{
    "count": 10,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 4898,
            "url": "https://svs.gsfc.nasa.gov/4898/",
            "result_type": "Visualization",
            "release_date": "2022-11-23T00:00:00-05:00",
            "title": "Heliophysics Sentinels 2022",
            "description": "There has been one significant change since the 2020 Heliophysics Fleet.  SET has been decommissioned.  As of Fall 2022, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ",
            "hits": 33
        },
        {
            "id": 4887,
            "url": "https://svs.gsfc.nasa.gov/4887/",
            "result_type": "Visualization",
            "release_date": "2021-03-01T10:00:00-05:00",
            "title": "Heliophysics Sentinels 2020 (Forecast Version)",
            "description": "In addition to the NASA missions used in research for space weather (see 2020 Heliophysics Fleet) there are additional missions operated by NOAA used for space weather forecasting.  As of spring 2020, here's a tour of the NASA and NOAA Heliophysics fleets from the near-Earth satellites out to the inner solar system.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ",
            "hits": 25
        },
        {
            "id": 4822,
            "url": "https://svs.gsfc.nasa.gov/4822/",
            "result_type": "Visualization",
            "release_date": "2020-09-15T10:00:00-04:00",
            "title": "Heliophysics Sentinels 2020",
            "description": "There have been few changes since the 2018 Heliophysics Fleet.  Van Allen Probes and SORCE have been decommissioned, while Solar Orbiter, ICON and SET have been added.  As of spring 2020, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ",
            "hits": 20
        },
        {
            "id": 4360,
            "url": "https://svs.gsfc.nasa.gov/4360/",
            "result_type": "Visualization",
            "release_date": "2018-12-10T11:00:00-05:00",
            "title": "Heliophysics Sentinels 2018",
            "description": "This movie presents the trajectories of the heliophysics fleet from close to Earth to out beyond the heliopause. || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_print.jpg (1024x576) [74.5 KB] || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_searchweb.png (180x320) [65.6 KB] || Sentinels2018.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_thm.png (80x40) [5.1 KB] || Sentinels2018.Sentinels2Voyager_1080p30.mp4 (1920x1080) [40.3 MB] || Sentinels2018.Sentinels2Voyager_1080p30.webm (1920x1080) [6.3 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || Sentinels2018.Sentinels2Voyager_2160p30.mp4 (3840x2160) [125.7 MB] || Sentinels2018.Sentinels2Voyager_1080p30.mp4.hwshow || ",
            "hits": 41
        },
        {
            "id": 4595,
            "url": "https://svs.gsfc.nasa.gov/4595/",
            "result_type": "Visualization",
            "release_date": "2017-11-27T10:00:00-05:00",
            "title": "Mapping Particle Injections in Earth's Magnetosphere",
            "description": "A view from above the northern hemisphere of particle injection propagation constructed from their respective satellite detections.  Distinct injections, and their detection by satellites, are represented by different colors. || MagnetosphereMultiMission.top.GSE.AU.clockSlate_EarthTarget.HD1080i.01200_print.jpg (1024x576) [115.4 KB] || MagnetosphereMultiMission.top.GSE.AU.clockSlate_EarthTarget.HD1080i.01200_searchweb.png (320x180) [82.7 KB] || MagnetosphereMultiMission.top.GSE.AU.clockSlate_EarthTarget.HD1080i.01200_thm.png (80x40) [6.3 KB] || TopView (1920x1080) [0 Item(s)] || MagnetosphereMultiMission.top.HD1080i_p30.mp4 (1920x1080) [29.7 MB] || MagnetosphereMultiMission.top.HD1080i_p30.webm (1920x1080) [6.1 MB] || TopView (3840x2160) [0 Item(s)] || MagnetosphereMultiMission.top.UHD3840_2160p30.mp4 (3840x2160) [93.0 MB] || MagnetosphereMultiMission.top.HD1080i_p30.mp4.hwshow [207 bytes] || ",
            "hits": 46
        },
        {
            "id": 4589,
            "url": "https://svs.gsfc.nasa.gov/4589/",
            "result_type": "Visualization",
            "release_date": "2017-10-25T10:00:00-04:00",
            "title": "Heliophysics Sentinels 2017",
            "description": "This visualization starts from near Earth and the Earth orbiting satellite fleet out to the Moon, then past the Sun-Earth Lagrange point 1 to out beyond the heliopause.  This is the long-play version. || Sentinels2017.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_print.jpg (1024x576) [136.1 KB] || Sentinels2017.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_searchweb.png (180x320) [84.6 KB] || Sentinels2017.Sentinels2Voyager.GSE.AU.clockSlate_EarthTarget.UHD3840.00000_thm.png (80x40) [6.0 KB] || Sentinels2017.Sentinels2Voyager.HD1080i_p30.webm (1920x1080) [12.4 MB] || SlowPlay (1920x1080) [0 Item(s)] || Sentinels2017.Sentinels2Voyager.HD1080i_p30.mp4 (1920x1080) [111.6 MB] || SlowPlay (3840x2160) [0 Item(s)] || Sentinels2017.Sentinels2Voyager_2160p30.mp4 (3840x2160) [336.2 MB] || Sentinels2017.Sentinels2Voyager.HD1080i_p30.mp4.hwshow [209 bytes] || ",
            "hits": 23
        },
        {
            "id": 30822,
            "url": "https://svs.gsfc.nasa.gov/30822/",
            "result_type": "Infographic",
            "release_date": "2016-12-06T00:00:00-05:00",
            "title": "NASA's Heliophysics Fleet",
            "description": "The current Heliophysics fleet || hpd-fleet-chart-jan-2024_print.jpg (1024x576) [180.0 KB] || hpd-fleet-chart-jan-2024.png (3840x2160) [7.3 MB] || hpd-fleet-chart-jan-2024_searchweb.png (320x180) [91.3 KB] || hpd-fleet-chart-jan-2024_thm.png (80x40) [7.2 KB] || nasas-fleets-by-division-helio-jewel.hwshow [228 bytes] ||",
            "hits": 56
        },
        {
            "id": 2862,
            "url": "https://svs.gsfc.nasa.gov/2862/",
            "result_type": "Visualization",
            "release_date": "2003-12-03T12:00:00-05:00",
            "title": "ViSBARD: Insights into the Sun-Earth Connection",
            "description": "ViSBARD (Visual System for Browsing, Analysis, and Retrieval of Data) is a data analysis application that brings together measurements from collections of spacecraft near the Earth or throughout the heliosphere  In this visualization created from ViSBARD screenshots, we see the magnetic field as measured from six different satellites.  The position of each spacecraft is marked by a small color glyph (ACE = yellow, Cluster = dark blue, Geotail = green, GOES 10 = red, Polar = light blue, Wind = purple).  The direction of the arrow signifies the direction of the magnetic field while the color represents the intensity (red being the highest, blue the lowest).  The magnetic pole of the Earth is in yellow, and it rotates properly as the animation proceeds.  This view of the magnetic storm shows highly disturbed fields at geosynchronous orbit (GOES), many crossings of the 'magnetotail current sheet' where the field changes sign and points at the opposite pole of the Earth, close encounters with the Earth (large red fields that are truncated to keep the arrows from becoming huge), and the entry from the back of the picture of Wind and Geotail through the bow shock (wire-frame) and magnetopause (sometimes visible as a transparent surface). || ",
            "hits": 18
        },
        {
            "id": 2863,
            "url": "https://svs.gsfc.nasa.gov/2863/",
            "result_type": "Visualization",
            "release_date": "2003-12-03T12:00:00-05:00",
            "title": "ViSBARD: The Wind from the Sun",
            "description": "The ViSBARD (Visual System for Browsing, Analysis, and Retrieval of Data) analysis package has an option to propagate measurements carried by the solar wind.  In this visualization created from ViSBARD screenshots, three spacecraft ahead of the Earth's bow shock measure the magnetic field as it is carried by the solar wind towards the Earth.  Their positions as projected according to the flow speed are noted with the small glyph (Wind = yellow, Geotail = blue, IMP-8 = green).  The spacecraft actually move very little over the time interval shown, but a spatial picture emerges when we use a knowledge of the wind velocity to spread the vectors out according to how they flowed past the point of observation.  Arrows on the satellite glyphs indicate the magnitude and direction of the magnetic field while the color also represents the intensity (red being the highest, blue the lowest).  As the wind flows, we can rapidly obtain information on the extended geometry of convected structures.  The wire-frame at the left is a representation of the Earth's bow shock (about 100 Earth radii across in what is shown) that shows where the Sun's magnetic field would begin to be affected by that the Earth.  (The effect of the interaction is not shown.) || ",
            "hits": 15
        },
        {
            "id": 2435,
            "url": "https://svs.gsfc.nasa.gov/2435/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/LENA Observes Oxygen Atoms in the near-Earth Environment",
            "description": "Electrically charged oxygen atoms (green) are ejected into the magnetosphere due to heating in the ionosphere.  The red 'thermometer' displays the intensity of the solar wind (dynamic pressure) measured by the Geotail spacecraft.  The yellow 'thermometer' represents the source intensity or hydrogen counts as measured by IMAGE/LENA. || ",
            "hits": 20
        }
    ]
}