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    "results": [
        {
            "id": 31380,
            "url": "https://svs.gsfc.nasa.gov/31380/",
            "result_type": "Hyperwall Visual",
            "release_date": "2026-03-30T12:00:00-04:00",
            "title": "APEX-12 (Advanced Plant EXperiment-12) on the ISS",
            "description": "The findings of the APEX series of experiments offer insight into the effects of spaceflight on plant chromosomes, and how these findings could impact human health.",
            "hits": 310
        },
        {
            "id": 14956,
            "url": "https://svs.gsfc.nasa.gov/14956/",
            "result_type": "Produced Video",
            "release_date": "2026-01-26T16:00:00-05:00",
            "title": "Space Weather Effects Animations",
            "description": "Solar flares, coronal mass ejections, solar particle events, and the solar wind form the recipe for space weather that affects life on Earth and astronauts in space. A farmer stops their planting operations due to poor GPS signal for their autonomous tractor. A power grid manager changes the configuration of their network to ensure a blackout doesn’t occur due to voltage instability. A pilot switches to back-up communication equipment due to loss of high-frequency radio. A commercial internet company providing service to the military must change the orbit of their spacecraft to avoid a collision due to increased atmospheric drag.These are a few examples of the ways the Sun influences our everyday lives. This is what we define as space weather – the conditions of the space environment driven by the Sun and it’s impacts on objects in the solar system. Learn more about space weather: https://science.nasa.gov/space-weather-2/ || ",
            "hits": 504
        },
        {
            "id": 5373,
            "url": "https://svs.gsfc.nasa.gov/5373/",
            "result_type": "Visualization",
            "release_date": "2024-09-03T13:00:00-04:00",
            "title": "PREFIRE First Light",
            "description": "Visualization emphasizing two passes of PREFIRE over Greenland. Information about the rates of atmospheric emission can be derived from the change in emission at the intersection of the passes. || prefire_first_light_FINAL_2160p30.00450_print.jpg (1024x576) [224.8 KB] || prefire_first_light_FINAL_2160p30.00450_thm.png (80x40) [6.3 KB] || prefire_first_light_FINAL_2160p30.00450_searchweb.png (320x180) [78.7 KB] || prefire_first_light_FINAL [0 Item(s)] || prefire_first_light_FINAL_1080p30.mp4 (1920x1080) [47.2 MB] || prefire_first_light_FINAL_4K [0 Item(s)] || prefire_first_light_FINAL_2160p30.mp4 (3840x2160) [133.7 MB] || prefire_first_light_FINAL_2160p30.mp4.hwshow [199 bytes] || ",
            "hits": 73
        },
        {
            "id": 5173,
            "url": "https://svs.gsfc.nasa.gov/5173/",
            "result_type": "Visualization",
            "release_date": "2023-10-10T00:00:00-04:00",
            "title": "Earth's Radiation Balance, 2000-2023",
            "description": "A plotted view of planetary heat uptake since the beginning of the CERES data record showing an oscillating, monthly mean (yellow) and twelve-month running average (red line). These data show how much energy is added (absorbed) by Earth during the CERES period. || planetary_heat_anomaly.1800_print.jpg (1024x576) [69.7 KB] || planetary_heat_anomaly.1800_searchweb.png (320x180) [21.2 KB] || planetary_heat_anomaly.1800_thm.png (80x40) [3.0 KB] || phu_2023 (3840x2160) [0 Item(s)] || planetary_heat_anomaly_2160p60.mp4 (3840x2160) [4.2 MB] || ",
            "hits": 358
        },
        {
            "id": 4935,
            "url": "https://svs.gsfc.nasa.gov/4935/",
            "result_type": "Visualization",
            "release_date": "2021-04-16T00:00:00-04:00",
            "title": "CERES Radiation Balance",
            "description": "A plotted view of planetary heat uptake since the beginning of the CERES data record showing an oscillating, monthly mean (yellow) and twelve-month running average (red line). These data show how much energy is added (absorbed) by Earth during the CERES period. || CERES_2021_update_final.01650_print.jpg (1024x576) [69.5 KB] || CERES_2021_update_final.01650_searchweb.png (320x180) [23.5 KB] || CERES_2021_update_final.01650_thm.png (80x40) [3.3 KB] || CERES_2021_update_final.mp4 (1920x1080) [9.2 MB] || CERES_2021_update_final.webm (1920x1080) [6.2 MB] || CERES_2021_update_final.mp4.hwshow [194 bytes] || ",
            "hits": 119
        },
        {
            "id": 4817,
            "url": "https://svs.gsfc.nasa.gov/4817/",
            "result_type": "Visualization",
            "release_date": "2020-04-17T00:00:00-04:00",
            "title": "Earth Day 2020: CERES Net TOA Radiation",
            "description": "CERES Net TOA Radiation, WIth LabelsThis video is also available on our YouTube channel. || ceres_w_labels.00001_print.jpg (1024x576) [98.8 KB] || ceres_w_labels.00001_searchweb.png (320x180) [51.5 KB] || ceres_w_labels.00001_thm.png (80x40) [4.4 KB] || ceres_w_labels.webm (1920x1080) [6.9 MB] || ceres_w_labels.mp4 (1920x1080) [111.3 MB] || captions_silent.29564.en_US.srt [43 bytes] || ceres_w_labels.mp4.hwshow [180 bytes] || ",
            "hits": 51
        },
        {
            "id": 4794,
            "url": "https://svs.gsfc.nasa.gov/4794/",
            "result_type": "Visualization",
            "release_date": "2020-02-21T08:00:00-05:00",
            "title": "CERES Radiation Balance",
            "description": "The Clouds and the Earth’s Energy Radiant System (CERES) instrument is a key component of NASA’s Earth Observing System, with six active CERES instruments on satellites orbiting Earth and taking data.  For Earth’s temperature to be stable over long periods of time, absorbed solar and emitted thermal radiation must be equal. Increases in greenhouse gases, like carbon dioxide and methane, trap emitted thermal radiation from the surface and reduce how much is lost to space, resulting in a net surplus of energy into the Earth system. Most of the extra energy ends up being stored as heat in the ocean and the remainder warms the atmosphere and land, and melts snow and ice. As a consequence, global mean surface temperature increases and sea levels rise. Much like a pulse or heartbeat, CERES monitors reflected solar and emitted thermal infrared radiation, which together with solar irradiance measurements is one of Earth’s ‘vital signs.’ Better understanding Earth’s energy balance enables us to be informed and adapt to a changing world. || ",
            "hits": 156
        },
        {
            "id": 13315,
            "url": "https://svs.gsfc.nasa.gov/13315/",
            "result_type": "Produced Video",
            "release_date": "2019-09-17T10:00:00-04:00",
            "title": "Apollo Moon Soil Radiation Experiment",
            "description": "Profile of the Radiation Effects Laboratory at the Goddard Space Flight Center in Greenbelt, Maryland. Song: \"Gateway Identified\" from Universal Production Music. Watch this video on the NASA Goddard YouTube channel. || 13315_New_Thumb_print.jpg (1024x576) [125.3 KB] || 13315_New_Thumb.jpg (3840x2160) [573.4 KB] || 13315_New_Thumb_searchweb.png (320x180) [100.3 KB] || 13315_New_Thumb_thm.png (80x40) [7.6 KB] || TWITTER_720_13315_Apollo_Sample_MASTER_twitter_720.mp4 (1280x720) [22.0 MB] || 13315_Apollo_Sample_MASTER.webm (960x540) [34.5 MB] || FACEBOOK_720_13315_Apollo_Sample_MASTER_facebook_720.mp4 (1280x720) [128.2 MB] || 13315_Apollo_Sample_MASTER_Output.en_US.srt [44 bytes] || 13315_Apollo_Sample_MASTER_Output.en_US.vtt [57 bytes] || YOUTUBE_4K_13315_Apollo_Sample_MASTER_youtube_4k.mp4 (3840x2160) [717.7 MB] || 13315_Apollo_Sample_MASTER.mov (3840x2160) [7.4 GB] || ",
            "hits": 117
        },
        {
            "id": 13275,
            "url": "https://svs.gsfc.nasa.gov/13275/",
            "result_type": "Produced Video",
            "release_date": "2019-08-07T11:30:00-04:00",
            "title": "How NASA Will Protect Astronauts From Space Radiation",
            "description": "Today, the Apollo-era flares serve as a reminder of the threat of radiation exposure for technology and astronauts in space. Understanding and predicting solar eruptions is crucial for safe space exploration. Almost 50 years since those 1972 storms, the data, technology and resources available to NASA have improved, enabling advancements towards space weather forecasts and astronaut protection — key to NASA’s Artemis program to return astronauts to the Moon.",
            "hits": 549
        },
        {
            "id": 13221,
            "url": "https://svs.gsfc.nasa.gov/13221/",
            "result_type": "Produced Video",
            "release_date": "2019-06-10T10:00:00-04:00",
            "title": "NASA Tech on SpaceX Falcon Heavy Launch - Media Telecon Resources",
            "description": "NASA is sending four technology missions that will help improve future spacecraft design and performance into space on the next SpaceX Falcon Heavy rocket launch. Experts will discuss these technologies, and how they complement NASA’s Moon to Mars exploration plans, during a media teleconference Monday, June 10 at 1 p.m. EDT.Audio of the teleconference will be streamed live online at: https://www.nasa.gov/liveParticipants in the briefing will be:Jim Reuter, acting associate administrator of NASA’s Space Technology Mission Directorate, will discuss how technology drives exploration to the Moon and beyond.Jill Seubert, deputy principal investigator for the Deep Space Atomic Clock at NASA’s Jet Propulsion Laboratory, will discuss how to advance exploration in deep space with a miniaturized, ultra-precise, mercury-ion atomic clock that is orders of magnitude more stable than today’s best navigation clocks.Don Cornwell, director of the Advanced Communications and Navigation Division of NASA’s Space Communications and Navigation program, will discuss how a more stable, space-based atomic clock could benefit future missions to the Moon and Mars.Christopher McLean, principal investigator for NASA’s Green Propellant Infusion Mission (GPIM) at Ball Aerospace, will discuss the demonstration of a green alternative to conventional chemical propulsion systems for next-generation launch vehicles and spacecraft. Joe Cassady, executive director for space at Aerojet Rocketdyne, will discuss the five thrusters and propulsion system aboard GPIM.Nicola Fox, director of the Heliophysics Division of NASA’s Science Mission Directorate, will discuss Space Environment Testbeds and the importance of protecting satellites from space radiation.Richard Doe, payload program manager for the Enhanced Tandem Beacon Experiment at SRI International, will discuss how a pair of NASA CubeSats will work with six satellites of the National Oceanographic and Atmospheric Administration’s (NOAA’s) COSMIC-2 mission to study disruptions of signals that pass through Earth’s upper atmosphere.To participate in the teleconference, media must contact Clare Skelly at 202-358-4273 or clare.a.skelly@nasa.gov by 10 a.m. June 10. Media questions may be submitted on Twitter during the teleconference using the hashtag #askNASA.NASA’s four missions will share a ride on the Falcon Heavy with about 20 satellites from government and research institutions that make up the Department of Defense’s Space Test Program-2 (STP-2) mission. SpaceX and the U.S. Air Force Space and Missile Systems Center, which manages STP-2, are targeting 11:30 p.m. Saturday, June 22, for launch from historic Launch Complex 39A at NASA’s Kennedy Space Center in Florida.Charged with returning astronauts to the Moon within five years, NASA’s Artemis lunar exploration plans are based on a two-phase approach: the first is focused on speed – landing astronauts on the Moon by 2024 – while the second will establish a sustained human presence on and around the Moon by 2028. We will use what we learn on the Moon to prepare to send astronauts to Mars. The technology missions on this launch will advance a variety of future exploration missions.For more information about NASA’s Moon to Mars exploration plans, visit:https://www.nasa.gov/moontomarsFor more information about the NASA technologies aboard this launch, visit:https://www.nasa.gov/spacexLearn more about NASA’s Deep Space Atomic Clock: https://www.nasa.gov/mission_pages/tdm/clock/index.htmlLearn more about NASA’s Green Propellant Infusion Mission: https://www.nasa.gov/mission_pages/tdm/green/index.htmlSPACE TEST PROGRAM-2 || ",
            "hits": 43
        },
        {
            "id": 13148,
            "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] || ",
            "hits": 153
        },
        {
            "id": 30944,
            "url": "https://svs.gsfc.nasa.gov/30944/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-07T10:00:00-04:00",
            "title": "Vision Across the Full Spectrum: The Crab Nebula, from Radio to X-ray",
            "description": "This animation shows the Crab Nebula from the lowest-frequency light (radio), to infrared, visible, ultraviolet, and finally X-ray. || STScI-H-CrabNebula_1x-1920x1080.00001_print.jpg (1024x576) [40.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_searchweb.png (320x180) [26.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_thm.png (80x40) [2.3 KB] || STScI-H-CrabNebula_1x-1280x720.mp4 (1280x720) [3.8 MB] || STScI-H-CrabNebula_1x-1920x1080.mp4 (1920x1080) [7.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-CrabNebula_1x-1920x1080.webm (1920x1080) [8.0 MB] || STScI-H-CrabNebula_1x-640x360.mp4 (640x360) [1.4 MB] || STScI-H-CrabNebula_1x-3840x2160.mp4 (3840x2160) [16.2 MB] || STScI-H-CrabNebula_1x-H265_3840x2160.mp4 (3840x2160) [3.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 373
        },
        {
            "id": 12709,
            "url": "https://svs.gsfc.nasa.gov/12709/",
            "result_type": "Produced Video",
            "release_date": "2017-09-12T10:00:00-04:00",
            "title": "Cassini's Infrared Saturn",
            "description": "Since arriving at Saturn in 2004, Cassini has used its Composite Infrared Spectrometer (CIRS) to study the ringed planet and its moons in heat radiation. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Particle Waves,\" \"Odyssey,\" \"Solaris,\" \"Expansive,\"\"Horizon Ahead,\" \"Ion Bridge,\" \"Outer Space\" || CassiniCIRSpreviewShort.jpg (1920x1080) [591.6 KB] || CassiniCIRSpreviewShort_searchweb.png (320x180) [125.9 KB] || CassiniCIRSpreviewShort_thm.png (80x40) [8.4 KB] || 12709_Cassini_CIRS_Short_TWTR.mp4 (1280x720) [102.0 MB] || WEBM-12709_Cassini_CIRS_Short_APR.webm (960x540) [191.9 MB] || 12709_Cassini_CIRS_Short_FB.mp4 (1280x720) [574.1 MB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.srt [10.3 KB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.vtt [10.3 KB] || 12709_Cassini_CIRS_Short_YT.mp4 (1920x1080) [1.2 GB] || 12709_Cassini_CIRS_Short_APR.mov (1920x1080) [6.0 GB] || 12709_Cassini_CIRS_Short_YT.hwshow [96 bytes] || ",
            "hits": 55
        },
        {
            "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": 83
        },
        {
            "id": 11964,
            "url": "https://svs.gsfc.nasa.gov/11964/",
            "result_type": "Produced Video",
            "release_date": "2015-07-29T10:00:00-04:00",
            "title": "How Sunlight Pushes Asteroids",
            "description": "Rotating asteroids have a tough time sticking to their orbits. Their surfaces heat up during the day and cool down at night, giving off radiation that can act as a sort of mini-thruster. This force, called the Yarkovsky effect, can cause rotating asteroids to drift widely over time, making it hard for scientists to predict their long-term risk to Earth. Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Yarkovsky_stylized_poster.png (1920x1080) [1.0 MB] || Yarkovsky_stylized_poster_print.jpg (1024x576) [105.7 KB] || Yarkovsky_stylized_poster_searchweb.png (320x180) [62.8 KB] || Yarkovsky_stylized_poster_thm.png (80x40) [8.4 KB] || YOUTUBE_HQ_G2015-063_Yarkovsky_Effect_MASTER_youtube_hq.mov (1280x720) [84.5 MB] || APPLE_TV_G2015-063_Yarkovsky_Effect_MASTER_appletv.m4v (1280x720) [72.0 MB] || WMV_G2015-063_Yarkovsky_Effect_MASTER_1280x720.wmv (1280x720) [47.7 MB] || WEBM_G2015-063_Yarkovsky_Effect_MASTER.webm (960x540) [42.2 MB] || APPLE_TV_G2015-063_Yarkovsky_Effect_MASTER_appletv_subtitles.m4v (1280x720) [72.1 MB] || NASA_PODCAST_G2015-063_Yarkovsky_Effect_MASTER_ipod_sm.mp4 (320x240) [27.5 MB] || G2015-063_Yarkovsky_Effect_MASTER_H264.en_US.srt [2.6 KB] || G2015-063_Yarkovsky_Effect_MASTER_H264.en_US.vtt [2.6 KB] || G2015-063_Yarkovsky_Effect_MASTER.mov (1920x1080) [1.9 GB] || G2015-063_Yarkovsky_Effect_MASTER_H264.mov (1920x1080) [369.3 MB] || NASA_TV_G2015-063_Yarkovsky_Effect_MASTER.mpeg (1280x720) [422.5 MB] || ",
            "hits": 164
        },
        {
            "id": 11070,
            "url": "https://svs.gsfc.nasa.gov/11070/",
            "result_type": "Produced Video",
            "release_date": "2012-08-15T10:00:00-04:00",
            "title": "The QWIP Detector; an Infrared Instrument",
            "description": "All objects emit infrared radiation and the characteristics of the infrared radiation are primarily dependent on the temperature of the object. One of the unique features of the new Quantum Well Infrared Photodetector (QWIP) instrument technology is the ability to, what engineers call \"band gap.\" This means it can spectrally respond to specific wavelengths. This video shows the evolution of taking this instrument from inception, to testing on the ground and from a plane, and ultimately to a NASA science mission. The applications are range from finding caves on Mars to loking for thermal polution in rivers or residual hot spots in forest fires, or monitoring food spoilage. || ",
            "hits": 40
        },
        {
            "id": 11005,
            "url": "https://svs.gsfc.nasa.gov/11005/",
            "result_type": "Produced Video",
            "release_date": "2012-06-25T00:00:00-04:00",
            "title": "Thermal Radiation and the Electromagnetic Spectrum",
            "description": "A short animation illustrating the relationship of temperature and wavelength.  Hotter objects have a shorter wavelength and cooler objects have a longer wavelength.  The animation also compares the wavelengths of visible light and thermal infrared radiation. || ",
            "hits": 283
        },
        {
            "id": 10937,
            "url": "https://svs.gsfc.nasa.gov/10937/",
            "result_type": "Produced Video",
            "release_date": "2012-03-16T15:00:00-04:00",
            "title": "RBSP Animation",
            "description": "Animations of the Radiation Belt Storm Probe spacecraft. || ",
            "hits": 79
        },
        {
            "id": 10651,
            "url": "https://svs.gsfc.nasa.gov/10651/",
            "result_type": "Produced Video",
            "release_date": "2010-09-17T00:00:00-04:00",
            "title": "Radiation Generated in Electric Fields Over Thunderstorms",
            "description": "The small satellite, with a big mission, is appropriately named \"Firefly.\" Sponsored by the National Science Foundation (NSF), the pint-sized satellite will study the most powerful natural particle accelerator on Earth - lightning - when it launches from the Marshall Islands aboard an Air Force Falcon 1E rocket vehicle next year. In particular, Firefly will focus on Terrestrial Gamma-ray Flashes (TGFs), a little understood phenomenon first discovered by NASA's Compton Gamma-Ray Observatory in the early 1990s.Although no one knows why, it appears these flashes of gamma rays that were once thought to occur only far out in space near black holes or other high-energy cosmic phenomena are somehow linked to lightning.fly's instruments, Goddard scientist Doug Rowland and his collaborators - Universities Space Research Association in Columbia, Md., Siena College, located near Albany, N.Y., and the Hawk Institute for Space Studies in Pocomoke City, Md. - hope to answer what causes these high-energy flashes. In particular, they want to find out if lightning triggers them or if they trigger lightning. Could they be responsible for some of the high-energy particles in the Van Allen radiation belts, which damage satellites? Firefly is expected to observe up to 50 lightning strokes per day, and about one large TGF every couple days. || ",
            "hits": 87
        },
        {
            "id": 10587,
            "url": "https://svs.gsfc.nasa.gov/10587/",
            "result_type": "Produced Video",
            "release_date": "2010-03-12T00:00:00-05:00",
            "title": "The Cosmic Ray Telescope for the Effects of Radiation",
            "description": "This animation shows how the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) instrument on LRO works.  It starts with a wide view of the LRO spacecraft with cosmic rays buzzing by around it then graduallly pushes in on the CRaTER instrument.  We see a cutaway of the instrument as a cosmic ray enters the telescope and passes through layers of tissue-equivalent plastics with sensors laid in between. || CRaTER_Animation_ipodLG.00002_print.jpg (1024x576) [94.1 KB] || CRaTER_Animation_ipodLG_web.png (320x180) [135.5 KB] || CRaTER_Animation_ipodLG_thm.png (80x40) [13.6 KB] || CRaTER_Animation_YouTubeHQ.webmhd.webm (960x540) [3.1 MB] || CRaTER_Animation_YouTubeHQ.mov (1280x720) [11.1 MB] || CRaTER_Animation_prores.mov (1280x720) [326.3 MB] || 1280x720_16x9_60p (1280x720) [128.0 KB] || CRaTER_Animation_ipodLG.m4v (640x360) [3.4 MB] || CRaTER_Animation__PORTAL.wmv (346x260) [3.0 MB] || CRaTER_Animation_ipodSM.m4v (320x180) [1.4 MB] || CRaTER_Animation_SVS.mpg (512x288) [2.9 MB] || ",
            "hits": 44
        },
        {
            "id": 10438,
            "url": "https://svs.gsfc.nasa.gov/10438/",
            "result_type": "Produced Video",
            "release_date": "2009-05-21T00:00:00-04:00",
            "title": "LRO: Mapping Our Future",
            "description": "The Lunar Reconnaissance Orbiter (LRO) is the first mission in NASA's planned return to the moon. LRO is an unmanned mission to create the comprehensive atlas of the moon's features and resources necessary to design all future lunar exploration efforts. LRO focuses on the selection of safe landing sites, identification of lunar resources and the study of how lunar radiation will affect humans.For complete transcript, click here. || LRO_MappingOurFuture_ipod.00905_print.jpg (1024x576) [30.4 KB] || LRO_MappingOurFuture_ipod_web.png (320x180) [33.3 KB] || LRO_MappingOurFuture_ipod_thm.png (80x40) [3.6 KB] || LRO_MappingOurFuture_AppleTV.webmhd.webm (960x540) [84.8 MB] || LRO_MappingOurFuture_YouTube.mov (1280x720) [100.5 MB] || LRO_MappingOurFuture_fullres.mov (1280x720) [192.6 MB] || LRO_MappingOurFuture_AppleTV.m4v (960x540) [210.6 MB] || LRO_MappingOurFuture_ipod.m4v (640x360) [67.2 MB] || GSFC_20090521_LRO_m10438_Mapping1a.en_US.srt [7.5 KB] || GSFC_20090521_LRO_m10438_Mapping1a.en_US.vtt [7.5 KB] || LRO_MappingOurFuture_320x240.mp4 (320x240) [16.6 MB] || LRO_MappingOurFuture_portal.wmv (346x260) [48.7 MB] || LRO_MappingOurFuture_svs.mpg (512x288) [54.2 MB] || ",
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        {
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            "url": "https://svs.gsfc.nasa.gov/10415/",
            "result_type": "Produced Video",
            "release_date": "2009-04-16T12:00:00-04:00",
            "title": "LRO's CRaTER: Man, On The Moon",
            "description": "Harlan Spence, Principal Investigator for LRO's CRaTER instrument, explains how the mission will prepare the way for long-term human presence in space.For complete transcript, click here. || LRO_BUvideo_CRaTER_ipod.03065_print.jpg (1024x768) [108.8 KB] || LRO_BUvideo_CRaTER_ipod_web.png (320x240) [280.0 KB] || LRO_BUvideo_CRaTER_ipod_thm.png (80x40) [16.9 KB] || LRO_BUvideo_CRaTER_ipod_searchweb.png (320x180) [79.2 KB] || LRO_BUvideo_CRaTER_dv1.webmhd.webm (960x540) [37.6 MB] || LRO_BUvideo_CRaTER_ipod.m4v (640x480) [29.2 MB] || LRO_BUvideo_CRaTER_dv1.mov (720x480) [548.3 MB] || LRO_BUvideo_CRaTER_nasacast.mp4 (320x240) [28.8 MB] || LRO_BUvideo_CRaTER_windows.wmv (346x260) [21.1 MB] || LRO_BUvideo_CRaTER_svs.mpg (512x384) [65.0 MB] || ",
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        {
            "id": 2980,
            "url": "https://svs.gsfc.nasa.gov/2980/",
            "result_type": "Visualization",
            "release_date": "2004-09-03T12:00:00-04:00",
            "title": "Ground Level UV Exposure",
            "description": "A large ozone hole means more ultraviolet exposure. TOMS tracks solar ultraviolet (UV-B radiation) measured at 290-320 nanometer wavelengths. Loss of stratospheric ozone has been linked to skin cancer in humans. Increased UV-B exposures for Southern continents can seriously impact phytoplankton and other species. Red is for high UV exposure and blue is for low UV exposure. || ",
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        {
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            "url": "https://svs.gsfc.nasa.gov/2316/",
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            "release_date": "2001-12-20T12:00:00-05:00",
            "title": "Fraction of Photosynthetically Active Radiation for Africa September, 2000, through May, 2001",
            "description": "MODIS' observations also allow scientists to track two 'vital signs' of Earth's vegetation. At Boston University, a team of researchers is using MODIS data to create global estimates of the green leaf area of Earth's vegetation and how much sunlight the leaves are absorbing. Called LAI, for 'Leaf Area Index,' and FPAR, for 'Fraction of absorbed Photosynthetically Active Radiation,' both pieces of information are necessary for understanding how sunlight interacts with the Earth's vegetated surfaces-from the top layer, called the canopy, through the understory vegetation, and down to the ground. || ",
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}