{
    "id": 5443,
    "url": "https://svs.gsfc.nasa.gov/5443/",
    "page_type": "Visualization",
    "title": "Heliophysics Sentinels 2024",
    "description": "There have been some changes since the 2022 Heliophysics Fleet.  AIM and ICON have been decommissioned while two other instruments have been added.  AWE is an instrument mounted on the ISS, and RAD is a particle detector on the Curiosity Mars rover.  As of Winter 2024, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause. || ",
    "release_date": "2024-12-17T00:00:00-05:00",
    "update_date": "2025-02-02T23:15:27.884357-05:00",
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        "filename": "Sentinels2024.NearEarth.GSE.AU.clockSlate_CRTT.HD1080.02400_print.jpg",
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    "main_video": null,
    "main_credits": {
        "Visualizations by": [
            {
                "name": "Tom Bridgman",
                "employer": "Global Science and Technology, Inc."
            }
        ]
    },
    "progress": "Complete",
    "media_groups": [
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            "description": "There have been some changes since the <a href=\"/4898\">2022 Heliophysics Fleet</a>.  <a href=\"https://science.nasa.gov/science-research/heliophysics/night-shining-cloud-mission-ends-yields-high-science-results-for-nasa/\" target=\"_blank\">AIM</a> and <a href=\"https://science.nasa.gov/science-research/heliophysics/nasas-icon-mission-ends-with-several-ionospheric-breakthroughs/\" target=\"_blank\">ICON</a> have been decommissioned while two other instruments have been added.  <a href=\"https://science.nasa.gov/mission/awe/\" target=\"_blank\">AWE</a> is an instrument mounted on the ISS, and <a href=\"https://www.nasa.gov/image-article/curiosity-radiation-assessment-device-rad/\" target=\"_blank\">RAD</a> is a particle detector on the Curiosity Mars rover.  <p>As of Winter 2024, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.<p>",
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            "description": "<p>Excepting the Voyager missions, the satellite orbits are color coded for their observing program:<p><ul><li><DROP_SHADOW><font style=\"color:#ff00ff\">Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observations</font></DROP_SHADOW></li><p><li><DROP_SHADOW><font color=\"#ffc400\">Yellow-Orange: solar observations and imagery</font></DROP_SHADOW></li><p><li><DROP_SHADOW><font color=\"#00ffff\">Cyan: Geospace and magnetosphere</font></DROP_SHADOW></li><p><li><DROP_SHADOW><font color=\"#8888ff\">Violet: Heliospheric observations</font></DROP_SHADOW></li><p></ul></p><hr><h3>Near-Earth Fleet:</h3>",
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                    "id": 445255,
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                    "instance": {
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        {
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            "description": "<ul><li><a href='http://solarb.msfc.nasa.gov/' target='_blank'>Hinode</a>: Observes the Sun in multiple wavelengths up to x-rays. <a href='search/?missions=Hinode+%28Solar-b%29' target='_blank'>SVS page</a></li><li><a href='http://www.timed.jhuapl.edu/WWW/index.php' target='_blank'>TIMED</a>: Studies the upper layers (40-110 miles up) of  Earth's atmosphere. <a href='/search/?missions=TIMED' target='_blank'>SVS page</a></li><li><a href=\"https://science.nasa.gov/mission/awe/\" target=\"_blank\">AWE (on the ISS)</a> studies atmospheric gravity waves</li><li><a href=\"http://www.nasa.gov/mission_pages/iris/index.html\" target='_blank'>IRIS</a>: Interface Region Imaging Spectrograph is designed to take high-resolution spectra and images of the region between the solar photosphere and solar atmosphere. <a href=\"/gallery/irisnasas-new-eyeonthe-sun/\" target='_blank'>SVS page</a></li></ul><h3>Geosynchronous Fleet:</h3><ul><li><a href=\"http://sdo.gsfc.nasa.gov/\" target='_blank'>SDO</a>: Solar Dynamics Observatory keeps the Sun under continuous observation at 16 megapixel resolution. <a href=\"gallery/sdo/\" target='_blank'>SVS page</a></li><li><a href=\"https://www.nasa.gov/content/goddard/gold\" target='_blank'>GOLD</a>:  Global-scale Observations of the Limb and Disk is a spectroscopic imager for studying the ionosphere. <a href=\"/search/?missions=Global-scale+Observations+of+the+Limb+and+Disk+%28GOLD%29\" target=\"_blank\">SVS page</a></li></ul><h3>Geospace Fleet:</h3><ul><li><a href='http://pwg.gsfc.nasa.gov/geotail.shtml' target='_blank'>Geotail</a>: Conducts measurements of electrons and ions in the Earth's magnetotail. <a href=\"/search/?search=geotail\" target='_blank'>SVS page</a></li><li><a href='http://sci.esa.int/science-e/www/area/index.cfm?fareaid=8' target='_blank'>Magnetospheric Multi-scale (MMS)</a>: 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. <a href='/search/?missions=Magnetospheric+Multiscale+%28MMS%29' target='_blank'>SVS page</a></li><li><a href='http://themis.ssl.berkeley.edu/index.shtml' target='_blank'>THEMIS</a>: This is a fleet of three satellites to study how magnetospheric instabilities produce <a href='http://www.phy6.org/Education/wsubstrm.html' target='_blank'>substorms</a>. Two of the original five satellites were <a href=\"/3682\">moved into lunar orbit to become THEMIS-ARTEMIS.</a>   (<a href='/search/?missions=THEMIS' target='_blank'>SVS page</a>) </li><li><a href=\"http://ibex.swri.edu/\" target='_blank'>IBEX:</a> The Interstellar Boundary Explorer measures the flux of neutral atoms from the heliopause. <a href='/search/?missions=IBEX' target='_blank'>SVS page</a></li></ul><h3>Lunar Orbiting Fleet:</h3>",
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            "description": "The L1 point is a <a href='http://en.wikipedia.org/wiki/Lagrange_points' target='_blank'>Lagrange Point</a> between the Sun and the Earth. Spacecraft can orbit this location for continuous coverage of the Sun.<ul><li><a href='http://sohowww.nascom.nasa.gov/' target='_blank'>SOHO</a>: Studies the Sun with cameras and a multitude of other instruments. <a href='/search/?missions=SOHO' target='_blank'>SVS page</a></li><li><a href='http://www.srl.caltech.edu/ACE/' target='_blank'>ACE</a>: Measures the composition and characteristics of the solar wind. <a href='/search/?keywords=ACE' target='_blank'>SVS page</a></li><li><a href='http://wind.nasa.gov/' target='_blank'>Wind</a>: Measures particle flows and fields in the solar wind. <a href='/search/?missions=Wind' target='_blank'>SVS page</a></li></ul><hr><h3>Solar Orbiting Fleet:</h3>",
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            "description": "This visualization presents orbits of the current heliophysics satellites covering the space near Earth, through to the inner solar system.  In this view, we also see the last Venus flyby of Parker Solar Probe (November 6, 2024) to its ultimate record perihelion (December 24, 2024).",
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        {
            "id": 14744,
            "url": "https://svs.gsfc.nasa.gov/14744/",
            "page_type": "Produced Video",
            "title": "GDC and DYNAMIC to Explore Earth’s Upper Atmosphere",
            "description": "Two upcoming missions, the Geospace Dynamics Constellation (GDC) and Dynamical Neutral Atmosphere-Ionosphere Coupling (DYNAMIC) will revolutionize our understanding of Earth’s upper atmosphere. This region includes Earth’s ionosphere, thermosphere, and mesosphere, and stretches from roughly 50 to 400 miles above Earth’s surface. Space weather disturbances can impact communications, navigation signals, and satellite orbits, and induce currents can trigger power outages on Earth — making the region a crucial area of study.GDC is a team of satellites that will study Earth’s upper atmosphere and provide the first direct global measurements of our planet’s dynamic and complex interface with the space environment. Working in tandem with the DYNAMIC spacecraft, scientists will be able paint a fuller picture of how energy transforms and travels throughout the upper atmosphere. GDC will fly at an altitude of 350-400 km.DYNAMIC is a pair of satellites that will work in tandem with GDC to study how changes in Earth’s lower atmosphere influence our planet’s upper atmosphere. Between the multiple spacecraft of GDC and DYNAMIC, simultaneous observations from different locations can give scientists a more complete picture of how atmospheric waves propagate up through this unique part of the atmosphere. DYNAMIC will fly at an altitude of 550-800 km. || ",
            "release_date": "2025-01-03T00:00:00-05:00",
            "update_date": "2025-01-02T16:44:26.122491-05:00",
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            "id": 14741,
            "url": "https://svs.gsfc.nasa.gov/14741/",
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            "title": "Parker Solar Probe: Humanity’s Closest Encounter with the Sun",
            "description": "Controllers have confirmed NASA’s mission to “touch” the Sun survived its record-breaking closest approach to the solar surface on Dec. 24, 2024.Breaking its previous record by flying just 3.8 million miles above the surface of the Sun, NASA’s Parker Solar Probe hurtled through the solar atmosphere at a blazing 430,000 miles per hour — faster than any human-made object has ever moved. A beacon tone received in the late evening hours of Dec. 26 confirmed the spacecraft had made it through the encounter safely and is operating normally.This pass, the first of more to come at this distance, allows the spacecraft to conduct unrivaled scientific measurements with the potential to change our understanding of the Sun. || ",
            "release_date": "2024-12-27T13:00:00-05:00",
            "update_date": "2024-12-27T13:59:21.228827-05:00",
            "main_image": {
                "id": 1140135,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014700/a014741/PSP_AcrossAcutalSun_H264.00001_print.jpg",
                "filename": "PSP_AcrossAcutalSun_H264.00001_print.jpg",
                "media_type": "Image",
                "alt_text": "Conceptual AnimationA conceptual animation of Parker Solar Probe making its closest approach to the Sun.Credit: NASA/Johns Hopkins APL/Steve Gribben",
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            "url": "https://svs.gsfc.nasa.gov/4822/",
            "page_type": "Visualization",
            "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 || ",
            "release_date": "2020-09-15T10:00:00-04:00",
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                "filename": "Sentinels2020.InnerSolarSystem.GSE.AU.clockSlate_EarthTarget.HD1080i.01500_print.jpg",
                "media_type": "Image",
                "alt_text": "This visualization presents orbits of the current heliophysics satellites covering the space near Earth, out to the Sun-Earth Lagrange point, L1, and finally a view of the current missions operating in the inner solar system.",
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