{
    "count": 19,
    "next": null,
    "previous": null,
    "results": [
        {
            "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": 91
        },
        {
            "id": 10610,
            "url": "https://svs.gsfc.nasa.gov/10610/",
            "result_type": "Produced Video",
            "release_date": "2010-04-28T11:00:00-04:00",
            "title": "SDO First Light High Resolution Stills",
            "description": "Stills from the AIA instrument on SDO. They show the March 30, 2010 \"First Light\" prominence eruption captured just after the AIA sensors were activated. All images are from the ultraviolet part of the spectrum, specifically the wavelengths of 304, 211, 193, and 171 Ångstroms. The stills are in multiple resolutions and are available as tiff and jpeg files. || ",
            "hits": 109
        },
        {
            "id": 3692,
            "url": "https://svs.gsfc.nasa.gov/3692/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/AIA CME Event of April 8, 2010 (Multiband)",
            "description": "This is a close-up view of the April 8 CME in ultraviolet light which reveals a wave (darker regions) expanding outward from the flare event. This movie creates a color image by combining filters for 211 Ångstroms (red), 193 Ångstroms (green) and 171 Ångstroms (blue). || ",
            "hits": 33
        },
        {
            "id": 3693,
            "url": "https://svs.gsfc.nasa.gov/3693/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/AIA Zoom-In on Launching Filament (Bands 304, 171, 211)",
            "description": "As the AIA camera was activated, one of its first views was this fliament launching from the Sun. || ",
            "hits": 33
        },
        {
            "id": 3695,
            "url": "https://svs.gsfc.nasa.gov/3695/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/AIA CME Event of April 8, 2010 Full Disk (Multiband)",
            "description": "This visualization is a full-disk view of the CME launched from the Sun on April 8, 2010. This is a 3-color image produced by combining three different filters from the AIA instrument: 211 (red), 193 (green), and 171 (blue). || ",
            "hits": 34
        },
        {
            "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": 66
        },
        {
            "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": 58
        },
        {
            "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": 38
        },
        {
            "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": 32
        },
        {
            "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": 49
        },
        {
            "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": 20
        },
        {
            "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": 70
        },
        {
            "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": 38
        },
        {
            "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": 31
        },
        {
            "id": 3715,
            "url": "https://svs.gsfc.nasa.gov/3715/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/AIA Close-up on Launching Filament (band 304)",
            "description": "A close-up view of the filament launch in the 304 band, which corresponds to a wavelength of about 304 Ångstroms. || ",
            "hits": 26
        },
        {
            "id": 3716,
            "url": "https://svs.gsfc.nasa.gov/3716/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/AIA Full-Disk View of Launching Filament (Band 304)",
            "description": "Full disk view of a filament launch in the SDO AIA 304 band. || ",
            "hits": 45
        },
        {
            "id": 3717,
            "url": "https://svs.gsfc.nasa.gov/3717/",
            "result_type": "Visualization",
            "release_date": "2010-04-21T14:15:00-04:00",
            "title": "SDO/AIA Zoom-out of Launching Filament (Band 304)",
            "description": "This view of the filament launch loops several times before pulling out to show the full solar disk. || ",
            "hits": 30
        },
        {
            "id": 3691,
            "url": "https://svs.gsfc.nasa.gov/3691/",
            "result_type": "Visualization",
            "release_date": "2010-03-31T00:00:00-04:00",
            "title": "A Comparative View of the Sun: SDO/AIA 193 and SOHO/EIT 195",
            "description": "This movie compares the spatial and temporal resolutions of the SDO/AIA (Atmospheric Imaging Assembly) imager to the SOHO/EIT (Extreme ultraviolet Imaging Telescope) imager. SOHO/EIT's highest resolution is 1024x1024 pixels with images taken about every 12 minutes for the 195 Ångstrom band. The SDO/AIA 193 band takes images at 4096x4096 pixels every twelve seconds!In this movie we can see the difference this makes for a closeup view of Active Region 1087. EIT reveals changes in the active region, which AIA reveals many details.This visualization is a companion piece to A Comparative View of the Sun: SDO/AIA 193 and STEREO-B/EUVI 195. || ",
            "hits": 61
        },
        {
            "id": 3694,
            "url": "https://svs.gsfc.nasa.gov/3694/",
            "result_type": "Visualization",
            "release_date": "2010-03-24T00:00:00-04:00",
            "title": "A Comparative View of the Sun: SDO/AIA 193 and STEREO-B/EUVI 195",
            "description": "This movie compares the spatial and temporal resolutions of the SDO/AIA (Atmospheric Imaging Assembly) imager to the STEREO/EUVI (Extreme UltraViolet Imager) imager. STEREO-B/EUVI's highest resolution is 2048x2048 pixels with images taken about every 5 minutes for the 195 Ångstrom band. The SDO/AIA 193 band takes images at 4096x4096 pixels every twelve seconds!While STEREO's vantage point at this time is very different from SDO, we can still identify some features of the Active Region 1087 in these two views. EUVI shows the launch of the filament, while AIA reveals many finer details.This visualization is a companion piece to A Comparative View of the Sun: SDO/AIA 193 and SOHO/EIT 195. || ",
            "hits": 52
        }
    ]
}