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    "results": [
        {
            "id": 14095,
            "url": "https://svs.gsfc.nasa.gov/14095/",
            "result_type": "Produced Video",
            "release_date": "2022-02-09T09:00:00-05:00",
            "title": "NASA’s New Views of Venus’ Surface From Space",
            "description": "NASA’s Parker Solar Probe has taken its first visible light images of the surface of Venus from space. Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entire nightside in wavelengths of the visible spectrum – the type of light that the human eye can see – and extending into the near-infrared.The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet.Link to NASA.gov feature.Link to associated research paper. || ",
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        {
            "id": 14055,
            "url": "https://svs.gsfc.nasa.gov/14055/",
            "result_type": "Produced Video",
            "release_date": "2021-12-20T22:00:00-05:00",
            "title": "Parker Solar Probe's WISPR Images Inside The Sun's Atmosphere",
            "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. As Parker Solar Probe flew through the corona, its WISPR instrument captured images.The Wide-Field Imager for Parker Solar Probe (WISPR) is the only imaging instrument aboard the spacecraft. WISPR looks at the large-scale structure of the corona and solar wind before the spacecraft flies through it. About the size of a shoebox, WISPR takes images from afar of structures like coronal mass ejections, or CMEs, jets and other ejecta from the Sun. These structures travel out from the Sun and eventually overtake the spacecraft, where the spacecraft’s other instruments take in-situ measurements. WISPR helps link what’s happening in the large-scale coronal structure to the detailed physical measurements being captured directly in the near-Sun environment.To image the solar atmosphere, WISPR uses the heat shield to block most of the Sun’s light, which would otherwise obscure the much fainter corona. Specially designed baffles and occulters reflect and absorb the residual stray light that has been reflected or diffracted off the edge of the heat shield or other parts of the spacecraft.WISPR uses two cameras with radiation-hardened Active Pixel Sensor CMOS detectors. These detectors are used in place of traditional CCDs because they are lighter and use less power. They are also less susceptible to effects of radiation damage from cosmic rays and other high-energy particles, which are a big concern close to the Sun. The camera’s lenses are made of a radiation hard BK7, a common type of glass used for space telescopes, which is also sufficiently hardened against the impacts of dust.WISPR was designed and developed by the Solar and Heliophysics Physics Branch at the Naval Research Laboratory in Washington, D.C. (principal investigator Russell Howard), which will also develop the observing program. || ",
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        },
        {
            "id": 13282,
            "url": "https://svs.gsfc.nasa.gov/13282/",
            "result_type": "Produced Video",
            "release_date": "2019-12-04T13:00:00-05:00",
            "title": "5 New Discoveries from NASA's Parker Solar Probe",
            "description": "Music Credit: Smooth as Glass by The Freeharmonic OrchestraWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || parkerscience.thumb.jpg (1920x1080) [731.2 KB] || parkerscience.thumb_thm.png (80x40) [6.8 KB] || parkerscience.thumb_searchweb.png (320x180) [87.7 KB] || 13282_ParkerFirstScience_Twitter1080.mp4 (1920x1080) [53.4 MB] || 13282_ParkerFirstScience.YouTube1080.webm (1920x1080) [26.9 MB] || 13282_ParkerFirstScience.mp4 (1920x1080) [246.1 MB] || 13282_ParkerFirstScience_Mobile1080.mp4 (1920x1080) [194.5 MB] || 13282_ParkerFirstScience.YouTube1080.mp4 (1920x1080) [387.1 MB] || 13282_ParkerFirstScience_Twitter1080.en_US.srt [4.5 KB] || 13282_ParkerFirstScience_Twitter1080.en_US.vtt [4.5 KB] || 13282_ParkerFirstScienceMASTER.APR1080.mov (1920x1080) [3.2 GB] || ",
            "hits": 105
        },
        {
            "id": 13072,
            "url": "https://svs.gsfc.nasa.gov/13072/",
            "result_type": "Produced Video",
            "release_date": "2018-09-19T12:00:00-04:00",
            "title": "Parker Solar Probe First Light Data",
            "description": "Just over a month into its mission, Parker Solar Probe has returned first-light data from each of its four instrument suites. These early observations – while not yet examples of the key science observations Parker Solar Probe will take closer to the Sun – show that each of the instruments is working well. The instruments work in tandem to measure the Sun's electric and magnetic fields, particles from the Sun and the solar wind, and capture images of the environment around the spacecraft. The mission’s first close approach to the Sun will be in November 2018, but even now, the instruments are able to gather measurements of what’s happening in the solar wind closer to Earth. || ",
            "hits": 148
        },
        {
            "id": 13035,
            "url": "https://svs.gsfc.nasa.gov/13035/",
            "result_type": "Produced Video",
            "release_date": "2018-08-08T16:00:00-04:00",
            "title": "Parker Solar Probe Instruments",
            "description": "SWEAPThe Solar Wind Electrons Alphas and Protons investigation, or SWEAP, gathers observations using two complementary instruments: the Solar Probe Cup, or SPC, and the Solar Probe Analyzers, or SPAN. The instruments count the most abundant particles in the solar wind — electrons, protons and helium ions — and measure such properties as velocity, density, and temperature to improve our understanding of the solar wind and coronal plasma. SWEAP was built mainly at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and at the Space Sciences Laboratory at the University of California, Berkeley. The institutions jointly operate the instrument. The principal investigator is Justin Kasper from the University of Michigan. || SWEAP.00001_print.jpg (1024x581) [151.9 KB] || SWEAP_thumb.png (2560x1448) [4.7 MB] || SWEAP.00001_searchweb.png (320x180) [86.1 KB] || SWEAP.00001_web.png (320x181) [86.8 KB] || SWEAP.00001_thm.png (80x40) [5.6 KB] || SWEAP.webm (1902x1080) [21.8 MB] || SWEAP.mp4 (1902x1080) [195.4 MB] || SWEAP.en_US.srt [3.8 KB] || SWEAP.en_US.vtt [3.8 KB] || ",
            "hits": 415
        },
        {
            "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": 158
        },
        {
            "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. || ",
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        }
    ]
}