{
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    "results": [
        {
            "id": 5302,
            "url": "https://svs.gsfc.nasa.gov/5302/",
            "result_type": "Visualization",
            "release_date": "2024-06-05T00:00:00-04:00",
            "title": "A Long View of the last Solar Minimum",
            "description": "A month-long view of the Solar Cycle 24 solar minimum, as seen in the 171A filter of Solar Dynamics Observatory (SDO).",
            "hits": 57
        },
        {
            "id": 5165,
            "url": "https://svs.gsfc.nasa.gov/5165/",
            "result_type": "Visualization",
            "release_date": "2024-01-05T00:00:00-05:00",
            "title": "STEREO - The Second Time Around...",
            "description": "In mid-August 2023, the still-operational STEREO-A (STEREO-B went offline in October 2014) passed Earth for the first time since its launch 17 years ago. See also STEREO-A Returns by Earth.While STEREO-B is no longer available, it is possible to construct stereo imagery of the Sun using STEREO-A with Solar Dynamics Observatory (SDO).  Here we present a series of images for corresponding filters between the two missions which can be used for stereo viewing.Color (SDO color table) Left/Right Image PairsIn this section, we present frame-synchronized left eye (STEREO-A) and right eye (SDO) for the specified ultraviolet filter.  They are provided as separate movie and frame-sets to maximize flexibility for the target viewing technology.  Time stamps are provided as separate image files for compositing if desired.   If you match frame numbers for the image sets for a specific filter, you will have images closest in time for apropriate left/right eye pairing.171 Angstrom filter || ",
            "hits": 55
        },
        {
            "id": 5015,
            "url": "https://svs.gsfc.nasa.gov/5015/",
            "result_type": "Visualization",
            "release_date": "2022-08-25T00:00:00-04:00",
            "title": "A Small (M5) Flare from Active Region 13078",
            "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.These movies were generated around a small M5 class solar flare that occurred on April 17, 2022 near the center of the lower hemisphere || ",
            "hits": 24
        },
        {
            "id": 4963,
            "url": "https://svs.gsfc.nasa.gov/4963/",
            "result_type": "Visualization",
            "release_date": "2022-08-19T00:00:00-04:00",
            "title": "Fifty Days of Continuous Sun from Solar Dynamics Observatory (171A filter)",
            "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun.  The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.This movie was generated as a test case for a new movie pipeline for SDO, here's SDO AIA 171A imagery, sampled every two minutes for 50 days (April 12 through June 3, 2014), resulting in 30 minutes of continuous play (at 20 frames per second). || ",
            "hits": 56
        },
        {
            "id": 4966,
            "url": "https://svs.gsfc.nasa.gov/4966/",
            "result_type": "Visualization",
            "release_date": "2022-08-19T00:00:00-04:00",
            "title": "AR 12938 - Slow Building Active Region on Left Limb",
            "description": "The slow build-up of a solar active region, as seen in AIA 171 Angstrom filter. Correction is applied for the instrument Point-Spread Function (PSF). || AR12938_AIA171_stamped.001680_print.jpg (1024x1024) [235.2 KB] || AR12938_AIA171_stamped.001680_searchweb.png (320x180) [89.7 KB] || AR12938_AIA171_stamped.001680_thm.png (80x40) [6.7 KB] || AR12938_AIA171_PSF_2048p30.mp4 (2048x2048) [261.0 MB] || AR12938_AIA171_PSF_stamped_2048p30.mp4 (2048x2048) [262.2 MB] || AR12938_AIA171_stamped_1024p30.mp4 (1024x1024) [33.1 MB] || AR12938_AIA171_stamped_1024p30.webm (1024x1024) [7.1 MB] || AIA171-Frames.PSF (4096x4096) [128.0 KB] || AIA171-Frames.PSF.stamped (4096x4096) [128.0 KB] || AIA171-Time.PSF (4096x4096) [128.0 KB] || AR12938_AIA171_PSF_4096p30_h265.mp4 (4096x4096) [813.9 MB] || AR12938_AIA171_PSF_stamped_4096p30_h265.mp4 (4096x4096) [814.7 MB] || ",
            "hits": 22
        },
        {
            "id": 4911,
            "url": "https://svs.gsfc.nasa.gov/4911/",
            "result_type": "Visualization",
            "release_date": "2021-07-23T10:00:00-04:00",
            "title": "Aging (Instruments) in Space",
            "description": "The space environment is harsh not only on humans and other living organisms, but instruments also.Damage from solar energetic particles and cosmic rays can slowly degrade performance of an instrument.  Fortunately there are ways to characterize and correct for this degradation.  The graphics on this page are based on the tutorial AIApy: Modeling Channel Degradation over Time. || ",
            "hits": 48
        },
        {
            "id": 13742,
            "url": "https://svs.gsfc.nasa.gov/13742/",
            "result_type": "Produced Video",
            "release_date": "2020-11-05T09:55:00-05:00",
            "title": "Hubble's Extraordinary ULLYSES Program",
            "description": "The universe would be a pretty boring place without stars. Without them, the universe would remain a diffuse plasma of mostly hydrogen and helium from the big bang. To better understand stellar evolution, a new Hubble initiative has been launched called ULLYSES (UV Legacy Library of Young Stars as Essential Standards). This is the largest observing program ever undertaken by NASA’s Hubble Space Telescope, which will be used to look at over 300 stars. Ultraviolet (UV) light from the target stars will be used to produce a library of the spectral fingerprints of young, low-mass stars from eight star-forming regions in the Milky Way, as well as fully mature high-mass stars in several nearby dwarf galaxies including the Magellanic Clouds.For more information, visit https://nasa.gov/hubble.Music Credits:\"Red Giant\" by Christian Tschuggnall [AKM] and Michael Edwards [APRA] via Atmosphere Music Ltd [PRS] and Universal Production Music || ",
            "hits": 73
        },
        {
            "id": 4766,
            "url": "https://svs.gsfc.nasa.gov/4766/",
            "result_type": "Visualization",
            "release_date": "2020-09-21T11:00:00-04:00",
            "title": "IRIS views Nano-Flares on the Sun",
            "description": "Opening full-disk solar view from AIA 304 angstroms, zooming in and fading in IRIS SJI at 1400 angstroms. || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i.00663_print.jpg (1024x576) [139.8 KB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i.00663_searchweb.png (320x180) [67.9 KB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i.00663_thm.png (80x40) [5.0 KB] || SDO304-IRIS1400-nanoflare2014-zoomHD (1920x1080) [0 Item(s)] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i_p30.mp4 (1920x1080) [60.5 MB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i_p30.webm (1920x1080) [3.0 MB] || SDO304-IRIS1400-nanoflare2014-zoomHD (3840x2160) [0 Item(s)] || SDO304-IRIS1400-nanoflare2014-zoom_stand.UHD2160_p30.mp4 (3840x2160) [203.9 MB] || SDO304-IRIS1400-nanoflare2014-zoom_stand.HD1080i_p30.mp4.hwshow [218 bytes] || ",
            "hits": 25
        },
        {
            "id": 4854,
            "url": "https://svs.gsfc.nasa.gov/4854/",
            "result_type": "Visualization",
            "release_date": "2020-09-15T10:00:00-04:00",
            "title": "Coronal Holes at Solar Minimum and Solar Maximum",
            "description": "A sample of solar coronal holes around the time of the maximum of sunspot activity (April 2014).  Note the polar regions are devoid of coronal holes but a large hole appears in the southern hemisphere. || CoronalHoleMax_AIA193_00150_print.jpg (1024x1024) [173.1 KB] || CoronalHoleMax_AIA193_00150_searchweb.png (320x180) [89.6 KB] || CoronalHoleMax_AIA193_00150_thm.png (80x40) [7.4 KB] || CoronalHoleMax_AIA193_2048p30.mp4 (2048x2048) [61.7 MB] || CoronalHoleMax_AIA193_2048p30.webm (2048x2048) [2.9 MB] || AIA193-Time (4096x4096) [64.0 KB] || AIA193-Frames (4096x4096) [64.0 KB] || CoronalHoleMax_Timestamp (600x100) [64.0 KB] || ",
            "hits": 281
        },
        {
            "id": 4776,
            "url": "https://svs.gsfc.nasa.gov/4776/",
            "result_type": "Visualization",
            "release_date": "2020-06-24T10:00:00-04:00",
            "title": "Ten Years of Solar Dynamics Observatory",
            "description": "Ten years of SDO AIA 171 angstrom data with day time stamp overlay.  Frames are sampled approximately one image every hour. || SDOat10_AIA171_stand.UHD2160.01500_print.jpg (1024x576) [47.4 KB] || SDOat10_AIA171_stand.UHD2160.01500_searchweb.png (320x180) [40.9 KB] || SDOat10_AIA171_stand.UHD2160.01500_thm.png (80x40) [4.0 KB] || SDOat10_AIA171.1080p30.webm (1920x1080) [348.5 MB] || SDOat10_AIA171.baseimage (3840x2160) [0 Item(s)] || SDOat10_AIA171.1080p30.mp4 (1920x1080) [3.9 GB] || SDOat10_AIA171.UHD2160_p30.mp4 (3840x2160) [13.0 GB] || SDOat10_AIA171.1080p30.mp4.hwshow [188 bytes] || ",
            "hits": 85
        },
        {
            "id": 4491,
            "url": "https://svs.gsfc.nasa.gov/4491/",
            "result_type": "Visualization",
            "release_date": "2019-05-01T00:00:00-04:00",
            "title": "The X8.2 Flare of September 2017, as Seen by SDO",
            "description": "40 hours of AIA 131 angstrom imager at 12 second cadence viewing the time around the X8.2 solar flare. || Sept2017_X8Flare_131A_stand.UHD3840.07800_print.jpg (1024x576) [61.1 KB] || AIA131A (1920x1080) [0 Item(s)] || Sept2017_X8Flare_131A.HD1080i_p30.webm (1920x1080) [47.6 MB] || Sept2017_X8Flare_131A.HD1080i_p30.mp4 (1920x1080) [843.8 MB] || AIA131A (3840x2160) [0 Item(s)] || Sept2017_X8Flare_131A.HD1080i_p30.mp4.hwshow || ",
            "hits": 51
        },
        {
            "id": 12916,
            "url": "https://svs.gsfc.nasa.gov/12916/",
            "result_type": "Produced Video",
            "release_date": "2018-12-11T14:00:00-05:00",
            "title": "50th Anniversary of NASA's OAO 2 Mission",
            "description": "“Seas of Infinity” (1968), full-length version scanned from 16mm color film and color corrected; run time 14:25. Original description: The film opens with an explanation of the electromagnetic spectrum. The limited capabilities of skyhook balloons and sounding rockets are used to illustrate the need for orbiting observatories. Reviews the planning, development, launching and function of the Orbiting Astronomical Observatory, a series of orbiting telescopes which are being used to study our solar system and the stars beyond. Features comments by the following leading scientists on the potential of this advancement in astronomy: Dr. Arthur Code, Wisconsin telescopes; Dr. James Kupperian, Goddard Flight Center using Cassegrain designs; Dr. Fred Whipple on the ultraviolet light sky mapping project; and Dr. Donald Morton on the Princeton OAO ultraviolet spectroscopy project. The film has scenes of the assembly of the OAO. The OAO will be launched by an Atlas-Centaur.  Credit: NASAComplete transcript available. || Seas_Of_Infinity_OAO2_Color_Corrected.22261_print.jpg (1024x768) [40.5 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.22261_searchweb.png (320x180) [42.3 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.22261_thm.png (80x40) [4.5 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.mp4 (640x480) [136.1 MB] || Seas_Of_Infinity_OAO2_SRT_Captions.en_US.srt [16.6 KB] || Seas_Of_Infinity_OAO2_SRT_Captions.en_US.vtt [16.6 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.webm (640x480) [110.9 MB] || ",
            "hits": 96
        },
        {
            "id": 30960,
            "url": "https://svs.gsfc.nasa.gov/30960/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-06-04T10:00:00-04:00",
            "title": "Eagle Nebula: M16 Wide",
            "description": "This series of images shows the environment around the Pillars of Creation, the Eagle Nebula, Messier 16.  The images reveal the nebula in optical, X-ray, mid-infrared, and far-infrared light. || STScI-H-M16wide_1x-1920x1080.00001_print.jpg (1024x576) [163.7 KB] || STScI-H-M16wide_1x-1920x1080.00001_searchweb.png (320x180) [108.4 KB] || STScI-H-M16wide_1x-1920x1080.00001_thm.png (80x40) [6.9 KB] || STScI-H-M16wide_1x-1280x720.mp4 (1280x720) [8.5 MB] || STScI-H-M16wide_1x-1920x1080.mp4 (1920x1080) [17.9 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-M16wide_1x-1920x1080.webm (1920x1080) [5.2 MB] || STScI-H-M16wide_1x-640x360.mp4 (640x360) [2.9 MB] || STScI-H-M16wide_1x-3840x2160.mp4 (3840x2160) [17.1 MB] || STScI-H-M16wide_1x-H265-3840x2160.mp4 (3840x2160) [7.6 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 178
        },
        {
            "id": 30944,
            "url": "https://svs.gsfc.nasa.gov/30944/",
            "result_type": "Hyperwall Visual",
            "release_date": "2018-05-07T10:00:00-04:00",
            "title": "Vision Across the Full Spectrum: The Crab Nebula, from Radio to X-ray",
            "description": "This animation shows the Crab Nebula from the lowest-frequency light (radio), to infrared, visible, ultraviolet, and finally X-ray. || STScI-H-CrabNebula_1x-1920x1080.00001_print.jpg (1024x576) [40.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_searchweb.png (320x180) [26.4 KB] || STScI-H-CrabNebula_1x-1920x1080.00001_thm.png (80x40) [2.3 KB] || STScI-H-CrabNebula_1x-1280x720.mp4 (1280x720) [3.8 MB] || STScI-H-CrabNebula_1x-1920x1080.mp4 (1920x1080) [7.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || STScI-H-CrabNebula_1x-1920x1080.webm (1920x1080) [8.0 MB] || STScI-H-CrabNebula_1x-640x360.mp4 (640x360) [1.4 MB] || STScI-H-CrabNebula_1x-3840x2160.mp4 (3840x2160) [16.2 MB] || STScI-H-CrabNebula_1x-H265_3840x2160.mp4 (3840x2160) [3.5 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || ",
            "hits": 521
        },
        {
            "id": 4623,
            "url": "https://svs.gsfc.nasa.gov/4623/",
            "result_type": "Visualization",
            "release_date": "2018-04-30T10:00:00-04:00",
            "title": "The Dynamic Solar Magnetic Field with Introduction",
            "description": "This narrated visualization  transitions from a view of the Sun in visible light, to a view in ultraviolet light showing the plasma flowing along solar magnetic structures, to the underlying magnetic field of the solar photosphere, to a model construction of magnetic fieldlines above the photosphere.This video is also available on our YouTube channel. || SolarMagnetism_UHD3840.04000_print.jpg (1024x576) [198.9 KB] || SolarMagnetism_UHD3840.04000_thm.png (80x40) [6.0 KB] || SolarMagnetism_UHD3840.04000_web.png (320x180) [84.1 KB] || SolarMagnetism_ProRes3_HD1080_p30_Narrated.webm (1280x720) [33.9 MB] || SolarMagnetism_ProRes3_HD1080_p30_Narrated.mov (1280x720) [7.4 GB] || SolarMagnetism_ProRes3_UHD2160_p30_Narrated.mov (3840x2160) [12.8 GB] || ",
            "hits": 105
        },
        {
            "id": 12613,
            "url": "https://svs.gsfc.nasa.gov/12613/",
            "result_type": "Produced Video",
            "release_date": "2017-06-02T11:00:00-04:00",
            "title": "SDO 4k Slow-rotation Sun Resource Page",
            "description": "Still Image for page || SDO_Slow_Gallery.jpg (1920x1080) [235.4 KB] || SDO_Slow_Gallery_searchweb.png (320x180) [43.0 KB] || SDO_Slow_Gallery_thm.png (80x40) [3.6 KB] || ",
            "hits": 156
        },
        {
            "id": 4496,
            "url": "https://svs.gsfc.nasa.gov/4496/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 171 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI171A_UHD3840.02000_print.jpg (1024x576) [69.0 KB] || 2007stereo_RedCyan_010_EUVI171A_2160p30.mp4 (3840x2160) [451.0 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI171A_2160p30.webm (3840x2160) [13.7 MB] || ",
            "hits": 23
        },
        {
            "id": 4500,
            "url": "https://svs.gsfc.nasa.gov/4500/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 195 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI195A_UHD3840.02000_print.jpg (1024x576) [51.7 KB] || 2007stereo_RedCyan_010_EUVI195A_2160p30.mp4 (3840x2160) [287.8 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI195A_2160p30.webm (3840x2160) [12.6 MB] || ",
            "hits": 13
        },
        {
            "id": 4501,
            "url": "https://svs.gsfc.nasa.gov/4501/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 284 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI284A_UHD3840.02000_print.jpg (1024x576) [59.2 KB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI284A_2160p30.mp4 (3840x2160) [506.4 MB] || 2007stereo_RedCyan_010_EUVI284A_2160p30.webm (3840x2160) [12.7 MB] || ",
            "hits": 20
        },
        {
            "id": 4502,
            "url": "https://svs.gsfc.nasa.gov/4502/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 304 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI304A_UHD3840.02000_print.jpg (1024x576) [80.1 KB] || 2007stereo_RedCyan_010_EUVI304A_2160p30.mp4 (3840x2160) [710.3 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI304A_2160p30.webm (3840x2160) [15.7 MB] || ",
            "hits": 23
        },
        {
            "id": 12375,
            "url": "https://svs.gsfc.nasa.gov/12375/",
            "result_type": "Produced Video",
            "release_date": "2016-09-26T14:00:00-04:00",
            "title": "Hubble Directly Images Possible Plumes on Europa",
            "description": "NASA's Hubble Space Telescope took direct ultraviolet images of the icy moon Europa transiting across the disk of Jupiter. Out of ten observations, Hubble saw what may be water vapor plumes on three of the images. This adds another piece of supporting evidence to the existence of water vapor plumes on Europa - Hubble also detected spectroscopic signatures of water vapor in 2012. The existence of water vapor plumes could provide NASA's Europa flyby mission the opportunity to study the conditions and habitability of Europa's subsurface ocean.Read the full nasa.gov story here: http://www.nasa.gov/press-release/nasa-s-hubble-spots-possible-water-plumes-erupting-on-jupiters-moon-europaRead the full science paper here: http://hubblesite.org/pubinfo/pdf/2016/33/pdf.pdfFull details on the images can be found on HubbleSite.org: http://hubblesite.org/newscenter/archive/releases/2016/33/Additional Resources:JPL's \"Europa: Tempting Target for Future Exploration\" video file is downloadable here: https://vimeo.com/118505538Read the Dec 2013 press release about Hubble's previous observations of Europa here: http://www.nasa.gov/content/goddard/hubble-europa-water-vapor || ",
            "hits": 91
        },
        {
            "id": 2917,
            "url": "https://svs.gsfc.nasa.gov/2917/",
            "result_type": "Visualization",
            "release_date": "2004-02-20T12:00:00-05:00",
            "title": "SORCE Monitors Solar Variability during Record Solar Flares",
            "description": "The SORCE mission monitors solar variability to determine its impact on the Earth's climate. The X-ray photometer aboard SORCE observes the record-breaking solar flares in the Fall of 2003. The line graph shows the photometer's measured solar radiation flux in the 1-7 nanometer wavelength band (x-ray) measured in milliwatts per square meter. The ultraviolet (195 angstrom) imagery from SOHO/EIT (green) illustrates where the flares (the bright white spots) are located on the solar disk. || ",
            "hits": 22
        },
        {
            "id": 2918,
            "url": "https://svs.gsfc.nasa.gov/2918/",
            "result_type": "Visualization",
            "release_date": "2004-02-20T12:00:00-05:00",
            "title": "SORCE Monitors Solar Variability during Record Solar Flares - Video version",
            "description": "The SORCE mission monitors solar variability to determine its impact on the Earth's climate. The X-ray photometer aboard SORCE observes the record-breaking solar flares in the Fall of 2003. The line graph shows the photometer's measured solar radiation flux in the 1-7 nanometer wavelength band (x-ray) measured in milliwatts per square meter. The ultraviolet (195 angstrom) imagery from SOHO/EIT (green) illustrates where the flares (the bright white spots) are located on the solar disk. This version has the contents slightly smaller for use in video. || ",
            "hits": 53
        }
    ]
}