{
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    "next": null,
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    "results": [
        {
            "id": 14228,
            "url": "https://svs.gsfc.nasa.gov/14228/",
            "result_type": "Produced Video",
            "release_date": "2022-10-31T11:00:00-04:00",
            "title": "Clouds 101",
            "description": "Complete transcript available. || Screen_Shot_2022-10-19_at_1.52.39_PM_print.jpg (1024x578) [66.1 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM.png (2844x1607) [3.9 MB] || Clouds_101_Lock.00001_searchweb.png (320x180) [34.8 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM_searchweb.png (320x180) [66.0 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM_web.png (320x180) [66.4 KB] || Screen_Shot_2022-10-19_at_1.52.39_PM_thm.png (80x40) [8.7 KB] || Clouds_101_audio_otter_ai.en_US.srt [9.6 KB] || Clouds_101_audio_otter_ai.en_US.vtt [9.6 KB] || Clouds_101_Lock.mp4 (1920x1080) [974.5 MB] || ",
            "hits": 41
        },
        {
            "id": 30396,
            "url": "https://svs.gsfc.nasa.gov/30396/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-24T12:00:00-04:00",
            "title": "Monthly Cirrus Reflectance (Aqua/MODIS)",
            "description": "Cirrus clouds are thin, wispy clouds high in the sky that can be hard to see with the unaided eye. They typically form at an altitude of 6000 meters (20,000 feet) or higher, where the air temperature is below freezing. Cirrus clouds are composed mostly of tiny ice crystals. They are scientifically interesting because they allow most incoming sunlight to pass through them, but they help to contain heat emitted from the surface. Thus, cirrus clouds exert a warming influence on Earth's surface. These maps show monthly average cirrus cloud fraction over the Earth from July 2002 to the present, produced using data collected by the Moderate Resolution Imaging Spectroradiometer (MODIS) instrument onboard NASA's Aqua satellite. The MODIS sensor has a unique band for measuring infrared light at a wavelength of 1.38 micrometers—a wavelength that NASA scientists recently found is highly sensitive to cirrus. Bright white pixels indicate regions completely covered by cirrus clouds. Greyish-white pixels show partial cirrus cover and dark pixels indicate little or no cirrus. || ",
            "hits": 91
        },
        {
            "id": 3436,
            "url": "https://svs.gsfc.nasa.gov/3436/",
            "result_type": "Visualization",
            "release_date": "2007-07-05T00:00:00-04:00",
            "title": "CloudSat, Calipso and MODIS over Central America",
            "description": "Associated with tropical thunderstorms are broad fields of cirrus clouds that flow out of the tops of the vigorous storm systems that form over warm tropical oceans. These clouds play a role in how much infrared energy is trapped in Earth's atmosphere. NASA's Tropical Composition, Cloud and Climate Coupling (TC4) mission, which runs from July 16, 2007 through August 8, 2007, aims to document the full lifecycle of these clouds. Observations from four A-Train satellites flying in formation will complement the aircraft measurements with large-scale views of many different features of the atmosphere. Observations from this mission along with previous studies will improve our understanding of what effect a warming climate with rising ocean temperatures will have on these cloud systems. These images over Central America, produced in support of the TC4 mission, show a tropical storm system over Central and South America on August 2, 2006 as measured from multiple satellite sensors, including Aqua MODIS, CloudSat and CALIPSO. In this view from the Pacific Ocean, Panama is on the left and South America is shown on the right. In the following series of still images, each satellite's measurement is shown individually and in combination with the others from the same camera viewpoint. The profile showing CloudSat and CALIPSO data is truncated at a height of twenty kilometers and exaggerated ten times. The land topography is also exaggerated by a factor of ten. || ",
            "hits": 33
        },
        {
            "id": 3175,
            "url": "https://svs.gsfc.nasa.gov/3175/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Outgoing Shortwave 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 reflected solar radiation measured by CERES during 29 orbits on June 20 and 21 of 2003 over infrared cloud images for the same period. Reflected solar radiation is shortwave radiation, and the most intense reflection comes from clouds. || ",
            "hits": 15
        },
        {
            "id": 3178,
            "url": "https://svs.gsfc.nasa.gov/3178/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Incoming Solar 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 incoming solar radiation within view of CERES during 29 orbits on June 20 and 21 of 2003. Because this is incoming solar flux, its magnitude only depends on the position of the sun, and, because the orbit is synchronized with the sun, the orbit crosses the equator in the daylight at about 1:30 PM local time on every orbit. This data is not actually measured from CERES, but is calculated to compare with the outgoing radiation that CERES does measure. Note that the infrared cloud image shown under the solar data shows high infrared as dark (land) and low infrared as light (clouds). || ",
            "hits": 61
        },
        {
            "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": 15
        },
        {
            "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": 9
        }
    ]
}