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    "results": [
        {
            "id": 12265,
            "url": "https://svs.gsfc.nasa.gov/12265/",
            "result_type": "Produced Video",
            "release_date": "2016-06-22T13:00:00-04:00",
            "title": "X-ray Echoes Map a 'Killer' Black Hole",
            "description": "NASA Goddard astronomer Erin Kara discusses the discovery of X-ray echoes from Swift J1644+57, a black hole that shattered a passing star. X-rays produced by flares near this million-solar-mass black hole bounced off the nascent accretion disk and revealed its structure.  Credit: NASA's Goddard Space Flight CenterMusic: \"The Orion Arm\" and \"Particle Acceleration\" both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || TD_Still.png (1920x1080) [11.0 MB] || TD_Still_print.jpg (1024x576) [109.7 KB] || TD_Still_searchweb.png (180x320) [91.6 KB] || TD_Still_thm.png (80x40) [7.0 KB] || 12265_BH_Echoes_FINAL2_ProRes_1920x1080_2997.mov (1920x1080) [3.8 GB] || 12265_BH_Echoes_FINAL2_youtube_hq.mov (1920x1080) [1.6 GB] || 12265_BH_Echoes_FINAL2-HD_1080p.mov (1920x1080) [443.2 MB] || 12265_BH_Echoes_FINAL2-Apple_Devices_Best.m4v (1920x1080) [295.2 MB] || 12265_BH_Echoes_FINAL2_appletv.m4v (1280x720) [150.6 MB] || 12265_BH_Echoes_FINAL2-Apple_HD_Compatible.m4v (960x540) [118.9 MB] || 12265_BH_Echoes_FINAL2_appletv_subtitles.m4v (1280x720) [150.7 MB] || 12265_BH_Echoes_FINAL2-Apple_HD_Compatible.webm (960x540) [31.7 MB] || 12265_BH_Echoes_FINAL2_SRT_Captions.en_US.srt [5.3 KB] || 12265_BH_Echoes_FINAL2_SRT_Captions.en_US.vtt [5.3 KB] || 12265_BH_Echoes_FINAL2_lowres.mp4 (480x272) [39.9 MB] || ",
            "hits": 170
        },
        {
            "id": 11600,
            "url": "https://svs.gsfc.nasa.gov/11600/",
            "result_type": "Produced Video",
            "release_date": "2014-09-02T11:45:00-04:00",
            "title": "Countdown To Mars",
            "description": "How did Mars’ climate change? How has the atmosphere been lost—and how quickly are gases escaping now? These are the questions that NASA’s MAVEN spacecraft will explore when it reaches the planet on September 21, 2014. Scientists believe Mars once had a thicker atmosphere that may have been gradually lost to space. The change would have had a considerable impact on the planet’s climate, liquid water and habitability, ultimately shaping the world we see today. Using a suite of instruments aboard the spacecraft, researchers will probe Mars’ upper atmosphere from orbit to study the processes that led to the thinning of its atmosphere over billions of years. Watch the video to learn more. || ",
            "hits": 33
        },
        {
            "id": 11595,
            "url": "https://svs.gsfc.nasa.gov/11595/",
            "result_type": "Produced Video",
            "release_date": "2014-08-14T11:00:00-04:00",
            "title": "The Three Percent",
            "description": "Freshwater seems abundant, but when accounting for all the water on Earth, it's in limited supply. Just three percent of the water on our planet is freshwater. A majority of this water, about two percent of the world total, is contained in glaciers and ice sheets or stored below ground. The remaining one percent is found in lakes, rivers and wetland areas or transported through the atmosphere in the form of water vapor, clouds and precipitation. Rain and snowfall replenish freshwater sources, making it vital to know when, where and how much water is falling at any given time. Using NASA's Global Precipitation Measurement satellite, researchers can track precipitation worldwide and monitor levels from space. Watch the video to learn more. || ",
            "hits": 811
        },
        {
            "id": 11619,
            "url": "https://svs.gsfc.nasa.gov/11619/",
            "result_type": "Produced Video",
            "release_date": "2014-07-30T16:00:00-04:00",
            "title": "Water Falls: Show Me the Water",
            "description": "This is a spinoff video for the Science On a Sphere film, \"Water Falls.\" || ",
            "hits": 35
        },
        {
            "id": 11403,
            "url": "https://svs.gsfc.nasa.gov/11403/",
            "result_type": "Produced Video",
            "release_date": "2013-11-08T11:00:00-05:00",
            "title": "MAVEN National Air and Space Museum Presentation",
            "description": "Ancient riverbeds, crater lakes and flood channels all attest to Mars's warm, watery past. So how did the Red Planet evolve from a once hospitable world into the cold, dry desert that we see today? One possibility is that Mars lost its early atmosphere, allowing its water to escape into space, and NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft will investigate just that. On September 25, 2013, MAVEN Principal Investigator Bruce Jakosky delivered a presentation at the Smithsonian National Air and Space Museum, discussing NASA's next mission to Mars. An edited version appears below. || ",
            "hits": 98
        },
        {
            "id": 11332,
            "url": "https://svs.gsfc.nasa.gov/11332/",
            "result_type": "Produced Video",
            "release_date": "2013-08-06T08:00:00-04:00",
            "title": "WATER FALLS — A Science On a Sphere Movie",
            "description": "The Global Precipitation Measurement mission (GPM) is a massive, multinational mission utilizing a fleet of spacecraft, sophisticated ground based data processing systems, and years of planning. To capture the essence of this immense undertaking and introduce it to broad audiences, NASA's GPM project office decided to do something out of the box. WATER FALLS is the result. Designed specifically for spherical screens, WATER FALLS abstracts the complex mechanics of the GPM mission, and explores the diversity of phenomena inherent to the water cycle. Presented in sensual, evocative, even surprising ways, WATER FALLS offers vital information about GPM's profound importance to everyone who lives on Earth. || ",
            "hits": 24
        },
        {
            "id": 11295,
            "url": "https://svs.gsfc.nasa.gov/11295/",
            "result_type": "Produced Video",
            "release_date": "2013-06-13T11:00:00-04:00",
            "title": "MAVEN Imaging Ultraviolet Spectrograph",
            "description": "The philosophy of NASA's Mars Program has been \"Follow the water,\" but \"Where did the atmosphere go?\" is still a lingering question. Although fluvial features such as dry riverbeds are visible on Mars, the atmosphere today is too thin to support liquid water, implying that Mars once had a thicker atmosphere that was lost to space. NASA's Mars Atmosphere and Volatile EvolutioN Mission, or MAVEN, will test this hypothesis. As part of its remote sensing instrument package, MAVEN's Imaging Ultraviolet Spectrograph (IUVS) will look at isotopic hydrogen ratios in the upper atmosphere of Mars, helping scientists to determine just how much water once flowed across the Red Planet. || ",
            "hits": 49
        },
        {
            "id": 10811,
            "url": "https://svs.gsfc.nasa.gov/10811/",
            "result_type": "Produced Video",
            "release_date": "2012-10-16T22:00:00-04:00",
            "title": "Media Produced for NASA's Goddard Space Flight Center by Montana State University SNHF Alumni",
            "description": "The Science and Natural History Filmmaking MFA program at Montana State University was the first program of its kind and is still the largest. There is a long-standing tradition of some graduates going on to work at the Goddard Space Flight Center as video producers. This short video samples some of the animations, visualizations and clips that they have produced. || ",
            "hits": 19
        },
        {
            "id": 11024,
            "url": "https://svs.gsfc.nasa.gov/11024/",
            "result_type": "Produced Video",
            "release_date": "2012-07-09T09:00:00-04:00",
            "title": "MAVEN Orbit Animations and Beauty Passes",
            "description": "This collection contains animations showing the MAVEN spacecraft in orbit around Mars, as well as MAVEN's overall orbit trajectory. || ",
            "hits": 58
        },
        {
            "id": 10985,
            "url": "https://svs.gsfc.nasa.gov/10985/",
            "result_type": "Produced Video",
            "release_date": "2012-07-03T00:00:00-04:00",
            "title": "Lightning Reverb",
            "description": "Lightning flashes some 50 times every second on Earth. These discharges release bursts of ultra-low-frequency energy that coalesce and get stronger, ultimately creating a beating pulse of electromagnetic waves around the planet. This phenomenon is called Schumann resonance, and it takes place between the ground and the lower ionosphere, a region of charged particles about 60 miles up in the atmosphere. Scientists had thought Schumann resonance was confined within the atmosphere and could only be observed from the planet's surface. Using NASA's Vector Electric Field Instrument (VEFI) aboard a U.S. Air Force satellite, scientists recently discovered that energy from the resonance sometimes leaks beyond Earth and can be detected from above, providing a new tool to analyze the chemical and physical makeup of the atmosphere. The animation shows how the electromagnetic energy from lightning gradually resonates around the planet and occasionally even reaches out into space. || ",
            "hits": 403
        },
        {
            "id": 10968,
            "url": "https://svs.gsfc.nasa.gov/10968/",
            "result_type": "Produced Video",
            "release_date": "2012-05-30T10:00:00-04:00",
            "title": "MAVEN Profiles",
            "description": "Spanish-language profile videos of MAVEN project managers Sandra Cauffman and Carlos Gomez-Rosa. || ",
            "hits": 35
        },
        {
            "id": 10909,
            "url": "https://svs.gsfc.nasa.gov/10909/",
            "result_type": "Produced Video",
            "release_date": "2012-03-13T11:00:00-04:00",
            "title": "NASA's Visualization Explorer iPad App Expands Coverage Across the Universe",
            "description": "NASA has peered 13 billion years back into the history of the universe. You won't have to look as far to find our cutting-edge science. The NASA Visualization Explorer app has broadened its scope to include more awe-inspiring discoveries beamed back to Earth from the agency's entire fleet of satellites, spacecraft and space telescopes. Expect stories each week that cover all four fields of NASA's science research: planetary, heliophysics, astrophysics and Earth. You'll get new views of the planets and sun from satellites such as Cassini and Solar Dynamics Observatory; visualizations and animations of stars, distant galaxies and the cosmic stuff in between; and dramatic images taken by the legendary Hubble Space Telescope. || ",
            "hits": 58
        },
        {
            "id": 10891,
            "url": "https://svs.gsfc.nasa.gov/10891/",
            "result_type": "Produced Video",
            "release_date": "2012-01-11T14:00:00-05:00",
            "title": "Schumann resonance animation",
            "description": "At any given moment about 2,000 thunderstorms roll over Earth, producing some 50 flashes of lightning every second. Each lightning burst creates electromagnetic waves that begin to circle around Earth captured between Earth's surface and a boundary about 60 miles up. Some of the waves - if they have just the right wavelength - combine, increasing in strength, to create a repeating atmospheric heartbeat known as Schumann resonance. This resonance provides a useful tool to analyze Earth's weather, its electric environment, and to even help determine what types of atoms and molecules exist in Earth's atmosphere.The waves created by lightning do not look like the up and down waves of the ocean, but they still oscillate with regions of greater energy and lesser energy. These waves remain trapped inside an atmospheric ceiling created by the lower edge of the \"ionosphere\" - a part of the atmosphere filled with charged particles, which begins about 60 miles up into the sky. In this case, the sweet spot for resonance requires the wave to be as long (or twice, three times as long, etc) as the circumference of Earth. This is an extremely low frequency wave that can be as low as 8 Hertz (Hz) - some one hundred thousand times lower than the lowest frequency radio waves used to send signals to your AM/FM radio. As this wave flows around Earth, it hits itself again at the perfect spot such that the crests and troughs are aligned. Voila, waves acting in resonance with each other to pump up the original signal.While they'd been predicted in 1952, Schumann resonances were first measured reliably in the early 1960s. Since then, scientists have discovered that variations in the resonances correspond to changes in the seasons, solar activity, activity in Earth's magnetic environment, in water aerosols in the atmosphere, and other Earth-bound phenomena. || ",
            "hits": 4440
        },
        {
            "id": 10869,
            "url": "https://svs.gsfc.nasa.gov/10869/",
            "result_type": "Produced Video",
            "release_date": "2012-01-10T11:00:00-05:00",
            "title": "NASA's RXTE Helps Pinpoint Launch of 'Bullets' in a Black Hole's Jet",
            "description": "Using observations from NASA's Rossi X-ray Timing Explorer (RXTE) satellite and the National Science Foundation's (NSF) Very Long Baseline Array (VLBA) radio telescope, an international team of astronomers has identified the moment when a black hole in our galaxy launched superfast knots of gas into space. Racing outward at about one-quarter the speed of light, these \"bullets\" of ionized gas are thought to arise from a region located just outside the black hole's event horizon, the point beyond which nothing can escape.The research centered on the mid-2009 outburst of a binary system known as H1743-322, located about 28,000 light-years away toward the constellation Scorpius. Discovered by NASA's HEAO-1 satellite in 1977, the system is composed of a normal star and a black hole of modest but unknown masses. Their orbit around each other is measured in days, which puts them so close together that the black hole pulls a continuous stream of matter from its stellar companion. The flowing gas forms a flattened accretion disk millions of miles across, several times wider than our sun, centered on the black hole. As matter swirls inward, it is compressed and heated to tens of millions of degrees, so hot that it emits X-rays.Some of the infalling matter becomes re-directed out of the accretion disk as dual, oppositely directed jets. Most of the time, the jets consist of a steady flow of particles. Occasionally, though, they morph into more powerful outflows that hurl massive gas blobs at significant fractions of the speed of light. || ",
            "hits": 84
        },
        {
            "id": 10889,
            "url": "https://svs.gsfc.nasa.gov/10889/",
            "result_type": "Produced Video",
            "release_date": "2012-01-04T00:00:00-05:00",
            "title": "NASA Finds Russian Runoff Freshening Canadian Arctic",
            "description": "A new NASA and University of Washington study allays concerns that melting Arctic sea ice could be increasing the amount of freshwater in the Arctic enough to have an impact on the global \"ocean conveyor belt\" that redistributes heat around our planet. Read the full press release here: http://www.nasa.gov/topics/earth/features/earth20120104.html || ",
            "hits": 18
        },
        {
            "id": 10824,
            "url": "https://svs.gsfc.nasa.gov/10824/",
            "result_type": "Produced Video",
            "release_date": "2011-09-22T00:00:00-04:00",
            "title": "A World Without The Montreal Protocol",
            "description": "A week ago marked the 24th anniversary of the signing of the Montreal Protocol, a landmark piece of legislation that began phasing out the production of ozone-depleting chemicals called chlorofluorocarbons (CFCs). These chemicals, also known by the trade name Freon, were common refrigerants and widely used in aerosol spray cans prior to the Montreal Protocol. In recent years, scientists have been using cutting-edge computer models of the atmosphere to ask a fascinating question: What would have happened to the ozone layer if nations had done nothing to limit the release of CFCs? The impact of inaction, the modeling shows, would have been ominous: increased rates of cancer, cataracts, and immune deficiency diseases are just a few of the consequences. By 2065, global ozone levels would drop to less than 110 Dobson units—a measure of the amount of ozone between the surface and space. (A healthy Dobson unit reading over Antarctica is around 275.) \"We wouldn't be able to go out much at all,\" says NASA scientist Paul Newman. In the visualization below, watch how ozone levels change in two simulated versions of the future: one where CFCs have been regulated, and one where they have not. || ",
            "hits": 85
        },
        {
            "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": 37
        },
        {
            "id": 10807,
            "url": "https://svs.gsfc.nasa.gov/10807/",
            "result_type": "Produced Video",
            "release_date": "2011-08-24T13:00:00-04:00",
            "title": "NASA's Swift Satellite Spots Black Hole Devouring A Star",
            "description": "In late March 2011, NASA's Swift satellite alerted astronomers to intense and unusual high-energy flares from a new source in the constellation Draco. They soon realized that the source, which is now known as Swift J1644+57, was the result of a truly extraordinary event — the awakening of a distant galaxy's dormant black hole as it shredded and consumed a star. The galaxy is so far away that the radiation from the blast has traveled 3.9 billion years before reaching Earth. Most galaxies, including our own, possess a central supersized black hole weighing millions of times the sun's mass. According to the new studies, the black hole in the galaxy hosting Swift J1644+57 may be twice the mass of the four-million-solar-mass black hole lurking at the center of our own Milky Way galaxy. As a star falls toward a black hole, it is ripped apart by intense tides. The gas is corralled into a disk that swirls around the black hole and becomes rapidly heated to temperatures of millions of degrees. The innermost gas in the disk spirals toward the black hole, where rapid motion and magnetism creates dual, oppositely directed \"funnels\" through which some particles may escape. Particle jets driving matter at velocities greater than 80-90 percent the speed of light form along the black hole's spin axis. In the case of Swift J1644+57, one of these jets happened to point straight at Earth.Theoretical studies of tidally disrupted stars suggested that they would appear as flares at optical and ultraviolet energies. The brightness and energy of a black hole's jet is greatly enhanced when viewed head-on. The phenomenon, called relativistic beaming, explains why Swift J1644+57 was seen at X-ray energies and appeared so strikingly luminous. When first detected on March 28, the flares were initially assumed to signal a gamma-ray burst, one of the nearly daily short blasts of high-energy radiation often associated with the death of a massive star and the birth of a black hole in the distant universe. But as the emission continued to brighten and flare, astronomers realized that the most plausible explanation was the tidal disruption of a sun-like star seen as beamed emission. || ",
            "hits": 440
        },
        {
            "id": 10789,
            "url": "https://svs.gsfc.nasa.gov/10789/",
            "result_type": "Produced Video",
            "release_date": "2011-06-07T14:00:00-04:00",
            "title": "NPPy: Big Planet, Little Bear",
            "description": "NPP is the prototype of the next generation weather satellites, named JPSS. NPP has five instruments on board and will continue the legacy of existing weather satellites like Terra and Aqua. NPP will deliver critical data not only for weather forecasters but for scientists who are trying to understand how climate is changing over long periods of time. || ",
            "hits": 35
        },
        {
            "id": 10694,
            "url": "https://svs.gsfc.nasa.gov/10694/",
            "result_type": "Produced Video",
            "release_date": "2010-11-19T11:30:00-05:00",
            "title": "Teen Sailor Meets NASA Team That Saved Her Life",
            "description": "The Geostationary Operational Environmental Satellites (GOES) have the ability to not only monitor Earth's weather but also to recieve distress signals from victims. Currently, the Search and Rescue Satellite-Aided System SARSAT, developed by a NASA Goddard team, has saved more than 27,000 lives since its launch 30 years ago. The same team is now developing a new system, which will use a constellation of 24 GPS satellites to be able to pick up a distress signal and relay the victim's location precisely and almost instantly. || ",
            "hits": 41
        },
        {
            "id": 10666,
            "url": "https://svs.gsfc.nasa.gov/10666/",
            "result_type": "Produced Video",
            "release_date": "2010-10-05T00:00:00-04:00",
            "title": "MAVEN Science Teaser",
            "description": "The Mars Atmosphere and Volatile Evolution Mission (MAVEN), set to launch in 2013, will explore the planet's upper atmosphere, ionosphere and interactions with the sun and solar wind. Scientists will use MAVEN data to determine the role that loss of volatile compounds from the Mars atmosphere to space has played through time, giving insight into the history of Mars atmosphere and climate, liquid water, and planetary habitability. || ",
            "hits": 63
        },
        {
            "id": 10553,
            "url": "https://svs.gsfc.nasa.gov/10553/",
            "result_type": "Produced Video",
            "release_date": "2010-05-24T08:45:00-04:00",
            "title": "Saved By A Weather Satellite",
            "description": "The Geostationary Operational Environmental Satellites (GOES) have the ability to constantly oversee a large area of the Earth and send real time data to users. GOES sends not only weather data but it also watches the sun continuously and at the same time provides critical data that helps rescue personal locate victims in distress. || ",
            "hits": 96
        },
        {
            "id": 10554,
            "url": "https://svs.gsfc.nasa.gov/10554/",
            "result_type": "Produced Video",
            "release_date": "2010-05-24T00:00:00-04:00",
            "title": "NASA Develops Enhanced Search and Rescue Technologies",
            "description": "The Search and Rescue Mission Office at the NASA Goddard Space Flight Center, in collaboration with NOAA, Coast Guard, Air Force, and other U.S. agency partners, has developed new technology that will more quickly identify the locations of people in distress and reduce the risk to rescuers. Called the Distress Alerting Satellite System (DASS), this next-generation search and rescue system reduces search times from hours to a few minutes. When it goes online, DASS will be able to almost instantaneously detect and locate distress signals generated by 406 MHz beacons installed on aircraft and vessels or carried by individuals, greatly enhancing the international community's ability to rescue people in distress. || ",
            "hits": 29
        },
        {
            "id": 10521,
            "url": "https://svs.gsfc.nasa.gov/10521/",
            "result_type": "Produced Video",
            "release_date": "2009-11-05T10:00:00-05:00",
            "title": "The Road to Glory",
            "description": "Glory is a unique research satellite designed to orbit the Earth and achieve two major goals.  Glory's first goal is to collect data on the properties of aerosols and black carbon in the Earth's atmosphere and climate system; its second goal is to collect data on solar irradiance for Earth's long-term climate record.  This seven-minute video introduces Glory's science objectives, people, and instruments, and provides an overview of the Glory mission.For complete transcript, click here. || The_Road_to_Glory_512x288.01102_print.jpg (1024x576) [74.3 KB] || The_Road_to_Glory_512x288_web.png (180x320) [222.3 KB] || The_Road_to_Glory_512x288_thm.png (80x40) [14.2 KB] || The_Road_to_Glory_AppleTV.webmhd.webm (960x540) [90.6 MB] || The_Road_to_Glory_1280x720_ProRes.mov (1280x720) [6.3 GB] || The_Road_to_Glory_1280x720_H264.mov (1280x720) [204.8 MB] || The_Road_to_Glory_AppleTV.m4v (960x540) [235.9 MB] || The_Road_to_Glory_640x480_ipod.m4v (640x360) [76.0 MB] || The_Road_to_Glory_512x288.mpg (512x288) [141.3 MB] || The_Road_to_Glory_320x240.mp4 (320x180) [33.4 MB] || The_Road_to_Glory.wmv (320x180) [37.8 MB] || ",
            "hits": 28
        },
        {
            "id": 10522,
            "url": "https://svs.gsfc.nasa.gov/10522/",
            "result_type": "Produced Video",
            "release_date": "2009-11-04T12:00:00-05:00",
            "title": "The Rough Road to Space",
            "description": "Space is a harsh environment, and building a space-bound satellite is no small feat!  Here's a look at how NASA engineers get the Glory mission off the ground and safely into space!For complete transcript, click here. || The_Rough_Road_to_Space_512x288.01977_print.jpg (1024x576) [89.7 KB] || The_Rough_Road_to_Space_512x288_web.png (320x180) [264.1 KB] || The_Rough_Road_to_Space_512x288_thm.png (80x40) [17.2 KB] || The_Rough_Road_to_Space_AppleTV.webmhd.webm (960x540) [29.2 MB] || Rough_Road_to_Space_1280x720_ProRes.mov (1280x720) [2.2 GB] || The_Rough_Road_to_Space_1280x720_H264.mov (1280x720) [67.9 MB] || The_Rough_Road_to_Space_AppleTV.m4v (960x540) [75.1 MB] || The_Rough_Road_to_Space_640x480_ipod.m4v (640x360) [27.2 MB] || The_Rough_Road_to_Space_512x288.mpg (512x288) [43.1 MB] || The_Rough_Road_to_Space_320x240.mp4 (320x180) [10.9 MB] || The_Rough_Road_to_Space.wmv (320x180) [14.6 MB] || ",
            "hits": 53
        },
        {
            "id": 10523,
            "url": "https://svs.gsfc.nasa.gov/10523/",
            "result_type": "Produced Video",
            "release_date": "2009-11-04T00:00:00-05:00",
            "title": "The Particle Puzzle",
            "description": "This short video, which is part of a seven part video podcast series about NASA's Glory mission, explores the complexity of small airborne particles called aerosols. Aerosols play a key role in the climate system, but they remain a terra incognito of sorts for climatologists because of challenges associated with measuring the ubiquitous particles.  Glory's Aerosol Polarimetery Sensor (APS), a unique instrument that measures the polarization of light as it scatters off the aerosols, offers a new and more accurate way to measure the perplexing particlesFor complete transcript, click here. || The_Particle_Puzzle_512x288.00452_print.jpg (1024x576) [97.2 KB] || The_Particle_Puzzle_512x288_web.png (320x180) [237.2 KB] || The_Particle_Puzzle_512x288_thm.png (80x40) [16.9 KB] || The_Particle_Puzzle_960x540_Apple_TV.webmhd.webm (960x540) [67.7 MB] || The_Particle_Puzzle_1280x720_ProRes.mov (1280x720) [5.0 GB] || The_Particle_Puzzle_1280x720_H264.mov (1280x720) [156.7 MB] || The_Particle_Puzzle_960x540_Apple_TV.m4v (960x540) [180.5 MB] || The_Particle_Puzzle_640x480_ipod.m4v (640x360) [55.3 MB] || The_Particle_Puzzle_512x288.mpg (512x288) [32.5 MB] || The_Particle_Puzzle_320x240.mp4 (320x180) [24.0 MB] || The_Particle_Puzzle.wmv (320x180) [33.5 MB] || ",
            "hits": 14
        },
        {
            "id": 10524,
            "url": "https://svs.gsfc.nasa.gov/10524/",
            "result_type": "Produced Video",
            "release_date": "2009-11-04T00:00:00-05:00",
            "title": "Glory's Suncatcher",
            "description": "The Sun's energy is one of the biggest forcings on Earth's climate, and for years satellites have measured total solar irradiance. Glory will continue collection of this critical climate data, which will contribute to the long-term climate record. The cutting edge TIM instrument will continue the work of NASA's SORCE mission. For complete transcript, click here. || Glorys_Suncatcher_512x288.00627_print.jpg (1024x576) [45.3 KB] || Glorys_Suncatcher_512x288_web.png (320x180) [150.8 KB] || Glorys_Suncatcher_512x288_thm.png (80x40) [15.2 KB] || Glorys_Suncatcher_960x540_AppleTV.webmhd.webm (960x540) [40.2 MB] || Glorys_Suncatcher_1280x720_ProRes.mov (1280x720) [3.2 GB] || Glorys_Suncatcher_1280x720_H264.mov (1280x720) [97.7 MB] || Glorys_Suncatcher_960x540_AppleTV.m4v (960x540) [107.5 MB] || Glorys_Suncatcher_640x480_ipod.m4v (640x360) [35.1 MB] || Glorys_Suncatcher_512x288.mpg (512x288) [36.1 MB] || Glorys_Suncatcher_320x240.mp4 (320x180) [14.3 MB] || Glorys_Suncatcher.wmv (320x180) [17.3 MB] || ",
            "hits": 14
        },
        {
            "id": 10525,
            "url": "https://svs.gsfc.nasa.gov/10525/",
            "result_type": "Produced Video",
            "release_date": "2009-11-04T00:00:00-05:00",
            "title": "Hello Crud",
            "description": "This segment provides an introduction to aerosols- their varied sources, brief lifetimes, and erratic behavior.  Glory's APS will help researchers determine the global distribution of aerosol particles.  This unique instrument will unravel the microphysical properties of aerosols, and will shed light on the chemical composition of natural and anthropogenic aerosols and clouds. For complete transcript, click here. || Hello_Crud__512x288.00727_print.jpg (1024x576) [58.9 KB] || Hello_Crud__512x288_web.png (320x180) [160.9 KB] || Hello_Crud__512x288_thm.png (80x40) [15.7 KB] || Hello_Crud_960x720_AppleTV.webmhd.webm (960x540) [66.8 MB] || Hello_Crud_1280x720_ProRes.mov (1280x720) [4.6 GB] || Hello_Crud_1280x720_H264.mov (1280x720) [128.2 MB] || Hello_Crud_960x720_AppleTV.m4v (960x540) [160.6 MB] || Hello_Crud__640x480_ipod.m4v (640x360) [52.5 MB] || Hello_Crud__512x288.mpg (512x288) [37.2 MB] || Hello_Crud_320x240.mp4 (320x180) [22.3 MB] || Hello_Crud.wmv (320x180) [32.7 MB] || ",
            "hits": 18
        },
        {
            "id": 10502,
            "url": "https://svs.gsfc.nasa.gov/10502/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "Climate Change and the Global Ocean",
            "description": "We know climate change can affect us, but does climate change alter something as vast, deep and mysterious as our oceans? For years, scientists have studied the world's oceans by sending out ships and divers, deploying data-gathering buoys, and by taking aerial measurements from planes. But one of the better ways to understand oceans is to gain an even broader perspective - the view from space. NASA's Earth observing satellites do more than just take pictures of our planet. High-tech sensors gather data, including ocean surface temperature, surface winds, sea level, circulation, and even marine life. Information the satellites obtain help us understand the complex interactions driving the world's oceans today - and gain valuable insight into how the impacts of climate change on oceans might affect us on dry land.For complete transcript, click here. || Global_Ocean_ipod_320x240.01252_print.jpg (1024x576) [77.3 KB] || Global_Ocean_ipod_320x240_web.png (320x180) [84.7 KB] || Global_Ocean_ipod_320x240_thm.png (80x40) [16.1 KB] || Global_Ocean_appletv.webmhd.webm (960x540) [78.2 MB] || Global_Ocean_broll_prores.mov (1280x720) [5.3 GB] || Global_Ocean_1280x720.mp4 (1280x720) [159.8 MB] || Global_Ocean_appletv.m4v (960x540) [187.1 MB] || Global_Ocean_H264_1280x720_30fps.mov (1280x720) [167.6 MB] || Global_Ocean_youtube_1280x720.mov (1280x720) [79.2 MB] || Global_Ocean_ipod_640x480.m4v (640x360) [59.9 MB] || Global_Ocean_ipod_320x240.m4v (320x180) [25.9 MB] || Global_Ocean.wmv (346x260) [39.1 MB] || ",
            "hits": 69
        },
        {
            "id": 10400,
            "url": "https://svs.gsfc.nasa.gov/10400/",
            "result_type": "Produced Video",
            "release_date": "2009-03-04T00:00:00-05:00",
            "title": "50 Years of Goddard",
            "description": "Pioneer rocket scientist Robert H. Goddard once said, 'It is difficult to say what is impossible, for the dream of yesterday is the hope of today and the reality of tomorrow.' Fifty years after its inception, NASA's Goddard Space Flight Center continues to live by these words, advancing science and engineering to new limits once thought impossible as it explores of the Earth, the sun, the solar system, and the universe. || ",
            "hits": 30
        },
        {
            "id": 10382,
            "url": "https://svs.gsfc.nasa.gov/10382/",
            "result_type": "Produced Video",
            "release_date": "2009-02-19T00:00:00-05:00",
            "title": "Glory Solar Array Deployment",
            "description": "The Glory spacecraft uses Orbital Sciences Corporation Space Systems Group's LEOStar-1 bus design, with deployable, four-panel solar arrays. This conceptual animation reveals Glory's unique solar array deployment sequence. || ",
            "hits": 48
        },
        {
            "id": 10383,
            "url": "https://svs.gsfc.nasa.gov/10383/",
            "result_type": "Produced Video",
            "release_date": "2009-02-19T00:00:00-05:00",
            "title": "Glory Instrument Flyover",
            "description": "Glory will help researchers better understand the direct and indirect effects of atmospheric aerosols and of the Sun on Earth's climate. This animation reveals Glory's trio of remote-sensing instruments:  Aerosol Polarimetry Sensor (APS) will provide new capabilities in the characterization of aerosol particle microphysical properties through the collection of multiangle and multispectral radiance and polarization measurements. Total Irradiance Monitor (TIM) is an electrical substitution radiometer (ESR) that records measurements of total solar irradiance (TSI) with extreme accuracy and precision. Cloud Camera data will provide cross track coverage over a broader swath of aerosol load than the APS. || ",
            "hits": 2718
        },
        {
            "id": 10384,
            "url": "https://svs.gsfc.nasa.gov/10384/",
            "result_type": "Produced Video",
            "release_date": "2009-02-19T00:00:00-05:00",
            "title": "Glory's Total Irradiance Monitor (TIM)",
            "description": "The Total Irradiance Monitor (TIM) is an electrical substitution radiometer (ESR) that measures total solar irradiance (TSI) with extreme accuracy and precision. It has four identical radiometers to provide redundancy and to detect changes in the instrument performance due to exposure to solar radiation. As illustrated by this animation, the TIM is mounted on a two-axis, gimbaled platform that tracks the Sun independent of spacecraft orientation. The Glory TIM will continue the TSI measurements currently being acquired by the TIM instrument on the NASA SORCE satellite, in orbit since 2003. || ",
            "hits": 22
        },
        {
            "id": 10379,
            "url": "https://svs.gsfc.nasa.gov/10379/",
            "result_type": "Produced Video",
            "release_date": "2009-02-18T00:00:00-05:00",
            "title": "Glory Launch Sequence",
            "description": "Glory will launch from Vandenberg Air Force Base onboard a Taurus XL launch vehicle. The Taurus launch service is provided by Orbital Sciences Corporation Launch Systems Group, under contract to the NASA Kennedy Space Center. The Taurus XL will place Glory into a circular, Sun-synchronous injection orbit with an altitude of 640 kilometers and an inclination of 97.9 degrees. || ",
            "hits": 21
        },
        {
            "id": 10380,
            "url": "https://svs.gsfc.nasa.gov/10380/",
            "result_type": "Produced Video",
            "release_date": "2009-02-18T00:00:00-05:00",
            "title": "Two Glory Beauty Passes",
            "description": "The Glory spacecraft uses Orbital Sciences Corporation Space Systems Group's LEOStar-1 bus design, with deployable solar arrays, 3-axis stabilization, and X-band/S-band RF communications capabilities. The structure consists of an octagonal aluminum space frame and a hydrazine propulsion module containing enough fuel to support initial orbit raising and at least 36 months of on-orbit service. The spacecraft bus also provides payload power; command, telemetry, and science data interfaces, including onboard storage of data; and an attitude control subsystem to support instrument pointing requirements. Two animated beauty passes reveal different perspectives of the spacecraft in orbit. || ",
            "hits": 33
        },
        {
            "id": 10333,
            "url": "https://svs.gsfc.nasa.gov/10333/",
            "result_type": "Produced Video",
            "release_date": "2008-08-13T00:00:00-04:00",
            "title": "The Cloud Makers",
            "description": "This segment provides an introduction to aerosols- their varied sources, brief lifetimes, and erratic behavior.  Glory's APS will help researchers determine the global distribution of aerosol particles.  This unique instrument will unravel the microphysical properties of aerosols, and will shed light on the chemical composition of natural and anthropogenic aerosols and clouds. For complete transcript, click here. || The_Cloud_Makers_512x28800502_print.jpg (1024x576) [80.6 KB] || The_Cloud_Makers_512x288_web.png (320x180) [235.4 KB] || The_Cloud_Makers_512x288_thm.png (80x40) [16.9 KB] || The_Cloud_Makers_960x540_AppleTV.webmhd.webm (960x540) [45.0 MB] || The_Cloud_Makers_1280x720_ProRes.mov (1280x720) [3.0 GB] || The_Cloud_Makers_1280x720_H264.mov (1280x720) [90.7 MB] || The_Cloud_Makers_960x540_AppleTV.m4v (960x540) [109.4 MB] || The_Cloud_Makers_640x480.m4v (640x360) [35.4 MB] || The_Cloud_Makers_512x288.mpg (512x288) [35.7 MB] || The_Cloud_Makers_320x240.mp4 (320x180) [14.7 MB] || The_Cloud_Makers.wmv (320x180) [21.0 MB] || ",
            "hits": 28
        },
        {
            "id": 10198,
            "url": "https://svs.gsfc.nasa.gov/10198/",
            "result_type": "Produced Video",
            "release_date": "2008-05-07T00:00:00-04:00",
            "title": "Striking a Solar Balance",
            "description": "This short film explores the vital connection between the Earth and the Sun.  NASA's Glory mission and the Total Irradiance Monitor will continue nearly three decades of solar irradiance measurments.  This crucial data will contribute to the long-term climate record.For complete transcript, click here. || Striking_a_Solar_Balance_640x48001227_print.jpg (1024x768) [110.2 KB] || Striking_a_Solar_Balance_640x480_web.png (320x240) [213.2 KB] || Striking_a_Solar_Balance_640x480_thm.png (80x40) [13.1 KB] || Striking_a_Solar_Balance_640x480_searchweb.png (320x180) [84.5 KB] || Striking_a_Solar_Balance_720x486_ProRes.webmhd.webm (960x540) [44.9 MB] || Striking_a_Solar_Balance_640x480.mpg (640x480) [118.9 MB] || Striking_a_Solar_Balance_720x486_ProRes.mov (720x486) [972.5 MB] || Striking_a_Solar_Balance_640x480_H264.mov (720x486) [171.0 MB] || Striking_a_Solar_Balance_640x480.m4v (640x480) [39.9 MB] || Striking_a_Solar_Balance_320x240.mp4 (320x240) [17.5 MB] || Striking_a_Solar_Balance.wmv (346x260) [30.4 MB] || ",
            "hits": 323
        },
        {
            "id": 20118,
            "url": "https://svs.gsfc.nasa.gov/20118/",
            "result_type": "Animation",
            "release_date": "2007-09-10T00:00:00-04:00",
            "title": "The Solar Dynamics Observatory (SDO)",
            "description": "SDO is designed to help us understand the Sun's influence on Earth and Near-Earth space by studying the solar atmosphere on small scales of space and time and in many wavelengths simultaneously. || ",
            "hits": 77
        }
    ]
}