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        {
            "id": 14861,
            "url": "https://svs.gsfc.nasa.gov/14861/",
            "result_type": "Produced Video",
            "release_date": "2025-07-07T10:00:00-04:00",
            "title": "NASA's Habitable Worlds Observatory Will Search For Life",
            "description": "No description available.",
            "hits": 509
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        {
            "id": 14775,
            "url": "https://svs.gsfc.nasa.gov/14775/",
            "result_type": "Produced Video",
            "release_date": "2025-01-29T10:00:00-05:00",
            "title": "Roman Instrument Posters",
            "description": "NASA’s Roman Coronagraph Instrument will greatly advance our ability to directly image exoplanets, or planets and disks around other stars.Credit: NASA/JPLDigital version of poster with back panelPress version of poster with back panel. FOR PRINT || CGI_Digital_12x18.jpg (1837x2737) [1.1 MB] || CGI_Digital_12x18-1.jpg (3663x5475) [5.7 MB] || CGI_Digital_12x18-1.png (3663x5475) [39.5 MB] || ",
            "hits": 45
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        {
            "id": 14757,
            "url": "https://svs.gsfc.nasa.gov/14757/",
            "result_type": "Produced Video",
            "release_date": "2025-01-21T00:00:00-05:00",
            "title": "Roman Space Telescope's Coronagraph Instrument Integration into the Instrument Carrier",
            "description": "The Coronagraph, one of two science instruments, finds it home in NASA's Nancy Grace Roman Telescope Instrument Carrier.Designed and built by NASA’s Jet Propulsion Laboratory, the Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars (exoplanets). Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet. The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs. The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature, and distance from its parent star. || ",
            "hits": 67
        },
        {
            "id": 14758,
            "url": "https://svs.gsfc.nasa.gov/14758/",
            "result_type": "Produced Video",
            "release_date": "2025-01-21T00:00:00-05:00",
            "title": "Roman Space Telescope's Coronagraph Instrument Arrives to Goddard Space Flight Center",
            "description": "The first of two scientific instruments for NASA's Nancy Grace Roman Space Telescope has arrived to Goddard Space Flight Center.Designed and built by NASA’s Jet Propulsion Laboratory, the Roman Coronagraph will advance scientists’ ability to directly image planets and disks around other stars (exoplanets). Coronagraphs work by blocking light from a bright object, like a star, so that the observer can more easily see a faint object, like a planet.The Roman Coronagraph is designed to detect planets 100 million times fainter than their stars, or 100 to 1,000 times better than existing space-based coronagraphs. The Roman Coronagraph will be capable of directly imaging reflected starlight from a planet akin to Jupiter in size, temperature, and distance from its parent star. || ",
            "hits": 89
        },
        {
            "id": 20394,
            "url": "https://svs.gsfc.nasa.gov/20394/",
            "result_type": "Animation",
            "release_date": "2024-11-12T15:00:00-05:00",
            "title": "Habitable Worlds Observatory (HWO) Animations and Stills",
            "description": "This page contains artist's concept computer renderings of a current possible design for the Habitable Worlds Observatory. HWO is a large infrared/optical/ultraviolet space telescope recommended by the National Academies' Pathways to Discovery in Astronomy and Astrophysics for the 2020s.HWO will be the first space telescope designed specifically to search for signs of life and determine how common life is beyond Earth.This \"super-Hubble\" will study the universe with unprecedented sensitivity and resolution, giving us new insights into the solar system, stars, galaxies, black holes, dark matter, and the evolution of cosmic structure. || ",
            "hits": 184
        },
        {
            "id": 14714,
            "url": "https://svs.gsfc.nasa.gov/14714/",
            "result_type": "B-Roll",
            "release_date": "2024-11-06T10:00:00-05:00",
            "title": "CODEX Heads to the Space Station for Install",
            "description": "On Nov. 4, 2024, the Coronal Diagnostic Experiment (CODEX) launched to space aboard NASA’s SpaceX CRS-31 – a commercial resupply mission of an uncrewed Dragon spacecraft headed for the International Space Station. Liftoff occurred at 9:29 p.m. EST.CODEX is a solar coronagraph that will be installed on the Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun’s outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contributions from Italy’s National Institute for Astrophysics (INAF).To learn more about the experiment, visit: https://science.nasa.gov/mission/codex/ || ",
            "hits": 84
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        {
            "id": 14693,
            "url": "https://svs.gsfc.nasa.gov/14693/",
            "result_type": "Produced Video",
            "release_date": "2024-10-02T12:00:00-04:00",
            "title": "NASA's Nancy Grace Roman Space Telescope: Systems, Assemble!",
            "description": "In September 2024, the Nancy Grace Roman Space Telescope passed a key milestone and was approved for the next stage of construction. Work on the main systems that will make up the final spacecraft is finishing, and the team at NASA’s Goddard Space Flight Center is ready to begin integration, the process of connecting them together. This video celebrates the effort to reach the final stages of assembly.Music: “The Call,” Torsti Juhani Spoof [BMI] Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || YTframe_Building_Roman_Main2.jpg (1280x720) [451.7 KB] || YTframe_Building_Roman_Main2_searchweb.png (320x180) [124.6 KB] || YTframe_Building_Roman_Main2_thm.png (80x40) [11.0 KB] || 14693_RomanSystemsAssemble_Good.mp4 (1920x1080) [234.1 MB] || 14693_RomanSystemsAssemble_Better.mp4 (1920x1080) [444.0 MB] || 14693RomanSystemsAssembleCaptions.en_US.srt [491 bytes] || 14693RomanSystemsAssembleCaptions.en_US.vtt [475 bytes] || 14693_RomanSystemsAssemble_YouTube.mp4 (1920x1080) [1012.1 MB] || 14693_RomanSystemsAssemble_ProRes1920x1080_2997.mov (1920x1080) [2.8 GB] || 14693_RomanSystemsAssemble_Better.hwshow [508 bytes] || ",
            "hits": 114
        },
        {
            "id": 14647,
            "url": "https://svs.gsfc.nasa.gov/14647/",
            "result_type": "B-Roll",
            "release_date": "2024-08-12T13:00:00-04:00",
            "title": "CODEX – Coronal Diagnostic Experiment",
            "description": "The Coronal Diagnostic Experiment (CODEX) is a solar coronagraph that will be installed on the International Space Station to gather important information about the solar wind and how it forms. A coronagraph blocks out the bright light from the Sun to better see details in the Sun's outer atmosphere, or corona. CODEX is a collaboration between NASA Goddard Space Flight Center and the Korea Astronomy and Space Science Institute (KASI) with additional contribution from Italy's National Institute for Astrophysics (INAF).Learn more: https://science.nasa.gov/mission/codex/ || ",
            "hits": 83
        },
        {
            "id": 14181,
            "url": "https://svs.gsfc.nasa.gov/14181/",
            "result_type": "Produced Video",
            "release_date": "2022-08-04T13:00:00-04:00",
            "title": "Roman Interactive Stills",
            "description": "Right-side view of the Roman Space Telescope.  Highlighted parts available under \"Download Options\" || ROMAN_interactive_Spacecraft_V009_R_Off_2080_print.jpg (1024x576) [57.5 KB] || ROMAN_interactive_V009_R_Roman_off_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080.png (2080x1170) [751.5 KB] || ROMAN_interactive_V009_R_Roman_on_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_V009_R_Roman_comms_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Comms_2080.png (2080x1170) [771.3 KB] || ROMAN_interactive_V009_R_Roman_support_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_Support_2080.png (2080x1170) [768.7 KB] || ROMAN_interactive_V009_R_Roman_tele_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_Tele_2080.png (2080x1170) [776.8 KB] || ROMAN_interactive_V009_R_Roman_SP_00000.png (3840x2160) [1.8 MB] || ROMAN_interactive_Spacecraft_V009_R_SP_2080.png (2080x1170) [786.4 KB] || ROMAN_interactive_V009_R_Roman_WFI_00000.png (3840x2160) [1.7 MB] || ROMAN_interactive_Spacecraft_V009_R_WFI_2080.png (2080x1170) [772.1 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_searchweb.png (320x180) [26.4 KB] || ROMAN_interactive_Spacecraft_V009_R_Off_2080_thm.png (80x40) [3.0 KB] || ",
            "hits": 47
        },
        {
            "id": 13623,
            "url": "https://svs.gsfc.nasa.gov/13623/",
            "result_type": "Produced Video",
            "release_date": "2020-06-17T10:00:00-04:00",
            "title": "Four of Our Favorite SOHO-discovered Comets",
            "description": "Karl Battams, manager of NASA's citizen science Sungrazer Project, talks about his four favorite comets that SOHO has observed.Music: \"Inducing Waves\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_print.jpg (1024x576) [155.4 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_searchweb.png (320x180) [72.1 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.01026_thm.png (80x40) [5.3 KB] || 13623_SOHO4FavoriteComets_ProRes_1920x1080_2997.mov (1920x1080) [3.1 GB] || 13623_SOHO4FavoriteComets_1080.mp4 (1920x1080) [245.9 MB] || 13623_SOHO4FavoriteComets_Good_1080.mp4 (1920x1080) [128.8 MB] || 13623_SOHO4FavoriteComets_1080.webm (1920x1080) [27.2 MB] || SOHO_4000Comets_SRT_Captions.en_US.srt [4.8 KB] || SOHO_4000Comets_SRT_Captions.en_US.vtt [4.8 KB] || ",
            "hits": 49
        },
        {
            "id": 13325,
            "url": "https://svs.gsfc.nasa.gov/13325/",
            "result_type": "Produced Video",
            "release_date": "2019-09-24T13:00:00-04:00",
            "title": "The Nancy Grace Roman Space Telescope's Coronagraph Instrument",
            "description": "Watch this video to learn more about the Roman Space Telescope's coronagraph instrument.Credit: NASA's Goddard Space Flight CenterMusic: \"Concept of Motion\" from Universe Production MusicComplete transcript available. || Roman_CGI_Still.jpg (1920x1080) [396.1 KB] || 13325_Roman_CGI_1080.mp4 (1920x1080) [96.8 MB] || 13325_Roman_CGI_Final_ProRes_1920x1080_2997.mov (1920x1080) [1.3 GB] || 13325_Roman_CGI_1080.webm (1920x1080) [13.9 MB] || Roman_CGI_SRT_Captions.en_US.srt [2.4 KB] || Roman_CGI_SRT_Captions.en_US.vtt [2.4 KB] || ",
            "hits": 127
        },
        {
            "id": 13296,
            "url": "https://svs.gsfc.nasa.gov/13296/",
            "result_type": "Produced Video",
            "release_date": "2019-09-02T00:00:00-04:00",
            "title": "Nancy Grace Roman Space Telescope 360 spacecraft animations PDR version",
            "description": "Animated 3D model of the Roman Space Telescope spacecraft rotated through 360 degrees in a neutral gray environment.Credit: NASA's Goddard Space Flight Center/CI Lab || WFIRST_TurntableRev01ProRes_3840x2160.00001_print.jpg (1024x576) [57.3 KB] || WFIRST_TurntableRev01ProRes_3840x2160.00001_searchweb.png (320x180) [44.6 KB] || WFIRST_TurntableRev01ProRes_3840x2160.00001_thm.png (80x40) [4.0 KB] || WFIRST_TurntableRev01_1080.mp4 (1920x1080) [36.9 MB] || WFIRST_TurntableRev01_1080.webm (1920x1080) [2.3 MB] || WFIRST_TurntableRev01_4k.mp4 (3840x2160) [133.0 MB] || WFIRST_TurntableRev01ProRes_3840x2160.mov (3840x2160) [1.1 GB] || ",
            "hits": 63
        },
        {
            "id": 13295,
            "url": "https://svs.gsfc.nasa.gov/13295/",
            "result_type": "Produced Video",
            "release_date": "2019-08-28T10:00:00-04:00",
            "title": "Take a Spin With NASA's Nancy Grace Roman Space Telescope",
            "description": "Learn more about the Roman Space Telescope spacecraft with this short tour of the main systems.Music: “Phenomenon\" from Above and Below Written and produced by Lars LeonhardCredit: NASA's Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Roman_Spacecraft_360STILL_1.jpg (1920x1080) [272.4 KB] || 13295_Roman_360_1080.mp4 (1920x1080) [219.9 MB] || 13295_Roman_360_Best_1080.mp4 (1920x1080) [807.1 MB] || 13295_Roman_360_ProRes_1920x1080_2997.mov (1920x1080) [2.8 GB] || 13295_Roman_360_1080.webm (1920x1080) [24.0 MB] || Roman_360_SRT_Captions.en_US.srt [4.3 KB] || Roman_360_SRT_Captions.en_US.vtt [4.3 KB] || ",
            "hits": 74
        },
        {
            "id": 13291,
            "url": "https://svs.gsfc.nasa.gov/13291/",
            "result_type": "Produced Video",
            "release_date": "2019-08-23T11:30:00-04:00",
            "title": "NASA’s New Solar Scope Is Ready For Balloon Flight",
            "description": "NASA and the Korea Astronomy and Space Science Institute, or KASI, are getting ready to test a new way to see the Sun, high over the New Mexico desert. A pearlescent balloon — large enough to hug a football field — is scheduled to take flight no earlier than Aug. 26, 2019, carrying beneath it a solar scope called BITSE. BITSE is a coronagraph, a kind of telescope that blocks the Sun’s bright face in order to reveal its dimmer atmosphere, called the corona. Short for Balloon-borne Investigation of Temperature and Speed of Electrons in the corona, BITSE seeks to explain how the Sun spits out the solar wind. || ",
            "hits": 33
        },
        {
            "id": 12238,
            "url": "https://svs.gsfc.nasa.gov/12238/",
            "result_type": "Produced Video",
            "release_date": "2017-12-22T13:00:00-05:00",
            "title": "WFIRST Will See the Big Picture of the Universe",
            "description": "Learn about the Wide Field Infrared Survey Telescope (WFIRST) mission.Music: \"We Dissolve in Stars\" and \"Climb the Ladder\" both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WFIRST_Beauty_still_print.jpg (1024x576) [97.2 KB] || WFIRST_Beauty_still.png (3840x2160) [36.5 MB] || WFIRST_Beauty_still.jpg (3840x2160) [988.6 KB] || WFIRST_Beauty_still_searchweb.png (320x180) [72.0 KB] || WFIRST_Beauty_still_thm.png (80x40) [5.1 KB] || YOUTUBE_1080_12238_WFIRST_Overview_V3_FINAL.mp4 (1920x1080) [845.8 MB] || 12238_WFIRST_Overview_V3_H264_1080p.mov (1920x1080) [759.1 MB] || 12238_WFIRST_Overview_V3_H264_1080_2997.m4v (1920x1080) [377.3 MB] || 12238_WFIRST_Overview_V3_H264_1080p.webm (1920x1080) [41.2 MB] || 12238_WFIRST_Overview_V3_ProRes_3840x2160_2997.mov (3840x2160) [19.3 GB] || YOUTUBE_HQ_12238_WFIRST_Overview_V3_FINAL_4k.mov (3840x2160) [6.5 GB] || 12238_WFIRST_Overview_V3_H264_4K.mov (3840x2160) [1.1 GB] || WFIRST_overview_SRT_Captions.en_US.srt [6.7 KB] || WFIRST_overview_SRT_Captions.en_US.vtt [6.4 KB] || ",
            "hits": 74
        },
        {
            "id": 12636,
            "url": "https://svs.gsfc.nasa.gov/12636/",
            "result_type": "Produced Video",
            "release_date": "2017-08-07T00:00:00-04:00",
            "title": "2 Minutes, 6 Hands, 1 Chance",
            "description": "Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credit: Patisserie Pressure by Benjamin James Parsons || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_print.jpg (1024x576) [159.7 KB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_searchweb.png (320x180) [112.1 KB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_thm.png (80x40) [7.9 KB] || APPLE_TV-12636_2Minutes6Hands1ChanceV6_appletv.m4v (1280x720) [86.9 MB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.webm (1920x1080) [16.4 MB] || APPLE_TV-12636_2Minutes6Hands1ChanceV6_appletv_subtitles.m4v (1280x720) [86.9 MB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.mp4 (1920x1080) [152.5 MB] || YOUTUBE_1080-12636_2Minutes6Hands1ChanceV6_youtube_1080.mp4 (1920x1080) [244.6 MB] || NASA_TV-12636_2Minutes6Hands1ChanceV6.mpeg (1280x720) [507.3 MB] || YOUTUBE_HQ-12636_2Minutes6Hands1ChanceV6_youtube_hq.mov (1920x1080) [672.4 MB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.en_US.srt [2.6 KB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.en_US.vtt [2.6 KB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.mp4 (320x240) [26.4 MB] || PRORES_B-ROLL-12636_2Minutes6Hands1ChanceV6_prores.mov (1280x720) [2.1 GB] || 12636_2Minutes6Hands1ChanceV6.mov (1920x1080) [4.0 GB] || ",
            "hits": 27
        },
        {
            "id": 20243,
            "url": "https://svs.gsfc.nasa.gov/20243/",
            "result_type": "Animation",
            "release_date": "2016-09-20T14:00:00-04:00",
            "title": "Roman Space Telescope Coronagraph Animation",
            "description": "Animation illustrating how a planet can disappear in a star's bright light, and how a coronagraph can reveal it. || Coronagraph_Still_print.jpg (1024x576) [23.5 KB] || Coronagraph_Still.png (3840x2160) [4.8 MB] || Coronagraph_Still_searchweb.png (320x180) [32.9 KB] || Coronagraph_Still_thm.png (80x40) [3.2 KB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.mov (1920x1080) [28.1 MB] || 3840x2160_16x9_60p (3840x2160) [128.0 KB] || WFIRST_exoplanet_Coronagraph_V2_H264_4K.mov (3840x2160) [47.0 MB] || WFIRST_exoplanet_Coronagraph_V2_ProRes_4k.webm (3840x2160) [3.3 MB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.key [29.9 MB] || WFIRST_exoplanet_Coronagraph_V2_H264_1080p.pptx [29.6 MB] || WFIRST_exoplanet_Coronagraph_V2_ProRes_4k.mov (3840x2160) [2.4 GB] || ",
            "hits": 219
        },
        {
            "id": 12147,
            "url": "https://svs.gsfc.nasa.gov/12147/",
            "result_type": "Produced Video",
            "release_date": "2016-03-03T10:00:00-05:00",
            "title": "2016 Eclipse",
            "description": "Solar scientists Natchimuthuk Gopalswamy, Nelson Reginal, Eric Christian, and Sarah Jaeggli discuss the 2016 eclipse and how it is great preparation for the 2017 eclipse.Complete transcript available. || eclipse_promo_thumb.jpg (1280x720) [53.1 KB] || eclipse_promo_thumb_searchweb.png (320x180) [69.9 KB] || eclipse_promo_thumb_thm.png (80x40) [12.8 KB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.mov (1920x1080) [534.5 MB] || PRORES_B-ROLL_12147_2016.eclipse_promo_V2_prores.mov (1280x720) [1.5 GB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv.m4v (1280x720) [63.3 MB] || NASA_TV_12147_2016.eclipse_promo_V2.mpeg (1280x720) [383.5 MB] || 12147_2016.eclipse_promo_V2.mov (1920x1080) [2.7 GB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.webm (1920x1080) [11.6 MB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv_subtitles.m4v (1280x720) [63.4 MB] || 12147_2016_eclipse_PROMO.en_US.srt [2.0 KB] || 12147_2016_eclipse_PROMO.en_US.vtt [2.0 KB] || NASA_PODCAST_12147_2016.eclipse_promo_V2_ipod_sm.mp4 (320x240) [21.4 MB] || ",
            "hits": 50
        },
        {
            "id": 12153,
            "url": "https://svs.gsfc.nasa.gov/12153/",
            "result_type": "Produced Video",
            "release_date": "2016-02-18T11:00:00-05:00",
            "title": "WFIRST: The Best of Both Worlds",
            "description": "With a view 100 times bigger than that of NASA’s Hubble Space Telescope, the Wide Field Infrared Survey Telescope WFIRST will aid researchers in their efforts to unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It also will discover new worlds outside our solar system and advance the search for worlds that could be suitable for life.  Scientists participating in the mission discuss the spacecraft, the science, and its potential.  Slated to launch in the mid-2020s, the observatory will operate at a gravitational balance point known as Earth-sun L2, which is located about 930,000 miles from Earth and directly opposite the sun.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || WfirstAfta-PrintStill2_print.jpg (1024x576) [79.3 KB] || WfirstAfta-PrintStill2.png (3840x2160) [4.7 MB] || WfirstAfta-PrintStill2_searchweb.png (320x180) [59.2 KB] || WfirstAfta-PrintStill2_thm.png (80x40) [4.6 KB] || 12153_WFIRST_Best_Both_Worlds_ProRes_1280x720_5994.mov (1280x720) [3.1 GB] || 12153_WFIRST_Best_Both_Worlds_H264_Best_1280x720_5994.mov (1280x720) [1.7 GB] || 12153_WFIRST_Best_Both_Worlds_FINAL_youtube_hq.mov (1280x720) [671.5 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.mov (1280x720) [174.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv.m4v (1280x720) [122.3 MB] || 12153_WFIRST_Best_Both_Worlds_H264_Good_1280x720_2997.webm (1280x720) [25.0 MB] || 12153_WFIRST_Best_Both_Worlds_FINAL_appletv_subtitles.m4v (1280x720) [122.4 MB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.srt [4.6 KB] || 12153_WFIRST_BestBoth_SRT_Captions.en_US.vtt [4.4 KB] || NASA_PODCAST_12153_WFIRST_Best_Both_Worlds_FINAL_ipod_sm.mp4 (320x240) [41.6 MB] || ",
            "hits": 66
        },
        {
            "id": 11811,
            "url": "https://svs.gsfc.nasa.gov/11811/",
            "result_type": "Produced Video",
            "release_date": "2015-03-17T13:15:00-04:00",
            "title": "SOHO Observes March 14 Coronal Mass Ejection",
            "description": "The Joint ESA/NASA Solar and Heliospheric Observatory, or SOHO, captured this image series of a coronal mass ejection, or CME, on March 14, 2015. || JHV_movie_created_2015-03-17_19.37.12_print.jpg (1024x576) [73.7 KB] || JHV_movie_created_2015-03-17_19.37.12_searchweb.png (320x180) [48.6 KB] || JHV_movie_created_2015-03-17_19.37.12_web.png (320x180) [48.6 KB] || JHV_movie_created_2015-03-17_19.37.12.webm (1920x1080) [334.4 KB] || JHV_movie_created_2015-03-17_19.37.12.mp4 (1920x1080) [9.0 MB] || ",
            "hits": 69
        },
        {
            "id": 11558,
            "url": "https://svs.gsfc.nasa.gov/11558/",
            "result_type": "Produced Video",
            "release_date": "2014-09-24T10:00:00-04:00",
            "title": "NASA's Many Views of a Massive CME",
            "description": "On July 23, 2012, a massive cloud of solar material erupted off the sun's right side, zooming out into space. It soon passed one of NASA's Solar Terrestrial Relations Observatory, or STEREO, spacecraft, which clocked the CME as traveling between 1,800 and 2,200 miles per second as it left the sun. This was the fastest CME ever observed by STEREO.  Two other observatories – NASA's Solar Dynamics Observatory and the joint European Space Agency/NASA Solar and Heliospheric Observatory — witnessed the eruption as well. The July 2012 CME didn't move toward Earth, but watching an unusually strong CME like this gives scientists an opportunity to observe how these events originate and travel through space.  STEREO's unique viewpoint from the sides of the sun combined with the other two observatories watching from closer to Earth helped scientists create models of the entire July 2012 event. They learned that an earlier, smaller CME helped clear the path for the larger event, thus contributing to its unusual speed. Such data helps advance our understanding of what causes CMEs and improves modeling of similar CMEs that could be Earth-directed. || ",
            "hits": 131
        },
        {
            "id": 11493,
            "url": "https://svs.gsfc.nasa.gov/11493/",
            "result_type": "Produced Video",
            "release_date": "2014-02-25T00:00:00-05:00",
            "title": "NASA's SDO Provides Images of Significant Solar Flare",
            "description": "The sun emitted a significant solar flare, peaking at 7:49 p.m. EST on Feb. 24, 2014. NASA's Solar Dynamics Observatory, which keeps a constant watch on the sun, captured images of the event.This flare is classified as an X4.9-class flare. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc. || ",
            "hits": 100
        },
        {
            "id": 10785,
            "url": "https://svs.gsfc.nasa.gov/10785/",
            "result_type": "Produced Video",
            "release_date": "2013-05-07T11:00:00-04:00",
            "title": "NASA's Heliophysics Fleet Captures May 1, 2013 Prominence Eruption and CME",
            "description": "On May 1, 2013, NASA's Solar Dynamics Observatory (SDO) watched as an active region just around the East limb (left edge) of the sun erupted with a huge cloud of solar material—a heated, charged gas called plasma. This eruption, called a coronal mass ejection, or CME, sent the plasma streaming out through the solar system. Viewing the sun in the extreme ultraviolet wavelength of 304 angstroms, SDO provided a beautiful view of the initial arc as it left the solar surface.  Such eruptions soon leave SDO's field of view, but other satellites in NASA's Heliophysics fleet can pick them up, tracking such space weather to determine if they are headed toward Earth or spacecraft near other planets. With advance warning, many space assets can be put into safe mode and protect themselves from the effects of such particle radiation.In addition to the images captured by SDO, the May 1, 2013 CME was also observed by the ESA/NASA Solar and Heliospheric Observatory (SOHO). SOHO houses two overlapping coronagraphs—telescopes where the bright sun is blocked by a disk so it doesn't overpower the fainter solar atmosphere—and they both saw the CME continue outward. The LASCO C2 coronagraph shows the region out to about 2.5 million miles. The LASCO C3 coronagraph expands even farther out to around 13.5 million miles. Both of these instruments show the CME as it expands and becomes fainter on its trip away from the sun.NASA's Solar Terrestrial Relations Observatory (STEREO) Ahead satellite saw the eruption from a very different angle. It, along with its twin STEREO Behind, is orbiting at a similar distance as Earth. STEREO-A orbits slightly faster than Earth and STEREO-B orbits slightly slower. Currently, STEREO-A is more than two-thirds of the way to being directly behind the sun, and has a view of the far side of the sun. From this perspective, the CME came off the right side of the sun. STEREO has an extreme ultraviolet camera similar to SDO's, but it also has coronagraphs like SOHO. As a result, using its two inner coronagraphs, it was able to track the CME from the solar surface out to 6.3 million miles.Working together, such missions provide excellent coverage of a wide variety of solar events, a wealth of scientific data—and lots of beautiful imagery.Watch this video on YouTube. || ",
            "hits": 96
        },
        {
            "id": 11207,
            "url": "https://svs.gsfc.nasa.gov/11207/",
            "result_type": "Produced Video",
            "release_date": "2013-02-07T10:30:00-05:00",
            "title": "The Sun Produces Two CMEs",
            "description": "In the evening of Feb. 5, 2013, the sun erupted with two coronal mass ejections or CMEs that may glance near-Earth space.  Experimental NASA research models, based on observations from the Solar Terrestrial Relations Observatory (STEREO) and ESA/NASA's Solar and Heliospheric Observatory, show that the first CME began at 7 p.m. EST and left the sun at speeds of around 750 miles per second. The second CME began at 10:36 p.m. EST and left the sun at speeds of around 350 miles per second. Historically, CMEs of this speed and direction have been benign.Not to be confused with a solar flare, a CME is a solar phenomenon that can send solar particles into space and reach Earth one to three days later.Earth-directed CMEs can cause a space weather phenomenon called a geomagnetic storm, which occurs when they connect with the outside of the Earth's magnetic envelope, the magnetosphere, for an extended period of time. In the past, CMEs at this strength have had little effect. They may cause auroras near the poles but are unlikely to disrupt electrical systems on Earth or interfere with GPS or satellite-based communications systems. || ",
            "hits": 65
        },
        {
            "id": 10998,
            "url": "https://svs.gsfc.nasa.gov/10998/",
            "result_type": "Produced Video",
            "release_date": "2012-06-04T11:00:00-04:00",
            "title": "SOHO LASCO View of Approaching Venus Transit",
            "description": "The LASCO C2 and C3 coronographs on board the SOHO spacecraft have been watching the approach of Venus for its last solar transit until 2117.With coronagraphs, the Sun is being blocked by an occulting disk, seen here in blue, so that SOHO can observe the much fainter features in the Sun's corona. The actual size of the Sun is represented by the white disk. The transit of Venus begins tomorrow, June 5, at about 6pm Eastern Daylight Time, or about 10pm Universal Time. It will last approximately 6 hours. || ",
            "hits": 59
        },
        {
            "id": 10619,
            "url": "https://svs.gsfc.nasa.gov/10619/",
            "result_type": "Produced Video",
            "release_date": "2010-07-22T00:00:00-04:00",
            "title": "20 Years of Hubble Science",
            "description": "This video series focuses on two areas of science that the Hubble Space Telescope has helped advance: thee formation and evolution of galaxies and detection of extrasolar planets. || ",
            "hits": 56
        },
        {
            "id": 3504,
            "url": "https://svs.gsfc.nasa.gov/3504/",
            "result_type": "Visualization",
            "release_date": "2008-04-02T00:00:00-04:00",
            "title": "Halloween 2003 Solar Storms: SOHO/EIT and SOHO/LASCO",
            "description": "Here is a view of the solar disk in 195 Å ultraviolet light (colored green in this movie) and the Sun's extended atmosphere, or corona, (blue and white in this movie). The corona is visible to the SOHO/LASCO coronagraph instruments, which block the bright disk of the Sun so the significantly fainter corona can be seen. In this movie, the inner coronagraph (designated C2) is combined with the outer coronagraph (C3). This movie covers a two week period in October and November 2003 which exhibited some of the largest solar activity events since the advent of space-based solar observing.As the movie plays, we can observe a number of features of the active Sun. Long streamers radiate outward from the Sun and wave gently due to their interaction with the solar wind. The bright white regions are visible due to their high density of free electrons which scatter the light from the photosphere towards the observer. Protons and other ionized atoms are there as well, but are not as visible since they do not interact with photons as strongly as electrons. Coronal Mass Ejections (CMEs) are occasionally observed launching from the Sun. Some of these launch particle events which can saturate the cameras with snow-like artifacts.Also visible in the coronagraphs are stars and planets. Stars are seen to drift slowly to the right, carried by the relative motion of the Sun and the Earth. The planet Mercury is visible as the bright point moving left of the Sun. The horizontal 'extension' in the image is called 'blooming' and is due to a charge leakage along the readout wires in the CCD imager in the camera.This movie is part of a series of movies with matching cadence designed to play synchronously with each other. The other movies in this series are  Halloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 195 angstromHalloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 304 angstromHalloween 2003 Solar Storms: SOHO/MDI Continuum Halloween 2003 Solar Storms: SOHO/MDI Magnetograms For more information, visit the SOHO project page.. || ",
            "hits": 50
        },
        {
            "id": 3406,
            "url": "https://svs.gsfc.nasa.gov/3406/",
            "result_type": "Visualization",
            "release_date": "2007-03-01T00:00:00-05:00",
            "title": "STEREO Coronal Mass Ejection:  From the EUVI to HI-2",
            "description": "This movie collects imagery from SOHO and STEREO-A of a coronal mass ejection (CME) during January of 2007. The instruments in this view, from left to right, are STEREO/HI-1, STEREO/HI-2, SOHO/LASCO/C3, SOHO/LASCO/C2, and STEREO/EUVI. The Heliospheric Imager, HI-2, shows some of the tail of comet McNaught. The dark trapezoidal shape on the left edge of the image in HI-2 is the Earth occulter which will block out the disk of the Earth when it moves into view (since the planet will appear so bright as to saturate the detectors). Due to ongoing work with the STEREO coronagraphs, COR1 and COR2, the SOHO/LASCO coronagraphs are used for this movie. The blue Sun in the center of the coronagraphs is STEREO/EUVI ultraviolet images.There is a 22 hour gap in the data coverage for HI-2 which creates the appearance of a jump in the playback.These are not standard images but are called 'running difference' images which highlight changes in the view. White pixels correspond to increases in brightness, while dark pixels reflect a decrease in brightness, with respect to the immediately previous image.'Running differencing' generates some unusual effects. For example, the mottled background is created by the motion of the stars through the field-of-view as the spacecraft pointing direction slowly changes (the Andromeda galaxy is the oblong 'smudge' near the upper left corner). The planets Venus (right edge of HI-2) and Mercury are visible (near center of HI-1), their column of pixels saturated due to their brightness.STEREO: Solar TErrestrial RElations ObservatorySOHO: SOlar Heliospheric ObservatoryLASCO: Large Angle and Spectrometric CoronagraphEUVI: Extreme UltraViolet Imager || ",
            "hits": 25
        }
    ]
}