{
    "count": 4,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 30603,
            "url": "https://svs.gsfc.nasa.gov/30603/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-06-25T00:00:00-04:00",
            "title": "CERES Cloud Radiative Effect",
            "description": "CERES Net Cloud Radiative Effect || ceres_net_cre_average_2000-2015_print.jpg (1024x574) [102.2 KB] || ceres_net_cre_average_2000-2015.png (4104x2304) [2.1 MB] || ceres_net_cre_average_2000-2015_searchweb.png (320x180) [69.4 KB] || ceres_net_cre_average_2000-2015_thm.png (80x40) [6.5 KB] || ceres_net_cre_average_2000-2015_30603.pptx [3.0 MB] || ceres_net_cre_average_2000-2015_30603.key [5.6 MB] || ",
            "hits": 140
        },
        {
            "id": 30370,
            "url": "https://svs.gsfc.nasa.gov/30370/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-24T12:00:00-04:00",
            "title": "Monthly Reflected Shortwave Radiation",
            "description": "If you look at Mars in the night sky, the planet is little more than a glowing dot. From Mars, Earth would have the same star-like appearance. What gives the planets this light? Do they shine like a star? No. The light is mostly reflected sunlight. These images show how much sunlight Earth reflects. Bright parts of Earth like snow, ice, and clouds, reflect the most light; dark surfaces, like the oceans, reflect less light. Earth's average temperature is determined by the balance between how much sunlight Earth reflects, how much it absorbs, and how much heat it gives off. These maps show monthly reflected-shortwave radiation from July 2006 to the present, from the Fast Longwave And Shortwave Radiative Fluxes, or FLASHFlux, Time Interpolation and Spatial Averaging (TISA) data product. The product contains daily observations collected by the Clouds and the Earth's Radiant Energy System (CERES) sensors on NASA's Aqua and Terra satellites. The colors in the map show the amount of shortwave energy (in Watts per square meter) that was reflected by the Earth system. The brighter, whiter regions show where more sunlight is reflected, while green regions show intermediate values, and blue regions are lower values. || ",
            "hits": 93
        },
        {
            "id": 3179,
            "url": "https://svs.gsfc.nasa.gov/3179/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Scene Identification Compared to Clouds (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere. As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights. The amount of reflection and absorption is critical to the climate. An instrument named CERES orbits the Earth every 99 minutes and measures the reflected solar energy. This animation shows the scene identification as measured by CERES during 29 orbits on June 20 and 21 of 2003. By comparing the incoming solar radiation with the outgoing reflected and thermal radiation, it is possible to identify the type of area being viewed, whether it be land, clouds, ocean, or ice. This scene identification is used together with the radiation flux measurements to build up a complete picture of the Earth's energy budget over time. || ",
            "hits": 10
        },
        {
            "id": 3104,
            "url": "https://svs.gsfc.nasa.gov/3104/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Scene Identification (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere. As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights. The amount of reflection and absorption is critical to th e climate. An instrument named CERES orbits the Earth every 99 minutes and measures the reflected solar energy. This animation shows the scene identification as measured by CERES during 29 orbits on June 20 and 21 of 2003. By comparing the incoming solar radiation with the outgoing reflected and thermal radiation, it is possible to identify the type of area being viewed, whether it be land, clouds, ocean, or ice. This scene identification is used together with the radiation flux measurements to build up a complete picture of the Earth's energy budget over time. || ",
            "hits": 20
        }
    ]
}