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            "result_type": "Produced Video",
            "release_date": "2025-05-12T00:00:00-04:00",
            "title": "Cosmic Dawn: The Untold Story of the James Webb Space Telescope",
            "description": "For more than three decades, NASA and an international team of scientists and engineers pushed the limits of technology, innovation, and perseverance to build and launch the James Webb Space Telescope, the most powerful space observatory ever created. Cosmic Dawn brings audiences behind the scenes with the Webb film crew, and never-before-heard testimonies revealing the real story of how this telescope overcame all odds. ||",
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            "result_type": "B-Roll",
            "release_date": "2023-06-21T09:00:00-04:00",
            "title": "Earth Information Center Media B-Roll",
            "description": "The Earth Information Center is a physical and virtual space that showcases NASA Earth information and how our partners and everyday people use Earth observations to solve our planet’s most pressing issues.  It provides a view of our home planet down to local neighborhoods, from outer space. It shows how our planet is changing and provides easy-to-use information and resources we need to mitigate, adapt, and respond to climate change.  The Earth Information Center at NASA’s headquarters building is a physical space that includes various parts: an Earth Pulse sculpture of lights showing NASA Earth data, a Hyperwall that showcases awe-inspiring visualizations and stories told by people using NASA Earth data, the Space for Earth immersive experience surrounding you with science, and an Eyes on Earth interactive kiosk.Images of the June 21, 2023 ribbon cutting ceremony can be found on the NASA Flickr account || ",
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            "result_type": "Hyperwall Visual",
            "release_date": "2023-02-15T00:00:00-05:00",
            "title": "NASA’s Perseverance Rover Completes Mars Sample Depot",
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            "release_date": "2022-03-23T00:00:00-04:00",
            "title": "The James Webb Space Telescope Mirror Alignment Press Conference Update",
            "description": "The press conference covering the latest updated on the James Webb Space Telescope and the mirror alignment. || ",
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            "release_date": "2020-12-03T17:00:00-05:00",
            "title": "Solar Activity Continues to Rise with 'Anemone' Eruption",
            "description": "Short video showing the solar flare and subsequent prominence eruption and \"arcade\" of loops.Credit: NASA/GSFC/SDOMusic: \"Beautiful Awesome\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Anemone_Eruption_131-171_Blend.jpg (1920x1080) [281.9 KB] || Anemone_Eruption_131-171_Blend_searchweb.png (180x320) [78.6 KB] || Anemone_Eruption_131-171_Blend_thm.png (80x40) [6.6 KB] || 13778_Anemone_Eruption_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 13778_Anemone_Eruption_Best_1080.mp4 (1920x1080) [718.2 MB] || 13778_Anemone_Eruption_1080.mp4 (1920x1080) [220.6 MB] || 13778_Anemone_Eruption_Best_1080.webm (1920x1080) [16.0 MB] || AnemoneEruption_SRT_Captions.en_US.srt [500 bytes] || AnemoneEruption_SRT_Captions.en_US.vtt [513 bytes] || ",
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            "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 || ",
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            "result_type": "Animation",
            "release_date": "2020-08-14T09:00:00-04:00",
            "title": "Solar Energetic Particles",
            "description": "The Sun goes through phases of strong activity, during which eruptions can occur. Such eruptions can have multiple components, including X rays, coronal mass ejection plasma, and solar energetic particles – bursts or events of fast-moving particles.  These events can occur suddenly and have the potential to rapidly change the radiation environment of wide swaths of the inner solar system where they may create hazardous conditions.  Not only are such conditions dangerous for humans in space, but the intense ionizing radiation can also affect the interior of spacecraft, including sensitive electronics.  Solar energetic particles can reach all regions of near-Earth space, including the lunar surface, with the exception of  low-altitude and low-latitude Earth orbit, where the Earth’s magnetic field is strong enough to form a protective barrier. || ",
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            "release_date": "2020-02-07T14:30:00-05:00",
            "title": "Solar Orbiter Science Press Briefing",
            "description": "NASA and the European Space Agency (ESA) will present Solar Orbiter, the ESA/NASA mission to the Sun, during a science press briefing on Friday, Feb. 7. 2020, at 2.30 p.m. EST. Solar Orbiter will observe the Sun with high spatial resolution telescopes and capture observations in the environment directly surrounding the spacecraft to create a one-of-a-kind picture of how the Sun can affect the space environment throughout our solar system. The spacecraft also will provide the first-ever images of the Sun’s poles and the never-before-observed magnetic environment there, which helps drive the Sun’s 11-year solar cycle and its periodic outpouring of solar storms.The teleconference audio will stream live at:https://www.nasa.gov/liveParticipants include:European Space Agency• Daniel Müller, Solar Orbiter Project Scientist• Günther Hasinger, Director of ScienceNASA• Nicky Fox, Heliophysics Division Director, NASA HQ• Thomas Zurbuchen, Associate Administrator for the Science Mission Directorate, NASA HQ || ",
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            "result_type": "Animation",
            "release_date": "2020-01-27T14:00:00-05:00",
            "title": "Solar Orbiter - NASA Animations",
            "description": "Solar Orbiter is an international cooperative mission between the European Space Agency and NASA that addresses a central question of heliophysics: How does the Sun create and control the constantly changing space environment throughout the solar system? The Sun creates what’s known as the heliosphere — a giant bubble of charged particles and magnetic fields blown outward by the Sun that stretches more than twice the distance to Pluto at its nearest edge, enveloping every planet in our solar system and shaping the space around us. To understand it, Solar Orbiter will travel as close as 26 million miles from the Sun, inside the orbit of Mercury. There, it will measure the magnetic fields, waves, energetic particles and plasma escaping the Sun while they are in their pristine state, before being modified and mixed in their long journey from the Sun. || ",
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            "release_date": "2019-12-10T13:00:00-05:00",
            "title": "How NASA Studies The Space Near Earth",
            "description": "NASA studies the space around our home planet, a region we call geospace. It might appear empty, but geospace is bustling with electrically charged particles and magnetic fields — all of which can impact the technology and satellites we have flying through it. NASA uses specialized tools to study changing conditions in geospace, known as space weather. Each examines geospace in its own way. Together, they help us visualize, and better understand, the invisible processes shaping the space that is closest to home. || ",
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            "url": "https://svs.gsfc.nasa.gov/13282/",
            "result_type": "Produced Video",
            "release_date": "2019-12-04T13:00:00-05:00",
            "title": "5 New Discoveries from NASA's Parker Solar Probe",
            "description": "Music Credit: Smooth as Glass by The Freeharmonic OrchestraWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || parkerscience.thumb.jpg (1920x1080) [731.2 KB] || parkerscience.thumb_thm.png (80x40) [6.8 KB] || parkerscience.thumb_searchweb.png (320x180) [87.7 KB] || 13282_ParkerFirstScience_Twitter1080.mp4 (1920x1080) [53.4 MB] || 13282_ParkerFirstScience.YouTube1080.webm (1920x1080) [26.9 MB] || 13282_ParkerFirstScience.mp4 (1920x1080) [246.1 MB] || 13282_ParkerFirstScience_Mobile1080.mp4 (1920x1080) [194.5 MB] || 13282_ParkerFirstScience.YouTube1080.mp4 (1920x1080) [387.1 MB] || 13282_ParkerFirstScience_Twitter1080.en_US.srt [4.5 KB] || 13282_ParkerFirstScience_Twitter1080.en_US.vtt [4.5 KB] || 13282_ParkerFirstScienceMASTER.APR1080.mov (1920x1080) [3.2 GB] || ",
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            "id": 13484,
            "url": "https://svs.gsfc.nasa.gov/13484/",
            "result_type": "Produced Video",
            "release_date": "2019-12-04T13:00:00-05:00",
            "title": "Parker Solar Probe First Findings - Media Telecon",
            "description": "NASA to Present First Parker Solar Probe Findings in Media TeleconferenceNASA will announce the first results from the Parker Solar Probe mission, the agency's mission to \"touch\" the Sun, during a media teleconference at 1:30 pm EST on Wednesday, Dec. 4, 2019.Parker has traveled closer to our star than any human-made object before it. The teleconference will discuss the first papers from the principal investigators of the mission’s four instruments. The papers will be published online Wednesday in Nature at 1 pm EST.The teleconference audio will stream live at:https://www.nasa.gov/nasaliveParticipants in the call are: •Nicola Fox, director of the Heliophysics Division, Science Mission Directorate, NASA Headquarters, Washington•Stuart Bale, principal investigator of the FIELDS instrument at the University of California, Berkeley•Justin Kasper, principal investigator of the SWEAP instrument at the University of Michigan in Ann Arbor•Russ Howard, principal investigator of the WISPR instrument at the Naval Research Laboratory in Washington•David McComas, principal investigator of the ISʘIS instrument at Princeton University in Princeton, N.J. || ",
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            "result_type": "Produced Video",
            "release_date": "2019-12-04T00:00:00-05:00",
            "title": "NASA Science Live: New Discoveries from Our Mission to Touch the Sun (Episode 12)",
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            "url": "https://svs.gsfc.nasa.gov/13438/",
            "result_type": "Produced Video",
            "release_date": "2019-11-18T04:30:00-05:00",
            "title": "NASA's Sounding Rockets Show: Cutting-edge Science, 15 Minutes at a Time",
            "description": "Some of the smallest and lightest rockets in NASA’s lineup have made some of the biggest impacts on science. With a flight time of just about 15 minutes before falling back to Earth, sounding rockets collect unique observations on everything from our planet’s atmosphere to the Sun and even distant galaxies.Join us live to hear from scientists who have traveled to the ends of the Earth to launch sounding rockets, flown cutting-edge instruments on these suborbital flights, and used sounding rockets to make brand-new scientific discoveries.Watch on Facebook or YouTube. || ",
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            "id": 13159,
            "url": "https://svs.gsfc.nasa.gov/13159/",
            "result_type": "Produced Video",
            "release_date": "2019-03-27T10:00:00-04:00",
            "title": "5 Things About Interstellar Space",
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            "url": "https://svs.gsfc.nasa.gov/13148/",
            "result_type": "Produced Video",
            "release_date": "2019-02-12T08:00:00-05:00",
            "title": "5 Things About Earth’s Radiation Donuts",
            "description": "5 Things About Earth’s Radiation Donuts || HalloweenBeltProfile.slate_GSE.HRstills.0000_print.jpg (1024x576) [124.2 KB] || HalloweenBeltProfile.slate_GSE.HRstills.0000.jpg (2560x1440) [721.8 KB] || HalloweenBeltProfile.slate_GSE.HRstills.0000_searchweb.png (320x180) [88.2 KB] || HalloweenBeltProfile.slate_GSE.HRstills.0000_thm.png (80x40) [6.1 KB] || RADIATIONDONUTSSVSV2.mp4 (1280x720) [114.9 MB] || RADIATIONDONUTSSVSV2.webm (1280x720) [12.2 MB] || VanAllenShowCaptions.en_US.srt [2.2 KB] || VanAllenShowCaptions.en_US.vtt [2.2 KB] || ",
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            "id": 12670,
            "url": "https://svs.gsfc.nasa.gov/12670/",
            "result_type": "Produced Video",
            "release_date": "2018-12-10T11:00:00-05:00",
            "title": "Voyager 2 Leaves the Heliosphere",
            "description": "Animated graph of Voyager 2's Cosmic Ray Subsystem (CRS) data, showing the abrupt change as it left the heliosphere. || V2AnimatedGraph16x9_2_print.jpg (1024x576) [124.7 KB] || V2AnimatedGraph16x9_2.jpg (3840x2160) [1.0 MB] || V2AnimatedGraph16x9_2_searchweb.png (320x180) [70.9 KB] || V2AnimatedGraph16x9_2_thm.png (80x40) [5.1 KB] || V2AnimatedGraph16x9_3_date_ProRes_3840x2160.webm (3840x2160) [2.0 MB] || V2AnimatedGraph16x9_3_date_ProRes_3840x2160.mov (3840x2160) [718.6 MB] || V2AnimatedGraph16x9_3_date.mp4 (3840x2160) [19.2 MB] || ",
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            "result_type": "Produced Video",
            "release_date": "2018-11-06T03:30:00-05:00",
            "title": "Tour the Plane Giving NASA’s ICON a Ride to Space",
            "description": "Early in the morning of Nov. 7, 2018, NASA launches the Ionospheric Connection Explorer, or ICON, a spacecraft that will explore the dynamic region where Earth meets space. ICON launches on a Northrop Grumman Pegasus XL rocket, which is carried aloft by the Stargazer L-1011 aircraft.Join NASA on a behind-the-scenes tour of this plane, once a jet airliner and now uniquely retrofitted to boost spacecraft into low-Earth orbit. Learn about ICON’s science and meet the people — including an engineer, technician, and pilot — who will help launch the spacecraft into orbit.Learn more at: nasa.gov/icon || ",
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            "id": 13105,
            "url": "https://svs.gsfc.nasa.gov/13105/",
            "result_type": "Produced Video",
            "release_date": "2018-11-02T14:00:00-04:00",
            "title": "First Perihelion: Into the Unknown with Parker Solar Probe",
            "description": "Complete transcript available.Watch this video on the JHU/APL YouTube channel. || 1803932PSPRISKmixedfinalscreener.03961_print.jpg (1024x576) [97.7 KB] || 1803932PSPRISKmixedfinalscreener.03961_searchweb.png (320x180) [78.1 KB] || 1803932PSPRISKmixedfinalscreener.03961_thm.png (80x40) [5.7 KB] || 1803932PSPRISKmixedfinalscreener.mp4 (1280x720) [130.4 MB] || 1803932PSPRISKmixedfinalscreener.webm (1280x720) [23.0 MB] || FirstPerihelioncaptions.en_US.srt [3.5 KB] || FirstPerihelioncaptions.en_US.vtt [3.6 KB] || ",
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            "id": 12971,
            "url": "https://svs.gsfc.nasa.gov/12971/",
            "result_type": "Produced Video",
            "release_date": "2018-10-19T13:00:00-04:00",
            "title": "Unboxing a New NASA Spacecraft",
            "description": "Go behind the scenes as we unbox NASA’s Ionospheric Connection Explorer, or ICON, after its arrival at Vandenberg Air Force Base in California. Northrop Grumman engineer Steve Turek and NASA EDGE’s Chris Giersch walk us through the whole process of unboxing a spacecraft – from the instrument that records every tiny bump on its journey to the special crane used to lift the spacecraft to its new home.ICON launches in fall 2018 from NASA's Kennedy Space Center in Florida to study Earth’s interface to space. Read more about the ICON mission: nasa.gov/icon || ",
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        {
            "id": 13029,
            "url": "https://svs.gsfc.nasa.gov/13029/",
            "result_type": "Produced Video",
            "release_date": "2018-08-09T00:00:00-04:00",
            "title": "Parker Solar Probe Pre-Launch Briefing",
            "description": "Hosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Scott Messer - Program Manager, NASA Programs, United Launch AllianceOmar Baez - Launch Director, NASA, Kennedy Space CenterKathy Rice - Launch Weather Officer, 45th Weather Squadron, Cape Canaveral Air Force StationThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASANicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAndy Dreisman - Project Manger The Johns Hopkins University Applied Physics Lab || ",
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        {
            "id": 13017,
            "url": "https://svs.gsfc.nasa.gov/13017/",
            "result_type": "Produced Video",
            "release_date": "2018-08-08T11:00:00-04:00",
            "title": "It's Surprisingly Hard to Go to the Sun",
            "description": "Why does the Parker Solar Probe have such a long and complex orbit to get close to the Sun?  Why doesn't it just fall right toward it?  Turns out it's a lot harder to approach the Sun than you might think.  This video explains why.Music: Percs and Pizz from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || PSP_Orbit_Shot_1_still.jpg (1920x1080) [324.1 KB] || PSP_Orbit_Shot_1_still_print.jpg (1024x576) [131.5 KB] || PSP_Orbit_Shot_1_still_searchweb.png (320x180) [88.1 KB] || PSP_Orbit_Shot_1_still_thm.png (80x40) [6.8 KB] || 13017_ParkerSolarProbe_Orbit_ProRes_1920x1080_2997.mov (1920x1080) [2.2 GB] || 13017_ParkerSolarProbe_Orbit.mp4 (1920x1080) [177.5 MB] || 13017_ParkerSolarProbe_Orbit_ProRes_1920x1080_2997.webm (1920x1080) [18.4 MB] || 13017_ParkerSolarProbe_Orbit_SRT_Captions.en_US.srt [3.4 KB] || 13017_ParkerSolarProbe_Orbit_SRT_Captions.en_US.vtt [3.3 KB] || ",
            "hits": 279
        },
        {
            "id": 4671,
            "url": "https://svs.gsfc.nasa.gov/4671/",
            "result_type": "Infographic",
            "release_date": "2018-08-07T14:00:00-04:00",
            "title": "Parker Solar Probe - Close to the Sun",
            "description": "Image representing Parker Solar Probe's distance from the Sun. || Parker_Close_to_Sun_Infographic_print.jpg (1024x662) [60.0 KB] || Parker_Close_to_Sun_Infographic.jpg (5100x3300) [1001.2 KB] || Parker_Close_to_Sun_Infographic_borderless.jpg (4628x2572) [1.0 MB] || Parker_Close_to_Sun_Infographic_searchweb.png (320x180) [86.8 KB] || Parker_Close_to_Sun_Infographic_thm.png (80x40) [7.1 KB] || parker-solar-probe-close-to-the-sun.hwshow [306 bytes] || ",
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        },
        {
            "id": 13003,
            "url": "https://svs.gsfc.nasa.gov/13003/",
            "result_type": "Produced Video",
            "release_date": "2018-07-20T12:30:00-04:00",
            "title": "Parker Solar Probe Science Briefing - Visual Resources",
            "description": "July 20, 2018 - Live from NASA Kennedy - 1:00 p.m. ESTHosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Nicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAlex Young - Solar Scientist from NASA GoddardThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASABetsy Congdon - Thermal Protection System Engineer at The Johns Hopkins University Applied Physics Lab || ",
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        {
            "id": 4653,
            "url": "https://svs.gsfc.nasa.gov/4653/",
            "result_type": "Visualization",
            "release_date": "2018-06-05T10:00:00-04:00",
            "title": "Parker Solar Probe and Solar Orbiter Trajectories",
            "description": "This visualization opens near Earth for the launch of Parker Solar Probe August 12,  2018.  Then the camera moves around the Sun to match of with Earth again for the launch of Solar Orbiter in 2020.  After that, the camera moves in a slow drift around the Sun as the orbits evolve.  The Parker Solar Probe orbit fades out after the nominal end of mission in 2025.  This version has longer orbit trails to better view orbit changes, and the red along the orbits indicate the nominal science operations portions of the missions. || ParkerAndSolarOrbiter.InnerTourDeluxe.HAE.AU.clockSlate_EarthTarget.HD1080i.02000_print.jpg (1024x576) [100.7 KB] || DeluxeTour (1920x1080) [0 Item(s)] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.webm (1920x1080) [17.6 MB] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.mp4 (1920x1080) [179.8 MB] || DeluxeTour (3840x2160) [0 Item(s)] || ParkerAndSolarOrbiter.InnerTourDeluxe_2160p30.mp4 (3840x2160) [489.0 MB] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.mp4.hwshow [270 bytes] || ParkerAndSolarOrbiter.InnerTourDeluxe_2160p30.mp4.hwshow [211 bytes] || ",
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        {
            "id": 4623,
            "url": "https://svs.gsfc.nasa.gov/4623/",
            "result_type": "Visualization",
            "release_date": "2018-04-30T10:00:00-04:00",
            "title": "The Dynamic Solar Magnetic Field with Introduction",
            "description": "This narrated visualization  transitions from a view of the Sun in visible light, to a view in ultraviolet light showing the plasma flowing along solar magnetic structures, to the underlying magnetic field of the solar photosphere, to a model construction of magnetic fieldlines above the photosphere.This video is also available on our YouTube channel. || SolarMagnetism_UHD3840.04000_print.jpg (1024x576) [198.9 KB] || SolarMagnetism_UHD3840.04000_thm.png (80x40) [6.0 KB] || SolarMagnetism_UHD3840.04000_web.png (320x180) [84.1 KB] || SolarMagnetism_ProRes3_HD1080_p30_Narrated.webm (1280x720) [33.9 MB] || SolarMagnetism_ProRes3_HD1080_p30_Narrated.mov (1280x720) [7.4 GB] || SolarMagnetism_ProRes3_UHD2160_p30_Narrated.mov (3840x2160) [12.8 GB] || ",
            "hits": 114
        },
        {
            "id": 12917,
            "url": "https://svs.gsfc.nasa.gov/12917/",
            "result_type": "Produced Video",
            "release_date": "2018-04-13T19:00:00-04:00",
            "title": "Parker Solar Probe Travels to Florida",
            "description": "Parker Solar Probe Arrives in FloridaOn April 4, 2018, Parker Solar Probe project scientist Nicky Fox of Johns Hopkins APL describes the spacecraft's April 3 journey to Florida and arrival at Astrotech Space Operations, the probe's new home before a scheduled launch on July 31, 2018 from NASA's Kennedy Space Center. Credit: NASA/Johns Hopkins APL/Lee HobsonWatch this video on the Johns Hopkins APL YouTube channel. || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_print.jpg (1024x576) [103.8 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_thm.png (80x40) [7.1 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_web.png (320x180) [85.2 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_searchweb.png (320x180) [85.2 KB] || PRORES_B-ROLL_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_prores.mov (1280x720) [642.5 MB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_appletv_subtitles.m4v (1280x720) [48.0 MB] || NASA_TV_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD.mpeg (1280x720) [309.1 MB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_appletv.m4v (1280x720) [48.0 MB] || YOUTUBE_1080_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_youtube_1080.mp4 (1920x1080) [146.4 MB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.mp4 (3840x2160) [97.6 MB] || Nicky_Fox_Welcomes_PSP_To_ASO_UHD.mp4 (3840x2160) [502.0 MB] || YOUTUBE_4K_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_youtube_4k.mp4 (3840x2160) [373.1 MB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.webm (3840x2160) [12.3 MB] || 12917_Parker_Solar_Probe_Arrives_in_Florida.en_US.srt [1.3 KB] || 12917_Parker_Solar_Probe_Arrives_in_Florida.en_US.vtt [1.3 KB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_Prores.mov (3840x2160) [4.9 GB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_ipod_sm.mp4 (320x240) [15.8 MB] || ",
            "hits": 125
        },
        {
            "id": 12825,
            "url": "https://svs.gsfc.nasa.gov/12825/",
            "result_type": "Infographic",
            "release_date": "2018-01-24T12:00:00-05:00",
            "title": "GOLD Resources",
            "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. The more we know about the fundamental physics of this region of space, the more we can protect our assets there.Gathering observations from geostationary orbit above the Western Hemisphere, GOLD measures the temperature and composition of neutral gases in Earth’s thermosphere. This part of the atmosphere co-mingles with the ionosphere, which is made up of charged particles. Both the Sun from above and terrestrial weather from below can change the types, numbers, and characteristics of the particles found here — and GOLD helps track those changes.Activity in this region is responsible for a variety of key space weather events. GOLD scientists are particularly interested in the cause of dense, unpredictable bubbles of charged gas that appear over the equator and tropics, sometimes causing communication problems. As we discover the very nature of the Sun-Earth interaction in this region, the mission could ultimately lead to ways to improve forecasts of such space weather and mitigate its effects. || ",
            "hits": 148
        },
        {
            "id": 12820,
            "url": "https://svs.gsfc.nasa.gov/12820/",
            "result_type": "Produced Video",
            "release_date": "2018-01-04T00:00:00-05:00",
            "title": "Going for GOLD: Exploring the Interface to Space",
            "description": "Going for GOLD: Exploring the Interface to Space || 12820_GOLD_FB_Live.00001_print.jpg (1024x576) [125.3 KB] || 12820_GOLD_FB_Live.00001_searchweb.png (320x180) [84.7 KB] || 12820_GOLD_FB_Live.00001_thm.png (80x40) [6.6 KB] || 12820_GOLD_FB_Live.mp4 (1280x720) [5.1 GB] || 12820_GOLD_FB_Live.mov (1280x720) [41.9 GB] || 12820_GOLD_FB_Live.webm (960x540) [1.7 GB] || 12820_GOLD_FB_Live.en_US.srt [119.6 KB] || 12820_GOLD_FB_Live.en_US.vtt [112.9 KB] || ",
            "hits": 59
        },
        {
            "id": 12699,
            "url": "https://svs.gsfc.nasa.gov/12699/",
            "result_type": "Produced Video",
            "release_date": "2017-10-18T14:00:00-04:00",
            "title": "Meet ICON: NASA’s Airglow Explorer",
            "description": "Music credit: Design Principle by Wayne RobertsComplete transcript available. || iss_composite_test_182.jpg (4256x2832) [12.8 MB] || iss_composite_test_182_searchweb.png (320x180) [99.0 KB] || iss_composite_test_182_thm.png (80x40) [6.2 KB] || LARGE_MP4-12699_ICON_Overview_V2__large.mp4 (1920x1080) [148.3 MB] || NASA_TV-12699_ICON_Overview_V2_.mpeg (1280x720) [494.2 MB] || APPLE_TV-12699_ICON_Overview_V2__appletv.m4v (1280x720) [75.3 MB] || YOUTUBE_1080-12699_ICON_Overview_V2__youtube_1080.mp4 (1920x1080) [234.8 MB] || PRORES_B-ROLL-12699_ICON_Overview_V2__prores.mov (1280x720) [1.9 GB] || YOUTUBE_HQ-12699_ICON_Overview_V2__youtube_hq.mov (1920x1080) [539.3 MB] || 12699_ICON_Overview_V2_.mov (1920x1080) [3.7 GB] || LARGE_MP4-12699_ICON_Overview_V2__large.webm (1920x1080) [16.3 MB] || APPLE_TV-12699_ICON_Overview_V2__appletv_subtitles.m4v (1280x720) [75.3 MB] || 12699_ICON_Overview_V2.en_US.srt [2.4 KB] || 12699_ICON_Overview_V2.en_US.vtt [2.5 KB] || NASA_PODCAST-12699_ICON_Overview_V2__ipod_sm.mp4 (320x240) [25.4 MB] || 12699_ICON_Overview_V2__lowres.mp4 (480x272) [20.3 MB] || ",
            "hits": 65
        },
        {
            "id": 12729,
            "url": "https://svs.gsfc.nasa.gov/12729/",
            "result_type": "Produced Video",
            "release_date": "2017-09-22T19:00:00-04:00",
            "title": "Parker Solar Probe Animations",
            "description": "Animated Sequence Of Parker Solar ProbeCredit: NASA/JHUAPL || ParkerSolarProbe-AnimatedSequence.00001_print.jpg (1024x576) [41.9 KB] || ParkerSolarProbe-AnimatedSequence.00001_searchweb.png (180x320) [37.2 KB] || ParkerSolarProbe-AnimatedSequence.00001_web.png (320x180) [37.2 KB] || ParkerSolarProbe-AnimatedSequence.00001_thm.png (80x40) [3.2 KB] || ParkerAnimatedSeq.mov (1920x1080) [2.9 GB] || ParkerAnimatedSeq.mp4 (1920x1080) [343.1 MB] || ParkerAnimatedSeq.webm (1920x1080) [21.1 MB] || ",
            "hits": 201
        },
        {
            "id": 12726,
            "url": "https://svs.gsfc.nasa.gov/12726/",
            "result_type": "Produced Video",
            "release_date": "2017-09-22T18:00:00-04:00",
            "title": "Parker Solar Probe: Testing and Integration",
            "description": "Main flight harness installation.Credit: NASA/JHUAPL || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_print.jpg (1024x576) [120.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_searchweb.png (320x180) [75.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_web.png (320x180) [75.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_thm.png (80x40) [5.6 KB] || 12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_prores.mov (1920x1080) [2.9 GB] || PRORES_B-ROLL-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_prores.mov (1280x720) [1.5 GB] || YOUTUBE_1080-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_youtube_1080.mp4 (1920x1080) [373.7 MB] || APPLE_TV-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_appletv.m4v (1280x720) [117.9 MB] || NASA_TV-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072.mpeg (1280x720) [697.9 MB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.mp4 (1920x1080) [209.3 MB] || 17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_1080p.mp4 (1920x1080) [408.5 MB] || LARGE_MP4-12726_ParkerSolarProbe_blanketing_17-08-01-08_SPP_Timelapse_17-00_large.webm (1280x720) [15.6 MB] || NASA_PODCAST-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_ipod_sm.mp4 (320x240) [38.5 MB] || ",
            "hits": 179
        },
        {
            "id": 12728,
            "url": "https://svs.gsfc.nasa.gov/12728/",
            "result_type": "Produced Video",
            "release_date": "2017-09-22T17:00:00-04:00",
            "title": "What is Parker Solar Probe?",
            "description": "Parker Solar Probe will swoop to within four million miles of the Sun's surface, facing heat and radiation like no spacecraft before it. Launching in 2018, Parker Solar Probe will provide new data on solar activity and make critical contributions to our ability to forecast major space-weather events that impact life on Earth.Parker Solar Probe is an extraordinary and historic mission exploring arguably the last and most important region of the solar system to be visited by a spacecraft to finally answer top-priority science goals for over five decades.But we don't do this just for the basic science.One recent study by the National Academy of Sciences estimated that without advance warning a huge solar event could cause two trillion dollars in damage in the U.S. alone, and the eastern seaboard of the U.S. could be without power for a year.In order to unlock the mysteries of the corona, but also to protect a society that is increasingly dependent on technology from the threats of space weather, we will send Parker Solar Probe to touch the Sun. || ",
            "hits": 228
        },
        {
            "id": 12706,
            "url": "https://svs.gsfc.nasa.gov/12706/",
            "result_type": "Produced Video",
            "release_date": "2017-09-06T11:00:00-04:00",
            "title": "A Powerful Sequence of Flares Start September 2017",
            "description": "Short video showing the sequence of M and X flares starting on September 4, 2017 and culminating with an X9.3 flare — the largest of the solar cycle.Music: \"Networked\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || SDO_Flare_Still_3.jpg (1920x1080) [326.8 KB] || 12706_SDO_September_2017_Flares_ProRes_1920x1080_2997.mov (1920x1080) [2.9 GB] || 12706_SDO_September_2017_Flares_H264_Best_1080.mov (1920x1080) [1.1 GB] || 12706_SDO_September_2017_Flares_H264_Good_1080.m4v (1920x1080) [223.8 MB] || 12706_SDO_September_2017_Flares_Compatible.m4v (960x540) [90.1 MB] || 12706_SDO_September_2017_Flares_Compatible.webm (960x540) [23.8 MB] || 12706_SDO_September_2017_Flares_SRT_Captions.en_US.srt [2.4 KB] || 12706_SDO_September_2017_Flares_SRT_Captions.en_US.vtt [2.3 KB] || ",
            "hits": 189
        },
        {
            "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": 85
        },
        {
            "id": 12061,
            "url": "https://svs.gsfc.nasa.gov/12061/",
            "result_type": "Produced Video",
            "release_date": "2017-08-07T12:00:00-04:00",
            "title": "Eclipse Safety",
            "description": "Learn how to watch the 2017 American Eclipse safely. || BillIngalls_16x9.jpg (1153x649) [267.3 KB] || BillIngalls_1024x576.jpg (1024x576) [227.9 KB] || BillIngalls_1024x576_thm.png (80x40) [7.7 KB] || BillIngalls_1024x576_searchweb.png (320x180) [106.1 KB] || ",
            "hits": 118
        },
        {
            "id": 12105,
            "url": "https://svs.gsfc.nasa.gov/12105/",
            "result_type": "Produced Video",
            "release_date": "2017-08-04T09:00:00-04:00",
            "title": "Two Weeks in the Life of a Sunspot",
            "description": "Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credit: Foraging at Dusk by Benjamin James Parsons || sunspotthumb1_print.jpg (1024x576) [139.0 KB] || sunspotthumb1.jpg (1920x1080) [144.7 KB] || sunspotthumb1_thm.png (80x40) [8.2 KB] || sunspotthumb1_web.png (320x180) [137.9 KB] || sunspotthumb1_searchweb.png (320x180) [137.9 KB] || APPLE_TV-12105_Life_of_a_SunspotV5_appletv.m4v (1280x720) [56.1 MB] || 12105_Life_of_a_SunspotV5.webm (1920x1080) [12.4 MB] || APPLE_TV-12105_Life_of_a_SunspotV5_appletv_subtitles.m4v (1280x720) [56.1 MB] || FACEBOOK_720-12105_Life_of_a_SunspotV5_facebook_720.mp4 (1280x720) [131.6 MB] || LARGE_MP4-12105_Life_of_a_SunspotV5_large.mp4 (1920x1080) [114.4 MB] || YOUTUBE_1080-12105_Life_of_a_SunspotV5_youtube_1080.mp4 (1920x1080) [180.9 MB] || NASA_TV-12105_Life_of_a_SunspotV5.mpeg (1280x720) [377.0 MB] || YOUTUBE_HQ-12105_Life_of_a_SunspotV5_youtube_hq.mov (1920x1080) [805.0 MB] || PRORES_B-ROLL-12105_Life_of_a_SunspotV5_prores.mov (1280x720) [787.9 MB] || lifeofasunspotV5.en_US.vtt [1.3 KB] || lifeofasunspotV5.en_US.srt [1.3 KB] || 12105_Life_of_a_SunspotV5.mov (1920x1080) [1.5 GB] || NASA_PODCAST-12105_Life_of_a_SunspotV5_ipod_sm.mp4 (320x240) [19.1 MB] || 12105_Life_of_a_SunspotV5_lowres.mp4 (480x272) [15.4 MB] || ",
            "hits": 110
        },
        {
            "id": 12646,
            "url": "https://svs.gsfc.nasa.gov/12646/",
            "result_type": "Produced Video",
            "release_date": "2017-06-21T13:00:00-04:00",
            "title": "2017 Solar Eclipse Press Conference",
            "description": "For the first time in 99 years, a total solar eclipse will cross the entire nation Aug. 21. Representatives from NASA, other federal agencies, and science organizations, will provide important viewing safety, travel and science information during two briefings at the Newseum in Washington starting at 1 p.m. EDT Wednesday, June 21.The event will air live on NASA Television and stream on the agency’s website.Over the course of 100 minutes, 14 states across the United States will experience more than two minutes of darkness in the middle of the day. Additionally, a partial eclipse will be viewable across all of North America. The eclipse will provide a unique opportunity to study the sun, Earth, moon and their interaction because of the eclipse’s long path over land coast to coast. Scientists will be able to take ground-based and airborne observations over a period of an hour and a half to complement the wealth of data and images provided by space assets.The June 21 briefings are:Logistics Briefing: 1 to 2 p.m.Thomas Zurbuchen, associate administrator of NASA’s Science Mission Directorate at the agency’s headquarters in WashingtonVanessa Griffin, director of the National Oceanic and Atmospheric Administration’s Office of Satellite and Product Operations in Suitland, MarylandBrian Carlstrom, deputy associate director of Natural Resource Stewardship and Science at the National Park Service in WashingtonMartin Knopp, associate administrator of the Office of Operations in the Federal Highway Administration at the U.S. Department of Transportation in WashingtonScience Briefing: 2:30 to 3:30 p.m.Thomas ZurbuchenAngela Des Jardins, principal investigator of the Eclipse Ballooning Project at Montana State University, BozemanAngela Speck, professor of astrophysics and director of astronomy at the University of Missouri, ColumbiaDave Boboltz, program director of solar physics in the Division of Astronomical Sciences at the National Science Foundation in Arlington, VirginiaLinda Shore, executive director of the Astronomical Society of the Pacific in San FranciscoMatt Penn, astronomer at the National Solar Observatory in Tucson, Arizona || ",
            "hits": 53
        },
        {
            "id": 12517,
            "url": "https://svs.gsfc.nasa.gov/12517/",
            "result_type": "Produced Video",
            "release_date": "2017-06-21T00:00:00-04:00",
            "title": "Watching the Friendly Skies - Eclipse Safety Tutorial",
            "description": "Music Credit: Chic to Chic by Piero PiccioniWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || safetyThumbnail.jpg (1920x1080) [115.2 KB] || safetyThumbnail_searchweb.png (320x180) [92.4 KB] || safetyThumbnail_thm.png (80x40) [7.7 KB] || 12517_eclipse_safety_wpost.webm (1920x1080) [24.0 MB] || TWITTER_720-12517_eclipse_safety_wpost_VX-691382_twitter_720.mp4 (1280x720) [45.5 MB] || 12517_eclipse_safety_wpost.mp4 (1920x1080) [211.6 MB] || FACEBOOK_720-12517_eclipse_safety_wpost_VX-691382_facebook_720.mp4 (1280x720) [259.9 MB] || YOUTUBE_1080-12517_eclipse_safety_wpost_VX-691382_youtube_1080.mp4 (1920x1080) [346.3 MB] || YOUTUBE_720-12517_eclipse_safety_wpost_VX-691382_youtube_720.mp4 (1280x720) [347.9 MB] || 12517_eclipse_safety_wpost.en_US.srt [3.8 KB] || 12517_eclipse_safety_wpost.en_US.vtt [3.8 KB] || 12517_eclipse_safety_wpost_VX-691382_lowres.mp4 (480x272) [28.3 MB] || NASA_PODCAST-12517_eclipse_safety_wpost_VX-691382_ipod_sm.mp4 (320x240) [40.1 MB] || 12517_eclipse_safety_wpost.mov (1920x1080) [5.1 GB] || ",
            "hits": 50
        },
        {
            "id": 12614,
            "url": "https://svs.gsfc.nasa.gov/12614/",
            "result_type": "Produced Video",
            "release_date": "2017-06-02T11:00:00-04:00",
            "title": "SDO Anniversary Series",
            "description": "The sun is always changing and NASA's Solar Dynamics Observatory is always watching. Launched on Feb. 11, 2010, SDO keeps a 24-hour eye on the entire disk of the sun, with a prime view of the graceful dance of solar material coursing through the sun's atmosphere, the corona.Year 1 || ",
            "hits": 68
        },
        {
            "id": 12591,
            "url": "https://svs.gsfc.nasa.gov/12591/",
            "result_type": "Produced Video",
            "release_date": "2017-05-17T11:00:00-04:00",
            "title": "NASA's Van Allen Probes Find Human-Made Bubble Shrouding Earth",
            "description": "Music: Alternate and Parallel by Richard BirkinComplete transcript available. || 12591_VLF_bubbleV3.01194_print.jpg (1024x608) [101.5 KB] || 12591_VLF_bubbleV3.01194_searchweb.png (320x180) [58.6 KB] || 12591_VLF_bubbleV3.01194_thm.png (80x40) [5.6 KB] || 12591_VLF_bubbleV3_appletv.m4v (1280x720) [40.3 MB] || 12591_VLF_bubbleV3_appletv_subtitles.m4v (1280x720) [40.3 MB] || 12591_VLF_bubbleV3_prores.mov (1280x720) [555.6 MB] || 12591_VLF_bubbleV2.en_US.srt [1.3 KB] || 12591_VLF_bubbleV2.en_US.vtt [1.3 KB] || 12591_VLF_bubbleV3.webm (4000x2376) [12.6 MB] || 12591_VLF_bubbleV3_ipod_sm.mp4 (320x240) [15.1 MB] || 12591_VLF_bubbleV3.mov (4000x2376) [3.6 GB] || ",
            "hits": 67
        },
        {
            "id": 12593,
            "url": "https://svs.gsfc.nasa.gov/12593/",
            "result_type": "Produced Video",
            "release_date": "2017-05-17T11:00:00-04:00",
            "title": "Human Activity Impacted Space Weather",
            "description": "Music: Hybrid Technology by Le Fat Club [SACEM] Complete transcript available. || 12593_Anthropogenic_Space_WeatherV1_prores.00751_print.jpg (1024x576) [140.4 KB] || 12593_Anthropogenic_Space_WeatherV1_prores.00751_searchweb.png (320x180) [66.5 KB] || 12593_Anthropogenic_Space_WeatherV1_prores.00751_thm.png (80x40) [5.6 KB] || 12593_Anthropogenic_Space_WeatherV1_appletv.m4v (1280x720) [38.4 MB] || 12593_Anthropogenic_Space_WeatherV1_appletv_subtitles.m4v (1280x720) [38.5 MB] || 12593_Anthropogenic_Space_WeatherV1_prores.mov (1280x720) [607.9 MB] || 12593_Anthropogenic_Space_WeatherV1.mp4 (3908x2304) [84.0 MB] || 12593_Anthropogenic_Space_WeatherV1.en_US.srt [1.4 KB] || 12593_Anthropogenic_Space_WeatherV1.en_US.vtt [1.4 KB] || 12593_Anthropogenic_Space_WeatherV1_prores.webm [0 bytes] || 12593_Anthropogenic_Space_WeatherV1_youtube_hq.mov (4032x2376) [578.4 MB] || 12593_Anthropogenic_Space_WeatherV1_ipod_sm.mp4 (320x240) [14.0 MB] || 12593_Anthropogenic_Space_WeatherV1.mov (4032x2376) [4.4 GB] || ",
            "hits": 42
        },
        {
            "id": 12379,
            "url": "https://svs.gsfc.nasa.gov/12379/",
            "result_type": "Produced Video",
            "release_date": "2016-09-28T10:00:00-04:00",
            "title": "Space Radiation Highlights",
            "description": "A collection of space radiation highlights featuring:NASA's Van Allen ProbesNASA's CubeSats || ",
            "hits": 56
        },
        {
            "id": 12336,
            "url": "https://svs.gsfc.nasa.gov/12336/",
            "result_type": "Produced Video",
            "release_date": "2016-08-11T11:00:00-04:00",
            "title": "Solar Fireworks",
            "description": "A NASA spacecraft records a trio of flares on the sun. || c30-1024.jpg (1024x576) [196.5 KB] || c30-1280.jpg (1280x720) [267.1 KB] || c30-1920.jpg (1920x1080) [406.2 KB] || c30-1024_print.jpg (1024x576) [211.3 KB] || c30-1024_searchweb.png (320x180) [99.0 KB] || c30-1024_web.png (320x180) [99.0 KB] || c30-1024_thm.png (80x40) [7.1 KB] || ",
            "hits": 33
        },
        {
            "id": 12326,
            "url": "https://svs.gsfc.nasa.gov/12326/",
            "result_type": "Produced Video",
            "release_date": "2016-07-25T14:00:00-04:00",
            "title": "SDO Sees Trio of Mid-Level Flares",
            "description": "The sun emitted three mid-level solar flares on July 22-23, 2016, the strongest peaking at 1:16 am EDT on July 23. The sun is currently in a period of low activity, moving toward what's called solar minimum when there are few to no solar eruptions – so these flares were the first large ones observed since April. They are categorized as mid-strength flares, substantially less intense than the most powerful solar flares. || ",
            "hits": 30
        },
        {
            "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": 108
        },
        {
            "id": 12280,
            "url": "https://svs.gsfc.nasa.gov/12280/",
            "result_type": "Produced Video",
            "release_date": "2016-06-14T11:00:00-04:00",
            "title": "Seeing Earth's Magnetism",
            "description": "NASA spacecraft fly through a magnetic explosion in space, and scientists visualize the result. || cf-1024.jpg (1024x576) [236.1 KB] || cf-1280.jpg (1280x720) [322.6 KB] || cf-1024_print.jpg (1024x576) [249.2 KB] || cf-1024_searchweb.png (320x180) [108.4 KB] || cf-1024_web.png (320x180) [108.4 KB] || cf-1024_thm.png (80x40) [22.3 KB] || ",
            "hits": 79
        },
        {
            "id": 12267,
            "url": "https://svs.gsfc.nasa.gov/12267/",
            "result_type": "Produced Video",
            "release_date": "2016-06-09T11:00:00-04:00",
            "title": "How Earth Lost Its Cool",
            "description": "Scientists think solar storms may have been key to warming our planet. || c-1024.jpg (1024x576) [165.2 KB] || c-1280.jpg (1280x720) [234.6 KB] || c-1920.jpg (1920x1080) [360.8 KB] || c-1024_print.jpg (1024x576) [172.3 KB] || c-1024_searchweb.png (320x180) [93.6 KB] || c-1024_web.png (320x180) [93.6 KB] || c-1024_thm.png (80x40) [20.3 KB] || ",
            "hits": 49
        },
        {
            "id": 12249,
            "url": "https://svs.gsfc.nasa.gov/12249/",
            "result_type": "Produced Video",
            "release_date": "2016-05-24T11:00:00-04:00",
            "title": "Earth's Magnetism In Action",
            "description": "Scientists make a breakthrough in observing the dynamic magnetic system surrounding our planet. || c-1024.jpg (1024x576) [385.4 KB] || c-1280.jpg (1280x720) [576.4 KB] || c-1024_print.jpg (1024x576) [403.6 KB] || c-1024_searchweb.png (320x180) [137.4 KB] || c-1024_web.png (320x180) [137.4 KB] || c-1024_thm.png (80x40) [24.5 KB] || ",
            "hits": 152
        },
        {
            "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": 116
        },
        {
            "id": 4453,
            "url": "https://svs.gsfc.nasa.gov/4453/",
            "result_type": "Visualization",
            "release_date": "2016-05-12T14:00:00-04:00",
            "title": "Zoom in to MMS and Magnetopause Reconnection",
            "description": "The visualization starts with an overview of the MMS orbit. || MMSpursuit_Fly2Pursuit2Stop_Oct16data_RE_MMS.slate_RigRHS.HD1080i.0200_print.jpg (1024x576) [91.6 KB] || MMSpursuit_Fly2Pursuit2Stop_Oct16data_RE_MMS.slate_RigRHS.HD1080i.0200_searchweb.png (320x180) [71.3 KB] || MMSpursuit_Fly2Pursuit2Stop_Oct16data_RE_MMS.slate_RigRHS.HD1080i.0200_thm.png (80x40) [4.9 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || MMSpursuit_Fly2Pursuit2Stop_Oct16data_HD1080i_p30.mp4 (1920x1080) [81.6 MB] || MMSpursuit_Fly2Pursuit2Stop_Oct16data_HD1080i_p30.webm (1920x1080) [9.3 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || MMSpursuit_Fly2Pursuit2Stop_Oct16data.UHD3840p30.mp4 (3840x2160) [238.2 MB] || MMSpursuit_Fly2Pursuit2Stop_Oct16data_HD1080i_p30.mp4.hwshow [270 bytes] || ",
            "hits": 65
        },
        {
            "id": 20237,
            "url": "https://svs.gsfc.nasa.gov/20237/",
            "result_type": "Animation",
            "release_date": "2016-05-12T14:00:00-04:00",
            "title": "Beyond Earth - Earth's Geomagnetic Activity",
            "description": "Space is a better vacuum than any we can create on Earth, but it's nonetheless bustling with activity. It overflows with energy, particles and a complex system of magnetic field lines. This animation shows the busy-ness of near-Earth space, where the magnetic environment around Earth can trap electrons and charged particles. || beyondearth.jpg (1280x720) [261.9 KB] || beyondearth_searchweb.png (320x180) [136.2 KB] || beyondearth_thm.png (80x40) [22.8 KB] || BeyondEarthAnimatedGIFFinal30fpsv02.webm (1920x1080) [4.4 MB] || BeyondEarthAnimatedGIFFinal30fpsv02.mov (1920x1080) [429.8 MB] || BeyondEarthAnimatedGIFFinal60fpsv02.mov (1920x1080) [429.8 MB] || beyond-earth-earths-geomagnetic-activity.hwshow || ",
            "hits": 84
        },
        {
            "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": 127
        },
        {
            "id": 12229,
            "url": "https://svs.gsfc.nasa.gov/12229/",
            "result_type": "Produced Video",
            "release_date": "2016-04-28T17:23:20-04:00",
            "title": "An Explosion On The Sun",
            "description": "A NASA spacecraft captures stunning views of a solar flare. || c-1024.jpg (1024x576) [222.0 KB] || c-1280.jpg (1280x720) [302.9 KB] || c-1024_print.jpg (1024x576) [245.3 KB] || c-1024_searchweb.png (320x180) [108.1 KB] || c-1024_web.png (320x180) [108.1 KB] || c-1024_thm.png (80x40) [17.4 KB] || ",
            "hits": 82
        },
        {
            "id": 12220,
            "url": "https://svs.gsfc.nasa.gov/12220/",
            "result_type": "Produced Video",
            "release_date": "2016-04-21T11:00:00-04:00",
            "title": "Earth's Ionosphere",
            "description": "See why the night sky is never completely dark. || c-1024.jpg (1024x576) [81.4 KB] || c-1280.jpg (1280x720) [102.7 KB] || c-1920.jpg (1920x1080) [162.3 KB] || c-1024_print.jpg (1024x576) [90.5 KB] || c-1024_searchweb.png (320x180) [49.3 KB] || c-1024_web.png (320x180) [49.3 KB] || c-1024_thm.png (80x40) [4.6 KB] || ",
            "hits": 98
        },
        {
            "id": 12154,
            "url": "https://svs.gsfc.nasa.gov/12154/",
            "result_type": "Produced Video",
            "release_date": "2016-02-18T11:00:00-05:00",
            "title": "Sun Time-lapse",
            "description": "See a year in the life of the sun. || c-1024.jpg (1024x576) [155.9 KB] || c-1280.jpg (1280x720) [212.0 KB] || c-1920.jpg (1920x1080) [363.6 KB] || c-1024_print.jpg (1024x576) [160.5 KB] || c-1024_searchweb.png (320x180) [65.2 KB] || c-1024_web.png (320x180) [65.2 KB] || c-1024_thm.png (80x40) [19.4 KB] || ",
            "hits": 100
        },
        {
            "id": 12144,
            "url": "https://svs.gsfc.nasa.gov/12144/",
            "result_type": "Produced Video",
            "release_date": "2016-02-12T09:00:00-05:00",
            "title": "SDO: Year 6",
            "description": "This ultra-high definition (3840x2160) video shows the sun in the 171 angstrom wavelength of extreme ultraviolet light. It covers a time period of January 2, 2015 to January 28, 2016 at a cadence of one frame every hour, or 24 frames per day.  This timelapse is repeated with narration by solar scientist Nicholeen Viall and contains close-ups and annotations. 171 angstrom light highlights material around 600,000 Kelvin and shows features in the upper transition region and quiet corona of the sun. The video is available to download here at 59.94 frames per second, double the rate YouTube currently allows for UHD content.  The music is titled \"Tides\" and is from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || SDO_Year6_HCblend_HD.png (1920x1080) [5.3 MB] || SDO_Year6_HCblend_HD.jpg (1920x1080) [545.9 KB] || SDO_Year6_HCblend_HD_print.jpg (1024x576) [179.5 KB] || SDO_Year6_HCblend_UHD.png (3840x2160) [19.7 MB] || SDO_Year6_HCblend_UHD.jpg (3840x2160) [1.2 MB] || SDO_Year6_HCblend_HD_searchweb.png (180x320) [59.6 KB] || SDO_Year6_HCblend_HD_thm.png (80x40) [4.8 KB] || 12144_SDO_Year_6_appletv.webm (1280x720) [50.5 MB] || 12144_SDO_Year_6_appletv.m4v (1280x720) [241.9 MB] || 12144_SDO_Year_6_appletv_appletv_subtitles.m4v (1280x720) [242.1 MB] || SDO_Year_6_SRT_Captions.en_US.srt [6.3 KB] || SDO_Year_6_SRT_Captions.en_US.vtt [6.3 KB] || 12144_SDO_Year_6_H264_Good_1920x1080_2997.mov (1920x1080) [1.4 GB] || 12144_SDO_Year_6_H264_Good_3840x2160_2997.mov (3840x2160) [9.1 GB] || 12144_SDO_Year_6_H264_Good_3840x2160_5994.mov (3840x2160) [10.2 GB] || 12144_SDO_Year_6_ProRes_3840x2160_5994.mov (3840x2160) [50.3 GB] || ",
            "hits": 142
        },
        {
            "id": 12142,
            "url": "https://svs.gsfc.nasa.gov/12142/",
            "result_type": "Produced Video",
            "release_date": "2016-02-04T11:00:00-05:00",
            "title": "The Storm That Missed Earth",
            "description": "The big solar storm of 2012 was one for the record books. || c-1920.jpg (1920x1080) [858.4 KB] || c-1280.jpg (1280x720) [493.8 KB] || c-1024.jpg (1024x576) [333.3 KB] || c-1024_print.jpg (1024x576) [348.1 KB] || c-1024_searchweb.png (320x180) [115.4 KB] || c-1024_web.png (320x180) [115.4 KB] || c-1024_thm.png (80x40) [20.0 KB] || ",
            "hits": 699
        },
        {
            "id": 4391,
            "url": "https://svs.gsfc.nasa.gov/4391/",
            "result_type": "Visualization",
            "release_date": "2016-01-29T10:00:00-05:00",
            "title": "The Dynamic Solar Magnetic Field",
            "description": "A visualization of the slow changes of the solar magnetic field over the course of four years. || PFSSbasicView_inertial.HD1080i.0400_print.jpg (1024x576) [168.7 KB] || PFSSbasicView_inertial.HD1080i.0400_searchweb.png (180x320) [78.9 KB] || PFSSbasicView_inertial.HD1080i.0400_thm.png (80x40) [5.8 KB] || PFSSbasicView_inertial_1080p30.webm (1920x1080) [18.1 MB] || PFSSbasicView (1920x1080) [128.0 KB] || PFSSbasicView_inertial_1080p30.mp4 (1920x1080) [326.6 MB] || PFSSbasicView_inertial_1080p10.mp4 (1920x1080) [470.2 MB] || PFSSbasicView_HD1080p10.mov (1920x1080) [804.4 MB] || PFSSbasicView_inertial_1080p30.mp4.hwshow [232 bytes] || ",
            "hits": 151
        },
        {
            "id": 12073,
            "url": "https://svs.gsfc.nasa.gov/12073/",
            "result_type": "Produced Video",
            "release_date": "2015-12-10T11:00:00-05:00",
            "title": "Fast-Growing Sunspots",
            "description": "Scientists observe dynamic magnetic regions on the sun the size of planets. || cxf-1024.jpg (1024x576) [501.8 KB] || cxf-1024_print.jpg (1024x576) [515.3 KB] || cxf-1024_searchweb.png (320x180) [130.0 KB] || cxf-1024_web.png (320x180) [130.0 KB] || cxf-1024_thm.png (80x40) [26.9 KB] || ",
            "hits": 245
        },
        {
            "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": 69
        },
        {
            "id": 11935,
            "url": "https://svs.gsfc.nasa.gov/11935/",
            "result_type": "Produced Video",
            "release_date": "2015-09-29T11:00:00-04:00",
            "title": "Comet Hunter",
            "description": "A sun-observing spacecraft discovers its 3,000th comet. || c-1280.jpg (1280x720) [228.3 KB] || c-1024.jpg (1024x576) [165.9 KB] || c-1024_print.jpg (1024x576) [176.1 KB] || c-1024_searchweb.png (320x180) [91.4 KB] || c-1024_web.png (320x180) [91.4 KB] || c-1024_thm.png (80x40) [15.9 KB] || ",
            "hits": 25
        },
        {
            "id": 4342,
            "url": "https://svs.gsfc.nasa.gov/4342/",
            "result_type": "Visualization",
            "release_date": "2015-09-15T10:00:00-04:00",
            "title": "Sixteen Comets Touring the Inner Solar System",
            "description": "This visualization presents a small sample of the 9 years of comets seen by SOHO from the perspective a an observer at a fixed point above the ecliptic plane with the Sun at the center. || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [109.1 KB] || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [72.2 KB] || SixteenComets-oblique.slate_HAEmove.HD1080i.1000_thm.png (80x40) [4.3 KB] || SixteenComets-oblique.HD1080.webm (1920x1080) [11.3 MB] || SixteenComets-oblique.HD1080.mov (1920x1080) [109.2 MB] || Oblique (1920x1080) [512.0 KB] || SixteenComets-oblique_1080p30.mp4 (1920x1080) [64.2 MB] || ",
            "hits": 44
        },
        {
            "id": 4343,
            "url": "https://svs.gsfc.nasa.gov/4343/",
            "result_type": "Visualization",
            "release_date": "2015-09-15T10:00:00-04:00",
            "title": "Lots of Comets - Long trail version",
            "description": "This visualization presents 14 years of comets seen by SOHO from the perspective of an observer orbiting a fixed point above the ecliptic plane with the Sun at the center.This video is also available on our YouTube channel. || LotsaComets-orbit.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [110.2 KB] || LotsaComets-orbit.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [71.5 KB] || LotsaComets-orbit.slate_HAEmove.HD1080i.1000_thm.png (80x40) [4.7 KB] || Orbit (1920x1080) [512.0 KB] || LotsaComets-orbit_1080p30.mp4 (1920x1080) [188.3 MB] || LotsaComets-orbit_1080p30.webm (1920x1080) [20.8 MB] || ",
            "hits": 39
        },
        {
            "id": 4344,
            "url": "https://svs.gsfc.nasa.gov/4344/",
            "result_type": "Visualization",
            "release_date": "2015-09-15T10:00:00-04:00",
            "title": "Lots of Comets - Short trail version",
            "description": "This visualization presents 14 years of comets seen by SOHO from the perspective of an observer at a fixed point above the ecliptic plane with the Sun at the center. || LotsaCometsST-oblique.slate_HAEmove.HD1080i.1000_print.jpg (1024x576) [97.7 KB] || LotsaCometsST-oblique.slate_HAEmove.HD1080i.1000_searchweb.png (320x180) [65.2 KB] || LotsaCometsST-oblique.slate_HAEmove.HD1080i.1000_thm.png (80x40) [3.5 KB] || Oblique (1920x1080) [768.0 KB] || LotsaCometsST-oblique_1080p30.mp4 (1920x1080) [103.6 MB] || LotsaCometsST-oblique_1080p30.webm (1920x1080) [20.3 MB] || ",
            "hits": 20
        },
        {
            "id": 4333,
            "url": "https://svs.gsfc.nasa.gov/4333/",
            "result_type": "Visualization",
            "release_date": "2015-07-29T10:00:00-04:00",
            "title": "MMS Spacecraft Transition to Tetrahedral Flying Formation",
            "description": "This movie illustrates two orbits of the four MMS spacecraft. || Helio2015A.MMSPursuit.fieldlines_RigRHS.HD1080i.0570_print.jpg (1024x576) [111.7 KB] || Helio2015A.MMSPursuit.fieldlines_RigRHS.HD1080i.0570_searchweb.png (320x180) [72.4 KB] || Helio2015A.MMSPursuit.fieldlines_RigRHS.HD1080i.0570_thm.png (80x40) [4.3 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Helio2015A.MMSPursuit.fieldlines.HD1080.webm (1920x1080) [5.8 MB] || Helio2015A_1080p30.mp4 (1920x1080) [79.2 MB] || Helio2015A.MMSPursuit.fieldlines.HD1080.mov (1920x1080) [313.6 MB] || ",
            "hits": 52
        },
        {
            "id": 11916,
            "url": "https://svs.gsfc.nasa.gov/11916/",
            "result_type": "Produced Video",
            "release_date": "2015-07-23T11:45:00-04:00",
            "title": "Taking A Slice Of Light",
            "description": "Sometimes studying the sun requires looking at it one strip at a time. || c-1920.jpg (1920x1080) [542.3 KB] || c-1280.jpg (1280x720) [361.9 KB] || c-1024.jpg (1024x576) [269.6 KB] || c-1024_print.jpg (1024x576) [257.0 KB] || c-1024_searchweb.png (320x180) [121.9 KB] || c-1024_thm.png (80x40) [26.6 KB] || ",
            "hits": 38
        },
        {
            "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": 25
        },
        {
            "id": 11912,
            "url": "https://svs.gsfc.nasa.gov/11912/",
            "result_type": "Produced Video",
            "release_date": "2015-07-09T11:00:00-04:00",
            "title": "Arching Eruption",
            "description": "A NASA spacecraft sees the sun unleash a stunning explosion. || c-1920.jpg (1920x1080) [472.0 KB] || c-1280.jpg (1280x720) [293.8 KB] || c-1024.jpg (1024x576) [216.5 KB] || c-1024_print.jpg (1024x576) [208.1 KB] || c-1024_searchweb.png (320x180) [102.7 KB] || c-1024_thm.png (80x40) [22.4 KB] || ",
            "hits": 48
        },
        {
            "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": 49
        },
        {
            "id": 4318,
            "url": "https://svs.gsfc.nasa.gov/4318/",
            "result_type": "Visualization",
            "release_date": "2015-06-26T14:00:00-04:00",
            "title": "A Slice of Light: How IRIS Observes the Sun",
            "description": "Short version of the IRIS visualization with windowed SJI imagery. || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_print.jpg (1024x576) [122.9 KB] || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_searchweb.png (320x180) [95.6 KB] || SDO304IRISspectraWin4.2015MarA_stand.HD1080i.00400_thm.png (80x40) [7.6 KB] || SDO304IRISspectraWin4_1080p.mp4 (1920x1080) [22.3 MB] || Windowed.short (1920x1080) [128.0 KB] || SDO304IRISspectraWin4_1080p.webm (1920x1080) [4.3 MB] || ",
            "hits": 374
        },
        {
            "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": 30
        },
        {
            "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": 92
        },
        {
            "id": 4282,
            "url": "https://svs.gsfc.nasa.gov/4282/",
            "result_type": "Visualization",
            "release_date": "2015-03-25T00:00:00-04:00",
            "title": "March Solar X-flare from IRIS and SDO",
            "description": "Zoom in on the view of the flare, using SDO and IRIS. || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_print.jpg (1024x576) [151.2 KB] || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_searchweb.png (320x180) [88.9 KB] || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_web.png (320x180) [88.9 KB] || SDO304_IRIS1330_March2015A_stand.HD1080i.00500_thm.png (80x40) [6.9 KB] || SDO304_IRIS1330_March2015A_HD1080.webm (1920x1080) [4.0 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || SDO304_IRIS1330_March2015A_stand_HD1080.mp4 (1920x1080) [121.2 MB] || SDO304_IRIS1330_March2015A_HD1080.mov (1920x1080) [353.5 MB] || SDO304_IRIS1330_March2015A_stand_HD1080.mp4.hwshow [205 bytes] || ",
            "hits": 66
        },
        {
            "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": 68
        },
        {
            "id": 11805,
            "url": "https://svs.gsfc.nasa.gov/11805/",
            "result_type": "Produced Video",
            "release_date": "2015-03-11T14:00:00-04:00",
            "title": "Sun Emits an X2.2 Flare on March 11, 2015",
            "description": "An X2.2 class solar flare flashes in the middle of the sun on Mar. 11, 2015. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 171 and 131 angstrom wavelengths.Credit: NASA/GSFC/SDO || March_11_2015_X2pt2_Flare_171-131-crop_2.png (1920x1200) [12.7 MB] || March_11_2015_X2pt2_Flare_171-131-crop_2.jpg (1920x1200) [682.3 KB] || March_11_2015_X2pt2_Flare_171-131-crop_2_print.jpg (1024x640) [168.4 KB] || March_11_2015_X2pt2_Flare_171-131-crop_2_web.jpg (320x200) [24.0 KB] || March_11_2015_X2pt2_Flare_171-131-crop_2_searchweb.png (320x180) [118.6 KB] || March_11_2015_X2pt2_Flare_171-131-crop_2_thm.png (80x40) [10.5 KB] || ",
            "hits": 67
        },
        {
            "id": 11801,
            "url": "https://svs.gsfc.nasa.gov/11801/",
            "result_type": "Produced Video",
            "release_date": "2015-03-11T09:45:00-04:00",
            "title": "Goddard's Speedy MMS Instruments Will Measure Mysterious Physics",
            "description": "MMS Fast Plasma InvestigationHost Katrina Jackson talks with Craig Pollock and Ulrik Gliese about Goddard's contribution to the Magnetospheric Multiscale mission - the Fast Plasma Investigation suite of instruments.  These instruments will study a little-understood physics phenomenon known as magnetic reconnection, which is common throughout the universe and affects space weather in Earth's magnetosphere.  Watch the video on NASA Explorer. For complete transcript, click here. || MMS_FPI_thumbnail_print.jpg (1024x577) [129.0 KB] || MMS_FPI_thumbnail.png (1407x793) [1.3 MB] || MMS_FPI_thumbnail_thm.png (80x40) [9.9 KB] || MMS_FPI_thumbnail_web.png (320x180) [100.1 KB] || MMS_FPI_thumbnail_searchweb.png (320x180) [100.1 KB] || G2015-003_MMS_FPI_MASTER_youtube_hq.mov (1280x720) [299.8 MB] || G2015-003_MMS_FPI_MASTER_appletv_subtitles.m4v (960x540) [105.8 MB] || G2015-003_MMS_FPI_MASTER_appletv.m4v (960x540) [105.9 MB] || G2015-003_MMS_FPI_MASTER_prores.mov (1280x720) [3.7 GB] || G2015-003_MMS_FPI_MASTER_1280x720.wmv (1280x720) [122.7 MB] || G2015-003_MMS_FPI_MASTER_720x480.webm (720x480) [28.1 MB] || G2015-003_MMS_FPI_MASTER_ipod_lg.m4v (640x360) [41.8 MB] || G2015-003_MMS_FPI_MASTER_720x480.wmv (720x480) [114.2 MB] || MMS_FPI_captions.en_US.srt [5.3 KB] || MMS_FPI_captions.en_US.vtt [5.3 KB] || G2015-003_MMS_FPI_MASTER_nasaportal.mov (640x360) [103.0 MB] || G2015-003_MMS_FPI_MASTER_ipod_sm.mp4 (320x240) [22.6 MB] || ",
            "hits": 40
        },
        {
            "id": 11749,
            "url": "https://svs.gsfc.nasa.gov/11749/",
            "result_type": "Produced Video",
            "release_date": "2015-02-19T11:00:00-05:00",
            "title": "Sun Watcher",
            "description": "For more than five years, a NASA spacecraft has recorded the sun’s every move. || c-1280.jpg (1280x720) [258.3 KB] || c-1024.jpg (1024x576) [196.2 KB] || c-1024_print.jpg (1024x576) [197.5 KB] || c-1024_searchweb.png (320x180) [118.0 KB] || ",
            "hits": 52
        },
        {
            "id": 11742,
            "url": "https://svs.gsfc.nasa.gov/11742/",
            "result_type": "Produced Video",
            "release_date": "2015-02-11T10:00:00-05:00",
            "title": "SDO: Year 5",
            "description": "Highlights from the Solar Dynamics Observatory's five years of watching the sun.The music is \"Expanding Universe\" and \"Facing the Unknown\" both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here.Information about the individual clips used in this video is here.Credit: NASA's Goddard Space Flight Center/SDO || Year_5_STILL_print.jpg (1024x576) [73.2 KB] || Year_5_STILL_1080.jpg (1920x1080) [289.2 KB] || Year_5_STILL_1080.png (1920x1080) [2.2 MB] || Year_5_STILL.png (3840x2160) [8.1 MB] || SDO_Year_5_List.jpg (2550x3300) [988.9 KB] || Year_5_STILL.jpg (3840x2160) [857.5 KB] || Year_5_STILL_web.jpg (320x180) [14.0 KB] || Year_5_STILL_searchweb.png (180x320) [31.7 KB] || Year_5_STILL_thm.png (80x40) [6.0 KB] || SDO-Year_5_Final_appletv.webm (960x540) [35.1 MB] || SDO-Year_5_Final_appletv_subtitles.m4v (960x540) [123.0 MB] || SDO-Year_5_Final_appletv.m4v (960x540) [123.2 MB] || SDO-Year_5_Final_1280x720.wmv (1280x720) [145.5 MB] || 11742_SDO-Year_5_MPEG4_1920X1080_2997.mp4 (1920x1080) [373.3 MB] || 11742_SDO-Year_5_H264_Good_1280x720_2997.mov (1280x720) [737.8 MB] || SDO-Year_5_Final_ipod_lg.m4v (640x360) [50.5 MB] || 11742_SDO-Year_5.en_US.vtt [1.3 KB] || 11742_SDO-Year_5.en_US.srt [1.3 KB] || 11742_SDO-Year_5_H264_Good_1920x1080_2997.mov (1920x1080) [1.6 GB] || SDO-Year_5_Final_ipod_sm.mp4 (320x240) [26.7 MB] || 11742_SDO-Year_5_ProRes_1920x1080_2997.mov (1920x1080) [4.0 GB] || 11742_SDO-Year_5_H264_Best_1920x1080_2997.mov (1920x1080) [5.1 GB] || 11742_SDO-Year_5_MPEG4_1920X1080_2997.hwshow [123 bytes] || ",
            "hits": 161
        },
        {
            "id": 11737,
            "url": "https://svs.gsfc.nasa.gov/11737/",
            "result_type": "Produced Video",
            "release_date": "2015-02-05T11:00:00-05:00",
            "title": "Tracking Solar Eruptions",
            "description": "Explore how scientists trace the journey of material exploding from the sun. || c-1024.jpg (1024x576) [129.9 KB] || c-1920.jpg (1920x1080) [290.2 KB] || c-1280.jpg (1280x720) [181.0 KB] || c-1024_print.jpg (1024x576) [126.9 KB] || c-1024_searchweb.png (320x180) [78.3 KB] || c-1024_print_thm.png (80x40) [14.7 KB] || ",
            "hits": 52
        },
        {
            "id": 11745,
            "url": "https://svs.gsfc.nasa.gov/11745/",
            "result_type": "Produced Video",
            "release_date": "2015-02-05T00:00:00-05:00",
            "title": "Solarium - Resource Page",
            "description": "A child looks up at Solarium at the Goddard Visitor Center in Greenbelt, Maryland.Photo Credit: NASA's Goddard Space Flight Center || E_LowAngle_304_crop_print.jpg (1024x677) [110.0 KB] || E_LowAngle_304_crop.png (3938x2604) [11.3 MB] || E_LowAngle_304_crop.jpg (3938x2604) [1.8 MB] || E_LowAngle_304_crop_web.png (320x211) [82.5 KB] || ",
            "hits": 68
        },
        {
            "id": 11739,
            "url": "https://svs.gsfc.nasa.gov/11739/",
            "result_type": "Produced Video",
            "release_date": "2015-01-20T11:00:00-05:00",
            "title": "Telescope on NASA's SDO Collects Its 100 Millionth Image",
            "description": "100 million images of the sun: The Advanced Imaging Assembly on NASA's Solar Dynamics Observatory captured its 100 millionth image of the sun on Jan. 19, 2015. The image shows the glow in the solar atmosphere of gases at about 1.5 million Kelvin. Credit: NASA/SDO/AIA/LMSAL || SDO_AIA_193_100Millionth_print.jpg (1024x1024) [168.6 KB] || SDO_AIA_193_100Millionth.jpeg (4096x4096) [2.4 MB] || SDO_AIA_193_100Millionth_web.jpg (320x320) [27.3 KB] || SDO_AIA_193_100Millionth_searchweb.png (320x180) [95.6 KB] || SDO_AIA_193_100Millionth_thm.png (80x40) [10.2 KB] || ",
            "hits": 311
        },
        {
            "id": 11700,
            "url": "https://svs.gsfc.nasa.gov/11700/",
            "result_type": "Produced Video",
            "release_date": "2015-01-15T11:00:00-05:00",
            "title": "Exploring Earth's Magnetism",
            "description": "In March 2015, NASA will launch four spacecraft to study how magnetic fields around Earth connect and disconnect—a process known as magnetic reconnection. Magnetic reconnections take place on the day and night side of the planet and are caused by the interaction of Earth’s magnetic field with charged particles released from the sun called the solar wind. The four spacecraft, each identically engineered, make up the Magnetospheric Multiscale, or MMS, mission. Flying in a pyramid-shaped configuration, the spacecraft will orbit Earth and pass through areas known to be reconnection sites. Each reconnection event unleashes a massive burst of energy that can accelerate particles within Earth’s protective magnetic environment, known as the magnetosphere, to nearly the speed of light. Sensors onboard the spacecraft will measure the energy and movement of charged particles during an event, providing scientists with the first three-dimensional look at this phenomenon. Watch the video to learn more. || ",
            "hits": 43
        },
        {
            "id": 11689,
            "url": "https://svs.gsfc.nasa.gov/11689/",
            "result_type": "Produced Video",
            "release_date": "2014-12-09T11:00:00-05:00",
            "title": "Modeling Earth's Magnetism",
            "description": "Surrounding Earth is a giant magnetic field called the magnetosphere. Its shape is defined not only by the planet's north and south magnetic poles, but also by a steady stream of particles coming in from the sun called the solar wind. The magnetosphere is buffeted by this wind and can change shape dramatically when the sun lets loose an immense cloud of gas known as a coronal mass ejection. To understand and predict the impact of such space weather events on Earth, the Community-Coordinated Modeling Center at NASA’s Goddard Space Flight Center routinely runs computer simulations of past eruptions. Solar storms can inflict serious damage on things like power grids and Earth-orbiting satellites. The simulations let scientists estimate the consequences of outbursts of different magnitude, helping us to better plan for the future. Watch the video to learn more. || ",
            "hits": 221
        },
        {
            "id": 11682,
            "url": "https://svs.gsfc.nasa.gov/11682/",
            "result_type": "Produced Video",
            "release_date": "2014-11-13T11:00:00-05:00",
            "title": "Strange Days On The Sun",
            "description": "On October 18, 2014, a gigantic sunspot on the lower half of the sun rotated into view of NASA’s Solar Dynamics Observatory, or SDO, spacecraft. The sunspot measured 80,000 miles across—big enough to engulf at least a dozen Earths and larger than any seen in more than two decades. With temperatures around 7,000°F, sunspots are relatively cooler areas on the sun. In images taken at visible wavelengths they appear as dark spots on the sun’s surface, hence their name. Over the next 14 days, the massive sunspot unleashed multiple bursts of radiation known as solar flares. Some of these flares were classified as X-class, the strongest type of flare. The mightiest X-class flares (degree is indicated by number, with 1 being the lowest) are by far the largest explosions in the solar system and are awesome to watch. See views of different eruptions captured by SDO in the video. || ",
            "hits": 67
        },
        {
            "id": 10158,
            "url": "https://svs.gsfc.nasa.gov/10158/",
            "result_type": "Produced Video",
            "release_date": "2014-11-05T14:00:00-05:00",
            "title": "A Series of Flares from November Active Region 12205",
            "description": "Cropped image of the Nov. 7, 2014 X1.6 flare, as seen by NASA's Solar Dynamics Observatory in a blend of 171 and 131 angstroms.Credit: NASA/GSFC/SDO || 20141107_131.171blendX1.6CROP.jpg (1472x808) [143.0 KB] || 20141107_131.171blendX1.6CROP_print.jpg (1024x562) [170.0 KB] || 20141107_131.171blendX1.6CROP_searchweb.png (320x180) [118.6 KB] || 20141107_131.171blendX1.6CROP_web.png (320x175) [116.2 KB] || 20141107_131.171blendX1.6CROP_thm.png (80x40) [26.6 KB] || ",
            "hits": 24
        },
        {
            "id": 11678,
            "url": "https://svs.gsfc.nasa.gov/11678/",
            "result_type": "Produced Video",
            "release_date": "2014-10-30T11:45:00-04:00",
            "title": "Solar Explosions",
            "description": "On October 2, 2014, the sun unleashed a powerful burst of radiation known as a solar flare. The flare erupted on the right side of the sun, emitting a bright flash of light. Along with a sudden release of energy, a cloud of solar material shot up into the sun’s outer atmosphere, the corona. This region of the sun is millions of miles thick and consists of strong magnetic fields that extend far into space. NASA's Solar Dynamics Observatory, which watches the sun 24 hours a day, captured images of the explosions in multiple wavelengths. Views collected by the spacecraft help scientists monitor the sun and predict how changes in its activity will affect our planet. Watch the video to see the explosions up close. || ",
            "hits": 264
        },
        {
            "id": 11718,
            "url": "https://svs.gsfc.nasa.gov/11718/",
            "result_type": "Produced Video",
            "release_date": "2014-10-24T23:00:00-04:00",
            "title": "Giant Sunspot Continues to Erupt with Substantial Flares",
            "description": "Video tracking a giant sunspot from Oct. 19 - Oct. 27, 2014. The active region released many significant flares. This video highlights 5 X-class flares. NASAexplorer YouTube channel. || xclass720.jpg (1280x720) [145.6 KB] || xclass720_print.jpg (1024x576) [169.8 KB] || xclass720_searchweb.png (320x180) [123.9 KB] || xclass720_web.png (320x180) [123.9 KB] || xclass720_thm.png (80x40) [26.4 KB] || 11718_Five_X-class_flaresV3_ProRes_1920x1080_2997.mov (1920x1080) [3.0 GB] || G2014-096_Five_X-class_flaresV3-H264_Best_1920x1080_2997.mov (1920x1080) [3.6 GB] || G2014-096_Five_X-class_flaresV3_youtube_hq.mov (1920x1080) [1.3 GB] || G2014-096_Five_X-class_flaresV3_appletv.m4v (960x540) [87.3 MB] || G2014-096_Five_X-class_flaresV3_1280x720.wmv (1280x720) [103.7 MB] || G2014-096_Five_X-class_flaresV3_appletv_subtitles.m4v (960x540) [87.2 MB] || G2014-096_Five_X-class_flaresV3_appletv.webmhd.webm (960x540) [47.6 MB] || G2014-096_Five_X-class_flaresV3_ipod_lg.m4v (640x360) [35.0 MB] || G2014-096_Five_X-class_flaresV3.en_US.srt [1.8 KB] || G2014-096_Five_X-class_flaresV3.en_US.vtt [1.8 KB] || G2014-096_Five_X-class_flaresV3_ipod_sm.mp4 (320x240) [19.0 MB] || ",
            "hits": 288
        },
        {
            "id": 11717,
            "url": "https://svs.gsfc.nasa.gov/11717/",
            "result_type": "Produced Video",
            "release_date": "2014-10-22T09:00:00-04:00",
            "title": "Second Substantial Flare in Two Days",
            "description": "An active region on the sun erupted with a mid-level flare on Oct. 21, 2014, as seen in the bright light of this image captured by NASA's Solar Dynamics Observatory. This image shows extreme ultraviolet light that highlights the hot solar material in the sun's atmosphere. Credit: NASA/GSFC/SDO || Oct_21_Mflare_304-171-soft_Crop.jpg (2048x1536) [938.6 KB] || Oct_21_Mflare_304-171-soft_Crop_print.jpg (1024x768) [171.6 KB] || Oct_21_Mflare_304-171-soft_Crop_web.jpg (320x240) [26.4 KB] || Oct_21_Mflare_304-171-soft_Crop_searchweb.png (320x180) [84.6 KB] || Oct_21_Mflare_304-171-soft_Crop_thm.png (80x40) [8.5 KB] || Oct_21_Mflare_304-171-soft_Crop.tiff (2048x1536) [24.0 MB] || ",
            "hits": 55
        },
        {
            "id": 11708,
            "url": "https://svs.gsfc.nasa.gov/11708/",
            "result_type": "Produced Video",
            "release_date": "2014-10-16T14:00:00-04:00",
            "title": "NASA's IRIS Helps Explain Mysterious Heat of the Solar Atmosphere",
            "description": "This movie shows succeeding images from NASA’s IRIS of the same area of the sun in different wavelengths.  Each image carries information about how fast the solar material is moving, which has shown scientists that a series of loops are twisting in the sun’s lower atmosphere.Credit: NASA/IRIS/Pereira || S3_still.png (1534x1154) [1.1 MB] || S3_still_web.jpg (319x240) [22.4 KB] || S3_still_searchweb.png (320x180) [67.4 KB] || S3_still_thm.png (80x40) [8.5 KB] || S3.mov (768x576) [2.8 MB] || S3.webmhd.webm (960x540) [1.8 MB] || ",
            "hits": 37
        },
        {
            "id": 11711,
            "url": "https://svs.gsfc.nasa.gov/11711/",
            "result_type": "Produced Video",
            "release_date": "2014-10-10T13:00:00-04:00",
            "title": "Pumpkin Sun",
            "description": "On October 8, 2014, active regions on the sun gave it the appearance of a jack-o'-lantern.  This image is a blend of 171 and 193 angstrom light as captured by the Solar Dynamics Observatory.Credit: NASA/GSFC/SDO || Halloween_Sun_2014_2k.jpg (2048x2048) [1.2 MB] || Halloween_Sun_2014_1k.jpg (1024x1024) [209.2 KB] || Halloween_Sun_2014_2k_print.jpg (1024x1024) [185.7 KB] || Halloween_Sun_2014.jpg (4096x4096) [3.3 MB] || Halloween_Sun_2014_web.jpg (320x320) [26.3 KB] || Halloween_Sun_2014_2k_searchweb.png (320x180) [86.1 KB] || Halloween_Sun_2014_2k_thm.png (80x40) [8.8 KB] || Halloween_Sun_2014_2k.tiff (2048x2048) [32.0 MB] || Halloween_Sun_2014.tiff (4096x4096) [128.0 MB] || ",
            "hits": 155
        },
        {
            "id": 11705,
            "url": "https://svs.gsfc.nasa.gov/11705/",
            "result_type": "Produced Video",
            "release_date": "2014-10-06T14:00:00-04:00",
            "title": "NASA's SDO Watches Giant Filament on the Sun",
            "description": "A snaking, extended filament of solar material currently lies on the front of the sun— some 1 million miles across from end to end. Filaments are clouds of solar material suspended above the sun by powerful magnetic forces. Though notoriously unstable, filaments can last for days or even weeks.NASA's Solar Dynamics Observatory, or SDO, which watches the sun 24 hours a day, has observed this gigantic filament for several days as it rotated around with the sun. If straightened out, the filament would reach almost across the whole sun, about 1 million miles or 100 times the size of Earth.SDO captured images of the filament in numerous wavelengths, each of which helps highlight material of different temperatures on the sun. By looking at any solar feature in different wavelengths and temperatures, scientists can learn more about what causes such structures, as well as what catalyzes their occasional giant eruptions out into space.Look at the images to see how the filament appears in different wavelengths. The brownish combination image was produced by blending two wavelengths of extreme UV light with a wavelength of 193 and 335 angstroms. The red image shows the 304 angstrom wavelength of extreme UV light. || ",
            "hits": 57
        },
        {
            "id": 11670,
            "url": "https://svs.gsfc.nasa.gov/11670/",
            "result_type": "Produced Video",
            "release_date": "2014-10-03T15:00:00-04:00",
            "title": "Sun Emits Mid-Level Flare on October 2, 2014",
            "description": "The sun emitted a mid-level solar flare, peaking at 3:01 p.m. EDT on Oct. 2, 2014.  NASA's Solar Dynamics Observatory, which watches the sun 24-hours a day, captured images of the flare. 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.This flare is classified as an M7.3 flare. M-class flares are one-tenth as powerful as the most powerful flares, which are designated X-class flares. || ",
            "hits": 139
        },
        {
            "id": 11558,
            "url": "https://svs.gsfc.nasa.gov/11558/",
            "result_type": "Produced Video",
            "release_date": "2014-09-24T10:00:00-04:00",
            "title": "NASA's Many Views of a Massive CME",
            "description": "On July 23, 2012, a massive cloud of solar material erupted off the sun's right side, zooming out into space. It soon passed one of NASA's Solar Terrestrial Relations Observatory, or STEREO, spacecraft, which clocked the CME as traveling between 1,800 and 2,200 miles per second as it left the sun. This was the fastest CME ever observed by STEREO.  Two other observatories – NASA's Solar Dynamics Observatory and the joint European Space Agency/NASA Solar and Heliospheric Observatory — witnessed the eruption as well. The July 2012 CME didn't move toward Earth, but watching an unusually strong CME like this gives scientists an opportunity to observe how these events originate and travel through space.  STEREO's unique viewpoint from the sides of the sun combined with the other two observatories watching from closer to Earth helped scientists create models of the entire July 2012 event. They learned that an earlier, smaller CME helped clear the path for the larger event, thus contributing to its unusual speed. Such data helps advance our understanding of what causes CMEs and improves modeling of similar CMEs that could be Earth-directed. || ",
            "hits": 250
        },
        {
            "id": 11642,
            "url": "https://svs.gsfc.nasa.gov/11642/",
            "result_type": "Produced Video",
            "release_date": "2014-09-23T11:45:00-04:00",
            "title": "Solar Edge",
            "description": "How big is the sun’s atmosphere? In a word: huge. Like Earth, the sun’s atmosphere consists of multiple layers. It has a lower atmosphere, called the chromosphere, and a significantly larger upper atmosphere, called the corona. Although the exact boundaries of these regions are fuzzy, the outer limit of the corona is marked by the place where the sun’s solar wind breaks free. Using NASA’s STEREO spacecraft, scientists have found the extent of the corona is greater than previously thought, stretching some five million miles from the surface. The distance is equivalent to approximately six times the sun's length. Knowing this information will help guide the planning of future sun-observing missions. Watch the video to see solar material streaming from the sun. || ",
            "hits": 34
        },
        {
            "id": 11667,
            "url": "https://svs.gsfc.nasa.gov/11667/",
            "result_type": "Produced Video",
            "release_date": "2014-09-22T10:00:00-04:00",
            "title": "The Difference Between CMEs and Flares",
            "description": "Coronal mass ejections (CMEs) and flares are both solar events, but they are not the same. This video shows the differences between the two by highlighting specific features of each. || ",
            "hits": 327
        },
        {
            "id": 11651,
            "url": "https://svs.gsfc.nasa.gov/11651/",
            "result_type": "Produced Video",
            "release_date": "2014-09-11T08:00:00-04:00",
            "title": "September 10, 2014 X1.6 flare",
            "description": "The sun emitted a significant solar flare, peaking at 1:48 p.m. EDT on Sept. 10, 2014. NASA's Solar Dynamics Observatory captured images 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.This flare is classified as an X1.6 class flare. \"X-class\" denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc. || ",
            "hits": 112
        },
        {
            "id": 11599,
            "url": "https://svs.gsfc.nasa.gov/11599/",
            "result_type": "Produced Video",
            "release_date": "2014-08-28T11:30:00-04:00",
            "title": "Beautiful Explosion",
            "description": "A giant burst of solar material surged off the side of the sun on May 9, 2014—and NASA's newest sun-watching mission caught the event in extraordinary detail. This was the first explosion known as a coronal mass ejection (CME) that the Interface Region Imaging Spectrograph, or IRIS, spacecraft was able to observe. The spacecraft must commit to pointing at certain areas of the sun at least a day in advance, so catching a CME in the act involves some educated guesses and a little bit of luck. On this day it focused in on the left side of the sun and happened to see the base of the CME.  It recorded super-hot material erupting from the sun at speeds of 1.5 million mph. Watch the video to see it for yourself. || ",
            "hits": 28
        },
        {
            "id": 11613,
            "url": "https://svs.gsfc.nasa.gov/11613/",
            "result_type": "Produced Video",
            "release_date": "2014-08-01T10:00:00-04:00",
            "title": "EUNIS Sees Evidence for Nanoflare Heating",
            "description": "Scientists have recently gathered some of the strongest evidence to date to explain what makes the sun's outer atmosphere so much hotter than its surface. The new observations show temperatures in the atmosphere so hot that only one current theory explains them: something called nanoflares – a constant peppering of impulsive bursts of heating, none of which can be individually detected — provide the mysterious extra heat. These new observations come from just six minutes worth of data from one of NASA's least expensive type of missions, a sounding rocket. The EUNIS mission, short for Extreme Ultraviolet Normal Incidence Spectrograph, launched on April 23, 2013, gathering a new snapshot of data every 1.3 seconds to track the properties of material over a wide range of temperatures in the complex solar atmosphere. The unique capabilities of EUNIS enabled researchers to obtain these results. The spectrograph was able to clearly and unambiguously distinguish the observations representing the extremely hot material – emission lines showing light with a wavelength of 592.6 angstrom, where an angstrom is the size of an atom — from a very nearby light wavelength of 592.2 angstroms. || ",
            "hits": 27
        },
        {
            "id": 11602,
            "url": "https://svs.gsfc.nasa.gov/11602/",
            "result_type": "Produced Video",
            "release_date": "2014-07-03T11:00:00-04:00",
            "title": "STEREO Solar Conjunction",
            "description": "Since February 2011, the two spacecraft of NASA's STEREO mission have been providing scientists with unprecedented views of the far side of the sun. Placed in an orbit that allows their perspective to changed over the eight years since their launch in 2008 (ck), the satellites are about to enter a new phase of their journey: a time when the bright light and heat of the sun will stand in the way of sending data back to Earth.This phase is a direct result of the orbits for STEREO, which is short for the Solar Terrestrial Relations Observatory. The spacecraft travel at different speeds. This means that over time, the satellites become increasingly out of sync, appearing from Earth's perspective to drift farther apart, able to observe first the sides and eventually the far side of the sun. For the first time ever, thanks to STEREO and near-Earth solar telescopes such as NASA’s Solar Dynamics Observatory the human race has had its first 360-degree view of the sun.The orbits have continued to cause the STEREO spacecraft's position to change, however, and now they are nearing each other once again, this time on the other side of the sun. During this period when the sun blocks Earth's view — a geometrical position known in astronomy as a superior conjunction — radio receivers on Earth will not be able to distinguish STEREO's signal from the sun's radiation. Communication with the spacecraft will cease and the satellites will both go into safe mode without collecting data for a time. This will happen for STEREO-Ahead from March 24 to July 7, 2015. STEREO-Behind will be in superior conjunction from Jan. 22 to March 23, 2015. At least one spacecraft, therefore, will always be collecting data. Before this occurs, the heating from the sun will also begin to affect – though not shut down — data collection. From wherever they are in space, the STEREO spacecraft aim their antenna toward Earth to send down data. This position puts the antenna fairly close to pointing at the sun, exposing the instruments to more heat than it can safely bear. The antenna can be adjusted to point in different directions, but the signal coming to Earth will be much fainter and won't allow for as much data to be downloaded.  This antenna adjustment will begin on Aug. 20, 2014, for the STEREO-Ahead spacecraft and on Dec. 1, 2014, for STEREO-Behind. During this phase, STEREO instruments will continue to run 24 hours a day, but they will gather lower-resolution data than usual. Some of this data will be downloaded whenever STEREO can link up with an Earth receiver. The rest of the data will be stored on board to be downloaded when the spacecraft reach a more auspicious geometrical position in early 2016. To test for this off-pointing from the sun, STEREO-Ahead will undergo tests and not be collecting data from July 6-12, 2014.  The same tests will be performed on STEREO-Behind from Sept. 29 – Oct. 6, 2014. Throughout this entire phase until 2016, at least one STEREO spacecraft will be capturing data at any one time, so scientists will have an uninterrupted record of events on the sun to coordinate with the observations of solar telescopes on the Earth side. Real time monitoring of the sun, its flares and coronal mass ejections – information used by the US National Oceanic and Atmospheric Administration to help forecast space weather — will also continue via a fleet of NASA spacecraft closer to Earth. || ",
            "hits": 38
        }
    ]
}