{ "count": 363, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=Coronal+Mass+Ejections", "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": 2134 }, { "id": 40550, "url": "https://svs.gsfc.nasa.gov/gallery/voyager/", "result_type": "Gallery", "release_date": "2026-03-04T00:00:00-05:00", "title": "Voyager", "description": "Launched in 1977, the twin Voyager spacecraft are NASA’s longest operating and most distant spacecraft. Hurtling through space at over 38,000 miles per hour, Voyager 1 and 2 were the first confirmed human-made objects to cross the threshold into interstellar space. After completing an in-depth reconnaissance of the outer planets, the Voyager spacecraft departed the heliosphere, the protective bubble of particles and magnetic fields generated by the Sun, in two separate directions and are now exploring the edges of interstellar space. \n\nLearn more: https://science.nasa.gov/mission/voyager/", "hits": 639 }, { "id": 40548, "url": "https://svs.gsfc.nasa.gov/gallery/solarand-heliospheric-observatory-soho/", "result_type": "Gallery", "release_date": "2026-03-03T00:00:00-05:00", "title": "SOHO – Solar and Heliospheric Observatory", "description": "Launched in December 1995, the Solar and Heliospheric Observatory (SOHO) is a joint mission between NASA and ESA (European Space Agency) designed to study the Sun inside out. Though its mission was originally scheduled to last until 1998, SOHO continues to collect observations about the Sun’s interior, the solar atmosphere, and the constant stream of solar particles known as the solar wind, adding to scientists' understanding of our closest star and making many new discoveries, including finding more than 5,000 comets.\n\nLearn more: https://science.nasa.gov/mission/soho/", "hits": 421 }, { "id": 14956, "url": "https://svs.gsfc.nasa.gov/14956/", "result_type": "Produced Video", "release_date": "2026-01-26T16:00:00-05:00", "title": "Space Weather Effects Animations", "description": "Solar flares, coronal mass ejections, solar particle events, and the solar wind form the recipe for space weather that affects life on Earth and astronauts in space. 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 it’s impacts on objects in the solar system. Learn more about space weather: https://science.nasa.gov/space-weather-2/ || ", "hits": 443 }, { "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": 247 }, { "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": 672 }, { "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": 419 }, { "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": 280 }, { "id": 14927, "url": "https://svs.gsfc.nasa.gov/14927/", "result_type": "Produced Video", "release_date": "2025-11-19T10:00:00-05:00", "title": "The Sun Unleashes Six November X-class Flares", "description": "A blended composite image highlighting all six X-class flares from November 2025. The main image shows 131 Angstrom light, a subset of extreme ultraviolet light. The inset images show a variety of 131 and blends of 131, 171, and 304 Angstrom light. Credit: NASA/SDO/Scott Wiessinger || November_XFlares_All_6_Inset_Multi.jpg (7000x7000) [7.0 MB] || ", "hits": 443 }, { "id": 14925, "url": "https://svs.gsfc.nasa.gov/14925/", "result_type": "Produced Video", "release_date": "2025-11-14T13:00:00-05:00", "title": "Intense Solar Storm Delays ESCAPADE Launch", "description": "NASA’s ESCAPADE mission launched on Nov. 13, 2025!But it wasn’t without any hiccups — or maybe a series of violent burps? — from the Sun!The launch of ESCAPADE, our next mission to Mars, was delayed by a day due to the most powerful geomagnetic storm of 2025. The storm was caused by multiple flares and eruptions known as coronal mass ejections heading toward Earth.With the help of NASA satellites and models, the team could monitor when the storm subsided and by the following day, it was safe to launch. || ", "hits": 492 }, { "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": 211 }, { "id": 14885, "url": "https://svs.gsfc.nasa.gov/14885/", "result_type": "Produced Video", "release_date": "2025-09-12T06:00:00-04:00", "title": "NASA Interview Opportunity: Groundbreaking New NASA Mission Will Give Us The Most Detailed Look Yet At Our Solar System’s Shield", "description": "Scroll down page for associated cut b-roll and pre-recorded soundbites. || IMAP_banner.jpeg (1600x640) [185.0 KB] || IMAP_banner_print.jpg (1024x409) [110.6 KB] || IMAP_banner_searchweb.png (320x180) [73.1 KB] || IMAP_banner_thm.png (80x40) [6.7 KB] || ", "hits": 89 }, { "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": 397 }, { "id": 5567, "url": "https://svs.gsfc.nasa.gov/5567/", "result_type": "Visualization", "release_date": "2025-07-21T18:59:59-04:00", "title": "New Missions to L1", "description": "Three missions, Carruthers, IMAP and SWFO-L1 will be launched to the Sun-Earth Lagrange Point, L1.", "hits": 164 }, { "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": 136 }, { "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": 100 }, { "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": 165 }, { "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": 158 }, { "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": 31 }, { "id": 40535, "url": "https://svs.gsfc.nasa.gov/gallery/tracers/", "result_type": "Gallery", "release_date": "2025-04-23T00:00:00-04:00", "title": "TRACERS – Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites", "description": "The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) helps understand magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when two magnetic fields, such as the Sun’s and Earth’s, intertwine and explosively realign. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth.\n\nTRACERS launched on July 23, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: https://science.nasa.gov/mission/tracers/", "hits": 234 }, { "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": 266 }, { "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": 250 }, { "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": 311 }, { "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": 45 }, { "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": 132 }, { "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": 60 }, { "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": 150 }, { "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": 48 }, { "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": 21 }, { "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": 318 }, { "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": 156 }, { "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": 24 }, { "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": 31 }, { "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": 25 }, { "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": 19 }, { "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": 28 }, { "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": 200 }, { "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": 55 }, { "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": 23 }, { "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": 31 }, { "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": 121 }, { "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": 34 }, { "id": 40532, "url": "https://svs.gsfc.nasa.gov/gallery/punch/", "result_type": "Gallery", "release_date": "2025-01-22T00:00:00-05:00", "title": "PUNCH – Polarimeter to Unify the Corona and Heliosphere", "description": "NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a constellation of four small satellites in low Earth orbit capturing global, 3D observations of the Sun's corona to better understand how the mass and energy there becomes the solar wind, a stream of charged particles from the Sun that fills the solar system. By using PUNCH to image the Sun’s corona and the solar wind together, scientists hope to better understand the entire inner heliosphere — including the Sun, solar wind, and Earth — as a single connected system.\n\nPUNCH launched on March 11, 2025, from Vandenberg Space Force Base in California.\n\nLearn more: science.nasa.gov/mission/punch", "hits": 274 }, { "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": 312 }, { "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": 24 }, { "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": 14 }, { "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": 58 }, { "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": 58 }, { "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": 53 }, { "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": 19 }, { "id": 5413, "url": "https://svs.gsfc.nasa.gov/5413/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X1.8 & M9.5 flare from Active Region 13873 - October 26, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Double flares launch from the same active region (AR 13873) less than an hour apart. For more details, see the Space Weather Database entry for M9.5 @ 2024-10-26T06:23 TAI and X1.8 @ 2024-10-26T07:19 TAI.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 21 }, { "id": 5420, "url": "https://svs.gsfc.nasa.gov/5420/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An M7.2 flare from Active Region 13878 - October 30,2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 launches an M7.2 flare. For more details, see the Space Weather Database entry.For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 17 }, { "id": 5421, "url": "https://svs.gsfc.nasa.gov/5421/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "An X2.0 and M9.4 flare from Active Region 13878 - October 31, 2024", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.Active Region 13878 presents a 'double whammy' of two strong flares (X 2.0 and M9.4) only about 30 minutes apart. For more details, see the Space Weather Database entries for X2.0 (peak @ 2024-10-31T21:20) and M9.4 (peak @ 2024-10-31T21:54).For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares. The point-spread function correction (PSF) has been applied to some of this imagery. || ", "hits": 37 }, { "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": 22 }, { "id": 20392, "url": "https://svs.gsfc.nasa.gov/20392/", "result_type": "Animation", "release_date": "2024-11-12T14:00:00-05:00", "title": "Space Weather and NOAA's Space Weather Follow On at Lagrange point 1 (SWFO-L1)", "description": "NOAA and Impacts of Space Weather || SWFO_0924_2MinVer_HD_v02.01800_print.jpg (1024x576) [187.1 KB] || SWFO_0924_2MinVer_HD_v02.01800_searchweb.png (180x320) [89.8 KB] || SWFO_0924_2MinVer_HD_v02.01800_thm.png (80x40) [6.3 KB] || SWFO_0924_2MinVer_FHD_v02.mp4 (1920x1080) [159.2 MB] || SWFO_0924_2MinVer_HD_v02.mp4 (1280x720) [157.5 MB] || SWFO_0924_2MinVer_SD_v02.mp4 (852x480) [156.8 MB] || SWFO_0924_2MinVer_4k_v02.mp4 (3840x2160) [231.9 MB] || SWFO_0924_2MinVer_4k_v02.mov (3840x2160) [15.8 GB] || ", "hits": 133 }, { "id": 14706, "url": "https://svs.gsfc.nasa.gov/14706/", "result_type": "Produced Video", "release_date": "2024-11-08T13:00:00-05:00", "title": "NASA's Illuminate Series (2024)", "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ", "hits": 99 }, { "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": 25 }, { "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": 31 }, { "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": 71 }, { "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": 134 }, { "id": 14683, "url": "https://svs.gsfc.nasa.gov/14683/", "result_type": "Produced Video", "release_date": "2024-10-15T13:30:00-04:00", "title": "NASA, NOAA Announce That the Sun Has Reached the Solar Maximum Period", "description": "In a teleconference with reporters on Tuesday, October 15, 2024, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South Poles swapping places every decade — and the Sun transitions from sluggish to active and stormy.During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity, such as the storm in May 2024, has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.Listen to the media telecon.Read NASA's article about the news. || ", "hits": 867 }, { "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": 46 }, { "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": 134 }, { "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": 1963 }, { "id": 40520, "url": "https://svs.gsfc.nasa.gov/gallery/solar-cycle25/", "result_type": "Gallery", "release_date": "2024-06-28T00:00:00-04:00", "title": "Solar Cycle 25", "description": "The Solar Cycle 25 Prediction Panel, an international group of experts co-sponsored by NASA and the National Oceanic and Atmospheric Administration (NOAA), announced that solar minimum occurred in December 2019, marking the start of Solar Cycle 25. Since then, the Sun’s activity has been steadily increasing as it approaches solar maximum — the peak of Solar Cycle 25.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the Sun transitions from relatively calm to active and stormy, and then quiet again. At its peak, the Sun’s magnetic poles flip.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts, including eruptions known as solar flares and coronal mass ejections, can disturb satellites and communication signals traveling around Earth. Scientists study the solar cycle so we can better understand and predict solar activity.", "hits": 592 }, { "id": 14602, "url": "https://svs.gsfc.nasa.gov/14602/", "result_type": "Produced Video", "release_date": "2024-06-17T06:00:00-04:00", "title": "NOAA Interview Opportunity: Ready to GOES! NOAA’s Latest GOES Weather Satellite Ready To Launch Next Week!", "description": "Join a NOAA expert on June 25, 2024 to celebrate the launch of the next and final installment of the GOES weather satellite series!From Earth weather to space weather, NOAA’s fleet of geostationary satellites play an important role in our everyday lives. And on June 25th, the fourth and final installation of the GOES-R series is set to launch from NASA’s Kennedy Space Center. As the final satellite in NOAA’s GOES-R (Geostationary Operational Environmental Satellites) series, GOES-U will continue to provide fast, clear and reliable weather-tracking information. GOES-U will provide real-time data for monitoring severe weather, hurricanes, wildfires, floods, fog and even lightning. Not only that, GOES-U carries a suite of instruments, including the first operational compact coronagraph, to monitor the Sun and warn us of approaching space weather hazards. A coronagraph is an instrument that blocks out the bright disk of the Sun so that researchers can see our star’s fainter outer atmosphere where much of the solar activity originates. This new coronagraph will better detect and characterize coronal mass ejections. The GOES series of weather satellites are parked in a geostationary orbit at points over the equator and rotate at the same speed as the Earth. The fixed location provides continuous coverage of weather conditions across the Western hemisphere. Once in orbit GOES-U will be renamed GOES-19. After an on-orbit check out to ensure its instruments and systems are working properly, GOES-19 will go into service as GOES-East, replacing GOES-16. In this location, GOES-19 will watch over most of North America, including the contiguous United States and Mexico, as well as Central and South America, the Caribbean, and the Atlantic Ocean to the west coast of Africa.* Live interviews are available June 25, 2024, between 6 a.m. - 1 p.m. EDT* Click here to request an interview: https://forms.gle/ny5wyq2mP52hQcyu7* Requests sent via the above form will have scheduling priority. Please do not email requests.* Find out more about GOES and other NOAA missions here @NOAASatellites and https://www.nesdis.noaa.gov/goes-uSuggested Anchor Intro:The nation’s most advanced fleet of weather satellites is about to get an update. Later today the fourth and final installation of NOAA’s GOES-R series will launch from NASA’s Kennedy Space Center. The new satellite, named GOES-U, will join the fleet that helps keep us safe here on the ground and in space. Welcome NOAA expert XX live from Cape Canaveral where GOES-U will launch in just a few hours.Suggested Questions:1. What is the GOES-U mission and why is it important? 2. GOES-U is the final installment in the series and we hear it has a new instrument on board that will be focused on space weather from the Sun. Can you tell us about this new instrument? 3. Here in our area, we’re particularly concerned about ______. How will GOES-U help forecasters better predict these types of extremes? [stations choice]: Wildfire and smoke monitoring and tracking Hurricane & storm tracking Lightning trackingFlooding4. What are you most excited about with the GOES-U launch?5. How can viewers watch the launch today and keep up to date on this mission? Questions for longer interviews: 6. What's next after GOES-U? What does NOAA have planned?7. Once GOES-U is launched, where will it be positioned in orbit?8. What is a geostationary orbit, and why is it used for the GOES satellites? || ", "hits": 55 }, { "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": 170 }, { "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": 608 }, { "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": 203 }, { "id": 5136, "url": "https://svs.gsfc.nasa.gov/5136/", "result_type": "Visualization", "release_date": "2023-08-22T00:00:00-04:00", "title": "STEREO-A Returns by Earth", "description": "The Solar Terrestrial Relations Observatory (STEREO) mission was launched on October 25, 2006, with the purpose of tracing the flow of energy and matter from the Sun to Earth. The STEREO mission began with two spacecraft: STEREO-A and STEREO-B. Each was launched into Sun-orbiting trajectories - STEREO-A moving ahead of Earth, and STEREO-B moving behind Earth (STEREO's Routes to Solar Orbits). In mid-August 2023, the still-operational STEREO-A (STEREO-B went offline in October 2014) will pass Earth for the first time since its launch 17 years ago. Like race cars driving different speeds around a circular track, STEREO-A is traveling slightly faster than Earth around the Sun. After launch, STEREO-A pulled ahead of Earth and extended its lead a little bit more with each orbit. Now, STEREO-A’s lead is so great that it is catching up to Earth from behind and is about to “lap” Earth, having completed 18 circuits around the Sun while Earth completed just 17. || ", "hits": 108 }, { "id": 40455, "url": "https://svs.gsfc.nasa.gov/gallery/spacecraft-animations/", "result_type": "Gallery", "release_date": "2023-01-24T00:00:00-05:00", "title": "Satellite Animations", "description": "A collection of spacecraft beauty pass animations for current missions.", "hits": 351 }, { "id": 20363, "url": "https://svs.gsfc.nasa.gov/20363/", "result_type": "Animation", "release_date": "2022-03-09T18:00:00-05:00", "title": "Animation: Heliosphere", "description": "The sun sends out a constant flow of charged particles called the solar wind, which ultimately travels past all the planets to some three times the distance to Pluto before being impeded by the interstellar medium. This forms a giant bubble around the sun and its planets, known as the heliosphere. NASA studies the heliosphere to better understand the fundamental physics of the space surrounding us - which, in turn, provides information regarding space throughout the rest of the universe, as well as regarding what makes planets habitable.The solar wind is a gas of charged particles known as plasma, a state of matter governed by its own set physical laws just as the more common solids, liquids, and gases are. As the solar wind sweeps out into space, it creates a space environment filled with radiation as well as magnetic fields that trail all the way back to the sun. This space environment is augmented by interstellar cosmic rays and occasional concentrated clouds of solar material that burst off the sun, known as coronal mass ejections.This complex environment surrounds the planets and ultimately has a crucial effect on the formation, evolution, and destiny of planetary systems. For one thing, our heliosphere acts as a giant shield, protecting the planets from galactic cosmic radiation. Earth is additionally shielded by its own magnetic field, the magnetosphere, which protects us not only from solar and cosmic particle radiation but also from erosion of the atmosphere by the solar wind. Planets without a shielding magnetic field, such as Mars and Venus, are exposed to such processes and have evolved differently.NASA's studies of the heliosphere include research into: how the solar wind behaves near Earth; what causes and sustains magnetic and electric fields around other planets; how does the heliosphere interact with the interstellar medium; what do the boundaries of the heliosphere look like; what is the origin and evolution of the solar wind and the interstellar cosmic rays; and what contributes to the habitability of exoplanets.The field is, therefore, intensely cross-disciplinary. Heliospheric research often works hand in hand with planetary scientists, astrophysicists, astrobiologists, and space weather researchers.NASA heliophysics missions contributing to heliospheric research are: the Advanced Composition Explorer; NOAA's Deep Space Climate Observatory, the Interstellar Boundary Explorer, the Solar Terrestrial Relations Observatory; Voyager, and Wind. || ", "hits": 544 }, { "id": 14055, "url": "https://svs.gsfc.nasa.gov/14055/", "result_type": "Produced Video", "release_date": "2021-12-20T22:00:00-05:00", "title": "Parker Solar Probe's WISPR Images Inside The Sun's Atmosphere", "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. As Parker Solar Probe flew through the corona, its WISPR instrument captured images.The Wide-Field Imager for Parker Solar Probe (WISPR) is the only imaging instrument aboard the spacecraft. WISPR looks at the large-scale structure of the corona and solar wind before the spacecraft flies through it. About the size of a shoebox, WISPR takes images from afar of structures like coronal mass ejections, or CMEs, jets and other ejecta from the Sun. These structures travel out from the Sun and eventually overtake the spacecraft, where the spacecraft’s other instruments take in-situ measurements. WISPR helps link what’s happening in the large-scale coronal structure to the detailed physical measurements being captured directly in the near-Sun environment.To image the solar atmosphere, WISPR uses the heat shield to block most of the Sun’s light, which would otherwise obscure the much fainter corona. Specially designed baffles and occulters reflect and absorb the residual stray light that has been reflected or diffracted off the edge of the heat shield or other parts of the spacecraft.WISPR uses two cameras with radiation-hardened Active Pixel Sensor CMOS detectors. These detectors are used in place of traditional CCDs because they are lighter and use less power. They are also less susceptible to effects of radiation damage from cosmic rays and other high-energy particles, which are a big concern close to the Sun. The camera’s lenses are made of a radiation hard BK7, a common type of glass used for space telescopes, which is also sufficiently hardened against the impacts of dust.WISPR was designed and developed by the Solar and Heliophysics Physics Branch at the Naval Research Laboratory in Washington, D.C. (principal investigator Russell Howard), which will also develop the observing program. || ", "hits": 478 }, { "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": 116 }, { "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": 57 }, { "id": 13860, "url": "https://svs.gsfc.nasa.gov/13860/", "result_type": "Produced Video", "release_date": "2021-06-17T16:00:00-04:00", "title": "Animation of USPS Stamps Featuring NASA's Solar Dynamic Observatory", "description": "The U.S. Postal Service illuminates the light and warmth of our nearest star by highlighting these stunning images of the Sun on stamps. These images come from NASA’s Solar Dynamics Observatory, a spacecraft launched in February 2010 to keep a constant watch on the Sun.The Sun is the only star that humans are able to observe in great detail, making it a vital source of information about the universe. The Solar Dynamics Observatory lets us see the Sun in wavelengths of ultraviolet light that would otherwise be invisible to our eyes. Each black-and-white image is colorized to the bright hues seen here.The stamps highlight different features on the Sun that help scientists learn about how our star works and how its constantly churning magnetic fields create the solar activity we see. Sunspots, coronal holes and coronal loops, for example, can reveal how those magnetic fields dance through the Sun and its atmosphere. Observing plasma blasts and solar flares can help us better understand and mitigate the impact of such eruptions on technology in space.The Sun Science stamps are being issued as Forever stamps, which will always be equal in value to the current First-Class Mail 1-ounce price. || ", "hits": 30 }, { "id": 13775, "url": "https://svs.gsfc.nasa.gov/13775/", "result_type": "Produced Video", "release_date": "2020-12-02T11:00:00-05:00", "title": "25 Years of Sun from ESA/NASA's SOHO", "description": "December 2, 1995 marks the 25th anniversary of the Solar and Heliospheric Observatory, or SOHO — a joint mission of the European Space Agency and NASA. Since its launch on that date, the mission has kept watch on the Sun. || ", "hits": 59 }, { "id": 13714, "url": "https://svs.gsfc.nasa.gov/13714/", "result_type": "Produced Video", "release_date": "2020-09-15T13:00:00-04:00", "title": "Solar Cycle 25 Is Here. NASA, NOAA Scientists Explain What This Means", "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.Click here for the NOAA press kit.Listen to the media telecon.Participants:• Lisa Upton, Co-chair, Solar Cycle 25 Prediction Panel; Solar Physicist, Space Systems Research Corporation• Doug Biesecker, Solar Physicist, NOAA’s Space Weather Prediction Center; Co-chair, Solar Cycle 25 Prediction Panel• Elsayed Talaat, Director, Office of Projects, Planning and Analysis; NOAA’s Satellite and Information Service • Lika Guhathakurta, Heliophysicist, Heliophysics Division, NASA Headquarters • Jake Bleacher, Chief Exploration Scientist, NASA Human Exploration and Operations Mission Directorate || ", "hits": 207 }, { "id": 13715, "url": "https://svs.gsfc.nasa.gov/13715/", "result_type": "Produced Video", "release_date": "2020-09-15T13:00:00-04:00", "title": "How To Track The Solar Cycle", "description": "A new solar cycle comes roughly every 11 years. Over the course of each cycle, the Sun transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity. As of 2020, the Sun has begun to shake off the sleep of minimum, which occurred in December 2019, and Solar Cycle 25 is underway. Scientists use several indicators to track solar cycle progress. || ", "hits": 351 }, { "id": 40421, "url": "https://svs.gsfc.nasa.gov/gallery/the-solar-cycle/", "result_type": "Gallery", "release_date": "2020-09-14T00:00:00-04:00", "title": "The Solar Cycle", "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.\nA new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.\n\nUnderstanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.", "hits": 64 }, { "id": 13534, "url": "https://svs.gsfc.nasa.gov/13534/", "result_type": "Produced Video", "release_date": "2020-01-31T16:00:00-05:00", "title": "The Countdown is on for Launch of NASA’s Next Mission to Face the Sun Live Shots", "description": "B-roll and canned interviews will be added by Thursday at 4:00 p.m. ESTSolar Orbiter Will Give Humanity Its First Close-Up Look At The Sun’s Poles || screengrab.png (2306x724) [2.8 MB] || screengrab_print.jpg (1024x321) [99.4 KB] || screengrab_searchweb.png (320x180) [126.2 KB] || screengrab_thm.png (80x40) [8.4 KB] || ", "hits": 43 }, { "id": 40409, "url": "https://svs.gsfc.nasa.gov/gallery/fermi-stills/", "result_type": "Gallery", "release_date": "2020-01-22T00:00:00-05:00", "title": "Fermi Stills", "description": "A collection of Fermi-related still images, illustrations, graphics and short clips.", "hits": 275 }, { "id": 40400, "url": "https://svs.gsfc.nasa.gov/gallery/solar-orbiter/", "result_type": "Gallery", "release_date": "2019-12-16T00:00:00-05:00", "title": "Solar Orbiter", "description": "An international cooperative mission between the European Space Agency and NASA, Solar Orbiter is a Sun-observing satellite with 10 science instruments, all designed to provide unprecedented insight into our Sun. Solar Orbiter carries in situ instruments, which directly sample particles streaming from the Sun, as well as remote-sensing instruments, which capture images of the solar surface from a vantage point closer than any spacecraft before it. Solar Orbiter follows a “tilted” orbit that has given it the first views of the Sun’s polar regions. \n\nSolar Orbiter launched on Feb. 10, 2020, from Cape Canaveral in Florida.\n\nLearn more: https://science.nasa.gov/mission/solar-orbiter/", "hits": 191 }, { "id": 13494, "url": "https://svs.gsfc.nasa.gov/13494/", "result_type": "Produced Video", "release_date": "2019-12-11T13:00:00-05:00", "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission", "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ", "hits": 129 }, { "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": 257 }, { "id": 4491, "url": "https://svs.gsfc.nasa.gov/4491/", "result_type": "Visualization", "release_date": "2019-05-01T00:00:00-04:00", "title": "The X8.2 Flare of September 2017, as Seen by SDO", "description": "40 hours of AIA 131 angstrom imager at 12 second cadence viewing the time around the X8.2 solar flare. || Sept2017_X8Flare_131A_stand.UHD3840.07800_print.jpg (1024x576) [61.1 KB] || AIA131A (1920x1080) [0 Item(s)] || Sept2017_X8Flare_131A.HD1080i_p30.webm (1920x1080) [47.6 MB] || Sept2017_X8Flare_131A.HD1080i_p30.mp4 (1920x1080) [843.8 MB] || AIA131A (3840x2160) [0 Item(s)] || Sept2017_X8Flare_131A.HD1080i_p30.mp4.hwshow || ", "hits": 54 }, { "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": 114 }, { "id": 4680, "url": "https://svs.gsfc.nasa.gov/4680/", "result_type": "Visualization", "release_date": "2018-10-04T00:00:00-04:00", "title": "Space Weather to the Edge of the Solar System - Revisited", "description": "Cropped view of the Enlil model from early 2015 to just after the New Horizons flyby of Pluto. || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_print.jpg (1024x576) [97.2 KB] || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_searchweb.png (320x180) [79.1 KB] || NewHorizons.topfixed.HD1080frames.clockSlate_HAE.HD1080i.01000_thm.png (80x40) [5.0 KB] || TopView (1920x1080) [0 Item(s)] || NewHorizons.topfixed_HAE.HD1080i_p30.mp4 (1920x1080) [41.0 MB] || NewHorizons.topfixed_HAE.HD1080i_p30.webm (1920x1080) [6.6 MB] || TopView (3840x2160) [0 Item(s)] || NewHorizons.topfixed_HAE.UHD3840_2160p30.mp4 (3840x2160) [125.3 MB] || NewHorizons.topfixed_HAE.HD1080i_p30.mp4.hwshow [202 bytes] || ", "hits": 128 }, { "id": 13035, "url": "https://svs.gsfc.nasa.gov/13035/", "result_type": "Produced Video", "release_date": "2018-08-08T16:00:00-04:00", "title": "Parker Solar Probe Instruments", "description": "SWEAPThe Solar Wind Electrons Alphas and Protons investigation, or SWEAP, gathers observations using two complementary instruments: the Solar Probe Cup, or SPC, and the Solar Probe Analyzers, or SPAN. The instruments count the most abundant particles in the solar wind — electrons, protons and helium ions — and measure such properties as velocity, density, and temperature to improve our understanding of the solar wind and coronal plasma. SWEAP was built mainly at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and at the Space Sciences Laboratory at the University of California, Berkeley. The institutions jointly operate the instrument. The principal investigator is Justin Kasper from the University of Michigan. || SWEAP.00001_print.jpg (1024x581) [151.9 KB] || SWEAP_thumb.png (2560x1448) [4.7 MB] || SWEAP.00001_searchweb.png (320x180) [86.1 KB] || SWEAP.00001_web.png (320x181) [86.8 KB] || SWEAP.00001_thm.png (80x40) [5.6 KB] || SWEAP.webm (1902x1080) [21.8 MB] || SWEAP.mp4 (1902x1080) [195.4 MB] || SWEAP.en_US.srt [3.8 KB] || SWEAP.en_US.vtt [3.8 KB] || ", "hits": 311 }, { "id": 13028, "url": "https://svs.gsfc.nasa.gov/13028/", "result_type": "Produced Video", "release_date": "2018-08-08T00:00:00-04:00", "title": "Parker Solar Probe Media Telecons", "description": "This is a resource page for the media teleconferences on August 8, 2018. || ", "hits": 46 }, { "id": 13011, "url": "https://svs.gsfc.nasa.gov/13011/", "result_type": "Produced Video", "release_date": "2018-07-25T00:00:00-04:00", "title": "Sounds of the Sun", "description": "An illustration of a sunspot inspired by imagery from NASA's Solar Dynamics Observatory (SDO). || sunspot.gif (1280x720) [1.5 MB] || sunspot_searchweb.png (320x180) [95.7 KB] || ", "hits": 245 }, { "id": 12927, "url": "https://svs.gsfc.nasa.gov/12927/", "result_type": "Produced Video", "release_date": "2018-04-16T12:00:00-04:00", "title": "Looking at the Corona with WISPR on Parker Solar Probe", "description": "The Wide-Field Imager for Solar Probe, or WISPR, is aboard NASA’s Parker Solar Probe to take images of the solar corona (the Sun’s atmosphere) and inner heliosphere. WISPR’s telescopes will provide white-light images of the solar wind, shocks, solar ejecta and other structures as they approach and pass the spacecraft. Parker Solar Probe is scheduled for launch in July 2018. It will be the first spacecraft ever to fly through the solar corona to investigate the evolution of the solar wind and heating of the solar corona. WISPR does not look directly at the Sun. Its very wide field-of-view extends from 13° away from the center of the Sun to 108° from the Sun. || ", "hits": 54 }, { "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": 12796, "url": "https://svs.gsfc.nasa.gov/12796/", "result_type": "Produced Video", "release_date": "2017-12-13T11:30:00-05:00", "title": "2017 AGU Habitability Press Conference", "description": "Spanning Disciplines to Search for Life Beyond EarthThe search for life beyond Earth is riding a surge of creativity and innovation. Following a gold rush of exoplanet discovery over the past two decades, it is time to tackle the next step: determining which of the known exoplanets are proper candidates for life. Scientists from NASA and two universities presented new results dedicated to this task in fields spanning astrophysics, Earth science, heliophysics and planetary science — demonstrating how a cross-disciplinary approach is essential to finding life on other worlds — at the fall meeting of the American Geophysical Union on Dec. 13, 2017, in New Orleans, Louisiana.PANELISTS:• Giada Arney, NASA’s Goddard Space Flight Center• Stephen Kane, University of California-Riverside• Katherine Garcia-Sage, NASA’s Goddard Space Flight Center/Catholic University of America• Dave Brain, University of Colorado-Boulder || ", "hits": 97 }, { "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": 146 }, { "id": 12704, "url": "https://svs.gsfc.nasa.gov/12704/", "result_type": "Produced Video", "release_date": "2017-08-31T12:00:00-04:00", "title": "NASA Eclipse Imagery", "description": "As millions of people across the United States experienced a total eclipse as the umbra, or Moon’s shadow passed over them, only six people witnessed the umbra from space. Viewing the eclipse from orbit were NASA’s Randy Bresnik, Jack Fischer and Peggy Whitson, ESA (European Space Agency’s) Paolo Nespoli, and Roscosmos’ Commander Fyodor Yurchikhin and Sergey Ryazanskiy. The space station crossed the path of the eclipse three times as it orbited above the continental United States at an altitude of 250 miles. Credit: NASA || iss052e056122.jpg (4928x3280) [844.0 KB] || ", "hits": 348 }, { "id": 30893, "url": "https://svs.gsfc.nasa.gov/30893/", "result_type": "Hyperwall Visual", "release_date": "2017-08-31T00:00:00-04:00", "title": "2017 Eclipse Image Collection", "description": "This image is a composite photograph that shows the progression of the total solar eclipse over Madras, Oregon.http://earthobservatory.nasa.gov/NaturalHazards/view.php?id=90796 || eclipsecomposite_pho_lrg.jpg (2231x1487) [541.4 KB] || eclipsecomposite_pho_lrg_searchweb.png (320x180) [47.2 KB] || eclipsecomposite_pho_lrg_thm.png (80x40) [3.3 KB] || 2017-eclipse-images-7.hwshow [293 bytes] || ", "hits": 212 }, { "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": 62 }, { "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": 109 }, { "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": 48 } ] }