{
    "count": 4,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 30357,
            "url": "https://svs.gsfc.nasa.gov/30357/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-12-22T12:00:00-05:00",
            "title": "Computer-simulated Global View of Venus",
            "description": "This global view of the surface of Venus is centered at 180 degrees east longitude. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneer Venus Orbiter data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. || ",
            "hits": 98
        },
        {
            "id": 30358,
            "url": "https://svs.gsfc.nasa.gov/30358/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-22T12:00:00-04:00",
            "title": "Hemispheric View of Venus",
            "description": "The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered at 180 degrees east longitude. The Magellan spacecraft imaged more than 98 percent of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km. A mosaic of the Magellan images (most with illumination from the west) forms the image base. Gaps in the Magellan coverage were filled with images from the Earth-based Arecibo radar in a region centered roughly on 0 degree latitude and longitude, and with a neutral tone elsewhere (primarily near the south pole). The composite image was processed to improve contrast and to emphasize small features, and was color-coded to represent elevation. Gaps in the elevation data from the Magellan radar altimeter were filled with altimetry from the Venera spacecraft and the U.S. Pioneer Venus missions. An orthographic projection was used, simulating a distant view of one hemisphere of the planet. || ",
            "hits": 391
        },
        {
            "id": 30173,
            "url": "https://svs.gsfc.nasa.gov/30173/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "Observing wildfires using UAVSAR",
            "description": "Synthetic aperture radar systems that are able to transmit and receive multiple polarizations may provide useful information to help combat, and possibly detect, wildfires as this image of the 2009 Station Fire in the Angeles National Forest shows. The data shown here in a grayscale overlay represent the change in the component of the radar scattering that is attributable to leafy vegetation, with lighter shading representing greater changes than darker shading. The blue outline delineates the boundary of the total burned zone as determined by an independent survey conducted by the U.S. Forest Service.  The radar data were collected by NASA's Uninhabited Aerial Vehicle Synthetic Aperture Radar system on February 27 and September 18, 2009 while most of the damage from the Station Fire occurred between August 26 and September 4, 2009. || ",
            "hits": 15
        },
        {
            "id": 4007,
            "url": "https://svs.gsfc.nasa.gov/4007/",
            "result_type": "Visualization",
            "release_date": "2012-12-12T00:00:00-05:00",
            "title": "Ground-Penetrating Radar Measurements of Antarctic Ice Sheet",
            "description": "This visualization presents data collected by the 2010 Satellite Era Accumulation Traverse (SEAT). Accumulation, the amount of snow that falls on an ice sheet, is one of the most important inputs for determining the mass balance of an ice sheet. There are, however, relatively few direct accumulation measurements because the most precise measurements come from ice cores at a single point location.Recently, new large-bandwidth, very-high frequency radars have been developed and used over the ice sheets to image internal layers in the near surface which represent about the past 30-40 years of accumulation. The SEAT traverses are making the link between near surface radar layers and ice cores by collecting both simultaneously across the West Antarctic Ice Sheet Divide region. || ",
            "hits": 51
        }
    ]
}