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    "results": [
        {
            "id": 14401,
            "url": "https://svs.gsfc.nasa.gov/14401/",
            "result_type": "Produced Video",
            "release_date": "2023-10-31T10:00:00-04:00",
            "title": "NASA’s Eclipse Art",
            "description": "“The greatest scientists are artists as well.” ~Albert EinsteinArt and science have been treated as separate disciplines but have more in common than is often realized. Creativity is critical to making scientific breakthroughs, and art is often an expression (or product) of scientific knowledge. And both art and science begin in the experience of awe, of beholding something grand. The experience of a solar eclipse is a prime example of where these two human endeavors meet.Eclipses are celestial events we can predict with extreme precision, and their occurrence reveals fundamental truths about our place in the universe. Yet, as many eclipse watchers will attest, there is no anticipating how you will feel when experiencing one. The emotional resonance of eclipses is underlined by their presence in artforms in cultures across the world going back millennia.To celebrate the special role of eclipses in connecting art and science, creatives across NASA will be sharing their eclipse-inspired artwork in anticipation of two solar eclipses that will cross the United States on October 14, 2023, and April 8, 2024.The first two pieces in the series are presented below, with short biographies of their creators. || ",
            "hits": 104
        },
        {
            "id": 5141,
            "url": "https://svs.gsfc.nasa.gov/5141/",
            "result_type": "Visualization",
            "release_date": "2023-09-22T00:00:00-04:00",
            "title": "Sea Surface Salinity Near The Maritime Continent",
            "description": "This animation of sea surface salinity shows the flow of freshwater from the Pacific into the Indian Ocean. The flow of freshwater (low salinity, blue color in 30-32 range) through narrow gaps of the maritime continent is known as Indonesian Throughflow. || sss.2020110117_print.jpg (1024x576) [172.0 KB] || sss.2020110117.png (5760x3240) [3.0 MB] || sss.2020110117_searchweb.png (320x180) [94.3 KB] || sss.2020110117_thm.png (80x40) [8.5 KB] || fixed_sss_1080p60_h265.mp4 (1920x1080) [88.2 MB] || 5760x3240_16x9_30p (5760x3240) [1.0 MB] || 3840x2160_16x9_30p (3840x2160) [1.0 MB] || fixed_sss_2160p60.mp4 (3840x2160) [482.0 MB] || ",
            "hits": 651
        },
        {
            "id": 4948,
            "url": "https://svs.gsfc.nasa.gov/4948/",
            "result_type": "Visualization",
            "release_date": "2023-09-13T10:00:00-04:00",
            "title": "Reforestation in Kigoma region of Tanzania: 2005 - 2014",
            "description": "This visualization begins by showing the location of the village of Kigalye, south of the Gombe National Park in Tanzania.  The topography of that region is draped with a satellite image taken on May 14, 2005.  As we fly up the valley between Kigalye and the park, scars from deforestation cover much of the landscape. || habitat_reforestation_4k_60fps_2005.1000_print.jpg (1024x576) [290.7 KB] || habitat_reforestation_4k_30fps_2005_1080p30.webmhd.webm (1080x606) [10.0 MB] || habitat_reforestation_4k_30fps_2005_1080p30.mp4 (1920x1080) [49.6 MB] || habitat_reforestation_4k_60fps_2005_1080p60.mp4 (1920x1080) [52.8 MB] || Yr_2005 (3840x2160) [0 Item(s)] || Yr_2005 (3840x2160) [0 Item(s)] || habitat_reforestation_2005_2160p30.mp4 (3840x2160) [151.6 MB] || habitat_reforestation_2005_2160p60.mp4 (3840x2160) [152.5 MB] || ",
            "hits": 55
        },
        {
            "id": 14387,
            "url": "https://svs.gsfc.nasa.gov/14387/",
            "result_type": "Produced Video",
            "release_date": "2023-09-12T06:00:00-04:00",
            "title": "Worth the wait! NASA’s First Ever Sample From An Asteroid Just Days Away From Returning to Earth Live Shots",
            "description": "Live coverage will begin at 10 a.m. EDT on Sept. 24 and air on NASA Television and the agency’s website, as well as YouTube, X, Facebook,  and NASA’s App.For more information click NASA Invites Public to Share Excitement of Asteroid Sample Return || OREX_landing_banner5.jpeg (1800x720) [300.4 KB] || OREX_landing_banner5_print.jpg (1024x409) [97.4 KB] || OREX_landing_banner5_searchweb.png (320x180) [87.8 KB] || OREX_landing_banner5_thm.png (80x40) [7.7 KB] || ",
            "hits": 27
        },
        {
            "id": 5145,
            "url": "https://svs.gsfc.nasa.gov/5145/",
            "result_type": "Visualization",
            "release_date": "2023-08-30T00:00:00-04:00",
            "title": "Franklin Re-intensifies over the Western Atlantic",
            "description": "Hurricane Franklin in the Atlantic on August 29, 2023 at 2:41Z || Franklin_001.4300_print.jpg (1024x576) [237.7 KB] || Franklin_001.4300_searchweb.png (320x180) [108.1 KB] || Franklin_001.4300_thm.png (80x40) [8.4 KB] || Franklin_001_1080p30_2.mp4 (1920x1080) [52.4 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Franklin_001_1080p30_2.webm (1920x1080) [5.7 MB] || Franklin_001_1080p30_2.mp4.hwshow [188 bytes] || ",
            "hits": 38
        },
        {
            "id": 14035,
            "url": "https://svs.gsfc.nasa.gov/14035/",
            "result_type": "Produced Video",
            "release_date": "2021-12-14T12:00:00-05:00",
            "title": "AGU 2021 - Major discoveries as NASA’s Parker Solar Probe closes in on the Sun",
            "description": "NASA’s Parker Solar Probe has now done what no spacecraft has done before—it has officially touched the Sun. Launched in 2018 to study the Sun’s biggest mysteries, the spacecraft has now grazed the edge of the solar atmosphere and gathered new close-up observations of our star. This is allowing us to see the Sun as never before—including the findings in two new papers, which were presented at AGU, that are helping scientists answer fundamental questions about the Sun.PANELISTSDr. Nicola Fox• Heliophysics Division Director of the Science Mission Directorate at NASA HeadquartersDr. Nour Raouafi• Project Scientist for NASA’s Parker Solar Probe• The Johns Hopkins Applied Physics Laboratory Dr. Justin Kasper• Principal Investigator for Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Parker Solar Probe  • BWX Technologies, Inc., University of MichiganProf. Stuart D. Bale• Principal Investigator for Fields Experiment (FIELDS) on Parker Solar Probe  • University of California, Berkeley Dr. Kelly Korreck• Program Scientist at NASA Headquarters• Smithsonian Astrophysical Observatory || ",
            "hits": 200
        },
        {
            "id": 13907,
            "url": "https://svs.gsfc.nasa.gov/13907/",
            "result_type": "Produced Video",
            "release_date": "2021-08-12T10:00:00-04:00",
            "title": "Go Now! Landsat & the Calypso Caper",
            "description": "During the summer of 1975, Jacques Cousteau and his divers helped NASA determine if Landsat could measure the depth of shallow ocean waters. The story of this NASA-led satellite bathymetry experiment unfolds through the photography and expedition documents preserved by David Lychenheim, the expedition’s communications engineer. Research done during that expedition determined that in certain conditions Landsat could measure depths up to 22 meters (72 feet), which gave birth to the field of satellite-derived bathymetry. This new technology enabled charts in clear water areas around the world to be revised, helping boats and deep-drafted supertankers avoid running aground on hazardous shoals or seamounts.Music: “Science of Life,” “Moving In Thought,” and “The Right Move” by Andrew Michael Britton [PRS] & David Stephen Goldsmith [PRS], “Midsummer” by Uwe Buschkotter [GEMA], “The Grand Opening” by Laurent Dury [SACEM], “Drifting Satellite” by Théo Boulenger [SACEM], “Man and Machine” by Larry Groupe [BMI], “A Little Optimism 1” by Joel Goodman [ASCAP], “Easy Does It” by Alchemist [SIAE], “Variations” by Stephan Sechi [ASCAP], “Bright and Playful” by Oscar Lo Brutto [PRS]; via Universal Production MusicComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || 13907_Landsat_Cousteau_poster.png (1920x1080) [3.1 MB] || 13907_Landsat_Cousteau_poster_print.jpg (1024x576) [287.2 KB] || 13907_Landsat_Cousteau_poster_searchweb.png (320x180) [114.6 KB] || 13907_Landsat_Cousteau_poster_thm.png (80x40) [8.1 KB] || 13907_Landsat_Cousteau-pr.mov (1920x1080) [7.2 GB] || 13907_Landsat_Cousteau-yt.mp4 (1920x1080) [938.3 MB] || 13907_Landsat_Cousteau-tw.mp4 (1280x720) [301.1 MB] || 13907_Landsat_Cousteau-tw.webm (1280x720) [59.6 MB] || 13907_Landsat_Cousteau-captions.en_US.srt [11.3 KB] || 13907_Landsat_Cousteau-captions.en_US.vtt [10.8 KB] || ",
            "hits": 49
        },
        {
            "id": 13654,
            "url": "https://svs.gsfc.nasa.gov/13654/",
            "result_type": "Produced Video",
            "release_date": "2020-07-01T10:00:00-04:00",
            "title": "NASA Prepares to Explore the Moon: Spacesuits and Tools",
            "description": "Kelsey Young (GSFC) and Trevor Graff (JSC) talk about the geology training astronauts receive before embarking on their mission back to the Lunar South Pole. They discuss new tools being developed for the Artemis Mission and the importance of going back to the Moon to conduct science. Music credits: \"Saana\" and \"Seasons\" by Torsti Juhani Spoof from Universal Production Music. || 13654_thumb.jpg (1920x1080) [114.3 KB] || 13654_Artemis_Geology_MASTER.03841_searchweb.png (320x180) [69.9 KB] || 13654_Artemis_Geology_MASTER.03841_thm.png (80x40) [5.7 KB] || 13654_Artemis_Geology_MASTER.mp4 (1920x1080) [285.4 MB] || 13654_Artemis_Geology_MASTER.webm (960x540) [108.9 MB] || 13654_Artemis_Geology_MASTER_facebook_720.mp4 (1280x720) [311.7 MB] || 13654_Artemis_Geology_MASTER_twitter_720.mp4 (1280x720) [52.7 MB] || 13654_caption.en_US.srt [6.0 KB] || 13654_caption.en_US.vtt [5.8 KB] || ",
            "hits": 23
        },
        {
            "id": 12821,
            "url": "https://svs.gsfc.nasa.gov/12821/",
            "result_type": "Produced Video",
            "release_date": "2018-05-31T09:50:00-04:00",
            "title": "NASA Studies Hurricane Edouard in HS3 Mission (2014)",
            "description": "NASA's Global Hawk in 2014 traveled to the middle of the Atlantic and flew over Hurricane Edouard. Remote sensing nstruments on the plane measured temperature, relative humidity, wind speed, wind direction as well as other data. Along with measurements from the aircraft, NASA scientists also collected data from dropsondes that parachuted down through the hurricane.Complete transcript available.Music: Who Done It? by Robert Leslie Bennett [ASCAP]Watch this video on the NASA Goddard YouTube channel. || 12821_HS3_dropsondes_youtube_1080.00555_print.jpg (1024x576) [53.6 KB] || 12821_HS3_dropsondes_youtube_1080.00555_searchweb.png (320x180) [43.1 KB] || 12821_HS3_dropsondes_youtube_1080.00555_thm.png (80x40) [4.2 KB] || 12821_HS3_dropsondes_1920.mov (1920x1080) [2.7 GB] || 12821_HS3_dropsondes_1920_large.mp4 (1920x1080) [101.8 MB] || 12821_HS3_dropsondes_youtube_1080.mp4 (1920x1080) [152.1 MB] || 12821_HS3_dropsondes_facebook_720.mp4 (1280x720) [112.6 MB] || 12821_HS3_dropsondes.webm (960x540) [40.3 MB] || 12821_HS3_dropsondes_UHD.mov (3840x2160) [11.0 GB] || 12821_HS3_dropsondes_youtube_4k.mp4 (3840x2160) [377.0 MB] || 12821_HS3_dropsondes-captions.en_US.srt [2.1 KB] || 12821_HS3_dropsondes-captions.en_US.vtt [2.1 KB] || ",
            "hits": 19
        },
        {
            "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": 157
        },
        {
            "id": 12704,
            "url": "https://svs.gsfc.nasa.gov/12704/",
            "result_type": "Produced Video",
            "release_date": "2017-08-31T12:00:00-04:00",
            "title": "NASA Eclipse Imagery",
            "description": "As millions of people across the United States experienced a total eclipse as the umbra, or Moon’s shadow passed over them, only six people witnessed the umbra from space. Viewing the eclipse from orbit were NASA’s Randy Bresnik, Jack Fischer and Peggy Whitson, ESA (European Space Agency’s) Paolo Nespoli, and Roscosmos’ Commander Fyodor Yurchikhin and Sergey Ryazanskiy. The space station crossed the path of the eclipse three times as it orbited above the continental United States at an altitude of 250 miles. Credit: NASA || iss052e056122.jpg (4928x3280) [844.0 KB] || ",
            "hits": 232
        },
        {
            "id": 30893,
            "url": "https://svs.gsfc.nasa.gov/30893/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-08-31T00:00:00-04:00",
            "title": "2017 Eclipse Image Collection",
            "description": "This image is a composite photograph that shows the progression of the total solar eclipse over Madras, Oregon.http://earthobservatory.nasa.gov/NaturalHazards/view.php?id=90796 || eclipsecomposite_pho_lrg.jpg (2231x1487) [541.4 KB] || eclipsecomposite_pho_lrg_searchweb.png (320x180) [47.2 KB] || eclipsecomposite_pho_lrg_thm.png (80x40) [3.3 KB] || 2017-eclipse-images-7.hwshow [293 bytes] || ",
            "hits": 105
        },
        {
            "id": 4496,
            "url": "https://svs.gsfc.nasa.gov/4496/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 171 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI171A_UHD3840.02000_print.jpg (1024x576) [69.0 KB] || 2007stereo_RedCyan_010_EUVI171A_2160p30.mp4 (3840x2160) [451.0 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI171A_2160p30.webm (3840x2160) [13.7 MB] || ",
            "hits": 18
        },
        {
            "id": 4500,
            "url": "https://svs.gsfc.nasa.gov/4500/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 195 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI195A_UHD3840.02000_print.jpg (1024x576) [51.7 KB] || 2007stereo_RedCyan_010_EUVI195A_2160p30.mp4 (3840x2160) [287.8 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI195A_2160p30.webm (3840x2160) [12.6 MB] || ",
            "hits": 20
        },
        {
            "id": 4501,
            "url": "https://svs.gsfc.nasa.gov/4501/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 284 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI284A_UHD3840.02000_print.jpg (1024x576) [59.2 KB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI284A_2160p30.mp4 (3840x2160) [506.4 MB] || 2007stereo_RedCyan_010_EUVI284A_2160p30.webm (3840x2160) [12.7 MB] || ",
            "hits": 21
        },
        {
            "id": 4502,
            "url": "https://svs.gsfc.nasa.gov/4502/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 304 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI304A_UHD3840.02000_print.jpg (1024x576) [80.1 KB] || 2007stereo_RedCyan_010_EUVI304A_2160p30.mp4 (3840x2160) [710.3 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI304A_2160p30.webm (3840x2160) [15.7 MB] || ",
            "hits": 20
        },
        {
            "id": 30771,
            "url": "https://svs.gsfc.nasa.gov/30771/",
            "result_type": "Hyperwall Visual",
            "release_date": "2016-04-29T00:00:00-04:00",
            "title": "4K Video from the ISS, April 2016",
            "description": "ISS crew Earth observations, || earth_obs_00720_print.jpg (1024x576) [164.4 KB] || earth_obs_00720.png (3840x2160) [31.7 MB] || earth_obs_00720_searchweb.png (320x180) [85.1 KB] || earth_obs_00720_thm.png (80x40) [6.3 KB] || ISS_Crew_Earth_Observations_720p.mp4 (1280x720) [19.7 MB] || ISS_Crew_Earth_Observations_720p.webm (1280x720) [7.5 MB] || ISS_Crew_Earth_Observations_2160p.mp4 (3840x2160) [80.1 MB] || ",
            "hits": 765
        },
        {
            "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": 100
        },
        {
            "id": 40271,
            "url": "https://svs.gsfc.nasa.gov/gallery/live-shots-gallery/",
            "result_type": "Gallery",
            "release_date": "2015-11-27T00:00:00-05:00",
            "title": "Live Shots Gallery Collection",
            "description": "Collection of live shot pages of b-roll and interviews!",
            "hits": 172
        },
        {
            "id": 4378,
            "url": "https://svs.gsfc.nasa.gov/4378/",
            "result_type": "Visualization",
            "release_date": "2015-10-02T17:00:00-04:00",
            "title": "Visualizations: A NASA Eye View of Our Earth",
            "description": "This gallery was created for Earth Science Week 2015 and beyond. It includes a quick start guide for educators and first-hand stories (blogs) for learners of all ages by NASA visualizers, scientists and educators. We hope that your understanding and use of NASA's visualizations will only increase as your appreciation grows for the beauty of the science they portray, and the communicative power they hold. Read all the blogs and find educational resources for all ages at: the Earth Science Week 2015 page.Nearly every time I give a talk at the Hyperwall — a genius NASA creation which combines 9 to 15 high definition screens together to show amazing visualizations, pictures, movies and more — I always like to start with the GEOS-5 model of aerosols. This visualization shows how different types of aerosols (black and organic carbon, sea salt, dust, and sulfates) move around our planet. From this mesmerizing movie, you can see where dust storms originate from the Sahara, where fires in the Amazon are spewing black carbon into the atmosphere and how sea salt is spiraling around the southern oceans in huge bands.The funny thing is that this visualization has very little to do with my own research... I just think it is really cool and most people agree with me! By getting them engaged through this visualization, they quickly see how our Earth system is interconnected and how a dust storm over China could actually impact them in their own backyards in the U.S.As a scientist, I always get excited when someone asks me about my work with the Global Precipitation Measurement (GPM) mission. Usually when I start describing how the GPM Core satellite measures rainfall and why it's important, I do a lot of hand waving. Sometimes I try to describe what we can do with satellites with a metaphor or two. Those are all helpful in painting a picture. But what really seems to make the point is when I pull up a particular visualization of a dozen or so different satellites all taking precipitation measurements over the globe within the same 3-hour window. With a short movie you can see how we can get a global picture of rain and snow everywhere around the world within a few hours! || ",
            "hits": 44
        },
        {
            "id": 11899,
            "url": "https://svs.gsfc.nasa.gov/11899/",
            "result_type": "Produced Video",
            "release_date": "2015-07-21T13:00:00-04:00",
            "title": "Scientists Link Earlier Melting Of Snow To Dark Aerosols",
            "description": "Tiny particles suspended in the air, known as aerosols, can darken snow and ice causing it to absorb more of the sun’s energy. But until recently, scientists rarely considered the effect of all three major types of light-absorbing aerosols together in climate models.In a new study, NASA scientists used a climate model to examine the impact of this snow-darkening phenomenon on Northern Hemisphere snowpacks, including how it affects snow amount and heating on the ground in spring.The study looked at three types of light-absorbing aerosols – dust, black carbon and organic carbon. Black carbon and organic carbon are produced from the burning of fossil fuels, like coal and oil, as well as biofuels and biomass, such as forests.With their snow darkening effect added to NASA’s GEOS-5 climate model, scientists analyzed results from 2002 to 2011, and compared them to model runs done without the aerosols on snow. They found that the aerosols indeed played a role in absorbing more of the sun’s energy. Over broad places in the Northern Hemisphere, the darkened snow caused some surface temperatures to be up to 10 degrees Fahrenheit warmer than it would be if the snow were pristine. As a result, warmer, snow-darkened areas had less snow in spring than they would have had under pristine snow conditions.According to the study, dust’s snow darkening effect significantly contributed to surface warming in Central Asia and the western Himalayas. Black carbon’s snow darkening effect had a larger impact primarily in Europe, the eastern Himalayas and East Asia. It had a smaller impact in North America. Organic carbon’s snow darkening effect was relatively lower but present in regions such as southeastern Siberia, northeastern East Asia and western Canada.“As we add more of these aerosols to the mix, we are potentially increasing our overall impact on Earth’s climate,” said research scientist Teppei Yasunari at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.Research: Impact of snow darkening via dust, black carbon, and organic carbon on boreal spring climate in the Earth systemJournal: Geophysical Research: Atmospheres, June 15, 2015.Link to paper: http://onlinelibrary.wiley.com/doi/10.1002/2014JD022977/fullHere is the YouTube video. || ",
            "hits": 239
        },
        {
            "id": 11900,
            "url": "https://svs.gsfc.nasa.gov/11900/",
            "result_type": "Produced Video",
            "release_date": "2015-07-21T13:00:00-04:00",
            "title": "Instagram: Scientists Link Earlier Melting Of Snow To Dark Aerosols",
            "description": "Tiny particles suspended in the air, known as aerosols, can darken snow and ice causing it to absorb more of the sun’s energy. But until recently, scientists rarely considered the effect of all three major types of light-absorbing aerosols together in climate models.In a new study, NASA scientists used a climate model to examine the impact of this snow-darkening phenomenon on Northern Hemisphere snowpacks, including how it affects snow amount and heating on the ground in spring.The study looked at three types of light-absorbing aerosols – dust, black carbon and organic carbon. Black carbon and organic carbon are produced from the burning of fossil fuels, like coal and oil, as well as biofuels and biomass, such as forests.With their snow darkening effect added to NASA’s GEOS-5 climate model, scientists analyzed results from 2002 to 2011, and compared them to model runs done without the aerosols on snow. They found that the aerosols indeed played a role in absorbing more of the sun’s energy. Over broad places in the Northern Hemisphere, the darkened snow caused some surface temperatures to be up to 10 degrees Fahrenheit warmer than it would be if the snow were pristine. As a result, warmer, snow-darkened areas had less snow in spring than they would have had under pristine snow conditions.According to the study, dust’s snow darkening effect significantly contributed to surface warming in Central Asia and the western Himalayas. Black carbon’s snow darkening effect had a larger impact primarily in Europe, the eastern Himalayas and East Asia. It had a smaller impact in North America. Organic carbon’s snow darkening effect was relatively lower but present in regions such as southeastern Siberia, northeastern East Asia and western Canada.“As we add more of these aerosols to the mix, we are potentially increasing our overall impact on Earth’s climate,” said research scientist Teppei Yasunari at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.Research: Impact of snow darkening via dust, black carbon, and organic carbon on boreal spring climate in the Earth systemJournal: Geophysical Research: Atmospheres, June 15, 2015.Link to paper: http://onlinelibrary.wiley.com/doi/10.1002/2014JD022977/fullHere is the YouTube video. || ",
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        },
        {
            "id": 40415,
            "url": "https://svs.gsfc.nasa.gov/gallery/whats-newwith-earth-today/",
            "result_type": "Gallery",
            "release_date": "2015-01-04T00:00:00-05:00",
            "title": "What's New with Earth Today",
            "description": "Explore the latest visualizations of NASA's Earth Observing satellites and the data they collect.  NASA researchers are constantly tracking remote-sensing data and modeling processes to better understand our home planet.",
            "hits": 145
        },
        {
            "id": 11557,
            "url": "https://svs.gsfc.nasa.gov/11557/",
            "result_type": "Produced Video",
            "release_date": "2014-05-30T18:00:00-04:00",
            "title": "NASA Administrator Bolden visits ATK Space Systems Division",
            "description": "NASA Administrator Charles Bolden and Goddard Space Flight Center Director Christopher Scolese got a first hand look at work being done at ATK Space Systems Division in Beltsville, Maryland during a visit on May 28, 2014. Their tour included a visit to ATK’s Robotic Rendezvous and Proximity Operations (RPO) Lab where they saw a demonstration of how robotic technology may be used to extend the life of satellites. Bolden and Scolese also had an opportunity to see space tools used by astronauts during service calls to the Hubble Space Telescope as well as hear about new tools being developed for astronauts on the International Space Station. Interviews:1. Chris Scolese / Goddard Center Director       2. Tom Wilson / ATK General Manager        3. Charles Bolden / NASA Administrator                                       4. Charles Bolden / NASA Administrator || ",
            "hits": 13
        },
        {
            "id": 11071,
            "url": "https://svs.gsfc.nasa.gov/11071/",
            "result_type": "Produced Video",
            "release_date": "2013-01-23T11:30:00-05:00",
            "title": "SDO Wavelength Graphics",
            "description": "Specialized instruments, either in ground-based or space-based telescopes, can observe light far beyond the ranges visible to the naked eye. Different wavelengths convey information about different components of the sun's surface and atmosphere, so scientists use them to paint a full picture of our constantly changing and varying star.Yellow light of 5800 angstroms, for example, generally emanates from material of about 10,000 degrees F (5700 degrees C), which represents the surface of the sun. Extreme ultraviolet light of 94 angstroms, on the other hand, comes from atoms that are about 11 million degrees F (6,300,000 degrees C) and is a good wavelength for looking at solar flares, which can reach such high temperatures. By examining pictures of the sun in a variety of wavelengths — as is done through such telescopes as NASA's Solar Dynamics Observatory (SDO), NASA's Solar Terrestrial Relations Observatory (STEREO) and the ESA/NASA Solar and Heliospheric Observatory (SOHO) — scientists can track how particles and heat move through the sun's atmosphere.We see the visible spectrum of light simply because the sun is made up of a hot gas — heat produces light just as it does in an incandescent light bulb. But when it comes to the shorter wavelengths, the sun sends out extreme ultraviolet light and x-rays because it is filled with many kinds of atoms, each of which give off light of a certain wavelength when they reach a certain temperature. Not only does the sun contain many different atoms — helium, hydrogen, iron, for example — but also different kinds of each atom with different electrical charges, known as ions. Each ion can emit light at specific wavelengths when it reaches a particular temperature. Scientists have cataloged which atoms produce which wavelengths since the early 1900s, and the associations are well documented in lists that can take up hundreds of pages.Instruments that produce conventional images of the sun focus exclusively on light around one particular wavelength, sometimes not one that is visible to the naked eye. SDO scientists, for example, chose 10 different wavelengths to observe for its Atmospheric Imaging Assembly (AIA) instrument. Each wavelength is largely based on a single, or perhaps two types of ions — though slightly longer and shorter wavelengths produced by other ions are also invariably part of the picture. Each wavelength was chosen to highlight a particular part of the sun's atmosphere.From the sun's surface on out, the wavelengths SDO observes, measured in angstroms, are: 4500: Showing the sun's surface or photosphere. 1700: Shows surface of the sun, as well as a layer of the sun's atmosphere called the chromosphere, which lies just above the photosphere and is where the temperature begins rising. 1600: Shows a mixture between the upper photosphere and what's called the transition region, a region between the chromosphere and the upper most layer of the sun's atmosphere called the corona. The transition region is where the temperature rapidly rises. 304: This light is emitted from the chromosphere and transition region. 171: This wavelength shows the sun's atmosphere, or corona, when it's quiet. It also shows giant magnetic arcs known as coronal loops. 193: Shows a slightly hotter region of the corona, and also the much hotter material of a solar flare. 211: This wavelength shows hotter, magnetically active regions in the sun's corona. 335: This wavelength also shows hotter, magnetically active regions in the corona. 94: This highlights regions of the corona during a solar flare. 131: The hottest material in a flare. || ",
            "hits": 642
        },
        {
            "id": 10742,
            "url": "https://svs.gsfc.nasa.gov/10742/",
            "result_type": "Produced Video",
            "release_date": "2011-08-25T12:00:00-04:00",
            "title": "NPP Resource Reel",
            "description": "The NPOESS Preparatory Project (NPP) represents a critical first step in building the next-generation weather satellite system. Goddard Space Flight Center is leading NASA's effort to launch a satellite that will carry the first of the new sensors developed for this next-generation system, previously called the National Polar-orbiting Operational Environmental Satellite System (NPOESS) and now the Joint Polar Satellite System (JPSS). || ",
            "hits": 28
        },
        {
            "id": 10321,
            "url": "https://svs.gsfc.nasa.gov/10321/",
            "result_type": "Produced Video",
            "release_date": "2008-08-01T00:00:00-04:00",
            "title": "HST SM4 Resource Reel v2.0",
            "description": "1. Hubble Space Telescope Service Mission 4 Animation: A collection of several animations showing the Hubble Space Telescope orbiting Earth and in space shuttle Atlantis cargo bay. All animations depict the Hubble Space Telescope in its current (July 2008) configuration. || 1-resource-hstsm4animation-resourcereelreference_MPEG-100852_print.jpg (1024x768) [98.4 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_web.png (320x240) [107.6 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_thm.png (80x40) [16.4 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1_searchweb.png (320x180) [85.3 KB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1.webmhd.webm (960x540) [12.8 MB] || 1-resource-hstsm4animation-resourcereelreference_MPEG-1.mpg (320x240) [63.5 MB] || ",
            "hits": 35
        },
        {
            "id": 10318,
            "url": "https://svs.gsfc.nasa.gov/10318/",
            "result_type": "Produced Video",
            "release_date": "2008-07-26T00:00:00-04:00",
            "title": "HST SM4 Extended Resource Reel v2.0",
            "description": "Full HD Resource ReelThis resource reel includes all the clips shown below on this page. || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.00001_print.jpg (1024x576) [99.1 KB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1.mov (1280x720) [57.2 GB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.mp4 (1280x720) [4.1 GB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1_1.webm (1280x720) [454.7 MB] || G2008-009HD-HST_SM4_Footage_Resource_Reel_v2.0_Reel_1.webm [0 bytes] || ",
            "hits": 47
        },
        {
            "id": 10237,
            "url": "https://svs.gsfc.nasa.gov/10237/",
            "result_type": "Produced Video",
            "release_date": "2008-05-20T00:00:00-04:00",
            "title": "HST SM4 — Astronauts Close HST Doors for Last Time",
            "description": "Animation showing the Hubble Servicing Mission Servicing Mission 4 crew closing Hubble's aft doors for the last time. Astronaut gives camera 'thumbs-up' sign. || ",
            "hits": 22
        },
        {
            "id": 40116,
            "url": "https://svs.gsfc.nasa.gov/gallery/jwst/",
            "result_type": "Gallery",
            "release_date": "2000-01-01T00:00:00-05:00",
            "title": "James Webb Space Telescope",
            "description": "The James Webb Space Telescope (sometimes called JWST) is a large, infrared-optimized space telescope. The observatory launched into space on an Ariane 5 rocket from the Guiana Space Centre in Kourou, French Guiana on December 25, 2021.  After launch, the observatory was successfully unfolded and is being readied for science. \n\nWebb will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy. Webb will peer through dusty clouds to see stars forming planetary systems, connecting the Milky Way to our own Solar System. Webb's instruments are designed to work primarily in the infrared range of the electromagnetic spectrum, with some capability in the visible range.\n\nWebb has a large primary mirror, 6.5 meters (21.3 feet) in diameter and a sunshield the size of a tennis court. Both the mirror and sunshade are too large to fit onto the Ariane 5 rocket fully open, so both were folded which meant they needed to be unfolded in space. \n\nWebb is currently in its operational orbit about 1.5 million km (1 million miles) from the Earth at a location known as Lagrange Point 2 (L2).\n\nThe James Webb Space Telescope was named after the NASA Administrator who crafted the Apollo program, and who was a staunch supporter of space science.",
            "hits": 843
        }
    ]
}