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    "results": [
        {
            "id": 13195,
            "url": "https://svs.gsfc.nasa.gov/13195/",
            "result_type": "Produced Video",
            "release_date": "2019-04-23T15:00:00-04:00",
            "title": "Goddard Space Flight Center Archival Footage",
            "description": "Footage of cleanroom work, scientists on SOHO, XTE and the STOCC || YOUTUBE_720_GSFC_40_anniversary_b-roll_youtube_720.00361_print.jpg (1024x576) [96.5 KB] || YOUTUBE_720_GSFC_40_anniversary_b-roll_youtube_720.00361_searchweb.png (320x180) [82.5 KB] || YOUTUBE_720_GSFC_40_anniversary_b-roll_youtube_720.00361_thm.png (80x40) [5.8 KB] || GSFC_40_anniversary_b-roll.mov (1280x720) [7.6 GB] || YOUTUBE_720_GSFC_40_anniversary_b-roll_youtube_720.mp4 (1280x720) [1.0 GB] || GSFC_40_anniversary_b-roll.webm [0 bytes] || ",
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        },
        {
            "id": 11602,
            "url": "https://svs.gsfc.nasa.gov/11602/",
            "result_type": "Produced Video",
            "release_date": "2014-07-03T11:00:00-04:00",
            "title": "STEREO Solar Conjunction",
            "description": "Since February 2011, the two spacecraft of NASA's STEREO mission have been providing scientists with unprecedented views of the far side of the sun. Placed in an orbit that allows their perspective to changed over the eight years since their launch in 2008 (ck), the satellites are about to enter a new phase of their journey: a time when the bright light and heat of the sun will stand in the way of sending data back to Earth.This phase is a direct result of the orbits for STEREO, which is short for the Solar Terrestrial Relations Observatory. The spacecraft travel at different speeds. This means that over time, the satellites become increasingly out of sync, appearing from Earth's perspective to drift farther apart, able to observe first the sides and eventually the far side of the sun. For the first time ever, thanks to STEREO and near-Earth solar telescopes such as NASA’s Solar Dynamics Observatory the human race has had its first 360-degree view of the sun.The orbits have continued to cause the STEREO spacecraft's position to change, however, and now they are nearing each other once again, this time on the other side of the sun. During this period when the sun blocks Earth's view — a geometrical position known in astronomy as a superior conjunction — radio receivers on Earth will not be able to distinguish STEREO's signal from the sun's radiation. Communication with the spacecraft will cease and the satellites will both go into safe mode without collecting data for a time. This will happen for STEREO-Ahead from March 24 to July 7, 2015. STEREO-Behind will be in superior conjunction from Jan. 22 to March 23, 2015. At least one spacecraft, therefore, will always be collecting data. Before this occurs, the heating from the sun will also begin to affect – though not shut down — data collection. From wherever they are in space, the STEREO spacecraft aim their antenna toward Earth to send down data. This position puts the antenna fairly close to pointing at the sun, exposing the instruments to more heat than it can safely bear. The antenna can be adjusted to point in different directions, but the signal coming to Earth will be much fainter and won't allow for as much data to be downloaded.  This antenna adjustment will begin on Aug. 20, 2014, for the STEREO-Ahead spacecraft and on Dec. 1, 2014, for STEREO-Behind. During this phase, STEREO instruments will continue to run 24 hours a day, but they will gather lower-resolution data than usual. Some of this data will be downloaded whenever STEREO can link up with an Earth receiver. The rest of the data will be stored on board to be downloaded when the spacecraft reach a more auspicious geometrical position in early 2016. To test for this off-pointing from the sun, STEREO-Ahead will undergo tests and not be collecting data from July 6-12, 2014.  The same tests will be performed on STEREO-Behind from Sept. 29 – Oct. 6, 2014. Throughout this entire phase until 2016, at least one STEREO spacecraft will be capturing data at any one time, so scientists will have an uninterrupted record of events on the sun to coordinate with the observations of solar telescopes on the Earth side. Real time monitoring of the sun, its flares and coronal mass ejections – information used by the US National Oceanic and Atmospheric Administration to help forecast space weather — will also continue via a fleet of NASA spacecraft closer to Earth. || ",
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        },
        {
            "id": 30511,
            "url": "https://svs.gsfc.nasa.gov/30511/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-06-03T00:00:00-04:00",
            "title": "Coccolithophores Near the Patagonia Shelf",
            "description": "Coccolithophores, a type of phytoplankton, are one-celled, microscopic marine plants that live in large numbers throughout the upper layers of the ocean. They surround themselves with minute calcium carbonate plates called “coccoliths,” which are highly reflective such that populations of these plants can be seen from space. Near the Patagonia Shelf, located east of Argentina and Uruguay, ocean waters thrive with high concentrations of microscopic phytoplankton—e.g., coccolithiphores, dinoflagellates, and diatoms to name a few. That is because in this region the warm, saline, southward-flowing Brazil Current flows past and mixes with the cool, less-saline, nutrient-rich northward-flowing Falklands/Malvinas Current, creating an ideal environment for biological productivity. Scientists use true color satellite images like these, taken by Aqua/MODIS from December 15, 2010 to February 15, 2011, to observe the recurring coccolithophore blooms in the Patagonia Shelf region and study the impacts of ocean acidification on these microscopic organisms. Imagery from these two months shows a coccolithophore bloom (turquoise) near the shelf break. The shelf's unique ecosystem supports important fisheries in the region, providing a favorable reproductive habitat for anchovies and sardines. || ",
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        },
        {
            "id": 30362,
            "url": "https://svs.gsfc.nasa.gov/30362/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-22T12:00:00-04:00",
            "title": "Full Map of the Sun's Surface",
            "description": "This movie shows the evolution of the Sun's entire surface as seen in extreme ultraviolet light (304 angstroms)  for the time period Jan 1 - Sep 27, 2012. The movie was made by combining nearly simultaneous view of the Sun from three spacecraft: STEREO AHEAD and BEHIND (seeing the Sun's far side) and the Solar Dynamic Observer (seeing the near side). This EUV light comes primarily from the solar chromosphere.  The bright patches are active regions. Many dark prominence eruptions can also be seen. The data is plotted in Carrington coordinates which are \"fixed\" to the surface of the Sun. In this coordinate system, the active regions tend to stay at the same location.  However, the Sun's rotation rate actually changes with latitude and this can be seen in the movie. || ",
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        }
    ]
}