12, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13825 launches an X1.3 flare on the lower left limb on September 12, 2024. Later, an M6.8 (14:43 TAI) erupts on the right limb. For more details, see the Space Weather Database for X1.3 and M6.8. An additional small filament eruption occurs near the center of the disk about 17:24 TAI.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 16 }, { "id": 5355, "url": "https://svs.gsfc.nasa.gov/5355/", "result_type": "Visualization", "release_date": "2024-10-02T00:00:00-04:00", "title": "An X1.7 flare from Active Region 13765 and some extra energetic activity - August 5, 2024", "description": "Active Region AR 13765 launches an X1.7 flare on August 5, 2024 on the rightmost part of the solar limb. Shortly thereafter, an X1.1 flare launches near the left limb from AR 13780. For more details, see the Space Weather Database entry for X1.7 and X1.1. Towards the end of this visualization, around 18:35 TAI, a bright filament launches near the center of the disk.", "hits": 8 }, { "id": 40523, "url": "https://svs.gsfc.nasa.gov/gallery/escapade/", "result_type": "Gallery", "release_date": "2024-09-04T00:00:00-04:00", "title": "ESCAPADE – Escape and Plasma Acceleration and Dynamics Explorer", "description": "Using two identical spacecraft in orbit around Mars, the Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will investigate how a stream of charged particles from the Sun called the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE will use its twin orbiters to take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time. The data returned from ESCAPADE will provide new insight into the evolution of Mars’ climate, helping to understand how Mars began losing its atmosphere and water.\n\nESCAPADE launched on Nov. 13, 2025, from NASA’s Kennedy Space Center in Florida and is expected to reach Mars in September 2027.\n\nLearn more: https://science.nasa.gov/mission/escapade/ ", "hits": 300 }, { "id": 5288, "url": "https://svs.gsfc.nasa.gov/5288/", "result_type": "Visualization", "release_date": "2024-07-09T00:00:00-04:00", "title": "An X1.5 flare and more from Active Region 13664 - May 11, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.An X1.5 flare erupts from Active Region 13664 (lower right quadrant) on May 11, 2024. Less than four hours later, a smaller M8.8 flare erupts from the same region. For more details, see the Space Weather Database for the X1.5 and M8.8 entries. A large filament is also forming on the lower right solar limb.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 38 }, { "id": 5268, "url": "https://svs.gsfc.nasa.gov/5268/", "result_type": "Visualization", "release_date": "2024-05-08T00:00:00-04:00", "title": "Double Filament Eruptions from AR 13614 - March 21, 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 13614 (upper left) launches two CMEs on March 21, 2024. For details of this event, see the Space Weather database entry. || ", "hits": 27 }, { "id": 5223, "url": "https://svs.gsfc.nasa.gov/5223/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "M9.0 flare at Active Region 13576 - February 10, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13576 near the center of the solar disk, launches an M9.0 class flare. A bright filament of plasma is launched to the upper right from the site of the event. 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": 26 }, { "id": 5225, "url": "https://svs.gsfc.nasa.gov/5225/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "X2.5 flare at Active Region 13576 - February 16, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13576, now carried by solar rotation to the lower right limb of the solar disk, launches an X2.5 class flare. For details of this event, see the Space Weather database entry. Lots of post-flare filament activity on the limb, particularly solar material falling back towards the Sun.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": 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": 195 }, { "id": 5108, "url": "https://svs.gsfc.nasa.gov/5108/", "result_type": "Visualization", "release_date": "2023-06-27T00:00:00-04:00", "title": "An 9.6 M-class flare and Filament - May 16, 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 AR13310 at the lower left solar limb launches an M 9.6 class flare followed by a bright filament launched almost tangent to the 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.Event Description. || ", "hits": 18 }, { "id": 5084, "url": "https://svs.gsfc.nasa.gov/5084/", "result_type": "Visualization", "release_date": "2023-06-06T00:00:00-04:00", "title": "Several impressive filament eruptions leading up to an M 8.7 Flare at Active Region 13234 - February 27-28, 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.Some impressive filaments erupt on the solar limb (lower left and lower right) in the early part of this image series. Later (17:46:42 TAI), an active region in the upper right quadrant of the solar disk launches a mid-level M 8.7 class flare.Event Description || ", "hits": 30 }, { "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": 16 }, { "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": 49 }, { "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": 37 }, { "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": 406 }, { "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": 64 }, { "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": 277 }, { "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": 355 }, { "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": 352 }, { "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": 211 }, { "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": 800 }, { "id": 30944, "url": "https://svs.gsfc.nasa.gov/30944/", "result_type": "Hyperwall Visual", "release_date": "2018-05-07T10:00:00-04:00", "title": "Vision Across the Full Spectrum: The Crab Nebula, from Radio to X-ray", "description": "This animation shows the Crab Nebula from the lowest-frequency light (radio), to infrared, visible, ultraviolet, and finally X-ray. || STScI-H-CrabNebula_1x-1920x1080.00001_print.jpg (1024x576) [40.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_searchweb.png (320x180) [26.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_thm.png (80x40) [2.3 KB] || STScI-H-CrabNebula_1x-1280x720.mp4 (1280x720) [3.8 MB] || STScI-H-CrabNebula_1x-1920x1080.mp4 (1920x1080) [7.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-CrabNebula_1x-1920x1080.webm (1920x1080) [8.0 MB] || STScI-H-CrabNebula_1x-640x360.mp4 (640x360) [1.4 MB] || STScI-H-CrabNebula_1x-3840x2160.mp4 (3840x2160) [16.2 MB] || STScI-H-CrabNebula_1x-H265_3840x2160.mp4 (3840x2160) [3.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 312 }, { "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": 49 }, { "id": 40337, "url": "https://svs.gsfc.nasa.gov/gallery/lrosolar-eclipse/", "result_type": "Gallery", "release_date": "2017-07-17T00:00:00-04:00", "title": "LRO and Solar Eclipse Events", "description": "This page features videos for the 2017 Solar Eclipse Events being coordinated with the LRO Mission production team.", "hits": 150 }, { "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": 178 }, { "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": 25 }, { "id": 12377, "url": "https://svs.gsfc.nasa.gov/12377/", "result_type": "Produced Video", "release_date": "2016-09-29T11:00:00-04:00", "title": "Solar Surveyor", "description": "The Hinode Solar Observatory celebrates 10 years in space. || cz-1024.jpg (1024x576) [120.8 KB] || cz-1280.jpg (1280x720) [161.4 KB] || cz-1024_print.jpg (1024x576) [127.4 KB] || cz-1024_searchweb.png (320x180) [49.2 KB] || cz-1024_web.png (320x180) [49.2 KB] || cz-1024_thm.png (80x40) [4.2 KB] || ", "hits": 21 }, { "id": 12292, "url": "https://svs.gsfc.nasa.gov/12292/", "result_type": "Produced Video", "release_date": "2016-06-24T15:00:00-04:00", "title": "Solar Highlights of 2016/2017", "description": "A collection of solar highlights featuring:- NASA's Solar Dynamics Observatory (SDO)- NASA's Interface Region Imaging Spectrograph (IRIS) mission- ESA/NASA's Solar and Heliospheric Observatory (SOHO)- NASA's Solar TErrestrial RElations Observatory (STEREO) mission || ", "hits": 158 }, { "id": 4380, "url": "https://svs.gsfc.nasa.gov/4380/", "result_type": "Visualization", "release_date": "2015-10-14T00:00:00-04:00", "title": "The Sun from SDO: The See-Saw Filament", "description": "1080HD movie of the Sun in AIA 304 angstrom filter. || May2015SeeSawFilament_304A_stand.HD1080i.00300_print.jpg (1024x576) [65.5 KB] || May2015SeeSawFilament_304A_stand.HD1080i.00300_searchweb.png (320x180) [37.8 KB] || May2015SeeSawFilament_304A_stand.HD1080i.00300_thm.png (80x40) [3.1 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || May2015SeeSawFilament_304A_stand_1080p.webm (1920x1080) [3.0 MB] || May2015SeeSawFilament_304A_stand_1080p.mp4 (1920x1080) [28.7 MB] || May2015SeeSawFilament_304A_stand_1080p.mp4.hwshow [204 bytes] || ", "hits": 17 }, { "id": 12021, "url": "https://svs.gsfc.nasa.gov/12021/", "result_type": "Produced Video", "release_date": "2015-10-13T13:00:00-04:00", "title": "Hubble Maps Jupiter in 4k Ultra HD", "description": "New imagery from the Hubble Space Telescope is revealing details never before seen on Jupiter. Hubble’s new Jupiter maps were used to create this Ultra HD animation.Watch this video on the NASA Explorer YouTube channel. || JupiterThumbnailSmall.png (2160x1215) [1.4 MB] || G2015-085_Jupiter720_MASTER_appletv_appletv_subtitles.m4v (1280x720) [39.0 MB] || G2015-085_Jupiter720_MASTER_appletv.m4v (1280x720) [39.0 MB] || WEBM_G2015-085_Jupiter4k_MASTER_YouTube.webm (960x540) [28.5 MB] || G2015-085_Jupiter720_MASTER.mp4 (1280x720) [98.9 MB] || G2015-085_Jupiter720_MASTER_nasa_tv.mpeg (1280x720) [249.3 MB] || G2015-085_Jupiter720_MASTER_prores.mov (1280x720) [917.9 MB] || G2015-085_Jupiter720_MASTER.en_US.srt [98 bytes] || G2015-085_Jupiter720_MASTER.en_US.vtt [111 bytes] || G2015-085_Jupiter720_.key [41.8 MB] || G2015-085_Jupiter720_.pptx [39.3 MB] || G2015-085_Jupiter720_MASTER_12021.key [41.7 MB] || G2015-085_Jupiter720_MASTER_12021.pptx [39.3 MB] || G2015-085_Jupiter4k_MASTER_YouTube.mp4 (3840x2160) [495.9 MB] || G2015-085_Jupiter4k_MASTER.mov (3840x2160) [4.5 GB] || G2015-085_Jupiter4k_MASTER_YouTube.hwshow [94 bytes] || G2015-085_Jupiter720_MASTER_appletv.m4v.hwshow [88 bytes] || ", "hits": 1018 }, { "id": 11755, "url": "https://svs.gsfc.nasa.gov/11755/", "result_type": "Produced Video", "release_date": "2015-03-10T11:00:00-04:00", "title": "Solar Exposures", "description": "See a five-year time-lapse of the sun. || c_1024.jpg (1024x576) [180.4 KB] || c_1280.jpg (1280x720) [254.4 KB] || c_1920.jpg (1920x1080) [1.3 MB] || c_1024_print.jpg (1024x576) [181.8 KB] || c_1024_searchweb.png (320x180) [70.7 KB] || c_1024_print_thm.png (80x40) [14.9 KB] || ", "hits": 115 }, { "id": 4166, "url": "https://svs.gsfc.nasa.gov/4166/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "March 2014: Erupting Solar Prominence", "description": "A solar filament, in the upper left quadrant of the image, erupts from the Sun (about time stamp 2014 March 29 01:54:00 UTC).There is a gap of 40 minutes in the data coverage, from 03:00 - 03:40 UT. || ", "hits": 29 }, { "id": 11696, "url": "https://svs.gsfc.nasa.gov/11696/", "result_type": "Produced Video", "release_date": "2014-12-25T11:00:00-05:00", "title": "Twisted Solar Blob", "description": "NASA’s Solar Dynamics Observatory (SDO) monitors the sun 24/7, recording its outbursts in high-definition. On September 26, 2014, the spacecraft captured a twisted blob of plasma erupting in a dramatic liftoff. The plasma, which is ionized helium cooked to over 100,000 degrees Fahrenheit, corkscrewed outward along the path of the sun's complex magnetic field. Like densely looped carpeting, magnetic field lines crisscross through the sun's surface and outer layers. This weave usually prevents plasma from escaping. But if the magnetic field lines become unsteady or suddenly align into new patterns, a filament can whip into space. Watch the video to see the event unfold. || ", "hits": 60 }, { "id": 11705, "url": "https://svs.gsfc.nasa.gov/11705/", "result_type": "Produced Video", "release_date": "2014-10-06T14:00:00-04:00", "title": "NASA's SDO Watches Giant Filament on the Sun", "description": "A snaking, extended filament of solar material currently lies on the front of the sun— some 1 million miles across from end to end. Filaments are clouds of solar material suspended above the sun by powerful magnetic forces. Though notoriously unstable, filaments can last for days or even weeks.NASA's Solar Dynamics Observatory, or SDO, which watches the sun 24 hours a day, has observed this gigantic filament for several days as it rotated around with the sun. If straightened out, the filament would reach almost across the whole sun, about 1 million miles or 100 times the size of Earth.SDO captured images of the filament in numerous wavelengths, each of which helps highlight material of different temperatures on the sun. By looking at any solar feature in different wavelengths and temperatures, scientists can learn more about what causes such structures, as well as what catalyzes their occasional giant eruptions out into space.Look at the images to see how the filament appears in different wavelengths. The brownish combination image was produced by blending two wavelengths of extreme UV light with a wavelength of 193 and 335 angstroms. The red image shows the 304 angstrom wavelength of extreme UV light. || ", "hits": 54 }, { "id": 11596, "url": "https://svs.gsfc.nasa.gov/11596/", "result_type": "Produced Video", "release_date": "2014-08-19T11:00:00-04:00", "title": "Solar Arcs", "description": "On June 3, 2014, NASA’s Solar Dynamics Observatory, or SDO, spacecraft captured a 500,000-mile-long filament stretching across the sun’s atmosphere. Resembling a fiery whip, these suspended clouds made of million-degree electrified gases rise and fall in giant arcs above the surface. Scientists actually have two different names for these types of features depending on where on the sun they’re observed. When seen hanging over the sun’s face, scientists call them filaments. But when projecting from the sun’s limb, they’re called prominences. The massive structures can last up to several months, and will occasionally break apart in sudden eruptions. When this happens, solar material can be sent out into space, and if it moves toward Earth, it can spark stunning auroras. Watch the video for an up-close look at a solar filament. || ", "hits": 60 }, { "id": 11373, "url": "https://svs.gsfc.nasa.gov/11373/", "result_type": "Produced Video", "release_date": "2013-12-12T00:00:00-05:00", "title": "Canyon Of Fire", "description": "In September 2013, a 200,000-mile-long loop of solar material erupted in the sun's atmosphere leaving behind what looks like a canyon of fire. These giant loops, called filaments, consist of charged particles held in place by magnetic fields that extend out from the sun’s surface. On September 29-30, NASA’s Solar Dynamics Observatory spacecraft watched as a filament about 25 times the Earth’s width expanded and then collapsed just north of the sun’s equator. Moments later, it saw a glowing canyon trace the channel where magnetic fields held the structure aloft. Watch the video to see the event unfold. || ", "hits": 24 }, { "id": 11379, "url": "https://svs.gsfc.nasa.gov/11379/", "result_type": "Produced Video", "release_date": "2013-10-24T10:00:00-04:00", "title": "Filament Eruption Creates 'Canyon of Fire' on the Sun", "description": "A magnetic filament of solar material erupted on the sun in late September, breaking the quiet conditions in a spectacular fashion. The 200,000 mile long filament ripped through the sun's atmosphere, the corona, leaving behind what looks like a canyon of fire. The glowing canyon traces the channel where magnetic fields held the filament aloft before the explosion. Visualizers at NASA's Goddard Space Flight Center in Greenbelt, Md. combined two days of satellite data to create a short movie of this gigantic event on the sun.In reality, the sun is not made of fire, but of something called plasma: particles so hot that their electrons have boiled off, creating a charged gas that is interwoven with magnetic fields. These images were captured on Sept. 29-30, 2013, by NASA's Solar Dynamics Observatory, or SDO, which constantly observes the sun in a variety of wavelengths. Different wavelengths help capture different aspect of events in the corona. The red images shown in the movie help highlight plasma at temperatures of 90,000° F and are good for observing filaments as they form and erupt. The yellow images, showing temperatures at 1,000,000° F, are useful for observing material coursing along the sun's magnetic field lines, seen in the movie as an arcade of loops across the area of the eruption. The browner images at the beginning of the movie show material at temperatures of 1,800,000° F, and it is here where the canyon of fire imagery is most obvious. By comparing this with the other colors, one sees that the two swirling ribbons moving farther away from each other are, in fact, the footprints of the giant magnetic field loops, which are growing and expanding as the filament pulls them upward. || ", "hits": 151 }, { "id": 3999, "url": "https://svs.gsfc.nasa.gov/3999/", "result_type": "Visualization", "release_date": "2012-10-26T00:00:00-04:00", "title": "The View from SDO: The August 31, 2012 Filament Eruption", "description": "The Solar Dynamics Observatory (SDO) observed a large filament eruption on August 31, 2012. This visualization was generated using high time resolution (12 seconds) data from the Atmospheric Imaging Assembly (AIA). Two datasets are used, the SDO/AIA 304 Ångstrom wavelength (orange color table) and the 171 Ångstrom wavelength (gold color table). These are wavelengths in the ultraviolet band of the electromagnetic spectrum. They are not visible to the human eye or to ground-based telescopes so coded colors are used in presentation.It is the source material for \"August 31, 2012 Magnificent CME\" visualization. || ", "hits": 98 }, { "id": 11078, "url": "https://svs.gsfc.nasa.gov/11078/", "result_type": "Produced Video", "release_date": "2012-09-13T00:00:00-04:00", "title": "Class Act", "description": "In August 2012, a long filament of solar material coalesced in the sun's atmosphere. For several days it was visible, appearing from Earth's viewpoint to curl up and over the left side of the sun. Scientists estimate its length was approximately 186,000 miles, equivalent to 30 Earths placed side by side. On August 31 at 4:36 p.m. EDT, the filament expanded and erupted, releasing particles into space at speeds of 900 miles per second. The ejected material did not head directly toward Earth, though some of it did glance off the planet's magnetic environment, or magnetosphere, causing aurora to appear on the night of Monday, September 3. The video shows the eruption—a particularly gorgeous one, even for veteran observers of the sun—as seen by three NASA spacecraft. || ", "hits": 49 }, { "id": 11095, "url": "https://svs.gsfc.nasa.gov/11095/", "result_type": "Produced Video", "release_date": "2012-09-04T14:00:00-04:00", "title": "August 31, 2012 Magnificent CME", "description": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3. || ", "hits": 190 }, { "id": 3931, "url": "https://svs.gsfc.nasa.gov/3931/", "result_type": "Visualization", "release_date": "2012-03-31T00:00:00-04:00", "title": "Launching Filament: November 14, 2011", "description": "A large filament launches from the Sun in this sequence of 304 Ångstrom imagery from Solar Dynamics Observatory. || ", "hits": 32 }, { "id": 10748, "url": "https://svs.gsfc.nasa.gov/10748/", "result_type": "Produced Video", "release_date": "2011-04-21T09:00:00-04:00", "title": "SDO: Year One", "description": "April 21, 2011 marks the one-year anniversary of the Solar Dynamics Observatory (SDO) First Light press conference, where NASA revealed the first images taken by the spacecraft.In the last year, the sun has gone from its quietest period in years to the activity marking the beginning of solar cycle 24. SDO has captured every moment with a level of detail never-before possible. The mission has returned unprecedented images of solar flares, eruptions of prominences, and the early stages of coronal mass ejections (CMEs). In this video are some of the most beautiful, interesting, and mesmerizing events seen by SDO during its first year.In the order they appear in the video the events are:1. Prominence Eruption from AIA in 304 Ångstroms on March 30, 20102. Cusp Flow from AIA in 171 Ångstroms on February 14, 20113. Prominence Eruption from AIA in 304 Ångstroms on February 25, 20114. Cusp Flow from AIA in 304 Ångstroms on February 14, 20115. Merging Sunspots from HMI in Continuum on October 24-28, 20106. Prominence Eruption and active region from AIA in 304 Ångstroms on April 30, 20107. Solar activity and plasma loops from AIA in 171 Ångstroms on March 4-8, 20118. Flowing plasma from AIA in 304 Ångstroms on April 19, 20109. Active regions from HMI in Magnetogram on March 10, 201110. Filament eruption from AIA in 304 Ångstroms on December 6, 201011. CME start from AIA in 211 Ångstroms on March 8, 201112. X2 flare from AIA in 304 Ångstroms on February 15, 2011 || ", "hits": 87 }, { "id": 3693, "url": "https://svs.gsfc.nasa.gov/3693/", "result_type": "Visualization", "release_date": "2010-04-21T14:15:00-04:00", "title": "SDO/AIA Zoom-In on Launching Filament (Bands 304, 171, 211)", "description": "As the AIA camera was activated, one of its first views was this fliament launching from the Sun. || ", "hits": 30 }, { "id": 3715, "url": "https://svs.gsfc.nasa.gov/3715/", "result_type": "Visualization", "release_date": "2010-04-21T14:15:00-04:00", "title": "SDO/AIA Close-up on Launching Filament (band 304)", "description": "A close-up view of the filament launch in the 304 band, which corresponds to a wavelength of about 304 Ångstroms. || ", "hits": 25 }, { "id": 3716, "url": "https://svs.gsfc.nasa.gov/3716/", "result_type": "Visualization", "release_date": "2010-04-21T14:15:00-04:00", "title": "SDO/AIA Full-Disk View of Launching Filament (Band 304)", "description": "Full disk view of a filament launch in the SDO AIA 304 band. || ", "hits": 50 }, { "id": 3717, "url": "https://svs.gsfc.nasa.gov/3717/", "result_type": "Visualization", "release_date": "2010-04-21T14:15:00-04:00", "title": "SDO/AIA Zoom-out of Launching Filament (Band 304)", "description": "This view of the filament launch loops several times before pulling out to show the full solar disk. || ", "hits": 28 }, { "id": 40069, "url": "https://svs.gsfc.nasa.gov/gallery/sdofirst-light/", "result_type": "Gallery", "release_date": "2010-03-25T00:00:00-04:00", "title": "SDO First Light", "description": "These are \"First Light\" release movies for Solar Dynamics Observatory (SDO) from April 11, 2010. For more information about SDO, visit the SDO web site @ NASA.gov.", "hits": 78 }, { "id": 3694, "url": "https://svs.gsfc.nasa.gov/3694/", "result_type": "Visualization", "release_date": "2010-03-24T00:00:00-04:00", "title": "A Comparative View of the Sun: SDO/AIA 193 and STEREO-B/EUVI 195", "description": "This movie compares the spatial and temporal resolutions of the SDO/AIA (Atmospheric Imaging Assembly) imager to the STEREO/EUVI (Extreme UltraViolet Imager) imager. STEREO-B/EUVI's highest resolution is 2048x2048 pixels with images taken about every 5 minutes for the 195 Ångstrom band. The SDO/AIA 193 band takes images at 4096x4096 pixels every twelve seconds!While STEREO's vantage point at this time is very different from SDO, we can still identify some features of the Active Region 1087 in these two views. EUVI shows the launch of the filament, while AIA reveals many finer details.This visualization is a companion piece to A Comparative View of the Sun: SDO/AIA 193 and SOHO/EIT 195. || ", "hits": 36 } ] }