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    "results": [
        {
            "id": 12522,
            "url": "https://svs.gsfc.nasa.gov/12522/",
            "result_type": "Produced Video",
            "release_date": "2017-02-23T09:00:00-05:00",
            "title": "NASA-funded Balloon Recovered From Antarctica",
            "description": "For 12 days in January 2016, a football-field-sized balloon with a telescope hanging beneath it floated 24 miles above the Antarctic continent, riding the spiraling polar vortex. On Jan. 31, 2016, scientists sent the pre-planned command to cut the balloon – and the telescope parachuted to the ground in the Queen Maud region of Antarctica. The telescope sat on the ice for an entire year. The scientists did quickly recover the data vaults from the NASA-funded mission, called GRIPS, which is short for Gamma-Ray Imager/Polarimeter for Solar flares. But due to incoming winter weather – summer only runs October through February in Antarctica – they had to leave the remaining instruments on the ice and schedule a recovery effort for the following year. Finally, in January 2017, it was warm and safe enough to recover the instruments.For more information visit the NASA.gov feature. || ",
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        },
        {
            "id": 11522,
            "url": "https://svs.gsfc.nasa.gov/11522/",
            "result_type": "Produced Video",
            "release_date": "2014-05-07T12:00:00-04:00",
            "title": "The Best Observed X-class Flare",
            "description": "On March 29, 2014 the sun released an X-class flare. It was observed by NASA's Interface Region Imaging Spectrograph, or IRIS; NASA's Solar Dynamics Observatory, or SDO; NASA's Reuven Ramaty High Energy Solar Spectroscopic Imager, or RHESSI; the Japanese Aerospace Exploration Agency's Hinode; and the National Solar Observatory's Dunn Solar Telescope located at Sacramento Peak in New Mexico. To have a record of such an intense flare from so many observatories is unprecedented.  Such research can help scientists better understand what catalyst sets off these large explosions on the sun. Perhaps we may even some day be able to predict their onset and forewarn of the radio blackouts solar flares can cause near Earth – blackouts that can interfere with airplane, ship and military communications. || ",
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        },
        {
            "id": 4164,
            "url": "https://svs.gsfc.nasa.gov/4164/",
            "result_type": "Visualization",
            "release_date": "2014-05-07T10:00:00-04:00",
            "title": "A Multi-Mission View of a Solar Flare: Optical to Gamma-rays",
            "description": "To improve our understanding of complex phenomena such as solar flares, a wide variety of tools are needed.  In the case of astronomy, those tools enable us to analyze the light in many different wavelengths and many different ways.Many different instruments are observing the Sun almost continuously, both from space and on the surface of the Earth.  On March 29, 2014, the Dunn Solar Telescope at Sacramento Peak, New Mexico was observing a solar active region and requested other observatories to watch as well.  As a result of this coordination, the region was being observed by a large number of different instruments, ground and space-based, when it subsequently erupted with an X-class flare.  This visualization presents various combinations of the datasets collected during this effort.  The color text represents the dominant color of the dataset in the imagery.Solar Dynamics Observatory (SDO): HMI (617.1nm).  This data represents the Sun is visible light similar to how we see it from the ground.Solar Dynamics Observatory (SDO): AIA (17.1nm).  Solar ultraviolet emission, which can only be seen from space, reveals plasma flowing, and escaping, along magnetic fields.IRIS Slit-Jaw Imager: 140.0nm.  This high-resolution imager also contains a slit (the dark vertical line in the center of the field) which directs the light to an ultraviolet spectrometer which is used to extract even more information about the light.  The imager slews back-and-forth across the region, providing spectra over a larger area of the Sun.Hinode/X-ray Telescope: x-ray band. Indicates very hot plasma.RHESSI: 50-100 keV.  High-energy gamma-ray emission.  Emission from these locations represent the very highest energy photons from the flare event.Dunn Solar Telescope: G-band filter.  This filter, showing much of the solar surface (photosphere) in visible light, provides a detailed view of the sunspots and convection cells.  The view moves because the instrument was repointed several times during the observation.Dunn Solar Telescope: IBIS ( Hydrogen alpha, 656.3nm;  Calcium 854.2 nm;  Iron 630.15nm).  This is the small rectangular view within the Dunn Solar Telescope G-band view.  This instrument can tune the wavelength during the observation, which provides views of the solar atmosphere at different depths. || ",
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        }
    ]
}