{ "count": 91, "next": null, "previous": null, "results": [ { "id": 14957, "url": "https://svs.gsfc.nasa.gov/14957/", "result_type": "Produced Video", "release_date": "2026-01-27T10:00:00-05:00", "title": "IMAP Arrives at L1", "description": "NASA’s IMAP (Interstellar Mapping and Acceleration Probe) reached its destination at Lagrange point 1, or L1, approximately 1 million miles from Earth toward the Sun on Jan. 10, 2026.The mission’s operations team sent commands to the spacecraft on the morning of Jan. 9 to begin trajectory maneuvers to enter orbit at L1. Early on the morning of Jan. 10, the team confirmed the spacecraft had successfully entered its final L1 orbit, where it will stay for the duration of its mission.From L1, IMAP will explore and map the very boundaries of our heliosphere — the protective bubble created by the solar wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.Learn more about the milestone: https://science.nasa.gov/blogs/imap/2026/01/12/nasas-imap-mission-reaches-its-destination/ || ", "hits": 387 }, { "id": 14865, "url": "https://svs.gsfc.nasa.gov/14865/", "result_type": "Produced Video", "release_date": "2025-07-10T14:00:00-04:00", "title": "The Closest Images Ever Taken of the Sun’s Atmosphere", "description": "On its record-breaking pass by the Sun in December 2024, NASA’s Parker Solar Probe captured stunning new images from within the Sun’s atmosphere. These newly released images — taken closer to the Sun than we’ve ever been before — are helping scientists better understand the Sun’s influence across the solar system, including events that can affect Earth.Parker Solar Probe started its closest approach to the Sun on Dec. 24, 2024, flying just 3.8 million miles from the solar surface. As it skimmed through the Sun’s outer atmosphere, called the corona, in the days around the perihelion, it collected data with an array of scientific instruments, including the Wide-Field Imager for Solar Probe, or WISPR.Learn more - https://science.nasa.gov/science-research/heliophysics/nasas-parker-solar-probe-snaps-closest-ever-images-to-sun/Find the latest WISPR imagery here. || ", "hits": 594 }, { "id": 14816, "url": "https://svs.gsfc.nasa.gov/14816/", "result_type": "Produced Video", "release_date": "2025-04-11T11:00:00-04:00", "title": "IMAP Testing and Integration at NASA's Marshall Space Flight Center", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, arrived at NASA’s Marshall Space Flight Center on March 18, 2025, to undergo testing prior to launch. At Marshall, IMAP will be exposed to extreme temperature changes during a 28-day-long test inside a thermal vacuum chamber (TVAC). By simulating the harsh conditions in space, scientists and engineers can identify any potential issues before launch.To learn more about the testing visit: https://science.nasa.gov/blogs/imap/2025/05/07/nasas-imap-completes-thermal-vacuum-testing-campaign/After thermal vacuum testing concluded at NASA's Marshall Space Flight Center, IMAP was transported to Florida: https://science.nasa.gov/blogs/imap/2025/05/10/nasas-interstellar-mapping-mission-arrives-in-florida/ || ", "hits": 95 }, { "id": 14815, "url": "https://svs.gsfc.nasa.gov/14815/", "result_type": "B-Roll", "release_date": "2025-04-09T14:00:00-04:00", "title": "IMAP Testing and Integration at NASA's Goddard Space Flight Center", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, is embarking on its yearlong integration and testing campaign, during which its instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission.", "hits": 37 }, { "id": 14814, "url": "https://svs.gsfc.nasa.gov/14814/", "result_type": "B-Roll", "release_date": "2025-04-09T08:00:00-04:00", "title": "IMAP Testing and Integration at Johns Hopkins Applied Physics Lab", "description": "NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, is embarking on its yearlong integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission.", "hits": 92 }, { "id": 14802, "url": "https://svs.gsfc.nasa.gov/14802/", "result_type": "Produced Video", "release_date": "2025-03-28T14:31:59-04:00", "title": "Earth to Space: A National Symphony Orchestra Concert", "description": "Explore the vastness of space with music inspired by the planets, stars, and beyond! In anticipation of the upcoming voyage of Artemis II, the National Symphony Orchestra celebrates the discoveries and beauty of space through music and images produced by NASA. Explore this page to learn more about the visuals used in the Kennedy Center's 2025 Earth to Space Festival NSO Family Concert.", "hits": 117 }, { "id": 14741, "url": "https://svs.gsfc.nasa.gov/14741/", "result_type": "Produced Video", "release_date": "2024-12-27T13:00:00-05:00", "title": "Parker Solar Probe: Humanity’s Closest Encounter with the Sun", "description": "Controllers have confirmed NASA’s mission to “touch” the Sun survived its record-breaking closest approach to the solar surface on Dec. 24, 2024.Breaking its previous record by flying just 3.8 million miles above the surface of the Sun, NASA’s Parker Solar Probe hurtled through the solar atmosphere at a blazing 430,000 miles per hour — faster than any human-made object has ever moved. A beacon tone received in the late evening hours of Dec. 26 confirmed the spacecraft had made it through the encounter safely and is operating normally.This pass, the first of more to come at this distance, allows the spacecraft to conduct unrivaled scientific measurements with the potential to change our understanding of the Sun. || ", "hits": 604 }, { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "result_type": "Visualization", "release_date": "2024-12-12T12:00:00-05:00", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "hits": 297 }, { "id": 14622, "url": "https://svs.gsfc.nasa.gov/14622/", "result_type": "Produced Video", "release_date": "2024-07-03T13:00:00-04:00", "title": "Annular Solar Eclipse Broadcast Packages", "description": "Watch NASA's live broadcast as a “ring of fire” eclipse travels across the United States on Oct. 14, 2023, from Oregon to Texas. This event occurs when the Moon passes directly in front of the Sun, but appears too small to completely cover the Sun’s surface – resulting in what appears as a ring of fire in the sky. It’s also known as an annular solar eclipse. Everyone in the contiguous 48 states had the opportunity to see at least a partial eclipse on Oct. 14, 2023.Below is the collection of packages created for NASA's annular eclipse broadcast. || ", "hits": 44 }, { "id": 14596, "url": "https://svs.gsfc.nasa.gov/14596/", "result_type": "Produced Video", "release_date": "2024-05-29T11:00:00-04:00", "title": "Lucy Sees Asteroid Dinkinesh in Detail", "description": "Narrated video of Lucy’s encounter with the main-belt asteroid Dinkinesh and its satellite, Selam, on Nov. 1, 2023.Complete transcript available.Universal Production Music: “Gaining Positivity” by Ho Ling Tang [BMI] and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || Dinkinesh_Detailed_View_V2_print.jpg (1024x576) [64.4 KB] || Dinkinesh_Detailed_View_V2.jpg (1280x720) [159.2 KB] || Dinkinesh_Detailed_View_V2.png (1280x720) [165.4 KB] || Dinkinesh_Detailed_View_V2_searchweb.png (320x180) [13.4 KB] || Dinkinesh_Detailed_View_V2_thm.png (80x40) [1.9 KB] || 14596_Dinkinesh_Detailed_View_1080.mp4 (1920x1080) [55.5 MB] || 14596_Dinkinesh_Detailed_View_720.mp4 (1280x720) [11.4 MB] || DinkineshDetailedCaptions.en_US.srt [1.2 KB] || DinkineshDetailedCaptions.en_US.vtt [1.1 KB] || 14596_Dinkinesh_Detailed_View_4K.mp4 (3840x2160) [539.3 MB] || 14596_Dinkinesh_Detailed_View_ProRes.mov (3840x2160) [3.3 GB] || ", "hits": 47 }, { "id": 14582, "url": "https://svs.gsfc.nasa.gov/14582/", "result_type": "Produced Video", "release_date": "2024-05-14T10:00:00-04:00", "title": "DAVINCI Drop Testing at UTTR", "description": "The DAVINCI Project is led by NASA GSFC with primary partners at Lockheed Martin as well as from NASA’s JPL, JHU’s APL, Malin Space Science Systems, NASA’s LaRC, NASA ARC, University of Michigan, and Kinetx.The PI, Deputy PI’s and Program management team are at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The artwork shown here was developed for the DAVINCI team by CI Labs and the SVS. Special data analysis by the PI and Project Science team led by Dr. Jim Garvin, Dr. Stephanie Getty, and Dr. Giada Areny with Dr. Natasha Johnson and Dr. Erika Kohler is included. NASA Langley (LaRC) partners include Dr. S. Dutta and his team who developed the probe aerodynamic drop test experiment for the DAVINCI project. Narration is by Dr. Jim Garvin, PI for the DAVINCI mission to Venus. The DAVINCI Project acknowledges the continuing support of NASA’s Discovery Program, with DAVINCI Program Executive Andrea Riley and Program scientist Nick Lang, and Mission Manager Kevin Sykes. Music is \"Great Secrets\" by Thomas Alexander Farnon of Universal Production Music. || DAVINCI_REEL_THUMB.jpg (1080x1920) [584.4 KB] || DAVINCI_UTTR.01191_searchweb.png (320x180) [71.8 KB] || DAVINCI_UTTR.01191_thm.png (80x40) [6.4 KB] || DAVINCI_UTTR.en_US.srt [2.5 KB] || DAVINCI_UTTR.en_US.vtt [2.3 KB] || DAVINCI_UTTR.mp4 [30.7 MB] || ", "hits": 57 }, { "id": 14542, "url": "https://svs.gsfc.nasa.gov/14542/", "result_type": "Produced Video", "release_date": "2024-03-05T10:00:00-05:00", "title": "EZIE – Electrojet Zeeman Imaging Explorer", "description": "Slated to launch in 2025, NASA’s Electrojet Zeeman Imaging Explorer (EZIE) will be the first mission to image the magnetic fingerprint of the auroral electrojets — intense electric currents flowing high above Earth’s poles that are central to the electrical circuit coupling the planet’s magnetosphere to its atmosphere.Led by the Johns Hopkins Applied Physics Laboratory (APL), EZIE will use a trio of small satellites to characterize and record the electrojets’ structure over space and time. It will fill gaps in our understanding of this space weather phenomenon and provide findings that scientists can apply to other magnetized planets, both within and outside our solar system.Learn more:https://science.nasa.gov/mission/ezie/ || ", "hits": 99 }, { "id": 5214, "url": "https://svs.gsfc.nasa.gov/5214/", "result_type": "Visualization", "release_date": "2024-02-08T08:00:00-05:00", "title": "Geomagnetic Storm Causes Satellite Loss for Fulldome", "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events.This is 4k fulldome imagery intended for projection in a planetarium or other hemispherical dome theater. || ", "hits": 96 }, { "id": 5193, "url": "https://svs.gsfc.nasa.gov/5193/", "result_type": "Visualization", "release_date": "2023-12-11T09:00:00-05:00", "title": "Geomagnetic Storm Causes Satellite Loss", "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events. || ", "hits": 484 }, { "id": 31194, "url": "https://svs.gsfc.nasa.gov/31194/", "result_type": "Hyperwall Visual", "release_date": "2022-10-04T00:00:00-04:00", "title": "DART: Double Asteroid Redirection Test", "description": "The DART mission is NASA's demonstration of kinetic impactor technology, impacting an asteroid to adjust its speed and path. DART was the first-ever space mission to demonstrate asteroid deflection by kinetic impactor. It impacted the moonlet Dimorphos on September 26, 2022. || ", "hits": 287 }, { "id": 14210, "url": "https://svs.gsfc.nasa.gov/14210/", "result_type": "Produced Video", "release_date": "2022-09-20T06:00:00-04:00", "title": "History In The Making! Next Week NASA’s First Planetary Defense Mission Will Intentionally Crash Into A Small Asteroid Live Shots", "description": "Associated b-roll for the live shots to be added shortly. Click here for DART PRESS KITClick here for full IMAGE/VIDEO/ANIMATION gallery || LIVE_INTERVIEW_OPPORTUNITIES_AVAILABLE_print.jpg (1024x576) [162.9 KB] || LIVE_INTERVIEW_OPPORTUNITIES_AVAILABLE.png (2240x1260) [3.9 MB] || LIVE_INTERVIEW_OPPORTUNITIES_AVAILABLE_searchweb.png (320x180) [99.3 KB] || LIVE_INTERVIEW_OPPORTUNITIES_AVAILABLE_thm.png (80x40) [7.4 KB] || ", "hits": 139 }, { "id": 14151, "url": "https://svs.gsfc.nasa.gov/14151/", "result_type": "Produced Video", "release_date": "2022-05-05T06:00:00-04:00", "title": "NASA Interview Opportunity: Skywatchers’ Delight! Chat with NASA About How YOU Can See Next Weekend’s Total Lunar Eclipse", "description": "QUICK LINK TO EDITED, CUT B-ROLLQuick link to canned interview with NOAH PETROQuick link to canned interview with BRETT DENEVI Canned interview in SPANISH with FRANCISCO ANDOLZNEW!!: NASA Extends Exploration for 8 Planetary Science Missions including the Lunar Reconnaissance Orbiter. || updated_banner_lunar_eclipse_1.png (3125x1042) [2.0 MB] || updated_banner_lunar_eclipse_1_print.jpg (1024x341) [70.0 KB] || updated_banner_lunar_eclipse_1_searchweb.png (320x180) [63.6 KB] || updated_banner_lunar_eclipse_1_thm.png (80x40) [6.0 KB] || ", "hits": 39 }, { "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. || ", "hits": 861 }, { "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. || ", "hits": 650 }, { "id": 14035, "url": "https://svs.gsfc.nasa.gov/14035/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "AGU 2021 - Major discoveries as NASA’s Parker Solar Probe closes in on the Sun", "description": "NASA’s Parker Solar Probe has now done what no spacecraft has done before—it has officially touched the Sun. Launched in 2018 to study the Sun’s biggest mysteries, the spacecraft has now grazed the edge of the solar atmosphere and gathered new close-up observations of our star. This is allowing us to see the Sun as never before—including the findings in two new papers, which were presented at AGU, that are helping scientists answer fundamental questions about the Sun.PANELISTSDr. Nicola Fox• Heliophysics Division Director of the Science Mission Directorate at NASA HeadquartersDr. Nour Raouafi• Project Scientist for NASA’s Parker Solar Probe• The Johns Hopkins Applied Physics Laboratory Dr. Justin Kasper• Principal Investigator for Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Parker Solar Probe • BWX Technologies, Inc., University of MichiganProf. Stuart D. Bale• Principal Investigator for Fields Experiment (FIELDS) on Parker Solar Probe • University of California, Berkeley Dr. Kelly Korreck• Program Scientist at NASA Headquarters• Smithsonian Astrophysical Observatory || ", "hits": 161 }, { "id": 14036, "url": "https://svs.gsfc.nasa.gov/14036/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "Animation: NASA's Parker Solar Probe Enters Solar 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. The new milestone marks one major step for Parker Solar Probe and one giant leap for solar science. Just as landing on the Moon allowed scientists to understand how it was formed, touching the very stuff the Sun is made of will help scientists uncover critical information about our closest star and its influence on the solar system. On April 28, 2021, during its eighth flyby of the Sun, Parker Solar Probe encountered the specific magnetic and particle conditions at 18.8 solar radii (8.127 million miles) above the solar surface that told scientists it had crossed the Alfvén critical surface for the first time and finally entered the solar atmosphere.More information here. || ", "hits": 299 }, { "id": 14045, "url": "https://svs.gsfc.nasa.gov/14045/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "NASA's Parker Solar Probe Touches The Sun For The First Time", "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. The new milestone marks one major step for Parker Solar Probe and one giant leap for solar science. Just as landing on the Moon allowed scientists to understand how it was formed, touching the very stuff the Sun is made of will help scientists uncover critical information about our closest star and its influence on the solar system. More information here. || ", "hits": 243 }, { "id": 13985, "url": "https://svs.gsfc.nasa.gov/13985/", "result_type": "Produced Video", "release_date": "2021-11-16T06:00:00-05:00", "title": "NASA Just Days Away From Launching Humanity’s First-Ever Asteroid-Deflecting Mission Live Shots", "description": "Click here for the DART PRESS KITClick here for B-ROLL resourcesQuick link for cut Live Shot B-ROLLClick here for quick link to CANNED INTERVIEW with Tom Statler / DART Program Scientist || DART_banner_2.png (3214x804) [3.0 MB] || DART_banner_2_print.jpg (1024x256) [74.4 KB] || DART_banner_2_searchweb.png (320x180) [78.8 KB] || DART_banner_2_thm.png (80x40) [9.8 KB] || ", "hits": 136 }, { "id": 13887, "url": "https://svs.gsfc.nasa.gov/13887/", "result_type": "Produced Video", "release_date": "2021-07-27T10:00:00-04:00", "title": "DAVINCI Probe's Eye View", "description": "An overview of the DAVINCI mission through the eyes of the descent probe.Music is \"Mountains of Hokkaido\" by Natalie Holt and Yoann Le Dantec of Universal Production Music || 13887_DAVINCI_PEVAA.02257_print.jpg (1024x576) [101.1 KB] || 13887_thumbnail.jpg (1920x1080) [157.6 KB] || 13887_DAVINCI_PEVAA.02257_searchweb.png (320x180) [69.3 KB] || 13887_DAVINCI_PEVAA.02257_thm.png (80x40) [5.1 KB] || 13887_DAVINCI_PEVAA.mp4 (1920x1080) [177.3 MB] || 13887_DAVINCI_PEVAA_twitter_720.mp4 (1280x720) [32.7 MB] || 13887_DAVINCI_PEVAA_facebook_720.mp4 (1280x720) [190.4 MB] || 13887_DAVINCI_PEVAA.webm (960x540) [47.1 MB] || 13877_DAVINCI_PEVAA_caption.en_US.srt [2.9 KB] || 13877_DAVINCI_PEVAA_caption.en_US.vtt [2.8 KB] || ", "hits": 89 }, { "id": 13862, "url": "https://svs.gsfc.nasa.gov/13862/", "result_type": "Produced Video", "release_date": "2021-05-12T16:00:00-04:00", "title": "Chromatics Centrifuge Concert", "description": "The Chromatics, an AstroCappella group, sings in front of NASA Goddard’s centrifuge. || Chromatics_-_Dance_of_the_Planets_larger_version.00017_print.jpg (1024x576) [1.3 KB] || Chromatics_-_Dance_of_the_Planets_larger_version.00017_searchweb.png (320x180) [278 bytes] || Chromatics_-_Dance_of_the_Planets_larger_version.00017_thm.png (80x40) [262 bytes] || Chromatics_-_Dance_of_the_Planets_larger_version.mp4 (3840x2160) [515.8 MB] || The_Chromatics.en_US.srt [3.0 KB] || The_Chromatics.en_US.vtt [2.8 KB] || Chromatics_-_Dance_of_the_Planets_larger_version.webm (3840x2160) [60.8 MB] || ", "hits": 10 }, { "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": 49 }, { "id": 13738, "url": "https://svs.gsfc.nasa.gov/13738/", "result_type": "Produced Video", "release_date": "2020-10-19T11:30:00-04:00", "title": "OSIRIS-REx Science and Engineering Briefing", "description": "Main title for T-1 OSIRIS-REx Science and Engineering Briefing || t-1_title.jpg (2878x1618) [2.5 MB] || t-1_title_searchweb.png (320x180) [58.9 KB] || t-1_title_thm.png (80x40) [4.2 KB] || ", "hits": 41 }, { "id": 13724, "url": "https://svs.gsfc.nasa.gov/13724/", "result_type": "Produced Video", "release_date": "2020-09-24T14:25:00-04:00", "title": "OSIRIS-REx: Countdown to TAG", "description": "Trailer for the OSIRIS-REx TAG EventUniversal Production Music: \"The Glory of Victory\" by Frederik WiedmannCredit: NASA/Goddard || tagtrailer13725_print.jpg (1024x576) [67.1 KB] || tagtrailer13725.jpg (3840x2160) [354.2 KB] || tagtrailer_twitter_720.mp4 (1280x720) [18.8 MB] || tagtrailer_facebook_720.webm (1280x720) [11.4 MB] || tagtrailer_facebook_720.mp4 (1280x720) [107.3 MB] || tagtrailercaption.en_US.srt [1.6 KB] || tagtrailercaption.en_US.vtt [1.6 KB] || tagtrailer.mp4 (3840x2160) [106.9 MB] || ", "hits": 58 }, { "id": 13687, "url": "https://svs.gsfc.nasa.gov/13687/", "result_type": "Produced Video", "release_date": "2020-08-14T10:00:00-04:00", "title": "NASA Spacecraft Uncover Mystery Behind Auroral Beads", "description": "A special type of aurora, draped east-west across the night sky like a glowing pearl necklace, is helping scientists better understand the science of auroras and their powerful drivers out in space. Known as auroral beads, these lights often show up just before large auroral displays, which are caused by electrical storms in space called substorms. Until now, scientists weren’t sure if auroral beads are somehow connected to other auroral displays as a phenomenon in space that precedes substorms, or if they are caused by disturbances closer to Earth’s atmosphere.But powerful new computer models, combined with observations from NASA’s Time History of Events and Macroscale Interactions during Substorms – THEMIS – mission, have provided the first direct evidence of the events in space that lead to the appearance of these beads, and demonstrated the important role they play in our local space environment. || ", "hits": 80 }, { "id": 13661, "url": "https://svs.gsfc.nasa.gov/13661/", "result_type": "Produced Video", "release_date": "2020-07-10T09:50:00-04:00", "title": "NASA Missions Spot Comet NEOWISE", "description": "These images from ESA and NASA’s Solar and Heliospheric Observatory show comet NEOWISE as it approached the Sun in late June 2020. The instrument that produced this data is a coronagraph, which uses a solid disk to block out the Sun’s bright face, revealing the comparatively outer atmosphere, the corona, along with objects like comet NEOWISE. Credit: ESA/NASA/SOHO || wide.00250_print.jpg (1024x576) [164.4 KB] || wide.mp4 (3840x2160) [72.2 MB] || wide.webm (3840x2160) [6.2 MB] || ", "hits": 82 }, { "id": 13628, "url": "https://svs.gsfc.nasa.gov/13628/", "result_type": "Produced Video", "release_date": "2020-06-12T10:00:00-04:00", "title": "Parker Solar Probe Teams Up with Observatories Around the Solar System for Fourth Solar Encounter", "description": "At the heart of understanding our space environment is the knowledge that conditions throughout space — from the Sun to the atmospheres of planets to the radiation environment in deep space — are connected.Studying this connection – a field of science called heliophysics — is a complex task: Researchers track sudden eruptions of material, radiation, and particles against the background of the ubiquitous outflow of solar material.A confluence of events in early 2020 created a nearly ideal space-based laboratory, combining the alignment of some of humanity’s best observatories — including Parker Solar Probe, during its fourth solar flyby — with a quiet period in the Sun’s activity, when it’s easiest to study those background conditions. These conditions provided a unique opportunity for scientists to study how the Sun influences conditions at points throughout space, with multiple angles of observation and at different distances from the Sun. || ", "hits": 65 }, { "id": 13562, "url": "https://svs.gsfc.nasa.gov/13562/", "result_type": "Produced Video", "release_date": "2020-02-25T16:00:00-05:00", "title": "The Science of Dragonfly", "description": "Dragonfly’s suite of science instruments will investigate the chemistry and habitability of Titan.Universal Production Music: “Clediss” by Thomas Stempfle and Tom Sue, “Downloading Landscapes” by Andrew Michael Britton and David Stephen GoldsmithWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || FACEBOOK_720_13562_Dragonfly_Science_MASTER_facebook_720.mp4 (1280x720) [145.8 MB] || DragonflySciencePreview_print.jpg (1024x576) [96.9 KB] || DragonflySciencePreview.jpg (3840x2160) [637.4 KB] || DragonflySciencePreview_searchweb.png (320x180) [72.4 KB] || DragonflySciencePreview_thm.png (80x40) [5.5 KB] || TWITTER_720_13562_Dragonfly_Science_MASTER_twitter_720.mp4 (1280x720) [27.2 MB] || 13562_Dragonfly_Science_MASTER.webm (960x540) [46.9 MB] || 13562_Dragonfly_Science_CAPTIONS.en_US.srt [3.4 KB] || 13562_Dragonfly_Science_CAPTIONS.en_US.vtt [3.4 KB] || 13562_Dragonfly_Science_YouTube.mp4 (3840x2160) [2.7 GB] || 13562_Dragonfly_Science_MASTER.mov (3840x2160) [16.6 GB] || ", "hits": 140 }, { "id": 20311, "url": "https://svs.gsfc.nasa.gov/20311/", "result_type": "Animation", "release_date": "2020-02-25T16:00:00-05:00", "title": "Dragonfly Animation Resource Page", "description": "Dragonfly on Titan || DF_End_Pan_4K_Prores.00420_print.jpg (1024x576) [77.6 KB] || DF_End_Pan_H264_1080.mp4 (1920x1080) [27.1 MB] || DF_End_Pan_4K_H264.mp4 (3840x2160) [15.4 MB] || DF_End_Pan_4K_Prores_PNG (3840x2160) [0 Item(s)] || DF_End_Pan_4K_Prores.webm (3840x2160) [7.0 MB] || DF_End_Pan_4K_Prores.mov (3840x2160) [1.7 GB] || ", "hits": 278 }, { "id": 13494, "url": "https://svs.gsfc.nasa.gov/13494/", "result_type": "Produced Video", "release_date": "2019-12-11T13:00:00-05:00", "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission", "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 || ", "hits": 101 }, { "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": 13484, "url": "https://svs.gsfc.nasa.gov/13484/", "result_type": "Produced Video", "release_date": "2019-12-04T13:00:00-05:00", "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. || ", "hits": 68 }, { "id": 13491, "url": "https://svs.gsfc.nasa.gov/13491/", "result_type": "Produced Video", "release_date": "2019-12-04T00:00:00-05:00", "title": "NASA Science Live: New Discoveries from Our Mission to Touch the Sun (Episode 12)", "description": "NASA Science Live: New Discoveries from Our Mission to Touch the Sun (Episode 12) || 13491_NSL_Parker_Ep12.00001_print.jpg (1024x576) [85.1 KB] || 13491_NSL_Parker_Ep12.00001_searchweb.png (320x180) [82.0 KB] || 13491_NSL_Parker_Ep12.00001_thm.png (80x40) [5.7 KB] || 13491_NSL_Parker_Ep12_lowres.mp4 (1280x720) [1.1 GB] || 13491_NSL_Parker_Ep12_youtube_720.mp4 (1280x720) [6.4 GB] || 13491_NSL_Parker_Ep12.mov (1280x720) [42.2 GB] || 13491_NSL_Parker_Ep12_youtube_720.webm (1280x720) [453.7 MB] || 13491_NSL_Parker_Ep12.en_US.srt [113.5 KB] || 13491_NSL_Parker_Ep12.en_US.vtt [106.5 KB] || ", "hits": 84 }, { "id": 13245, "url": "https://svs.gsfc.nasa.gov/13245/", "result_type": "Produced Video", "release_date": "2019-06-27T00:00:00-04:00", "title": "NASA Science Live: NASA's Next New Frontiers Mission [Special Edition]", "description": "NASA Science Live: NASA's Next New Fountiers Mission [Special Edition]Program Aired June 27, 2019 || 13245_NSL_SE_Dragonfly_youtube.00001_print.jpg (1024x576) [77.7 KB] || 13245_NSL_SE_Dragonfly_youtube.00001_searchweb.png (320x180) [81.3 KB] || 13245_NSL_SE_Dragonfly_youtube.00001_thm.png (80x40) [5.6 KB] || 13245_NSL_SE_Dragonfly_youtube.webm (1280x720) [338.5 MB] || 13245_NSL_SE_Dragonfly_lowres.mp4 (1280x720) [844.5 MB] || 13245_NSL_SE_Dragonfly.en_US.srt [72.8 KB] || 13245_NSL_SE_Dragonfly.en_US.vtt [68.8 KB] || 13245_NSL_SE_Dragonfly_youtube.mp4 (1280x720) [4.9 GB] || 13245_NSL_SE_Dragonfly.mov (1280x720) [31.7 GB] || ", "hits": 68 }, { "id": 13078, "url": "https://svs.gsfc.nasa.gov/13078/", "result_type": "Produced Video", "release_date": "2019-04-15T11:00:00-04:00", "title": "Water Released from Moon During Meteor Showers", "description": "Data from the LADEE spacecraft reveal that the lunar surface is periodically releasing water.Music provided by Killer Tracks: Virtual MemoryComplete transcript available. Watch this video on the NASA Goddard YouTube channel. || LADEE_Moon_Earth_Preview_V4_print.jpg (1024x576) [181.9 KB] || LADEE_Moon_Earth_Preview_V4.jpg (1280x720) [281.6 KB] || LADEE_Moon_Earth_Preview_V4_searchweb.png (180x320) [46.5 KB] || LADEE_Moon_Earth_Preview_V4_thm.png (80x40) [3.9 KB] || TWITTER_720_13078_LADEE_Water_Short_MASTER_twitter_720.mp4 (1280x720) [21.1 MB] || 13078_LADEE_Water_Short_MASTER.webm (960x540) [48.9 MB] || YOUTUBE_1080_13078_LADEE_Water_Short_MASTER_youtube_1080.mp4 (1920x1080) [176.0 MB] || FACEBOOK_720_13078_LADEE_Water_Short_MASTER_facebook_720.mp4 (1280x720) [134.7 MB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.srt [2.6 KB] || 13078_LADEE_Water_Short_MASTER_Output.en_US.vtt [2.6 KB] || 13078_LADEE_Water_Short_MASTER.mp4 (3840x2160) [940.5 MB] || 13078_LADEE_Water_Short_MASTER.mov (3840x2160) [5.5 GB] || ", "hits": 91 }, { "id": 20278, "url": "https://svs.gsfc.nasa.gov/20278/", "result_type": "Animation", "release_date": "2019-04-15T11:00:00-04:00", "title": "Water Released from Moon During Meteor Showers: Animations", "description": "Scientists have discovered that water is being released from the moon during meteor showers. When a speck of comet debris strikes the moon it vaporizes on impact, creating a shock wave in the lunar soil. For a sufficiently large impactor, this shock wave can breach the soil’s dry upper layer and release water molecules from a hydrated layer below. The LADEE spacecraft detects these water molecules as they enter the tenuous lunar atmosphere. || ", "hits": 402 }, { "id": 13153, "url": "https://svs.gsfc.nasa.gov/13153/", "result_type": "Produced Video", "release_date": "2019-02-27T00:00:00-05:00", "title": "NASA Science Live: To the Moon and Beyond (Episode 01)", "description": "NASA Science Live Episode 01: To the Moon and BeyondProgram Aired February 27, 2019 at 3pm || 13153_NASA_Science_Live_Ep01_youtube.00471_print.jpg (1024x576) [80.0 KB] || 13153_NASA_Science_Live_Ep01_youtube.00471_searchweb.png (320x180) [79.0 KB] || 13153_NASA_Science_Live_Ep01_youtube.00471_thm.png (80x40) [5.6 KB] || 13153_NASA_Science_Live_Ep01_lowres.mp4 (1280x720) [551.7 MB] || 13153_NASA_Science_Live_Ep01_youtube.mp4 (1280x720) [3.3 GB] || 13153_NASA_Science_Live_Ep01.mov (1280x720) [20.8 GB] || 13153_NASA_Science_Live_Ep01.webm (960x540) [825.0 MB] || 13153_NASA_Science_Live_Ep01.en_US.srt [50.8 KB] || 13153_NASA_Science_Live_Ep01.en_US.vtt [48.0 KB] || ", "hits": 86 }, { "id": 13113, "url": "https://svs.gsfc.nasa.gov/13113/", "result_type": "Produced Video", "release_date": "2018-12-12T15:00:00-05:00", "title": "AGU 2018 - Expected Data and Scientific Discovery from NASA’s Parker Solar Probe", "description": "Animation of NASA's Parker Solar Probe in the solar wind. Credit: NASA/GSFC/CIL/Brian Monroe || 1_Nicky_ParkerBeautyPass_1.00200_print.jpg (1024x576) [34.0 KB] || 1_Nicky_ParkerBeautyPass_1.mp4 (1920x1080) [24.5 MB] || 1_Nicky_ParkerBeautyPass_1.webm (1920x1080) [2.4 MB] || ", "hits": 35 }, { "id": 13105, "url": "https://svs.gsfc.nasa.gov/13105/", "result_type": "Produced Video", "release_date": "2018-11-02T14:00:00-04:00", "title": "First Perihelion: Into the Unknown with Parker Solar Probe", "description": "Complete transcript available.Watch this video on the JHU/APL YouTube channel. || 1803932PSPRISKmixedfinalscreener.03961_print.jpg (1024x576) [97.7 KB] || 1803932PSPRISKmixedfinalscreener.03961_searchweb.png (320x180) [78.1 KB] || 1803932PSPRISKmixedfinalscreener.03961_thm.png (80x40) [5.7 KB] || 1803932PSPRISKmixedfinalscreener.mp4 (1280x720) [130.4 MB] || 1803932PSPRISKmixedfinalscreener.webm (1280x720) [23.0 MB] || FirstPerihelioncaptions.en_US.srt [3.5 KB] || FirstPerihelioncaptions.en_US.vtt [3.6 KB] || ", "hits": 241 }, { "id": 13046, "url": "https://svs.gsfc.nasa.gov/13046/", "result_type": "Produced Video", "release_date": "2018-08-22T14:00:00-04:00", "title": "Sunset Show for Parker Solar Probe", "description": "Early in the morning of Aug. 12, NASA launched Parker Solar Probe, humanity’s first mission to the Sun. This spacecraft will fly closer to the Sun than any before it, in a daring journey facing brutal heat and radiation. Parker Solar Probe sets its sights on the Sun’s scorching outer atmosphere, called the corona, in order to solve our star’s greatest mysteries. It will revolutionize our understanding not only of the Sun, but also the space around us, and even the lives of stars beyond our solar system — crucial information as we explore more of space.On Aug. 10, scientists and mission experts gathered at NASA’s Kennedy Space Center for a live sunset show — one of the last times the Sun set on Parker Solar Probe before it launched — to talk about what this landmark mission will teach us of the Sun. Guests included: - Jim Spann, Chief Solar Scientist, NASA HQ- Yari Collado-Vega, Space Weather Scientist, NASA Goddard- C. Alex Young, Solar Scientist, NASA Goddard- Nicola Fox, Parker Solar Probe Project Scientist, JHU Applied Physics Laboratory (APL) || ", "hits": 46 }, { "id": 13039, "url": "https://svs.gsfc.nasa.gov/13039/", "result_type": "Produced Video", "release_date": "2018-08-12T05:00:00-04:00", "title": "Eugene Parker Reacts To Parker Solar Probe Launch", "description": "B-roll - Short versionDr. Eugene Parker watches the launch of the spacecraft that bears his name — NASA’s Parker Solar Probe — early in the morning of Aug. 12, 2018. Parker Solar Probe is humanity’s first mission to the Sun and will travel closer to our star than any spacecraft before. || Parker1024.jpg (1024x568) [667.9 KB] || Parker_SearchWeb.jpg (320x180) [77.7 KB] || Parker_Thumbnail.jpg (80x40) [7.4 KB] || 18-08-12_Eugene_Parker_Views_PSP_Launch_UHD_ShortVersion_18-00001.mp4 (3840x2160) [567.9 MB] || 18-08-12_Eugene_Parker_Views_PSP_Launch_UHD_ShortVersion_18-00001.webm (3840x2160) [17.5 MB] || ", "hits": 41 }, { "id": 13029, "url": "https://svs.gsfc.nasa.gov/13029/", "result_type": "Produced Video", "release_date": "2018-08-09T00:00:00-04:00", "title": "Parker Solar Probe Pre-Launch Briefing", "description": "Hosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Scott Messer - Program Manager, NASA Programs, United Launch AllianceOmar Baez - Launch Director, NASA, Kennedy Space CenterKathy Rice - Launch Weather Officer, 45th Weather Squadron, Cape Canaveral Air Force StationThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASANicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAndy Dreisman - Project Manger The Johns Hopkins University Applied Physics Lab || ", "hits": 39 }, { "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": 303 }, { "id": 13028, "url": "https://svs.gsfc.nasa.gov/13028/", "result_type": "Produced Video", "release_date": "2018-08-08T00:00:00-04:00", "title": "Parker Solar Probe Media Telecons", "description": "This is a resource page for the media teleconferences on August 8, 2018. || ", "hits": 63 }, { "id": 13024, "url": "https://svs.gsfc.nasa.gov/13024/", "result_type": "Produced Video", "release_date": "2018-07-31T11:00:00-04:00", "title": "Parker Solar Probe Prepares to Head Toward Launch Pad", "description": "NASA’s Parker Solar Probe is lifted to the third stage rocket motor on July 11, 2018, at Astrotech Space Operations in Titusville, Florida. In addition to using the largest operational launch vehicle, the Delta IV Heavy, Parker Solar Probe will use a third stage rocket to gain the speed needed to reach the Sun, which takes 55 times more energy than reaching Mars.Credit: NASA/Johns Hopkins APL/Ed Whitman || aPSPLift3.jpg (1920x1280) [1.7 MB] || ", "hits": 51 }, { "id": 13001, "url": "https://svs.gsfc.nasa.gov/13001/", "result_type": "Produced Video", "release_date": "2018-07-30T11:50:00-04:00", "title": "Parker Solar Probe", "description": "NASA's mission to touch the Sun begins its journey in 2018 || 01_Cover_forStory.png (1280x720) [920.1 KB] || 01_Cover_forStory_print.jpg (1024x576) [74.5 KB] || 01_Cover_forStory_thm.png (80x40) [5.2 KB] || 01_Cover_forStory_searchweb.png (320x180) [71.7 KB] || ", "hits": 120 }, { "id": 12903, "url": "https://svs.gsfc.nasa.gov/12903/", "result_type": "Produced Video", "release_date": "2018-07-25T14:00:00-04:00", "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. || ", "hits": 260 }, { "id": 12911, "url": "https://svs.gsfc.nasa.gov/12911/", "result_type": "Produced Video", "release_date": "2018-07-20T13:00:00-04:00", "title": "Parker Solar Probe Trailer", "description": "Trailer without text introduction. Music credit: Luminous Skies [Underscore] by Andrew Prahlow from www.killertracks.comComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || 1080trailer_updated_animation2_youtube_1080.02350_print.jpg (1024x576) [78.9 KB] || 1080trailer_updated_animation2_youtube_1080.02350_thm.png (80x40) [5.1 KB] || 1080trailer_updated_animation2_youtube_1080.02350_searchweb.png (320x180) [67.6 KB] || 1080trailer_updated_animation2_appletv.m4v (1280x720) [44.4 MB] || 1080trailer_updated_animation2_appletv_subtitles.m4v (1280x720) [44.4 MB] || 1080trailer_updated_animation_TEXT_large.mp4 (1920x1080) [80.8 MB] || 1080trailer_updated_animation2_youtube_1080.webm (1920x1080) [8.9 MB] || 1080trailer_updated_animation2_large.mp4 (1920x1080) [80.6 MB] || 1080trailer_updated_animation2_youtube_1080.mp4 (1920x1080) [136.9 MB] || 1080trailer_updated_animation2.mpeg (1280x720) [262.4 MB] || 1080trailer_updated_animation2_prores.mov (1280x720) [897.5 MB] || 1080trailer_updated_animation2.en_US.srt [741 bytes] || 1080trailer_updated_animation2.en_US.vtt [754 bytes] || 1080trailer_updated_animation2_youtube_4k.mp4 (3840x2160) [338.7 MB] || 1080trailer_updated_animation2.mov (1920x1080) [1.7 GB] || 1080trailer_updated_animationTEXT_ipod_sm.mp4 (320x240) [14.6 MB] || 1080trailer_updated_animation2_ipod_sm.mp4 (320x240) [14.1 MB] || ", "hits": 45 }, { "id": 13003, "url": "https://svs.gsfc.nasa.gov/13003/", "result_type": "Produced Video", "release_date": "2018-07-20T12:30:00-04:00", "title": "Parker Solar Probe Science Briefing - Visual Resources", "description": "July 20, 2018 - Live from NASA Kennedy - 1:00 p.m. ESTHosted by Karen Fox - Heliophysics Communications Lead, NASA Goddard/NASA HQSpeakers:Nicola Fox - Parker Solar Probe Project Scientist, The Johns Hopkins University Applied Physics LabAlex Young - Solar Scientist from NASA GoddardThomas Zurbuchen - Associate Administrator for the Science Mission Directorate at NASABetsy Congdon - Thermal Protection System Engineer at The Johns Hopkins University Applied Physics Lab || ", "hits": 51 }, { "id": 12867, "url": "https://svs.gsfc.nasa.gov/12867/", "result_type": "Produced Video", "release_date": "2018-07-19T15:00:00-04:00", "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] || ", "hits": 55 }, { "id": 12866, "url": "https://svs.gsfc.nasa.gov/12866/", "result_type": "Produced Video", "release_date": "2018-07-19T13:00:00-04:00", "title": "Blowtorch vs Heat Shield", "description": "Music Credit: Toy Factory In Progress by Laurent Dury from www.killertracks.com This music requires a license for use.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || torchtestthumb.jpg (1920x1080) [270.1 KB] || torchtestthumb_searchweb.png (320x180) [90.3 KB] || torchtestthumb_thm.png (80x40) [7.1 KB] || 12866_torchtest_V3_APR422.59.94.mov (1920x1080) [3.2 GB] || 12866_torchtest_V3_appletv.m4v (1280x720) [63.3 MB] || 12866_torchtest_V3_youtube_hq.mov (1920x1080) [1.7 GB] || 12866_torchtest_V3.mpeg (1280x720) [391.6 MB] || 12866_torchtest_V3_youtube_hq.webm (1920x1080) [13.4 MB] || 12866_torchtest_V3_appletv_subtitles.m4v (1280x720) [63.3 MB] || 12866_torchtest_V3_youtube_4k.mp4 (3840x2160) [510.1 MB] || 12866_torchtest_V3_APR422.en_US.srt [2.0 KB] || 12866_torchtest_V3_APR422.en_US.vtt [2.0 KB] || ", "hits": 177 }, { "id": 12997, "url": "https://svs.gsfc.nasa.gov/12997/", "result_type": "Produced Video", "release_date": "2018-07-12T15:00:00-04:00", "title": "Parker Solar Probe Beauty Images", "description": "Still ImageParker Solar Probe sits in a clean room on July 6, 2018, at Astrotech Space Operations in Titusville, Florida, after the installation of its heat shield.Credit: NASA/Johns Hopkins APL/Ed Whitman || 5D1_9384_print.jpg (1024x774) [479.3 KB] || 5D1_9384.jpg (3840x2903) [6.6 MB] || 5D1_9384_searchweb.png (320x180) [88.4 KB] || 5D1_9384_web.png (320x241) [114.7 KB] || 5D1_9384_thm.png (80x40) [6.8 KB] || ", "hits": 108 }, { "id": 12992, "url": "https://svs.gsfc.nasa.gov/12992/", "result_type": "Produced Video", "release_date": "2018-07-05T11:00:00-04:00", "title": "Cutting-Edge Heat Shield Installed on NASA’s Parker Solar Probe", "description": "The launch of Parker Solar Probe, the mission that will get closer to the Sun than any human-made object has ever gone, is quickly approaching, and on June 27, 2018, Parker Solar Probe’s heat shield – called the Thermal Protection System, or TPS – was installed on the spacecraft. A mission sixty years in the making, Parker Solar Probe will make a historic journey to the Sun’s corona, a region of the solar atmosphere. With the help of its revolutionary heat shield, now permanently attached to the spacecraft in preparation for its August 2018 launch, the spacecraft’s orbit will carry it to within 4 million miles of the Sun's fiercely hot surface, where it will collect unprecedented data about the inner workings of the corona. The eight-foot-diameter heat shield will safeguard everything within its umbra, the shadow it casts on the spacecraft. At Parker Solar Probe’s closest approach to the Sun, temperatures on the heat shield will reach nearly 2,500 degrees Fahrenheit, but the spacecraft and its instruments will be kept at a relatively comfortable temperature of about 85 degrees Fahrenheit. The heat shield is made of two panels of superheated carbon-carbon composite sandwiching a lightweight 4.5-inch-thick carbon foam core. The Sun-facing side of the heat shield is also sprayed with a specially formulated white coating to reflect as much of the Sun’s energy away from the spacecraft as possible. The heat shield itself weighs only about 160 pounds – here on Earth, the foam core is 97% air. Because Parker Solar Probe travels so fast – 430,000 miles per hour at its closest approach to the Sun, fast enough to travel from Philadelphia to Washington, D.C., in about one second – the shield and spacecraft have to be light to achieve the needed orbit. The reinstallation of the Thermal Protection System – which was briefly attached to the spacecraft during testing at the Johns Hopkins Applied Physics Lab in Laurel, Maryland, in fall 2017 – marks the first time in months that Parker Solar Probe has been fully integrated. The heat shield and spacecraft underwent testing and evaluation separately at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, before shipping out to Astrotech Space Operations in Titusville, Florida, in April 2018. With the recent reunification, Parker Solar Probe inches closer to launch and toward the Sun. Parker Solar Probe is part of NASA’s Living with a Star Program, or LWS, to explore aspects of the Sun-Earth system that directly affect life and society. LWS is managed by NASA Goddard for the Heliophysics Division of NASA’s Science Mission Directorate in Washington, D.C. The Johns Hopkins Applied Physics Laboratory manages the Parker Solar Probe mission for NASA. APL designed and built the spacecraft and will also operate it. || ", "hits": 243 }, { "id": 12979, "url": "https://svs.gsfc.nasa.gov/12979/", "result_type": "Produced Video", "release_date": "2018-06-06T15:00:00-04:00", "title": "Power Up: Solar Arrays Installed on NASA’s Mission to Touch the Sun", "description": "NASA’s Parker Solar Probe depends on the Sun, not just as an object of scientific investigation, but also for the power that drives its instruments and systems. On Thursday, May 31, 2018, the spacecraft’s solar arrays were installed and tested. These arrays will power all of the spacecraft’s systems, including the suites of scientific instruments studying the solar wind and the Sun’s corona as well as the Solar Array Cooling System (SACS) that will protect the arrays from the extreme heat at the Sun. “Unlike solar-powered missions that operate far from the Sun and are focused only on generating power from it, we need to manage the power generated along with the substantial heat that comes from being so close to the Sun,” said Andy Driesman, project manager from the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland. “When we’re out around the orbit of Venus, we fully extend the arrays to get the power we need. But when we’re near the Sun, we tuck the arrays back until only a small wing is exposed, and that portion is enough to provide needed electrical power.”The solar arrays are cooled by a gallon of water that circulates through tubes in the arrays and into large radiators at the top of the spacecraft. They are just over three and a half feet (1.12 meters) long and nearly two and a half feet (0.69 meters) wide. Mounted on motorized arms, the arrays will retract almost all of their surface behind the Thermal Protection System – the heat shield – when the spacecraft is close to the Sun. The solar array installation marks some of the final preparation and testing of Parker Solar Probe leading up to the mission’s July 31 launch date. || ", "hits": 41 }, { "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": 268 }, { "id": 12959, "url": "https://svs.gsfc.nasa.gov/12959/", "result_type": "Produced Video", "release_date": "2018-05-21T11:00:00-04:00", "title": "More than 1.1 Million Names Installed on NASA’s Parker Solar Probe", "description": "Still imageA Parker Solar Probe team member from the Johns Hopkins Applied Physics Laboratory holds the memory card containing 1,137,202 names submitted by the public to travel to the Sun aboard the spacecraft. The card was installed on a plaque which was placed on the spacecraft on May 18, 2018, at Astrotech Space Operations in Titusville, Florida. The plaque dedicated the mission to Eugene Parker, who first theorized the existence of the solar wind. Parker Solar Probe is the first NASA mission to be named for a living person.Credit: NASA/Johns Hopkins APL/Ed Whitman || PlaqueChip1.jpg (1920x1280) [1.2 MB] || PlaqueChip1_print.jpg (1024x682) [319.1 KB] || PlaqueChip1_searchweb.png (320x180) [61.8 KB] || PlaqueChip1_web.png (320x213) [72.0 KB] || PlaqueChip1_thm.png (80x40) [6.0 KB] || ", "hits": 56 }, { "id": 12953, "url": "https://svs.gsfc.nasa.gov/12953/", "result_type": "Produced Video", "release_date": "2018-05-17T18:00:00-04:00", "title": "Parker Solar Probe Gets Visit From Namesake", "description": "B-rollEugene N. Parker, professor emeritus at the University of Chicago, today visited the spacecraft that bears his name: NASA’s Parker Solar Probe. This is the first NASA mission that has been named for a living researcher, and is humanity’s first mission to the Sun.Parker proposed the existence of the constant outflow of solar material from the sun, which is now called the solar wind, and theorized other fundamental stellar science processes. On Oct. 3, 2017, he viewed the spacecraft in a clean room at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, where the probe was designed and is being built. He discussed the revolutionary heat shield and instruments with the Parker Solar Probe team and learned how the spacecraft will answer some of the crucial questions Parker identified about how stars work.NASA’s Parker Solar Probe is scheduled for launch on July 31, 2018, from Cape Canaveral Air Force Station, Florida. The spacecraft will explore the Sun’s outer atmosphere and make critical observations that will answer decades-old questions about the physics of stars. The resulting data will also improve forecasts of major eruptions on the sun and subsequent space weather events that impact life on Earth, as well as satellites and astronauts in space.Credit: NASA/Johns Hopkins APL/Lee Hobson || EugeneParkerVisitsPSPSC_March10_2017_large.00333_print.jpg (1024x576) [84.6 KB] || EugeneParkerVisitsPSPSC_March10_2017_large.00333_searchweb.png (320x180) [77.0 KB] || EugeneParkerVisitsPSPSC_March10_2017_large.00333_web.png (320x180) [77.0 KB] || EugeneParkerVisitsPSPSC_March10_2017_large.00333_thm.png (80x40) [6.3 KB] || EugeneParkerVisitsPSPSC_March10_2017.mp4 (1920x1080) [1.1 GB] || PRORES_B-ROLL_EugeneParkerVisitsPSPSC_March10_2017_prores.mov (1280x720) [4.4 GB] || YOUTUBE_1080_EugeneParkerVisitsPSPSC_March10_2017_youtube_1080.mp4 (1920x1080) [1.0 GB] || NASA_TV_EugeneParkerVisitsPSPSC_March10_2017.mpeg (1280x720) [2.1 GB] || EugeneParkerVisitsPSPSC_March10_2017_appletv.m4v (1280x720) [327.6 MB] || EugeneParkerVisitsPSPSC_March10_2017_large.mp4 (1920x1080) [632.9 MB] || EugeneParkerVisitsPSPSC_March10_2017_large.webm (1920x1080) [69.5 MB] || NASA_PODCAST_EugeneParkerVisitsPSPSC_March10_2017_ipod_sm.mp4 (320x240) [112.3 MB] || ", "hits": 91 }, { "id": 12946, "url": "https://svs.gsfc.nasa.gov/12946/", "result_type": "Produced Video", "release_date": "2018-05-08T12:00:00-04:00", "title": "Solar Power: Parker Solar Probe Tests Its Arrays", "description": "NASA’s Parker Solar Probe gets its power from the Sun, so the solar arrays that collect energy from our star need to be in perfect working order. This month, members of the mission team tested of the arrays at Astrotech Space Operations in Titusville, Florida, to ensure the system performs as designed and provides power to the spacecraft during its historic mission to the Sun.Parker Solar Probe is powered by two solar arrays, totaling just under 17 square feet (1.55 square meters) in area. They are mounted to motorized arms that will retract almost all of their surface behind the Thermal Protection System – the heat shield – when the spacecraft is close to the Sun. || ", "hits": 48 }, { "id": 12917, "url": "https://svs.gsfc.nasa.gov/12917/", "result_type": "Produced Video", "release_date": "2018-04-13T19:00:00-04:00", "title": "Parker Solar Probe Travels to Florida", "description": "Parker Solar Probe Arrives in FloridaOn April 4, 2018, Parker Solar Probe project scientist Nicky Fox of Johns Hopkins APL describes the spacecraft's April 3 journey to Florida and arrival at Astrotech Space Operations, the probe's new home before a scheduled launch on July 31, 2018 from NASA's Kennedy Space Center. Credit: NASA/Johns Hopkins APL/Lee HobsonWatch this video on the Johns Hopkins APL YouTube channel. || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_print.jpg (1024x576) [103.8 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_thm.png (80x40) [7.1 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_web.png (320x180) [85.2 KB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.00033_searchweb.png (320x180) [85.2 KB] || PRORES_B-ROLL_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_prores.mov (1280x720) [642.5 MB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_appletv_subtitles.m4v (1280x720) [48.0 MB] || NASA_TV_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD.mpeg (1280x720) [309.1 MB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_appletv.m4v (1280x720) [48.0 MB] || YOUTUBE_1080_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_youtube_1080.mp4 (1920x1080) [146.4 MB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.mp4 (3840x2160) [97.6 MB] || Nicky_Fox_Welcomes_PSP_To_ASO_UHD.mp4 (3840x2160) [502.0 MB] || YOUTUBE_4K_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_youtube_4k.mp4 (3840x2160) [373.1 MB] || LARGE_MP4_12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_large.webm (3840x2160) [12.3 MB] || 12917_Parker_Solar_Probe_Arrives_in_Florida.en_US.srt [1.3 KB] || 12917_Parker_Solar_Probe_Arrives_in_Florida.en_US.vtt [1.3 KB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_Prores.mov (3840x2160) [4.9 GB] || 12917_Nicky_Fox_Welcomes_PSP_To_ASO_UHD_ipod_sm.mp4 (320x240) [15.8 MB] || ", "hits": 167 }, { "id": 12890, "url": "https://svs.gsfc.nasa.gov/12890/", "result_type": "Produced Video", "release_date": "2018-03-09T10:00:00-05:00", "title": "Solar Highlights of 2018", "description": "3 NASA Satellite Recreate Solar Eruption in 3-DUsing data from three different satellites, scientists have developed new models that recreate, in 3-D, CMEs and shocks, separately. This movie illustrates the recreation of a CME and shock that erupted from the Sun on March 7, 2011. The pink lines show the CME structure and the yellow lines show the structure of the shock - a side effect of the CME that can spark space weather events around Earth.Scientists: Ryun Kwon (George Mason University), Angelos Vourlidas (The Johns Hopkins University Applied Physics Laboratory)Image credits: NASA’s Goddard Space Flight Center/GMU/APL/Joy NgWatch this video on the NASA.gov Video YouTube channel.Find this feature on NASA.gov. || 3DCME.00001_print.jpg (1024x576) [77.7 KB] || 3DCME.00001_searchweb.png (320x180) [52.1 KB] || 3DCME.00001_web.png (320x180) [52.1 KB] || 3DCME.00001_thm.png (80x40) [5.3 KB] || PRORES_B-ROLL_12890_3DCME_prores.mov (1280x720) [218.7 MB] || 3DCME_Prores.mov (1920x1080) [416.9 MB] || 3DCME.mp4 (1920x1080) [44.6 MB] || 12890_3DCME_appletv.m4v (1280x720) [24.5 MB] || NASA_TV_12890_3DCME.mpeg (1280x720) [102.5 MB] || LARGE_MP4_12890_3DCME_large.mp4 (1920x1080) [31.2 MB] || 3DCME.webm (1920x1080) [3.1 MB] || GSFC_20180309_CME_m12890_3DCME.en_US.vtt [64 bytes] || 12890_3DCME_ipod_sm.mp4 (320x240) [7.2 MB] || ", "hits": 60 }, { "id": 12861, "url": "https://svs.gsfc.nasa.gov/12861/", "result_type": "Produced Video", "release_date": "2018-02-14T09:00:00-05:00", "title": "NASA Valentines", "description": "Download our collection of valentines, featuring science visualizations and imagery from NASA missions.Want more NASA valentines? Visit https://mars.nasa.gov/free-holiday-ecard/love-valentine/#Send-A-Card ||", "hits": 95 }, { "id": 12841, "url": "https://svs.gsfc.nasa.gov/12841/", "result_type": "Produced Video", "release_date": "2018-01-30T15:00:00-05:00", "title": "Parker Solar Probe: Solar60 Series", "description": "Parker Solar Probe Enters Thermal Vacuum ChamberNASA's Parker Solar Probe Deputy Lead Mechanical Engineer Felipe Ruiz and Lead Thermal Engineer Jack Ercol - both from Johns Hopkins Applied Physics Lab - take us through the process of preparing the spacecraft for space environment testing. The Thermal Protection System (TPS) simulator placed on the spacecraft is to provide accurate simulation conditions during testing. Learn more here. Credit: NASA/Johns Hopkins APL/Lee HobsonWatch this video on the Johns Hopkins APL YouTube channel. || 1800101Solar6001PSPTVacV31080p.00037_print.jpg (1024x576) [194.3 KB] || 1800101Solar6001PSPTVacV31080p.00037_searchweb.png (320x180) [112.2 KB] || 1800101Solar6001PSPTVacV31080p.00037_web.png (320x180) [112.2 KB] || 1800101Solar6001PSPTVacV31080p.00037_thm.png (80x40) [7.6 KB] || 1800101Solar6001PSPTVacV31080p.mp4 (1920x1080) [189.9 MB] || 1800101Solar6001PSPTVacV31080p.webm (1920x1080) [12.1 MB] || Solar60_1captions.en_US.srt [1.7 KB] || Solar60_1captions.en_US.vtt [1.7 KB] || ", "hits": 24 }, { "id": 12813, "url": "https://svs.gsfc.nasa.gov/12813/", "result_type": "Produced Video", "release_date": "2017-12-19T11:00:00-05:00", "title": "Moving Day: Parker Solar Probe Travels from APL to NASA Goddard", "description": "Complete transcript available.Watch this video on YouTubeMusic credits: A Fresh Perspective, Album_Track: MX242_21, Composer: Christopher E. Hajian (ASCAP), Publisher: JRM Music (ASCAP)Performance Power, Album_Track: TS105_21, Composer: Edmund J King (ASCAP), Publisher:Saticoy Music (ASCAP) || 17-04038_PSP_Moving_Day_v15.00139_print.jpg (1024x576) [118.4 KB] || 17-04038_PSP_Moving_Day_v15.00139_searchweb.png (320x180) [80.0 KB] || 17-04038_PSP_Moving_Day_v15.00139_thm.png (80x40) [5.9 KB] || 17-04038_PSP_Moving_Day_v15.mp4 (1920x1080) [218.0 MB] || 17-04038_PSP_Moving_Day_v15.webm (1920x1080) [25.1 MB] || captions.en_US.srt [4.8 KB] || captions.en_US.vtt [4.9 KB] || ", "hits": 17 }, { "id": 12795, "url": "https://svs.gsfc.nasa.gov/12795/", "result_type": "Produced Video", "release_date": "2017-12-06T11:00:00-05:00", "title": "Parker Solar Probe: Environmental Testing", "description": "NASA’s Parker Solar Probe passed laser illumination testing the week of Nov. 27, 2017. During this test, each segment of the spacecraft’s solar panels was illuminated with lasers to check that they were still electrically connected after the vigorous vibration and acoustic testing completed earlier this fall. NASA’s Parker Solar Probe is in the midst of intense environmental testing at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, in preparation for its journey to the Sun. These tests have simulated the noise and shaking the spacecraft will experience during its launch from Cape Canaveral, Florida, scheduled for July 31, 2018.Parker Solar Probe’s integration and testing team must check over the spacecraft and systems to make sure everything is still in optimal working condition after experiencing these rigorous conditions – including a check of the solar arrays, which will provide electrical power to the spacecraft.Parker Solar Probe will explore the Sun's outer atmosphere and make critical observations that will answer decades-old questions about the physics of stars. The resulting data will also help improve how we forecast major eruptions on the Sun and subsequent space weather events that can impact life on Earth, as well as satellites and astronauts in space. The mission is named for Eugene N. Parker, whose profound insights into solar physics and processes have helped shape the field of heliophysics.Link to Parker Solar Probe blog post. || ", "hits": 141 }, { "id": 12717, "url": "https://svs.gsfc.nasa.gov/12717/", "result_type": "Produced Video", "release_date": "2017-10-02T12:00:00-04:00", "title": "Touching the Sun", "description": "Parker Solar Probe will observe the sun from a closer vantage point than ever before. || ObservingSunPoster_16x9_1024x576.jpg (1024x576) [444.2 KB] || ObservingSunPoster_16x9.jpg (2850x1603) [2.4 MB] || ObservingSunPoster_16x9_searchweb.png (320x180) [88.1 KB] || ObservingSunPoster_16x9_thm.png (80x40) [6.0 KB] || ", "hits": 39 }, { "id": 12729, "url": "https://svs.gsfc.nasa.gov/12729/", "result_type": "Produced Video", "release_date": "2017-09-22T19:00:00-04:00", "title": "Parker Solar Probe Animations", "description": "Animated Sequence Of Parker Solar ProbeCredit: NASA/JHUAPL || ParkerSolarProbe-AnimatedSequence.00001_print.jpg (1024x576) [41.9 KB] || ParkerSolarProbe-AnimatedSequence.00001_searchweb.png (180x320) [37.2 KB] || ParkerSolarProbe-AnimatedSequence.00001_web.png (320x180) [37.2 KB] || ParkerSolarProbe-AnimatedSequence.00001_thm.png (80x40) [3.2 KB] || ParkerAnimatedSeq.mov (1920x1080) [2.9 GB] || ParkerAnimatedSeq.mp4 (1920x1080) [343.1 MB] || ParkerAnimatedSeq.webm (1920x1080) [21.1 MB] || ", "hits": 267 }, { "id": 12726, "url": "https://svs.gsfc.nasa.gov/12726/", "result_type": "Produced Video", "release_date": "2017-09-22T18:00:00-04:00", "title": "Parker Solar Probe: Testing and Integration", "description": "Main flight harness installation.Credit: NASA/JHUAPL || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_print.jpg (1024x576) [120.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_searchweb.png (320x180) [75.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_web.png (320x180) [75.4 KB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.00021_thm.png (80x40) [5.6 KB] || 12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_prores.mov (1920x1080) [2.9 GB] || PRORES_B-ROLL-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_prores.mov (1280x720) [1.5 GB] || YOUTUBE_1080-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_youtube_1080.mp4 (1920x1080) [373.7 MB] || APPLE_TV-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_appletv.m4v (1280x720) [117.9 MB] || NASA_TV-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072.mpeg (1280x720) [697.9 MB] || LARGE_MP4-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_large.mp4 (1920x1080) [209.3 MB] || 17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_1080p.mp4 (1920x1080) [408.5 MB] || LARGE_MP4-12726_ParkerSolarProbe_blanketing_17-08-01-08_SPP_Timelapse_17-00_large.webm (1280x720) [15.6 MB] || NASA_PODCAST-12726_ParkerSolarProbe_17-04-05_Top_Deck_SACS_Installation_Dolbow_Ruiz_17-00072_ipod_sm.mp4 (320x240) [38.5 MB] || ", "hits": 128 }, { "id": 12728, "url": "https://svs.gsfc.nasa.gov/12728/", "result_type": "Produced Video", "release_date": "2017-09-22T17:00:00-04:00", "title": "What is Parker Solar Probe?", "description": "Parker Solar Probe will swoop to within four million miles of the Sun's surface, facing heat and radiation like no spacecraft before it. Launching in 2018, Parker Solar Probe will provide new data on solar activity and make critical contributions to our ability to forecast major space-weather events that impact life on Earth.Parker Solar Probe is an extraordinary and historic mission exploring arguably the last and most important region of the solar system to be visited by a spacecraft to finally answer top-priority science goals for over five decades.But we don't do this just for the basic science.One recent study by the National Academy of Sciences estimated that without advance warning a huge solar event could cause two trillion dollars in damage in the U.S. alone, and the eastern seaboard of the U.S. could be without power for a year.In order to unlock the mysteries of the corona, but also to protect a society that is increasingly dependent on technology from the threats of space weather, we will send Parker Solar Probe to touch the Sun. || ", "hits": 158 }, { "id": 12414, "url": "https://svs.gsfc.nasa.gov/12414/", "result_type": "Produced Video", "release_date": "2016-12-14T17:30:00-05:00", "title": "AGU 2017 Eclipse Press Conference", "description": "Graphic depicting the geometry of a total solar eclipse. Credit: NASA || Eclipse_Geometry.png (1158x548) [180.5 KB] || ", "hits": 20 }, { "id": 12410, "url": "https://svs.gsfc.nasa.gov/12410/", "result_type": "Produced Video", "release_date": "2016-11-07T13:45:00-05:00", "title": "Small Satellites for Earth Science", "description": "NASA has embraced the revolution in small spacecraft and satellites, from CubeSats you can hold in your hand to microsatellites the size of a small washing machine. The technology helps advance scientific and human exploration, reduces the cost of new missions, and expands access to space. The briefing will discuss NASA's overall program, technology development initiatives, and new Earth-observing missions that use individual and constellations of small satellites to study climate change, hurricanes and clouds.Briefing PanelistsEllen Stofan, chief scientists at NASA Headquarters in WashingtonThomas Zurbuchen, associate administrator for the Science Mission Directorate at NASA HeadquartersSteve Jurczyk, associate administrator for the Science Mission Directorate at NASA HeadquartersMichael Freilich, director of the Earth Science Division at NASA HeadquartersAaron Ridley, mission constellation scientist for NASA's Cyclone Global Navigation Satellite System (CYGNSS) at the University of Michigan in Ann ArborBill Swartz, CubeSat principal investigator for the Radiometer Assessment using Vertically Aligned Nanotubes (RAVAN) project at Johns Hopkins University Applied Physics Laboratory in Laurel, MarylandWilliam Blackwell, principal investigator for the Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsat (TROPICS) mission at the Massachusetts Institute of Technology Lincoln Laboratory, Lexington, Mass.More information is available. || ", "hits": 21 }, { "id": 12328, "url": "https://svs.gsfc.nasa.gov/12328/", "result_type": "Produced Video", "release_date": "2016-08-15T10:00:00-04:00", "title": "Supercharging the Radiation Belts", "description": "On March 17, 2015, an interplanetary shock – a shockwave created by the driving force of a coronal mass ejection, or CME, from the sun – struck the outermost radiation belt, triggering the greatest geomagnetic storm of the preceding decade. And NASA's Van Allen Probes were there to watch it. One of the most common forms of space weather, a geomagnetic storm describes any event in which Earth’s magnetic environment – called the magnetosphere – is suddenly, temporarily disturbed. Such an event can also lead to change in the radiation belts surrounding Earth, but researchers have seldom been able to observe what happens within the first few minutes immediately following a shock. But on the day of the March 2015 geomagnetic storm, one of the Van Allen Probes was located at just the right spot within the radiation belts, providing unprecedentedly high-resolution data from a rarely witnessed phenomenon. A paper on these observations was published in the Journal of Geophysical Research on Aug. 15, 2016. || ", "hits": 158 }, { "id": 11954, "url": "https://svs.gsfc.nasa.gov/11954/", "result_type": "Produced Video", "release_date": "2015-07-15T13:00:00-04:00", "title": "NASA’s Evolving Views of Pluto", "description": "NASA's New Horizons spacecraft flew within 8,000 miles of dwarf planet Pluto on July 14, 2015. Our view of this cold, previously unexplored world, 4.67 billion miles from Earth, has evolved since its discovery by Clyde W. Tombaugh in 1930. These short clips and images are from Tombaugh, Hubble and New Horizons over the years, arranged to illustrate improvements in resolution. || ", "hits": 366 }, { "id": 11833, "url": "https://svs.gsfc.nasa.gov/11833/", "result_type": "Produced Video", "release_date": "2015-04-07T11:30:00-04:00", "title": "Portrait Of An Asteroid", "description": "Scientists use lasers to create a 3-D model of asteroid Eros. || c-1280.jpg (1280x720) [118.7 KB] || c-1024.jpg (1024x576) [82.2 KB] || c-1024_print.jpg (1024x576) [77.5 KB] || c-1024_searchweb.png (320x180) [40.5 KB] || c-1024_print_thm.png (80x40) [10.2 KB] || ", "hits": 34 }, { "id": 11754, "url": "https://svs.gsfc.nasa.gov/11754/", "result_type": "Produced Video", "release_date": "2015-03-12T11:00:00-04:00", "title": "Epic Descents", "description": "A brief history of asteroid and comet landings. || cf-1280.jpg (1280x720) [136.4 KB] || cf-1024.jpg (1024x576) [104.0 KB] || cf-1920.jpg (1920x1080) [220.2 KB] || cf-1024_print.jpg (1024x576) [103.8 KB] || cf-1024_searchweb.png (320x180) [48.9 KB] || cf-1024_print_thm.png (80x40) [19.0 KB] || ", "hits": 31 }, { "id": 11212, "url": "https://svs.gsfc.nasa.gov/11212/", "result_type": "Produced Video", "release_date": "2013-02-28T14:00:00-05:00", "title": "Van Allen Probes Find Storage Ring in Earth's Outer Radiation Belt", "description": "Since their discovery over 50 years ago, the Earth's Van Allen radiation belts have been considered to consist of two distinct zones of trapped, highly energetic charged particles. Observations from NASA's Van Allen Probes reveal an isolated third ring in the outer radiation belt. || ", "hits": 681 }, { "id": 11027, "url": "https://svs.gsfc.nasa.gov/11027/", "result_type": "Produced Video", "release_date": "2012-08-09T14:00:00-04:00", "title": "RBSP L-14 Press Conference", "description": "The Radiation Belt Storm Probes mission is part of NASA's Living With a Star Geospace program to explore fundamental processes that operate throughout the solar system, in particular those that generate hazardous space weather effects near the Earth and phenomena that could affect solar system exploration.RBSP is designed to help us understand the sun's influence on the Earth and near-Earth space by studying the planet's radiation belts on various scales of space and time.Understanding the radiation belt environment and its variability has extremely important practical applications in the areas of spacecraft operations, spacecraft and spacecraft system design, mission planning, and astronaut safety.RBSP is scheduled to launch no earlier than 4:08 a.m. Thursday, Aug. 23 from Cape Canaveral Air Force Station in Florida. The twin probes will lift off on a United Launch Alliance Atlas V rocket.News conference panelists are:— Madhulika Guhathakurta, Living With a Star program scientist, NASA Headquarters, Washington— Mona Kessel, RBSP program scientist, NASA Headquarters— Barry Mauk, RBSP project scientist, Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md.— Rick Fitzgerald, RBSP project manager, APL, Laurel, Md. || ", "hits": 56 }, { "id": 10788, "url": "https://svs.gsfc.nasa.gov/10788/", "result_type": "Produced Video", "release_date": "2011-08-30T00:00:00-04:00", "title": "Why Auroras Erupt", "description": "Why does the aurora borealis—the typically steady green bands of light common in the nighttime sky over the Arctic—occasionally erupt in bouts of activity that leave the sky shimmering with a full palette of reds, whites and purples? Scientists have long known that disturbances in Earth's magnetic field driven by the solar wind can trigger such auroral eruptions, but it hasn't been clear whether the disturbances originate near the Earth or at more distant points closer to the moon. In recent years, a series of five satellites and a network of ground-based instruments in the Arctic have finally helped provide an answer. Hermetically-sealed cameras, called All Sky Imagers, placed strategically throughout the American and Canadian Arctic, look upward to observe nearly the entire arc of the sky where auroras occur. The ground network, considered the sixth \"satellite\" of NASA's aurora-monitoring THEMIS mission, takes auroral snapshots each three-seconds all night long, every night. In 2008, it helped make a breakthrough discovery: the magnetic disturbances that cause auroras to erupt begin about a third of the way to the moon when stressed magnetic lines reconnect and send massive bursts of energy toward Earth. The visualization below shows the first major aurora eruption that the imagers observed. || ", "hits": 39 }, { "id": 3590, "url": "https://svs.gsfc.nasa.gov/3590/", "result_type": "Visualization", "release_date": "2009-07-07T00:00:00-04:00", "title": "THEMIS/ASI Nights - High Resolution", "description": "A collection of ground-based All-Sky Imagers (ASI) makes an important component of the THEMIS mission in understanding the interaction of the magnetosphere and aurora. It is sometimes referred to as the sixth THEMIS satellite. Descriptions of the instruments are available on the THEMIS-Canada Home Page. Imagery from each camera is co-registered to the surface of the Earth and assembled into a view of the auroral events. This movie presents data from the first large auroral substorm since the THEMIS launch. The substorm reached its maximum between 6:00 and 7:00 UT. Note that the ASI data in this movie are assembled from significantly higher resolution datesets than the earlier version, THEMIS/ASI Nights. The higher resolution enables you to see much finer details in the aurora structure. In addition, one notices trees circling the horizon visible to the cameras located in western Canada. || ", "hits": 145 }, { "id": 3512, "url": "https://svs.gsfc.nasa.gov/3512/", "result_type": "Visualization", "release_date": "2008-07-23T00:00:00-04:00", "title": "THEMIS/ASI Nights", "description": "A collection of ground-based All-Sky Imagers (ASI) make up another important component of the THEMIS mission. It is sometimes referred to as the sixth THEMIS satellite. Descriptions of the instruments are available on the THEMIS-Canada Home Page. Imagery from each camera is co-registered to the surface of the Earth and assembled into a view of the auroral events. This movie presents data from the first large auroral substorm since the THEMIS launch. The substorm reached its maximum between 6:00 and 7:00 UT. Note that the ASI data in this movie are assembled from the lower resolution quick-look data sets. These create some extra pixellation of the data in the static high-resolution views. This animation has been superceded by ID 3590: THEMIS/ASI Nights-High Resolution, which uses higher-resolution ASI data. || ", "hits": 36 }, { "id": 3513, "url": "https://svs.gsfc.nasa.gov/3513/", "result_type": "Visualization", "release_date": "2008-07-23T00:00:00-04:00", "title": "Auroral Substorm from Polar", "description": "This movie is an auroral substorm event observed by the visible light camera aboard the Polar spacecraft. Because the visible light camera records in a single broad range of wavelengths, we do not have color imagery of the event. For this movie we will color the aurora green since that is the dominant color in most cases. The VIS camera is also low resolution so the fine aurora details visible from the ground are not apparent in this movie. || ", "hits": 44 }, { "id": 20101, "url": "https://svs.gsfc.nasa.gov/20101/", "result_type": "Animation", "release_date": "2007-04-06T00:00:00-04:00", "title": "Magnetic Reconnection 2", "description": "This is an update to an older magnetic reconnection animation (10072). The ionized wind from the Sun generates reconnection in the Earth's magnetic field. Particles leak in from the rediation belts producing the auroras. || ", "hits": 133 }, { "id": 20028, "url": "https://svs.gsfc.nasa.gov/20028/", "result_type": "Animation", "release_date": "2004-06-21T12:00:00-04:00", "title": "Cold Water Upwelling Promotes Phytoplankton Blooms", "description": "Carbon is the root of all life on Earth, and as it circulates through our biosphere, the Earth's state of health responds. Whenever the size of phytoplankton colonies in the ocean changes, it affects the amount of carbon absorbed from the atmosphere. These blooms are highly dependent on surrounding environmental conditions. As a hurricane passes over the tropical waters of the Atlantic, it draws up cold water from deep below the warmer surface. As the cooler water rises, it brings with it phytoplankton and nutrients necessary for life. These microscopic plants then bloom in higher than average amounts. Bigger storms cause larger plankton blooms and more plankton absorb a greater amount of carbon from our atmosphere. Scientists are still trying to determine how much carbon dioxide might be removed by such a process. || ", "hits": 58 }, { "id": 2857, "url": "https://svs.gsfc.nasa.gov/2857/", "result_type": "Visualization", "release_date": "2003-11-21T12:00:00-05:00", "title": "Geomagnetic Storm: November 2003", "description": "Coronal Mass Ejections from sunspot 10484 sweep by the Earth on November 20, 2003, generating aurora displays worldwide. This view is from the Polar spacecraft with a false-color data overlaid on the Earth's surface. Red marks the highest intensity, blue the lowest. || ", "hits": 33 }, { "id": 20073, "url": "https://svs.gsfc.nasa.gov/20073/", "result_type": "Animation", "release_date": "2003-03-26T12:00:00-05:00", "title": "Auroral Elements", "description": "Electrons rain down from the Earth's radiation belts, exciting atoms into radiative states along the way. || Electrons collide with atoms sending them into radiative states. || lfta3_pre.00627_print.jpg (1024x698) [35.3 KB] || lfta3_thm.png (80x40) [1.0 KB] || lfta3_pre.jpg (320x218) [2.3 KB] || lfta3_pre_searchweb.jpg (320x180) [7.5 KB] || lfta3.webmhd.webm (960x540) [1.8 MB] || lfta3.mpg (352x240) [7.3 MB] || ", "hits": 12 }, { "id": 20074, "url": "https://svs.gsfc.nasa.gov/20074/", "result_type": "Animation", "release_date": "2003-03-26T12:00:00-05:00", "title": "Ride the Electron", "description": "Electrons travel along the Earth's magnetic field lines, occasionally making it to the Earth's atmosphere. This animation is part of a larger animation. || Electrons travel along the magnetic field lines to the Earth's atmosphere. || magride_pre.00002_print.jpg (1024x698) [85.2 KB] || magride_thm.png (80x40) [6.2 KB] || magride_pre.jpg (320x218) [10.2 KB] || magride_pre_searchweb.jpg (320x180) [73.8 KB] || magride.webmhd.webm (960x540) [4.1 MB] || magride.mpg (352x240) [4.1 MB] || ", "hits": 9 }, { "id": 2444, "url": "https://svs.gsfc.nasa.gov/2444/", "result_type": "Visualization", "release_date": "2002-05-09T12:00:00-04:00", "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Rainbow Version)", "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a rainbow color table for oxygen intensity. || a002444.00100_print.png (720x480) [373.3 KB] || HENArainbow_pre.jpg (320x288) [13.5 KB] || a002444.webmhd.webm (960x540) [8.1 MB] || a002444.dv (720x480) [112.3 MB] || HENArainbow.mpg (320x288) [942.9 KB] || ", "hits": 22 }, { "id": 2445, "url": "https://svs.gsfc.nasa.gov/2445/", "result_type": "Visualization", "release_date": "2002-05-09T12:00:00-04:00", "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Blue Version)", "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a blue color table for oxygen intensity. || a002445.00010_print.png (720x480) [371.4 KB] || HENAblue_pre.jpg (320x320) [7.9 KB] || a002445.webmhd.webm (960x540) [8.1 MB] || a002445.dv (720x480) [153.6 MB] || HENAblue.mpg (320x320) [1.3 MB] || ", "hits": 15 } ] }