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        {
            "id": 4613,
            "url": "https://svs.gsfc.nasa.gov/4613/",
            "result_type": "Visualization",
            "release_date": "2018-01-31T00:00:00-05:00",
            "title": "JPSS Concept of Operations: Constellation Management",
            "description": "This visualization illustrates how JPSS-1 (now NOAA-20) orbit phasing and raising works relative to SNPP, the notional way SNPP can be maneuvered a quarter-orbit along-track separation from JPSS-1 prior to launch of JPSS-2, and how a three-satellite constellation operates on a sun-synchronous orbit node-crossing including sensor-swath footprints as the world turns below.This video is also available on our YouTube channel. || jpss_constellationManagement_05235_print.jpg (1024x576) [65.1 KB] || jpss_constellationManagement_05235_searchweb.png (320x180) [54.3 KB] || jpss_constellationManagement_05235_thm.png (80x40) [4.3 KB] || JPSS_constellationManagement_Full (1920x1080) [0 Item(s)] || jpss_constellationManagement_full_1080p30.webm (1920x1080) [34.8 MB] || jpss_constellationManagement_full_1080p30.mp4 (1920x1080) [250.4 MB] || jpss_constellationManagement_full_1080p30.mp4.hwshow [207 bytes] || ",
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        {
            "id": 4618,
            "url": "https://svs.gsfc.nasa.gov/4618/",
            "result_type": "Visualization",
            "release_date": "2018-01-31T00:00:00-05:00",
            "title": "Geostationary Operational Environmental Satellite (GOES) East and West",
            "description": "This animation depicts the areas of the Earth viewed by GOES-East and GOES-West from their vantage point 22,236 miles above the equator.This video is also available on our YouTube channel. || goes_EastWest.000945_print.jpg (1024x576) [50.9 KB] || goes_EastWest.000945_searchweb.png (320x180) [48.6 KB] || goes_EastWest.000945_thm.png (80x40) [2.9 KB] || goes_EastWest (1920x1080) [0 Item(s)] || goes_EastWest_1080p30.mp4 (1920x1080) [48.2 MB] || goes_EastWest_1080p30.webm (1920x1080) [6.5 MB] || goes_EastWest_1080p30.mp4.hwshow [187 bytes] || ",
            "hits": 220
        },
        {
            "id": 3969,
            "url": "https://svs.gsfc.nasa.gov/3969/",
            "result_type": "Visualization",
            "release_date": "2012-09-20T00:00:00-04:00",
            "title": "The 2012 Earth-Orbiting Heliophysics Fleet",
            "description": "Since Sentinels of the Heliosphere in 2008, there have been a few new missions, and a few missions have been shut down. As of Fall of 2012, here's a tour of the NASA Near-Earth Heliophysics fleet, covering the space from near-Earth orbit out to the orbit of the Moon.Revision (November 9, 2012): The RBSP mission has been renamed the Van Allen Probes. NASA Press Release.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observationsNear-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. SORCE: Monitors solar intensity across a broad range of the electromagnetic spectrum.AIM: Images and measures noctilucent clouds. SVS pageRBSP: (Renamed the Van Allen Probes) Designed to study the impact of space weather on Earth's radiation belts. SVS pageGeosynchronous Fleet:SDO: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution.GOES: The newest GOES satellites include a solar X-ray imager operated by NOAA.Geospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of three satellites to study how magnetospheric instabilities produce substorms. Two of the original five satellites were moved into lunar orbit to become ARTEMIS. SVS page IBEX: The Interstellar Boundary Explorer measures the flux of neutral atoms from the heliopause.Lunar Orbiting FleetARTEMIS: Two of the THEMIS satellites were moved into lunar orbit to study the interaction of the Earth's magnetosphere with the Moon.Note: A number of near-Earth missions had their orbits generated from Two-Line orbital elements valid in July 2012. Orbit perturbations since then may result in significant deviation from the actual satellite position for the time frame of this visualization. || ",
            "hits": 35
        },
        {
            "id": 3994,
            "url": "https://svs.gsfc.nasa.gov/3994/",
            "result_type": "Visualization",
            "release_date": "2012-09-20T00:00:00-04:00",
            "title": "RBSP & SDO: Newest Heliophysics Missions",
            "description": "The newest members of NASA's Heliophysics fleet are the Solar Dynamics Observatory (SDO), launched February 11, 2010, and the Radiation Belt Storm Probes (RBSP), launched August 23, 2012.Revision (November 9, 2012): The RBSP mission has been renamed the Van Allen Probes. NASA Press Release. || ",
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        }
    ]
}