{ "count": 286, "next": "https://svs.gsfc.nasa.gov/api/search/?keywords=Coronal+Mass+Ejections&limit=100&offset=100", "previous": null, "results": [ { "id": 31381, "url": "https://svs.gsfc.nasa.gov/31381/", "result_type": "Hyperwall Visual", "release_date": "2026-03-31T11:51:59-04:00", "title": "NASA’S PUNCH Images Eruptions from the Sun", "description": "This video shows several coronal mass ejections (CMEs) erupting from the Sun’s surface from Oct. 21 to Nov. 12, 2025.", "hits": 641 }, { "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": 316 }, { "id": 31361, "url": "https://svs.gsfc.nasa.gov/31361/", "result_type": "Hyperwall Visual", "release_date": "2026-01-09T06:59:59-05:00", "title": "Large Solar Flares Erupt From the Sun", "description": "NASA’s Solar Dynamics Observatory captured images of two solar flares on Nov. 14 and Nov. 30, 2025.", "hits": 340 }, { "id": 5577, "url": "https://svs.gsfc.nasa.gov/5577/", "result_type": "Animation", "release_date": "2025-11-20T09:00:00-05:00", "title": "SDO Sun This Week", "description": "This visualization shows SDO AIA-304 imagery from the past 7 days with a color table and image processing applied. Archive folders are provided in the Download menu.", "hits": 305 }, { "id": 5503, "url": "https://svs.gsfc.nasa.gov/5503/", "result_type": "Visualization", "release_date": "2025-11-19T12:00:00-05:00", "title": "ESCAPADE Theoretical Flight Through Active Mars Magnetosphere", "description": "NASA's Escape and Plasma Acceleration Dynamics Explorers mission, or ESCAPADE, aims to study Mars' real-time response to the solar wind and how the Martian magnetosphere changes over time, helping us better understand Mars' climate history. In this data visualization, we use the September 13, 2017 solar storm that arrived at Mars as an example of a storm that the twin ESCAPADE spacecraft might study.", "hits": 228 }, { "id": 14907, "url": "https://svs.gsfc.nasa.gov/14907/", "result_type": "Produced Video", "release_date": "2025-09-30T14:00:00-04:00", "title": "What is space weather?", "description": "Though it is almost 100 million miles away from Earth, the Sun influences our daily lives in ways you may not realize.A farmer stops their planting operations due to poor GPS signal for their autonomous tractor. A power grid manager changes the configuration of their network to ensure a blackout doesn’t occur due to voltage instability. A pilot switches to back-up communication equipment due to loss of high-frequency radio. A commercial internet company providing service to the military must change the orbit of their spacecraft to avoid a collision due to increased atmospheric drag.These are a few examples of the ways the Sun influences our everyday lives. This is what we define as space weather – the conditions of the space environment driven by the Sun and its impacts on objects in the solar system. || ", "hits": 208 }, { "id": 5375, "url": "https://svs.gsfc.nasa.gov/5375/", "result_type": "Visualization", "release_date": "2025-08-07T14:00:00-04:00", "title": "Carrington Class Coronal Mass Ejection - ENLIL Simulation of A Series of CMEs", "description": "A series of visualizations of the simulation of a series of CMEs between July 2012 and August 2012, including a carrington class coronal mass ejection that hit STEREO-A.", "hits": 414 }, { "id": 5551, "url": "https://svs.gsfc.nasa.gov/5551/", "result_type": "Visualization", "release_date": "2025-07-09T10:00:00-04:00", "title": "M8.1 flare from Active Region 14100 - May 30, 2025", "description": "Solar active region 14100 launches an M8.1 flare on May 30, 2025.", "hits": 33 }, { "id": 5549, "url": "https://svs.gsfc.nasa.gov/5549/", "result_type": "Visualization", "release_date": "2025-06-25T10:00:00-04:00", "title": "X1.1 flare from Active Region 14098 - May 25, 2025", "description": "X1.1 flare from Active Region 14098 - May 25, 2025", "hits": 48 }, { "id": 31354, "url": "https://svs.gsfc.nasa.gov/31354/", "result_type": "Animation", "release_date": "2025-06-13T16:19:00-04:00", "title": "PUNCH", "description": "NASA’s PUNCH Releases Its First Images of Huge Eruptions from Sun", "hits": 129 }, { "id": 5407, "url": "https://svs.gsfc.nasa.gov/5407/", "result_type": "Visualization", "release_date": "2025-05-28T00:00:00-04:00", "title": "Solar Loops and Eruptions - October 8, 2024", "description": "A fourteen hour continuous observation of the Sun, showing the variety of eruptions.", "hits": 54 }, { "id": 5527, "url": "https://svs.gsfc.nasa.gov/5527/", "result_type": "Visualization", "release_date": "2025-05-22T00:00:00-04:00", "title": "M5.6 flare from Active Region 14046 - April 1, 2025 - No foolin'!", "description": "Active Region 14046 launches an M5.6 flare on April 1, 2025.", "hits": 17 }, { "id": 5526, "url": "https://svs.gsfc.nasa.gov/5526/", "result_type": "Visualization", "release_date": "2025-04-14T00:00:00-04:00", "title": "X1.1 flare from Active Region 14046 - March 28, 2025", "description": "Active region 14046 (on the left limb of the Sun) launches an X1.1 flare and a significant amount of plasma.", "hits": 47 }, { "id": 5514, "url": "https://svs.gsfc.nasa.gov/5514/", "result_type": "Visualization", "release_date": "2025-04-07T09:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere for Fulldome", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents and magnetic fields combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 285 }, { "id": 5502, "url": "https://svs.gsfc.nasa.gov/5502/", "result_type": "Visualization", "release_date": "2025-04-07T00:00:00-04:00", "title": "Solar Storm Excites Martian Magnetosphere", "description": "On September 13, 2017, a coronal mass ejection from the Sun arrived at Mars. This data visualization shows how solar-wind-induced currents (green colors) and magnetic fields (pink lines) combine with Mars' relatively weak and irregular native crustal magnetic fields to contribute to Mars’ \"hybrid\" magnetosphere.", "hits": 260 }, { "id": 5482, "url": "https://svs.gsfc.nasa.gov/5482/", "result_type": "Visualization", "release_date": "2025-03-17T00:00:00-04:00", "title": "An M9.4 flare from Active Region 13910 - November 25, 2024", "description": "As solar rotation carries it over the left limb of the Sun, Active Region 13910 launches an M9.4 flare.", "hits": 21 }, { "id": 5513, "url": "https://svs.gsfc.nasa.gov/5513/", "result_type": "Visualization", "release_date": "2025-03-12T00:00:00-04:00", "title": "X2.0 flare from Active Region 14001 - February 23, 2025", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Just before rotating over the right solar limb, active region 14001 launches an X2.0 flare. For more details see the Space Weather database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 49 }, { "id": 5488, "url": "https://svs.gsfc.nasa.gov/5488/", "result_type": "Visualization", "release_date": "2025-03-05T08:02:00-05:00", "title": "An M7.1 flare from Active Region 13936 - December 29, 2024", "description": "Active Region 13936 launches an M7.1 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 19 }, { "id": 5483, "url": "https://svs.gsfc.nasa.gov/5483/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X2.2 flare from Active Region 13912 - December 8, 2024", "description": "Active region 13912 launches an X2.2 flare near the right limb on December 8, 2024.", "hits": 28 }, { "id": 5486, "url": "https://svs.gsfc.nasa.gov/5486/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M8.9 flare from Active Region 13932 - December 23, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13932 (in the lower left quadrant) launches an M8.9 flare on December 23. 2024. Some filaments of plasma launch from the site after the flare. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 12 }, { "id": 5487, "url": "https://svs.gsfc.nasa.gov/5487/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An M7.4 flare from Active Region 13938 - December 26, 2024", "description": "Active region 13938 (upper left quadrant) launches an M7.4 flare.", "hits": 10 }, { "id": 5489, "url": "https://svs.gsfc.nasa.gov/5489/", "result_type": "Visualization", "release_date": "2025-03-05T00:00:00-05:00", "title": "An X1.1 flare from Active Region 13936 - December 29, 2024", "description": "Active region 13936 (upper right quadrant) launches an X1.1 flare.", "hits": 37 }, { "id": 5484, "url": "https://svs.gsfc.nasa.gov/5484/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.4 flare from Active Region 13922 - December 10, 2024", "description": "Active region 13922 launches an M6.4 flare near the left limb of the Sun on December 10, 2024.", "hits": 39 }, { "id": 5485, "url": "https://svs.gsfc.nasa.gov/5485/", "result_type": "Visualization", "release_date": "2025-03-04T00:00:00-05:00", "title": "An M6.7 flare from Active Region 13912 - December 11, 2024", "description": "Active region 13912 on the right limb of the Sun launches an M6.7 flare on December 11, 2024.", "hits": 10 }, { "id": 5500, "url": "https://svs.gsfc.nasa.gov/5500/", "result_type": "Visualization", "release_date": "2025-03-03T00:00:00-05:00", "title": "M7.6 flare from Active Region 13981 - February 6, 2025", "description": "Active Region 13981 (in the upper right quadrant of the disk) launches an M7.6 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 16 }, { "id": 5501, "url": "https://svs.gsfc.nasa.gov/5501/", "result_type": "Visualization", "release_date": "2025-03-03T00:00:00-05:00", "title": "M7.5 flare from Active Region 13981 - February 7, 2025", "description": "Active Region 13981 (in the upper right quadrant of the disk) launches an M7.5 flare in this view from Solar Dynamics Observatory (SDO).", "hits": 15 }, { "id": 5495, "url": "https://svs.gsfc.nasa.gov/5495/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M7.4 flare from Active Region 13964 - January 17, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13964 (in the upper right quadrant of the disk) launch an M7.4 flare followed by some complex post-flare evolution.", "hits": 16 }, { "id": 5496, "url": "https://svs.gsfc.nasa.gov/5496/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.7 flare from Active Region 13978 - January 31, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13978 launch an M6.7 flare on January 31, 2025.", "hits": 10 }, { "id": 5497, "url": "https://svs.gsfc.nasa.gov/5497/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M5.1 flare from Active Region 13977 - February 2, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13977 (in the upper center of the disk) launch an M5.1 flare and a filament of material on February 2, 2025.", "hits": 46 }, { "id": 5498, "url": "https://svs.gsfc.nasa.gov/5498/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M8.8 flare from Active Region 13981 - February 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13981 launch an M8.8 flare early February 3, 2025 (a smaller M3.1 fires off near the same location about two hours later). The Earth eclipses the view from SDO as the video ends.", "hits": 28 }, { "id": 5499, "url": "https://svs.gsfc.nasa.gov/5499/", "result_type": "Visualization", "release_date": "2025-02-20T14:00:00-05:00", "title": "M6.1 flare from Active Region 13981 - February 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13981 launching an M6.1 flare on February 3, 2025.", "hits": 17 }, { "id": 5494, "url": "https://svs.gsfc.nasa.gov/5494/", "result_type": "Visualization", "release_date": "2025-02-20T00:00:00-05:00", "title": "X1.8 flare from Active Region 13947 - January 4, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active region 13947 launch an X1.8 flare on January 4, 2025.", "hits": 26 }, { "id": 5492, "url": "https://svs.gsfc.nasa.gov/5492/", "result_type": "Visualization", "release_date": "2025-02-19T00:00:00-05:00", "title": "X1.2 flare from Active Region 13947 - January 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes active region 13947 launch an X1.2 flare on January 3, 2025.", "hits": 39 }, { "id": 5493, "url": "https://svs.gsfc.nasa.gov/5493/", "result_type": "Visualization", "release_date": "2025-02-19T00:00:00-05:00", "title": "X1.1 and M- flares from Active Region 13947 - January 3, 2025", "description": "Solar Dynamics Observatory (SDO) observes Active Region 13947 launch an X1.1 flare followed by a couple of M-class flares on January 3-4 of 2025.", "hits": 24 }, { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "result_type": "Visualization", "release_date": "2024-12-12T12:00:00-05:00", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "hits": 438 }, { "id": 5430, "url": "https://svs.gsfc.nasa.gov/5430/", "result_type": "Visualization", "release_date": "2024-12-02T00:00:00-05:00", "title": "An M9.4 flare from Active Region 13889 and more - November 10, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13889 launches an M9.4 flare on November 10, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 14 }, { "id": 5426, "url": "https://svs.gsfc.nasa.gov/5426/", "result_type": "Visualization", "release_date": "2024-11-29T00:00:00-05:00", "title": "An M5.5 flare from Active Region 13883 - November 4, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13883 launched an M5.5 flare on November 4, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 7 }, { "id": 5427, "url": "https://svs.gsfc.nasa.gov/5427/", "result_type": "Visualization", "release_date": "2024-11-29T00:00:00-05:00", "title": "An X2.3 flare from Active Region 13878 and more - November 6, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 launches an X2.3 flare, between a couple of M5+ flares, on November 6, 2024. For more details, see the Space Weather Database for the entries M 5.8 (peek at 2024-11-06T08:50), X2.3 (peak at 2024-11-06T13:40) and M5.3 (peak at 2024-11-06T14:38).For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 24 }, { "id": 5411, "url": "https://svs.gsfc.nasa.gov/5411/", "result_type": "Visualization", "release_date": "2024-11-28T00:00:00-05:00", "title": "An M6.5 flare from Active Region 13854 - October 19, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.In a last flash before rotating over the limb, active region 13854 launches an M6.5 flare on October 19, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 20 }, { "id": 5403, "url": "https://svs.gsfc.nasa.gov/5403/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 flare from Active Region 13848 - October 9, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13848 launches an X1.8 flare on October 9, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 27 }, { "id": 5406, "url": "https://svs.gsfc.nasa.gov/5406/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.7 flare from Active Region 13842 - October 9, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.In a last flash before rotating over the limb, active region 13842 launches an M7.7 flare on October 9, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 15 }, { "id": 5413, "url": "https://svs.gsfc.nasa.gov/5413/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 & M9.5 flare from Active Region 13873 - October 26, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Double flares launch from the same active region (AR 13873) less than an hour apart. For more details, see the Space Weather Database entry for M9.5 @ 2024-10-26T06:23 TAI and X1.8 @ 2024-10-26T07:19 TAI.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 21 }, { "id": 5420, "url": "https://svs.gsfc.nasa.gov/5420/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.2 flare from Active Region 13878 - October 30,2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 launches an M7.2 flare. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 5 }, { "id": 5421, "url": "https://svs.gsfc.nasa.gov/5421/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X2.0 and M9.4 flare from Active Region 13878 - October 31, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 presents a 'double whammy' of two strong flares (X 2.0 and M9.4) only about 30 minutes apart. For more details, see the Space Weather Database entries for X2.0 (peak @ 2024-10-31T21:20) and M9.4 (peak @ 2024-10-31T21:54).For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 11 }, { "id": 5412, "url": "https://svs.gsfc.nasa.gov/5412/", "result_type": "Visualization", "release_date": "2024-11-26T00:00:00-05:00", "title": "An X3.3 flare from Active Region 13869 - October 24, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13869 launches an X3.3 flare on October 24, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 18 }, { "id": 5402, "url": "https://svs.gsfc.nasa.gov/5402/", "result_type": "Visualization", "release_date": "2024-11-05T00:00:00-05:00", "title": "An X2.1 and X1.0 flare from Active Region 13842 - October 7, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active region 13842 launches an X2.1, followed less than 30 minutes later by an X1.0 flare on October 7, 2024. For more details, see the Space Weather Database for the X2.1 flare and the X1.0 flare.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 31 }, { "id": 5399, "url": "https://svs.gsfc.nasa.gov/5399/", "result_type": "Visualization", "release_date": "2024-11-04T00:00:00-05:00", "title": "An M6.7 flare from Active Region 13843 - October 3, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.", "hits": 22 }, { "id": 5398, "url": "https://svs.gsfc.nasa.gov/5398/", "result_type": "Visualization", "release_date": "2024-10-30T00:00:00-04:00", "title": "An X9.0 flare from Active Region 13842 - October 3, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.", "hits": 64 }, { "id": 5397, "url": "https://svs.gsfc.nasa.gov/5397/", "result_type": "Visualization", "release_date": "2024-10-17T00:00:00-04:00", "title": "An X7.1 flare from Active Region 13842 - October 1, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region AR 13842 launches an X7.1 flare on October 1, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 57 }, { "id": 5396, "url": "https://svs.gsfc.nasa.gov/5396/", "result_type": "Visualization", "release_date": "2024-10-15T00:00:00-04:00", "title": "An M7.6 flare from Active Region 13842 - September 30, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.An M7.6 flare fires off from Active Region 13842 on September 30, 2024. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to all this imagery. || ", "hits": 41 }, { "id": 5388, "url": "https://svs.gsfc.nasa.gov/5388/", "result_type": "Visualization", "release_date": "2024-10-14T00:00:00-04:00", "title": "An X4.5 flare from Active Region 13825 - September 14, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.", "hits": 54 }, { "id": 5214, "url": "https://svs.gsfc.nasa.gov/5214/", "result_type": "Visualization", "release_date": "2024-02-08T08:00:00-05:00", "title": "Geomagnetic Storm Causes Satellite Loss for Fulldome", "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events.This is 4k fulldome imagery intended for projection in a planetarium or other hemispherical dome theater. || ", "hits": 194 }, { "id": 5193, "url": "https://svs.gsfc.nasa.gov/5193/", "result_type": "Visualization", "release_date": "2023-12-11T09:00:00-05:00", "title": "Geomagnetic Storm Causes Satellite Loss", "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events. || ", "hits": 3103 }, { "id": 4923, "url": "https://svs.gsfc.nasa.gov/4923/", "result_type": "Infographic", "release_date": "2021-08-25T00:00:00-04:00", "title": "Space Weather Infographics", "description": "Space and earth-based impacts of space weather. || SpaceWeatherIllustration_print.jpg (1024x791) [154.3 KB] || SpaceWeatherIllustration.png (3300x2550) [2.5 MB] || SpaceWeatherIllustration_searchweb.png (320x180) [56.2 KB] || SpaceWeatherIllustration_thm.png (80x40) [6.2 KB] || Multiple infographics illustrating the science and impact of space weather. || ", "hits": 141 }, { "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": 45 }, { "id": 13275, "url": "https://svs.gsfc.nasa.gov/13275/", "result_type": "Produced Video", "release_date": "2019-08-07T11:30:00-04:00", "title": "How NASA Will Protect Astronauts From Space Radiation", "description": "Today, the Apollo-era flares serve as a reminder of the threat of radiation exposure for technology and astronauts in space. Understanding and predicting solar eruptions is crucial for safe space exploration. Almost 50 years since those 1972 storms, the data, technology and resources available to NASA have improved, enabling advancements towards space weather forecasts and astronaut protection — key to NASA’s Artemis program to return astronauts to the Moon.", "hits": 242 }, { "id": 4699, "url": "https://svs.gsfc.nasa.gov/4699/", "result_type": "Visualization", "release_date": "2018-11-30T14:00:00-05:00", "title": "The CME Heard 'Round the Solar System", "description": "As the CMEs and SIRs move through the solar system, we include graphs of particle fluxes measured at Earth, Mars, and STEREO-A. || SEPsAtMars.topfixed.UHDframes.clockSlate_HAE.UHD3840.01000_print.jpg (1024x576) [100.6 KB] || SEPsAtMars.topfixed.UHDframes.clockSlate_HAE.UHD3840.01000_thm.png (80x40) [6.5 KB] || SEPsAtMars.topfixed.UHDframes.clockSlate_HAE.UHD3840.01000_searchweb.png (320x180) [87.5 KB] || SEPsAtMars.topfixed_HAE.HD1080i_p30.mp4 (1920x1080) [19.4 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || SEPsAtMars.topfixed_HAE.HD1080i_p30.webm (1920x1080) [3.0 MB] || SEPsAtMars.topfixed_HAE_2160p30.mp4 (3840x2160) [61.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ", "hits": 104 }, { "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": 38 }, { "id": 12532, "url": "https://svs.gsfc.nasa.gov/12532/", "result_type": "Produced Video", "release_date": "2017-11-07T14:00:00-05:00", "title": "Welcome to the Ionosphere", "description": "Music credit: Foxy Trot by Luis Enriquez Bacalov Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || ionosphere_thumb.jpg (1920x1080) [69.9 KB] || ionosphere_thumb_searchweb.png (320x180) [57.3 KB] || ionosphere_thumb_thm.png (80x40) [6.3 KB] || APPLE_TV-12532_Welcome_to_the_ionosphere_bsideV4_appletv.webm (1280x720) [24.0 MB] || APPLE_TV-12532_Welcome_to_the_ionosphere_bsideV4_appletv.m4v (1280x720) [116.4 MB] || APPLE_TV-12532_Welcome_to_the_ionosphere_bsideV4_appletv_subtitles.m4v (1280x720) [116.5 MB] || YOUTUBE_1080-12532_Welcome_to_the_ionosphere_bsideV4_youtube_1080.mp4 (1920x1080) [346.2 MB] || NASA_TV-12532_Welcome_to_the_ionosphere_bsideV4.mpeg (1280x720) [691.7 MB] || 12532_Welcome_to_the_ionosphere_bsideV2_lowres.en_US.srt [3.8 KB] || 12532_Welcome_to_the_ionosphere_bsideV2_lowres.en_US.vtt [3.8 KB] || 12532_Welcome_to_the_ionosphere_bsideV4_lowres.mp4 (480x272) [29.2 MB] || LARGE_MP4-12532_Welcome_to_the_ionosphere_bsideV4_large.mp4 (3840x2160) [220.8 MB] || NASA_PODCAST-12532_Welcome_to_the_ionosphere_bsideV4_ipod_sm.mp4 (320x240) [37.3 MB] || 12532_Welcome_to_the_ionosphere_bsideV4.mov (3840x2160) [10.1 GB] || ", "hits": 105 }, { "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": 39 }, { "id": 12693, "url": "https://svs.gsfc.nasa.gov/12693/", "result_type": "Produced Video", "release_date": "2017-08-17T11:00:00-04:00", "title": "A Total Solar Eclipse Revealed Solar Storms 100 Years Before Satellites", "description": "Eclipses set the stage for historic science. NASA is taking advantage of the Aug. 21, 2017 eclipse by funding 11 ground-based scientific studies. As our scientists prepare their experiments for next week, we're looking back to an historic 1860 total solar eclipse, which many think gave humanity our first glimpse of solar storms — called coronal mass ejections — 100 years before scientists first understood what they were.Scientists observed these eruptions in the 1970s during the beginning of the modern satellite era, when satellites in space were able to capture thousands of images of solar activity that had never been seen before. But in hindsight, scientists realized their satellite images might not be the first record of these solar storms. Hand-drawn records of an 1860 total solar eclipse bore surprising resemblance to these groundbreaking satellite images.Eclipse archive imagery from: http://mlso.hao.ucar.edu/hao-eclipse-archive.php || ", "hits": 43 }, { "id": 12687, "url": "https://svs.gsfc.nasa.gov/12687/", "result_type": "Produced Video", "release_date": "2017-08-15T12:00:00-04:00", "title": "NASA and ESA Spacecraft Track a Solar Storm Through Space", "description": "This animation follows the October 14, 2014 CME as it moves through the solar system and identifies a few of the NASA and ESA missions that observed it.Music: “Comely\" from FelicityWritten and produced by Lars LeonhardWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || CME_Solar_System_Still.jpg (3840x2160) [555.5 KB] || CME_Solar_System_Still_searchweb.png (320x180) [38.4 KB] || CME_Solar_System_Still_thm.png (80x40) [4.0 KB] || 12687_CME_Solar_System_1080p.mov (1920x1080) [90.8 MB] || 12687_CME_Solar_System_FINAL_appletv.m4v (1280x720) [71.7 MB] || 12687_CME_Solar_System_1080p.webm (1920x1080) [10.4 MB] || 12687_CME_Solar_System_FINAL_appletv_subtitles.m4v (1280x720) [71.7 MB] || FACEBOOK_720_12687_CME_Solar_System_FINAL_facebook_720.mp4 (1280x720) [158.9 MB] || 12687_CME_Solar_System_SRT_Captions.en_US.srt [1.2 KB] || 12687_CME_Solar_System_SRT_Captions.en_US.vtt [1.2 KB] || 12687_CME_Solar_System_-4K.mov (3840x2160) [287.7 MB] || 12687_CME_Solar_System_Apple_Devices_4K.m4v (3840x2160) [340.2 MB] || YOUTUBE_4K_12687_CME_Solar_System_FINAL_youtube_4k.mp4 (3840x2160) [627.2 MB] || 12687_CME_Solar_System_ProRes_3840x2160_2997.mov (3840x2160) [2.5 GB] || ", "hits": 66 }, { "id": 4526, "url": "https://svs.gsfc.nasa.gov/4526/", "result_type": "Infographic", "release_date": "2017-01-12T00:00:00-05:00", "title": "Ye Olde Tyme Heliophysics Map", "description": "Basic Olde Tyme Heliophysics Map. || OldeTimeHelioMapv4_print.jpg (1024x574) [245.1 KB] || OldeTimeHelioMapv4_searchweb.png (180x320) [110.2 KB] || OldeTimeHelioMapv4_thm.png (80x40) [7.6 KB] || OldeTimeHelioMapv4.pptx [6.5 MB] || OldeTimeHelioMapv4.tif (7819x4386) [98.1 MB] || OldeTimeHelioMapv4.key [98.8 MB] || ye-olde-tyme-heliophysics-map.hwshow || ", "hits": 39 }, { "id": 12390, "url": "https://svs.gsfc.nasa.gov/12390/", "result_type": "Produced Video", "release_date": "2016-10-17T16:00:00-04:00", "title": "NASA's STEREO Solar Probes 10th Anniversary Live Shots", "description": "B-roll that corresponds with the live shots. || B-Roll_2.00001_print.jpg (1024x576) [130.4 KB] || B-Roll_2.00001_searchweb.png (320x180) [78.8 KB] || B-Roll_2.00001_web.png (320x180) [78.8 KB] || B-Roll_2.00001_thm.png (80x40) [6.6 KB] || B-Roll.webm (1280x720) [19.6 MB] || B-Roll_2.webm (1280x720) [19.5 MB] || B-Roll_2.mov (1280x720) [3.1 GB] || ", "hits": 42 }, { "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": 107 }, { "id": 4469, "url": "https://svs.gsfc.nasa.gov/4469/", "result_type": "Visualization", "release_date": "2016-06-16T15:00:00-04:00", "title": "Dynamic Earth-A New Beginning", "description": "The visualization 'Excerpt from \"Dynamic Earth\"' has been one of the most popular visualizations that the Scientific Visualization Studio has ever created. It's often used in presentations and Hyperwall shows to illustrate the connections between the Earth and the Sun, as well as the power of computer simulation in understanding those connections.There is one part of this visualization, however, that has always seemed a little clumsy to us. The opening shot is a pullback from the limb of the sun, where the sun is represented by a movie of 304 Angstrom images from the Solar Dynamics Observatory (SDO). It is difficult to pull back from the limb of a flat sun image and make the sun look spherical, and the problem was made more difficult because the original sun images were in a spherical dome show format. As a result, the pullback from the sun showed some odd reprojection artifacts.The best solution to this issue was to replace the existing pullout with a new one, one which pulled directly out from the center of the solar disk. For the new beginning, we chose a series of SDO images in the 171 Angstrom channel that show a visible coronal mass ejection (CME) in the lower right corner of the solar disk. Although this is not the specific CME that is seen affecting Venus and Earth later in this visualization, its presence links the SDO animation thematically to the later solar storm. The SDO images were also brightened considerably and tinted yellow to match the common perception of the Sun as a bright yellow object (even though it is actually white).Please go to the original version of this visualization to see the complete credits and additional details. || ", "hits": 64 }, { "id": 12281, "url": "https://svs.gsfc.nasa.gov/12281/", "result_type": "Produced Video", "release_date": "2016-06-10T18:00:00-04:00", "title": "Instagram: Solar Storms May Have Been Key to Life on Earth", "description": "Our sun's adolescence was stormy—and new evidence shows that these tempests may have been just the key to seeding life as we know it.Some 4 billion years ago, the sun shone with only about three-quarters the brightness we see today, but its surface roiled with giant eruptions spewing enormous amounts of solar material and radiation out into space. These powerful solar explosions may have provided the crucial energy needed to warm Earth, despite the sun's faintness. The eruptions also may have furnished the energy needed to turn simple molecules into the complex molecules such as RNA and DNA that were necessary for life. The research was published in Nature Geoscience on May 23, 2016, by a team of scientists from NASA.Understanding what conditions were necessary for life on our planet helps us both trace the origins of life on Earth and guide the search for life on other planets. Until now, however, fully mapping Earth's evolution has been hindered by the simple fact that the young sun wasn't luminous enough to warm Earth.\"Back then, Earth received only about 70 percent of the energy from the sun than it does today,\" said Vladimir Airapetian, lead author of the paper and a solar scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. \"That means Earth should have been an icy ball. Instead, geological evidence says it was a warm globe with liquid water. We call this the Faint Young Sun Paradox. Our new research shows that solar storms could have been central to warming Earth.\" || ", "hits": 91 }, { "id": 11853, "url": "https://svs.gsfc.nasa.gov/11853/", "result_type": "Produced Video", "release_date": "2016-05-23T11:00:00-04:00", "title": "The Faint Young Star Paradox: Solar Storms May Have Been Key to Life on Earth", "description": "Energy from our young sun – 4 billion years ago -- aided in creating molecules in Earth's atmosphere that allowed it to warm up enough to incubate life. Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || faintyoung.jpg (1280x720) [105.6 KB] || faintyoung_searchweb.png (320x180) [81.4 KB] || faintyoung_thm.png (80x40) [15.3 KB] || WEBM_G2015-036_FaintYoungStarParadox_V2.webm (960x540) [39.6 MB] || G2015-036_FaintYoungStarParadox_V2.mov (1920x1080) [1.4 GB] || APPLE_TV_G2015-036_FaintYoungStarParadox_V2_appletv.m4v (1280x720) [54.0 MB] || YOUTUBE_HQ_G2015-036_FaintYoungStarParadox_V2_youtube_hq.mov (1920x1080) [318.5 MB] || NASA_TV_G2015-036_FaintYoungStarParadox_V2.mpeg (1280x720) [346.1 MB] || PRORES_B-ROLL_G2015-036_FaintYoungStarParadox_V2_prores.mov (1280x720) [719.8 MB] || APPLE_TV_G2015-036_FaintYoungStarParadox_V2_appletv_subtitles.m4v (1280x720) [54.0 MB] || G2015-036FaintYoungStarParadox_V2.en_US.srt [1.8 KB] || G2015-036FaintYoungStarParadox_V2.en_US.vtt [1.8 KB] || NASA_PODCAST_G2015-036_FaintYoungStarParadox_V2_ipod_sm.mp4 (320x240) [18.8 MB] || G2015-036_FaintYoungStarParadox_V2_lowres.mp4 (480x272) [14.8 MB] || ", "hits": 155 }, { "id": 12239, "url": "https://svs.gsfc.nasa.gov/12239/", "result_type": "Produced Video", "release_date": "2016-05-12T13:00:00-04:00", "title": "MMS First Results", "description": "This short video outlines the MMS mission and its first results. Since it launched, MMS has made more than 4,000 trips through the magnetic boundaries around Earth, each time gathering information about the way the magnetic fields and particles move. A surprising result was that at the moment of interconnection between the sun’s magnetic field lines and those of Earth the crescents turned abruptly so that the electrons flowed along the field lines. By watching these electron tracers, MMS made the first observation of the predicted breaking and interconnection of magnetic fields in space. Credit: NASA/GSFCWatch this video on the NASA Goddard YouTube channel. || mmsthumb.jpg (1280x720) [139.4 KB] || mmsthumb_print.jpg (1024x576) [161.8 KB] || mmsthumb_searchweb.png (320x180) [104.3 KB] || mmsthumb_web.png (320x180) [104.3 KB] || mmsthumb_thm.png (80x40) [6.8 KB] || 12239_MMS_First_ResultsV2_appletv.m4v (1280x720) [76.9 MB] || 12239_MMS_First_ResultsV2.webm (1920x1080) [18.1 MB] || 12239_MMS_First_ResultsV2_appletv_subtitles.m4v (1280x720) [77.0 MB] || 12239_MMS_First_ResultsV2.en_US.srt [3.0 KB] || 12239_MMS_First_ResultsV2.en_US.vtt [3.0 KB] || YOUTUBE_HQ_12239_MMS_First_ResultsV2_youtube_hq.mov (1920x1080) [1.1 GB] || 12239_MMS_First_ResultsV2_lowres.mp4 (480x272) [21.6 MB] || 12239_MMS_First_ResultsV2_ipod_sm.mp4 (320x240) [26.3 MB] || PRORES_B-ROLL_12239_MMS_First_ResultsV2_prores.mov (1280x720) [2.2 GB] || 12239_MMS_First_ResultsV2.mov (1920x1080) [4.2 GB] || YOUTUBE_HQ_12239_MMS_First_ResultsV2_youtube_hq.mov.hwshow [100 bytes] || ", "hits": 130 }, { "id": 12165, "url": "https://svs.gsfc.nasa.gov/12165/", "result_type": "Produced Video", "release_date": "2016-03-03T17:00:00-05:00", "title": "2016 Total Solar Eclipse Live Shots", "description": "Solar Eclipse Live Shot Roll-ins || Solar_Eclipse_Rollins_h264_print.jpg (1024x576) [28.9 KB] || Solar_Eclipse_Rollins.webmhd.webm (1280x720) [23.6 MB] || Solar_Eclipse_Rollins_h264.mov (1280x720) [499.9 MB] || Solar_Eclipse_Rollins.mov (1280x720) [1.7 GB] || ", "hits": 35 }, { "id": 12151, "url": "https://svs.gsfc.nasa.gov/12151/", "result_type": "Produced Video", "release_date": "2016-02-12T13:00:00-05:00", "title": "NASA On Air: NASA's SDO Satellite Captures HD Time Lapse Of The Sun (2/12/2016)", "description": "LEAD: NASA's Solar Dynamics Observatory catches the sun in HD video. 1: Images shown here are in the extreme ultraviolet range. 2: The temperature of the solar material is near 1 million degrees F.3: It's easy to see the sun's rotation, 1 full rotation every 25 days. TAG: Scientists study these images to better understand the solar flares and solar explosions called coronal mass ejections that can sometimes disrupt our technology such as GPS systems. || IPAD_DELIVERABLES_NASAonAir-SDOYr6-_iPad_1920x1080_print.jpg (1024x576) [97.7 KB] || IPAD_DELIVERABLES_NASAonAir-SDOYr6-_iPad_1920x1080_searchweb.png (320x180) [52.5 KB] || IPAD_DELIVERABLES_NASAonAir-SDOYr6-_iPad_1920x1080_thm.png (80x40) [4.2 KB] || WSI_WEATHER_CHANNEL_NASAonAir-SDOYr6-_1920x1080.mov (1920x1080) [681.2 MB] || WSI_WEATHER_CHANNEL_NASAonAir-SDOYr6-_1280x720.mov (1280x720) [737.5 MB] || NBC_TODAY_NASAonAir-SDOYr6-_NBC_Today.mov (1920x1080) [75.4 MB] || WeatherChannel_NASAonAir-SDOYr6-WeatherChannel.wmv (1280x720) [7.4 MB] || Accuweather_NASAonAir-SDOYr6-Accuweather.avi (1280x720) [5.8 MB] || BARON_SERVICE_NASAonAir-SDOYr6-_baron.mp4 (1920x1080) [25.9 MB] || WC_PRORES_422_NASAonAir-SDOYr6-_prores.mov (1920x1080) [508.1 MB] || IPAD_DELIVERABLES_NASAonAir-SDOYr6-_iPad_960x540.m4v (960x540) [31.3 MB] || IPAD_DELIVERABLES_NASAonAir-SDOYr6-_iPad_1280x720.m4v (1280x720) [58.8 MB] || IPAD_DELIVERABLES_NASAonAir-SDOYr6-_iPad_1920x1080.m4v (1920x1080) [94.0 MB] || WEBM_NASAonAir-SDOYr6-.webm (960x540) [14.3 MB] || ", "hits": 166 }, { "id": 4422, "url": "https://svs.gsfc.nasa.gov/4422/", "result_type": "Visualization", "release_date": "2016-02-12T09:30:00-05:00", "title": "SDO Year 6: A Year of the Sun", "description": "A year of SDO solar observations in HD1080. || SDOYear6hourly_171A_stand.HD1080i.02000_print.jpg (1024x576) [64.8 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || SDOYear6hourly_171A.HD1080.webm (1920x1080) [37.4 MB] || SDOYear6hourly_171A_1080p30.mp4 (1920x1080) [424.4 MB] || SDOYear6hourly_171A.HD1080.mov (1920x1080) [1.1 GB] || SDOYear6hourly_171A_1080p30.mp4.hwshow [193 bytes] || ", "hits": 90 }, { "id": 4319, "url": "https://svs.gsfc.nasa.gov/4319/", "result_type": "Visualization", "release_date": "2016-02-11T00:00:00-05:00", "title": "Solar Dynamics Observatory: April 21, 2015 Eruption on the Solar Limb", "description": "Movie of plasma eruption (upper left limb). || Apr2015LimbErupt_304A_stand.HD1080i.00945_print.jpg (1024x576) [73.9 KB] || Apr2015LimbErupt_304A_stand.HD1080i.00945_searchweb.png (320x180) [41.0 KB] || Apr2015LimbErupt_304A_stand.HD1080i.00945_thm.png (80x40) [3.5 KB] || Apr2015LimbErupt_304A_stand_1080p.webm (1920x1080) [6.4 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Apr2015LimbErupt_304A_stand_1080p.mp4 (1920x1080) [43.2 MB] || Apr2015LimbErupt_304A_stand_1080p.mp4.hwshow [199 bytes] || ", "hits": 62 }, { "id": 4323, "url": "https://svs.gsfc.nasa.gov/4323/", "result_type": "Visualization", "release_date": "2016-02-11T00:00:00-05:00", "title": "Summer Sun from SDO: Eruption and Coronal Loops on the Solar Limb", "description": "HD1080 movie of the Sun in the AIA 304 angstrom filter. Note the coronal loop structures on the lower right limb. || June2015LimbLoops_304A_stand.HD1080i.00256_print.jpg (1024x576) [68.0 KB] || June2015LimbLoops_304A_1080p.webm (1920x1080) [5.1 MB] || June2015LimbLoops_304AHD (1920x1080) [128.0 KB] || June2015LimbLoops_304A_1080p.mp4 (1920x1080) [34.7 MB] || June2015LimbLoops_304A.HD1080.mov (1920x1080) [108.5 MB] || June2015LimbLoops_304A_1080p.mp4.hwshow [228 bytes] || ", "hits": 50 }, { "id": 4392, "url": "https://svs.gsfc.nasa.gov/4392/", "result_type": "Visualization", "release_date": "2015-12-08T10:00:00-05:00", "title": "Space Weather to the Edge of the Solar System", "description": "Cropped view of the Enlil model from early 2015 to just after the New Horizons flyby of Pluto. || NewHorizons2015_40AU.NoSTEREO_1080p30.01000_print.jpg (1024x576) [72.7 KB] || NewHorizons2015_40AU.NoSTEREO_1080p30.mp4 (1920x1080) [27.9 MB] || NewHorizons2015_40AU.NoSTEREO_1080p30.webm (1920x1080) [6.6 MB] || NewHorizons2015_40AU.NoSTEREO.3840x2160_p30.mp4 (3840x2160) [82.5 MB] || 5760x3240_16x9_30p (5760x3240) [0 Item(s)] || NoSTEREO (3840x2160) [0 Item(s)] || space-weather-to-the-edge-of-the-solar-system-hd1080-movie.hwshow [336 bytes] || ", "hits": 75 }, { "id": 12052, "url": "https://svs.gsfc.nasa.gov/12052/", "result_type": "Produced Video", "release_date": "2015-12-01T10:00:00-05:00", "title": "SOHO Celebrates 20 Years of Space-based Science", "description": "Dr. Joe Gurman of NASA's Goddard Space Flight Center provides commentary on selected shots from SOHO's 20 years in space.Watch this video on YouTube || SOHO20thumb.jpg (1280x720) [108.1 KB] || SOHO20thumb_searchweb.png (320x180) [119.7 KB] || SOHO20thumb_thm.png (80x40) [19.1 KB] || APPLE_TV_12952_SOHO_20th_anniversary_ws_appletv.m4v (1280x720) [199.6 MB] || YOUTUBE_HQ_12952_SOHO_20th_anniversary_ws_youtube_hq.mov (1920x1080) [2.5 GB] || 12952_SOHO_20th_anniversary_ws-H264_Best_1920x1080_59.94.mov (1920x1080) [4.0 GB] || YOUTUBE_HQ_12952_SOHO_20th_anniversary_ws_youtube_hq.webm (1920x1080) [45.1 MB] || SOHO20.en_US.srt [7.6 KB] || 12952_SOHO_20th_anniversary_ws.key [200.0 MB] || 12952_SOHO_20th_anniversary_ws.pptx [199.8 MB] || 12952_SOHO_20th_anniversary_ws_lowres.mp4 (480x272) [52.9 MB] || NASA_PODCAST_12952_SOHO_20th_anniversary_ws_ipod_sm.mp4 (320x240) [67.5 MB] || ", "hits": 62 }, { "id": 12071, "url": "https://svs.gsfc.nasa.gov/12071/", "result_type": "Produced Video", "release_date": "2015-11-30T17:00:00-05:00", "title": "SOHO Anniversary Live Shot Page", "description": "B-roll for SOHO live shot || SOHO_Broadcast_broll_youtube_print.jpg (1024x576) [98.3 KB] || SOHO_Broadcast_broll_youtube_searchweb.png (320x180) [63.4 KB] || SOHO_Broadcast_broll_youtube_thm.png (80x40) [4.9 KB] || SOHO_Broadcast_broll_prores.mov (1280x720) [2.2 GB] || SOHO_Broadcast_broll_youtube.mp4 (1280x720) [250.3 MB] || SOHO_Broadcast_broll_youtube.webm (1280x720) [15.2 MB] || ", "hits": 29 }, { "id": 12040, "url": "https://svs.gsfc.nasa.gov/12040/", "result_type": "Produced Video", "release_date": "2015-11-04T16:00:00-05:00", "title": "NASA Observes Auroras Across Canada", "description": "These aurora images were taken from the ground looking up with a network of all-sky cameras spread across Canada, studying auroras in collaboration with NASA’s Time History of Events and Macroscale Interactions during Substorms, or THEMIS, mission. Taking images of aurora from the ground in conjunction with satellite data taken from above the atmosphere gives scientists a more comprehensive picture of how and why the aurora form. The ground-based camera network is also observing this week’s auroras. The aurora data is provided courtesy of S. Mende at University California Berkeley and E. Donovan at the University of Calgary, logistical support in fielding and data retrieval from the ground-based stations is provided by the Canadian Space Agency. The array of aurora images is funded by NSF in support of GIMNAST through grant AGS-1004736.Credit: NASA/CSA/University of California, Berkeley/University of Calgary/NSF || Storm_0386.jpg (1944x1080) [1.4 MB] || Storm_0386_print.jpg (1024x568) [476.9 KB] || Storm_0386_searchweb.png (180x320) [150.3 KB] || Storm_0386_thm.png (80x40) [33.8 KB] || 1944x1080_16x9_20p (1944x1080) [128.0 KB] || Auroras_Across_Canada-MPEG4_1944x1080_24.mp4 (1944x1080) [54.0 MB] || Auroras_Across_Canada_ProRes_1944x1080_24.webm (1944x1080) [10.3 MB] || Auroras_Across_Canada_ProRes_1944x1080_24.mov (1944x1080) [1.4 GB] || Auroras_Across_Canada-H264_Best_1944x1080_24.mov (1944x1080) [658.5 MB] || Auroras_Across_Canada-H264_Good_1944x1080_24.mov (1944x1080) [130.4 MB] || Auroras_Across_Canada.hwshow [223 bytes] || ", "hits": 44 }, { "id": 12034, "url": "https://svs.gsfc.nasa.gov/12034/", "result_type": "Produced Video", "release_date": "2015-11-01T08:00:00-05:00", "title": "NASA Enters World of 4K Video", "description": "The solar system? Big. The galaxy? Bigger. What's bigger than that? Before you smugly suggest \"The universe?\", check this out: 4K Videos from NASA!A little more than a decade ago, television transformed from the boxy, standard definition dimensions of 20th century engineers to the wider and sharper images of high definition TV. Well into the 21st century now, rapid growth in the next generation of video images promises to deliver spectacular pictures with profoundly greater fidelity and resolution than even the best HDTV. Officially known as Ultra-High Definition Television, it has rapidly come to be known as \"4K\", a moniker derived from the approximate width of images measured in pixels horizontally across a screen.NASA has a long legacy pushing the boundaries of advanced media technologies, befitting its unique role in presenting important, state-of-the-art science and engineering stories to the American public. On this web page you'll find the first major release of 4K video content, presented in the public domain. The release of these media are concurrent with the launch of a new, non-commercial Ultra-High Definition channel in partnership with Harmonic. For each of the following items on this website you may preview the program in your browser or you may select one of several different resolutions from the \"download\" button in the lower right hand corner of each. Be advised that the 4K videos will require fast internet connections and substantial storage space.SYNTHESIS: NASA DATA VISUALIZATIONS IN ULTRA-HD (4K) || ", "hits": 993 }, { "id": 11941, "url": "https://svs.gsfc.nasa.gov/11941/", "result_type": "Produced Video", "release_date": "2015-07-10T11:00:00-04:00", "title": "Tracking Space Weather for New Horizons with an Enlil Model", "description": "Dr. Leila Mays explains a space weather model that depicts conditions experienced by the New Horizons mission. Watch this video on the NASAexplorer YouTube channel.0 || enlil_thumb.jpg (1280x720) [60.5 KB] || enlil_thumb_searchweb.png (320x180) [79.7 KB] || enlil_thumb_thm.png (80x40) [17.0 KB] || G2015-058_newhorizonsEnlil.mov (1920x1080) [3.3 GB] || G2015-058_newhorizonsEnlil.webm (1920x1080) [12.6 MB] || G2015-058_newhorizonsEnlil.en_US.srt [2.2 KB] || G2015-058_newhorizonsEnlil.en_US.vtt [2.2 KB] || ", "hits": 32 }, { "id": 11942, "url": "https://svs.gsfc.nasa.gov/11942/", "result_type": "Produced Video", "release_date": "2015-07-02T11:00:00-04:00", "title": "NASA On Air: NASA's SDO Catches Arching Solar Eruption (7/2/2015)", "description": "LEAD: NASA caught a spectacular solar eruption this June. 1. The solar explosion threw out a giant cloud of solar material. 2. The activity is shown here in ultraviolet light that has been colorized in red. TAG: The surface temperature of the sun is over 10,000 degrees Fahrenheit. || WC_SDO_Solar_Eruption-iPad3_10_print.jpg (1024x576) [91.8 KB] || WC_SDO_Solar_Eruption-iPad3_10_searchweb.png (320x180) [78.9 KB] || WC_SDO_Solar_Eruption-iPad3_10_thm.png (80x40) [6.0 KB] || WC_SDO_Solar_Eruption_Weather_Channel_30_fps.mov (1920x1080) [832.9 MB] || WC_SDO_Solar_Eruption_Weather_Channel_60_fps.mov (1280x720) [969.5 MB] || WC_SDO_Solar_Eruption_NBC_Today.mov (1920x1080) [370.8 MB] || WC_SDO_Solar_Eruption-MASTER_4.wmv (1280x720) [5.4 MB] || WC_SDO_Solar_Eruption-Accuweather_5.avi (1280x720) [4.3 MB] || WC_SDO_Solar_Eruption_Baron_Services_MP4.mp4 (1920x1080) [14.0 MB] || WC_SDO_Solar_Eruption_APR_422_1920_30.mov (1920x1080) [299.1 MB] || WC_SDO_Solar_Eruption-iPad1_8.m4v (960x540) [8.4 MB] || WC_SDO_Solar_Eruption-iPad1_8.webm (960x540) [2.0 MB] || WC_SDO_Solar_Eruption-iPad3_10.webm (1920x1080) [2.0 MB] || WC_SDO_Solar_Eruption-iPad2_9.m4v (1280x720) [4.6 MB] || WC_SDO_Solar_Eruption-iPad3_10.m4v (1920x1080) [5.8 MB] || ", "hits": 49 }, { "id": 11908, "url": "https://svs.gsfc.nasa.gov/11908/", "result_type": "Produced Video", "release_date": "2015-06-30T11:00:00-04:00", "title": "Arching Eruption", "description": "Watch this video on the NASAexplorer YouTube channel.0 || june18.15thumb.jpg (720x480) [57.9 KB] || june18.15thumb_searchweb.png (320x180) [89.0 KB] || june18.15thumb_thm.png (80x40) [22.6 KB] || G2015-054ArchingEruption.mov (1920x1080) [2.9 GB] || G2015-054ArchingEruption-H264_Good_1080_29.97-1.mov (1920x1080) [253.1 MB] || G2015-054ArchingEruption-H264_Good_1080_29.97-1.webm (1920x1080) [11.9 MB] || G2015-054ArchingEruption-H264_Good_1080_29.en_US.srt [914 bytes] || G2015-054ArchingEruption-H264_Good_1080_29.en_US.vtt [927 bytes] || ", "hits": 80 }, { "id": 11897, "url": "https://svs.gsfc.nasa.gov/11897/", "result_type": "Produced Video", "release_date": "2015-06-26T14:00:00-04:00", "title": "A Slice of Light: How IRIS Observes the Sun", "description": "Watch this video on the NASAexplorer YouTube channel.0 || IRISthumb.jpg (720x480) [26.9 KB] || IRISthumb_searchweb.png (320x180) [44.2 KB] || IRISthumb_thm.png (80x40) [15.0 KB] || G2015-050_How_IRIS_Sees_Sun_appletv.m4v (960x540) [32.0 MB] || G2015-050_How_IRIS_Sees_Sun_youtube_hq.mov (1920x1080) [100.4 MB] || G2015-050_How_IRIS_Sees_Sun.mov (1920x1080) [2.0 GB] || G2015-050_How_IRIS_Sees_Sun_1280x720.wmv (1280x720) [32.4 MB] || G2015-050_How_IRIS_Sees_Sun_prores.mov (1280x720) [1.0 GB] || G2015-050_How_IRIS_Sees_Sun.webm (1920x1080) [8.5 MB] || G2015-050_How_IRIS_Sees_Sun_appletv_subtitles.m4v (960x540) [31.9 MB] || G2015-050_How_IRIS_Sees_Sun_ipod_lg.m4v (640x360) [12.8 MB] || G2015-050_How_IRIS_Sees_Sun.en_US.vtt [1.3 KB] || G2015-050_How_IRIS_Sees_Sun.en_US.srt [1.3 KB] || G2015-050_How_IRIS_Sees_Sun_ipod_sm.mp4 (320x240) [6.8 MB] || ", "hits": 79 }, { "id": 4322, "url": "https://svs.gsfc.nasa.gov/4322/", "result_type": "Visualization", "release_date": "2015-06-24T00:00:00-04:00", "title": "The Multiple CMEs of June, 2015", "description": "A view of multiple CMEs which erupted from the Sun in the latter half of June 2015. Their trajectories, and potential impacts on Earth and space assets, are propagated with the Enlil model. || 2015June20_high2AU.full.0006_print.jpg (1024x576) [48.8 KB] || 2015June20_high2AU.full.0006_searchweb.png (320x180) [38.5 KB] || 2015June20_high2AU.full.0006_thm.png (80x40) [4.7 KB] || 2015June20_high2AU.full.HD1080.webm (1920x1080) [406.6 KB] || 2015June20_high2AU.full.HD1080.mov (1920x1080) [1.8 MB] || 1920x1080_16x9_10p (1920x1080) [4.0 KB] || ", "hits": 45 }, { "id": 11905, "url": "https://svs.gsfc.nasa.gov/11905/", "result_type": "Produced Video", "release_date": "2015-06-23T12:00:00-04:00", "title": "Space Weather Imagery of June 22 - 23, 2015 Events", "description": "The sun emitted a CME and mid-level solar flare, peaking at 2:23 p.m. EDT, on June 22, 2015. Again on June 25, 2015, a mid-level solar flare peaked at 4:16 a.m. EDT.NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel. To see how this event may affect Earth, please visit NOAA's Space Weather Prediction Center at http://spaceweather.gov, the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This first flare is classified as an M6.6 flare and the second was M7.9. M-class flares are a tenth the size of the most intense flares, the X-class flares. The number provides more information about its strength. An M2 is twice as intense as an M1, an M3 is three times as intense, etc. || ", "hits": 57 }, { "id": 11868, "url": "https://svs.gsfc.nasa.gov/11868/", "result_type": "Produced Video", "release_date": "2015-05-06T09:45:00-04:00", "title": "NASA's SDO Observes a Cinco de Mayo Solar Flare", "description": "Video of May 5, 2015 X2.7 flare.Credit: NASA/GSFC/SDO || May_5_2015_Flare_Still_304-171.png (1920x1080) [8.1 MB] || May_5_2015_Flare_Still_304-171.jpg (1920x1080) [415.9 KB] || May_5_2015_Flare_Still_304-171_print.jpg (1024x576) [145.7 KB] || May_5_2015_Flare_Still_304-171_web.png (320x180) [83.3 KB] || 11868_May_5_X_Flare_MPEG4_1920X1080_2997.mp4 (1920x1080) [42.2 MB] || 11868_May_5_X_Flare_H264_Good_1920x1080_2997.webm (1920x1080) [4.8 MB] || 11868_May_5_X_Flare_1280x720.wmv (1280x720) [23.1 MB] || 11868_May_5_X_Flare_appletv.m4v (960x540) [19.0 MB] || 11868_May_5_X_Flare_appletv_subtitles.m4v (960x540) [19.0 MB] || 11868_May_5_X_Flare_ipod_lg.m4v (640x360) [7.1 MB] || 11868_May_5_X_Flare_ipod_sm.mp4 (320x240) [3.6 MB] || 11868_May_5_X_Flare_SRT_Captions.en_US.srt [230 bytes] || 11868_May_5_X_Flare_SRT_Captions.en_US.vtt [243 bytes] || 11868_May_5_X_Flare_ProRes_1920x1080_2997.mov (1920x1080) [674.9 MB] || 11868_May_5_X_Flare_H264_Best_1920x1080_2997.mov (1920x1080) [682.7 MB] || 11868_May_5_X_Flare_H264_Good_1920x1080_2997.mov (1920x1080) [219.1 MB] || ", "hits": 65 }, { "id": 11864, "url": "https://svs.gsfc.nasa.gov/11864/", "result_type": "Produced Video", "release_date": "2015-05-01T13:00:00-04:00", "title": "Phoenix Prominence Eruption", "description": "Edited video of a solar prominence seen by NASA's Solar Dynamics Observatory on April 21, 2015. Watch this video on the NASAexplorer YouTube channel. || phoenix.prominence.jpg (1920x1080) [107.6 KB] || phoenix.prominence_searchweb.png (320x180) [87.5 KB] || phoenix.prominence_thm.png (80x40) [23.2 KB] || G2015-042_4.21.Phoenix_Eruption_appletv.m4v (960x540) [61.1 MB] || G2015-042_4.21.Phoenix_Eruption.mpeg (1280x720) [479.4 MB] || G2015-042_4.21.Phoenix_Eruption_prores.mov (1280x720) [2.0 GB] || G2015-042_4.21.Phoenix_Eruption_1280x720.wmv (1280x720) [70.7 MB] || G2015-042_4.21.Phoenix_Eruption_youtube_hq.mov (1920x1080) [227.2 MB] || G2015-042_4.21.Phoenix_Eruption_appletv.webm (960x540) [15.9 MB] || G2015-042_4.21.Phoenix_Eruption_appletv_subtitles.m4v (960x540) [61.1 MB] || G2015-042_4.21.Phoenix_Eruption_ipod_lg.m4v (640x360) [24.2 MB] || phoenix.prominence.en_US.srt [1.2 KB] || phoenix.prominence.en_US.vtt [1.2 KB] || G2015-042_4.21.Phoenix_Eruption_ipod_sm.mp4 (320x240) [13.0 MB] || ", "hits": 176 }, { "id": 11811, "url": "https://svs.gsfc.nasa.gov/11811/", "result_type": "Produced Video", "release_date": "2015-03-17T13:15:00-04:00", "title": "SOHO Observes March 14 Coronal Mass Ejection", "description": "The Joint ESA/NASA Solar and Heliospheric Observatory, or SOHO, captured this image series of a coronal mass ejection, or CME, on March 14, 2015. || JHV_movie_created_2015-03-17_19.37.12_print.jpg (1024x576) [73.7 KB] || JHV_movie_created_2015-03-17_19.37.12_searchweb.png (320x180) [48.6 KB] || JHV_movie_created_2015-03-17_19.37.12_web.png (320x180) [48.6 KB] || JHV_movie_created_2015-03-17_19.37.12.webm (1920x1080) [334.4 KB] || JHV_movie_created_2015-03-17_19.37.12.mp4 (1920x1080) [9.0 MB] || ", "hits": 52 }, { "id": 11794, "url": "https://svs.gsfc.nasa.gov/11794/", "result_type": "Produced Video", "release_date": "2015-03-10T12:30:00-04:00", "title": "MMS L-2 Prelaunch News Conference", "description": "On March 12 from Cape Canaveral Florida, NASA is scheduled to launch the Magnetospheric Multiscale, or MMS, mission, which will provide unprecedented detail on a phenomenon called magnetic reconnection. The process of reconnection involves the explosive release of energy when the magnetic fields around Earth connect and disconnect. These fields help protect Earth from harmful effects of solar storms and cosmic rays. Magnetic reconnection also occurs throughout the universe and can accelerate particles up to nearly the speed of light.By studying reconnection in this local, natural laboratory, MMS helps us understand reconnection elsewhere as well, such as in the atmosphere of the Sun and other stars, in the vicinity of black holes and neutron stars, and at the boundary between our solar system's heliosphere and interstellar space.MMS consists of four identical observatories that will provide the first three-dimensional view of magnetic reconnection. The four MMS observatories will fly through reconnection regions in a tight formation in well under a second, so key sensors on each spacecraft are designed to measure the space environment at rates faster than any previous mission.For additional visuals regarding the MMS mission and science, please see our MMS Pre-launch Gallery.Briefing participants include:Geoffrey Yoder, deputy associate administratorNASA Science Mission Directorate, WashingtonOmar Baez, NASA launch managerKennedy Space Center, FloridaVernon Thorp, program manager, NASA MissionsUnited Launch Alliance, Centennial, ColoradoCraig Tooley, NASA MMS project manager,Goddard Space Flight Center, Greenbelt, MarylandJim Burch, principal investigatorSouthwest Research Institute, San Antonio, TexasClay Flinn, launch weather officer, 45th Weather SquadronCape Canaveral Air Force Station, Florida || ", "hits": 14 }, { "id": 11780, "url": "https://svs.gsfc.nasa.gov/11780/", "result_type": "Produced Video", "release_date": "2015-02-25T14:30:00-05:00", "title": "MMS Prelaunch Press Briefing", "description": "On March 12 from Cape Canaveral Florida, NASA is scheduled to launch the Magnetospheric Multiscale, or MMS, mission, which will provide unprecedented detail on a phenomenon called magnetic reconnection. The process of reconnection involves the explosive release of energy when the magnetic fields around Earth connect and disconnect. These fields help protect Earth from harmful effects of solar storms and cosmic rays. Magnetic reconnection also occurs throughout the universe and can accelerate particles up to nearly the speed of light.By studying reconnection in this local, natural laboratory, MMS helps us understand reconnection elsewhere as well, such as in the atmosphere of the Sun and other stars, in the vicinity of black holes and neutron stars, and at the boundary between our solar system’s heliosphere and interstellar space.MMS consists of four identical observatories that will provide the first three-dimensional view of magnetic reconnection. The four MMS observatories will fly through reconnection regions in a tight formation in well under a second, so key sensors on each spacecraft are designed to measure the space environment at rates faster than any previous mission.For additional visuals regarding the MMS mission and science, please see our MMS Pre-launch Gallery. || ", "hits": 19 }, { "id": 10204, "url": "https://svs.gsfc.nasa.gov/10204/", "result_type": "Produced Video", "release_date": "2015-02-18T11:30:00-05:00", "title": "MMS Mission Overview", "description": "Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || missionoverview_print.jpg (1024x576) [146.3 KB] || missionoverview.jpg (1280x720) [125.0 KB] || missionoverview_thm.png (80x40) [16.6 KB] || missionoverview_web.png (320x180) [72.7 KB] || missionoverview_searchweb.png (320x180) [72.7 KB] || missionoverview_web.jpg (320x180) [28.5 KB] || G2014-103_MMS_Mission_OverviewMASTER_appletv.webm (960x540) [31.6 MB] || G2014-103_MMS_Mission_OverviewMASTER_appletv_subtitles.m4v (960x540) [117.8 MB] || G2014-103_MMS_Mission_OverviewMASTER_youtube_hq.mov (1280x720) [183.1 MB] || G2014-103_MMS_Mission_OverviewMASTER_appletv.m4v (960x540) [117.9 MB] || G2014-103_MMS_Mission_OverviewMASTER_1280x720.wmv (1280x720) [136.2 MB] || G2014-103_MMS_Mission_OverviewMASTER_ipod_lg.m4v (640x360) [47.2 MB] || G2014-103_MMS_Mission_OverviewMASTER.en_US.vtt [5.6 KB] || G2014-103_MMS_Mission_OverviewMASTER.en_US.srt [5.6 KB] || G2014-103_MMS_Mission_OverviewMASTER_nasaportal.mov (640x360) [109.7 MB] || G2014-103_MMS_Mission_OverviewMASTER_ipod_sm.mp4 (320x240) [25.0 MB] || G2014-103_MMS_Mission_OverviewMASTER_prores.mov (1280x720) [4.3 GB] || ", "hits": 149 }, { "id": 4125, "url": "https://svs.gsfc.nasa.gov/4125/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "The Fast X4 Flare from February 2014", "description": "The Sun launches a fast X-ray flare in late February 2014 and is seen by the Solar Dynamics Observatory (SDO). The eruption sends a bright ribbon of plasma off the limb of the Sun. || ", "hits": 24 }, { "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": 51 }, { "id": 4182, "url": "https://svs.gsfc.nasa.gov/4182/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "Double Solar Flare of June 10, 2014 as Seen by SDO", "description": "Multiple flares erupted from the same active region just a few hours apart on June 10, 2014. The first flare, an M-class, erupted near the limb of the sun. Within a couple of hours, two more X-class flares erupted (see Classifying Solar Eruptions) peaked at 12:52UT. A number of smaller flares erupted from the same region before and after the largest events. || ", "hits": 30 }, { "id": 4202, "url": "https://svs.gsfc.nasa.gov/4202/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "August 24, 2014: Magnificent M-flare", "description": "M-flares are not the most powerful flares the Sun can emit, but sometimes even they can exhibit visually exciting behavior.Here we show the lead-up to an M-flare which lauches a large amount of plasma into space. The eruption takes place starting around 12:00 UTC and launches over the next 15 minutes. But stay with it, and you'll also see some of the plasma falling back towards the Sun around 13:50 UTC. || ", "hits": 30 }, { "id": 4211, "url": "https://svs.gsfc.nasa.gov/4211/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "Just over the Limb Solar Event captured by SDO and IRIS", "description": "On May 9, 2014, an active region has just rotated over the limb of the Sun when it launches a large amount of plasma into space. Both SDO and IRIS caught the event. || ", "hits": 30 }, { "id": 4216, "url": "https://svs.gsfc.nasa.gov/4216/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "September 2014 X-Flare", "description": "On September 10, 2014, the sun erupts with an X-flare of intensity X1.6 in the center of the solar disk. The event also launches a coronal mass ejection earthward. || ", "hits": 53 }, { "id": 4235, "url": "https://svs.gsfc.nasa.gov/4235/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "October X-flare from Solar Dynamics Observatory", "description": "Active Region AR12192 erupts with an X-class flare in the visualization in the SDO AIA 171 angstrom filter. || Oct2014Xflare_171A_stand.HD1080i.00334_print.jpg (1024x576) [65.0 KB] || Oct2014Xflare_171A_stand.HD1080i.00334_searchweb.png (320x180) [44.3 KB] || Oct2014Xflare_171A_stand.HD1080i.00334_web.png (320x180) [44.3 KB] || Oct2014Xflare_171A_stand.HD1080i.00334_thm.png (80x40) [4.1 KB] || Oct2014Xflare_171A_stand_1080.webmhd.webm (960x540) [2.1 MB] || Oct2014Xflare_171A_stand_1080.mp4 (1920x1080) [19.7 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Oct2014Xflare_171A_stand_1080.hwshow [82 bytes] || ", "hits": 47 }, { "id": 4250, "url": "https://svs.gsfc.nasa.gov/4250/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "Trebuchet Solar Eruption of February 2011", "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. || Feb2011Trebuchet_304A_stand.HD1080i.00460_print.jpg (1024x576) [101.4 KB] || Feb2011Trebuchet_304A_stand.HD1080i.00460_searchweb.png (320x180) [53.5 KB] || Feb2011Trebuchet_304A_stand.HD1080i.00460_thm.png (80x40) [4.1 KB] || Feb2011Trebuchet_304A_stand.HD1080i.00460_web.png (320x180) [53.5 KB] || AIA0304A (1920x1080) [128.0 KB] || Feb2011Trebuchet_304A_HD1080.mp4 (1920x1080) [80.6 MB] || Feb2011Trebuchet_304A_HD1080.webm (1920x1080) [7.1 MB] || ", "hits": 43 }, { "id": 4259, "url": "https://svs.gsfc.nasa.gov/4259/", "result_type": "Visualization", "release_date": "2015-02-11T00:00:00-05:00", "title": "April 2012 Solar Flare & Eruption", "description": "Full disk movie of the flare and eruption, as seen through the 171angstrom filter. || April2012Eruption_171A_stand.HD1080i.00192_print.jpg (1024x576) [64.6 KB] || April2012Eruption_171AHD (1920x1080) [128.0 KB] || April2012Eruption_171A.HD1080i.mov (1920x1080) [57.8 MB] || April2012Eruption_171A_stand_1080.mp4 (1920x1080) [22.2 MB] || April2012Eruption_171A.HD1080i.webm (1920x1080) [6.5 MB] || ", "hits": 50 } ] }