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        {
            "id": 4805,
            "url": "https://svs.gsfc.nasa.gov/4805/",
            "result_type": "Visualization",
            "release_date": "2020-12-07T10:00:00-05:00",
            "title": "Coordinated Heliosphere - How Solar Missions Work Together",
            "description": "Using Solar Orbiter, Parker Solar Probe, and other sun-observing missions, in coordinated observations, we can learn far more about the solar atmosphere which surrounds and impacts Earth and other missions in space, crewed and uncrewed. || ",
            "hits": 47
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        {
            "id": 4788,
            "url": "https://svs.gsfc.nasa.gov/4788/",
            "result_type": "Visualization",
            "release_date": "2020-02-04T12:00:00-05:00",
            "title": "The Solar Polar Magnetic Field",
            "description": "From our single vantage point of Earth, our view of the Sun is never complete.  While the far-side of the Sun eventually rotates into view, coverage of the Sun's polar regions is never satisfactory as perspective effects either completely block our view or create a distorted view.   We must often resort to computer modeling of these solar polar regions.This visualization presents the Potential Field Source Surface (PFSS) magnetic field model based on solar observations covering the years 2017-2019.  One version also presents the 'hole' in our measurements of the solar polar region.  The region oscillates in size over the course of the year due to the changing perspective created by the tilt of Earth's orbital plane with the solar equator.   In this region, researchers must resort to approximations to build a more complete view of the solar magnetic field.Why is the solar magnetic field in this region important?  Because the combined with the outgoing flow of the solar wind, the magnetic field lines from the polar regions curve up, and then back down to near the Sun's equatorial plane, which is still fairly close to the orbital plane of Earth and other planets in our solar system.  This gives the Sun's polar magnetic field a significant influence on the space weather impacting Earth and crewed and uncrewed assets around the solar system. || ",
            "hits": 63
        },
        {
            "id": 20306,
            "url": "https://svs.gsfc.nasa.gov/20306/",
            "result_type": "Animation",
            "release_date": "2020-01-27T14:00:00-05:00",
            "title": "Solar Orbiter - NASA Animations",
            "description": "Solar Orbiter is an international cooperative mission between the European Space Agency and NASA that addresses a central question of heliophysics: How does the Sun create and control the constantly changing space environment throughout the solar system? The Sun creates what’s known as the heliosphere — a giant bubble of charged particles and magnetic fields blown outward by the Sun that stretches more than twice the distance to Pluto at its nearest edge, enveloping every planet in our solar system and shaping the space around us. To understand it, Solar Orbiter will travel as close as 26 million miles from the Sun, inside the orbit of Mercury. There, it will measure the magnetic fields, waves, energetic particles and plasma escaping the Sun while they are in their pristine state, before being modified and mixed in their long journey from the Sun. || ",
            "hits": 76
        },
        {
            "id": 13528,
            "url": "https://svs.gsfc.nasa.gov/13528/",
            "result_type": "Produced Video",
            "release_date": "2020-01-27T13:50:00-05:00",
            "title": "Solar Orbiter Media Telecon",
            "description": "NASA and ESA scientists will present Solar Orbiter, the ESA/NASA collaboration soon to start its journey to the Sun, during a media teleconference on Monday, Jan. 27, 2020 at 2 p.m. EST.  Mission experts will discuss Solar Obiter’s uniquely tilted orbit, how the mission will capture the first images of the Sun’s North and South poles, and its ability to tackle major solar mysteries with its comprehensive suite of ten different instruments. The teleconference audio will stream live at:https://www.nasa.gov/liveParticipants include:•Nicola Fox, director of the Heliophysics Division in the Science Mission Directorate at NASA Headquarters in Washington•Chris St. Cyr, former NASA project scientist for the mission at NASA Goddard•Yannis Zouganelis, ESA deputy project scientist for Solar Orbiter at the European Space Astronomy Centre in Madrid, Spain•Anne Pacros, ESA Mission and Payload Manager || ",
            "hits": 27
        },
        {
            "id": 13527,
            "url": "https://svs.gsfc.nasa.gov/13527/",
            "result_type": "Produced Video",
            "release_date": "2020-01-27T12:00:00-05:00",
            "title": "New Mission Will Take First Peek at Sun’s Poles",
            "description": "A new spacecraft is journeying to the Sun to snap the first pictures of the Sun’s north and south poles. Solar Orbiter, a collaboration between ESA (the European Space Agency) and NASA will have its first opportunity to launch from Cape Canaveral on Feb. 7, 2020, at 11:15 p.m. EST. Launching on a United Launch Alliance Atlas V rocket, the spacecraft will use Venus’ and Earth’s gravity to swing itself out of the ecliptic plane — the swath of space, roughly aligned with the Sun’s equator, where all planets orbit. From there, Solar Orbiter's bird’s eye view will give it the first-ever look at the Sun's poles.Read more: https://www.nasa.gov/feature/goddard/2020/new-mission-will-take-first-peek-at-sun-s-poles || ",
            "hits": 51
        },
        {
            "id": 4653,
            "url": "https://svs.gsfc.nasa.gov/4653/",
            "result_type": "Visualization",
            "release_date": "2018-06-05T10:00:00-04:00",
            "title": "Parker Solar Probe and Solar Orbiter Trajectories",
            "description": "This visualization opens near Earth for the launch of Parker Solar Probe August 12,  2018.  Then the camera moves around the Sun to match of with Earth again for the launch of Solar Orbiter in 2020.  After that, the camera moves in a slow drift around the Sun as the orbits evolve.  The Parker Solar Probe orbit fades out after the nominal end of mission in 2025.  This version has longer orbit trails to better view orbit changes, and the red along the orbits indicate the nominal science operations portions of the missions. || ParkerAndSolarOrbiter.InnerTourDeluxe.HAE.AU.clockSlate_EarthTarget.HD1080i.02000_print.jpg (1024x576) [100.7 KB] || DeluxeTour (1920x1080) [0 Item(s)] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.webm (1920x1080) [17.6 MB] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.mp4 (1920x1080) [179.8 MB] || DeluxeTour (3840x2160) [0 Item(s)] || ParkerAndSolarOrbiter.InnerTourDeluxe_2160p30.mp4 (3840x2160) [489.0 MB] || ParkerAndSolarOrbiter.InnerTourDeluxe.HD1080i_p30.mp4.hwshow [270 bytes] || ParkerAndSolarOrbiter.InnerTourDeluxe_2160p30.mp4.hwshow [211 bytes] || ",
            "hits": 276
        }
    ]
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