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            "id": 4957,
            "url": "https://svs.gsfc.nasa.gov/4957/",
            "result_type": "Visualization",
            "release_date": "2021-12-14T12:00:00-05:00",
            "title": "Parker Solar Probe: The Origins of Switchbacks",
            "description": "Most of the magnetic field measured at Parker during this time is directed sunward (blue field lines and vectors).  A switchback occurs when the field changes direction almost 180 degrees for a short period of time.  FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows.  The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line.  The heliospheric magnetic field lines are represented as gold. || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_print.jpg (1024x576) [114.9 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_searchweb.png (320x180) [71.7 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_thm.png (80x40) [4.5 KB] || Switchbacks20181106A (1920x1080) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4 (1920x1080) [25.7 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.webm (1920x1080) [4.4 MB] || Switchbacks20181106A (3840x2160) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.UHD3840_2160p30.mp4 (3840x2160) [100.2 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4.hwshow [229 bytes] || ",
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            "id": 4958,
            "url": "https://svs.gsfc.nasa.gov/4958/",
            "result_type": "Visualization",
            "release_date": "2021-12-14T12:00:00-05:00",
            "title": "Parker Solar Probe: Crossing the Alfven Surface",
            "description": "Split window view illustrating the orbit of Parker with the orbit trail colored based on the Mach number of the solar wind and the magnetic field lines (represented as gold) connecting back to the Sun.  The Mach number drops below unity (one) when a field line transitions between two different coronal hole regions (the blue and red regions marked on the Sun). || Parker_SolarCloseup.combo.HD1080.00480_print.jpg (1024x576) [121.9 KB] || Parker_SolarCloseup.combo.HD1080.00480_searchweb.png (320x180) [74.1 KB] || Parker_SolarCloseup.combo.HD1080.00480_thm.png (80x40) [5.2 KB] || Parker_SolarCloseup.combo.HD1080 (1920x1080) [0 Item(s)] || Parker_SolarCloseup.combo.HD1080_p30.mp4 (1920x1080) [45.8 MB] || Parker_SolarCloseup.combo.HD1080_p30.webm (1920x1080) [5.6 MB] || Parker_SolarCloseup.combo.UHD2160 (3840x2160) [0 Item(s)] || Parker_SolarCloseup.combo.UHD2160_p30.mp4 (3840x2160) [124.5 MB] || Parker_SolarCloseup.combo.HD1080_p30.mp4.hwshow [202 bytes] || ",
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        }
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}