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        {
            "id": 11840,
            "url": "https://svs.gsfc.nasa.gov/11840/",
            "result_type": "Produced Video",
            "release_date": "2015-05-05T11:00:00-04:00",
            "title": "Solar Vibrations",
            "description": "Images from space reveal the chaotic motions on the surface of the sun. || c-1280.jpg (1280x720) [204.6 KB] || c-1024.jpg (1024x576) [136.5 KB] || c-1024_print.jpg (1024x576) [123.1 KB] || c-1024_searchweb.png (320x180) [50.0 KB] || ",
            "hits": 88
        },
        {
            "id": 3940,
            "url": "https://svs.gsfc.nasa.gov/3940/",
            "result_type": "Visualization",
            "release_date": "2012-06-12T00:00:00-04:00",
            "title": "Venus Transit 2012 from Solar Dynamics Observatory",
            "description": "Full disk and Tracking views of Venus Transit from Solar Dynamics Observatory (SDO). It includes images taken by the Helioseismic and Magnetic Imager (HMI) and the Atmospheric Imaging Assembly (AIA).These are the basic images, collected from the telemetry. To see the insets composited, see Venus Transit 2012 Composited Visuals. || ",
            "hits": 74
        },
        {
            "id": 10733,
            "url": "https://svs.gsfc.nasa.gov/10733/",
            "result_type": "Produced Video",
            "release_date": "2011-03-03T16:00:00-05:00",
            "title": "SDO First Light Media",
            "description": "A compilation of some of the videos and stills used during the SDO First Light press conference.There are more video and stills available. || ",
            "hits": 68
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        {
            "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": 30
        },
        {
            "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": 58
        },
        {
            "id": 3697,
            "url": "https://svs.gsfc.nasa.gov/3697/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Magnetogram Full Disk View - March 29, 2010",
            "description": "This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.The black and white region slightly above the center corresponds to a visible sunspot.  Weaker magnetic regions are visible around the disk. || ",
            "hits": 46
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        {
            "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. || ",
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        {
            "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": 42
        },
        {
            "id": 3705,
            "url": "https://svs.gsfc.nasa.gov/3705/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Magnetogram Sunspot Close-Up - March 29, 2010",
            "description": "This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.This version is a close-up view of a large sunspot group. || ",
            "hits": 45
        },
        {
            "id": 3706,
            "url": "https://svs.gsfc.nasa.gov/3706/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Magnetogram Sunspot Zoom-In - March 29, 2010",
            "description": "This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Grey is zero magnetic field.This movie zooms-in on a large sunspot group. || ",
            "hits": 26
        },
        {
            "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": 88
        },
        {
            "id": 3713,
            "url": "https://svs.gsfc.nasa.gov/3713/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Magnetogram Full Disk View - April 7, 2010",
            "description": "This early sequence of images from the HMI imager is processed to reveal the magnetic field structure (magnetogram). White locations represent a positive magnetic field value (north polarity) while black represents a negative magnetic field value (south polarity). Gray is zero magnetic field.Notice that the surface magnetic fields reveal much more structure than the white-light images in SDO/HMI Continuum Full Disk View - April 7, 2010. || ",
            "hits": 30
        },
        {
            "id": 3714,
            "url": "https://svs.gsfc.nasa.gov/3714/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/HMI Dopplergram Sunspot Close-Up - March 29, 2010",
            "description": "The dopplergram from SDO/HMI data shows the velocity of solar material on the line-of-sight. White pixels are moving away from the camera and black pixels are moving towards the camera. || ",
            "hits": 17
        },
        {
            "id": 3386,
            "url": "https://svs.gsfc.nasa.gov/3386/",
            "result_type": "Visualization",
            "release_date": "2006-11-08T00:00:00-05:00",
            "title": "Mercury Transit from SOHO/MDI",
            "description": "This is a view of the planet Mercury (the tiny moving black dot) as seen by the SOHO MDI.The narrow field-of-view for this camera mode necessitates the addition of black bars at the top and bottom of the frame to match HD720 resolution.This movie was generated from telemetry which has undergone a minimum of processing (to deliver quickly for the media) so data dropouts and other quick-processing artifacts may be visible. Special thanks to Steele Hill of the SOHO project for this effort. || ",
            "hits": 41
        },
        {
            "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": 27
        },
        {
            "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": 21
        },
        {
            "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
        },
        {
            "id": 2243,
            "url": "https://svs.gsfc.nasa.gov/2243/",
            "result_type": "Visualization",
            "release_date": "2001-11-06T13:00:00-05:00",
            "title": "SOHO/MDI Views the Sun - 1998",
            "description": "This version projects the solar image on a sphere for improved perspective. || Movie of the solar disk from April 30 to June 24, 1998. || a002243.00020_print.png (720x480) [376.5 KB] || FullDisk1998_pre.jpg (320x240) [4.6 KB] || a002243.webmhd.webm (960x540) [712.6 KB] || a002243.dv (720x480) [30.9 MB] || FullDisk1998.mpg (320x240) [922.3 KB] || ",
            "hits": 28
        },
        {
            "id": 2244,
            "url": "https://svs.gsfc.nasa.gov/2244/",
            "result_type": "Visualization",
            "release_date": "2001-11-06T13:00:00-05:00",
            "title": "SOHO/MDI Views the Sun - 2001",
            "description": "This version projects the solar image on a sphere for improved perspective. || SOHO-MDI views the Sun from March 1 to May 31, 2001. || a002244.00095_print.png (720x480) [393.7 KB] || FD2001_pre.jpg (320x238) [4.6 KB] || a002244.webmhd.webm (960x540) [4.2 MB] || a002244.dv (720x480) [157.8 MB] || FD2001.mpg (352x240) [6.3 MB] || ",
            "hits": 27
        },
        {
            "id": 2268,
            "url": "https://svs.gsfc.nasa.gov/2268/",
            "result_type": "Visualization",
            "release_date": "2001-11-06T13:00:00-05:00",
            "title": "SOHO/MDI Views the Sun - 1998",
            "description": "This version projects the solar image on a flat plane. It runs at a third of the speed of the original version. || SOHO-MDI images the sun from April 30 to June 24, 1998. || a002268.00095_print.png (720x480) [363.2 KB] || a002268_pre.jpg (320x240) [4.3 KB] || a002268.webmhd.webm (960x540) [1.5 MB] || a002268.dv (720x480) [75.5 MB] || a002268.mpg (320x240) [995.0 KB] || ",
            "hits": 52
        },
        {
            "id": 2269,
            "url": "https://svs.gsfc.nasa.gov/2269/",
            "result_type": "Visualization",
            "release_date": "2001-11-06T13:00:00-05:00",
            "title": "SOHO/MDI Views the Sun - 2001",
            "description": "This version projects the solar image on a flat plane. || A view of the Sun from SOHO-MDI from March thru May 2001. || a002269.00095_print.png (720x480) [379.6 KB] || Sunspots2001_pre.jpg (320x238) [4.2 KB] || a002269.webmhd.webm (960x540) [3.6 MB] || a002269.dv (720x480) [157.8 MB] || Sunspots2001.mpg (352x240) [6.3 MB] || ",
            "hits": 40
        }
    ]
}