{
    "count": 7,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 31059,
            "url": "https://svs.gsfc.nasa.gov/31059/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-11-13T00:00:00-05:00",
            "title": "CERES top of Atmosphere Fluxes",
            "description": "These maps show monthly top of atmosphere radiative fluxes from March 2000 to the present from the Energy Balanced and Filled (EBAF) data product. These data are produced by averaging observations collected by the Clouds and the Earth's Radiant Energy System (CERES) sensors on NASA's Aqua and Terra satellites, filling in gaps and constraining the fluxes to remove the inconsistency between average global net TOA flux and heat storage in the Earth-atmosphere system. || ",
            "hits": 127
        },
        {
            "id": 30604,
            "url": "https://svs.gsfc.nasa.gov/30604/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-06-28T00:00:00-04:00",
            "title": "CERES Radiation Fluxes",
            "description": "These maps show monthly reflected-shortwave radiation from March 2000 to the present from the Energy Balanced and Filled (EBAF) data product. These data are produced by averaging observations collected by the Clouds and the Earth's Radiant Energy System (CERES) sensors on NASA's Aqua and Terra satellites, filling in gaps and constraining the fluxes to remove the inconsistency between average global net TOA flux and heat storage in the Earth-atmosphere system. || ",
            "hits": 143
        },
        {
            "id": 30369,
            "url": "https://svs.gsfc.nasa.gov/30369/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-24T12:00:00-04:00",
            "title": "Monthly Net Radiation",
            "description": "The difference between how much solar energy enters the Earth system and how much heat energy escapes into space is called net radiation. Some places absorb more energy than they give off back to space, so they have an energy surplus. Other places lose more energy to space than they absorb, so they have an energy deficit. These maps show monthly net 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 show the net radiation (in Watts per square meter) that was contained in the Earth system. The maps illustrate the fundamental imbalance between net radiation surpluses at the equator (red areas), where sunlight is direct year-round, and net radiation deficits at high latitudes (blue areas), where direct sunlight is seasonal. || ",
            "hits": 128
        },
        {
            "id": 3177,
            "url": "https://svs.gsfc.nasa.gov/3177/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Net Radiation Flux 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 net radiation flux within view of CERES during 29 orbits on June 20 and 21 of 2003. The net flux is the incoming solar flux minus the outgoing reflected (shortwave) and thermal (longwave) radiation. If the flux in a region is positive, the Earth is being warmed by the sun in that region, while cooling regions have a negative flux. It is clear from the animation that the most intensive heating occurs in ocean regions with few clouds, while the second most intense are cloud-free regions over vegetated land areas. Deserts, cloudy regions, and ice caps all reflect enough solar radiation to reduce the amount of heating. Regions of night are, of course, cooling regions because there is no incoming flux at all. || ",
            "hits": 74
        },
        {
            "id": 3093,
            "url": "https://svs.gsfc.nasa.gov/3093/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Clear-sky Net Radiant Flux (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 average amount of reflection and absorption is critical to the climate, because the absorbed energy heats up the Earth until it is radiated away as thermal radiation.  This animation shows the monthly clear-sky average net radiant flux from July, 2002 through June, 2004 as measured by the CERES instrument.  This is  the incoming radiation minus the outgoing reflected or thermal energy given off by areas of the Earth when the sky is cloud-free.  Regions in red and yellow have a net incoming flux and are being heated.  Regions in blue have a net outgoing flux and are being cooled.  Regions in black are in rough equilibrium.  Summertime oceans are heated the most, while high latitude winter regions are cooled the most, probably because of the longer winter nights.  Note that the Earth's ice sheets are almost always regions of  cooling.  On average, the heating and cooling amounts must balance, or the Earth will change temperature and the climate will change. || ",
            "hits": 35
        },
        {
            "id": 3094,
            "url": "https://svs.gsfc.nasa.gov/3094/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Total-sky Net Radiant Flux (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 average amount of reflection and absorption is critical to the climate, because the absorbed energy heats up the Earth until it is radiated away as thermal radiation.  This animation shows the monthly average net radiant flux from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the incoming radiation minus the outgoing reflected or thermal energy given off by areas of the Earth.  Regions in red and yellow have a net incoming flux and are being heated. Regions in blue have a net outgoing flux and are being cooled.  Regions in black are in rough equilibrium.  Cloud-free summertime oceans are heated the most, while high latitude winter regions are cooled the most, probably because of the longer winter nights.  Note that regions that reflect a lot of sunlight, such as the polar ice sheets and the Sahara desert are almost always in equilibrium or are cooling regions. || ",
            "hits": 36
        },
        {
            "id": 3106,
            "url": "https://svs.gsfc.nasa.gov/3106/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Net Radiation Flux (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 net radiation flux within view of CERES during 29 orbits on June 20 and 21 of 2003. The net flux is the incoming solar flux minus the outgoing reflected (shortwave) and thermal (longwave) radiation. If the flux in a region is positive, the Earth is being warmed by the sun in that region, while cooling regions have a negative flux. It is clear from the animation that the most intensive heating occurs in ocean regions with few clouds, while the second most intense are cloud-free regions over vegetated land areas. Deserts, cloudy regions, and ice caps all reflect enough solar radiation to reduce the amount of heating. Regions of night are, of course, cooling regions because there is no incoming flux at all. || ",
            "hits": 33
        }
    ]
}