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            "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ",
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            "page_type": "Produced Video",
            "title": "New Results from Mission to Touch the Sun Live Shots",
            "description": "Read about the latest results HEREClick here for quick link to AUDIO interview with Eric ChristianClick here for quick link to canned interview with Aleida Higginson. Click here for quick link to canned interview with Nicholeen Viall. Click here for quick link to canned interview with Eric ChristianClick here for quick link to B-ROLL associated with this live shot. Click here for Education Outreach  questions and answers with Eric ChristianClick here for quick link to Education Outreach questions and answers with Aleida Higginson. || Screen_Shot_2019-11-19_at_2.18.38_PM.png (2732x436) [736.7 KB] || Screen_Shot_2019-11-19_at_2.18.38_PM_print.jpg (1024x163) [27.1 KB] || Screen_Shot_2019-11-19_at_2.18.38_PM_searchweb.png (320x180) [1.4 KB] || Screen_Shot_2019-11-19_at_2.18.38_PM_thm.png (80x40) [973 bytes] || ",
            "release_date": "2019-12-04T13:00:00-05:00",
            "update_date": "2023-05-03T13:45:28.051683-04:00",
            "main_image": {
                "id": 390142,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013400/a013457/Screen_Shot_2019-11-19_at_2.18.38_PM_print.jpg",
                "filename": "Screen_Shot_2019-11-19_at_2.18.38_PM_print.jpg",
                "media_type": "Image",
                "alt_text": "Read about the latest results HEREClick here for quick link to AUDIO interview with Eric ChristianClick here for quick link to canned interview with Aleida Higginson. Click here for quick link to canned interview with Nicholeen Viall. Click here for quick link to canned interview with Eric ChristianClick here for quick link to B-ROLL associated with this live shot. Click here for Education Outreach  questions and answers with Eric ChristianClick here for quick link to Education Outreach questions and answers with Aleida Higginson.",
                "width": 1024,
                "height": 163,
                "pixels": 166912
            }
        },
        {
            "id": 13484,
            "url": "https://svs.gsfc.nasa.gov/13484/",
            "page_type": "Produced Video",
            "title": "Parker Solar Probe First Findings - Media Telecon",
            "description": "NASA to Present First Parker Solar Probe Findings in Media TeleconferenceNASA will announce the first results from the Parker Solar Probe mission, the agency's mission to \"touch\" the Sun, during a media teleconference at 1:30 pm EST on Wednesday, Dec. 4, 2019.Parker has traveled closer to our star than any human-made object before it. The teleconference will discuss the first papers from the principal investigators of the mission’s four instruments. The papers will be published online Wednesday in Nature at 1 pm EST.The teleconference audio will stream live at:https://www.nasa.gov/nasaliveParticipants in the call are: •Nicola Fox, director of the Heliophysics Division, Science Mission Directorate, NASA Headquarters, Washington•Stuart Bale, principal investigator of the FIELDS instrument at the University of California, Berkeley•Justin Kasper, principal investigator of the SWEAP instrument at the University of Michigan in Ann Arbor•Russ Howard, principal investigator of the WISPR instrument at the Naval Research Laboratory in Washington•David McComas, principal investigator of the ISʘIS instrument at Princeton University in Princeton, N.J. || ",
            "release_date": "2019-12-04T13:00:00-05:00",
            "update_date": "2025-02-02T00:22:29.115807-05:00",
            "main_image": {
                "id": 389475,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013400/a013484/wispr_merged_L3_rel_enc01.00200_print.jpg",
                "filename": "wispr_merged_L3_rel_enc01.00200_print.jpg",
                "media_type": "Image",
                "alt_text": "Image #5: The WISPR instrument on NASA's Parker Solar Probe captured imagery of the constant outflow of material from the Sun during its close approach to the Sun in November 2018.  Credit: NASA/NRL/APL",
                "width": 1024,
                "height": 635,
                "pixels": 650240
            }
        },
        {
            "id": 12903,
            "url": "https://svs.gsfc.nasa.gov/12903/",
            "page_type": "Produced Video",
            "title": "Discovering the Sun’s Mysteriously Hot Atmosphere",
            "description": "Something mysterious is going on at the Sun. In defiance of all logic, its atmosphere gets much, much hotter the farther it stretches from the Sun’s blazing surface.Temperatures in the corona — the tenuous, outermost layer of the solar atmosphere — spike upwards of 2 million degrees Fahrenheit, while just 1,000 miles below, the underlying surface simmers at a balmy 10,000 F. How the Sun manages this feat remains one of the greatest unanswered questions in astrophysics; scientists call it the coronal heating problem. A new, landmark mission, NASA’s Parker Solar Probe — scheduled to launch no earlier than Aug. 11, 2018 — will fly through the corona itself, seeking clues to its behavior and offering the chance for scientists to solve this mystery.From Earth, as we see it in visible light, the Sun’s appearance — quiet, unchanging — belies the life and drama of our nearest star. Its turbulent surface is rocked by eruptions and intense bursts of radiation, which hurl solar material at incredible speeds to every corner of the solar system. This solar activity can trigger space weather events that have the potential to disrupt radio communications, harm satellites and astronauts, and at their most severe, interfere with power grids.Above the surface, the corona extends for millions of miles and roils with plasma, gases superheated so much that they separate into an electric flow of ions and free electrons. Eventually, it continues outward as the solar wind, a supersonic stream of plasma permeating the entire solar system. And so, it is that humans live well within the extended atmosphere of our Sun. To fully understand the corona and all its secrets is to understand not only the star that powers life on Earth, but also, the very space around us.Read more on NASA.gov. || ",
            "release_date": "2018-07-25T14:00:00-04:00",
            "update_date": "2023-05-03T13:46:35.139868-04:00",
            "main_image": {
                "id": 405605,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012900/a012903/CHP_Discovery_1080_4.00001_print.jpg",
                "filename": "CHP_Discovery_1080_4.00001_print.jpg",
                "media_type": "Image",
                "alt_text": "Discovering the Sun’s Mysteriously Hot Atmosphere Something mysterious is going on at the Sun. In defiance of all logic, its atmosphere gets much, much hotter the farther it stretches from the Sun’s blazing surface.Temperatures in the corona — the Sun’s outer atmosphere — spike to 3 million degrees Fahrenheit, while just 1,000 miles below, the underlying surface simmers at a balmy 10,000 F. How the Sun manages this feat is a mystery that dates back nearly 150 years, and remains one of the greatest unanswered questions in astrophysics. Scientists call it the coronal heating problem.Watch the video to learn how astronomers first discovered evidence for this mystery during an eclipse in the 1800s, and what scientists today think could explain it.Music credits: 'Developing Over Time' by Ben Niblett [PRS], Jon Cotton [PRS], 'Eternal Circle' by Laurent Dury [SACEM], ‘Starlight Andromeda' by Ben Niblett [PRS], Jon Cotton [PRS]Coronal spectrum image credit: Constantine EmmanouilidiComplete transcript available.Watch this video on the NASA Goddard YouTube channel.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        },
        {
            "id": 12867,
            "url": "https://svs.gsfc.nasa.gov/12867/",
            "page_type": "Produced Video",
            "title": "Why Won't it Melt? How NASA's Solar Probe will Survive the Sun",
            "description": "Music credit: Cheeky Chappy [Main Track] by Jimmy Kaleth, Ross Andrew McLean from www.killertracks.com This music requires a license for use.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || meltthumb.jpg (1920x1080) [311.2 KB] || meltthumb_searchweb.png (320x180) [76.6 KB] || meltthumb_thm.png (80x40) [5.4 KB] || 12867WhyWontItMeltV8.mov (1920x1080) [5.4 GB] || 12867WhyWontItMeltV8.webm (1920x1080) [23.3 MB] || 12867WhyWontItMeltV8_appletv.m4v (1280x720) [148.8 MB] || 12867WhyWontItMeltV8_youtube_1080.mp4 (1920x1080) [443.5 MB] || 12867WhyWontItMeltV8_youtube_hq.mov (1920x1080) [1.3 GB] || 12867WhyWontItMeltV8_appletv_subtitles.m4v (1280x720) [148.9 MB] || 12867WhyWontItMeltV8.en_US.srt [4.2 KB] || 12867WhyWontItMeltV8.en_US.vtt [4.2 KB] || 12867WhyWontItMeltV8_ipod_sm.mp4 (320x240) [38.2 MB] || ",
            "release_date": "2018-07-19T15:00:00-04:00",
            "update_date": "2023-05-03T13:46:37.467124-04:00",
            "main_image": {
                "id": 406488,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012800/a012867/meltthumb.jpg",
                "filename": "meltthumb.jpg",
                "media_type": "Image",
                "alt_text": "Music credit: Cheeky Chappy [Main Track] by Jimmy Kaleth, Ross Andrew McLean from www.killertracks.com This music requires a license for use.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.",
                "width": 1920,
                "height": 1080,
                "pixels": 2073600
            }
        }
    ],
    "sources": [
        {
            "id": 20299,
            "url": "https://svs.gsfc.nasa.gov/20299/",
            "page_type": "Animation",
            "title": "Parker Science Result animations",
            "description": "On Dec. 4, 2019, four new papers in the journal Nature describe what scientists working with data from NASA's Parker Solar Probe have learned from this unprecedented exploration of our star — and what they look forward to learning next. These findings reveal new information about the behavior of the material and particles that speed away from the Sun, bringing scientists closer to answering fundamental questions about the physics of our star. These animations represent five of those findings. || ",
            "release_date": "2019-12-04T13:00:00-05:00",
            "update_date": "2025-03-16T23:28:24.418035-04:00",
            "main_image": {
                "id": 392323,
                "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020200/a020299/SwitchbackSun_4k_0000_print.jpg",
                "filename": "SwitchbackSun_4k_0000_print.jpg",
                "media_type": "Image",
                "alt_text": "Top-down view of Switchback Magnetic FieldsParker indicated that the solar magnetic field embedded in the solar wind flips in the direction. These reversals — dubbed \"switchbacks\" — last anywhere from a few seconds to several minutes as they flow over Parker Solar Probe. During a switchback, the magnetic field whips back on itself until it is pointed almost directly back at the Sun.Credit: NASA Goddard/CIL/Adriana Manrique Gutierrez",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        }
    ],
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