{ "count": 15, "next": null, "previous": null, "results": [ { "id": 14631, "url": "https://svs.gsfc.nasa.gov/14631/", "result_type": "Produced Video", "release_date": "2024-07-22T11:00:00-04:00", "title": "Model Behavior: Visualizing Global CO2", "description": "Universal Production Music: Prismatic by David Stephen Goldsmith [ PRS ]Complete transcript available. || 14631_DYAMONDThumbnailHorz.jpg (1280x720) [291.1 KB] || 14631_DYAMONDThumbnailHorz_print.jpg (1024x576) [222.2 KB] || 14631_DYAMONDThumbnailHorz_searchweb.png (320x180) [91.4 KB] || 14631_DYAMONDThumbnailHorz_thm.png (80x40) [7.1 KB] || 14631_dyamondhorz_US.en.en_US.srt [2.3 KB] || 14631_dyamondhorz_US.en.en_US.vtt [2.2 KB] || 14631_DYAMOND_Horz.webm (3840x2160) [32.4 MB] || 14631_DYAMOND_Horz.mp4 (3840x2160) [267.6 MB] || ", "hits": 366 }, { "id": 14134, "url": "https://svs.gsfc.nasa.gov/14134/", "result_type": "Produced Video", "release_date": "2022-05-02T13:00:00-04:00", "title": "NASA Simulation Suggests Some Volcanoes Might Warm Climate, Destroy Ozone Layer", "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Good Omens\" by Count Zero and Rohan Stevenson and \"Blue Moons\" by Gresby Race Nash of Universal Production Music || 14134_thumb.jpg (1920x1080) [450.5 KB] || volcanism_14134.00242_searchweb.png (320x180) [71.1 KB] || volcanism_14134.00242_thm.png (80x40) [5.5 KB] || volcanism_14134.mp4 (1920x1080) [377.7 MB] || volcanism_14134.webm (1920x1080) [27.0 MB] || volcanism_14134_caption.en_US.srt [4.9 KB] || volcanism_14134_caption.en_US.vtt [4.7 KB] || ", "hits": 78 }, { "id": 4987, "url": "https://svs.gsfc.nasa.gov/4987/", "result_type": "Visualization", "release_date": "2022-04-28T11:00:00-04:00", "title": "Fast Magnetic Reconnection and the Hall Effect", "description": "Magnetic reconnection is one of the most complex processes known for converting energy from magnetic fields to particle motion. It takes place in solar flares and regions of planetary (and stellar) magnetospheres. Having been studied since the 1950s, many details of the process are still undergoing study.One of the key components in magnetic reconnection is the collision of two magnetic field regions with opposite-directed field lines, imbedded in a plasma. The field and plasma combination forms an X-shaped configuration at their closest, and most intense point.These visualizations are plotted from a reconnection model generated by VPIC (Vector Particle-In-Cell) code. Quantities are plotted in 'dimensionless' coordinates, that are normalized to the ion inertial length (di). || ", "hits": 172 }, { "id": 14116, "url": "https://svs.gsfc.nasa.gov/14116/", "result_type": "Produced Video", "release_date": "2022-03-18T00:00:00-04:00", "title": "Two Scientists Have a Frank and Honest Discussion about Antarctica", "description": "NASA Glaciologists Kelly Brunt and Alex Gardner discuss the history, challenges and evolution of mapping the Antarctic continent and what it means for science and society. || ", "hits": 43 }, { "id": 13954, "url": "https://svs.gsfc.nasa.gov/13954/", "result_type": "Produced Video", "release_date": "2021-10-06T04:00:00-04:00", "title": "With NASA Data, Researchers Find Standing Waves at Edge of Earth’s Magnetic Bubble", "description": "Earth sails the solar system in a ship of its own making: the magnetosphere, the magnetic field that envelops and protects our planet. The celestial sea we find ourselves in is filled with charged particles flowing from the Sun, known as the solar wind. Just as ocean waves follow the wind, scientists expected that waves traveling along the magnetosphere should ripple in the direction of the solar wind. But a new study reveals some waves do just the opposite.Studying these magnetospheric waves, which transport energy, helps scientists understand the complicated ways that solar activity plays out in the space around Earth. Changing conditions in space driven by the Sun are known as space weather. That weather can impact our technology from communications satellites in orbit to power lines on the ground. “Understanding the boundaries of any system is a key problem,” said Martin Archer, a space physicist at Imperial College London who led the new study, published today in Nature Communications. “That’s how stuff gets in: energy, momentum, matter.” || ", "hits": 192 }, { "id": 13753, "url": "https://svs.gsfc.nasa.gov/13753/", "result_type": "Produced Video", "release_date": "2020-11-17T11:00:00-05:00", "title": "NASA Studies How COVID-19 Shutdowns Affect Emissions", "description": "Music: \"Lab Analysis\" from Universal Production MusicComplete transcript available.Coming soon to our YouTube channel. || Screen_Shot_2020-11-13_at_1.08.17_PM_print.jpg (1024x572) [164.1 KB] || Screen_Shot_2020-11-13_at_1.08.17_PM.png (3568x1994) [6.4 MB] || Screen_Shot_2020-11-13_at_1.08.17_PM_searchweb.png (320x180) [85.1 KB] || Screen_Shot_2020-11-13_at_1.08.17_PM_thm.png (80x40) [9.8 KB] || NASA_Studies_How_COVID-19_Shutdowns_Affect_Emissions.mp4 (1920x1080) [442.5 MB] || NASA_Studies_How_COVID-19_Shutdowns_Affect_Emissions.webm (1920x1080) [25.9 MB] || COVIDNO2.en_US.srt [4.4 KB] || COVIDNO2.en_US.vtt [4.4 KB] || ", "hits": 91 }, { "id": 4872, "url": "https://svs.gsfc.nasa.gov/4872/", "result_type": "Visualization", "release_date": "2020-11-17T00:00:00-05:00", "title": "Deviation of Modeled Normal Pollution Levels from Measurements Following COVID-19 Lockdown", "description": "Deviation from modeled normal nitrogen dioxide levels after COVID-19 lockdowns || covid_19_7_day_no2.0810_print.jpg (1024x576) [207.7 KB] || covid_19_7_day_no2.0810_searchweb.png (320x180) [83.4 KB] || covid_19_7_day_no2.0810_thm.png (80x40) [6.4 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || covid_19_7_day_no2_1080p30.mp4 (1920x1080) [25.3 MB] || covid_19_7_day_no2_1080p30.webm (1920x1080) [5.0 MB] || covid_19_7_day_no2_1080p30.mp4.hwshow [192 bytes] || ", "hits": 38 }, { "id": 13685, "url": "https://svs.gsfc.nasa.gov/13685/", "result_type": "Produced Video", "release_date": "2020-08-12T11:00:00-04:00", "title": "5 Things that Changed Weather Forecasting Forever", "description": "Complete transcript available.Watch this video on the NASA Goddard YouTube Channel || Weather_forecasting_history_FINAL_smallest.00180_print.jpg (1024x576) [114.4 KB] || Weather_forecasting_history_FINAL_smallest.00180_searchweb.png (320x180) [43.1 KB] || Weather_forecasting_history_FINAL_smallest.00180_web.png (320x180) [43.1 KB] || Weather_forecasting_history_FINAL_smallest.00180_thm.png (80x40) [3.0 KB] || Weather_forecasting_history_FINAL_smallest.mp4 (1920x1080) [653.6 MB] || Weather_forecasting_history_FINAL_smaller.mp4 (1920x1080) [1.1 GB] || Weather_forecasting_history_FINAL_smallest.webm (1920x1080) [123.4 MB] || Weather_forecasting_history_FINAL.mp4 (3840x2160) [1.2 GB] || Weather_forecasting_final.en_US.vtt [22.5 KB] || Weather_forecasting_final_corrected.en_US.srt [21.7 KB] || Weather_forecasting_final_corrected.en_US.vtt [21.6 KB] || ", "hits": 40 }, { "id": 13580, "url": "https://svs.gsfc.nasa.gov/13580/", "result_type": "Produced Video", "release_date": "2020-04-14T10:30:00-04:00", "title": "NASA Models the Complex Chemistry of Earth's Atmosphere", "description": "Music: \"Interconnecting Threads\" by Axel Tenner [GEMA]; \"Night Drift\" by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS], from Universal Production MusicWatch this video on the NASA Goddard YouTube channel. Complete transcript available. || ChemicalSpecies_Still_print.jpg (1024x576) [313.1 KB] || ChemicalSpecies_Still.jpg (3840x2160) [2.0 MB] || ChemicalSpecies_Still_searchweb.png (320x180) [104.5 KB] || ChemicalSpecies_Still_web.png (320x180) [104.5 KB] || ChemicalSpecies_Still_thm.png (80x40) [7.8 KB] || 13580_ChemSpecies_Final.mov (1920x1080) [1.8 GB] || 13580_ChemSpecies_Final_lowres.mp4 (1280x720) [82.5 MB] || 13580_ChemSpecies_Final.mp4 (1920x1080) [467.4 MB] || 13580_ChemSpecies_Final.webm (1920x1080) [2.7 MB] || ChemicalSpecies.en_US.srt [4.2 KB] || ChemicalSpecies.en_US.vtt [4.2 KB] || ", "hits": 50 }, { "id": 13559, "url": "https://svs.gsfc.nasa.gov/13559/", "result_type": "Produced Video", "release_date": "2020-03-23T10:00:00-04:00", "title": "NASA Models Methane Sources and Movement Around the Globe", "description": "Complete transcript available.Music: \"Reported Missing\" by Andrew Michael Britton [PRS] and David Stephen Goldsmith [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 Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html. || Methane_Still.jpg (1920x1080) [408.5 KB] || Methane_Still_print.jpg (1024x576) [181.8 KB] || Methane_Still_searchweb.png (180x320) [71.4 KB] || Methane_Still_web.png (320x180) [71.4 KB] || Methane_Still_thm.png (80x40) [6.4 KB] || 13559_Methane_Final.webm (960x540) [62.2 MB] || TWITTER_720_13559_Methane_Final_twitter_720.mp4 (1280x720) [28.5 MB] || 13559_Methane_Final_lowres.mp4 (1280x720) [43.6 MB] || 13559_Methane_Final.mp4 (1920x1080) [272.5 MB] || Mathen_captions.en_US.srt [3.2 KB] || Mathen_captions.en_US.vtt [3.3 KB] || 13559_Methane_Final.mov (1920x1080) [3.4 GB] || ", "hits": 74 }, { "id": 13567, "url": "https://svs.gsfc.nasa.gov/13567/", "result_type": "Produced Video", "release_date": "2020-03-06T09:00:00-05:00", "title": "How Does NASA Model Atmospheric Patterns?", "description": "Music: Favor by Victor Maitre [SACEM]Complete transcript available. || GMAOThumb.jpg (1920x1080) [251.3 KB] || GMAOThumb_print.jpg (1024x576) [131.2 KB] || GMAOThumb_searchweb.png (180x320) [82.2 KB] || GMAOThumb_web.png (320x180) [82.2 KB] || GMAOThumb_thm.png (80x40) [6.4 KB] || 13567_GMAO_Atmospheric_Model.mp4 (1920x1080) [88.5 MB] || 13567_GMAO_Atmospheric_Model.webm (1920x1080) [10.2 MB] || 13567_GMAO_Atmospheric_Model.mov (1920x1080) [673.0 MB] || captions.en_US.srt [1.3 KB] || captions.en_US.vtt [1.4 KB] || ", "hits": 31 }, { "id": 13233, "url": "https://svs.gsfc.nasa.gov/13233/", "result_type": "Produced Video", "release_date": "2019-06-19T14:00:00-04:00", "title": "Modeling the Future of the Greenland Ice Sheet", "description": "Music: Tides by Jon Cotton [PRS], Ben Niblett [PRS]Complete transcript available. || Greenland_Still_Two.jpg (1920x1080) [941.0 KB] || Greenland_Still_Two_searchweb.png (320x180) [152.3 KB] || Greenland_Still_Two_thm.png (80x40) [8.8 KB] || 13233_Greenland_Outlet_FINAL.mp4 (1920x1080) [253.2 MB] || 13233_Greenland_Outlet_FINAL.mov (1920x1080) [3.4 GB] || 13233_Greenland_Outlet_FINAL.webm (1920x1080) [17.2 MB] || 13233_Greenland_Outlet_FINAL_VX-303985.webm (960x540) [54.0 MB] || GreenlandOutletModel_Fine_V2.en_US.srt [2.9 KB] || GreenlandOutletModel_Fine_V2.en_US.vtt [2.9 KB] || ", "hits": 105 }, { "id": 12927, "url": "https://svs.gsfc.nasa.gov/12927/", "result_type": "Produced Video", "release_date": "2018-04-16T12:00:00-04:00", "title": "Looking at the Corona with WISPR on Parker Solar Probe", "description": "The Wide-Field Imager for Solar Probe, or WISPR, is aboard NASA’s Parker Solar Probe to take images of the solar corona (the Sun’s atmosphere) and inner heliosphere. WISPR’s telescopes will provide white-light images of the solar wind, shocks, solar ejecta and other structures as they approach and pass the spacecraft. Parker Solar Probe is scheduled for launch in July 2018. It will be the first spacecraft ever to fly through the solar corona to investigate the evolution of the solar wind and heating of the solar corona. WISPR does not look directly at the Sun. Its very wide field-of-view extends from 13° away from the center of the Sun to 108° from the Sun. || ", "hits": 128 }, { "id": 30912, "url": "https://svs.gsfc.nasa.gov/30912/", "result_type": "Hyperwall Visual", "release_date": "2017-11-13T00:00:00-05:00", "title": "2017 North Atlantic Hurricane Season Simulation Compared With Observations", "description": "A video comparing model output and satellite imagery. || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000_print.jpg (1024x547) [132.7 KB] || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000.png (5760x3081) [5.8 MB] || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000_searchweb.png (320x180) [60.4 KB] || ir_compare2m-globe_F517R06K-F517R06K_20170801_0000_thm.png (80x40) [5.7 KB] || ir_compare2m-globe_720p.webm (1280x720) [16.1 MB] || ir_compare2m-globe_720p.mp4 (1280x720) [198.3 MB] || ", "hits": 15 }, { "id": 12604, "url": "https://svs.gsfc.nasa.gov/12604/", "result_type": "Produced Video", "release_date": "2017-06-22T14:00:00-04:00", "title": "Scientists Uncover Origins of Dynamic Jets on Sun's Surface", "description": "At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance, scientists didn’t understand how they form. Now, for the first time, a computer simulation — so detailed it took a full year to run — shows how spicules form, helping scientists understand how spicules can break free of the sun’s surface and surge upward so quickly. This work relied upon high-cadence observations from NASA’s Interface Region Imaging Spectrograph, or IRIS, and the Swedish 1-meter Solar Telescope in La Palma. Together, the spacecraft and telescope peer into the lower layers of the sun’s atmosphere, known as the interface region, where spicules form. The results of this NASA-funded study were published in Science on June 22, 2017 — a special time of the year for the IRIS mission, which celebrates its fourth anniversary in space on June 26.Research: On the generation of solar spicules and Alfvénic waves.Journal: Science, June 22, 2017.Link to paper: http://science.sciencemag.org/content/356/6344/1269.full || ", "hits": 54 } ] }