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    "results": [
        {
            "id": 14492,
            "url": "https://svs.gsfc.nasa.gov/14492/",
            "result_type": "Produced Video",
            "release_date": "2024-01-05T08:50:00-05:00",
            "title": "XRISM Reveals Its First Look at X-ray Cosmos",
            "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ",
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        {
            "id": 14381,
            "url": "https://svs.gsfc.nasa.gov/14381/",
            "result_type": "B-Roll",
            "release_date": "2023-07-13T15:00:00-04:00",
            "title": "Webb Telescope Mission Overview 2023",
            "description": "A brief overview of the James Webb Space Telescope mission from its construction, launch, and complex unfolding to the incredible science it achieves. || ",
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        {
            "id": 14251,
            "url": "https://svs.gsfc.nasa.gov/14251/",
            "result_type": "B-Roll",
            "release_date": "2022-12-06T00:00:00-05:00",
            "title": "James Webb Mirror Alignment Completion and First Light Staff Meeting Results B-Roll",
            "description": "B-Roll footage of engineers and scientists completing the mirror alignment on the James Webb Space Telescope an a staff meeting to witness the final result of the tests at the Space Telescop Science Institute in Baltimore, MD. || ",
            "hits": 35
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        {
            "id": 31186,
            "url": "https://svs.gsfc.nasa.gov/31186/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-08-09T00:00:00-04:00",
            "title": "Webb's Science Mission Begins: First Light Images",
            "description": "The Cartwheel Galaxy, a rare ring galaxy once shrouded in dust and mystery, has been unveiled by the imaging capabilities of NASA’s James Webb Space Telescope. The galaxy, which formed as a result of a collision between a large spiral galaxy and another smaller galaxy, not only retained a lot of its spiral character, but has also experienced massive changes throughout its structure. Webb’s high-precision instruments resolved individual stars and star-forming regions within the Cartwheel, and revealed the behavior of the black hole within its galactic center. These new details provide a renewed understanding of a galaxy in the midst of a slow transformation. || cartwheel_348_print.jpg (1024x576) [152.0 KB] || cartwheel_348.png (3840x2160) [9.1 MB] || webbs-science-mission-begins-first-light-images-cartwheel-galaxy.hwshow [314 bytes] || ",
            "hits": 73
        },
        {
            "id": 31188,
            "url": "https://svs.gsfc.nasa.gov/31188/",
            "result_type": "Hyperwall Visual",
            "release_date": "2022-08-09T00:00:00-04:00",
            "title": "Webb's Science Mission Begins: First Light Images As Compared to Hubble",
            "description": "NGC 3372: Eta Carinae Nebula || eta-carina-cliffs_1.00001_print.jpg (1024x576) [111.2 KB] || eta-carina-cliffs_1.00001_searchweb.png (320x180) [56.4 KB] || eta-carina-cliffs_1.00001_thm.png (80x40) [4.5 KB] || eta-carina-cliffs_1.mp4 (1920x1080) [17.2 MB] || eta-carina-cliffs_1.webm (1920x1080) [2.2 MB] || ",
            "hits": 97
        },
        {
            "id": 13987,
            "url": "https://svs.gsfc.nasa.gov/13987/",
            "result_type": "Produced Video",
            "release_date": "2021-11-05T17:00:00-04:00",
            "title": "Landsat 9 First Light Images",
            "description": "The first data from Landsat 9, of Australia's Kimberley Coast in Western Australia, shows off the capabilities of the two instruments on the spacecraft. This image, from the Operational Land Imager 2, or OLI-2, was acquired on Oct. 31, 2021. Although similar in design to its predecessor Landsat 8, the improvements to Landsat 9 allow it to detect more subtle differences, especially over darker areas like water or the dense mangrove forests along the coast. || L9_Australia_20211031_p109r070-lrg.jpg (7621x7811) [24.2 MB] || L9_Australia_20211031_p109r070-lrg_searchweb.png (320x180) [106.1 KB] || L9_Australia_20211031_p109r070-lrg_thm.png (80x40) [7.1 KB] || L9_Australia_20211031_p109r070-lrg.tif (7621x7811) [340.6 MB] || ",
            "hits": 69
        },
        {
            "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": 260
        },
        {
            "id": 12803,
            "url": "https://svs.gsfc.nasa.gov/12803/",
            "result_type": "Produced Video",
            "release_date": "2017-12-13T09:00:00-05:00",
            "title": "James Webb Space Telescope: An Overview",
            "description": "Complete transcript available. || YOUTUBE_1080_12803_JWST_An_Overview_youtube_1080.00001_print.jpg (1024x576) [49.2 KB] || YOUTUBE_1080_12803_JWST_An_Overview_youtube_1080.00001_searchweb.png (320x180) [10.1 KB] || YOUTUBE_1080_12803_JWST_An_Overview_youtube_1080.00001_thm.png (80x40) [2.5 KB] || 12803-_An_Overview_2018.webm (1920x1080) [22.0 MB] || 12803-James_Webb_Space_Telescope__An_Overview_6.25_large.mp4 (1920x1080) [204.6 MB] || 12803-James_Webb_Space_Telescope__An_Overview_6.25_youtube_hq.mov (1920x1080) [746.7 MB] || YOUTUBE_1080_12803-James_Webb_Space_Telescope__An_Overview_6.25_youtube_1080.mp4 (1920x1080) [390.8 MB] || 12803-_An_Overview_2018.en_US.srt [2.8 KB] || 12803-_An_Overview_2018.en_US.vtt [2.8 KB] || ",
            "hits": 317
        },
        {
            "id": 3888,
            "url": "https://svs.gsfc.nasa.gov/3888/",
            "result_type": "Visualization",
            "release_date": "2011-11-30T00:00:00-05:00",
            "title": "NPP/VIIRS First Light Image",
            "description": "On November 21, 2011 the first measurements from the Visible Infrared Imager Radiometer Suite (VIIRS) instrument on NASA's National Polar-orbiting Operational Environmental Satellite System Preparatory Project (NPP) satellite were acquired. These still images show one of the instrument's data swaths. The first image shows the data swath wrapped to a globe for context. The second image shows the data swath in a cartesian projection.This image was produced using VIIRS M-bands SVM05, SVM04, SVM03 (red, green, blue) at 1000 meter resolution. || ",
            "hits": 56
        },
        {
            "id": 30282,
            "url": "https://svs.gsfc.nasa.gov/30282/",
            "result_type": "Hyperwall Visual",
            "release_date": "2011-11-24T12:00:00-05:00",
            "title": "NPP VIIRS",
            "description": "The Visible Infrared Imager Radiometer Suite (VIIRS) on the United States’ newest Earth-observing satellite, NPP, acquired its first measurements on November 21, 2011. This image above shows a broad swath of eastern North America from the Great Lakes to Cuba. || ",
            "hits": 44
        },
        {
            "id": 10745,
            "url": "https://svs.gsfc.nasa.gov/10745/",
            "result_type": "Produced Video",
            "release_date": "2011-06-07T09:00:00-04:00",
            "title": "SDO Catches Surf Waves on the Sun",
            "description": "Scientists have spotted the iconic surfer's wave rolling through the atmosphere of the sun. This makes for more than just a nice photo-op: the waves hold clues as to how energy moves through that atmosphere, known as the corona. Since scientists know how these kinds of waves — initiated by a Kelvin-Helmholtz instability if you're being technical — disperse energy in the water, they can use this information to better understand the corona. This in turn, may help solve an enduring mystery of why the corona is thousands of times hotter than originally expected.Kelvin-Helmholtz instabilities occur when two fluids of different densities or different speeds flow by each other. In the case of ocean waves, that's the dense water and the lighter air. As they flow past each other, slight ripples can be quickly amplified into the giant waves loved by surfers. In the case of the solar atmosphere, which is made of a very hot and electrically charged gas called plasma, the two flows come from an expanse of plasma erupting off the sun's surface as it passes by plasma that is not erupting. The difference in flow speeds and densities across this boundary sparks the instability that builds into the waves. In order to confirm this description, the team developed a computer model to see what takes place in the region. Their model showed that these conditions could indeed lead to giant surfing waves rolling through the corona. Seeing the big waves suggests they can cascade down to smaller forms of turbulence too. Scientists believe that the friction created by turbulence — the simple rolling of material over and around itself — could help add heating energy to the corona. The analogy is the way froth at the top of a surfing wave provides friction that will heat up the wave. || ",
            "hits": 65
        },
        {
            "id": 10748,
            "url": "https://svs.gsfc.nasa.gov/10748/",
            "result_type": "Produced Video",
            "release_date": "2011-04-21T09:00:00-04:00",
            "title": "SDO: Year One",
            "description": "April 21, 2011 marks the one-year anniversary of the Solar Dynamics Observatory (SDO) First Light press conference, where NASA revealed the first images taken by the spacecraft.In the last year, the sun has gone from its quietest period in years to the activity marking the beginning of solar cycle 24. SDO has captured every moment with a level of detail never-before possible. The mission has returned unprecedented images of solar flares, eruptions of prominences, and the early stages of coronal mass ejections (CMEs). In this video are some of the most beautiful, interesting, and mesmerizing events seen by SDO during its first year.In the order they appear in the video the events are:1. Prominence Eruption from AIA in 304 Ångstroms on March 30, 20102. Cusp Flow from AIA in 171 Ångstroms on February 14, 20113. Prominence Eruption from AIA in 304 Ångstroms on February 25, 20114. Cusp Flow from AIA in 304 Ångstroms on February 14, 20115. Merging Sunspots from HMI in Continuum on October 24-28, 20106. Prominence Eruption and active region from AIA in 304 Ångstroms on April 30, 20107. Solar activity and plasma loops from AIA in 171 Ångstroms on March 4-8, 20118. Flowing plasma from AIA in 304 Ångstroms on April 19, 20109. Active regions from HMI in Magnetogram on March 10, 201110. Filament eruption from AIA in 304 Ångstroms on December 6, 201011. CME start from AIA in 211 Ångstroms on March 8, 201112. X2 flare from AIA in 304 Ångstroms on February 15, 2011 || ",
            "hits": 78
        },
        {
            "id": 1119,
            "url": "https://svs.gsfc.nasa.gov/1119/",
            "result_type": "Visualization",
            "release_date": "2000-04-19T12:00:00-04:00",
            "title": "First Light Image from MODIS (First Draft)",
            "description": "Viewing the very first image from MODIS (first draft) || Pan down the MODIS first light image || a001119.00005_print.png (720x480) [419.3 KB] || a001119_thm.png (80x40) [4.4 KB] || a001119_pre.jpg (320x238) [8.5 KB] || a001119_pre_searchweb.jpg (320x180) [48.2 KB] || a001119.webmhd.webm (960x540) [9.0 MB] || a001119.dv (720x480) [122.9 MB] || a001119.mp4 (640x480) [6.6 MB] || a001119.mpg (352x240) [4.8 MB] || ",
            "hits": 10
        },
        {
            "id": 1120,
            "url": "https://svs.gsfc.nasa.gov/1120/",
            "result_type": "Visualization",
            "release_date": "2000-04-19T12:00:00-04:00",
            "title": "First Light Image from MODIS (Second Draft)",
            "description": "Viewing the very first image from MODIS (second draft) || Pan down the MODIS first light image || a001120.00005_print.png (720x480) [417.4 KB] || a001120_pre.jpg (320x238) [9.1 KB] || a001120_thm.png (80x40) [5.0 KB] || a001120_pre_searchweb.jpg (320x180) [52.7 KB] || a001120.webmhd.webm (960x540) [24.1 MB] || a001120.dv (720x480) [363.0 MB] || a001120.mp4 (640x480) [19.7 MB] || a001120.mpg (352x240) [14.3 MB] || ",
            "hits": 7
        }
    ]
}