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    "results": [
        {
            "id": 11382,
            "url": "https://svs.gsfc.nasa.gov/11382/",
            "result_type": "Produced Video",
            "release_date": "2013-10-30T10:00:00-04:00",
            "title": "Five Years of Great Discoveries for NASA's IBEX",
            "description": "Launched on Oct. 19, 2008, the Interstellar Boundary Explorer, or IBEX, spacecraft, is unique to NASA's heliophysics fleet: it images the outer boundary of the heliosphere, a boundary at the furthest edges of the solar system, far past the planets, some 8 million miles away. There, the constant stream of solar particles flowing off the sun, the solar wind, pushes up against the interstellar material flowing in from the local galactic neighborhood.IBEX is also different because it creates images from particles instead of light. IBEX, scientists create maps from the observed neutral atoms. Some are of non-solar origin, others were created by collisions of solar wind particles with other neutral atoms far from the sun. Observing where these energetic neutral atoms, or ENAs, come from describes what's going on in these distant regions. Over the course of six months and many orbits around Earth, IBEX can paint a picture of the entire sky in ENAs.During its first five years, IBEX has made some astounding discoveries.IBEX is a NASA Heliophysics Small Explorer mission. The Southwest Research Institute in San Antonio, Texas, leads IBEX with teams of national and international partners. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the Explorers Program for the agency's Science Mission Directorate in Washington. || ",
            "hits": 59
        },
        {
            "id": 11379,
            "url": "https://svs.gsfc.nasa.gov/11379/",
            "result_type": "Produced Video",
            "release_date": "2013-10-24T10:00:00-04:00",
            "title": "Filament Eruption Creates 'Canyon of Fire' on the Sun",
            "description": "A magnetic filament of solar material erupted on the sun in late September, breaking the quiet conditions in a spectacular fashion. The 200,000 mile long filament ripped through the sun's atmosphere, the corona, leaving behind what looks like a canyon of fire. The glowing canyon traces the channel where magnetic fields held the filament aloft before the explosion. Visualizers at NASA's Goddard Space Flight Center in Greenbelt, Md. combined two days of satellite data to create a short movie of this gigantic event on the sun.In reality, the sun is not made of fire, but of something called plasma: particles so hot that their electrons have boiled off, creating a charged gas that is interwoven with magnetic fields. These images were captured on Sept. 29-30, 2013, by NASA's Solar Dynamics Observatory, or SDO, which constantly observes the sun in a variety of wavelengths. Different wavelengths help capture different aspect of events in the corona. The red images shown in the movie help highlight plasma at temperatures of 90,000° F and are good for observing filaments as they form and erupt. The yellow images, showing temperatures at 1,000,000° F, are useful for observing material coursing along the sun's magnetic field lines, seen in the movie as an arcade of loops across the area of the eruption. The browner images at the beginning of the movie show material at temperatures of 1,800,000° F, and it is here where the canyon of fire imagery is most obvious. By comparing this with the other colors, one sees that the two swirling ribbons moving farther away from each other are, in fact, the footprints of the giant magnetic field loops, which are growing and expanding as the filament pulls them upward. || ",
            "hits": 274
        },
        {
            "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": 21
        },
        {
            "id": 11007,
            "url": "https://svs.gsfc.nasa.gov/11007/",
            "result_type": "Produced Video",
            "release_date": "2012-06-20T15:00:00-04:00",
            "title": "Space Shuttle Discovery Comes to Dulles",
            "description": "On April 17, 2012 the space shuttle Discovery hitched a ride on the back of a 747 jumbo jet especially designed as a space shuttle transport. It landed at Dulles Airport in Washington, DC, and the process to deliver Discovery to its new home at the Steven F. Udvar-Hazy Center got under way. Through the eyes of a veteran NASA tour guide and aficionado, DJ Emmanuel, we get a behind-the-scenes view of what it was like to be there on such an historic and exciting day! || ",
            "hits": 24
        },
        {
            "id": 10995,
            "url": "https://svs.gsfc.nasa.gov/10995/",
            "result_type": "Produced Video",
            "release_date": "2012-05-30T00:00:00-04:00",
            "title": "Goddard Spring Interns 2012",
            "description": "Ever wonder what it's like to be part of a NASA team? Well, three student interns have been given the opportunity of a lifetime. They were asked to create a major component for the Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII) mission. Principal Investigator Stephen Rinehart mentored the students and gave them the freedom to be creative in making a star camera, which will study star birth in deep space. || ",
            "hits": 21
        },
        {
            "id": 10858,
            "url": "https://svs.gsfc.nasa.gov/10858/",
            "result_type": "Produced Video",
            "release_date": "2011-11-03T14:00:00-04:00",
            "title": "Fermi Discovers Youngest Millisecond Pulsar",
            "description": "An international team of scientists using NASA's Fermi Gamma-ray Space Telescope has discovered a surprisingly powerful millisecond pulsar that challenges existing theories about how these objects form. At the same time, another team has exploited improved analytical techniques to locate nine new gamma-ray pulsars in Fermi data.A pulsar, also called a neutron star, is the closest thing to a black hole astronomers can observe directly, crushing half a million times more mass than Earth into a sphere no larger than a city. This matter is so compressed that even a teaspoonful weighs as much as Mount Everest.Typically, millisecond pulsars are a billion years or more old, ages commensurate with a stellar lifetime. But in the Nov. 3 issue of Science, the Fermi team reveals a bright, energetic millisecond pulsar only 25 million years old.The object, named PSR J1823—3021A, lies within NGC 6624, a spherical assemblage of ancient stars called a globular cluster, one of about 160 similar objects that orbit our galaxy. The cluster is about 10 billion years old and lies about 27,000 light-years away toward the constellation Sagittarius.\"With this new batch of pulsars, Fermi now has detected more than 100, which is an exciting milestone when you consider that before Fermi's launch only seven of them were known to emit gamma rays,\" said Pablo Saz Parkinson, an astrophysicist at the Santa Cruz Institute for Particle Physics, University of California Santa Cruz. || ",
            "hits": 185
        },
        {
            "id": 10861,
            "url": "https://svs.gsfc.nasa.gov/10861/",
            "result_type": "Produced Video",
            "release_date": "2011-11-03T14:00:00-04:00",
            "title": "Fermi Pulsar Interactive Videos",
            "description": "These videos originally accompanied a Fermi Pulsar Interactive.  That interactive is now available here. || ",
            "hits": 151
        },
        {
            "id": 10804,
            "url": "https://svs.gsfc.nasa.gov/10804/",
            "result_type": "Produced Video",
            "release_date": "2011-10-27T08:00:00-04:00",
            "title": "The Solar Cycle",
            "description": "The number of sunspots increases and decreases over time in a regular, approximately 11-year cycle, called the sunspot cycle. The exact length of the cycle can vary. It has been as short as eight years and as long as fourteen, but the number of sunspots always increases over time, and then returns to low again. More sunspots mean increased solar activity, when great blooms of radiation known as solar flares or bursts of solar material known as coronal mass ejections (CMEs) shoot off the sun's surface. The highest number of sun spots in any given cycle is designated \"solar maximum,\" while the lowest number is designated \"solar minimum.\" Each cycle, varies dramatically in intensity, with some solar maxima being so low as to be almost indistinguishable from the preceding minimum. Sunspots are a magnetic phenomenon and the entire sun is magnetized with a north and a south magnetic pole just like a bar magnet. The comparison to a simple bar magnet ends there, however, as the sun's interior is constantly on the move. By tracking sound waves that course through the center of the sun, an area of research known as helioseismology, scientists can gain an understanding of what's deep inside the sun. They have found that the magnetic material inside the sun is constantly stretching, twisting, and crossing as it bubbles up to the surface. The exact pattern of movements is not conclusively mapped out, but over time they eventually lead to the poles reversing completely. The sunspot cycle happens because of this poles flip — north becomes south and south becomes north—approximately every 11 years. Some 11 years later, the poles reverse again back to where they started, making the full solar cycle actually a 22-year phenomenon. The sun behaves similarly over the course of each 11-year cycle no matter which pole is on top, however, so this shorter cycle tends to receive more attention. || ",
            "hits": 785
        },
        {
            "id": 10809,
            "url": "https://svs.gsfc.nasa.gov/10809/",
            "result_type": "Produced Video",
            "release_date": "2011-08-18T13:00:00-04:00",
            "title": "NASA Spacecraft Track Solar Storms From Sun To Earth",
            "description": "NASA's STEREO spacecraft and new data processing techniques have succeeded in tracking space weather events from their origin in the Sun's ultrahot corona to impact with the Earth 93 million miles away, resolving a 40-year mystery about the structure of the structures that cause space weather: how the structures that impact the Earth relate to the corresponding structures in the solar corona.Despite many instruments that monitor the Sun and a fleet of near-earth probes, the connection between near-Earth disturbances and their counterparts on the Sun has been obscure, because CMEs and the solar wind evolve and change during the 93,000,000 mile journey from the Sun to the Earth.STEREO includes \"heliospheric imager\" cameras that monitor the sky at large angles from the Sun, but the starfield and galaxy are 1,000 times brighter than the faint rays of sunlight reflected by free-floating electron clouds inside CMEs and the solar wind; this has made direct imaging of these important structures difficult or impossible, and limited understanding of the connection between space storms and the coronal structures that cause them.Newly released imagery reveals absolute brightness of detailed features in a large geoeffective CME in late 2008, connecting the original magnetized structure in the Sun's corona to the intricate anatomy of an interplanetary storm as it impacted the Earth three days later. At the time the data were collected, in late 2008, STEREO-A was nearly 45 degrees ahead of the Earth in its orbit, affording a very clear view of the Earth-Sun line.For the press conference Visual 1, a visualization of the STEREO orbits and the 2008 CME, go here.For Visual 7, a CME and reconnection animation, go here.For Visual 8, footage of the October 2003 solar storms, go here. || ",
            "hits": 135
        },
        {
            "id": 10109,
            "url": "https://svs.gsfc.nasa.gov/10109/",
            "result_type": "Produced Video",
            "release_date": "2011-08-09T10:00:00-04:00",
            "title": "X-Class: A Guide to Solar Flares",
            "description": "Flares happen when the powerful magnetic fields in and around the sun reconnect. They're usually associated with active regions, often seen as sun spots, where the magnetic fields are strongest. Flares are classified according to their strength. The smallest ones are B-class, followed by C, M and X, the largest. Similar to the Richter scale for earthquakes, each letter represents a ten-fold increase in energy output. So an X is 10 times an M and 100 times a C. Within each letter class, there is a finer scale from 1 to 9. C-class flares are too weak to noticeably affect Earth. M-class flares can cause brief radio blackouts at the poles and minor radiation storms that might endanger astronauts. Although X is the last letter, there are flares more than 10 times the power of an X1, so X-class flares can go higher than 9. The most powerful flare on record was in 2003, during the last solar maximum. It was so powerful that it overloaded the sensors measuring it. They cut-out at X17, and the flare was later estimated to be about X45. A powerful X-class flare like that can create long lasting radiation storms, which can harm satellites and even give airline passengers, flying near the poles, small radiation doses. X flares also have the potential to create global transmission problems and world-wide blackouts. || ",
            "hits": 3575
        },
        {
            "id": 10799,
            "url": "https://svs.gsfc.nasa.gov/10799/",
            "result_type": "Produced Video",
            "release_date": "2011-06-30T00:00:00-04:00",
            "title": "MicroSpec: Revolutionary Instrument on a Chip",
            "description": "Scientists may finally get a glimpse at our adolescent universe from a revolutionary new technology being developed at NASA's Goddard Space Flight Center. An instrument on a chip. This new, potentially game-changing instrument, called MicroSpec, is a far-infrared spectrometer that will be 10,000 times more sensitive and infinitely smaller than it's predecessor. || ",
            "hits": 31
        },
        {
            "id": 10790,
            "url": "https://svs.gsfc.nasa.gov/10790/",
            "result_type": "Produced Video",
            "release_date": "2011-06-09T12:00:00-04:00",
            "title": "Voyager Satellites Find Magnetic Bubbles at Edge of Solar System",
            "description": "The sun's magnetic field spins opposite directions on the north and south poles. These oppositely pointing magnetic fields are separated by a layer of current called the heliospheric current sheet. Due to the tilt of the magnetic axis in relation to the axis of rotation of the Sun, the heliospheric current sheet flaps like a flag in the wind. The flapping current sheet separates regions of oppositely pointing magnetic field, called sectors. As the solar wind speed decreases past the termination shock, the sectors squeeze together, bringing regions of opposite magnetic field closer to each other. The Voyager spacecraft have now found that when the separation of sectors becomes very small, the sectored magnetic field breaks up into a sea of nested \"magnetic bubbles\" in a phenomenon called magnetic reconnection. The region of nested bubbles is carried by the solar wind to the north and south filling out the entire front region of the heliopause and the sector region in the heliosheath.This discovery has prompted a complete revision of what the heliosheath region looks like. The smooth, streamlined look is gone, replaced with a bubbly, frothy outer layer. More animations about the Voyager magnetic bubbles discovery are available. || ",
            "hits": 168
        },
        {
            "id": 10745,
            "url": "https://svs.gsfc.nasa.gov/10745/",
            "result_type": "Produced Video",
            "release_date": "2011-06-07T09:00:00-04:00",
            "title": "SDO Catches Surf Waves on the Sun",
            "description": "Scientists have spotted the iconic surfer's wave rolling through the atmosphere of the sun. This makes for more than just a nice photo-op: the waves hold clues as to how energy moves through that atmosphere, known as the corona. Since scientists know how these kinds of waves — initiated by a Kelvin-Helmholtz instability if you're being technical — disperse energy in the water, they can use this information to better understand the corona. This in turn, may help solve an enduring mystery of why the corona is thousands of times hotter than originally expected.Kelvin-Helmholtz instabilities occur when two fluids of different densities or different speeds flow by each other. In the case of ocean waves, that's the dense water and the lighter air. As they flow past each other, slight ripples can be quickly amplified into the giant waves loved by surfers. In the case of the solar atmosphere, which is made of a very hot and electrically charged gas called plasma, the two flows come from an expanse of plasma erupting off the sun's surface as it passes by plasma that is not erupting. The difference in flow speeds and densities across this boundary sparks the instability that builds into the waves. In order to confirm this description, the team developed a computer model to see what takes place in the region. Their model showed that these conditions could indeed lead to giant surfing waves rolling through the corona. Seeing the big waves suggests they can cascade down to smaller forms of turbulence too. Scientists believe that the friction created by turbulence — the simple rolling of material over and around itself — could help add heating energy to the corona. The analogy is the way froth at the top of a surfing wave provides friction that will heat up the wave. || ",
            "hits": 49
        },
        {
            "id": 10770,
            "url": "https://svs.gsfc.nasa.gov/10770/",
            "result_type": "Produced Video",
            "release_date": "2011-05-20T09:00:00-04:00",
            "title": "Radio Telescopes Capture Best-Ever Snapshot of a Black Hole's Jets",
            "description": "Centaurus A is a giant elliptical active galaxy 12 million light years away. Radio and X-ray images reveal features associated with jets emanating from near the galaxy's central supermassive black hole, which has a mass of 55 million suns. Now, the TANAMI project has provided the best-ever view of these jets. In the radio image of the galaxy's core, the black hole is invisible but the jets show in great detail. Features as small as 15 light-days across can be resolved. The powerful jets feed vast lobes of radio-emitting gas that reach far beyond the visible galaxy. || ",
            "hits": 79
        },
        {
            "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": 121
        },
        {
            "id": 10772,
            "url": "https://svs.gsfc.nasa.gov/10772/",
            "result_type": "Produced Video",
            "release_date": "2011-05-06T00:00:00-04:00",
            "title": "Goddard's Global Impact 2010",
            "description": "With over fifty years of service, NASA's Goddard Space Flight Center has had, and will continue to have, an immeasurable global impact in our understanding of our Earth and its place in the universe. It is a vital player in national economics, infusing its budget into state and local economies with powerful results. || ",
            "hits": 7
        },
        {
            "id": 10747,
            "url": "https://svs.gsfc.nasa.gov/10747/",
            "result_type": "Produced Video",
            "release_date": "2011-04-28T09:00:00-04:00",
            "title": "Swift and Hubble Probe an Asteroid Crash",
            "description": "Late last year, astronomers noticed that an asteroid named Scheila had unexpectedly brightened and it was sporting short-lived plumes. Data from NASA's Swift satellite and Hubble Space Telescope show that these changes likely occurred after Scheila was struck by a much smaller asteroid. On Dec. 11, 2010, images from the University of Arizona's Catalina Sky Survey, a project of NASA's Near Earth Object Observations Program, revealed the Scheila to be twice as bright as expected and immersed in a faint comet-like glow. Looking through the survey's archived images, astronomers inferred the outburst began between Nov. 11 and Dec. 3. Three days after the outburst was announced, Swift's Ultraviolet/Optical Telescope (UVOT) captured multiple images and a spectrum of the asteroid. Ultraviolet sunlight breaks up the gas molecules surrounding comets; water, for example, is transformed into hydroxyl (OH) and hydrogen (H). But none of the emissions most commonly identified in comets — such as hydroxyl or cyanogen (CN) — show up in the UVOT spectrum. The absence of gas around Scheila led the Swift team to reject scenarios where exposed ice accounted for the activity.Images show the asteroid was flanked in the north by a bright dust plume and in the south by a fainter one. The dual plumes formed as small dust particles excavated by the impact were pushed away from the asteroid by sunlight. Hubble observed the asteroid's fading dust cloud on Dec. 27, 2010, and Jan. 4, 2011.The two teams found the observations were best explained by a collision with a small asteroid impacting Scheila's surface at an angle of less than 30 degrees, leaving a crater 1,000 feet across. Laboratory experiments show a more direct strike probably wouldn't have produced two distinct dust plumes. The researchers estimated the crash ejected more than 660,000 tons of dust—equivalent to nearly twice the mass of the Empire State Building.For the collision animation go to #10759. || ",
            "hits": 90
        },
        {
            "id": 10718,
            "url": "https://svs.gsfc.nasa.gov/10718/",
            "result_type": "Produced Video",
            "release_date": "2011-02-06T10:00:00-05:00",
            "title": "STEREO Sun360",
            "description": "Launched in October 2006, STEREO traces the flow of energy and matter from the sun to Earth. It also provides unique and revolutionary views of the sun-Earth system. The mission observed the sun in 3-D for the first time in 2007. In 2009, the twin spacecraft revealed the 3-D structure of coronal mass ejections which are violent eruptions of matter from the sun that can disrupt communications, navigation, satellites and power grids on Earth.Seeing?the whole sun front and back simultaneously will enable significant advances in space weather forecasting for Earth and for planning for future robotic and manned spacecraft missions throughout the solar system.These views are the result of observations by NASA's two Solar TErrestrial Relations Observatory (STEREO) spacecraft. The duo are on diametrically opposite sides of the sun, 180 degrees apart. One is ahead of Earth in its orbit, the other trailing behind.For the STEREO Sun360 Teaser, go here.For the full visualization showing STEREO's path go here.For the visualization showing STEREO's increasing coverage of the sun (visual 3) go here.For animations from the STEREO Teaser and stages of coverage, go here.For animations showing STEREO's 3D coverage of a CME go here. || ",
            "hits": 75
        },
        {
            "id": 10698,
            "url": "https://svs.gsfc.nasa.gov/10698/",
            "result_type": "Produced Video",
            "release_date": "2011-01-20T09:00:00-05:00",
            "title": "NASA's Swift Finds 'Missing' Active Galaxies",
            "description": "Most large galaxies contain a giant central black hole. In an active galaxy, matter falling toward the supermassive black hole powers high-energy emissions so intense that two classes of active galaxies, quasars and blazars, rank as the most luminous objects in the universe. Thick clouds of dust and gas near the central black hole screens out ultraviolet, optical and low-energy (or soft) X-ray light. Although there are many different types of active galaxy, astronomers explain the different observed properties based on how the galaxy angles into our line of sight. We view the brightest ones nearly face on, but as the angle increases, the surrounding ring of gas and dust absorbs increasing amounts of the black hole's emissions. || ",
            "hits": 157
        },
        {
            "id": 10708,
            "url": "https://svs.gsfc.nasa.gov/10708/",
            "result_type": "Produced Video",
            "release_date": "2011-01-12T12:00:00-05:00",
            "title": "A Flickering X-ray Candle",
            "description": "The Crab Nebula, created by a supernova seen nearly a thousand years ago, is one of the sky's most famous \"star wrecks.\" For decades, most astronomers have regarded it as the steadiest beacon at X-ray energies, but data from orbiting observatories show unexpected variations, showing astronomers their hard X-ray \"standard candle\" isn't as steady as they once thought. From 1999 to 2008, the Crab brightened and faded by as much as 3.5 percent a year, and since 2008, it has faded by 7 percent. The Gamma-ray Burst Monitor on NASA's Fermi satellite first detected the decline, and Fermi's Large Area Telescope also spotted two gamma-ray flares at even higher energies. Scientists think the X-rays reveal processes deep within the nebula, in a region powered by a rapidly spinning neutron star — the core of the star that blew up. But figuring out exactly where the Crab's X-rays are changing over the long term will require a new generation of X-ray telescopes. || ",
            "hits": 81
        },
        {
            "id": 10706,
            "url": "https://svs.gsfc.nasa.gov/10706/",
            "result_type": "Produced Video",
            "release_date": "2011-01-10T16:00:00-05:00",
            "title": "Terrestrial Gamma-ray Flashes Create Antimatter",
            "description": "NASA's Fermi Gamma-ray Space Telescope has detected beams of antimatter launched by thunderstorms. Acting like enormous particle accelerators, the storms can emit gamma-ray flashes, called TGFs, and high-energy electrons and positrons. Scientists now think that most TGFs produce particle beams and antimatter.For additional animations showing bremsstrahlung and pair production gamma ray reactions, go here.For more visualizations showing Fermi's TGF detections, go to#3747, #3748, and #3756.For animations of the Fermi spacecraft and matter/antimatter, go to#10707 and #10651. || ",
            "hits": 274
        },
        {
            "id": 10636,
            "url": "https://svs.gsfc.nasa.gov/10636/",
            "result_type": "Produced Video",
            "release_date": "2010-10-27T12:00:00-04:00",
            "title": "ARTEMIS Orbits Magnetic Moon",
            "description": "Launched in 2007, NASA's five THEMIS spacecraft have now successfully completed their 2 year mission to determine the cause of geomagnetic substorms. Because they are continuing to work perfectly, NASA is re-directing the outermost two spacecraft to special orbits at and around the Moon. This new mission, which is called ARTEMIS, uses some very complex maneuvers over two years (2009-2010) to get both spacecraft into position. As the Moon orbits the Earth, it passes in and out of the Earth's magnetic field and the million-mile per hour stream of particles emitted by the Sun known as the solar wind. While in these regions, the two ARTEMIS spacecraft will seek evidence for turbulence, particle acceleration, and magnetic reconnection, three fundamental phenomena that control the nature of the solar wind's interaction with the Earth's magnetosphere. Employing their full complement of instruments and unique two-point vantage points, the spacecraft will study the vacuum the Moon carves out in the solar wind, and the processes that eventually fill this lunar wake. Nearer the Moon, they will observe the effects of surface electric fields, ions sputtered off the lunar surface, and determine the internal structure of the Moon from transient variations in its magnetic field induced by external changes.Also available are the complete, unedited visualization and frames. || ",
            "hits": 72
        },
        {
            "id": 10635,
            "url": "https://svs.gsfc.nasa.gov/10635/",
            "result_type": "Produced Video",
            "release_date": "2010-09-23T09:00:00-04:00",
            "title": "Dust Simulations Paint Alien's View of the Solar System",
            "description": "Dust ground off icy bodies in the Kuiper Belt, the cold-storage zone that includes Pluto and millions of other objects, creates a faint infrared disk potentially visible to alien astronomers looking for planets around the sun. Neptune's gravitational imprint on the dust is always detectable in new simulations of how this dust moves through the solar system. By ramping up the collision rate, the simulations show how the distant view of the solar system might have changed over its history. More here. || ",
            "hits": 152
        },
        {
            "id": 10535,
            "url": "https://svs.gsfc.nasa.gov/10535/",
            "result_type": "Produced Video",
            "release_date": "2010-05-18T09:00:00-04:00",
            "title": "SDO: Commissioning and Handover",
            "description": "In order to provide the clearest scientific data for its entire 5 year mission, SDO had to undergo a rigorous, 2 month testing phase. After giving it an all-clear, the team of people who designed, built and tested the satellite now have to say goodbye as they hand it over to the scientists who will begin collecting data. || ",
            "hits": 16
        },
        {
            "id": 10577,
            "url": "https://svs.gsfc.nasa.gov/10577/",
            "result_type": "Produced Video",
            "release_date": "2010-02-25T00:00:00-05:00",
            "title": "Marco Midon - Black History Month",
            "description": "Marco Midon, who is visually impaired, is highlighted for NASA's Black History Month. He is the Lead Systems Engineer who oversees the design and implementation of NASA ground stations in the area of radio frequencies. Working with new, higher data-rate dishes at White Sands in New Mexico, he was instrumental in two successfully launched NASA missions - the Solar Dynamics Observatory (SDO) and the Lunar Reconnaissance Orbiter (LRO). He is also the Lead Systems Engineer for the new ground station at the McMurdo Station in Antarctica. His work continues in updating compatibility equipment testing for the next generation of vehicles and spacecraft. || ",
            "hits": 25
        },
        {
            "id": 10574,
            "url": "https://svs.gsfc.nasa.gov/10574/",
            "result_type": "Produced Video",
            "release_date": "2010-02-22T00:00:00-05:00",
            "title": "Piecing Together the Temperature Puzzle",
            "description": "The decade from 2000 to 2009 was the warmest in the modern record. \"Piecing Together the Temperature Puzzle\" illustrates how NASA satellites enable us to study possible causes of climate change. The video explains what role fluctuations in the solar cycle, changes in snow and cloud cover, and rising levels of heat-trapping gases may play in contributing to climate change. For complete transcript, click here. || Temperature_Puzzle_fullres.01252_print.jpg (1024x576) [113.2 KB] || Temperature_Puzzle_fullres_web.png (320x180) [207.8 KB] || Temperature_Puzzle_fullres_thm.png (80x40) [16.9 KB] || Temperature_Puzzle_AppleTV.webmhd.webm (960x540) [83.9 MB] || Temperature_Puzzle_fullres.mov (1280x720) [166.2 MB] || Temperature_Puzzle_AppleTV.m4v (960x720) [211.4 MB] || Temperature_Puzzle__Youtube.mov (1280x720) [87.7 MB] || Temperature_Puzzle_iPod_small.m4v (640x360) [67.9 MB] || Temperature_Puzzle_iPod_large.m4v (320x180) [27.9 MB] || Temperature_Puzzle_svs.mpg (512x288) [136.6 MB] || Temperature_Puzzle_portal.wmv (346x260) [38.8 MB] || ",
            "hits": 104
        },
        {
            "id": 10575,
            "url": "https://svs.gsfc.nasa.gov/10575/",
            "result_type": "Produced Video",
            "release_date": "2010-02-22T00:00:00-05:00",
            "title": "GOES-P: Mission Overview Video",
            "description": "GOES-P is set to launch in 2010. It will be the last in an improved series of satellites that has helped forecast the development of severe weather for 35 years. Operated by NOAA and launched by NASA, GOES-P will continue providing critical data used for real-time weather prediction on Earth as well as space weather events, and search and rescue efforts. || ",
            "hits": 14
        },
        {
            "id": 10557,
            "url": "https://svs.gsfc.nasa.gov/10557/",
            "result_type": "Produced Video",
            "release_date": "2010-01-21T12:00:00-05:00",
            "title": "2009 Global Temperature Package: Year Tied as Second Hottest",
            "description": "Reporters package style video about the new 2009 global temperature data. Scientists at the Goddard Institute for Space Science found that 2009 was tied as the second hottest year ever recorded.For complete transcript, click here. || G2010-004_Global_Temp_2009-H.264_for_iPod_video_and_iPhone_640x480.00302_print.jpg (1024x576) [104.3 KB] || G2010-004_Global_Temp_2009-H.264_for_iPod_video_and_iPhone_640x480_web.png (320x180) [104.3 KB] || G2010-004_Global_Temp_2009-H.264_for_iPod_video_and_iPhone_640x480_thm.png (80x40) [12.0 KB] || G2010-004_Global_Temp_2009-H.264_for_Apple_TV.webmhd.webm (960x540) [37.9 MB] || G2010-004_Global_Temp_2009_1280x720_ProRes.mov (1280x720) [2.6 GB] || G2010-004_Global_Temp_2009-H.264_1280x720_@30fps.mov (1280x720) [85.5 MB] || G2010-004_Global_Temp_2009-720_H.264_QT_for_16x9_Youtube.mov (1280x720) [37.9 MB] || G2010-004_Global_Temp_2009-H.264_for_Apple_TV.m4v (960x720) [92.0 MB] || G2010-004_Global_Temp_2009-H.264_for_iPod_video_and_iPhone_640x480.m4v (640x360) [27.3 MB] || G2010-004_Global_Temp_2009-MPEG1_512x288.mpg (512x288) [23.2 MB] || G2010-004_Global_Temp_2009-H.264_for_iPod_video_and_iPhone_320x240_QVGA.m4v (320x180) [10.8 MB] || G2010-004_Global_Temp_2009_WMVHQ_346x260_16_9.wmv (346x260) [25.2 MB] || ",
            "hits": 33
        },
        {
            "id": 10514,
            "url": "https://svs.gsfc.nasa.gov/10514/",
            "result_type": "Produced Video",
            "release_date": "2009-12-11T18:00:00-05:00",
            "title": "Terra@10: Terra 10th Anniversary Video",
            "description": "The Earth-observing satellite Terra celebrates its tenth anniversary in 2009. This video highlights how Terra has helped us better understand our home planet. The satellite's five instruments - ASTER, CERES, MISR, MODIS and MOPITT - reveal how our our world is changing. For complete transcript, click here. || Terra10_ipodlarge.08402_print.jpg (1024x576) [38.3 KB] || Terra10_ipodlarge_web.png (320x180) [47.8 KB] || Terra10_ipodlarge_thm.png (80x40) [4.3 KB] || Terra10_Apple_TV.webmhd.webm (960x540) [71.4 MB] || Terra10_Youtube.mov (1280x720) [72.8 MB] || Terra10_Apple_TV.m4v (960x720) [179.0 MB] || Terra10_H.264.mov (1280x720) [146.6 MB] || Terra10_ipodlarge.m4v (640x360) [55.7 MB] || Terra10.mpg (512x288) [118.8 MB] || Terra10_ipodsmall.m4v (320x180) [24.0 MB] || Terra10.wmv (346x260) [18.2 MB] || ",
            "hits": 18
        },
        {
            "id": 10537,
            "url": "https://svs.gsfc.nasa.gov/10537/",
            "result_type": "Produced Video",
            "release_date": "2009-12-08T13:00:00-05:00",
            "title": "Climate in a Box",
            "description": "Recent advances in computer technology and software design make it possible to run massive climate simulations on desktop sized machines. This is a paradigm shift from the need for room sized supercomputers to do important work in climate modelling. In a new initiative, NASA plans to facilitate the wider distribution of desktop sized supercomputers, aimed at democratizing climate research among scientists who might otherwise have been more resource contrained. Included in this video are modelling output runs using GEOS-5 and WRF. || ",
            "hits": 29
        },
        {
            "id": 10536,
            "url": "https://svs.gsfc.nasa.gov/10536/",
            "result_type": "Produced Video",
            "release_date": "2009-12-02T06:00:00-05:00",
            "title": "Suzaku: Intergalactic Prospector",
            "description": "Recently astronomers used the Suzaku orbiting X-ray observatory, operated jointly by NASA and the Japanese space agency, to discover the largest known reservoir of rare metals in the universe.  Suzaku detected the elements chromium and manganese while observing the central region of the Perseus galaxy cluster. The metallic atoms are part of the hot gas, or \"intergalactic medium,\" that lies between galaxies. Exploding stars, or supernovas, forge the heavy elements. The supernovas also create vast outflows, called superwinds. These galactic gusts transport heavy elements into the intergalactic void. || ",
            "hits": 28
        },
        {
            "id": 10530,
            "url": "https://svs.gsfc.nasa.gov/10530/",
            "result_type": "Produced Video",
            "release_date": "2009-11-23T23:00:00-05:00",
            "title": "Taking Earth's Temperature",
            "description": "The Earth is a complex system with a unique climate. Many scientists are concerned that Earth's climate is changing at an unprecedented rate. Each January, scientists at NASA Goddard Institute for Space Studies release temperature data for the previous year. How do scientists study how warm our home planet is, and how do they determine what factors affect its climate? This short video explores the tools NASA scientists use to take Earth's temperature.For complete transcript, click here. || Taking_Earths_Temperature_Updated_2009_640x480.00652_print.jpg (1024x768) [99.0 KB] || Taking_Earths_Temperature_Updated_2009_640x480_web.png (320x240) [281.6 KB] || Taking_Earths_Temperature_Updated_2009_640x480_thm.png (80x40) [16.1 KB] || Taking_Earths_Temperature_Updated_2009_640x480_searchweb.png (320x180) [85.4 KB] || Taking_Earths_Temperature_Updated_2009_1280x720_H264.webmhd.webm (960x540) [46.7 MB] || Taking_Earths_Temperature_Updated_2009_640x480.mpg (640x480) [126.9 MB] || Taking_Earths_Temperature_Updated_2009_1280x720_H264.mov (720x486) [158.2 MB] || Taking_Earths_Temperature_Updated_2009_640x480_ipod.m4v (640x480) [46.7 MB] || Taking_Earths_Temperature_Updated_2009320x240.mp4 (320x240) [18.7 MB] || Taking_Earths_Temperature_Updated_2009.wmv (346x260) [35.6 MB] || ",
            "hits": 45
        },
        {
            "id": 10529,
            "url": "https://svs.gsfc.nasa.gov/10529/",
            "result_type": "Produced Video",
            "release_date": "2009-11-18T00:00:00-05:00",
            "title": "The Cosmic Background Explorer (COBE) - 1989",
            "description": "NASA's Cosmic Background Explorer (COBE) satellite rocketed into Earth orbit on Nov. 18, 1989, and quickly revolutionized our understanding of the early cosmos. This video was reissued by NASA for COBE's 20th Anniversary. || ",
            "hits": 237
        },
        {
            "id": 10516,
            "url": "https://svs.gsfc.nasa.gov/10516/",
            "result_type": "Produced Video",
            "release_date": "2009-11-03T00:00:00-05:00",
            "title": "Science for a Hungry World: Agriculture and Climate Change",
            "description": "How will climate change impact agriculture? This episode explores the need for accurate, continuous and accessible data and computer models to track and predict the challenges farmers face as they adjust to a changing climate.For complete transcript, click here. || Thumbnail_1280x720.jpg (1280x720) [776.8 KB] || Thumbnail_80x40.jpg (80x40) [2.6 KB] || Thumbnail_160x80.jpg (160x80) [7.9 KB] || Thumbnail_320x180.jpg (320x180) [91.4 KB] || Ag_Ep6_Climate_AppleTV.webmhd.webm (960x540) [70.8 MB] || Ag_Ep6_Climate_AppleTV.m4v (960x540) [188.6 MB] || Ag_Ep6_Climate_1280x720.mp4 (1280x720) [285.4 MB] || Ag_Ep6_Climate_640x360.m4v (640x360) [54.7 MB] || Ag_Ep6_Climate_640x480.mp4 (640x480) [112.9 MB] || Ag_Ep6_Climate_320x180.mp4 (320x180) [23.4 MB] || Ag_Ep6_Climate.wmv (320x176) [34.9 MB] || Ag_Ep6_Climate_H264.mov (1280x720) [2.7 GB] || Ag_Ep6_Climate_FullRes.mov (1280x720) [5.1 GB] || bigmovie-agriculture_part6_video.hwshow || ",
            "hits": 34
        },
        {
            "id": 10510,
            "url": "https://svs.gsfc.nasa.gov/10510/",
            "result_type": "Produced Video",
            "release_date": "2009-10-28T00:00:00-04:00",
            "title": "Einstein's Cosmic Speed Limit",
            "description": "In its first year of operations, NASA's Fermi Gamma-ray Space Telescope has mapped the entire sky with unprecedented resolution and sensitivity in gamma-rays, the highest-energy form of light. On May 10, 2009 a pair of gamma-ray photons reached Fermi only 900 milliseconds apart after traveling for 7 billion years. Fermi's measurement gives us rare experimental evidence that space-time is smooth as Einstein predicted, and has shut the door on several approaches to gravity where space-time is foamy enough to interfere strongly with light.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || Einsteins_Cosmic_Speed_Limit_512x288_web.png (320x180) [223.5 KB] || Einsteins_Cosmic_Speed_Limit_512x288_thm.png (80x40) [16.5 KB] || Einsteins_Cosmic_Speed_Limit_Thumbnail.jpg (346x260) [107.4 KB] || Einsteins_Cosmic_Speed_Limit_AppleTV.webmhd.webm (960x540) [82.4 MB] || Einsteins_Cosmic_Speed_Limit_AppleTV.m4v (960x540) [208.4 MB] || Einsteins_Cosmic_Speed_Limit_1280x720_H264.mov (1280x720) [433.5 MB] || Einsteins_Cosmic_Speed_Limit_1280x720_ProRes.mov (1280x720) [5.2 GB] || Einsteins_Cosmic_Speed_Limit_640x480_ipod.m4v (640x360) [68.6 MB] || Einsteins_Cosmic_Speed_Limit_512x288.mpg (512x288) [38.3 MB] || Einsteins_Cosmic_Speed_Limit_320x240.mp4 (320x180) [26.5 MB] || GSFC_20091029_EinsteinsCosmicSpeedLimit.wmv (346x236) [38.4 MB] || ",
            "hits": 255
        },
        {
            "id": 10512,
            "url": "https://svs.gsfc.nasa.gov/10512/",
            "result_type": "Produced Video",
            "release_date": "2009-10-27T00:00:00-04:00",
            "title": "Science for a Hungry World: Growing Water Problems",
            "description": "One of the biggest changes to global agriculture is less about the food itself as it is about the water we use to grow it. In some areas, farmers are using freshwater resources - including groundwater - at an alarming rate. The GRACE satellites enable scientists to discover changes to underground aquifers by monitoring changes in the Earth's gravity. In northern India, farmers rely heavily on irrigation to grow crops, and the resulting massive aquifer depletion creates an uncertain future for the region. For complete transcript, click here. || Agriculture_Episode_5_Water_512x288.05177_print.jpg (1024x576) [180.7 KB] || Agriculture_Episode_5_Water_512x288_web.png (320x180) [321.0 KB] || Agriculture_Episode_5_Water_512x288_thm.png (80x40) [18.0 KB] || Agriculture_Episode_5_Water_960x540_AppleTV.webmhd.webm (960x540) [72.9 MB] || Agriculture_Episode_5_Water_1280x720_Youtube.mov (1280x720) [76.1 MB] || Agriculture_Episode_5_Water_960x540_AppleTV.m4v (960x540) [176.9 MB] || Agriculture_Episode_5_Water_1280x720_H264.mov (1280x720) [135.9 MB] || Agriculture_Episode_5_Water_640x480_ipod.m4v (640x360) [52.9 MB] || Agriculture_Episode_5_Water_512x288.mpg (512x288) [159.1 MB] || Agriculture_Episode_5_Water_320x240.mp4 (320x180) [23.2 MB] || bigmovie-science_for_a_hungry_world_5-water_problems.hwshow || ",
            "hits": 21
        },
        {
            "id": 10500,
            "url": "https://svs.gsfc.nasa.gov/10500/",
            "result_type": "Produced Video",
            "release_date": "2009-10-14T00:00:00-04:00",
            "title": "Science for a Hungry World: Food Security",
            "description": "Sponsored by USAID, the Famine Early Warning System Network (FEWS NET) was designed to help governments and aid agencies assess the need for food aid before a famine develops. This episode describes FEWS NET and looks at how FEWS NET uses NASA data to make decisions on the ground.For complete transcript, click here. || Thumbnail_320x180.02202_print.jpg (1024x576) [102.5 KB] || Thumbnail_80x40.jpg (80x40) [22.0 KB] || Thumbnail_160x80.jpg (160x80) [42.5 KB] || Thumbnail_320x180.jpg (320x180) [95.1 KB] || Food_Security_AppleTV.webmhd.webm (960x540) [84.2 MB] || Food_Security_youtube.mov (1280x720) [170.6 MB] || Food_Security_AppleTV.m4v (960x540) [214.4 MB] || Food_Security_1280x720.mp4 (1280x720) [227.1 MB] || Food_Security_h264qt.mov (1280x720) [433.4 MB] || Food_Security_ipod.m4v (640x360) [68.4 MB] || Food_Security_320x180.mp4 (320x180) [28.9 MB] || Agriculture_Food_Security.wmv (320x240) [22.5 MB] || Agriculture_Food_Security.mov (1280x720) [5.8 GB] || bigmovie-agriculture_part4_video.hwshow || ",
            "hits": 22
        },
        {
            "id": 10497,
            "url": "https://svs.gsfc.nasa.gov/10497/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "The Ocean's Green Machines",
            "description": "One tiny marine plant makes life on Earth possible: phytoplankton.  These microscopic photosynthetic drifters form the basis of the marine food web, they regulate carbon in the atmosphere, and are responsible for half of the photosynthesis that takes place on this planet.  Earth's climate is changing at an unprecedented rate, and as our home planet warms, so does the ocean.  Warming waters have big consequences for phytoplankton and for the planet.  For complete transcript, click here. || Oceans_Green_Machines_640x480_ESWpage.00427_print.jpg (1024x576) [65.8 KB] || Oceans_Green_Machines_640x480_ESWpage_web.png (320x180) [135.9 KB] || Oceans_Green_Machines_640x480_ESWpage_thm.png (80x40) [15.0 KB] || Oceans_Green_Machines_AppleTV.webmhd.webm (960x540) [80.8 MB] || Oceans_Green_Machines_1280x720_ProRes.mov (1280x720) [4.9 GB] || Oceans_Green_Machines_1280x720_H264.mov (1280x720) [176.1 MB] || Oceans_Green_Machines_1280x720_ESWpage.mp4 (1280x720) [115.8 MB] || Oceans_Green_Machines_AppleTV.m4v (960x540) [195.1 MB] || Oceans_Green_Machines_640x360_ipod.m4v (640x360) [62.2 MB] || Oceans_Green_Machines_640x480_ESWpage.mp4 (640x360) [62.2 MB] || Oceans_Green_Machines_512x288.mpg (512x288) [113.3 MB] || Oceans_Green_Machines_320x180.mp4 (320x180) [27.7 MB] || Oceans_Green_Machines.wmv (320x176) [37.8 MB] || ",
            "hits": 151
        },
        {
            "id": 10498,
            "url": "https://svs.gsfc.nasa.gov/10498/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "Keeping Up With Carbon",
            "description": "Carbon is all around us.  This unique atom is the basic building block of life, and its compounds form solids, liquids, or gases. Carbon helps form the bodies of living organisms; it dissolves in the ocean; mixes in the atmosphere; and can be stored in the crust of the planet. A carbon atom could spend millions of years moving through this complex cycle. The ocean plays the most critical role in regulating Earth's carbon balance, and understanding how the carbon cycle is changing is key to understanding Earth's changing climate. For complete transcript, click here. || Keeping_Up_with_Carbon_640x360_ESWpage.00577_print.jpg (1024x576) [71.2 KB] || Keeping_Up_with_Carbon_640x360_ESWpage_web.png (320x180) [128.6 KB] || Keeping_Up_with_Carbon_640x360_ESWpage_thm.png (80x40) [13.9 KB] || Keeping_Up_with_Carbon_AppleTV.webmhd.webm (960x540) [84.1 MB] || Keeping_Up_with_Carbon_1280x720_ProRes.mov (1280x720) [5.1 GB] || Keeping_Up_with_Carbon_1280x720_H264.mov (1280x720) [159.3 MB] || Keeping_Up_with_Carbon_1280x720_ESWpage.mp4 (1280x720) [133.5 MB] || Keeping_Up_with_Carbon_AppleTV.m4v (960x540) [201.6 MB] || Keeping_Up_with_Carbon_640x360_ipod.m4v (640x360) [63.2 MB] || Keeping_Up_with_Carbon_640x360_ESWpage.mp4 (640x360) [63.2 MB] || Keeping_Up_with_Carbon_512x288.mpg (512x288) [123.9 MB] || Keeping_Up_with_Carbon_320x180.mp4 (320x180) [26.0 MB] || Keeping_Up_with_Carbon.wmv (320x176) [39.0 MB] || ",
            "hits": 158
        },
        {
            "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": 35
        },
        {
            "id": 10503,
            "url": "https://svs.gsfc.nasa.gov/10503/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "Melting Ice, Rising Seas",
            "description": "Sea level rise is an indicator that our planet is warming. Much of the world's population lives on or near the coast, and rising seas are something worth watching. Sea level can rise for two reasons, both linked to a warming planet. When ice on land, such as mountain glaciers or the ice sheets of Greenland or Antarctica, melt, that water contributes to sea level rise. And when our oceans get warmer - another indicator of climate change - the water expands, also making sea level higher. Using satellites, lasers, and radar in space, and dedicated researchers on the ground, NASA is studying the Earth's ice and water to better understand how sea level rise might affect us all.For complete transcript, click here. || Melting_Seas_ipod_640x480.03027_print.jpg (1024x576) [80.7 KB] || Melting_Seas_ipod_640x480_web.png (320x180) [156.6 KB] || Melting_Seas_ipod_640x480_thm.png (80x40) [16.6 KB] || Melting_Seas_appletv_1280x720.webmhd.webm (960x540) [67.9 MB] || Melting_Seas_H264_1280x720_30fps.mov (1280x720) [128.9 MB] || Melting_Seas_1280x720.mp4 (1280x720) [125.1 MB] || Melting_Seas_broll_prores.mov (1280x720) [4.4 GB] || Melting_Seas_youtube_1280x720.mov (1280x720) [69.1 MB] || Melting_Seas_appletv_1280x720.m4v (960x540) [160.0 MB] || Melting_Seas_ipod_640x480.m4v (640x360) [49.7 MB] || Melting_Seas_ipod_320x240.m4v (320x180) [21.1 MB] || Rising_Seas.wmv (346x260) [38.5 MB] || ",
            "hits": 89
        },
        {
            "id": 10504,
            "url": "https://svs.gsfc.nasa.gov/10504/",
            "result_type": "Produced Video",
            "release_date": "2009-10-12T00:00:00-04:00",
            "title": "Salt of the Earth",
            "description": "Salinity plays a major role in how ocean waters circulate around the globe. Salinity changes can create ocean circulation changes that, in turn, may impact regional and global climates. The extent to which salinity impacts our global ocean circulation is still relatively unknown, but NASA's new Aquarius mission will help advance that understanding by painting a global picture of our planet's salty waters.For complete transcript, click here. || Salt_of_the_Earth_640x480.00519_print.jpg (1024x576) [66.1 KB] || Salt_of_the_Earth_640x480_web.png (320x180) [106.1 KB] || Salt_of_the_Earth_640x480_thm.png (80x40) [12.6 KB] || Salt_of_the_Earth_appletv_1280x720.webmhd.webm (960x540) [65.9 MB] || Salt_of_the_Earth_H264_1280x720_30fps.mov (1280x720) [150.0 MB] || Salt_of_the_Earth_appletv_1280x720.m4v (960x540) [166.5 MB] || Salt_of_the_Earth_1280x720.mp4 (1280x720) [99.9 MB] || Salt_of_the_Earth_broll_prores.mov (1280x720) [4.7 GB] || Salt_of_the_Earth_Youtube_1280x720.mov (1280x720) [72.2 MB] || Salt_of_the_Earth_640x480.m4v (640x360) [55.1 MB] || GSFC_20091012_Aquarius_m10504_Salt.en_US.srt [6.0 KB] || GSFC_20091012_Aquarius_m10504_Salt.en_US.vtt [6.1 KB] || Salt_of_the_Earth_ipod_320x240.m4v (320x180) [23.1 MB] || Salt_of_the_Earth.wmv (346x260) [35.0 MB] || ",
            "hits": 259
        },
        {
            "id": 10509,
            "url": "https://svs.gsfc.nasa.gov/10509/",
            "result_type": "Produced Video",
            "release_date": "2009-10-09T00:00:00-04:00",
            "title": "Water, Water Everywhere!",
            "description": "Water is all around us, and its importance to nearly every natural process on earth cannot be underestimated. The water cycle is the movement of water around the Earth in all its forms, from the ocean to the atmosphere, to snow, soil, aquifers, lakes, and streams on land, and ultimately backs to the ocean. This video explains what the water cycle is and how important it is to life on earth.For complete transcript, click here. || Water_Water_Everywhere_640x480.01727_print.jpg (1024x576) [218.0 KB] || Water_Water_Everywhere_640x480_web.png (320x180) [275.8 KB] || Water_Water_Everywhere_640x480_thm.png (80x40) [18.1 KB] || Water_Water_Everywhere_AppleTV.webmhd.webm (960x540) [95.5 MB] || Water_Water_Everywhere_640x480.mp4 (1280x720) [231.3 MB] || Water_Water_Everywhere_AppleTV.m4v (960x540) [229.2 MB] || Water_Water_Everywhere_H264.mov (1280x720) [2.0 GB] || Water_Water_Everywhere_friday_1280x720.mp4 (1280x720) [231.3 MB] || Water_Water_Everywhere_friday.mov (1280x720) [6.4 GB] || Water_Water_Everywhere_ipod_640x480m4v.m4v (640x360) [72.1 MB] || Water_Water_Everywhere_friday_640x480.mp4 (640x360) [72.1 MB] || Water_Water_Everywhere_1280x720.mp4 (640x480) [97.6 MB] || Water_Water_Everywhere_friday.mp4 (320x180) [30.1 MB] || Water_Water_Everywhere_friday.wmv (320x236) [26.9 MB] || ",
            "hits": 200
        },
        {
            "id": 10496,
            "url": "https://svs.gsfc.nasa.gov/10496/",
            "result_type": "Produced Video",
            "release_date": "2009-10-07T09:00:00-04:00",
            "title": "Science for a Hungry World: Land Cover Land Use Change",
            "description": "NASA remote sensing data is used to measure how much land is used for agriculture and where farms are in relation to population density. This episode explore the transition between native vegetation, farms, and cities. Satellites show where land use changes have been most significant.For complete transcript, click here. || 320x190.10127_print.jpg (1024x576) [132.1 KB] || 80x40_thumbnail.jpg (80x40) [5.6 KB] || 160x80_gallery_thumbnail.jpg (160x80) [16.8 KB] || 320x190_web_thumbnail.jpg (320x239) [73.7 KB] || 320x190_web_thumbnail_searchweb.jpg (320x180) [121.2 KB] || LCLUC_1280x720_AppleTV.webmhd.webm (960x540) [59.0 MB] || LCLUC_1280x720_AppleTV.m4v (960x540) [157.9 MB] || LCLUC_1280x720_H264.mov (1280x720) [178.8 MB] || LCLUC_640x480_ipod.m4v (640x360) [50.4 MB] || LCLUC_320x240_ipod.mp4 (320x180) [18.5 MB] || Ag_LCLUC_Ep3_FullRes.mov (1280x720) [4.2 GB] || bigmovie-agriculture_part3_video.hwshow || ",
            "hits": 75
        },
        {
            "id": 10491,
            "url": "https://svs.gsfc.nasa.gov/10491/",
            "result_type": "Produced Video",
            "release_date": "2009-09-30T00:00:00-04:00",
            "title": "Science For a Hungry World: NASA's Partners",
            "description": "Every day, NASA collects information vital to food production all over the world. This information is a valuable asset.  NASA's mission: to give it away for free. With the data they collect, teams of NASA researchers and their partners at the USDA Foreign Agriculture Service, USAID Famine Early Warning Network (FEWS NET), NOAA, and several major universities including the University of Maryland, work to increase crop yields, ease famine, and keep the global agricultural system functioning.For complete transcript, click here. || ag_ep_2_H.264_iPod_320x240.01192_print.jpg (1024x576) [85.5 KB] || ag_ep_2_H.264_iPod_320x240_web.png (320x180) [108.6 KB] || ag_ep_2_H.264_iPod_320x240_thm.png (80x40) [12.4 KB] || Ag_Ep_2_full_res-H.264_for_Apple_TV.webmhd.webm (960x540) [65.1 MB] || ag_ep_2_draft_5-Ag_ep2_Partners_09-25-09_1804_copy-720_H.264_QT_for_16x9_Youtube.mov (1280x720) [69.5 MB] || Ag_Ep_2_full_res-H.264_for_Apple_TV.m4v (960x540) [166.6 MB] || ag_ep_2_draft_5-Ag_ep2_Partners_09-25-09_1804_copy-H.264_for_iPod_video_and_iPhone_640x480.m4v (640x360) [56.2 MB] || GSFC_20090930_ag_ep_2_m10491.en_US.srt [11.6 KB] || GSFC_20090930_ag_ep_2_m10491.en_US.vtt [11.2 KB] || ag_ep_2_H.264_iPod_320x240.m4v (320x180) [20.7 MB] || Ag_Ep_2_full_res.wmv (320x236) [43.4 MB] || bigmovie-agriculture_part2_video.hwshow || ",
            "hits": 18
        },
        {
            "id": 10490,
            "url": "https://svs.gsfc.nasa.gov/10490/",
            "result_type": "Produced Video",
            "release_date": "2009-09-22T23:00:00-04:00",
            "title": "Science For a Hungry World: Introduction",
            "description": "As the first of six episodes, Science for a Hungry World: Part 1 sets the groundwork for explaining why NASA data is critical to ensure a stable global food system. This video reveals how satellite remote sensing data provide the world with essential information like the Normalized Difference Vegetation Index, or NDVI, which allows scientists and governments to see the health of crops on a global scale. This video reinforces the idea that a unique perspective from space is essential for continuous global agricultural monitoring and accurate forecasting.For complete transcript, click here. || Science_for_a_Hungry_World_Part_1_320x240.01627_print.jpg (1024x576) [111.9 KB] || Science_for_a_Hungry_World_Part_1_320x240_thm.png (80x40) [17.4 KB] || Science_for_a_Hungry_World_Part_1_320x240_web.png (180x320) [152.7 KB] || Science_for_a_Hungry_World_Part_1_AppleTV.webmhd.webm (960x540) [68.9 MB] || Science_for_a_Hungry_World_Part_1_AppleTV.m4v (960x540) [174.3 MB] || Science_for_a_Hungry_World_Part_1_H264_1280x720.mov (1280x720) [194.6 MB] || Science_for_a_Hungry_World_Part_1_640x480_ipod.m4v (640x360) [57.4 MB] || Science_for_a_Hungry_World_Part_1_for_Rob.m4v (640x360) [39.4 MB] || Science_for_a_Hungry_World_Part_1_320x240.mp4 (320x180) [22.5 MB] || Science_for_a_Hungry_World_Part_1.wmv (320x236) [37.8 MB] || bigmovie-science_for_a_hungry_world_1-introduction.hwshow || ",
            "hits": 20
        },
        {
            "id": 10485,
            "url": "https://svs.gsfc.nasa.gov/10485/",
            "result_type": "Produced Video",
            "release_date": "2009-09-16T09:40:00-04:00",
            "title": "Swift's UV portrait of the Andromeda Galaxy",
            "description": "NASA's Swift satellite has acquired the highest-resolution view of the neighboring spiral galaxy M31. Also known as the Andromeda Galaxy, M31 is the largest and closest such galaxy to our own. It's more than 220,000 light-years across and lies 2.5 million light-years away in the constellation Andromeda. Between May 25 and July 26, 2008, Swift's Ultraviolet/Optical Telescope (UVOT) acquired 330 images of M31 at wavelengths of 192.8, 224.6, and 260 nanometers. The images represent a total exposure time of 24 hours. Some 20,000 ultraviolet sources are visible in the image, including M32, a small galaxy in orbit around M31. Dense clusters of hot, young, blue stars sparkle in the disk beyond the galaxy's smooth, redder central bulge. Star clusters are especially plentiful along a ring about 150,000 light-years across. || ",
            "hits": 577
        },
        {
            "id": 10484,
            "url": "https://svs.gsfc.nasa.gov/10484/",
            "result_type": "Produced Video",
            "release_date": "2009-09-14T00:00:00-04:00",
            "title": "Landsat: A Space Age Water Gauge",
            "description": "Agriculture consumes a great deal of water. As demand for water increases, the pressure's on to make sure every drop counts. || ",
            "hits": 25
        },
        {
            "id": 10479,
            "url": "https://svs.gsfc.nasa.gov/10479/",
            "result_type": "Produced Video",
            "release_date": "2009-09-11T00:00:00-04:00",
            "title": "A Tour of the LRO Instrument Suite",
            "description": "Lunar Reconnaissance Orbiter Project Scientist Rich Vondrak explains the LRO suite of instruments and how each will greatly benefit our understanding of the Moon.For complete transcript, click here. || LRO_vondrak_ipod.02402_print.jpg (1024x576) [90.1 KB] || LRO_vondrak_ipod_web.png (320x180) [177.9 KB] || LRO_vondrak_ipod_thm.png (80x40) [16.3 KB] || LRO_vondrak_ipod.webmhd.webm (960x540) [46.3 MB] || LRO_vondrak_ipod.m4v (640x360) [70.8 MB] || LRO_vondrak.wmv (320x236) [37.5 MB] || LRO_vondrak_nasacast.mp4 (320x176) [21.6 MB] || ",
            "hits": 15
        },
        {
            "id": 10471,
            "url": "https://svs.gsfc.nasa.gov/10471/",
            "result_type": "Produced Video",
            "release_date": "2009-09-04T00:00:00-04:00",
            "title": "SDO Engineers Create What Never Was",
            "description": "Scientists discover what there is, but engineers create that which never was. This special group of folks at Goddard Space Flight Center are creators, like any artist, but instead of working with art they are working wiht scientific, mechanical, or electrical things with fantastic problems to solve.  Watch engineers talk about what it is like to be an engineer as they build, assemble, integrate, and test the Solary Dynamics Observatory (SDO) soon to be launched in early 2010. If you have a strong tendancy towards science and mathematics, and enjoy working and building things with your hands, then you could also come up with creative solutions, to create something, to do a certain job and do it well. || ",
            "hits": 23
        },
        {
            "id": 3619,
            "url": "https://svs.gsfc.nasa.gov/3619/",
            "result_type": "Visualization",
            "release_date": "2009-09-01T18:00:00-04:00",
            "title": "A Tour of the Cryosphere 2009",
            "description": "The cryosphere consists of those parts of the Earth's surface where water is found in solid form, including areas of snow, sea ice, glaciers, permafrost, ice sheets, and icebergs. In these regions, surface temperatures remain below freezing for a portion of each year. Since ice and snow exist relatively close to their melting point, they frequently change from solid to liquid and back again due to fluctuations in surface temperature. Although direct measurements of the cryosphere can be difficult to obtain due to the remote locations of many of these areas, using satellite observations scientists monitor changes in the global and regional climate by observing how regions of the Earth's cryosphere shrink and expand.This animation portrays fluctuations in the cryosphere through observations collected from a variety of satellite-based sensors. The animation begins in Antarctica, showing some unique features of the Antarctic landscape found nowhere else on earth. Ice shelves, ice streams, glaciers, and the formation of massive icebergs can be seen clearly in the flyover of the Landsat Image Mosaic of Antarctica. A time series shows the movement of iceberg B15A, an iceberg 295 kilometers in length which broke off of the Ross Ice Shelf in 2000. Moving farther along the coastline, a time series of the Larsen ice shelf shows the collapse of over 3,200 square kilometers ice since January 2002. As we depart from the Antarctic, we see the seasonal change of sea ice and how it nearly doubles the apparent area of the continent during the winter.From Antarctica, the animation travels over South America showing glacier locations on this mostly tropical continent. We then move further north to observe daily changes in snow cover over the North American continent. The clouds show winter storms moving across the United States and Canada, leaving trails of snow cover behind. In a close-up view of the western US, we compare the difference in land cover between two years: 2003 when the region received a normal amount of snow and 2002 when little snow was accumulated. The difference in the surrounding vegetation due to the lack of spring melt water from the mountain snow pack is evident.As the animation moves from the western US to the Arctic region, the areas affected by permafrost are visible. As time marches forward from March to September, the daily snow and sea ice recede and reveal the vast areas of permafrost surrounding the Arctic Ocean.The animation shows a one-year cycle of Arctic sea ice followed by the mean September minimum sea ice for each year from 1979 through 2008. The superimposed graph of the area of Arctic sea ice at this minimum clearly shows the dramatic decrease in Artic sea ice over the last few years.While moving from the Arctic to Greenland, the animation shows the constant motion of the Arctic polar ice using daily measures of sea ice activity. Sea ice flows from the Arctic into Baffin Bay as the seasonal ice expands southward. As we draw close to the Greenland coast, the animation shows the recent changes in the Jakobshavn glacier. Although Jakobshavn receded only slightly from 1964 to 2001, the animation shows significant recession from 2001 through 2009. As the animation pulls out from Jakobshavn, the effect of the increased flow rate of Greenland costal glaciers is shown by the thinning ice shelf regions near the Greenland coast.This animation shows a wealth of data collected from satellite observations of the cryosphere and the impact that recent cryospheric changes are making on our planet.For more information on the data sets used in this visualization, visit NASA's EOS DAAC website.Note: This animation is an update of the animation 'A Short Tour of the Cryosphere', which is itself an abridged version of the animation 'A Tour of the Cryosphere'. The popularity of the earlier animations and their continuing relevance prompted us to update the datasets in parts of the animation and to remake it in high definition. In certain cases, our experiences in using the earlier work have led us to tweak the presentation of some of the material to make it clearer. Our thanks to Dr. Robert Bindschadler for suggesting and supporting this remake. || ",
            "hits": 38
        },
        {
            "id": 10481,
            "url": "https://svs.gsfc.nasa.gov/10481/",
            "result_type": "Produced Video",
            "release_date": "2009-08-25T00:00:00-04:00",
            "title": "Feeling the Sting of Climate Change",
            "description": "NASA research scientist Wayne Esaias uses honey bees as tiny data collectors to understand how climate change is affecting pollination. His citizen-scientist project, HoneyBeeNet, compares bee data from across North America to satellite imagery in order to gain a big-picture perspective of how our warming climate is affecting both plants and pollinators. || ",
            "hits": 29
        },
        {
            "id": 10472,
            "url": "https://svs.gsfc.nasa.gov/10472/",
            "result_type": "Produced Video",
            "release_date": "2009-07-28T00:00:00-04:00",
            "title": "NASA/NOAA GOES-14: First Full Disk Image",
            "description": "Exactly a month ago on June 27 NASA launched a new and improved weather satellite called GOES-O. Now that GOES-O is safely into its orbit, it has been renamed to GOES-14. On July 27, 2009 NOAA and NASA released the first full disk image from GOES-14 showing that the satellite is operating correctly. NASA Goddard Producer Silvia Stoyanova, visits the NOAA Satellite Operations Facility in Suitland, Md. for the release of the first image and talks to NOAA Meteorologist Tom Renkevens about it.For complete transcript, click here. || GOES14FirstImageiPod.03452_print.jpg (1024x576) [82.8 KB] || GOES14FirstImageiPod_web.png (320x180) [100.6 KB] || GOES14FirstImageiPod_thm.png (80x40) [9.5 KB] || G2009-073_GOES-14_First_Image.webmhd.webm (960x540) [50.3 MB] || G2009-073_GOES-14_First_Image.mov (960x720) [1.4 GB] || GOES14FirstImageYouTube.mov (1280x720) [69.0 MB] || GOES14FirstImageAppleTV.m4v (960x540) [118.4 MB] || GOES14FirstImageiPod.m4v (640x360) [35.3 MB] || GOES14FirstImageNASAPodcast.mp4 (320x240) [10.8 MB] || GOES14FirstImageNASAPortal.wmv (346x260) [27.7 MB] || GOES14FirstImageSVS.mpg (512x288) [31.8 MB] || ",
            "hits": 59
        },
        {
            "id": 3595,
            "url": "https://svs.gsfc.nasa.gov/3595/",
            "result_type": "Visualization",
            "release_date": "2009-07-27T00:00:00-04:00",
            "title": "Sentinels of the Heliosphere",
            "description": "Heliophysics is a term to describe the study of the Sun, its atmosphere or the heliosphere, and the planets within it as a system. As a result, it encompasses the study of planetary atmospheres and their magnetic environment, or magnetospheres. These environments are important in the study of space weather.As a society dependent on technology, both in everyday life, and as part of our economic growth, space weather becomes increasingly important. Changes in space weather, either by solar events or geomagnetic events, can disrupt and even damage power grids and satellite communications. Space weather events can also generate x-rays and gamma-rays, as well as particle radiations, that can jeopardize the lives of astronauts living and working in space.This visualization tours the regions of near-Earth orbit; the Earth's magnetosphere, sometimes called geospace; the region between the Earth and the Sun; and finally out beyond Pluto, where Voyager 1 and 2 are exploring the boundary between the Sun and the rest of our Milky Way galaxy. Along the way, we see these regions patrolled by a fleet of satellites that make up NASA's Heliophysics Observatory Telescopes. Many of these spacecraft do not take images in the conventional sense but record fields, particle energies and fluxes in situ. Many of these missions are operated in conjunction with international partners, such as the European Space Agency (ESA) and the Japanese Space Agency (JAXA).The Earth and distances are to scale. Larger objects are used to represent the satellites and other planets for clarity.Here are the spacecraft featured in this movie:Near-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTRACE: Observes the Sun in visible and ultraviolet wavelengths. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. AIM: Images and measures noctilucent clouds. SVS pageGeospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of five satellites to study how magnetospheric instabilities produce substorms. SVS pageL1 Fleet: The L1 point is a Lagrange Point, a point between the Earth and the Sun where the gravitational pull is approximately equal. Spacecraft can orbit this location for continuous coverage of the Sun.SOHO: Studies the Sun with cameras and a multitude of other instruments. SVS pageACE: Measures the composition and characteristics of the solar wind. Wind: Measures particle flows and fields in the solar wind. Heliospheric FleetSTEREO-A and B: These two satellites observe the Sun, with imagers and particle detectors, off the Earth-Sun line, providing a 3-D view of solar activity. SVS pageHeliopause FleetVoyager 1 and 2: These spacecraft conducted the original 'Planetary Grand Tour' of the solar system in the 1970s and 1980s. They have now travelled further than any human-built spacecraft and are still returning measurements of the interplanetary medium. SVS pageThis enhanced, narrated visualization was shown at the SIGGRAPH 2009 Computer Animation Festival in New Orleans, LA in August 2009; an eariler version created for AGU was called NASA's Heliophysics Observatories Study the Sun and Geospace. || ",
            "hits": 162
        },
        {
            "id": 10468,
            "url": "https://svs.gsfc.nasa.gov/10468/",
            "result_type": "Produced Video",
            "release_date": "2009-07-21T00:00:00-04:00",
            "title": "Journey to Galapagos",
            "description": "NASA oceanographer Dr. Gene Carl Feldman is no stranger to the Galapagos Islands, although he has never been there. He has studied these \"Enchanted Isles\" from the vantage point of space for the last 25 years, but in July 2009 he will set foot on the islands for the first time. 2009 marks the 200th anniversary of the birth of Charles Darwin as well as the 150th anniversary of the publication of The Origin of Species. In celebration of these two events, the Charles Darwin Foundation is holding an international symposium to assess the current state of knowledge about this remarkable place, and has invited Dr. Feldman to present a paper on his perspective of the Galapagos. || ",
            "hits": 23
        },
        {
            "id": 10451,
            "url": "https://svs.gsfc.nasa.gov/10451/",
            "result_type": "Produced Video",
            "release_date": "2009-07-16T09:01:00-04:00",
            "title": "NASA Releases Preview Partially Restored Apollo 11 Video",
            "description": "To commemorate the 40th anniversary of Apollo 11, NASA released partially restored video of a series of 15 memorable moments from the July 20 moonwalk. The source material for the restoration project is the best of the available broadcast-format video. Lowry Digital, Burbank, Calif., is significantly enhancing the video using the company's proprietary software technology and other restoration techniques. The video is part of a larger restoration project that will be completed in September and provide a newly restored high definition video of the entire Apollo 11 moonwalk. The completed restoration will provide the public with the highest quality video of this historic event.For professional resolution quicktimes, please click here.All items currently available in this series are: Highlights Neil Armstrong Making His Way to the Lunar Surface Buzz Aldrin Following Neil Armstrong Down the Lunar Module Ladder Astronauts Buzz Aldrin and Neil Armstrong Unveil the Commemorative Plaque Neil Armstrong's Television Panorama Neil Armstrong Photographs Buzz Aldrin Setting Up a Solar Wind Collector Raising the American Flag Buzz Aldrin Walking and Running Astronauts Talking with President Nixon Buzz Aldrin Kicking Moon Dust Buzz Aldrin Carrying Experiment Packages Buzz Aldrin Hammering a Core Sample Tube into the Moon's Surface Buzz Aldrin Entering the LM after an EVA Astronauts Storing Rock Samples into the LM Neil Armstrong Climbing the Ladder After the Three Hour EVA Astronauts Jettisoning Backpacks || ",
            "hits": 104
        },
        {
            "id": 10441,
            "url": "https://svs.gsfc.nasa.gov/10441/",
            "result_type": "Produced Video",
            "release_date": "2009-07-02T15:00:00-04:00",
            "title": "SDO's Science",
            "description": "These animations and web shorts explain how SDO's instruments will look at the sun and allow us to better predict how the sun will affect us in the future. || ",
            "hits": 67
        },
        {
            "id": 10445,
            "url": "https://svs.gsfc.nasa.gov/10445/",
            "result_type": "Produced Video",
            "release_date": "2009-06-23T00:00:00-04:00",
            "title": "LRO Enters Lunar Orbit (Highlights)",
            "description": "After a four and a half day journey from the Earth, the Lunar Reconnaissance Orbiter, or LRO, successfully entered orbit around the moon. Engineers at NASA's Goddard Space Flight Center in Greenbelt, Md., confirmed the spacecraft's lunar orbit insertion at 6:27 a.m. EDT Tuesday, June 23, 2009.During transit to the moon, engineers performed a mid-course correction to get the spacecraft in the proper position to reach its lunar destination. Since the moon is always moving, the spacecraft shot for a target point ahead of the moon. When close to the moon, LRO used its rocket motor to slow down until the gravity of the moon caught the spacecraft in lunar orbit.To see the full one hour video produced live during the orbit insertion burns, visit entry #10444 || ",
            "hits": 21
        },
        {
            "id": 10252,
            "url": "https://svs.gsfc.nasa.gov/10252/",
            "result_type": "Produced Video",
            "release_date": "2009-06-18T01:01:00-04:00",
            "title": "GOES-O Ready to Launch!",
            "description": "This video shows a quick tour and overview of the facilities where the GOES-O satellite was built and tested prior to launch. GOES-O was integrated by Boeing Space and Intelligence Systems in El Segundo, CA and then transported to the testing facility in Titusville, FL. After completion of the test program, performed at the Astrotech facility in Titusville, the spacecraft will be launched on a United Launch Alliance Delta IV rocket from Cape Canaveral, FL.For complete transcript, click here. || SVSDeliverable4_640x360.01752_print.jpg (1023x769) [76.5 KB] || SVSDeliverable4_640x360_thm.png (80x40) [16.9 KB] || SVSDeliverable4_640x360_web.png (320x240) [332.5 KB] || GOES-O_ReadyToLaunch_podcast_searchweb.png (320x180) [241 bytes] || GOES-O_ReadyToLaunch_appletv.webmhd.webm (960x540) [51.9 MB] || GOES-O_ReadyToLaunch_youtube.mov (1280x720) [64.3 MB] || GOES-O_ReadyToLaunch_appletv.m4v (960x540) [128.0 MB] || GOES-O_ReadyToLaunch_fullres.mov (1280x720) [136.0 MB] || GOES-O_ReadyToLaunch_ipod.m4v (640x360) [42.2 MB] || GOES-O_ReadyToLaunch_portal.wmv (346x260) [40.7 MB] || GOES-O_ReadyToLaunch_podcast.mp4 (320x240) [16.3 MB] || GOES-O_ReadyToLaunch_svs.mpg (512x288) [33.7 MB] || ",
            "hits": 17
        },
        {
            "id": 10443,
            "url": "https://svs.gsfc.nasa.gov/10443/",
            "result_type": "Produced Video",
            "release_date": "2009-06-17T00:00:00-04:00",
            "title": "Lunar Reconnaissance Orbiter (LRO) Launch Videos",
            "description": "The videos on this page were shot during the week of the LRO/LCROSS launch (June 15-19, 2009) at Kennedy Space Center.For more views of the LRO/LCROSS launch, including footage from inside the Missions Operations Control Room at Goddard and individual camera feeds of the launch from Kennedy, check out entry #10469. || ",
            "hits": 102
        },
        {
            "id": 10422,
            "url": "https://svs.gsfc.nasa.gov/10422/",
            "result_type": "Produced Video",
            "release_date": "2009-06-10T12:01:00-04:00",
            "title": "GOES-O Mission Overview Video",
            "description": "For more info on the GOES-O Mission, visit: http://www.nasa.gov/GOES-O. || ",
            "hits": 25
        },
        {
            "id": 10438,
            "url": "https://svs.gsfc.nasa.gov/10438/",
            "result_type": "Produced Video",
            "release_date": "2009-05-21T00:00:00-04:00",
            "title": "LRO: Mapping Our Future",
            "description": "The Lunar Reconnaissance Orbiter (LRO) is the first mission in NASA's planned return to the moon. LRO is an unmanned mission to create the comprehensive atlas of the moon's features and resources necessary to design all future lunar exploration efforts. LRO focuses on the selection of safe landing sites, identification of lunar resources and the study of how lunar radiation will affect humans.For complete transcript, click here. || LRO_MappingOurFuture_ipod.00905_print.jpg (1024x576) [30.4 KB] || LRO_MappingOurFuture_ipod_web.png (320x180) [33.3 KB] || LRO_MappingOurFuture_ipod_thm.png (80x40) [3.6 KB] || LRO_MappingOurFuture_AppleTV.webmhd.webm (960x540) [84.8 MB] || LRO_MappingOurFuture_YouTube.mov (1280x720) [100.5 MB] || LRO_MappingOurFuture_fullres.mov (1280x720) [192.6 MB] || LRO_MappingOurFuture_AppleTV.m4v (960x540) [210.6 MB] || LRO_MappingOurFuture_ipod.m4v (640x360) [67.2 MB] || GSFC_20090521_LRO_m10438_Mapping1a.en_US.srt [7.5 KB] || GSFC_20090521_LRO_m10438_Mapping1a.en_US.vtt [7.5 KB] || LRO_MappingOurFuture_320x240.mp4 (320x240) [16.6 MB] || LRO_MappingOurFuture_portal.wmv (346x260) [48.7 MB] || LRO_MappingOurFuture_svs.mpg (512x288) [54.2 MB] || ",
            "hits": 65
        },
        {
            "id": 10436,
            "url": "https://svs.gsfc.nasa.gov/10436/",
            "result_type": "Produced Video",
            "release_date": "2009-05-12T00:00:00-04:00",
            "title": "Making Hubble More Powerful",
            "description": "The Hubble Space Telescope would not be able to produce its breathtaking science without the upgraded infrastructure targeted during the HST SM4 mission: Fine Guidance Sensor, Scientific Instrument Command and Data Handling, Soft Capture Mechanism, Batteries, and New Outer Blanket Layers. Along with all new cameras, scientific instruments, the Hubble telescope will work better than it ever has in its lifetime. || ",
            "hits": 25
        },
        {
            "id": 10435,
            "url": "https://svs.gsfc.nasa.gov/10435/",
            "result_type": "Produced Video",
            "release_date": "2009-05-10T00:00:00-04:00",
            "title": "Hubble SM4 Launch Highlights",
            "description": "Employees at NASA's Goddard Space Flight Center cheered and applauded as shuttle Atlantis successfully launched at 2:01:56 p.m. ET on May 11. The Atlantis crew embarked on the fifth and final shuttle mission to the Hubble Space Telescope. The work they do will extend Hubble's lifespan by at least five years. Goddard employees had the opportunity to watch the launch in Building 8's auditorium and at the Goddard Visitor Center, where members of the public could enjoy the viewing as well. In the Building 8 auditorium during the hour before the launch, Mansoor Ahmed, manager of the Hubble Operations Project, and Dr. Jim Garvin, Goddard's chief scientist highlighted the complexity of the mission, which will make Hubble more powerful than ever before. Goddard plays a major role in the Hubble servicing mission. Astronauts trained with sophisticated Hubble models in Goddard facilities, and all of the telescope's components went through extensive testing at the center. Goddard's Space Telescope Operations Control Center staff upload the commands to Hubble that tell it where to point and when, what sensing instruments to use, and when to send data back to Earth. They also troubleshoot any problems that arise. During the servicing mission, the control center plays a vital role in ensuring all the new Hubble components will operate properly after the astronauts install them. || ",
            "hits": 20
        },
        {
            "id": 10434,
            "url": "https://svs.gsfc.nasa.gov/10434/",
            "result_type": "Produced Video",
            "release_date": "2009-05-06T00:00:00-04:00",
            "title": "Earth Observatory 10 Year Anniversary",
            "description": "April 29, 2009, marked the tenth anniversary of the launch of NASA's Earth Observatory. For the last decade, the Earth Observatory has been using the stunning images and data provided by NASA satellites to tell the story of our planet and the scientists who are working to help us understand it. || ",
            "hits": 33
        },
        {
            "id": 10428,
            "url": "https://svs.gsfc.nasa.gov/10428/",
            "result_type": "Produced Video",
            "release_date": "2009-04-25T00:00:00-04:00",
            "title": "Earth Day 2009 with Kenji Williams",
            "description": "The DLN teamed with director and violinist Kenji Williams to present an out of this world experience known as Bella Gaia (Beautiful Earth). This one-of-a-kind multimedia journey of Earth, as observed from space, combined his music with NASA imagery. Bella Gaia was presented to students and teachers around the world during two webcasts from the Goddard studio. || ",
            "hits": 17
        },
        {
            "id": 10416,
            "url": "https://svs.gsfc.nasa.gov/10416/",
            "result_type": "Produced Video",
            "release_date": "2009-04-07T00:00:00-04:00",
            "title": "Guided Tour of LIMA Flyover",
            "description": "In 2007, more than 1,100 Landsat 7 images were used to create the first ever, high-resolution, true color map of Antarctica.  The Landsat Image Mosaic of Antarctica (LIMA) is a virtually cloud-free, 3-D view of Antarctica's frozen landscape produced by NASA, working with the National Science Foundation, the U.S. Geological Survey and the British Antarctic Survey.Visualizers stitched together Landsat 7 satellite imagery acquired in 1999 and 2001 with a digital elevation model and field data measurements. || ",
            "hits": 110
        },
        {
            "id": 10411,
            "url": "https://svs.gsfc.nasa.gov/10411/",
            "result_type": "Produced Video",
            "release_date": "2009-03-18T00:00:00-04:00",
            "title": "The Top 5 Solar Discoveries",
            "description": "A countdown of the top 5 solar discoveries from the Sun-Earth Connection Education Forum. These include the discoveries of sunspots, the solar cycle, the heliosphere, aurora formation, and space weather. || ",
            "hits": 92
        },
        {
            "id": 10401,
            "url": "https://svs.gsfc.nasa.gov/10401/",
            "result_type": "Produced Video",
            "release_date": "2009-03-01T00:00:00-05:00",
            "title": "Earth Observing Landsat 5 Turns 25 Years Old",
            "description": "Still observing the Earth after 25 years—22 beyond its three-year primary mission lifetime—Landsat 5 collects valuable scientific data daily. Some attribute the satellite's longevity to over-engineering. Others say it's a long run of good luck. Whatever the reason, no one who attended the satellite's March 1984 launch could have expected it would still be working today.For complete transcript, click here. || Landsat5_turns_25_ipodLG.00202_print.jpg (1024x576) [73.2 KB] || Landsat5_turns_25_ipodLG_web.png (320x180) [149.4 KB] || Landsat5_turns_25_ipodLG_thm.png (80x40) [13.9 KB] || Landsat5_turns_25_appletv.webmhd.webm (960x540) [51.8 MB] || Landsat5_turns_25_appletv.m4v (960x540) [87.6 MB] || Landsat5_turns_25_YouTube.mov (1280x720) [56.6 MB] || Landsat5_turns_25_fullresH264.mov (1280x720) [119.3 MB] || Landsat5_turns_25_ipodLG.m4v (640x360) [42.3 MB] || Landsat5_turns_25_svsSM.mpg (512x288) [32.8 MB] || Landsat5_turns_25_ipodSM.m4v (320x180) [16.4 MB] || Landsat5_turns_25_NASAcast.mp4 (320x236) [30.9 MB] || GSFC_20090227_Landsat5turns25.wmv (346x260) [30.5 MB] || ",
            "hits": 83
        },
        {
            "id": 10376,
            "url": "https://svs.gsfc.nasa.gov/10376/",
            "result_type": "Produced Video",
            "release_date": "2009-02-17T12:00:00-05:00",
            "title": "LRO's Team Spirit with Joanne Baker",
            "description": "The Lunar Reconnaissance Orbiter (LRO) is the first step to future missions to the Moon, Mars, and beyond. But a lot has to happen before we get there and one woman on the LRO team played a key role in 'putting it together.' || Joanne_Baker_Profile.01252_print.jpg (1024x576) [56.3 KB] || Joanne_Baker_Profile_web.png (320x180) [240.1 KB] || Joanne_Baker_Profile_thm.png (80x40) [16.3 KB] || Joanne_Baker_Profile_AppleTV.webmhd.webm (960x540) [30.2 MB] || Joanne_Baker_Profile_AppleTV.m4v (960x540) [57.0 MB] || Joanne_Baker_Profile.mov (1280x720) [82.9 MB] || Joanne_Baker_Profile.mpg (640x360) [31.5 MB] || Joanne_Baker_Profile_ipod.m4v (640x360) [26.2 MB] || Joanne_Baker_Profile.m4v (320x180) [11.8 MB] || Joanne_Baker_Profile.mp4 (320x240) [6.2 MB] || Joanne_Baker_Profile_SVSsmall.mpg (512x288) [21.1 MB] || Joanne_Baker_Profile.wmv (346x260) [19.4 MB] || ",
            "hits": 17
        },
        {
            "id": 10385,
            "url": "https://svs.gsfc.nasa.gov/10385/",
            "result_type": "Produced Video",
            "release_date": "2009-01-26T00:00:00-05:00",
            "title": "Welcome",
            "description": "Welcome to Goddard's Space Flight Center. This short video will give you a quick look at what Goddard is all about. || ",
            "hits": 17
        },
        {
            "id": 10356,
            "url": "https://svs.gsfc.nasa.gov/10356/",
            "result_type": "Produced Video",
            "release_date": "2008-12-15T00:00:00-05:00",
            "title": "THEMIS Discovers Biggest Breach of Earth's Magnetosphere",
            "description": "NASA's THEMIS mission has overturned a longstanding belief about the interaction between solar particles and Earth's protective magnetic field. This new discovery could help scientists predict when the solar storms that can disrupt power grids, satellites and even GPS signals, could be especially severe.For more information: www.nasa.gov/themisFor complete transcript, click here. || THEMIS_ipodLG.00702_print.jpg (1024x576) [97.3 KB] || THEMIS_ipodLG_web.png (180x320) [228.6 KB] || THEMIS_ipodLG_thm.png (80x40) [16.4 KB] || THEMIS_AppleTV.webmhd.webm (960x540) [32.1 MB] || THEMIS_1280.mov (1280x720) [83.9 MB] || THEMIS_AppleTV.m4v (960x540) [81.1 MB] || THEMIS_ipodLG.m4v (640x360) [26.4 MB] || THEMIS_svsLG.mpg (640x360) [31.9 MB] || THEMIS_YouTube.mov (640x480) [30.0 MB] || THEMIS320.mp4 (320x240) [6.2 MB] || THEMIS_ipodSM.m4v (320x180) [12.0 MB] || THEMIS_svsSM.mpg (512x288) [21.4 MB] || THEMIS.wmv (346x260) [20.1 MB] || ",
            "hits": 143
        },
        {
            "id": 10338,
            "url": "https://svs.gsfc.nasa.gov/10338/",
            "result_type": "Produced Video",
            "release_date": "2008-10-30T00:00:00-04:00",
            "title": "Looking Back at 2003s Spooky Halloween Solar Storms",
            "description": "In the weeks surrounding Halloween in 2003, the sun unleashed a series of spooky storms towards the Earth, storms that ignited lots of ghostly looking auroras, but that also wreaked havoc with power grids, satellites and other electrical equipment. On the fifth anniversary of these unprecedented storms, NASA takes a look back at the Sun during these haunting days. || ",
            "hits": 100
        },
        {
            "id": 10206,
            "url": "https://svs.gsfc.nasa.gov/10206/",
            "result_type": "Produced Video",
            "release_date": "2008-10-16T00:00:00-04:00",
            "title": "Sample Analysis at Mars (SAM)",
            "description": "Sample Analysis at Mars (SAM) is a suite of instruments developed for use on the Mars Science Laboratory. By looking for evidence of water, carbon, and other important building blocks of life in the Mars soil and atmosphere, this suite will help answer one of humankind's biggest questions about the planet: did it ever support life? SAM was designed and built in an international collaboration between Goddard Space Flight Center, the Jet Propulsion Laboratory, the University of Paris, and Honeybee Robotics. This video series highlights the mission, its objectives, and some of Goddard's contributors to the project. || ",
            "hits": 125
        },
        {
            "id": 10331,
            "url": "https://svs.gsfc.nasa.gov/10331/",
            "result_type": "Produced Video",
            "release_date": "2008-10-15T00:00:00-04:00",
            "title": "In The Zone",
            "description": "Earth's oceans are wide reaching and teeming with life. One microscopic aquatic organism plays a major role in making life on Earth possible: phytoplankton. Under certain conditions, excessive phytoplankton growth can result in an area known as a dead zone. Dead zones form when big blooms of phytoplankton at the surface trigger large quantities of organic matter, which then sink to the bottom. Bacteria break down the organic material, releasing carbon dioxide but absorbing oxygen as they work. Most marine organisms need oxygen for survival and dead zones prove fatal for many aquatic species. This short web video features dynamic animations, science data visualizations, and interview excerpts with a NASA oceanographer to explore this fascinating marine phenomenon. || ",
            "hits": 51
        },
        {
            "id": 10259,
            "url": "https://svs.gsfc.nasa.gov/10259/",
            "result_type": "Produced Video",
            "release_date": "2008-09-29T00:00:00-04:00",
            "title": "Vision. Hope. Triumph.",
            "description": "'They had to have vision; they had to have hope. And ultimately there was the triumph of seeing it come to fruition.' Heidi Hammel, a Senior Research Scientist from the Space Science Institute in Boulder, Colorado, expresses her views on the past, present, and future of the Hubble Space Telescope and its upcoming repair mission.For more information go to http://www.nasa.gov/hubble. || ",
            "hits": 29
        },
        {
            "id": 10353,
            "url": "https://svs.gsfc.nasa.gov/10353/",
            "result_type": "Produced Video",
            "release_date": "2008-09-25T00:00:00-04:00",
            "title": "Sea Ice 2008",
            "description": "Arctic sea ice declined this summer to its second smallest extent in the satellite era, suggesting that the record set in 2007 may not have been an anomaly. If recent trends in the melt rate continue, we could see a virtually ice-free Arctic each summer much sooner than previously thought.For complete transcript, click here. || SeaIce2008_320iPod.03621_print.jpg (1024x576) [95.6 KB] || SeaIce2008_320iPod_web.png (320x180) [129.4 KB] || SeaIce2008_320iPod_thm.png (80x40) [17.3 KB] || SeaIce2008_AppleTV.webmhd.webm (960x540) [46.7 MB] || SeaIce2008_AppleTV.m4v (960x540) [115.0 MB] || SeaIce2008_fullH264.mov (1280x720) [112.5 MB] || SeaIce2008_640iPod.m4v (640x360) [37.0 MB] || Sea_Ice_2008_640x360_Youtube.mov (640x480) [40.7 MB] || GSFC_20080925_SeaIce_m10353_2008.en_US.srt [6.0 KB] || GSFC_20080925_SeaIce_m10353_2008.en_US.vtt [5.7 KB] || SeaIce2008_320iPod.m4v (320x180) [16.6 MB] || SeaIce2008_podcast.mp4 (320x236) [14.7 MB] || SeaIce2008_512x288.mpg (512x288) [50.7 MB] || ",
            "hits": 40
        },
        {
            "id": 10349,
            "url": "https://svs.gsfc.nasa.gov/10349/",
            "result_type": "Produced Video",
            "release_date": "2008-09-03T00:00:00-04:00",
            "title": "LRO Scouts for Safe Landing Sites (Narrated)",
            "description": "The Lunar Reconnaissance Orbiter (LRO) is NASA's scouting mission to prepare for a return to the moon. One of its primary objectives will be to assess the lunar terrain for areas that would provide safe landing sites for future missions, both manned and unmanned, that plan to touch down on the moon's surface. This video helps explain how LRO will accomplish its objective.The raw animation sequences used to create this video feature as well as high resolution stills from the video can be viewed and downloaded from How LRO Will Find Safe Landing Sites on the Moon (#3533). || ",
            "hits": 11
        },
        {
            "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": 17
        },
        {
            "id": 10289,
            "url": "https://svs.gsfc.nasa.gov/10289/",
            "result_type": "Produced Video",
            "release_date": "2008-07-18T02:00:00-04:00",
            "title": "Rain Rain Go Away Come Again on a Work Day?",
            "description": "During the scorching summer months an afternoon rainstorm can be a common and refreshing sight. But for residents in the southeastern United States, a recent NASA study has found, these storms are more intense during the work week than on the weekends. This trend, scientists belive, is driven by pollution that also increases during the work week, from sources like businesses, traffic and factories. || ",
            "hits": 15
        },
        {
            "id": 10238,
            "url": "https://svs.gsfc.nasa.gov/10238/",
            "result_type": "Produced Video",
            "release_date": "2008-06-17T00:00:00-04:00",
            "title": "HST SM4 Countdown Status 1",
            "description": "An update on instrument, tool and carrier preparations for STS-125: HST Servicing Mission 4 at NASA Goddard Space Flight Center in Maryland. Update as of January 2, 2008.For complete transcript, click here. || G08-001HD-Countdown_to_SM4_Status-fullres-HD_iPod01027_print.jpg (1024x576) [62.2 KB] || G08-001HD-Countdown_to_SM4_Status-fullres-HD_iPod_web.png (320x180) [87.2 KB] || G08-001HD-Countdown_to_SM4_Status-fullres-HD_iPod_thm.png (80x40) [17.3 KB] || G08-001HD-Countdown_to_SM4_Status-fullres-MPEG4-h264.webmhd.webm (960x540) [37.5 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-MPEG4-h264.mov (1280x720) [152.3 MB] || GSFC_20080617_HST_m10238_Countdown.mp4 (1280x720) [278.9 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-iTunes.m4v (640x360) [21.8 MB] || GSFC_20080617_HST_m10238_Countdown.en_US.srt [3.1 KB] || GSFC_20080617_HST_m10238_Countdown.en_US.vtt [3.0 KB] || G08-001HD-Countdown_to_SM4_Status-fullres-HD_iPod.m4v (320x180) [13.1 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-MPEG4.mp4 (512x288) [259.7 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-QuickTime.mov (512x288) [118.3 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-Sorenson3_MPEG1.mpg (320x240) [39.5 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-WindowsMedia.mp4 (512x288) [38.8 MB] || G08-001HD-Countdown_to_SM4_Status-fullres-YouTube.mov (320x240) [71.0 MB] || ",
            "hits": 11
        },
        {
            "id": 10239,
            "url": "https://svs.gsfc.nasa.gov/10239/",
            "result_type": "Produced Video",
            "release_date": "2008-06-17T00:00:00-04:00",
            "title": "Enter NASA's Spacecraft Chamber of Horrors",
            "description": "To prepare for Servicing Mission 4, Hubble components must endure harsh tests at NASA's Goddard Space Flight Center.  This feature explores test facilities at Goddard like: launch phase simulator centrifuge, the acoustic test chamber, electromagnetic interference testing, vibration tables, static load test facility, and the space environment simulator.For complete transcript, click here. || G08-022HD-NASAsChamber-of-horrors-H-iPod02052_print.jpg (1024x576) [84.7 KB] || G08-022HD-NASAsChamber-of-horrors-H-iPod_web.png (320x180) [109.0 KB] || G08-022HD-NASAsChamber-of-horrors-H-iPod_thm.png (80x40) [17.6 KB] || Chamber_of_Horrors_AppleTv.webmhd.webm (960x540) [56.4 MB] || G08-022HD-NASAsChamber-of-horrors-MPEG4-h264.mov (1280x720) [254.1 MB] || Chamber_of_Horrors_AppleTv.m4v (960x540) [140.5 MB] || GSFC_20080617_HST_m10239_Chamber_of_Horrors.mp4 (1280x720) [422.6 MB] || G08-022HD-NASAsChamber-of-horrors-iTunes.m4v (640x360) [34.0 MB] || GSFC_20080617_HST_m10239_Chamber_of_Horrors.en_US.srt [4.5 KB] || GSFC_20080617_HST_m10239_Chamber_of_Horrors.en_US.vtt [4.3 KB] || G08-022HD-NASAsChamber-of-horrors-H-iPod.m4v (320x180) [19.0 MB] || G08-022HD-NASAsChamber-of-horrors-MPEG4.mp4 (512x288) [315.5 MB] || G08-022HD-NASAsChamber-of-horrors-QuickTime.mov (512x288) [151.0 MB] || G08-022HD-NASAsChamber-of-horrors-Sorenson3-MPEG1.mpg (320x240) [61.7 MB] || G08-022HD-NASAsChamber-of-horrors-WindowsMedia.mp4 (512x288) [59.6 MB] || ",
            "hits": 37
        },
        {
            "id": 10257,
            "url": "https://svs.gsfc.nasa.gov/10257/",
            "result_type": "Produced Video",
            "release_date": "2008-06-11T00:00:00-04:00",
            "title": "Return with LRO",
            "description": "The Deputy Project Manager for the Lunar Reconnaissance Orbiter (LRO) program, Cathy Peddie, expresses her personal and professional thoughts on the upcoming LRO mission. || ",
            "hits": 17
        },
        {
            "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": 443
        },
        {
            "id": 10207,
            "url": "https://svs.gsfc.nasa.gov/10207/",
            "result_type": "Produced Video",
            "release_date": "2008-04-20T12:00:00-04:00",
            "title": "NASA Satellites Aid in Chesapeake Bay Recovery",
            "description": "From the distant reaches of the Universe, to black holes, and the Martian surface, NASA explores some of the most far out parts of space. But NASA also does research much closer to home. In fact, NASA Earth Science satellites are taking part in the management and recovery of an ecosystem right in our backyard, the Chesapeake Bay. || ",
            "hits": 20
        },
        {
            "id": 10192,
            "url": "https://svs.gsfc.nasa.gov/10192/",
            "result_type": "Produced Video",
            "release_date": "2008-03-31T12:00:00-04:00",
            "title": "Venus: Long Time, No See",
            "description": "The last U.S. spacecraft mission to Venus was in 1989 with the launch of Magellan. Even though Magellan spent the next five years radar mapping the surface and gathering high resolution gravity data, much remains a mystery about our so-called sister planet. Did Venus experience a run-a-way greenhouse effect at some point in its history? Why is the surface pressure 90 times greater on Venus then on Earth? Why is the planet so hot? These are only a few of the question that must be answered if we are to learn more about Venus's past and possibly Earth's future. || ",
            "hits": 35
        },
        {
            "id": 10188,
            "url": "https://svs.gsfc.nasa.gov/10188/",
            "result_type": "Produced Video",
            "release_date": "2008-03-02T00:00:00-05:00",
            "title": "NASA's SDO Mission",
            "description": "A new NASA spacecraft called the Solar Dynamics Observatory (SDO) will deliver startling images of the sun with ten times more detail than HDTV. The goal of the mission is to help scientists zoom in on solar activity such as sunspots, solar flares and coronal mass ejections, thus improving forcasts of solar storms. The complete script is available. For more information on the Solar Dynamics Observatory, check out their web site at http://sdo.gsfc.nasa.gov. || ",
            "hits": 53
        },
        {
            "id": 3413,
            "url": "https://svs.gsfc.nasa.gov/3413/",
            "result_type": "Visualization",
            "release_date": "2007-05-10T00:00:00-04:00",
            "title": "Towers in the Tempest",
            "description": "This visualization won Honorable Mention in the National Science Foundation's Science and Engineering Visualization Challenge in September 2007. It was also shown during the SIGGRAPH 2008 Computer Animation Festival in Los Angeles, CA. 'Towers in the Tempest' is a 4.5 minute narrated animation that explains recent scientific insights into how hurricanes intensify. This intensification can be caused by a phenomenon called a 'hot tower'. For the first time, research meteorologists have run complex simulations using a very fine temporal resolution of 3 minutes. Combining this simulation data with satellite observations enables detailed study of 'hot towers'. The science of 'hot towers' is described using: observed hurricane data from a satellite, descriptive illustrations, and volumetric visualizations of simulation data. The first section of the animation shows actual data from Hurricane Bonnie observed by NASA's Tropical Rainfall Measuring Mission (TRMM) spacecraft. Three dimensional precipitation radar data reveal a strong 'hot tower' in Hurricane Bonnie's internal structure. The second section uses illustrations to show the dynamics of a hurricane and the formation of 'hot towers'. 'Hot towers' are formed as air spirals inward towards the eye and is forced rapidly upwards, accelerating the movement of energy into high altitude clouds. The third section shows these processes using volumetric cloud, wind, and vorticity data from a supercomputer simulation of Hurricane Bonnie. Vertical wind speed data highlights a 'hot tower'. Arrows representing the wind field move rapidly up into the 'hot tower, boosting the energy and intensifying the hurricane. Combining satellite observations with super-computer simulations provides a powerful tool for studying Earth's complex systems. The complete script is available here . The storyboard is available here . There is also a movie of storyboard drawings with narration below. || ",
            "hits": 67
        }
    ]
}