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            "id": 31384,
            "url": "https://svs.gsfc.nasa.gov/31384/",
            "result_type": "Hyperwall Visual",
            "release_date": "2026-04-01T12:00:00-04:00",
            "title": "Gigantic Jet Seen from the ISS",
            "description": "A Gigantic Jet event was photographed by NASA astronaut Nichole Ayers from aboard the International Space Station",
            "hits": 203
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        {
            "id": 14986,
            "url": "https://svs.gsfc.nasa.gov/14986/",
            "result_type": "Produced Video",
            "release_date": "2026-03-20T00:00:00-04:00",
            "title": "See How NASA’s GUARDIAN Tsunami Detection System Works",
            "description": "Complete transcript available.Universal Music Production: “Something’s Afoot Instrumental” || thumbnail_horizontal.jpg (3840x2160) [4.0 MB] || thumbnail_horizontal_print.jpg (1024x576) [472.5 KB] || thumbnail_horizontal_searchweb.png (320x180) [108.0 KB] || thumbnail_horizontal_web.png (320x180) [108.0 KB] || thumbnail_horizontal_thm.png (80x40) [7.2 KB] || 03132026_Guardian_Full_Final.webm (3840x2160) [26.1 MB] || 03132026_Guardian_Full_Final.mp4 (3840x2160) [463.8 MB] || ",
            "hits": 159
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        {
            "id": 31347,
            "url": "https://svs.gsfc.nasa.gov/31347/",
            "result_type": "Hyperwall Visual",
            "release_date": "2026-03-03T18:59:59-05:00",
            "title": "Astronaut Don Pettit’s Photos from Space",
            "description": "hyperwall hwshows for photos from https://www.nasa.gov/gallery/astronaut-don-pettits-photos-from-space/",
            "hits": 597
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        {
            "id": 20411,
            "url": "https://svs.gsfc.nasa.gov/20411/",
            "result_type": "Animation",
            "release_date": "2026-01-14T10:00:00-05:00",
            "title": "A Pathway to Protocells on Titan – Animations",
            "description": "These animations illustrate how simple protocells could form in the lakes of Titan, Saturn’s largest moon. When rain falls from Titan’s methane clouds into its hydrocarbon lakes, it can transport organic molecules like acrylonitrile that are attracted to both water and oil. Such amphiphile molecules are likely to collect in a thin film on the surface of Titan’s lakes. As large raindrops pelt the lakes, they could stir up this floating “pond scum” to form spherical droplets of methane coated in a bilayer of amphiphiles – structures called vesicles that resemble cell membranes on Earth.Although such vesicles have yet to be detected on Titan, a 2025 study by Christian Mayer and NASA scientist Conor Nixon lays out the process for their formation and evolution, and it proposes a mechanism for their discovery by a future mission to Titan. The paper also proposes that different mixtures of amphiphiles could stabilize vesicles and lead to the evolution of simple protocells on Titan. || ",
            "hits": 200
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            "id": 14666,
            "url": "https://svs.gsfc.nasa.gov/14666/",
            "result_type": "Produced Video",
            "release_date": "2025-11-13T12:00:00-05:00",
            "title": "ESCAPADE Launch Phase and Deployment Animations",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE mission will be carried into orbit on the second launch of Blue Origin’s New Glenn rocket. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 96
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        {
            "id": 14920,
            "url": "https://svs.gsfc.nasa.gov/14920/",
            "result_type": "Produced Video",
            "release_date": "2025-11-13T12:00:00-05:00",
            "title": "Preparing for Martian Explorers: NASA's ESCAPADE Investigates Mars Space Weather",
            "description": "NASA’s new ESCAPADE mission is launching to Mars to help us better understand the Sun’s influence on Mars’ past and present. Its work could help protect future human explorers from potentially dangerous space weather when they set foot on the Red Planet.For the first time, the mission will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. Its observations will reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE orbiters build on earlier Mars missions, such as NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) orbiter. The MAVEN mission has one spacecraft that has been studying Mars’ atmospheric loss since arriving at the Red Planet in 2014.ESCAPADE is scheduled to launch no earlier than fall 2025 from Cape Canaveral Space Force Station Launch Complex 36 in Florida.Find out more about the ESCAPADE mission: https://science.nasa.gov/mission/escapade/ || ",
            "hits": 76
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        {
            "id": 14915,
            "url": "https://svs.gsfc.nasa.gov/14915/",
            "result_type": "Produced Video",
            "release_date": "2025-11-13T00:00:00-05:00",
            "title": "ESCAPADE Trajectory Animations",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, mission will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE mission is being carried into orbit on the second launch of Blue Origin’s New Glenn rocket (NG-2) and is scheduled to launch in November 2025 from Cape Canaveral, Florida. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin.Below are animations demonstrating the different phases of the mission's trajectory from traveling from Earth to Mars to implementing its science orbits around the Red Planet. || ",
            "hits": 290
        },
        {
            "id": 14918,
            "url": "https://svs.gsfc.nasa.gov/14918/",
            "result_type": "Produced Video",
            "release_date": "2025-11-11T00:00:00-05:00",
            "title": "ESCAPADE Prepares for Flight (2025)",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.The ESCAPADE mission is being carried into orbit on the second launch of Blue Origin’s New Glenn rocket (NG-2) and is scheduled to launch in November 2025 from Cape Canaveral, Florida. New Glenn is a single-configuration, heavy-lift orbital launch vehicle capable of routinely carrying both spacecraft and people to low Earth orbits, geostationary transfer orbits, cislunar orbits (between Earth and the Moon), and beyond via Earth-departure orbits like the one required for ESCAPADE. The vehicle is named after John Glenn, the first American astronaut to orbit Earth.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 106
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            "id": 14863,
            "url": "https://svs.gsfc.nasa.gov/14863/",
            "result_type": "Produced Video",
            "release_date": "2025-07-17T09:00:00-04:00",
            "title": "Quickshot: New NASA Mission Launching Soon To Study Earth’s Space Weather Shield",
            "description": "Scroll down page for advisory with suggested questions and anchor intro. You will also find the associated cut b-roll and pre-recorded soundbites below.Click here for more information about TRACERS || Live_Shot_Banner_TRACERS_final.jpg (1800x720) [256.8 KB] || Live_Shot_Banner_TRACERS_final_print.jpg (1024x409) [150.1 KB] || Live_Shot_Banner_TRACERS_final_searchweb.png (320x180) [82.8 KB] || Live_Shot_Banner_TRACERS_final_thm.png (80x40) [6.5 KB] || ",
            "hits": 81
        },
        {
            "id": 20405,
            "url": "https://svs.gsfc.nasa.gov/20405/",
            "result_type": "Animation",
            "release_date": "2025-07-08T16:00:00-04:00",
            "title": "Carruthers Atmospheric Layers Animation",
            "description": "Earth’s atmosphere is divided into five main layers, differentiated by factors such as temperature, chemical composition, and air density. The troposphere is the lowest layer, extending from Earth's surface up to about 10 miles above it, and is where almost all weather phenomena occur. Above the troposphere is the stratosphere, which reaches up to around 31 miles. It contains the ozone layer, which absorbs harmful ultraviolet (UV) radiation from the Sun. Next is the mesosphere, which extends from about 31 to 53 miles above Earth. It is the coldest layer of the atmosphere, and it is where most meteors burn up upon entering. Above the mesosphere is the thermosphere, ranging from about 53 to 375 miles above Earth. Known as the upper atmosphere, this region contains the ionosphere, a region filled with charged particles that enable radio communications and where auroras often occur. The outermost layer is the exosphere, which gradually transitions into outer space. It is extremely thin and composed mainly of hydrogen and helium. Together, these layers form a protective shield that regulates Earth’s energy balance and helps sustain life. || ",
            "hits": 834
        },
        {
            "id": 5419,
            "url": "https://svs.gsfc.nasa.gov/5419/",
            "result_type": "Visualization",
            "release_date": "2025-06-09T00:00:00-04:00",
            "title": "The Carruthers Geocorona Observatory at the Earth-Sun Lagrange Point 1",
            "description": "The Carruthers Geocorona Obervatory observes Earth's exosphere, or geocorona, from the Earth-Sun Lagrange Point 1.",
            "hits": 103
        },
        {
            "id": 14846,
            "url": "https://svs.gsfc.nasa.gov/14846/",
            "result_type": "Produced Video",
            "release_date": "2025-05-29T11:00:00-04:00",
            "title": "Is This How Mars Lost Its Atmosphere?",
            "description": "Mars is losing its atmosphere. Over billions of years, the Red Planet has transformed from a potentially habitable world with lakes, rivers, and a thicker atmosphere into the cold, dry desert we see today. NASA’s MAVEN mission has been tracking this process in real time, catching Mars in the act of slowly sputtering its atmosphere into space.This phenomenon—called “atmospheric sputtering”—happens when high-energy particles from the Sun slam into Mars’s upper atmosphere, knocking atoms and molecules loose. Without a global magnetic field to protect it, Mars is especially vulnerable. MAVEN has shown that this atmospheric escape accelerates during solar storms, offering a powerful view of how the Sun shapes the evolution of planetary atmospheres.The data from MAVEN doesn’t just tell us about Mars—it helps us understand how atmospheres behave across the solar system and beyond. It’s a glimpse into what makes a planet stay habitable—or lose that potential entirely.For more information, visit https://science.nasa.gov/mission/maven/Credit: NASA's Goddard Space Flight Center Dan Gallagher: Lead ProducerPaul Morris: Producer / EditorDr. Shannon Curry: Scientist / IntervieweeWillow Reed: Public AffairsNancy Jones: Public AffairsGreg Shirah: Data VisualizerCindy Starr: Data VisualizerKel Elkins: Data VisualizerWalt Feimer: AnimatorMichael Lentz: AnimatorChris Smith: AnimatorJonathan North: AnimatorBrian Monroe: AnimatorLisa Poje: Graphic DesignerAdriana Manrique Gutierrez: Graphic DesignerKim Dongjae: Graphic DesignerErnie Wright: SupportAaron E. Lepsch: Technical SupportMusic Credit:\"The Greatest Unknown\" by Samuel Sim [PRS] via Abbey Road Masters [PRS] and Universal Production MusicVideo Credits:Periodic Table Focusing On Argon With Properties by S_D_Brath via Pond5Ashes Of A Camp Fire Next To Chair by BlackBoxGuild via Pond5Wood Burning In A Camp Fire by Edb3_16 via Pond5 || ",
            "hits": 428
        },
        {
            "id": 14840,
            "url": "https://svs.gsfc.nasa.gov/14840/",
            "result_type": "Produced Video",
            "release_date": "2025-05-20T09:00:00-04:00",
            "title": "Why Is Neptune Glowing Like This?",
            "description": "Neptune is glowing—and it’s not what we expected.NASA’s James Webb Space Telescope just spotted auroras stretching across Neptune’s mid-latitudes—not the poles. Why?The planet’s bizarre magnetic field and a shockingly cold upper atmosphere may hold the answer. These new findings are rewriting what we know about the solar system’s most distant planet.Watch to see how Webb is revealing Neptune in a whole new light.For more information, visit https://nasa.gov/webbCredit:Producer: Paul MorrisWriter: Thaddeus CesariNarrator: Dr. Quyen HartImages: NASA, ESA, CSA, STSciMusic Credit:\"Float On\" by Layla Pavey [PRS] and Samuel John Chase [PRS] via Zone Music Ltd [PRS] and Universal Production Music || ",
            "hits": 95
        },
        {
            "id": 20403,
            "url": "https://svs.gsfc.nasa.gov/20403/",
            "result_type": "Animation",
            "release_date": "2025-05-14T09:00:00-04:00",
            "title": "Titan science results from James Webb Space Telescope: animation resource page",
            "description": "Push into JWST to Saturn and Titan. || JWST_Titan_Intro_Final_V001.00957_print.jpg (1024x576) [145.8 KB] || JWST_Titan_Intro_Final_V001.00957_searchweb.png (320x180) [78.0 KB] || JWST_Titan_Intro_Final_V001.00957_thm.png [5.5 KB] || JWST_Titan_Intro_Final_1080.mp4 (1920x1080) [72.8 MB] || JWST_Titan_Intro_Final_V001.mp4 (3840x2160) [38.4 MB] || JWST_Titan_Intro_Final_V001.mov (3840x2160) [6.8 GB] || ",
            "hits": 192
        },
        {
            "id": 14779,
            "url": "https://svs.gsfc.nasa.gov/14779/",
            "result_type": "Produced Video",
            "release_date": "2025-02-11T09:00:00-05:00",
            "title": "NASA's Illuminate Series (2025)",
            "description": "NASA's Illuminate is a video series about out-of-this-world images that shine light on our Sun and solar system. || ",
            "hits": 100
        },
        {
            "id": 14744,
            "url": "https://svs.gsfc.nasa.gov/14744/",
            "result_type": "Produced Video",
            "release_date": "2025-01-03T00:00:00-05:00",
            "title": "GDC and DYNAMIC to Explore Earth’s Upper Atmosphere",
            "description": "Two upcoming missions, the Geospace Dynamics Constellation (GDC) and Dynamical Neutral Atmosphere-Ionosphere Coupling (DYNAMIC) will revolutionize our understanding of Earth’s upper atmosphere. This region includes Earth’s ionosphere, thermosphere, and mesosphere, and stretches from roughly 50 to 400 miles above Earth’s surface. Space weather disturbances can impact communications, navigation signals, and satellite orbits, and induce currents can trigger power outages on Earth — making the region a crucial area of study.GDC is a team of satellites that will study Earth’s upper atmosphere and provide the first direct global measurements of our planet’s dynamic and complex interface with the space environment. Working in tandem with the DYNAMIC spacecraft, scientists will be able paint a fuller picture of how energy transforms and travels throughout the upper atmosphere. GDC will fly at an altitude of 350-400 km.DYNAMIC is a pair of satellites that will work in tandem with GDC to study how changes in Earth’s lower atmosphere influence our planet’s upper atmosphere. Between the multiple spacecraft of GDC and DYNAMIC, simultaneous observations from different locations can give scientists a more complete picture of how atmospheric waves propagate up through this unique part of the atmosphere. DYNAMIC will fly at an altitude of 550-800 km. || ",
            "hits": 82
        },
        {
            "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": 314
        },
        {
            "id": 14722,
            "url": "https://svs.gsfc.nasa.gov/14722/",
            "result_type": "Produced Video",
            "release_date": "2024-12-06T15:00:00-05:00",
            "title": "NASA Interview Opportunity: NASA Spacecraft Days Away From Historic Close Approach to the Sun",
            "description": "Scroll down the page for associated cut b-roll for the live shots and pre-recorded soundbites.Find out more about NASA's Parker Solar Probe here! nasa.gov/parker || Screenshot_2024-12-06_at_2.24.02 PM.png (1546x606) [1.9 MB] || Screenshot_2024-12-06_at_2.24.02 PM_print.jpg (1024x401) [195.3 KB] || Screenshot_2024-12-06_at_2.24.02 PM_searchweb.png (320x180) [128.7 KB] || Screenshot_2024-12-06_at_2.24.02 PM_thm.png (80x40) [12.2 KB] || ",
            "hits": 60
        },
        {
            "id": 14716,
            "url": "https://svs.gsfc.nasa.gov/14716/",
            "result_type": "Produced Video",
            "release_date": "2024-11-07T13:00:00-05:00",
            "title": "Hurricane Helene’s Gravity Waves Revealed by NASA’s AWE",
            "description": "On Sept. 26, 2024, Hurricane Helene slammed into the Gulf Coast of Florida, inducing storm surges and widespread destruction on the land below. At the same time, NASA’s Atmospheric Waves Experiment (AWE), which is mounted on the outside of the International Space Station, recorded enormous swells that the hurricane produced in the atmosphere roughly 55 miles above the ground.These massive ripples through the upper atmosphere, known as atmospheric gravity waves, appear in AWE’s images as concentric bands extending away from northern Florida.Visit this page to learn more. || ",
            "hits": 112
        },
        {
            "id": 31319,
            "url": "https://svs.gsfc.nasa.gov/31319/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-10-23T00:00:00-04:00",
            "title": "2025 NASA Science Calendar",
            "description": "Images from the 2025 NASA Science Calendar",
            "hits": 151
        },
        {
            "id": 14690,
            "url": "https://svs.gsfc.nasa.gov/14690/",
            "result_type": "Produced Video",
            "release_date": "2024-09-23T14:00:00-04:00",
            "title": "Ten Years at Mars with NASA’s MAVEN Mission",
            "description": "During its first decade at Mars, MAVEN has helped to explain how the Red Planet evolved from warm and wet into the cold, dry world we see today. Complete transcript available.Universal Production Music: “Executive Deceit” by Samuel Karl Bohn [PRS], Chalk Music [PRS]; “Quasar” by Ross Stephen Gilmartin [PRS], Chappell Recorded Music Library Ltd [PRS]; “Modular Odyssey” and “Synthology” by Laetitia Frenod [SACEM], Koka Media [SACEM]Watch this video on the NASA Goddard YouTube channel. || MAVEN-10th-Anniversary-Preview_print.jpg (1024x576) [160.7 KB] || MAVEN-10th-Anniversary-Preview.jpg (1280x720) [622.5 KB] || MAVEN-10th-Anniversary-Preview.png (1280x720) [1.2 MB] || MAVEN-10th-Anniversary-Preview_searchweb.png (320x180) [80.6 KB] || MAVEN-10th-Anniversary-Preview_thm.png (80x40) [6.3 KB] || 14690_MAVEN_10th_Anniversary_720.mp4 (1280x720) [92.2 MB] || 14690_MAVEN_10th_Anniversary_1080.mp4 (1920x1080) [516.6 MB] || Maven10thAnniversaryCaptionsV3.en_US.srt [8.9 KB] || Maven10thAnniversaryCaptionsV3.en_US.vtt [8.5 KB] || 14690_MAVEN_10th_Anniversary_4K.mp4 (3840x2160) [6.3 GB] || 14690_MAVEN_10th_Anniversary_ProRes.mov (3840x2160) [36.5 GB] || ",
            "hits": 172
        },
        {
            "id": 14675,
            "url": "https://svs.gsfc.nasa.gov/14675/",
            "result_type": "Produced Video",
            "release_date": "2024-09-03T17:00:00-04:00",
            "title": "ESCAPADE Testing and Integration",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The spacecraft were designed, built, integrated, and tested by Rocket Lab at their Spacecraft Production Complex and Headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 87
        },
        {
            "id": 14628,
            "url": "https://svs.gsfc.nasa.gov/14628/",
            "result_type": "Produced Video",
            "release_date": "2024-08-28T11:30:00-04:00",
            "title": "Discovering Earth’s Third Global Energy Field",
            "description": "High above the Earth’s North and South Poles, a steady stream of particles escapes from our atmosphere into space. Scientists call this mysterious outflow the “polar wind,” and for almost 60 years, spacecraft have been flying through it as scientists have theorized about its cause. The leading theory was that a planet-wide electric field was drawing those particles up into space. But this so-called ambipolar electric field, if it exists, is so weak that all attempts to measure it have failed – until now.In 2022, scientists traveled to Svalbard, a small archipelago in Norway, to launch a rocket in an attempt to measure Earth’s ambipolar electric field for the first time. This was NASA’s Endurance rocketship mission, and this is its story.To learn more, visit: https://science.nasa.gov/science-research/heliophysics/nasa-discovers-long-sought-global-electric-field-on-earth/ || ",
            "hits": 175
        },
        {
            "id": 14664,
            "url": "https://svs.gsfc.nasa.gov/14664/",
            "result_type": "Produced Video",
            "release_date": "2024-08-23T16:00:00-04:00",
            "title": "ESCAPADE Mission Trailer",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 44
        },
        {
            "id": 14667,
            "url": "https://svs.gsfc.nasa.gov/14667/",
            "result_type": "Produced Video",
            "release_date": "2024-08-22T14:00:00-04:00",
            "title": "ESCAPADE Instrument Build and Testing",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 49
        },
        {
            "id": 14665,
            "url": "https://svs.gsfc.nasa.gov/14665/",
            "result_type": "Produced Video",
            "release_date": "2024-08-21T09:00:00-04:00",
            "title": "ESCAPADE Spacecraft Development Images",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin.The spacecraft were designed, built, integrated, and tested at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more. || ",
            "hits": 94
        },
        {
            "id": 31302,
            "url": "https://svs.gsfc.nasa.gov/31302/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-08-02T00:00:00-04:00",
            "title": "NASA's Balloon Program",
            "description": "Scientific Balloon Program Infographic || nasa-scientific-balloon-facts_print.jpg (1024x576) [171.2 KB] || nasa-scientific-balloon-facts.png (3840x2160) [3.0 MB] || nasa-scientific-balloon-facts_searchweb.png (320x180) [58.8 KB] || nasa-scientific-balloon-facts_thm.png (80x40) [6.3 KB] || nasas-balloon-program-infographic.hwshow [280 bytes] || ",
            "hits": 279
        },
        {
            "id": 14641,
            "url": "https://svs.gsfc.nasa.gov/14641/",
            "result_type": "Infographic",
            "release_date": "2024-07-30T15:00:00-04:00",
            "title": "ESCAPADE Mission Posters",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first coordinated multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 72
        },
        {
            "id": 14642,
            "url": "https://svs.gsfc.nasa.gov/14642/",
            "result_type": "Infographic",
            "release_date": "2024-07-30T15:00:00-04:00",
            "title": "ESCAPADE Spacecraft Specifications",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission, led by Rob Lillis at the University of California, Berkeley, Space Sciences Laboratory (UCBSSL), is a twin-spacecraft science mission that will orbit two spacecraft around Mars to understand the structure, composition, variability, and dynamics of Mars' unique hybrid magnetosphere. The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time. ESCAPADE is being developed under NASA’s Small Innovative Missions for Planetary Exploration (SIMPLEx) program in the Science Mission Directorate (SMD). The mission is led by UCBSSL with spacecraft design provided by Rocket Lab.The spacecraft were designed, built, integrated, and tested at Rocket Lab’s Spacecraft Production Complex and headquarters in Long Beach, California. Based on Rocket Lab’s Explorer spacecraft, a configurable, high delta-V interplanetary platform, the duo features Rocket Lab-built components and subsystems, including solar panels, star trackers, propellant tanks, reaction wheels, reaction control systems, radios, and more. || ",
            "hits": 111
        },
        {
            "id": 14635,
            "url": "https://svs.gsfc.nasa.gov/14635/",
            "result_type": "Produced Video",
            "release_date": "2024-07-22T12:00:00-04:00",
            "title": "ESCAPADE Mission Spacecraft Beauty Passes",
            "description": "NASA’s Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will study the interaction between the solar wind and Martian atmosphere. Two identical spacecraft will orbit around the Red Planet to understand the structure, composition, variability, and dynamics of Mars’ unique hybrid magnetosphere, including its real-time response to space weather.The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time — so much that Mars no longer supports liquid water on its surface. The pair will be the first coordinated multi-spacecraft orbital science mission to Mars.ESCAPADE is part of the NASA Small Innovative Missions for Planetary Exploration (SIMPLEx) program. The mission is managed by the University of California Berkeley’s Space Sciences Laboratory, with key partners Rocket Lab, NASA Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 82
        },
        {
            "id": 5238,
            "url": "https://svs.gsfc.nasa.gov/5238/",
            "result_type": "Visualization",
            "release_date": "2024-06-27T11:00:00-04:00",
            "title": "Our Active Ionosphere",
            "description": "In this view of Earth on October 7, 2019, just past sunset, GOLD observed an X-shaped structure in the equatorial ionization anomaly. || GOLD_O5S_20191007.00034_print.jpg (1024x576) [76.3 KB] || GOLD_O5S_20191007 [0 Item(s)] || GOLD_O5S_20191007_1080p4.mp4 (1920x1080) [1.8 MB] || ",
            "hits": 108
        },
        {
            "id": 14592,
            "url": "https://svs.gsfc.nasa.gov/14592/",
            "result_type": "Produced Video",
            "release_date": "2024-05-14T00:00:00-04:00",
            "title": "Largest Flare yet from Solar Cycle 25",
            "description": "On May 14, 2024, the Sun emitted a strong solar flare. This solar flare is the largest of Solar Cycle 25 and is classified as an X8.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.A solar flare is an intense burst of radiation, or light, on the Sun. Flares are our solar system’s most powerful explosive events. Light only takes about 8 minutes to travel from the Sun to Earth, so that’s how long it would take the energy from a flare to reach our planet. Stronger solar flares — those rated class M5 or above — can have impacts on technology that depends on Earth’s ionosphere (our electrically charged upper atmosphere), like high-frequency radio used for navigation and GPS.NASA’s Solar Dynamics Observatory (SDO) captured these images of the flare, which peaked at 12:51 p.m. ET on May 14. The X8.7 flare appears on the lower right edge of the Sun. (A small eruption appears afterward in the upper left.) SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. Different wavelengths are shown in this video to highlight different features of the flare.Music credit: “Ethereal Mirrorscape” from the album Reflections written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || X8pt7_flare_May_14_2024.00_00_40_22.Still001.jpg (3840x2160) [3.0 MB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_print.jpg (1024x576) [342.3 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_searchweb.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_web.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_thm.png (80x40) [6.1 KB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.webm (3840x2160) [20.4 MB] || 14592_SDO_X8pt7_flare_May_14_2024_Good_Outro.mp4 (3840x2160) [175.9 MB] || 14592_SDO_X8pt7_flare_May_14_2024_YouTube_Outro.mp4 (3840x2160) [673.0 MB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.mov (3840x2160) [4.2 GB] || ",
            "hits": 410
        },
        {
            "id": 5240,
            "url": "https://svs.gsfc.nasa.gov/5240/",
            "result_type": "Visualization",
            "release_date": "2024-04-22T00:00:00-04:00",
            "title": "Radio Signal Reflection & Refraction on a Simple Ionosphere Model",
            "description": "A simple animated plotting of radio wave refraction and reflection on a simplified ionosphere model, landscape format. || polar.propagation.basic.sample.1920x1080.png (1920x1080) [178.8 KB] || polar.propagation.basic.sample.1920x1080.1590_print.jpg (1024x576) [69.8 KB] || polar.propagation.basic.sample.1920x1080.1590_searchweb.png (320x180) [20.5 KB] || polar.propagation.basic.sample.1920x1080.1590_thm.png (80x40) [3.2 KB] || polar.propagation.basic.sample.1920x1080_p30.mp4 (1920x1080) [456.4 KB] || polar.propagation.basic.sample.1920x1080 (1920x1080) [0 Item(s)] || ",
            "hits": 263
        },
        {
            "id": 14399,
            "url": "https://svs.gsfc.nasa.gov/14399/",
            "result_type": "Produced Video",
            "release_date": "2023-12-20T11:00:00-05:00",
            "title": "Fermi's 14-Year Time-Lapse of the Gamma-Ray Sky",
            "description": "From solar flares to black hole jets: NASA’s Fermi Gamma-ray Space Telescope has produced a unique time-lapse tour of the dynamic high-energy sky. Fermi Deputy Project Scientist Judy Racusin narrates this movie, which compresses 14 years of gamma-ray observations into 6 minutes. Credit: NASA’s Goddard Space Flight Center and NASA/DOE/LAT CollaborationMusic: \"Expanding Shell\" written and produced by Lars Leonhard.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Video descriptive text available. || Fermi_14Year_Narrated_Still_print.jpg (1024x576) [157.6 KB] || Fermi_14Year_Narrated_Still.jpg (3840x2160) [891.9 KB] || Fermi_14Year_Narrated_Still_searchweb.png (320x180) [39.2 KB] || Fermi_14Year_Narrated_Still_thm.png (80x40) [4.2 KB] || 14399_Fermi_14Year_Narrated_sub100.mp4 (1920x1080) [90.5 MB] || 14399_Fermi_14Year_Narrated_1080.webm (1920x1080) [49.4 MB] || 14399_Fermi_14Year_Narrated_1080.mp4 (1920x1080) [908.7 MB] || Fermi_14Year_Narrated_SRT_Captions.en_US.srt [8.4 KB] || Fermi_14Year_Narrated_SRT_Captions.en_US.vtt [8.0 KB] || 14399_Fermi_14Year_Narrated_4k.mp4 (3840x2160) [2.2 GB] || 14399_Fermi_14Year_Narrated_ProRes_3840x2160_2997.mov (3840x2160) [19.4 GB] || ",
            "hits": 143
        },
        {
            "id": 14477,
            "url": "https://svs.gsfc.nasa.gov/14477/",
            "result_type": "Produced Video",
            "release_date": "2023-12-11T12:00:00-05:00",
            "title": "The Day the Solar Wind Disappeared from Mars",
            "description": "Learn about the “disappearance” of the solar wind at Mars that was witnessed by MAVEN – an event last seen nearly a quarter-century ago at Earth.Complete transcript available.Universal Production Music: “Space Museum” by Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]; “Currents and Crime Scenes” by Dylan Matthew Love and Harry Gregson Williams [BMI], Atmosphere Music Ltd. [PRS]Watch this video on the NASA Goddard YouTube channel. || MAVEN_Solar_Wind_Disappear_V4_print.jpg (1024x576) [142.7 KB] || MAVEN_Solar_Wind_Disappear_V4.jpg (1280x720) [459.3 KB] || MAVEN_Solar_Wind_Disappear_V4.png (1280x720) [800.2 KB] || MAVEN_Solar_Wind_Disappear_V4_searchweb.png (320x180) [69.9 KB] || MAVEN_Solar_Wind_Disappear_V4_thm.png (80x40) [6.5 KB] || 14477_MAVEN_Solar_Wind_Disappear_720.mp4 (1280x720) [43.4 MB] || 14477_MAVEN_Solar_Wind_Disappear_1080.mp4 (1920x1080) [243.1 MB] || MavenSolarWindCaptionsV2.en_US.srt [3.8 KB] || MavenSolarWindCaptionsV2.en_US.vtt [3.6 KB] || 14477_MAVEN_Solar_Wind_Disappear_4K.mp4 (3840x2160) [3.0 GB] || 14477_MAVEN_Solar_Wind_Disappear_ProRes.mov (3840x2160) [20.7 GB] || ",
            "hits": 64
        },
        {
            "id": 14464,
            "url": "https://svs.gsfc.nasa.gov/14464/",
            "result_type": "Produced Video",
            "release_date": "2023-11-17T14:00:00-05:00",
            "title": "NASA Mission Catching AWEsome Waves in Earth’s Airglow",
            "description": "Attached to the International Space Station, NASA’s Atmospheric Waves Experiment, or AWE, is studying airglow, an ethereal radiance at the boundary between Earth’s atmosphere and space, to look for an invisible phenomenon called atmospheric gravity waves.Caused by winds rushing over mountain ranges or severe weather events such as hurricanes, thunderstorms, and tornadoes, atmospheric gravity waves can grow and reach all the way to space, where it interacts with space weather. Find out more about the AWE mission and how it will help us better understand the connection between weather on Earth and weather in space. || ",
            "hits": 102
        },
        {
            "id": 14440,
            "url": "https://svs.gsfc.nasa.gov/14440/",
            "result_type": "Produced Video",
            "release_date": "2023-10-25T08:00:00-04:00",
            "title": "Atmospheric Waves Experiment (AWE) Media Resources",
            "description": "From its unique vantage point on the International Space Station, NASA’s Atmospheric Waves Experiment (AWE) will look directly down into Earth’s atmosphere to study how gravity waves travel through the upper atmosphere. Data collected by AWE will enable scientists to determine the physics and characteristics of atmospheric gravity waves and how terrestrial weather influences the ionosphere, which can affect communication with satellites.AWE is led by Michael Taylor at Utah State University in Logan, and it is managed by the Explorers Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Utah State University’s Space Dynamics Laboratory built the AWE instrument and will provide the mission operations center.Visit https://science.nasa.gov/mission/awe/ to learn more. Watch AWE launch aboard NASA's SpaceX Cargo Dragon. Download isolated launch views of NASA's SpaceX CRS-29 mission. || ",
            "hits": 122
        },
        {
            "id": 40513,
            "url": "https://svs.gsfc.nasa.gov/gallery/awe/",
            "result_type": "Gallery",
            "release_date": "2023-10-25T00:00:00-04:00",
            "title": "AWE – Atmospheric Waves Experiment",
            "description": "From its unique vantage point on the International Space Station, NASA’s Atmospheric Waves Experiment (AWE) looks directly down into Earth’s atmosphere to study how atmospheric gravity waves — naturally occurring waves often caused by weather disturbances — travel through the upper atmosphere. Data collected by AWE enables scientists to determine the physics and characteristics of atmospheric gravity waves and how terrestrial weather influences the ionosphere, which can affect communication with satellites.\n\nAWE launched on Nov. 9, 2023, from NASA’s Kennedy Space Center in Florida.\n\nLearn more: https://science.nasa.gov/mission/awe/",
            "hits": 165
        },
        {
            "id": 13288,
            "url": "https://svs.gsfc.nasa.gov/13288/",
            "result_type": "Produced Video",
            "release_date": "2023-10-14T13:00:00-04:00",
            "title": "Study Total Solar Eclipses With Ham Radio",
            "description": "Music credit: “Make a Change” by Eric Chevalier [SACEM] from Universal Production Music.Complete transcript available. || HamSCI_Thumbnail.jpg (1280x720) [448.6 KB] || HamSCI_Thumbnail_print.jpg (1024x576) [358.9 KB] || HamSCI_Thumbnail_searchweb.png (320x180) [71.1 KB] || HamSCI_Thumbnail_web.png (320x180) [71.1 KB] || HamSCI_Thumbnail_thm.png (80x40) [6.2 KB] || HamSCI_Video_2024.webm (1920x1080) [12.0 MB] || HamSCI_Video_2024.mp4 (1920x1080) [194.9 MB] || HAMSCI.en_US.srt [2.2 KB] || HAMSCI.en_US.vtt [2.1 KB] || ",
            "hits": 56
        },
        {
            "id": 20385,
            "url": "https://svs.gsfc.nasa.gov/20385/",
            "result_type": "Animation",
            "release_date": "2023-10-04T15:00:00-04:00",
            "title": "Atmospheric Waves Experiment (AWE) Beauty Pass",
            "description": "AWE aboard the ISS || ISS_AWE_ProRes.00420_print.jpg (576x1024) [133.9 KB] || ISS_AWE_ProRes.00420_searchweb.png (180x320) [81.4 KB] || ISS_AWE_ProRes.00420_thm.png (80x40) [6.7 KB] || ISS_AWE_1080_h264.mov (1920x1080) [27.7 MB] || ISS_AWE_ProRes.mov (3840x2160) [1.7 GB] || ISS_AWE_h264.mov (3840x2160) [66.2 MB] || AWE_frames (3840x2160) [32.0 KB] || ISS_AWE_ProRes.webm (3840x2160) [9.6 MB] || ",
            "hits": 65
        },
        {
            "id": 14204,
            "url": "https://svs.gsfc.nasa.gov/14204/",
            "result_type": "Produced Video",
            "release_date": "2022-08-31T09:00:00-04:00",
            "title": "Mars Patchy Proton Aurora",
            "description": "NASA’s MAVEN (Mars Atmosphere and Volatile Evolution) mission and the United Arab Emirates’ Emirates Mars Mission (EMM) have released joint observations of dynamic proton aurora events at Mars. Remote auroral observations by EMM paired with in-situ plasma observations made by MAVEN open new avenues for understanding the Martian atmosphere. This collaboration was made possible by recent data-sharing between the two missions and highlights the value of multi-point observations in space.Learn more about this discovery by MAVEN and EMM. || ",
            "hits": 84
        },
        {
            "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": 608
        },
        {
            "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": 137
        },
        {
            "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": 229
        },
        {
            "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": 362
        },
        {
            "id": 14025,
            "url": "https://svs.gsfc.nasa.gov/14025/",
            "result_type": "Produced Video",
            "release_date": "2021-11-29T11:00:00-05:00",
            "title": "Strong Winds Power Electric Fields in the Upper Atmosphere",
            "description": "Using observations from NASA’s ICON mission, scientists presented the first direct measurements of Earth’s long-theorized dynamo on the edge of space: a wind-driven electrical generator that spans the globe 60-plus miles above our heads. The dynamo churns in the ionosphere, the electrically charged boundary between Earth and space. It’s powered by tidal winds in the upper atmosphere that are faster than most hurricanes and rise from the lower atmosphere, creating an electrical environment that can affect satellites and technology on Earth. The new work, published today in Nature Geoscience, improves our understanding of the ionosphere, which helps scientists better predict space weather and protect our technology from its effects.More information: https://www.nasa.gov/feature/goddard/2021/strong-winds-power-electric-fields-in-upper-atmosphere-icon/ || ",
            "hits": 96
        },
        {
            "id": 20351,
            "url": "https://svs.gsfc.nasa.gov/20351/",
            "result_type": "Animation",
            "release_date": "2021-11-09T10:00:00-05:00",
            "title": "The DAVINCI Mission to Venus",
            "description": "DAVINCI the Movie || DaVinci1021cut422HQ.00130_print.jpg (1024x438) [75.7 KB] || DaVinci1021cut422HQ.00130_searchweb.png (180x320) [61.3 KB] || DaVinci1021cut422HQ.00130_thm.png (80x40) [5.3 KB] || DaVinci1021cut1080h264.mp4 (1920x820) [208.7 MB] || DaVinci1021cut720422HQ.mov (1682x720) [3.5 GB] || DaVinci1021cut720h264.mp4 (1280x548) [133.2 MB] || DaVinci1021cut720h264.webm (1280x548) [22.0 MB] || DaVinci1021cut422HQ.mov (5045x2160) [20.3 GB] || DaVinci1021cut1080422HQ.mov (2523x1080) [5.6 GB] || 20351_DAVINCIMissiontoVenus_CAPTIONS.en_US.srt [3.8 KB] || 20351_DAVINCIMissiontoVenus_CAPTIONS.en_US.vtt [3.6 KB] || ",
            "hits": 233
        },
        {
            "id": 13969,
            "url": "https://svs.gsfc.nasa.gov/13969/",
            "result_type": "Produced Video",
            "release_date": "2021-10-21T00:00:00-04:00",
            "title": "Geospace Dynamics Constellation",
            "description": "\"Moonstone,\" by Rainman [PRS]; Atmosphere; Universal Production Music || 13969_GDC_Mission_FINAL.mov (1920x1080) [4.9 GB] || GDC_MissionVideo_Still.png (1920x1080) [3.7 MB] || GDC_Mission_SITLL.jpg (1920x1080) [441.3 KB] || 13969_GDC_Mission_FINAL_lowres.mp4 (1280x720) [62.3 MB] || TWITTER_720_13969_GDC_Mission_FINAL_twitter_720.mp4 (1280x720) [42.8 MB] || 13969_GDC_Mission_FINAL.webm (960x540) [94.7 MB] || YOUTUBE_1080_13969_GDC_Mission_FINAL_youtube_1080.mp4 (1920x1080) [339.8 MB] || 13969_GDC_Mission_FINAL.en_US.srt [4.8 KB] || 13969_GDC_Mission_FINAL.en_US.vtt [4.6 KB] || YOUTUBE_4K_13969_GDC_Mission_FINAL_youtube_4k.mp4 (3840x2160) [1.4 GB] || ",
            "hits": 34
        },
        {
            "id": 13847,
            "url": "https://svs.gsfc.nasa.gov/13847/",
            "result_type": "Produced Video",
            "release_date": "2021-05-03T09:00:00-04:00",
            "title": "NASA’s Parker Solar Probe Discovers Natural Radio Emission in Venus’ Atmosphere",
            "description": "During a brief swing by Venus, NASA’s Parker Solar Probe detected a natural radio signal that revealed the spacecraft had flown through the planet’s upper atmosphere. This was the first direct measurement of the Venusian atmosphere in nearly 30 years — and it looks quite different from Venus past. A study published today in Geophysical Research Letters confirms that Venus’ upper atmosphere undergoes puzzling changes over a solar cycle, the Sun’s 11-year activity cycle. This marks the latest clue to untangling how and why Venus and Earth are so different. || ",
            "hits": 277
        },
        {
            "id": 4904,
            "url": "https://svs.gsfc.nasa.gov/4904/",
            "result_type": "Infographic",
            "release_date": "2021-04-28T00:00:00-04:00",
            "title": "Heliophysics Background Images for MS-Teams & PowerPoint",
            "description": "Upper atmosphere & ionosphere theme. || Helio_Teams_Bkgrd_1.jpg (1920x1080) [218.8 KB] || Helio_Teams_Bkgrd_1_with_Logos.png (1920x1080) [2.3 MB] || Helio_Teams_Bkgrd_1_with_Logos_and_Txt.png (1920x1080) [2.3 MB] || Helio_Teams_Bkgrd_1_print.jpg (1024x576) [151.3 KB] || Helio_Teams_Bkgrd_PPT_1.pptx [520.0 KB] || Six theme images for NASA Heliophysics - image, image+logos, image+logos+text, and PowerPoint files.  Suitable as background images for MS-Teams and PowerPoint presentations. || ",
            "hits": 43
        },
        {
            "id": 13714,
            "url": "https://svs.gsfc.nasa.gov/13714/",
            "result_type": "Produced Video",
            "release_date": "2020-09-15T13:00:00-04:00",
            "title": "Solar Cycle 25 Is Here. NASA, NOAA Scientists Explain What This Means",
            "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.Click here for the NOAA press kit.Listen to the media telecon.Participants:• Lisa Upton, Co-chair, Solar Cycle 25 Prediction Panel; Solar Physicist, Space Systems Research Corporation• Doug Biesecker, Solar Physicist, NOAA’s Space Weather Prediction Center; Co-chair, Solar Cycle 25 Prediction Panel• Elsayed Talaat, Director, Office of Projects, Planning and Analysis; NOAA’s Satellite and Information Service • Lika Guhathakurta, Heliophysicist, Heliophysics Division, NASA Headquarters • Jake Bleacher, Chief Exploration Scientist, NASA Human Exploration and Operations Mission Directorate || ",
            "hits": 206
        },
        {
            "id": 13664,
            "url": "https://svs.gsfc.nasa.gov/13664/",
            "result_type": "Produced Video",
            "release_date": "2020-07-16T08:00:00-04:00",
            "title": "ESA and NASA Release First Images From Solar Orbiter Mission",
            "description": "Scientists from ESA (European Space Agency) and NASA will present the first images captured by Solar Orbiter, the joint ESA/NASA mission to study the Sun, during an online news briefing at 8 a.m. EDT Thursday, July 16. Launched on Feb. 9, 2020, Solar Orbiter turned on all 10 of its instruments together for the first time in mid-June as it made its first close pass of the Sun. The flyby captured the closest images ever taken of the Sun. During the briefing, mission experts will discuss what these closeup images reveal about our star, including what we can learn from Solar Orbiter’s new measurements of particles and magnetic fields flowing from the Sun.The briefing will stream live at:https://www.nasa.gov/solarorbiterfirstlight/Participants in the call include:•Daniel Müller – Solar Orbiter Project Scientist at ESA•Holly R. Gilbert – Solar Orbiter Project Scientist at NASA•José Luis Pellón Bailón – Solar Orbiter Deputy Spacecraft Operations Manager at ESA•David Berghmans – Principal investigator of the Extreme Ultraviolet Imager (EUI) at the Royal Observatory of Belgium•Sami Solanki – Principal investigator of the Polarimetric and Helioseismic Imager (PHI) and director of the Max Planck Institute for Solar System Research•Christopher J. Owen – Principal investigator of the Solar Wind Analyser (SWA) at Mullard Space Science Laboratory, University College London•ESA’s first light images•ESA press release •NASA feature story || ",
            "hits": 131
        },
        {
            "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": 34
        },
        {
            "id": 4730,
            "url": "https://svs.gsfc.nasa.gov/4730/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T11:00:00-04:00",
            "title": "MAVEN – Mars Electric Current Systems",
            "description": "The current systems formed around Mars as a result of a solar wind driven convective electric field(Note: These frame sets were converted to the sRGB color space on 6/16/2020)This video is also available on our YouTube channel. || ideal_currents_1080.00600_print.jpg (1024x576) [71.1 KB] || ideal_currents_1080.00600_searchweb.png (320x180) [21.7 KB] || ideal_currents_1080.00600_thm.png (80x40) [2.0 KB] || ideal_currents_1080p30.mp4 (1920x1080) [74.0 MB] || ideal_currents_1080.webm (1920x1080) [9.9 MB] || ideal_curr (1920x1080) [0 Item(s)] || ideal_curr (3840x2160) [0 Item(s)] || captions_silent.25991.en_US.srt [43 bytes] || ideal_currents_4k_2160p30.mp4 (3840x2160) [170.1 MB] || idealized_currents_prores.mov (1920x1080) [2.9 GB] || Mars_idealized_currents_4k_prores.mov (3840x2160) [3.5 GB] || ideal_currents_1080p30.mp4.hwshow || ",
            "hits": 82
        },
        {
            "id": 13625,
            "url": "https://svs.gsfc.nasa.gov/13625/",
            "result_type": "Produced Video",
            "release_date": "2020-05-25T11:00:00-04:00",
            "title": "First Map of Mars Electric Currents",
            "description": "MAVEN data have enabled the first map of the electric current systems (blue and red arrows) that shape the induced magnetic field surrounding Mars.Credit: NASA/Goddard/MAVEN/CU Boulder/SVSUniversal Production Music: “A Lucid Dream” and “Shimmer Oscillations” by James Joshua OttoWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || MarsElectricCurrentsPreview6_print.jpg (1024x576) [305.8 KB] || MarsElectricCurrentsPreview6.jpg (1920x1080) [853.6 KB] || MarsElectricCurrentsPreview6_searchweb.png (320x180) [50.6 KB] || MarsElectricCurrentsPreview6_thm.png (80x40) [5.3 KB] || 13625_Mars_Electric_Currents_Twitter.mp4 (1280x720) [63.8 MB] || 13625_Mars_Electric_Currents_Facebook.mp4 (1920x1080) [359.1 MB] || 13625_Mars_Electric_Currents_YouTube.webm (3840x2160) [91.7 MB] || 13625_Mars_Electric_Currents_Captions.en_US.srt [7.2 KB] || 13625_Mars_Electric_Currents_Captions.en_US.vtt [6.8 KB] || 13625_Mars_Electric_Currents_YouTube.mp4 (3840x2160) [2.8 GB] || 13625_Mars_Electric_Currents_MASTER.mov (3840x2160) [14.2 GB] || 13625_Mars_Electric_Currents_Facebook.mp4.hwshow [134 bytes] || ",
            "hits": 102
        },
        {
            "id": 4824,
            "url": "https://svs.gsfc.nasa.gov/4824/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T00:00:00-04:00",
            "title": "MAVEN Observes Solar Particle Velocities and the Induced Magnetic Field",
            "description": "MAVEN orbits Mars and measures solar particle velocities and variations in the solar wind’s magnetic field. || maven_vels_magField.03000_print.jpg (1024x576) [92.5 KB] || maven_vels_magField.03000_searchweb.png (320x180) [63.5 KB] || maven_vels_magField.03000_thm.png (80x40) [4.2 KB] || maven_vels_magField_1080p30.mp4 (1920x1080) [83.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || maven_vels_magField_1080p30.webm (1920x1080) [19.0 MB] || 4824_MAVEN_Solar_Wind_Data_1080_30p.mov (1920x1080) [2.6 GB] || maven_vels_magField_1080p30.mp4.hwshow [193 bytes] || ",
            "hits": 71
        },
        {
            "id": 4825,
            "url": "https://svs.gsfc.nasa.gov/4825/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T00:00:00-04:00",
            "title": "MAVEN – Mars and Solar Wind Simulation",
            "description": "This simulation depicts the solar wind interacting with the Mars upper atmosphere, with MAVEN's orbit embedded. || maven_cme44.03600_print.jpg (1024x512) [253.9 KB] || maven_cme44.03600_searchweb.png (320x180) [92.7 KB] || maven_cme44.03600_thm.png (80x40) [5.2 KB] || 1920x1080_16x9_30p (2048x1024) [0 Item(s)] || maven_cme44_1024p30.webm (2048x1024) [5.9 MB] || maven_cme44_1024p30.mp4 (2048x1024) [195.1 MB] || maven_cme44_1024p30.mp4.hwshow [58 bytes] || ",
            "hits": 107
        },
        {
            "id": 31115,
            "url": "https://svs.gsfc.nasa.gov/31115/",
            "result_type": "Hyperwall Visual",
            "release_date": "2020-02-12T00:00:00-05:00",
            "title": "Airglow over Australia",
            "description": "airglow over australia seen from the ISS || airglow-australia_print.jpg (1024x576) [150.3 KB] || airglow-australia.png (3840x2160) [15.1 MB] || airglow-australia_searchweb.png (320x180) [80.8 KB] || airglow-australia_thm.png (80x40) [4.7 KB] || airglow-over-australia.hwshow [280 bytes] || ",
            "hits": 39
        },
        {
            "id": 13342,
            "url": "https://svs.gsfc.nasa.gov/13342/",
            "result_type": "Produced Video",
            "release_date": "2020-02-03T11:00:00-05:00",
            "title": "MAVEN Explores Mars to Understand Radio Interference at Earth",
            "description": "The MAVEN mission explores Mars’ atmosphere to better study a phenomenon observed at Earth, known as “Sporadic-E Layers.” They are concentrations of plasma that form in the ionosphere and interfere with radio waves. This video is animated in a comic book style.Music from Universal Production Music. Songs include: \"Alpha and Omega,\" \"Break the News,\" and \"Waiting for a Sensation.\" || MAVEN_thumb.jpg (3840x2160) [801.1 KB] || MAVEN_thumb_searchweb.png (320x180) [106.4 KB] || MAVEN_thumb_thm.png (80x40) [5.2 KB] || 13342_SPORADIC_MAVEN_MASTER.webm (960x540) [63.4 MB] || 13342_SPORADIC_MAVEN_MASTER_twitter_720.mp4 (1280x720) [29.9 MB] || 13342_SPORADIC_MAVEN_MASTER_facebook_720.mp4 (1280x720) [178.5 MB] || 13442_MAVEN_caption.en_US.srt [4.4 KB] || 13442_MAVEN_caption.en_US.vtt [4.4 KB] || 13342_SPORADIC_MAVEN_MASTER.mov (3840x2160) [10.8 GB] || ",
            "hits": 41
        },
        {
            "id": 31098,
            "url": "https://svs.gsfc.nasa.gov/31098/",
            "result_type": "Hyperwall Visual",
            "release_date": "2020-01-31T00:00:00-05:00",
            "title": "Beyond City Lights—Java Sea",
            "description": "Beyond City Lights—Java Sea || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8_print.jpg (1024x576) [114.4 KB] || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8.png (5760x3240) [13.6 MB] || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8_searchweb.png (320x180) [78.2 KB] || Page23JAVASEA_Hyperwall_5760x3240_19.2x10.8_thm.png (80x40) [4.7 KB] || beyond-city-lightsjava-sea.hwshow [336 bytes] || ",
            "hits": 84
        },
        {
            "id": 4755,
            "url": "https://svs.gsfc.nasa.gov/4755/",
            "result_type": "Visualization",
            "release_date": "2019-12-12T14:00:00-05:00",
            "title": "Mars Upper Level Winds Observed by MAVEN - Visualizations",
            "description": "MAVEN observes upper level Martian winds over the course of about two years. || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_print.jpg (1024x576) [42.9 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_searchweb.png (320x180) [49.1 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_thm.png (80x40) [4.0 KB] || maven_upper_winds_campaigns_1080p60.mp4 (1920x1080) [51.0 MB] || maven_upper_winds_campaigns_1080p30.mp4 (1920x1080) [46.4 MB] || maven_upper_winds.0104_cam_mainShape_190909182423_beauty_1080p30.webm (1920x1080) [9.6 MB] || campaigns (3840x2160) [0 Item(s)] || maven_upper_winds_campaigns_2160p60.mp4 (3840x2160) [162.2 MB] || maven_upper_winds_campaigns_2160p30.mp4 (3840x2160) [146.8 MB] || 4755_MAVEN_Wind_Currents_Full.mov (3840x2160) [9.7 GB] || maven_upper_winds_campaigns_1080p30.mp4.hwshow [201 bytes] || ",
            "hits": 68
        },
        {
            "id": 13485,
            "url": "https://svs.gsfc.nasa.gov/13485/",
            "result_type": "Produced Video",
            "release_date": "2019-12-12T14:00:00-05:00",
            "title": "Mars Wind Currents Reveal a Surprising Feature",
            "description": "By measuring windspeed and direction in the Mars upper atmosphere, MAVEN has discovered that high-altitude wind currents are being disturbed by terrain features far below.Credit: NASA/Goddard/MAVEN/CU Boulder/University of MichiganUniversal Production Music: “Glacial Shifts” by James Joshua OttoWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || FACEBOOK_720_13485_Mars_Upper_Winds_MASTER_facebook_720.mp4 (1280x720) [216.5 MB] || 13485_MarsUpperWinds_Preview_print.jpg (1024x576) [77.9 KB] || 13485_MarsUpperWinds_Preview.jpg (3840x2160) [399.6 KB] || 13485_MarsUpperWinds_Preview_searchweb.png (320x180) [57.6 KB] || 13485_MarsUpperWinds_Preview_thm.png (80x40) [4.8 KB] || TWITTER_720_13485_Mars_Upper_Winds_MASTER_twitter_720.mp4 (1280x720) [37.3 MB] || 13485_Mars_Upper_Winds_MASTER.webm (960x540) [78.1 MB] || 13485_Mars_Upper_Winds_Captions.en_US.srt [4.2 KB] || 13485_Mars_Upper_Winds_Captions.en_US.vtt [4.2 KB] || CH28_13485_Mars_Upper_Winds_MASTER_ch28.mov (1280x720) [1.8 GB] || 13485_Mars_Upper_Winds_YouTube.mp4 (3840x2160) [2.0 GB] || 13485_Mars_Upper_Winds_MASTER.mov (3840x2160) [19.2 GB] || ",
            "hits": 70
        },
        {
            "id": 20302,
            "url": "https://svs.gsfc.nasa.gov/20302/",
            "result_type": "Animation",
            "release_date": "2019-12-12T14:00:00-05:00",
            "title": "Mars Wind Currents Reveal a Surprising Feature - Animations",
            "description": "By measuring windspeed and direction in the Mars upper atmosphere, MAVEN has discovered that high-altitude wind currents are being disturbed by terrain features far below. || 20302_MarsUpperWinds_Preview_print.jpg (1024x576) [131.1 KB] || 20302_MarsUpperWinds_Preview.jpg (3840x2160) [676.6 KB] || 20302_MarsUpperWinds_Preview_searchweb.png (320x180) [86.0 KB] || 20302_MarsUpperWinds_Preview_thm.png (80x40) [6.4 KB] || TWITTER_720_MAVEN_Mars_Terrain_Winds_twitter_720.mp4 (1280x720) [16.4 MB] || MAVEN_Mars_Terrain_Winds.webm (960x540) [39.0 MB] || YOUTUBE_1080_MAVEN_Mars_Terrain_Winds_youtube_1080.mp4 (1920x1080) [135.6 MB] || FACEBOOK_720_MAVEN_Mars_Terrain_Winds_facebook_720.mp4 (1280x720) [104.1 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || YOUTUBE_4K_MAVEN_Mars_Terrain_Winds_youtube_4k.mp4 (3840x2160) [595.8 MB] || MAVEN_Mars_Terrain_Winds.mov (3840x2160) [10.6 GB] || YOUTUBE_4K_MAVEN_Mars_Terrain_Winds_youtube_4k.mp4.hwshow [143 bytes] || ",
            "hits": 86
        },
        {
            "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": 138
        },
        {
            "id": 13502,
            "url": "https://svs.gsfc.nasa.gov/13502/",
            "result_type": "Produced Video",
            "release_date": "2019-12-10T17:00:00-05:00",
            "title": "AGU 2019 — Postcards from the edge of space: New images, new phenomena, and new insights",
            "description": "In a Dec. 10 press event at the fall meeting of the American Geophysical Union in San Francisco, California, three scientists presented new images of the ionosphere, the dynamic region where Earth’s atmosphere meets space. Home to astronauts and everyday technology like radio and GPS, the ionosphere constantly responds to changes from space above and Earth below.The collection of images presented include the first images from NASA’s ICON, new science results from NASA’s GOLD, and observations of a fleeting, never-before-studied aurora. Together, they bring color to invisible processes that have widespread implications for the part of space that is closest to home.SPEAKERS:• Jennifer Briggs, Pepperdine University, Malibu, California, United States• Richard Eastes, University of Colorado Boulder, Boulder, Colorado, United States• Thomas Immel, University of California Berkeley, Berkeley, California, United States || ",
            "hits": 47
        },
        {
            "id": 13427,
            "url": "https://svs.gsfc.nasa.gov/13427/",
            "result_type": "Produced Video",
            "release_date": "2019-11-20T13:00:00-05:00",
            "title": "A New Era in Gamma-ray Science",
            "description": "On Jan. 14, 2019, the Major Atmospheric Gamma Imaging Cherenkov (MAGIC) observatory in the Canary Islands captured the highest-energy light every recorded from a gamma-ray burst. MAGIC began observing the fading burst just 50 seconds after it was detected thanks to positions provided by NASA's Fermi and Swift spacecraft (top left and right, respectively, in this illustration). The gamma rays packed energy up to 10 times greater than previously seen. Credit: NASA/Fermi and Aurore Simonnet, Sonoma State University || GRB190114CbASimonnet.jpg (2475x3300) [4.5 MB] || GRB190114CbASimonnet_searchweb.png (320x180) [106.4 KB] || GRB190114CbASimonnet_thm.png (80x40) [6.6 KB] || ",
            "hits": 78
        },
        {
            "id": 13335,
            "url": "https://svs.gsfc.nasa.gov/13335/",
            "result_type": "Produced Video",
            "release_date": "2019-10-04T10:00:00-04:00",
            "title": "NASA’s Mission to Explore the Connection Between Earth’s Weather and Space",
            "description": "Broll and Canned Interviews will be added on October 9th at 5:45 a.m. Click HERE for audio sound bites with NASA Scientist Sarah Jones.Click HERE for a canned interview with NASA Scientist Alex Young.Click HERE for a canned interview with NASA Scientist Alex Young looking off camera. || Screen_Shot_2019-10-01_at_4.31.11_PM.png (2764x382) [2.0 MB] || Screen_Shot_2019-10-01_at_4.31.11_PM_print.jpg (1024x141) [52.3 KB] || Screen_Shot_2019-10-01_at_4.31.11_PM_searchweb.png (320x180) [112.1 KB] || Screen_Shot_2019-10-01_at_4.31.11_PM_thm.png (80x40) [6.6 KB] || ",
            "hits": 30
        },
        {
            "id": 4737,
            "url": "https://svs.gsfc.nasa.gov/4737/",
            "result_type": "Visualization",
            "release_date": "2019-07-17T11:00:00-04:00",
            "title": "Observing Earth's Ionosphere with GOLD",
            "description": "A visualization of GOLD data observing Earth's ionosphere in ultraviolet light around the wavelength of an atomic oxygen emission. || GOLDData201903.GOLDview_O5S.clockSlate_CRTT.UHD3840.000267_print.jpg (1024x576) [70.4 KB] || GOLD_March2019_animated.gif (1042x586) [5.5 MB] || GOLDData201903.GOLDview_O5S.clockSlate_CRTT.UHD3840.000267_searchweb.png (320x180) [72.3 KB] || GOLDData201903.GOLDview_O5S.clockSlate_CRTT.UHD3840.000267_thm.png (80x40) [5.4 KB] || GOLDData201903.GOLDview_O5S.HD1080i_p10.mp4 (1920x1080) [24.0 MB] || basic (1920x1080) [0 Item(s)] || GOLDData201903.GOLDview_O5S.HD1080i_p10.webm (1920x1080) [3.1 MB] || basic (3840x2160) [0 Item(s)] || GOLDData201903.GOLDview_O5S_2160p10.mp4 (3840x2160) [72.0 MB] || ",
            "hits": 58
        },
        {
            "id": 13235,
            "url": "https://svs.gsfc.nasa.gov/13235/",
            "result_type": "Produced Video",
            "release_date": "2019-06-26T09:50:00-04:00",
            "title": "NASA's Nancy Grace Roman Space Telescope's Wide Field Instrument",
            "description": "The Nancy Grace Roman Space Telescope is a next-generation space telescope that will survey the infrared universe from beyond the orbit of the Moon. The spacecraft's giant camera, the Wide Field Instrument (WFI), will be fundamental to this exploration. The WFI features the same angular resolution as Hubble but with 100 times the field of view. Data it gathers will enable scientists to discover new and uniquely detailed information about planetary systems around other stars. The WFI will also map how matter is structured and distributed throughout the cosmos, which should ultimately allow scientists to discover the fate of the universe. Watch this video to see a simplified version of how it works.Credit: NASA's Goddard Space Flight Center.Music\" \"Horizon Ahead\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || RomanWide_Field_Still.jpg (3840x2160) [827.1 KB] || 13235_WFI_Roman_1080.mp4 (1920x1080) [92.9 MB] || 13235_WFI_Roman_1080.webm (1920x1080) [13.2 MB] || 13235_WFI_Roman_Best_1080.mp4 (1920x1080) [272.1 MB] || WFI_Roman_SRT_Captions.en_US.srt [2.5 KB] || WFI_Roman_SRT_Captions.en_US.vtt [2.5 KB] || 13235_WFI_Roman_ProRes_1920x1080_2997.mov (1920x1080) [1.6 GB] || ",
            "hits": 155
        },
        {
            "id": 13221,
            "url": "https://svs.gsfc.nasa.gov/13221/",
            "result_type": "Produced Video",
            "release_date": "2019-06-10T10:00:00-04:00",
            "title": "NASA Tech on SpaceX Falcon Heavy Launch - Media Telecon Resources",
            "description": "NASA is sending four technology missions that will help improve future spacecraft design and performance into space on the next SpaceX Falcon Heavy rocket launch. Experts will discuss these technologies, and how they complement NASA’s Moon to Mars exploration plans, during a media teleconference Monday, June 10 at 1 p.m. EDT.Audio of the teleconference will be streamed live online at: https://www.nasa.gov/liveParticipants in the briefing will be:Jim Reuter, acting associate administrator of NASA’s Space Technology Mission Directorate, will discuss how technology drives exploration to the Moon and beyond.Jill Seubert, deputy principal investigator for the Deep Space Atomic Clock at NASA’s Jet Propulsion Laboratory, will discuss how to advance exploration in deep space with a miniaturized, ultra-precise, mercury-ion atomic clock that is orders of magnitude more stable than today’s best navigation clocks.Don Cornwell, director of the Advanced Communications and Navigation Division of NASA’s Space Communications and Navigation program, will discuss how a more stable, space-based atomic clock could benefit future missions to the Moon and Mars.Christopher McLean, principal investigator for NASA’s Green Propellant Infusion Mission (GPIM) at Ball Aerospace, will discuss the demonstration of a green alternative to conventional chemical propulsion systems for next-generation launch vehicles and spacecraft. Joe Cassady, executive director for space at Aerojet Rocketdyne, will discuss the five thrusters and propulsion system aboard GPIM.Nicola Fox, director of the Heliophysics Division of NASA’s Science Mission Directorate, will discuss Space Environment Testbeds and the importance of protecting satellites from space radiation.Richard Doe, payload program manager for the Enhanced Tandem Beacon Experiment at SRI International, will discuss how a pair of NASA CubeSats will work with six satellites of the National Oceanographic and Atmospheric Administration’s (NOAA’s) COSMIC-2 mission to study disruptions of signals that pass through Earth’s upper atmosphere.To participate in the teleconference, media must contact Clare Skelly at 202-358-4273 or clare.a.skelly@nasa.gov by 10 a.m. June 10. Media questions may be submitted on Twitter during the teleconference using the hashtag #askNASA.NASA’s four missions will share a ride on the Falcon Heavy with about 20 satellites from government and research institutions that make up the Department of Defense’s Space Test Program-2 (STP-2) mission. SpaceX and the U.S. Air Force Space and Missile Systems Center, which manages STP-2, are targeting 11:30 p.m. Saturday, June 22, for launch from historic Launch Complex 39A at NASA’s Kennedy Space Center in Florida.Charged with returning astronauts to the Moon within five years, NASA’s Artemis lunar exploration plans are based on a two-phase approach: the first is focused on speed – landing astronauts on the Moon by 2024 – while the second will establish a sustained human presence on and around the Moon by 2028. We will use what we learn on the Moon to prepare to send astronauts to Mars. The technology missions on this launch will advance a variety of future exploration missions.For more information about NASA’s Moon to Mars exploration plans, visit:https://www.nasa.gov/moontomarsFor more information about the NASA technologies aboard this launch, visit:https://www.nasa.gov/spacexLearn more about NASA’s Deep Space Atomic Clock: https://www.nasa.gov/mission_pages/tdm/clock/index.htmlLearn more about NASA’s Green Propellant Infusion Mission: https://www.nasa.gov/mission_pages/tdm/green/index.htmlSPACE TEST PROGRAM-2 || ",
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        },
        {
            "id": 4702,
            "url": "https://svs.gsfc.nasa.gov/4702/",
            "result_type": "Infographic",
            "release_date": "2019-02-11T06:00:00-05:00",
            "title": "MAVEN Aerobraking to Achieve Science and Relay Orbit",
            "description": "Aerobraking plan for MAVEN.  (left) Current MAVEN orbit around Mars — 6200-km highest altitude, and an orbit period of ~4.5 hours.  (center) Aerobraking process — MAVEN performs a series of “deep dip” orbits approaching to within ~125 km of Mars at lowest altitude, causing drag from the atmosphere slow down the spacecraft.  Over roughly three-hundred and sixty orbits spanning about two months, this slowing reduces the spacecraft’s highest altitude to ~4500 km and its orbit period to ~3.5 hours.  (right) Post-aerobraking orbit, with reduced altitude and shorter orbit period. || maven_aerobraking_comp_03_print.jpg (1024x576) [90.4 KB] || MavenAerobrakingDiagram.jpg (3840x2160) [679.4 KB] || maven_aerobraking_comp_03_searchweb.png (320x180) [38.7 KB] || maven_aerobraking_comp_03_thm.png (80x40) [4.9 KB] || maven_aerobraking_comp_03.tif (3840x2160) [23.8 MB] || ",
            "hits": 48
        },
        {
            "id": 12397,
            "url": "https://svs.gsfc.nasa.gov/12397/",
            "result_type": "Produced Video",
            "release_date": "2019-02-04T12:00:00-05:00",
            "title": "Mars' Magnetic Tail",
            "description": "Mars' magnetic tail is shaped and twisted by the solar wind. || Mars_vs_Solar_Storm_1024x576.jpg (1024x576) [131.3 KB] || Mars_vs_Solar_Storm_print.jpg (1024x576) [145.9 KB] || Mars_vs_Solar_Storm.png (3840x2160) [9.8 MB] || Mars_vs_Solar_Storm_searchweb.png (320x180) [96.6 KB] || Mars_vs_Solar_Storm_thm.png (80x40) [6.4 KB] || ",
            "hits": 159
        },
        {
            "id": 12672,
            "url": "https://svs.gsfc.nasa.gov/12672/",
            "result_type": "Produced Video",
            "release_date": "2018-12-17T11:00:00-05:00",
            "title": "Saturn's Rings Are Disappearing",
            "description": "Scientists from NASA Goddard have discovered that not only are Saturn's rings younger than previously thought, but also that the rings are actually disappearing at a rapid pace through a process called \"ring rain.\" Learn more about this phenomena in this animated video.Video narrated by: Jerome HruskaMusic Provided by Killer Tracks: \"The Butterfly Effect\" - Gresby Race NashWatch this video on the NASA Goddard YouTube channel. || SaturnRingRainThumbnail1.jpg (1920x1080) [591.1 KB] || SaturnRingRainThumbnail2.jpg (1920x1080) [530.2 KB] || SaturnRingRainThumbnail1_searchweb.png (320x180) [56.1 KB] || SaturnRingRainThumbnail1_thm.png (80x40) [3.6 KB] || 12672_SaturnRingsDisappearing_Twitter.mp4 (1280x720) [27.1 MB] || 12672_SaturnRingsDisappearing_YouTubeHD.webm (1920x1080) [13.7 MB] || 12672_SaturnRingsDisappearing_YouTubeHD.mp4 (1920x1080) [187.2 MB] || 12672_SaturnRingsDisappearing_Facebook.mp4 (1920x1080) [144.4 MB] || SaturnRingsDisappearingCaptions.en_US.srt [2.3 KB] || SaturnRingsDisappearingCaptions.en_US.vtt [2.3 KB] || 12672_SaturnRingsDisappearing_MASTER.mov (1920x1080) [1.6 GB] || ",
            "hits": 321
        },
        {
            "id": 12902,
            "url": "https://svs.gsfc.nasa.gov/12902/",
            "result_type": "Produced Video",
            "release_date": "2018-10-22T10:00:00-04:00",
            "title": "The Secrets behind Earth’s Multi-colored Glow",
            "description": "What does our planet look like from space? Most are familiar with the beloved images of the blue marble or pale blue dot — Earth from 18,000 and 3.7 billion miles away, respectively. But closer to home, within the nearest region of space, you might encounter an unfamiliar sight. If you peer down on Earth from just 300 miles above the surface, near the orbit of the International Space Station, you can see vibrant swaths of red and green or purple and yellow light emanating from the upper atmosphere. This is airglow. Airglow occurs when atoms and molecules in the upper atmosphere, excited by sunlight, emit light in order to shed their excess energy. Or, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, they eject a particle of light — called a photon — in order to relax again. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is energized by day-to-day solar radiation. || ",
            "hits": 220
        },
        {
            "id": 13096,
            "url": "https://svs.gsfc.nasa.gov/13096/",
            "result_type": "Produced Video",
            "release_date": "2018-10-18T13:00:00-04:00",
            "title": "ICON Pre-Launch Live Shots",
            "description": "B-roll and canned interviews will be added on Wednesday, Oct 24 by 6:00pm || ICON_WebBanner_2018.jpg (3792x597) [550.7 KB] || ICON_WebBanner_2018_print.jpg (1024x161) [101.5 KB] || ICON_WebBanner_2018_searchweb.png (320x180) [119.7 KB] || ICON_WebBanner_2018_thm.png (80x40) [6.5 KB] || ",
            "hits": 34
        },
        {
            "id": 12947,
            "url": "https://svs.gsfc.nasa.gov/12947/",
            "result_type": "Produced Video",
            "release_date": "2018-10-16T12:00:00-04:00",
            "title": "Launching an ICON",
            "description": "The Ionospheric Connection Explorer will explore the mysteries of where Earth meets space. || STORYCOVER_ICON_Image_Portrait16x9_1024x576.jpg (1024x576) [187.1 KB] || STORYCOVER_ICON_Image_Portrait16x9.jpg (2550x1434) [637.0 KB] || STORYCOVER_NEW_ICON_Image_Portrait.jpg (2550x3300) [707.1 KB] || STORYCOVER_ICON_Image_Portrait16x9_searchweb.png (320x180) [82.4 KB] || STORYCOVER_ICON_Image_Portrait16x9_thm.png (80x40) [5.7 KB] || ",
            "hits": 41
        },
        {
            "id": 12986,
            "url": "https://svs.gsfc.nasa.gov/12986/",
            "result_type": "Produced Video",
            "release_date": "2018-07-23T11:00:00-04:00",
            "title": "Mars Proton Aurora",
            "description": "On Earth, the northern and southern lights occur when the solar wind (electrically charged particles from the Sun) follow our planet's geomagnetic field lines to the poles and collide with the upper atmosphere. Mars lacks a global magnetic field, so instead the solar wind piles up in front of Mars in a bow shock, which blocks charged particles from reaching the bulk of the atmosphere. However, in a process first observed by the MAVEN mission, some solar wind protons can slip past the bow shock by first bonding with electrons from the Mars upper atmosphere to form hydrogen atoms. Because these hydrogen atoms are electrically neutral, they can pass through the bow shock and go on to create an ultraviolet proton aurora on the dayside of Mars.Learn more about MAVEN's observation of a proton aurora at Mars. || ",
            "hits": 132
        },
        {
            "id": 12736,
            "url": "https://svs.gsfc.nasa.gov/12736/",
            "result_type": "Produced Video",
            "release_date": "2018-06-04T12:00:00-04:00",
            "title": "Building Blocks for Surviving Titan",
            "description": "Saturn’s moon, Titan, may have a building block for potential cell membranes. || PIA14909_16x9.jpg (1024x576) [86.6 KB] || PIA14909_16x9_print.jpg (1024x576) [86.1 KB] || PIA14909_16x9_searchweb.png (320x180) [34.1 KB] || PIA14909_16x9_thm.png (80x40) [3.2 KB] || ",
            "hits": 133
        },
        {
            "id": 12963,
            "url": "https://svs.gsfc.nasa.gov/12963/",
            "result_type": "Produced Video",
            "release_date": "2018-06-02T15:00:00-04:00",
            "title": "Airglow Imagery",
            "description": "Airglow occurs when atoms and molecules in the upper atmosphere, excited by sunlight, emit light in order to shed their excess energy. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is sparked by day-to-day solar radiation. Airglow carries information on the upper atmosphere’s temperature, density, and composition, but it also helps us trace how particles move through the region itself. Vast, high-altitude winds sweep through the ionosphere, pushing its contents around the globe — and airglow’s subtle dance follows their lead, highlighting global patterns. || ",
            "hits": 847
        },
        {
            "id": 12973,
            "url": "https://svs.gsfc.nasa.gov/12973/",
            "result_type": "Infographic",
            "release_date": "2018-06-01T23:00:00-04:00",
            "title": "NASA's Heliophysics Fleet",
            "description": "Heliophysics encompasses science that improves our un­derstanding of fundamental physical processes throughout the solar system, and enables us to understand how the Sun, as the major driver of the energy throughout the solar system, impacts our technological society. The scope of heliophysics is vast, spanning from the Sun’s interior to Earth’s upper atmosphere, throughout interplanetary space, to the edges of the heliosphere, where the solar wind interacts with the local interstellar medium. Heliophysics incorporates studies of the interconnected elements in a single system that produces dynamic space weather and that evolves in response to solar, planetary, and interstellar conditions. || ",
            "hits": 36
        },
        {
            "id": 12960,
            "url": "https://svs.gsfc.nasa.gov/12960/",
            "result_type": "Infographic",
            "release_date": "2018-05-31T19:00:00-04:00",
            "title": "Ionosphere Graphics",
            "description": "Stretching from roughly 50 to 400 miles above Earth’s surface, the ionosphere is an electrified layer of the upper atmosphere, generated by extreme ultraviolet radiation from the Sun. It’s neither fully Earth nor space, and instead, reacts to both terrestrial weather below and solar energy streaming in from above, forming a complex space weather system of its own. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground. Positioned on the edge of space and intermingled with the neutral atmosphere, the ionosphere’s response to conditions on Earth and in space is difficult to pin down. || ",
            "hits": 442
        },
        {
            "id": 4641,
            "url": "https://svs.gsfc.nasa.gov/4641/",
            "result_type": "Infographic",
            "release_date": "2018-05-03T00:00:00-04:00",
            "title": "Terrestrial Atmosphere ITM (Ionosphere, Thermosphere, Mesosphere) Processes",
            "description": "Large image version || Terrestrial_Atmos_ITM_Processes.jpg (3355x2205) [1.2 MB] || Terrestrial_Atmos_ITM_Processes_searchweb.png (320x180) [65.0 KB] || Terrestrial_Atmos_ITM_Processes_thm.png (80x40) [7.1 KB] || This graphic presents an overview of the physical processes that have been identified in Earth's upper atmosphere. || ",
            "hits": 151
        },
        {
            "id": 12823,
            "url": "https://svs.gsfc.nasa.gov/12823/",
            "result_type": "Produced Video",
            "release_date": "2018-02-05T12:00:00-05:00",
            "title": "Where Earth Meets Space",
            "description": "NASA’s newest mission, GOLD, will explore the ever-changing boundary between Earth and space. || 12827_GOLD_SES14satellite.00300_print.png (1920x1080) [2.2 MB] || 12827_GOLD_SES14satellite.00300_print_1024x576.jpg (1024x576) [122.0 KB] || 12827_GOLD_SES14satellite.00300_print_print.jpg (1024x576) [133.7 KB] || 12827_GOLD_SES14satellite.00300_print_searchweb.png (320x180) [82.5 KB] || 12827_GOLD_SES14satellite.00300_print_thm.png (80x40) [5.7 KB] || ",
            "hits": 140
        },
        {
            "id": 4617,
            "url": "https://svs.gsfc.nasa.gov/4617/",
            "result_type": "Visualization",
            "release_date": "2018-01-31T14:00:00-05:00",
            "title": "Interface to Space: The Equatorial Fountain",
            "description": "Visualization illustrating the Fountain Effect of ions in the near-Earth electric and magnetic fields. || IRIConceptual.Limb2PullOut_OionFountainIGRF.noslate_CRTT.HD1080i.000660_print.jpg (1024x576) [114.5 KB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.noslate_CRTT.HD1080i.000660_searchweb.png (320x180) [87.8 KB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.noslate_CRTT.HD1080i.000660_thm.png (80x40) [7.2 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || IRIConceptual.Limb2PullOut_OionFountainIGRF.HD1080i_p30.mp4 (1920x1080) [32.1 MB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.HD1080i_p30.webm (1920x1080) [4.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || IRIConceptual.Limb2PullOut_OionFountainIGRF_2160p30.mp4 (3840x2160) [96.1 MB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.HD1080i_p30.mp4.hwshow [221 bytes] || ",
            "hits": 173
        },
        {
            "id": 4600,
            "url": "https://svs.gsfc.nasa.gov/4600/",
            "result_type": "Visualization",
            "release_date": "2018-01-31T00:00:00-05:00",
            "title": "Sixty Years of Earth Observations: from Explorer-1 (1958) to CYGNSS (2017)",
            "description": "Earth observing spacecraft from Explorer-1 to CYGNSSThis video is also available on our YouTube channel. || explorer1_68_1920x1080.09999_print.jpg (1024x576) [149.7 KB] || explorer1_68_1920x1080.09999_searchweb.png (320x180) [76.7 KB] || explorer1_68_1920x1080.09999_thm.png (80x40) [5.8 KB] || explorer1_68_1920x1080_p60.mp4 (1920x1080) [73.6 MB] || firsts (1920x1080) [0 Item(s)] || explorer1_68_1920x1080_p30.webm (1920x1080) [35.9 MB] || explorer1_68_1920x1080_p30.mp4 (1920x1080) [124.5 MB] || explorer1_68_1920x1080.1080p30.mp4 (1920x1080) [128.5 MB] || 9600x3240_16x9_30p (9600x3240) [0 Item(s)] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || explorer1_68_3840x2160_p30.mp4 (3840x2160) [461.5 MB] || ",
            "hits": 78
        },
        {
            "id": 12825,
            "url": "https://svs.gsfc.nasa.gov/12825/",
            "result_type": "Infographic",
            "release_date": "2018-01-24T12:00:00-05:00",
            "title": "GOLD Resources",
            "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. The more we know about the fundamental physics of this region of space, the more we can protect our assets there.Gathering observations from geostationary orbit above the Western Hemisphere, GOLD measures the temperature and composition of neutral gases in Earth’s thermosphere. This part of the atmosphere co-mingles with the ionosphere, which is made up of charged particles. Both the Sun from above and terrestrial weather from below can change the types, numbers, and characteristics of the particles found here — and GOLD helps track those changes.Activity in this region is responsible for a variety of key space weather events. GOLD scientists are particularly interested in the cause of dense, unpredictable bubbles of charged gas that appear over the equator and tropics, sometimes causing communication problems. As we discover the very nature of the Sun-Earth interaction in this region, the mission could ultimately lead to ways to improve forecasts of such space weather and mitigate its effects. || ",
            "hits": 154
        },
        {
            "id": 12833,
            "url": "https://svs.gsfc.nasa.gov/12833/",
            "result_type": "Produced Video",
            "release_date": "2018-01-24T12:00:00-05:00",
            "title": "GOLD Media Telecon",
            "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. On January 25, 2018, the mission will launch as NASA's first-ever hosted payload.Speakers for the January 24, 2018 media telecon about the mission include:Richard Eastes, Principal Investigator, Laboratory for Atmospheric and Space Physics at the University of Colorado BoulderElsayed Talaat, Heliophysics Chief Scientist, NASA HeadquartersSusan Batiste, Systems Engineer, LASP/CUKatelynn Greer, Research Scientist, LASP/CUReplay information will be available until January 31, 2018 noon ET, via: Toll free, from within the U.S.: 1-866-469-5761 \u2028Toll: 203-369-1460 || ",
            "hits": 40
        },
        {
            "id": 40345,
            "url": "https://svs.gsfc.nasa.gov/gallery/gold/",
            "result_type": "Gallery",
            "release_date": "2018-01-17T00:00:00-05:00",
            "title": "GOLD – Global-scale Observations of the Limb and Disk",
            "description": "NASA’s Global-scale Observations of the Limb and Disk (GOLD) mission focuses on two parts of Earth’s upper atmosphere stretching from about 50 to 400 miles in altitude — the neutral layer called the thermosphere, and the electrically charged particles that make up the ionosphere. From its vantage point on a commercial communications satellite in geostationary orbit, the GOLD instrument makes hemisphere-wide observations of the ionosphere about every 30 minutes. This unprecedented birds-eye view is giving scientists new insights into how this region changes.\n\nGOLD launched on Jan. 25, 2018, from the Guiana Space Centre in Kourou, French Guiana, aboard an Ariane 5 rocket as a hosted payload on the SES-14 commercial satellite.\n\nLearn more: https://science.nasa.gov/mission/gold/",
            "hits": 159
        },
        {
            "id": 12817,
            "url": "https://svs.gsfc.nasa.gov/12817/",
            "result_type": "Produced Video",
            "release_date": "2018-01-05T13:00:00-05:00",
            "title": "Why NASA Is Exploring The Edge Of Our Planet",
            "description": "The Global-scale Observations of the Limb and Disk, or GOLD, instrument launches aboard a commercial communications satellite in January 2018 to inspect the dynamic intermingling of space and Earth’s uppermost atmosphere. Together, GOLD and another NASA mission, Ionospheric Connection Explorer spacecraft, or ICON, will provide the most comprehensive of Earth’s upper atmosphere we’ve ever had.Above the ozone layer, the ionosphere is a part of Earth’s atmosphere where particles have been cooked into a sea of electrically-charged electrons and ions by the Sun’s radiation. The ionosphere is co-mingled with the very highest — and quite thin — layers of Earth’s neutral upper atmosphere, making this region an area that is constantly in flux undergoing the push-and-pull between Earth’s conditions and those in space. Increasingly, these layers of near-Earth space are part of the human domain, as it’s home not only to astronauts, but to radio signals used to guide airplanes and ships, and satellites that provide our communications and GPS systems. Understanding the fundamental processes that govern our upper atmosphere and ionosphere is crucial to improve situational awareness that helps protect astronauts, spacecraft and humans on the ground.GOLD, in geostationary orbit over the Western Hemisphere, will build up a full-disk view of the ionosphere and upper atmosphere every half hour, providing detailed large-scale measurements of related processes — a cadence which makes it the first mission to be able to monitor the true weather of the upper atmosphere. GOLD is also able to focus in on a tighter region and scan more quickly, to complement additional research plans as needed. || ",
            "hits": 131
        },
        {
            "id": 12820,
            "url": "https://svs.gsfc.nasa.gov/12820/",
            "result_type": "Produced Video",
            "release_date": "2018-01-04T00:00:00-05:00",
            "title": "Going for GOLD: Exploring the Interface to Space",
            "description": "Going for GOLD: Exploring the Interface to Space || 12820_GOLD_FB_Live.00001_print.jpg (1024x576) [125.3 KB] || 12820_GOLD_FB_Live.00001_searchweb.png (320x180) [84.7 KB] || 12820_GOLD_FB_Live.00001_thm.png (80x40) [6.6 KB] || 12820_GOLD_FB_Live.mp4 (1280x720) [5.1 GB] || 12820_GOLD_FB_Live.mov (1280x720) [41.9 GB] || 12820_GOLD_FB_Live.webm (960x540) [1.7 GB] || 12820_GOLD_FB_Live.en_US.srt [119.6 KB] || 12820_GOLD_FB_Live.en_US.vtt [112.9 KB] || ",
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        {
            "id": 4601,
            "url": "https://svs.gsfc.nasa.gov/4601/",
            "result_type": "Visualization",
            "release_date": "2017-12-18T11:00:00-05:00",
            "title": "Jupiter Quasi-Quadrennial Oscillation",
            "description": "Climate patterns on Jupiter can have striking similarities to those on Earth, making the gas giant a natural laboratory for understanding planetary atmospheres. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Lights,\" \"Times Waits,\" \"The Space Between\" || JupiterQQOpreview.jpg (1920x1080) [456.5 KB] || TWITTER_720_4601_Jupiter_QQO_Master_APR_twitter_720.mp4 (1280x720) [37.7 MB] || 4601_Jupiter_QQO_Master.webm (960x540) [72.7 MB] || FACEBOOK_720_4601_Jupiter_QQO_Master_APR_facebook_720.mp4 (1280x720) [218.0 MB] || YOUTUBE_HQ_4601_Jupiter_QQO_Master_APR_youtube_hq.mov (1920x1080) [875.9 MB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.srt [3.8 KB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.vtt [3.8 KB] || 4601_Jupiter_QQO_Master_APR.mov (1920x1080) [2.4 GB] || ",
            "hits": 190
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        {
            "id": 12783,
            "url": "https://svs.gsfc.nasa.gov/12783/",
            "result_type": "Infographic",
            "release_date": "2017-12-06T12:45:00-05:00",
            "title": "SuperTIGER Ready to Fly Again in Study of Heavy Cosmic Rays",
            "description": "SuperTIGER team members Brian Rauch, Jason Link and Nathan Walsh join NASA Blueshift's Sara Mitchell for a Skype conversation in November 2017 about the instrument's science, technology and upcoming launch from McMurdo Station, Antarctica. Credit: NASA's Goddard Space Flight CenterComplete transcript available. || SuperTIGER_Skype_Still.png (1280x720) [1.2 MB] || SuperTIGER_Skype2.webm (1280x720) [135.1 MB] || SuperTIGER_Skype2.mp4 (1280x720) [608.6 MB] || SuperTIGER_Skype2_SRT_Captions.en_US.srt [22.5 KB] || SuperTIGER_Skype2_SRT_Captions.en_US.vtt [22.5 KB] || SuperTIGER_Skype2_best.mp4 (1280x720) [1.2 GB] || ",
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        {
            "id": 4595,
            "url": "https://svs.gsfc.nasa.gov/4595/",
            "result_type": "Visualization",
            "release_date": "2017-11-27T10:00:00-05:00",
            "title": "Mapping Particle Injections in Earth's Magnetosphere",
            "description": "A view from above the northern hemisphere of particle injection propagation constructed from their respective satellite detections.  Distinct injections, and their detection by satellites, are represented by different colors. || MagnetosphereMultiMission.top.GSE.AU.clockSlate_EarthTarget.HD1080i.01200_print.jpg (1024x576) [115.4 KB] || MagnetosphereMultiMission.top.GSE.AU.clockSlate_EarthTarget.HD1080i.01200_searchweb.png (320x180) [82.7 KB] || MagnetosphereMultiMission.top.GSE.AU.clockSlate_EarthTarget.HD1080i.01200_thm.png (80x40) [6.3 KB] || TopView (1920x1080) [0 Item(s)] || MagnetosphereMultiMission.top.HD1080i_p30.mp4 (1920x1080) [29.7 MB] || MagnetosphereMultiMission.top.HD1080i_p30.webm (1920x1080) [6.1 MB] || TopView (3840x2160) [0 Item(s)] || MagnetosphereMultiMission.top.UHD3840_2160p30.mp4 (3840x2160) [93.0 MB] || MagnetosphereMultiMission.top.HD1080i_p30.mp4.hwshow [207 bytes] || ",
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            "id": 4594,
            "url": "https://svs.gsfc.nasa.gov/4594/",
            "result_type": "Visualization",
            "release_date": "2017-10-31T10:00:00-04:00",
            "title": "ICON Scans the Ionosphere",
            "description": "ICON orbits Earth at 575 kilometers altitude, measuring the composition and motions of the ionosphere. || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_print.jpg (1024x576) [105.7 KB] || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_searchweb.png (320x180) [63.8 KB] || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_thm.png (80x40) [5.0 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.mp4 (1920x1080) [76.4 MB] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.webm (1920x1080) [10.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || IRIDaily.limbwICON_OionHwindIGRF.UHD3840_2160p30.mp4 (3840x2160) [217.4 MB] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.mp4.hwshow [210 bytes] || ",
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        {
            "id": 12699,
            "url": "https://svs.gsfc.nasa.gov/12699/",
            "result_type": "Produced Video",
            "release_date": "2017-10-18T14:00:00-04:00",
            "title": "Meet ICON: NASA’s Airglow Explorer",
            "description": "Music credit: Design Principle by Wayne RobertsComplete transcript available. || iss_composite_test_182.jpg (4256x2832) [12.8 MB] || iss_composite_test_182_searchweb.png (320x180) [99.0 KB] || iss_composite_test_182_thm.png (80x40) [6.2 KB] || LARGE_MP4-12699_ICON_Overview_V2__large.mp4 (1920x1080) [148.3 MB] || NASA_TV-12699_ICON_Overview_V2_.mpeg (1280x720) [494.2 MB] || APPLE_TV-12699_ICON_Overview_V2__appletv.m4v (1280x720) [75.3 MB] || YOUTUBE_1080-12699_ICON_Overview_V2__youtube_1080.mp4 (1920x1080) [234.8 MB] || PRORES_B-ROLL-12699_ICON_Overview_V2__prores.mov (1280x720) [1.9 GB] || YOUTUBE_HQ-12699_ICON_Overview_V2__youtube_hq.mov (1920x1080) [539.3 MB] || 12699_ICON_Overview_V2_.mov (1920x1080) [3.7 GB] || LARGE_MP4-12699_ICON_Overview_V2__large.webm (1920x1080) [16.3 MB] || APPLE_TV-12699_ICON_Overview_V2__appletv_subtitles.m4v (1280x720) [75.3 MB] || 12699_ICON_Overview_V2.en_US.srt [2.4 KB] || 12699_ICON_Overview_V2.en_US.vtt [2.5 KB] || NASA_PODCAST-12699_ICON_Overview_V2__ipod_sm.mp4 (320x240) [25.4 MB] || 12699_ICON_Overview_V2__lowres.mp4 (480x272) [20.3 MB] || ",
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        {
            "id": 30901,
            "url": "https://svs.gsfc.nasa.gov/30901/",
            "result_type": "Hyperwall Visual",
            "release_date": "2017-10-03T00:00:00-04:00",
            "title": "Cassini's Final Image",
            "description": "Cassini's final image || PIA21895_print.jpg (1024x1030) [71.7 KB] || PIA21895_searchweb.png (320x180) [29.7 KB] || PIA21895_thm.png (80x40) [2.5 KB] || PIA21895.tif (505x508) [190.2 KB] || cassinis-final-image.hwshow [260 bytes] || ",
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        {
            "id": 40338,
            "url": "https://svs.gsfc.nasa.gov/gallery/parker-solar-probe/",
            "result_type": "Gallery",
            "release_date": "2017-09-22T00:00:00-04:00",
            "title": "Parker Solar Probe",
            "description": "On a mission to “touch the Sun,” NASA's Parker Solar Probe became the first spacecraft to fly through the corona — the Sun’s upper atmosphere — passing within 3.8 million miles of the solar surface during its closest approaches. Parker Solar Probe flies through the corona at speeds up to 430,000 mph taking measurements to help scientists better understand the fundamental drivers of solar activity and space weather events that can impact life on Earth. Facing brutal heat and radiation conditions, Parker Solar Probe employs four instrument suites designed to study electric and magnetic fields, plasma, waves and energetic particles, as well as image the solar wind, the constant stream of material released by the Sun. \n\nParker Solar Probe launched on Aug. 12, 2018, from the Cape Canaveral Air Force Station.\n\nLearn more: https://science.nasa.gov/mission/parker-solar-probe/",
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        {
            "id": 12602,
            "url": "https://svs.gsfc.nasa.gov/12602/",
            "result_type": "Produced Video",
            "release_date": "2017-08-02T10:35:00-04:00",
            "title": "NASA Set To Launch Shoebox-sized Satellite Studying Earth's Upper Atmosphere",
            "description": "NASA scientists and engineers named their new CubeSat after the mythological Norse god of the dawn. Now, just days from launch, they are confident the shoebox-sized satellite Dellingr will live up to its name and inaugurate a new era for scientists wanting to use small, highly reliable satellites to carry out important, and in some cases, never-before-tried science.Dellingr will study how the ionosphere, a region in Earth’s upper atmosphere, interacts with the Sun. Before launch, Dellingr is required to visit to the Magnetic Test Facility at NASA Goddard to test the spacecraft's magnetometers - key instruments for measuring the direction and strength of the magnetic fields that surround Earth.The spacecraft is scheduled to launch this August aboard a SpaceX Falcon 9 rocket to the International Space Station where it will be deployed later into a low-Earth orbit. || ",
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        {
            "id": 40335,
            "url": "https://svs.gsfc.nasa.gov/gallery/interfaceto-space/",
            "result_type": "Gallery",
            "release_date": "2017-06-23T00:00:00-04:00",
            "title": "Interface to Space",
            "description": "The ionosphere is layer of the upper atmosphere (60-1000 km up) where the neutral atoms and molecules of the lower atmosphere transition to the plasma of space.",
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        {
            "id": 12523,
            "url": "https://svs.gsfc.nasa.gov/12523/",
            "result_type": "Produced Video",
            "release_date": "2017-02-23T10:00:00-05:00",
            "title": "Aurora Imagery from Poker Flats",
            "description": "The northern lights were seen over Alaska the night of Feb. 16, 2017 at the the Poker Flat Research Range north of Fairbanks. Credit: NASA/Terry Zaperach || PFAurora2.gif (1200x800) [1.5 MB] || PFAurora2_searchweb.png (320x180) [57.6 KB] || PFAurora2_thm.png (80x40) [4.7 KB] || ",
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}