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    "results": [
        {
            "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": 157
        },
        {
            "id": 10551,
            "url": "https://svs.gsfc.nasa.gov/10551/",
            "result_type": "Produced Video",
            "release_date": "2010-06-10T00:00:00-04:00",
            "title": "SDO First Light Press Conference",
            "description": "A unique NASA spacecraft launched February 11, 2010, called the Solar Dynamics Observatory, or SDO, has started delivering images of the sun that have astonished scientists. SDO is the most advanced spacecraft ever designed to study the sun and its dynamic behavior. The spacecraft can produce images with clarity ten times better than high definition television and provide more comprehensive science data faster than any solar observing spacecraft in history. The goal of the mission is to help scientists study solar activity to improve forecasts of how the sun affects Earth.On April 21, 2010, NASA held a live press conference at the Newseum in Washington D.C. to unveil the first images and videos from SDO—SDO's First Light.A version of the press conference with captioning is available. || ",
            "hits": 29
        },
        {
            "id": 3696,
            "url": "https://svs.gsfc.nasa.gov/3696/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Continuum Full Disk View - March 29, 2010",
            "description": "This early sequence of HMI images from SDO focuses on a large sunspot group of Solar Cycle 24. || ",
            "hits": 53
        },
        {
            "id": 3703,
            "url": "https://svs.gsfc.nasa.gov/3703/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Continuum Sunspot Closeup - March 29, 2010",
            "description": "This is a close-up view of a large sunspot group visible as the HMI instrument turned on their imagers. || ",
            "hits": 26
        },
        {
            "id": 3704,
            "url": "https://svs.gsfc.nasa.gov/3704/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Continuum Sunspot Zoom-in - March 29, 2010",
            "description": "This is a zoom-in view of a large sunspot group visible as the HMI instrument turned on their imagers. || ",
            "hits": 38
        },
        {
            "id": 3712,
            "url": "https://svs.gsfc.nasa.gov/3712/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Continuum Full Disk View - April 7, 2010",
            "description": "This early sequence of HMI images from SDO focuses on a large sunspot group of Solar Cycle 24. || ",
            "hits": 76
        },
        {
            "id": 10583,
            "url": "https://svs.gsfc.nasa.gov/10583/",
            "result_type": "Produced Video",
            "release_date": "2010-03-16T00:00:00-04:00",
            "title": "Slices Through the Solar Interior",
            "description": "Scientists using SOHO/MDI data have looked just below the Sun's surface and clearly observed inward flowing material.The strong magnetic fields in the sunspots promote cooling. Cool material contracts and sinks at speeds of up to 3000 miles per hour. This drives an inward flow, like a planet-sized whirlpool, that holds the sunspot together as long as the field is strong enough. Scientists discovered this using a technique called acoustic tomography - a novel method similar to ultrasound diagnostics in medicine that uses sound waves to image structures inside the human body. Scientists also found that sunspots are surprisingly shallow. Conditions in sunspots change from cooler than the surrounding plasma to hotter than the surrounding plasma just 3000 miles below the surface. The cool part of a sunspot has the shape of a stack of two or three nickels. Sunspot magnetic fields block the flows that carry heat energy up from the hot solar interior. That results in higher temperatures below the blockage and cooler temperatures above. The downward flows mentioned above dissipate at the same depth. With these data one cannot get a sharp enough picture to really explain the details. Understanding sunspots is essential for understanding the 11-year solar cycle, solar flare explosions, and huge coronal mass ejections that affect life and society on Earth. || ",
            "hits": 54
        },
        {
            "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": 45
        },
        {
            "id": 3336,
            "url": "https://svs.gsfc.nasa.gov/3336/",
            "result_type": "Visualization",
            "release_date": "2006-04-01T00:00:00-05:00",
            "title": "The Visible Sun Revisited",
            "description": "Scientists working with the SOHO/MDI instrument have continued to improve on previous results. Since the first release (SOHO/MDI's 'Window' Through the Sun), improvements in helioseismology techniques have enabled them to extract more information from the same data. In this case, sonogram-type imaging of the solar far side (the side of the Sun NOT facing the Earth) has been improved to provide a more complete view of the farside. This is important in space weather forecasting as it enables us to see large sunspots and active regions before they are visible directly from the Earth. Active regions are a source of solar flares which can send high-energy protons towards the Earth. These protons can damage satellite electronics, endangering communications and weather forecasting, and are a health threat to astronauts. || ",
            "hits": 35
        },
        {
            "id": 2923,
            "url": "https://svs.gsfc.nasa.gov/2923/",
            "result_type": "Visualization",
            "release_date": "2004-03-08T12:00:00-05:00",
            "title": "SOHO/MDI's 'Window' Through the Sun",
            "description": "Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. || ",
            "hits": 27
        },
        {
            "id": 2304,
            "url": "https://svs.gsfc.nasa.gov/2304/",
            "result_type": "Visualization",
            "release_date": "2001-12-10T11:30:00-05:00",
            "title": "Under the Rotating Sunspot (Layers 0, 1, 2)",
            "description": "Using the SOHO Michelson Doppler Interferometer (MDI), scientists can use a process called Time-Distance helioseismology to determine temperatures and fluid flows under the surface of the Sun. || ",
            "hits": 11
        },
        {
            "id": 2314,
            "url": "https://svs.gsfc.nasa.gov/2314/",
            "result_type": "Visualization",
            "release_date": "2001-12-10T11:30:00-05:00",
            "title": "Temperature and Flows under a Sunspot (Layers 0, 2, 4)",
            "description": "Using the SOHO Michelson Doppler Interferometer (MDI), scientists can use a process called Time-Distance helioseismology to determine temperatures and fluid flows under the surface of the Sun. || ",
            "hits": 15
        },
        {
            "id": 2232,
            "url": "https://svs.gsfc.nasa.gov/2232/",
            "result_type": "Visualization",
            "release_date": "2001-11-06T13:00:00-05:00",
            "title": "SOHO/MDI Investigates Solar Flows Under Sunspots",
            "description": "SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot.  Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. || ",
            "hits": 34
        }
    ]
}