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    "results": [
        {
            "id": 5572,
            "url": "https://svs.gsfc.nasa.gov/5572/",
            "result_type": "Visualization",
            "release_date": "2025-08-08T14:00:02-04:00",
            "title": "GEOS Aerosols",
            "description": "Aerosols are tiny solid or liquid particles that float in the atmosphere and can travel long distances, affecting air quality and visibility far from their sources. This visualization covers the period from August 1 to September 14, 2024, and is based on NASA's Goddard Earth Observing System (GEOS) model, which delivers realistic, high-resolution weather and aerosol data that enable customized environmental prediction and advances in AI research.",
            "hits": 539
        },
        {
            "id": 14786,
            "url": "https://svs.gsfc.nasa.gov/14786/",
            "result_type": "Animation",
            "release_date": "2025-02-20T00:00:00-05:00",
            "title": "Swift Spacecraft Animations: 2025",
            "description": "NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, orbits Earth as it studies the ever-changing universe. Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab || SWIFT_S1_v2_4k_60fps_proRes.00005_print.jpg (1024x576) [148.3 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_searchweb.png (320x180) [64.4 KB] || SWIFT_S1_v2_4k_60fps_proRes.00005_thm.png [4.4 KB] || Swift_S1_v2_4k60.mp4 (3840x2160) [25.6 MB] || SWIFT_S1_v2_4k_60fps_proRes.mov (3840x2160) [4.2 GB] || Swift_S1_v2_4k60.hwshow [423 bytes] || ",
            "hits": 359
        },
        {
            "id": 14714,
            "url": "https://svs.gsfc.nasa.gov/14714/",
            "result_type": "B-Roll",
            "release_date": "2024-11-06T10:00:00-05:00",
            "title": "CODEX Heads to the Space Station for Install",
            "description": "On Nov. 4, 2024, the Coronal Diagnostic Experiment (CODEX) launched to space aboard NASA’s SpaceX CRS-31 – a commercial resupply mission of an uncrewed Dragon spacecraft headed for the International Space Station. Liftoff occurred at 9:29 p.m. EST.CODEX is a solar coronagraph that will be installed on the Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun’s outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contributions from Italy’s National Institute for Astrophysics (INAF).To learn more about the experiment, visit: https://science.nasa.gov/mission/codex/ || ",
            "hits": 75
        },
        {
            "id": 14647,
            "url": "https://svs.gsfc.nasa.gov/14647/",
            "result_type": "B-Roll",
            "release_date": "2024-08-12T13:00:00-04:00",
            "title": "CODEX – Coronal Diagnostic Experiment",
            "description": "The Coronal Diagnostic Experiment (CODEX) is a solar coronagraph that will be installed on the International Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contribution from Italy's National Institute for Astrophysics (INAF).Learn more: https://science.nasa.gov/mission/codex/ || ",
            "hits": 55
        },
        {
            "id": 14407,
            "url": "https://svs.gsfc.nasa.gov/14407/",
            "result_type": "Produced Video",
            "release_date": "2023-09-14T11:00:00-04:00",
            "title": "NASA Summer 2023 Temperature Media Resources",
            "description": "The summer of 2023 was Earth’s hottest since global records began in 1880, according to an analysis by scientists at NASA’s Goddard Institute of Space Studies (GISS) in New York.The months of June, July, and August combined were 0.41 degrees Fahrenheit (0.23 degrees Celsius) warmer than any other summer in NASA’s record, and 2.1 degrees F (1.2 C) warmer than the average summer between 1951 and 1980. August alone was 2.2 F (1.2 C) warmer than the average. June through August is considered meteorological summer in the Northern Hemisphere. This new record comes as exceptional heat swept across much of the world, exacerbating deadly wildfires in Canada and Hawaii, and searing heat waves in South America, Japan, Europe, and the U.S., while likely contributing to severe rainfall in Italy, Greece, and Central Europe.NASA assembles its temperature record, known as GISTEMP, from surface air temperature data acquired by tens of thousands of meteorological stations, as well as sea surface temperature data from ship- and buoy-based instruments. This raw data is analyzed using methods that account for the varied spacing of temperature stations around the globe and for urban heating effects that could skew the calculations. || ",
            "hits": 175
        },
        {
            "id": 4959,
            "url": "https://svs.gsfc.nasa.gov/4959/",
            "result_type": "Visualization",
            "release_date": "2021-12-13T00:00:00-05:00",
            "title": "Reduction in Tropospheric NOx and Ozone Corresponding to Worldwide COVID-19 Lockdowns",
            "description": "When the world went into lockdown to slow the spread of COVID-19, air pollution emissions started to rapidly decrease leaving a global atmospheric fingerprint detected by a team of scientists at NASA’s Jet Propulsion Laboratory using satellite measurements. These traces provided an unexpected window into what low-emissions world could look like, thus providing a means for identifying effective environmental policies. While many countries in the last few decades have implemented environmental policies to reduce human health risk from air pollution by controlling emissions, the impacts of those policies have not always been clear. The global lockdowns in response to COVID-19 represent a well-observed “scenario-of-opportunity” that allows us to assess how atmospheric emission and composition responds to reduced human activity. COVID-19 lockdowns effectively showed how reducing NOx emissions affects the global atmosphere. Its identifying signature shows up as in the atmosphere’s altered ability to produce harmful ozone pollution and ozone’s reduced influence on Earth’s heat balance that affects climate. These effects are not uniform across the world and depend on the location and season of the emission reductions.The results of this research indicate that in order to design effective environmental policies which benefit both air quality and climate, decision-makers need to carefully consider the complex relationships between emissions and atmospheric composition. || ",
            "hits": 92
        },
        {
            "id": 13926,
            "url": "https://svs.gsfc.nasa.gov/13926/",
            "result_type": "Animation",
            "release_date": "2021-09-08T15:00:00-04:00",
            "title": "Swift Spacecraft Animation",
            "description": "NASA’s Neil Gehrels Swift Observatory, shown in this illustration, launched into Earth orbit in November 2004. The satellite investigates gamma-ray bursts, the most energetic explosions in the universe. Swift observes the sky in visible, ultraviolet, X-ray, and gamma-ray light. Its name reflects its ability to rapidly follow up on interesting objects in the sky. Swift also studies supernova explosions, star-shredding black holes in other galaxies, comets, stellar remnants called neutron stars, and other cosmic phenomena. In 2018, NASA renamed Swift in honor of the late Neil Gehrels, who helped develop the mission and served as its principal investigator for 13 years.Credit: NASA’s Goddard Space Flight Center/Chris Smith (KBRwyle) || swift_spacecraft_update_still.jpg (1920x1080) [769.2 KB] || swift_spacecraft_update_still_print.jpg (1024x576) [328.5 KB] || swift_spacecraft_update_still_searchweb.png (320x180) [94.8 KB] || swift_spacecraft_update_still_web.png (320x180) [94.8 KB] || swift_spacecraft_update_still_thm.png (80x40) [6.5 KB] || swift_spacecraft_update_HQ.mp4 (1920x1080) [47.7 MB] || swift_spacecraft_update_LQ.mp4 (1920x1080) [24.7 MB] || swift_spacecraft_update_HQ.webm (1920x1080) [2.2 MB] || swift_spacecraft_update_prores.mov (1920x1080) [255.2 MB] || 13926_swift_spacecraft_update_HQ.hwshow [72 bytes] || ",
            "hits": 236
        },
        {
            "id": 31116,
            "url": "https://svs.gsfc.nasa.gov/31116/",
            "result_type": "Hyperwall Visual",
            "release_date": "2020-02-12T00:00:00-05:00",
            "title": "Unpopulated Slopes of an Active Volcano—Naples, Italy",
            "description": "Unpopulated Slopes of an Active Volcano—Naples, ItalyAn astronaut onboard the ISS took this photograph of the city lights of Naples and the Campania region of southern Italy on January 30, 2017. The Naples region is one of the brightest in Italy. Roughly three million people live in and around this metropolitan area.The large black circular area in the photo is Mount Vesuvius, the only active volcano on Europe’s mainland. Although any volcanic activity can endanger surrounding communities, eruptive pyroclastic flows of superheated ash and gas are among the most dangerous, moving at speeds of hundreds of kilometers per hour. Vesuvius has erupted on numerous occasions throughout history. Probably the most famous of those eruptions occurred in 79 A.D., when pyroclastic flows destroyed the cities of Pompeii and Herculaneum, trapping more than 16,000 people. Such historic catastrophes—and the fact that 600,000 people currently live in the immediate vicinity—are why the volcano is one of the most heavily monitored in the world, with several dozen sensors located at many points on and around the cone.The different colors of lights in the scene reflect some of the history of development in the area. The green lights are mercury vapor bulbs, an older variety that has been replaced in newer developments by yellow-orange sodium bulbs. To the northeast, the lightless gaps between the homes and businesses are agricultural fields. The bright yellow-orange complex amidst the fields is the Consorzio Intercomunale dei Servizi, the largest commercial facility in Europe. || Unpop_Slopes_Active_Volcan_Naples_It_print.jpg (1024x540) [202.8 KB] || Unpop_Slopes_Active_Volcan_Naples_It.png (4096x2160) [15.3 MB] || Unpop_Slopes_Active_Volcan_Naples_It_searchweb.png (320x180) [109.9 KB] || Unpop_Slopes_Active_Volcan_Naples_It_thm.png (80x40) [6.6 KB] || unpopulated-slopes-of-an-active-volcanonaples-italy.hwshow [347 bytes] || ",
            "hits": 47
        },
        {
            "id": 12740,
            "url": "https://svs.gsfc.nasa.gov/12740/",
            "result_type": "Produced Video",
            "release_date": "2017-10-16T10:00:00-04:00",
            "title": "Doomed Neutron Stars Create Blast of Light and Gravitational Waves",
            "description": "This animation captures phenomena observed over the course of nine days following the neutron star merger known as GW170817, detected on Aug. 17, 2017. They include gravitational waves (pale arcs), a near-light-speed jet that produced gamma rays (magenta), expanding debris from a kilonova that produced ultraviolet (violet), optical and infrared (blue-white to red) emission, and, once the jet directed toward us expanded into our view from Earth, X-rays (blue). Credit: NASA's Goddard Space Flight Center/CI LabMusic: \"Exploding Skies\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Neutron_Star_Merger_Still_2_new_1080.png (1920x1080) [2.5 MB] || Neutron_Star_Merger_Still_2_new_1080.jpg (1920x1080) [167.3 KB] || Neutron_Star_Merger_Still_2_new_print.jpg (1024x576) [50.4 KB] || Neutron_Star_Merger_Still_2_new.png (3840x2160) [7.7 MB] || Neutron_Star_Merger_Still_2_new.jpg (3840x2160) [1.0 MB] || Neutron_Star_Merger_Still_2_new_thm.png (80x40) [4.4 KB] || Neutron_Star_Merger_Still_2_new_searchweb.png (320x180) [51.4 KB] || 12740_NS_Merger_Update_1080.m4v (1920x1080) [50.3 MB] || 12740_NS_Merger_Update_H264_1080.mp4 (1920x1080) [96.9 MB] || 12740_NS_Merger_Update_1080p.mov (1920x1080) [101.9 MB] || NS_Merger_SRT_Captions.en_US.srt [417 bytes] || NS_Merger_SRT_Captions.en_US.vtt [399 bytes] || 12740_NS_Merger_4k_Update.webm (3840x2160) [10.0 MB] || 12740_NS_Merger_4k_Update_H264.mp4 (3840x2160) [254.9 MB] || 12740_NS_Merger_4k_Update_H264.mov (3840x2160) [516.7 MB] || 12740_NS_Merger_4k_Update_ProRes_3840x2160_5994.mov (3840x2160) [5.1 GB] || 12740_NS_Merger_4k_Update_H264.hwshow [90 bytes] || ",
            "hits": 950
        },
        {
            "id": 30693,
            "url": "https://svs.gsfc.nasa.gov/30693/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-10-20T00:00:00-04:00",
            "title": "Southwestern Europe and Australia at Night 2014-2015",
            "description": "One way to study the spatial distribution, or arrangement, of human settlements is to view the planet from space during nighttime hours. Scientists have observed the Earth’s lights at night for more than four decades using military satellites and astronaut photography; however, the view became significantly clearer after using satellite data from a low-light sensor onboard the Suomi National Polar-orbiting Partnership (NPP) satellite, launched in October 2011. The satellite’s Visible Infrared Imaging Radiometer Suite (VIIRS) “day-night band” can observe dim signals such as city lights (down to the scale of an isolated highway lamp), wildfires, gas flares, auroras, and reflected moonlight during nighttime hours. Swaths of VIIRS data are processed to find moonless, non-cloudy pixels. These “good” pixels are averaged at each location to produce a global image that depicts the Earth’s lights at night. Each pixel shows roughly 0.46 miles (742 meters) across.The top image, centered on France, is a composite of VIIRS data acquired between October 1, 2014 and April 30, 2015. Paris is visible just above the center of the image. North of Paris and across the English Channel (black), London is visible. The relatively dim Alps, characterized by their crescent-shaped geography, are speckled with lights from car headlights and lit roadways. South of the Alps several major cities in Italy are visible with the brightest spot being Milan. Rome is visible in the bottom right of the image. Strings and clusters of light out at sea are produced by ship lights. The second image, centered on France, is a composite of data from the Defense Meteorological Satellite Program (DMSP) Operational Linescan System (OLS) acquired during 2013. Each pixel shows roughly 1.86 miles (3 kilometers) across. The DMSP OLS night-lights data are available starting in 1992, and provide the ability to measure changes in light extent and locations over the past two decades.The image of Australia at night is a composite of VIIRS data acquired between January 1, 2015 and July 31, 2015. Major cities such as Brisbane, Sydney, Melbourne, and Perth are well lit along the coast. Alice Springs—situated in the geographic center of Australia—is some 1,500 kilometers from the nearest major city. Transient lights—those visible in only one monthly image—are colored red. These lights are mainly from brushfires burning during the dry season (May-July) in Australia’s Northern Territory and northern parts of Western Australia. Aside from fires, some of the transient lights could be attributed to natural gas flares, lightning, oil drilling, or mining operations. || ",
            "hits": 61
        },
        {
            "id": 11423,
            "url": "https://svs.gsfc.nasa.gov/11423/",
            "result_type": "Produced Video",
            "release_date": "2013-12-04T13:00:00-05:00",
            "title": "Glimpsing the Infrastructure of a Gamma-ray Burst Jet",
            "description": "A new study using observations from the Liverpool Telescope in the Canary Islands provides the best look to date at magnetic fields at the heart of gamma-ray bursts, the most energetic explosions in the universe. An international team of astronomers from Britain, Slovenia and Italy has glimpsed the infrastructure of a burst's high-speed jet.Gamma-ray bursts are the most luminous explosions in the cosmos. Most are thought to be triggered when the core of a massive star runs out of nuclear fuel, collapses under its own weight, and forms a black hole. The black hole then drives jets of particles that drill all the way through the collapsing star and erupt into space at nearly the speed of light.Theoretical models of gamma-ray bursts predict that light from part of the jet should show strong and stable polarized emissions if the jet possesses a structured magnetic field originating from the environment around the newly-formed black hole, thought to be the \"central engine\" driving the burst.Previous observations of optical afterglows detected polarizations of about 10 percent, but they provided no information about how this value changed with time. As a result, they could not be used to test competing jet models.The Liverpool Telescope's rapid targeting enabled the team to catch the explosion just four minutes after the initial outburst. Over the following 10 minutes, RINGO2 collected 5,600 photographs of the burst afterglow while the properties of the magnetic field were still encoded in its captured light. The observations show that the initial afterglow light was polarized by 28 percent, the highest value ever recorded for a burst, and slowly declined to 16 percent, while the angle of the polarized light remained the same. This supports the presence of a large-scale organized magnetic field linked to the black hole, rather than a tangled magnetic field produced by instabilities within the jet itself. || ",
            "hits": 117
        },
        {
            "id": 3958,
            "url": "https://svs.gsfc.nasa.gov/3958/",
            "result_type": "Visualization",
            "release_date": "2012-09-24T00:00:00-04:00",
            "title": "OSCAR Ocean Currents with Velocity",
            "description": "This visualization shows OSCAR (Ocean Surface Current Analysis Real-time) ocean currents colored by current velocities. OSCAR data (produced by Earth & Space Research and distributed through NOAA and PO.DAAC) is derived from observed satellite altimetry and wind vector data. The visualization runs from January 1, 2008 through July 27, 2012. Blues are slow currents, greens currents are about 0.5 meters per second, and red currents are about 1 meter per second. This visualization was rendered in a variety of sizes from standard 1080p HD to 4k to 6840x3420. The higher resolution versions were rendered for very high resolution display technologies such as hyperwalls and cinema projectors.For more information about the NOAA/NASA OSCAR projects, click here.These visualizations were developed, in part, for display at the \"20 Years of Progress in Radar Altimetry\" Symposium in Venice, Italy in September 2012 and for the Fall 2012 American Geophysical Union conference in December 2012. || ",
            "hits": 726
        },
        {
            "id": 30093,
            "url": "https://svs.gsfc.nasa.gov/30093/",
            "result_type": "Hyperwall Visual",
            "release_date": "2011-10-17T12:00:00-04:00",
            "title": "Chandra Tour of the Crab Nebula",
            "description": "The Crab Nebula is one of the brightest sources of high-energy radiation in the sky. In fact, itâs the expanding remains of an exploded star--a supernova. Scientists have used virtually every telescope to study the Crab. The supernova left behind a magnetized neutron star â a pulsar. The pulsar spins 30 times a second. Each rotation sweeps a lighthouse-like beam, creating a pulse of electromagnetic energy detectable across the spectrum. Recently, NASA's Fermi Gamma Ray Observatory and Italy's AGILE Satellite detected strong gamma-ray flares from the Crab, including a series of \"superflares\" in April 2011. To help pinpoint the location of these flares, astronomers enlisted NASA's Chandra X-ray Observatory. With its keen X-ray eyes, Chandra saw lots of activity, but none seemed to correlated with the superflare. This hints that whatever is causing the flares is happening about a third of a light year from the pulsar. Chandra observations will likely help scientists explain gamma-ray flares. || ",
            "hits": 53
        },
        {
            "id": 10767,
            "url": "https://svs.gsfc.nasa.gov/10767/",
            "result_type": "Produced Video",
            "release_date": "2011-05-11T12:00:00-04:00",
            "title": "NASA's Fermi Spots 'Superflares' in the Crab Nebula",
            "description": "The famous Crab Nebula supernova remnant has erupted in an enormous flare five times more powerful than any previously seen from the object. The outburst was first detected by NASA's Fermi Gamma-ray Space Telescope on April 12 and lasted six days.The nebula, which is the wreckage of an exploded star whose light reached Earth in 1054, is one of the most studied objects in the sky. At the heart of an expanding gas cloud lies what's left of the original star's core, a superdense neutron star that spins 30 times a second. With each rotation, the star swings intense beams of radiation toward Earth, creating the pulsed emission characteristic of spinning neutron stars (also known as pulsars). Apart from these pulses, astrophysicists regarded the Crab Nebula to be a virtually constant source of high-energy radiation. But in January, scientists associated with several orbiting observatories — including NASA's Fermi, Swift and Rossi X-ray Timing Explorer — reported long-term brightness changes at X-ray energies.Scientists think that the flares occur as the intense magnetic field near the pulsar undergoes sudden restructuring. Such changes can accelerate particles like electrons to velocities near the speed of light. As these high-speed electrons interact with the magnetic field, they emit gamma rays in a process known as synchrotron emission.To account for the observed emission, scientists say that the electrons must have energies 100 times greater than can be achieved in any particle accelerator on Earth. This makes them the highest-energy electrons known to be associated with any cosmic source.Based on the rise and fall of gamma rays during the April outbursts, scientists estimate that the size of the emitting region must be comparable in size to the solar system. If circular, the region must be smaller than roughly twice Pluto's average distance from the sun.For more Crab Nebula media go to #10708. || ",
            "hits": 129
        },
        {
            "id": 10766,
            "url": "https://svs.gsfc.nasa.gov/10766/",
            "result_type": "Produced Video",
            "release_date": "2011-05-04T00:00:00-04:00",
            "title": "HD Earth Views from Space",
            "description": "NASA presents images of Earth captured by cameras aboard the International Space Station and the Space Shuttle. Traveling at an approximate speed of 17,500 miles per hour, the space station orbits Earth every 90 minutes from an altitude of approximately 220 miles, and can be seen from Earth with the naked eye. Its crew experiences 16 sunrises and sunsets each day.Get more information about the \"Home Frontier Earth Day Video Contest\".Footage is in Apple ProRes 422 format, 1280x720 aspect ratio, 59.94 fps. || ",
            "hits": 1508
        },
        {
            "id": 10344,
            "url": "https://svs.gsfc.nasa.gov/10344/",
            "result_type": "Produced Video",
            "release_date": "2009-02-19T14:00:00-05:00",
            "title": "Fermi LAT movie of Gamma-ray Burst (GRB) 080916C",
            "description": "This movie compresses about 8 minutes of Fermi LAT observations of GRB 080916C into 6 seconds. Colored dots represent gamma rays of different energies. Visible light has energy between about 2 and 3 electron volts (eV). The blue dots represent lower-energy gamma rays (less than 100 million eV); green, moderate energies (100 million to 1 billion eV); and red, the highest energies (more than 1 billion eV). || ",
            "hits": 134
        },
        {
            "id": 10323,
            "url": "https://svs.gsfc.nasa.gov/10323/",
            "result_type": "Produced Video",
            "release_date": "2008-08-05T12:00:00-04:00",
            "title": "GLASTCast Episode 3 - Swift and GLAST",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.  What's the difference between the Swift and GLAST satellites? Both missions look at gamma-ray bursts (GRBs), but in different ways. Swift can rapidly and precisely determine the locations of GRBs and observe their afterglows at X-ray, ultraviolet, and optical wavelengths. GLAST will provide exquisite observations of the burst over the gamma ray spectrum, giving scientists their first complete view of the total energy released in these extraordinary events. Beyond GRB science, GLAST is a multipurpose observatory that will study a broad range of cosmic phenomena. Swift is also a multipurpose observatory, but was built primarily to study GRBs.  Interviews with (in order of appearance):  David Thompson - GLAST Deputy Project Scientist, NASA Goddard Charles \"Chip\" Meegan - GLAST Burst Monitor (GBM) Principal Investigator, NASA Marshall Lynn Cominsky - GLAST Astrophysicist and Education and Public Outreach Lead, Sonoma State University Neil Gehrels - GLAST Deputy Project Scientist, NASA Goddard Steve Ritz - GLAST Project Scientist, NASA Goddard Alan Marscher - Professor of Astronomy, Boston University || ",
            "hits": 70
        },
        {
            "id": 10324,
            "url": "https://svs.gsfc.nasa.gov/10324/",
            "result_type": "Produced Video",
            "release_date": "2008-08-05T12:00:00-04:00",
            "title": "GLASTcast Episode 4: Launching a Spacecraft",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.  The GLAST satellite will launch in 2008 from Cape Canaveral Air Station, on Florida's east coast. GLAST will be carried on a Delta II Heavy launch vehicle, with 9 solid rocket boosters. GLAST is the first imaging gamma-ray observatory to survey the entire sky every day and with high sensitivity. It will give scientists a unique opportunity to learn about the ever-changing Universe at extreme energies.  Interviews with (in order of appearance):  Peter Michaelson - Large Area Telescope (LAT) Principal Investigator, Stanford University Lynn Cominsky - GLAST Astrophysicist and Education and Public Outreach Lead, Sonoma State University David Thompson - GLAST Deputy Project Scientist, NASA Goddard Kevin Grady - GLAST Project Manager, NASA Goddard Neil Johnson - Large Area Telescope (LAT) Deputy Principal Investigator, US Naval Research Lab Jonathan Ormes - Large Area Telescope (LAT) Senior Scientist Advisory Committee, University of Denver Charles \"Chip\" Meegan - GLAST Burst Monitor (GBM) Principal Investigator, NASA Marshall Luke Drury - Professor of Astronomy, Dublin Institute for Advanced Studies Per Carlson - Professor of Elementary Particle Physics, Manne Siegbahn Laboratory Isabelle Grenier - Principal Investigator of the GLAST French contribution, French Atomic Energy Commission || ",
            "hits": 27
        },
        {
            "id": 10325,
            "url": "https://svs.gsfc.nasa.gov/10325/",
            "result_type": "Produced Video",
            "release_date": "2008-08-05T01:00:00-04:00",
            "title": "GLASTcast Episode 5: Meet the U.S. Team",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.  This video introduces only a small fraction of the hundreds of U.S. and international GLAST team members. To meet more of the team go to: www.nasa.gov/glast.  Interviews with (in order of appearance):  Bill Atwood - GLAST Co-Creator, Santa Cruz Institute of Particle Physics, University of California, Santa Cruz David Thompson - GLAST Deputy Project Scientist, NASA Goddard Julie McEnery - GLAST Deputy Project Scientist, NASA Goddard Steve Ritz - GLAST Project Scientist, NASA Goddard Neil Gehrels - GLAST Deputy Project Scientist, NASA Goddard Peter Michaelson - Large Area Telescope (LAT) Principal Investigator, Stanford University Kevin Grady - GLAST Project Manager, NASA Goddard Charles \"Chip\" Meegan - GLAST Burst Monitor (GBM) Principal Investigator, NASA Marshall || ",
            "hits": 21
        },
        {
            "id": 10322,
            "url": "https://svs.gsfc.nasa.gov/10322/",
            "result_type": "Produced Video",
            "release_date": "2008-07-30T00:00:00-04:00",
            "title": "GLAST Soundbites",
            "description": "Selected soundbites with Steve Ritz, GLAST Project Scientist; Peter Michelson, LAT Principal Investigator; Charles 'Chip' Meegan, GBM Principal Investigator. NASA's GLAST mission is an astrophysics partnership, developed in collaboration with the U.S. Department of Energy along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S. || ",
            "hits": 18
        },
        {
            "id": 10251,
            "url": "https://svs.gsfc.nasa.gov/10251/",
            "result_type": "Produced Video",
            "release_date": "2008-05-31T00:00:00-04:00",
            "title": "GLAST Prelude, for Brass Quintet, Op.12",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institiutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S. Music composed by Nolan Gasser, © 2008 Music performed by the American Brass Quintet || ",
            "hits": 25
        },
        {
            "id": 10247,
            "url": "https://svs.gsfc.nasa.gov/10247/",
            "result_type": "Produced Video",
            "release_date": "2008-05-29T00:00:00-04:00",
            "title": "GLASTcast Episode 1:  What is GLAST?",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.  The Universe is home to numerous exotic and beautiful phenomena, some of which can generate inconceivable amounts of energy. GLAST will open a new window on this high-energy world. With GLAST, astronomers will have a superior tool to study how black holes, notorious for pulling matter in, can accelerate jets of gas outward at fantastic speeds. Physicists will be able to search for signals of new fundamental processes that are inaccessible in ground-based accelerators and observatories. GLAST's spectacular high-energy gamma-ray \"eyeglasses\" will reveal hidden wonders, opening our minds to new possibilities and discoveries, expanding our understanding of the Universe and our place in it.  Interviews with (in order of appearance):  Steve Ritz - GLAST Project Scientist, NASA Goddard Peter Michaelson - Large Area Telescope (LAT) Principal Investigator, Stanford University Diego Torres - Large Area Telescope (LAT) Scientist, University of Barcelona Neil Gehrels - GLAST Deputy Project Scientist, NASA Goddard David Thompson - GLAST Deputy Project Scientist, NASA Goddard Luke Drury - Professor of Astronomy, Dublin Institute for Advanced Studies Valerie Connaughton - GLAST Burst Monitor (GBM) Team, NASA Marshall/University of Alabama Martin Pohl - GLAST Interdisciplinary Scientist, Iowa State University Per Carlson - Professor of Elementary Particle Physics, Manne Siegbahn Laboratory Charles \"Chip\" Meegan - GLAST Burst Monitor (GBM) Principal Investigator, NASA Marshall Alan Marscher - Professor of Astronomy, Boston University Julie McEnery - GLAST Deputy Project Scientist, NASA Goddard || ",
            "hits": 32
        },
        {
            "id": 10248,
            "url": "https://svs.gsfc.nasa.gov/10248/",
            "result_type": "Produced Video",
            "release_date": "2008-05-23T00:00:00-04:00",
            "title": "GLASTcast Episode 2:  What are Gamma Rays?",
            "description": "NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.  Somewhere out in the vast depths of space, a giant star explodes with the power of millions of suns. As the star blows up, a black hole forms at its center. The black hole blows two blowtorches in opposite directions, in narrow jets of gamma rays. NASA's Gamma-ray Large Area Space Telescope, or GLAST, will catch about 200 of these explosions, known as gamma-ray bursts, each year. GLAST's detailed observations may give astronomers the clues they need to unravel the mystery of what exactly produces these gamma-ray bursts, which are the brightest explosions in the universe since the Big Bang.  Interviews with (in order of appearance):  Phil Plait - Astronomer, Bad Astronomy David Thompson - GLAST Deputy Project Scientist, NASA Goddard Valerie Connaughton - GLAST Burst Monitor (GBM) Team, NASA Marshall/University of Alabama Neil Gehrels - GLAST Deputy Project Scientist, NASA Goddard Isabelle Grenier - Principal Investigator of the GLAST French contribution, French Atomic Energy Commission Peter Michaelson - Large Area Telescope (LAT) Principal Investigator, Stanford University Charles \"Chip\" Meegan - GLAST Burst Monitor (GBM) Principal Investigator, NASA Marshall Martin Pohl - GLAST Interdisciplinary Scientist, Iowa State University Steve Ritz - GLAST Project Scientist, NASA Goddard || ",
            "hits": 26
        },
        {
            "id": 10172,
            "url": "https://svs.gsfc.nasa.gov/10172/",
            "result_type": "Produced Video",
            "release_date": "2007-09-17T00:00:00-04:00",
            "title": "GLAST Promo Video",
            "description": "NASA's Gamma-ray Large Area Space Telescope (GLAST) is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light and the gamma-ray sky is spectacularly different from the one we perceive with our own eyes. With a huge leap in all key capabilities, GLAST data will enable scientists to answer persistent questions across a broad range of topics, including supermassive black-hole systems, pulsars, the origina of cosmic rays, and searches for signals new physics. NASA's GLAST mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S. || ",
            "hits": 57
        },
        {
            "id": 3270,
            "url": "https://svs.gsfc.nasa.gov/3270/",
            "result_type": "Visualization",
            "release_date": "2005-10-11T12:00:00-04:00",
            "title": "Seasonal Landcover Change over the Alps",
            "description": "The Blue Marble Next Generation data set provides a monthly global cloud-free true-color picture of the Earth's land cover at a 500-meter spatial resolution. This visualization of the data set shows seasonal variations such as snowfall, spring greening and droughts in a seamless fashion, thereby heightening awareness of changes in the Earth's climate. Here we focus on the seasonal land cover changes over the European Alps. This data set is derived from imagery taken in 2004 by the MODIS instrument on the Terra satellite. || ",
            "hits": 77
        },
        {
            "id": 2687,
            "url": "https://svs.gsfc.nasa.gov/2687/",
            "result_type": "Visualization",
            "release_date": "2003-01-23T12:00:00-05:00",
            "title": "Apollo 17 30th Anniversary: Blue Marble Italian Fly-over",
            "description": "In conjunction with the 30th Anniversary Apollo 17 mission, NASA put together a special release highlighting one of the most popular photos taken during that mission.  The photo (#AS17-148-22727) was taken on Dec. 7, 1972 from the Apollo 17 command module.  Over the years, many other satellites have taken imagery of Earth, including Terra/MODIS.  This animation uses a global mosaic derived from Terra/MODIS and flies us over Italy to celebrate how far Earth science imagery has come since the days of Apollo 17. || ",
            "hits": 26
        },
        {
            "id": 2212,
            "url": "https://svs.gsfc.nasa.gov/2212/",
            "result_type": "Visualization",
            "release_date": "2001-08-02T12:00:00-04:00",
            "title": "Mt. Etna, Sicily on July 13, 2001 from Landsat-7",
            "description": "Landsat-7 is capable of seeing in infrared, in this animation we can see the lava flows from the volcano. || Landsat-7, July 13, 2001, showing Mt. Etna in Sicily. || a002212.00005_print.png (720x480) [581.6 KB] || a002212_pre.jpg (320x240) [13.6 KB] || a002212.webmhd.webm (960x540) [1.1 MB] || a002212.dv (720x480) [43.5 MB] || a002212.mpg (320x240) [282.2 KB] || ",
            "hits": 21
        },
        {
            "id": 2213,
            "url": "https://svs.gsfc.nasa.gov/2213/",
            "result_type": "Visualization",
            "release_date": "2001-08-02T12:00:00-04:00",
            "title": "Mt. Etna, Sicily on July 29, 2001 from Landsat-7",
            "description": "Landsat-7 is capable of seeing in infrared, in this animation we can see the lava flows from the volcano. || True color and false color  close-ups of Mt. Etna, Sicily; Landsat-7 July 29, 2001. || a002213.00005_print.png (720x480) [569.6 KB] || a002213_pre.jpg (320x240) [13.3 KB] || a002213.webmhd.webm (960x540) [883.8 KB] || a002213.dv (720x480) [36.8 MB] || a002213.mpg (320x240) [280.9 KB] || ",
            "hits": 17
        },
        {
            "id": 2207,
            "url": "https://svs.gsfc.nasa.gov/2207/",
            "result_type": "Visualization",
            "release_date": "2001-07-24T12:00:00-04:00",
            "title": "Mt Etna Eruption, July 24, 2001",
            "description": "This is simple zoom into the Mount Etna eruption.  The plume from the ongoing eruption has changed color since the last SeaWiFS image.  In today's image, collected around 7:00 am EST, the ash plume has a greenish orange color in this 670/555/412 nanometer composite. || ",
            "hits": 16
        },
        {
            "id": 1269,
            "url": "https://svs.gsfc.nasa.gov/1269/",
            "result_type": "Visualization",
            "release_date": "1999-12-03T12:00:00-05:00",
            "title": "Italy in Winter (With Dates)",
            "description": "Zooming in to northern Italy, showing a time lapse series of SeaWiFS images from January, 2000 || a001269.00005_print.png (720x480) [655.6 KB] || a001269_thm.png (80x40) [7.0 KB] || a001269_pre.jpg (320x238) [14.3 KB] || a001269_pre_searchweb.jpg (320x180) [88.7 KB] || a001269.webmhd.webm (960x540) [3.5 MB] || a001269.dv (720x480) [89.0 MB] || a001269.mp4 (640x480) [4.8 MB] || a001269.mpg (352x240) [3.5 MB] || ",
            "hits": 5
        },
        {
            "id": 1270,
            "url": "https://svs.gsfc.nasa.gov/1270/",
            "result_type": "Visualization",
            "release_date": "1999-12-03T12:00:00-05:00",
            "title": "Italy in Winter (without dates)",
            "description": "Zooming in to northern Italy, showing a time lapse series of SeaWiFS images from January, 2000 || a001270.00005_print.png (720x480) [655.0 KB] || a001270_thm.png (80x40) [7.1 KB] || a001270_pre.jpg (320x238) [14.5 KB] || a001270_pre_searchweb.jpg (320x180) [89.3 KB] || a001270.webmhd.webm (960x540) [3.4 MB] || a001270.dv (720x480) [89.0 MB] || a001270.mp4 (640x480) [4.7 MB] || a001270.mpg (352x240) [3.4 MB] || ",
            "hits": 7
        },
        {
            "id": 863,
            "url": "https://svs.gsfc.nasa.gov/863/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Rome Flyby",
            "description": "A flyby of Rome, from Landsat data || a000863.00010_print.png (720x480) [592.3 KB] || a000863_thm.png (80x40) [5.2 KB] || a000863_pre.jpg (320x238) [8.9 KB] || a000863_pre_searchweb.jpg (320x180) [68.9 KB] || a000863.webmhd.webm (960x540) [13.8 MB] || a000863.dv (720x480) [247.0 MB] || a000863.mp4 (640x480) [13.1 MB] || a000863.mpg (352x240) [9.4 MB] || ",
            "hits": 6
        }
    ]
}