{
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    "results": [
        {
            "id": 5625,
            "url": "https://svs.gsfc.nasa.gov/5625/",
            "result_type": "Visualization",
            "release_date": "2026-03-25T00:00:00-04:00",
            "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami",
            "description": "GUARDIAN is a near-real-time ionospheric monitoring software that uses multi-GNSS total electron content time series to detect natural hazard signatures over the Pacific. Its AI-powered extension, GUARDIAN Scout, automates earthquake and tsunami detection. On July 29, 2025, GUARDIAN detected an incoming tsunami triggered by a magnitude 8.8 Kamchatka earthquake 32 minutes before the earliest tidal gauge detection, demonstrating its life-saving early warning potential.",
            "hits": 858
        },
        {
            "id": 5626,
            "url": "https://svs.gsfc.nasa.gov/5626/",
            "result_type": "Visualization",
            "release_date": "2026-03-25T00:00:00-04:00",
            "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami (Vertical version)",
            "description": "This data visualizaton show the Kamchatka earthquake, soon followed by GUARDIAN stations G027 and QSPP early warning detections. NOAA's MOST simulation then shows the progression of the tsunami waves across the Pacific Ocean. Guardian station KOKB (Hawaii) picks up the incoming tsunami wave followed by Hawaii's tidal gauge detectors.",
            "hits": 128
        },
        {
            "id": 14445,
            "url": "https://svs.gsfc.nasa.gov/14445/",
            "result_type": "Produced Video",
            "release_date": "2023-10-25T15:00:00-04:00",
            "title": "Atmospheric Gravity Waves Imagery",
            "description": "Atmospheric gravity waves are similar to what happens when you drop a stone into a calm pond, but they roll through the air and cloud tops instead of water. Just like waves form in the ocean or a lake when water is disturbed, waves also form in the atmosphere when air is disturbed. They form when air is forced upward by hills or mountains into a layer of stable air in the atmosphere. Gravity causes the air to fall back down, and it begins to oscillate, creating a ripple effect. Wind flowing over the Rocky Mountains, for example, can create gravity waves that are felt as turbulence on an airplane. || ",
            "hits": 902
        },
        {
            "id": 14177,
            "url": "https://svs.gsfc.nasa.gov/14177/",
            "result_type": "Produced Video",
            "release_date": "2022-07-19T11:00:00-04:00",
            "title": "How Climate Patterns Thousands of Miles Away Affect US Bird Migration",
            "description": "Stock footage: Pond5Radar video courtesy of Dr. Kyle Horton, Colorado State UniversityUniversal Production Music: “Two Ticks” by Michael Lesirge [PRS] and Tarek Christopher Modi [PRS]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by pond5.com and CSU is obtained through permission and may not be excised or remixed in other products. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.htmlComplete transcript available. || 14177_BirdMigration_Thumb.jpg (1920x1080) [268.4 KB] || 14177_BirdMigration_Thumb_print.jpg (1024x576) [130.4 KB] || 14177_BirdMigration_Thumb_searchweb.png (320x180) [64.3 KB] || 14177_BirdMigration_Thumb_web.png (320x180) [64.3 KB] || 14177_BirdMigration_Thumb_thm.png (80x40) [6.5 KB] || BirdMigration.mov (1920x1080) [4.0 GB] || BirdMigration.webm (960x540) [50.2 MB] || BirdMigration.mp4 (1920x1080) [380.5 MB] || TWITTER_720_BirdMigration.mp4 (1280x720) [35.5 MB] || YOUTUBE_1080_BirdMigration.mp4 (1920x1080) [289.5 MB] || 14177_BirdMigration_EN.US.en_US.srt [3.9 KB] || 14177_BirdMigration_EN.US.en_US.vtt [3.7 KB] || ",
            "hits": 67
        },
        {
            "id": 13848,
            "url": "https://svs.gsfc.nasa.gov/13848/",
            "result_type": "Produced Video",
            "release_date": "2021-04-29T11:00:00-04:00",
            "title": "NASA Sees Tides Under the Ocean’s Surface",
            "description": "Internal tides, or internal waves, can reach hundreds of feet underneath the ocean surface, but might only be a few inches high on the surface. Even though they're underwater, NASA can see these tides from satellites. They provide oceanographers with a unique way to map and study the much larger internal water motion. || ",
            "hits": 53
        },
        {
            "id": 12560,
            "url": "https://svs.gsfc.nasa.gov/12560/",
            "result_type": "Produced Video",
            "release_date": "2017-04-26T16:00:00-04:00",
            "title": "Tsunami Study Challenges Long-held Formation Theory",
            "description": "Music: A World to Rebuild by Brice de Margerie [SACEM]Complete transcript available. || LARGE_MP4-12560_tsunami_large.00165_print.jpg (1024x576) [77.5 KB] || LARGE_MP4-12560_tsunami_large.00165_searchweb.png (320x180) [60.6 KB] || LARGE_MP4-12560_tsunami_large.00165_thm.png (80x40) [4.9 KB] || WEBM-12560_tsunami.webm (960x540) [32.1 MB] || LARGE_MP4-12560_tsunami_large.mp4 (1280x720) [81.0 MB] || APPLE_TV-12560_tsunami_appletv.m4v (1280x720) [40.5 MB] || APPLE_TV-12560_tsunami_appletv_subtitles.m4v (1280x720) [40.5 MB] || YOUTUBE_HQ-12560_tsunami_youtube_hq.mov (1280x720) [108.4 MB] || NASA_TV-12560_tsunami.mpeg (1280x720) [268.1 MB] || 12560_tsunami.en_US.srt [1000 bytes] || 12560_tsunami.en_US.vtt [1011 bytes] || NASA_PODCAST-12560_tsunami_ipod_sm.mp4 (320x240) [13.1 MB] || ",
            "hits": 47
        },
        {
            "id": 12550,
            "url": "https://svs.gsfc.nasa.gov/12550/",
            "result_type": "Produced Video",
            "release_date": "2017-03-30T09:00:00-04:00",
            "title": "Rossby Waves on the Sun Could Aid in Space Weather Prediction",
            "description": "Music: Grand Design by Michael ConnComplete transcript available. || 12550_Rossby_Waves_MASTER_prores.00696_print.jpg (1024x576) [127.0 KB] || 12550_Rossby_Waves_MASTER_prores.00696_searchweb.png (320x180) [53.3 KB] || 12550_Rossby_Waves_MASTER_prores.00696_thm.png (80x40) [4.8 KB] || 12550_Rossby_Waves_MASTER_prores.mov (1280x720) [656.3 MB] || 12550_Rossby_Waves_MASTER_youtube_hq.mov (1920x1080) [165.2 MB] || 12550_Rossby_Waves_MASTER_appletv.m4v (1280x720) [19.9 MB] || 12550_Rossby_Waves_MASTER.mpeg (1280x720) [158.7 MB] || 12550_Rossby_Waves_MASTER_appletv_subtitles.m4v (1280x720) [20.0 MB] || 12550_Rossby_Waves_MASTER_youtube_hq.en_US.srt [763 bytes] || 12550_Rossby_Waves_MASTER_youtube_hq.en_US.vtt [776 bytes] || 12550_Rossby_Waves_MASTER_ipod_sm.mp4 (320x240) [7.4 MB] || 12550_Rossby_Waves_MASTER_prores.webm [0 bytes] || ",
            "hits": 35
        },
        {
            "id": 30504,
            "url": "https://svs.gsfc.nasa.gov/30504/",
            "result_type": "Hyperwall Visual",
            "release_date": "2014-05-13T00:00:00-04:00",
            "title": "Wind-Blown Marine Debris from Japanese Tsunami",
            "description": "On Friday, March 11, 2011, a magnitude 9.0 undersea megathrust earthquake struck off the Pacific coast of Japan that generated tsunami waves that reached 40.5 meters (~133 feet) high, traveling up to 10 kilometers (6 miles) inland in some areas (e.g., Sendai). The earthquake and resulting tsunami generated an estimated 24-25 million tons of rubble and debris in Japan. This simulation shows how winds near the ocean surface impacted the movement of marine debris as they moved across the Pacific from March 2011 to July 2012. The colors show the percentage of windage, or the amount of force (i.e., wind) created on an object by friction. Objects that float mostly above water are more impacted by the speed of the wind than the speed of the water; therefore, they have high windage values (orange and red shades). These objects move more quickly than objects that float mostly below water that are impacted more by the speed of the water and thus have low windage values (purple and blue shades). The results were used to assess the location of the tsunami debris in the ocean and the timeline of its arrival on the west coast of the United States. The International Pacific Research Center, Surface Currents Diagnostic model was used to run the simulation. || ",
            "hits": 62
        },
        {
            "id": 11204,
            "url": "https://svs.gsfc.nasa.gov/11204/",
            "result_type": "Produced Video",
            "release_date": "2013-03-14T14:30:00-04:00",
            "title": "Jupiter's Hot Spots",
            "description": "Jupiter's bright Equatorial Zone swirls with dark patches, dubbed \"hot spots\" for their infrared glow. These holes in the ammonia clouds at the top of the atmosphere allow a glimpse into Jupiter's darker, hotter layers below. In 1995 NASA's Galileo spacecraft dropped a probe directly into a hot spot, taking the first and only in situ measurements of Jupiter's atmosphere. Now, movies recorded by NASA's Cassini spacecraft reveal that hot spots are not just local weather phenomena, but are in fact linked to much larger-scale atmospheric structures called Rossby waves. || ",
            "hits": 47
        },
        {
            "id": 11003,
            "url": "https://svs.gsfc.nasa.gov/11003/",
            "result_type": "Produced Video",
            "release_date": "2012-06-19T00:00:00-04:00",
            "title": "Excerpt from \"Dynamic Earth\"",
            "description": "A giant explosion of magnetic energy from the sun, called a coronal mass ejection, slams into and is deflected completely by the Earth's powerful magnetic field. The sun also continually sends out streams of light and radiation energy. Earth's atmosphere acts like a radiation shield, blocking quite a bit of this energy.Much of the radiation energy that makes it through is reflected back into space by clouds, ice and snow and the energy that remains helps to drive the Earth system, powering a remarkable planetary engine — the climate. It becomes the energy that feeds swirling wind and ocean currents as cold air and surface waters move toward the equator and warm air and water moves toward the poles — all in an attempt to equalize temperatures around the world.A jury appointed by the National Science Foundation (NSF) and Science magazine has selected \"Excerpt from Dynamic Earth\" as the winner of the 2013 NSF International Science and Engineering Visualization Challenge for the Video category. This animation will be highlighted in the February 2014 special section of Science and will be hosted on ScienceMag.org and NSF.govThis animation was selected for the Computer Animation Festival's Electronic Theater at the Association for Computer Machinery's Special Interest Group on Computer Graphics and Interactive Techniques (SIGGRAPH), a prestigious computer graphics and technical research forum. This is an excerpt from the fulldome, high-resolution show 'Dynamic Earth: Exploring Earth's Climate Engine.' The Dynamic Earth dome show was selected as a finalist in the Jackson Hole Wildlife Film Festival Science Media Awards under the category \"Best Immersive Cinema - Fulldome\". || ",
            "hits": 114
        },
        {
            "id": 10927,
            "url": "https://svs.gsfc.nasa.gov/10927/",
            "result_type": "Produced Video",
            "release_date": "2012-03-13T13:00:00-04:00",
            "title": "RATTLING JET STREAM ON JUPITER",
            "description": "New movies of Jupiter are the first to catch an invisible wave shaking up one of the giant planet's jet streams, an interaction that also takes place in Earth's atmosphere and influences the weather.For complete transcript, click here. || G2012-013_Jupiter_Weather_portal.00752_print.jpg (1024x576) [69.0 KB] || G2012-013_Jupiter_Weather_portal_web.png (320x180) [190.6 KB] || G2012-013_Jupiter_Weather_portal_thm.png (80x40) [16.5 KB] || G2012-013_Jupiter_Weather.wmv (1280x720) [62.8 MB] || G2012-013_Jupiter_Weather_youtube_hq.mov (1280x720) [70.4 MB] || G2012-013_Jupiter_Weather_appletv.m4v (960x540) [56.5 MB] || G2012-013_Jupiter_Weather_appletv.webmhd.webm (960x540) [27.4 MB] || G2012-013_Jupiter_Weather_portal.mov (640x360) [53.2 MB] || G2012-013_Jupiter_Weather_ipod_lg.m4v (640x360) [22.3 MB] || GSFC_20120313_Jupiter_m10927_Weather.en_US.vtt [2.7 KB] || G2012-013_Jupiter_Weather_prores.mov (1280x720) [1.9 GB] || G2012-013_Jupiter_Weather_ipod_sm.mp4 (320x240) [11.7 MB] || ",
            "hits": 56
        },
        {
            "id": 10737,
            "url": "https://svs.gsfc.nasa.gov/10737/",
            "result_type": "Produced Video",
            "release_date": "2011-08-05T00:00:00-04:00",
            "title": "Tohoku Tsunami Creates Antarctic Icebergs",
            "description": "Nearly 50 square miles of ice broke off the Sulzberger Ice Shelf on the coast of Antarctica, resulting from waves generated by the Tohoku earthquake and tsunami that struck Japan in March 2011. || ",
            "hits": 44
        }
    ]
}