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    "results": [
        {
            "id": 12999,
            "url": "https://svs.gsfc.nasa.gov/12999/",
            "result_type": "Produced Video",
            "release_date": "2018-07-12T15:00:00-04:00",
            "title": "Parker Solar Probe Path Across Sun's Surface",
            "description": "The velocity of Parker Solar Probe is fastest right at perihelion. The spacecraft is so fast that near perihelion, it flies faster than the Sun rotates. This animation illustrates this by following the track of the spacecraft on map of the surface of the Sun. When the spacecraft flies faster than the Sun rotates, the orbit track on the surface goes backward (retrograde). At the turning points (labeled co-rotation periods), the spacecraft and the Sun are essential moving together (co-rotation). These periods of time, which last many hours, will be invaluable for making continuous measurements of solar wind from the same source.Credit: NASA/JPL/WISPR Team || 12999_PSPRelativeMotionToSun2018V81080p.00001_print.jpg (1024x576) [100.7 KB] || 12999_PSPRelativeMotionToSun2018V81080p.00001_searchweb.png (320x180) [54.3 KB] || 12999_PSPRelativeMotionToSun2018V81080p.00001_web.png (320x180) [54.3 KB] || 12999_PSPRelativeMotionToSun2018V81080p.00001_thm.png (80x40) [3.5 KB] || 12999_PSPRelativeMotionToSun2018V81080p.mp4 (1920x1080) [76.2 MB] || PRORES_B-ROLL_12999_PSPRelativeMotionToSun2018V81080p_prores.mov (1280x720) [335.3 MB] || YOUTUBE_1080_12999_PSPRelativeMotionToSun2018V81080p_youtube_1080.mp4 (1920x1080) [71.6 MB] || NASA_TV_12999_PSPRelativeMotionToSun2018V81080p.mpeg (1280x720) [156.1 MB] || 12999_PSPRelativeMotionToSun2018V81080p.webm (1920x1080) [3.7 MB] || 12999_PSPRelativeMotionToSun2018V81080p_appletv.m4v (1280x720) [22.9 MB] || NASA_PODCAST_12999_PSPRelativeMotionToSun2018V81080p_ipod_sm.mp4 (320x240) [6.6 MB] || ",
            "hits": 72
        },
        {
            "id": 12998,
            "url": "https://svs.gsfc.nasa.gov/12998/",
            "result_type": "Produced Video",
            "release_date": "2018-07-12T14:00:00-04:00",
            "title": "Parker Solar Probe Orbit From August 2018 - March 2019",
            "description": "This animation shows the first few orbits of Parker Solar Probe from August 2018 to March 2019 which includes two encounters with Venus. Note that the last orbit in this animation goes closer to the Sun than the early ones. This is because Parker Solar Probe uses “gravity assists” from Venus to modify its orbit to bring it closer to the Sun. The perihelion of the first orbit is about 35 solar radii whereas the perihelia of the final three orbits (December 2024 to June 2025) are less than 10 solar radii.  Credit: NASA/JPL/WISPR Team || 12998_PSPOrbitsUpToVenusEncountersv620181080p.00001_print.jpg (1024x576) [71.8 KB] || 12998_PSPOrbitsUpToVenusEncountersv620181080p.00001_searchweb.png (320x180) [36.9 KB] || 12998_PSPOrbitsUpToVenusEncountersv620181080p.00001_web.png (320x180) [36.9 KB] || 12998_PSPOrbitsUpToVenusEncountersv620181080p.00001_thm.png (80x40) [3.4 KB] || 12998_PSPOrbitsUpToVenusEncountersv620181080p.mp4 (1920x1080) [74.7 MB] || PRORES_B-ROLL_12998_PSPOrbitsUpToVenusEncountersv620181080p_prores.mov (1280x720) [355.1 MB] || YOUTUBE_1080_12998_PSPOrbitsUpToVenusEncountersv620181080p_youtube_1080.mp4 (1920x1080) [82.9 MB] || NASA_TV_12998_PSPOrbitsUpToVenusEncountersv620181080p.mpeg (1280x720) [161.2 MB] || 12998_PSPOrbitsUpToVenusEncountersv620181080p_appletv.m4v (1280x720) [27.6 MB] || 12998_PSPOrbitsUpToVenusEncountersv620181080p.webm (1920x1080) [4.7 MB] || NASA_PODCAST_12998_PSPOrbitsUpToVenusEncountersv620181080p_ipod_sm.mp4 (320x240) [8.5 MB] || ",
            "hits": 183
        },
        {
            "id": 12927,
            "url": "https://svs.gsfc.nasa.gov/12927/",
            "result_type": "Produced Video",
            "release_date": "2018-04-16T12:00:00-04:00",
            "title": "Looking at the Corona with WISPR on Parker Solar Probe",
            "description": "The Wide-Field Imager for Solar Probe, or WISPR, is aboard NASA’s Parker Solar Probe to take images of the solar corona (the Sun’s atmosphere)  and inner heliosphere. WISPR’s telescopes will provide white-light images of the solar wind, shocks, solar ejecta and other structures as they approach and pass the spacecraft. Parker Solar Probe is scheduled for launch in July 2018. It will be the first spacecraft ever to fly through the solar corona to investigate the evolution of the solar wind and heating of the solar corona. WISPR does not look directly at the Sun. Its very wide field-of-view extends from 13° away from the center of the Sun to 108° from the Sun. || ",
            "hits": 72
        },
        {
            "id": 3794,
            "url": "https://svs.gsfc.nasa.gov/3794/",
            "result_type": "Visualization",
            "release_date": "2010-11-09T00:00:00-05:00",
            "title": "STEREO in Stereo: April 8, 2007",
            "description": "Full Disk View: Image sequences taken April 8-9, 2007 by the EUVI telescopes on the two STEREO spacecraft (STEREO-B, left eye; STEREO-A, right eye). At this time the spacecraft were about 3.7 degrees apart. These images show the Sun in extreme ultraviolet light at a wavelength of 171 angstroms, highlighting parts of the Sun's atmosphere (the corona) at about one million degrees C. Note the bright active regions near the Sun's equator and the dark \"coronal holes\" at the north and south poles. These are features of the Sun's magnetic field. Coronal holes are areas where the magnetic field opens out to allow material to flow out into the solar system, while active regions are made up of strong, closed fields which bottle up hot plasma (ionized gas) close to the surface. This image was taken near the minimum in solar activity, so there are few active regions.Closeup View: Image sequences taken April 8-9, 2007 by the EUVI telescopes in the SECCHI imaging suites on the two STEREO spacecraft (STEREO-B, left eye; STEREO-A, right eye). At this time the spacecraft were about 3.7 degrees apart. Here we see a close up of solar magnetic active regions, flickering as they rotate out of sight around the sun. These are areas where the Sun's strong magnetic field bottles up million degree C plasma (ionized gas) low in the corona (the Sun's outer atmosphere). These images are taken at a wavelength of 171 angstroms (0.00000171 cm) in the extreme ultraviolet.Note for Large Displays: These movies are produced using images from STEREO where the angle between the spacecraft is getting larger than the optimum angle for stereo separation. While they work well on small displays, large-screens and projection systems can introduce significant distortions in the stereo effect which the audience may find uncomfortable. When doing large-screen projection, you may need to adjust the left-right image alignment for optimum viewing. However, this does not guarantee a distortion-free result. || ",
            "hits": 48
        },
        {
            "id": 3423,
            "url": "https://svs.gsfc.nasa.gov/3423/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 171 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 171 || ",
            "hits": 30
        },
        {
            "id": 3424,
            "url": "https://svs.gsfc.nasa.gov/3424/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: 284 Angstroms (Active Region)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 284 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+14=Fe XV), which forms at temperatures above 2x106K, and flows along the magnetic field lines of the solar active regions. New regions come into view as the Sun rotates. || ",
            "hits": 24
        },
        {
            "id": 3425,
            "url": "https://svs.gsfc.nasa.gov/3425/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 284 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 284 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+14=Fe XV), which forms at temperatures above 2x106K, and flows along the magnetic field lines of the solar active regions. New active regions come into view as the Sun rotates. || ",
            "hits": 25
        },
        {
            "id": 3426,
            "url": "https://svs.gsfc.nasa.gov/3426/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: 304 Angstroms (South Pole View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 304 || ",
            "hits": 15
        },
        {
            "id": 3427,
            "url": "https://svs.gsfc.nasa.gov/3427/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 171 Angstroms (South Pole View)",
            "description": "This movie shows the south pole of the Sun from the two STEREO spacecraft using the 171 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+8=Fe IX, Fe+9=Fe X) which forms at temperatures above 1.3x106K, and flows along the magnetic field lines of the solar active regions. New active regions come into view as the Sun rotates. || ",
            "hits": 13
        },
        {
            "id": 3428,
            "url": "https://svs.gsfc.nasa.gov/3428/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 195 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 195 || ",
            "hits": 42
        },
        {
            "id": 3421,
            "url": "https://svs.gsfc.nasa.gov/3421/",
            "result_type": "Visualization",
            "release_date": "2007-04-23T00:00:00-04:00",
            "title": "First 3-D stereo from STEREO: EUVI 171 Ångströms (Active Region)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 171 ? filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+8=Fe IX, Fe+9=Fe X) which forms at temperatures above 1.3x106K, and flows along the magnetic field lines of the solar active regions. New regions of solar activity come into view as the Sun rotates left to right. || ",
            "hits": 22
        },
        {
            "id": 3422,
            "url": "https://svs.gsfc.nasa.gov/3422/",
            "result_type": "Visualization",
            "release_date": "2007-04-23T00:00:00-04:00",
            "title": "First 3-D stereo from STEREO: EUVI 304",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 304 || ",
            "hits": 20
        }
    ]
}