{
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    "next": null,
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    "results": [
        {
            "id": 5355,
            "url": "https://svs.gsfc.nasa.gov/5355/",
            "result_type": "Visualization",
            "release_date": "2024-10-02T00:00:00-04:00",
            "title": "An X1.7 flare from Active Region 13765 and some extra energetic activity - August 5, 2024",
            "description": "Active Region AR 13765 launches an X1.7 flare on August 5, 2024 on the rightmost part of the solar limb. Shortly thereafter, an X1.1 flare launches near the left limb from AR 13780.  For more details, see the Space Weather Database entry for X1.7 and X1.1.  Towards the end of this visualization, around 18:35 TAI, a bright filament launches near the center of the disk.",
            "hits": 9
        },
        {
            "id": 5268,
            "url": "https://svs.gsfc.nasa.gov/5268/",
            "result_type": "Visualization",
            "release_date": "2024-05-08T00:00:00-04:00",
            "title": "Double Filament Eruptions from AR 13614 - March 21, 2024",
            "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.Active Region 13614 (upper left) launches two CMEs on March 21, 2024.   For details of this event, see the Space Weather database entry. || ",
            "hits": 27
        },
        {
            "id": 5108,
            "url": "https://svs.gsfc.nasa.gov/5108/",
            "result_type": "Visualization",
            "release_date": "2023-06-27T00:00:00-04:00",
            "title": "An 9.6 M-class flare and Filament - May 16, 2023",
            "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.Active region AR13310 at the lower left solar limb launches an M 9.6  class flare followed by a bright filament launched almost tangent to the limb.   For more information on the classification of solar flares, see Solar Flares: What Does It Take to Be X-Class? or X-Class: A Guide to Solar Flares.  The point-spread function correction (PSF) has been applied to all this imagery.Event Description. || ",
            "hits": 18
        },
        {
            "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": 373
        },
        {
            "id": 12588,
            "url": "https://svs.gsfc.nasa.gov/12588/",
            "result_type": "Produced Video",
            "release_date": "2017-04-26T13:00:00-04:00",
            "title": "A Solar Eruption in 5 Steps",
            "description": "Music credit: Prism Mystery by  Donn WilkersonComplete transcript available.Watch this video on the NASA Goddard YouTube channel. || filament.thumb.jpg (1920x1080) [239.3 KB] || filament.thumb_print.jpg (1024x576) [176.5 KB] || filament.thumb_searchweb.png (320x180) [106.4 KB] || filament.thumb_web.png (320x180) [106.4 KB] || filament.thumb_thm.png (80x40) [7.0 KB] || 12588_Mechanisms_for_Solar_EruptionsV4.mov (1920x1080) [3.2 GB] || 12588_Mechanisms_for_Solar_EruptionsV4.webm (1920x1080) [10.2 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_appletv.m4v (1280x720) [63.8 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_large.mp4 (1920x1080) [114.5 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_youtube_hq.mov (1920x1080) [244.4 MB] || 12588MechanismsforSolarEruptionsV4_VX-281901_appletv_subtitles.m4v (1280x720) [63.8 MB] || 12588_Mechanisms_for_Solar_EruptionsV4.en_US.srt [1.2 KB] || 12588_Mechanisms_for_Solar_EruptionsV4.en_US.vtt [1.2 KB] || 12588MechanismsforSolarEruptionsV4_VX-281901_ipod_sm.mp4 (320x240) [17.5 MB] || ",
            "hits": 28
        }
    ]
}