{ "count": 22, "next": null, "previous": null, "results": [ { "id": 40507, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Heliophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 186 }, { "id": 40449, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-science-stories2023/", "result_type": "Gallery", "release_date": "2023-01-04T00:00:00-05:00", "title": "Hyperwall Science Stories Products", "description": "The Science Support Office creates a variety of printed products to highlight and support NASA Science. You can find more information on the visualizations featured on each in the sections below. Visit svs.gsfc.nasa.gov to see the full catalog.", "hits": 3 }, { "id": 4971, "url": "https://svs.gsfc.nasa.gov/4971/", "result_type": "Visualization", "release_date": "2022-06-07T10:00:00-04:00", "title": "Monitoring Changing Waters using the Gulf of Maine Atlantic Time Series (GNATS)", "description": "Visualization of 20 years of data from the Gulf of Maine North Atlantic Time Series (GNATS). The data shown are temperatures at the water's surface and below the surface. Satellite based sea surface temperatures are also shown. This version does not include date or color bar overlays. || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_print.jpg (1024x576) [149.8 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_thm.png (80x40) [6.1 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_searchweb.png (320x180) [73.4 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458.02970_web.png (320x180) [73.4 KB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_1080p29.97.mp4 (1920x1080) [76.4 MB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_1080p29.97.webm (1920x1080) [12.0 MB] || 3840x2160_16x9_60p (3840x2160) [1.0 MB] || 9600x3240_16x9_30p (9600x3240) [1.0 MB] || ship_tracks.00341_FINAL_RfH24.3_H19_2022-02-23_1458_2160p59.94.mp4 (3840x2160) [249.3 MB] || preview_5x3_hyperwall_gulf_of_maine.mp4 (2400x810) [129.1 MB] || ", "hits": 130 }, { "id": 13557, "url": "https://svs.gsfc.nasa.gov/13557/", "result_type": "Produced Video", "release_date": "2020-02-24T11:00:00-05:00", "title": "Placing the Recent Hiatus Period in an Energy Balance Perspective", "description": "GLOBAL OBSERVATIONS OF EARTH’S ENERGY BALANCE With the launch of NASA’s Terra Satellite Earth Observing System on Dec. 18, 1999, and subsequent ‘first light’ of the Cloud’s and the Earth’s Energy Radiant System (CERES) instrument on February 26, 2000, NASA gave birth to what ultimately would become the first long-term global observational record of Earth’s energy balance. This key indicator of the climate system describes the delicate and complex balance between how much of the sun’s energy reaching Earth is absorbed and how much thermal infrared radiation is emitted back to space. “Absorbed solar radiation fuels the climate system and life on our planet,” said Norman Loeb, CERES Principal Investigator. “The Earth sheds heat by emitting outgoing radiation.” || ", "hits": 216 }, { "id": 40359, "url": "https://svs.gsfc.nasa.gov/gallery/sdostillsand-graphics/", "result_type": "Gallery", "release_date": "2018-09-13T10:02:59-04:00", "title": "SDO: Stills and Graphics", "description": "No description available.", "hits": 249 }, { "id": 40357, "url": "https://svs.gsfc.nasa.gov/gallery/sdo4k-content/", "result_type": "Gallery", "release_date": "2018-09-13T09:22:28-04:00", "title": "SDO: 4k Content", "description": "Since 2010, the Solar Dynamics Observatory has taken 60 million images of the sun and 2 comets. Here are a few of our favorites.", "hits": 241 }, { "id": 40356, "url": "https://svs.gsfc.nasa.gov/gallery/sdovisualizations/", "result_type": "Gallery", "release_date": "2018-09-07T00:00:00-04:00", "title": "SDO: Visualizations", "description": "No description available.", "hits": 79 }, { "id": 40358, "url": "https://svs.gsfc.nasa.gov/gallery/sdopresentation-resources/", "result_type": "Gallery", "release_date": "2018-09-07T00:00:00-04:00", "title": "SDO: Presentation Resources", "description": "No description available.", "hits": 69 }, { "id": 40339, "url": "https://svs.gsfc.nasa.gov/gallery/visualization-principles/", "result_type": "Gallery", "release_date": "2017-11-06T00:00:00-05:00", "title": "The Curious World of Scientific Visualization", "description": "Explore data brought to life by NASA’s artists and scientists\r\rData Brought to Life\rData is only as powerful as our ability to make sense of it. The right tools can help us find meaning in a trove of information and experience the wonder in it. When artists and scientists work in concert, they unearth stories within datasets and push the boundaries of knowledge. This collaboration is both a creative process and a mathematical one. Scientific visualization is not a mere translation of numbers into pictures: shapes and colors breathe life into real scientific data, allowing us to see patterns and complexities that were once invisible or unknown. The visualization itself becomes a vehicle for scientific inquiry, capturing the curiosity of both artist and scientist. When shared with the world, these data-driven artworks inspire as much as they educate and entertain. Scientific visualization reminds us of the beauty in understanding, and it is a means of discovery all its own. \r\rScientific Visualization at NASA\rAt NASA’s Goddard Space Flight Center, scientists work alongside a team of artists to extend their research into the visual space. The Scientific Visualization Studio creates animations and videos that showcase the latest discoveries in Earth and space sciences. These visualizations are both insightful tools for the NASA research community and accessible science stories designed to be enjoyed by people of all walks of life. As one of NASA’s leading outreach efforts, the Scientific Visualization Studio empowers scientists to share their work with as wide an audience as possible, in the most creative and engaging way possible. \r", "hits": 181 }, { "id": 40302, "url": "https://svs.gsfc.nasa.gov/gallery/svsyoutube-candidates/", "result_type": "Gallery", "release_date": "2016-06-03T00:00:00-04:00", "title": "SVS YouTube Candidates", "description": "These are the proposed visualization candidates to be included in the SVS YouTube Channel.", "hits": 213 }, { "id": 40263, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-20150910/", "result_type": "Gallery", "release_date": "2015-10-19T00:00:00-04:00", "title": "Hyperwall 10 Sep 2015", "description": "Content from the September 10, 2015 Hyperwall Content News mailing list", "hits": 4 }, { "id": 40254, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-heliophysics/", "result_type": "Gallery", "release_date": "2015-09-04T00:00:00-04:00", "title": "Hyperwall Heliophysics", "description": "A topically-organized Gallery of Hyperwall-ready heliophysics content.", "hits": 104 }, { "id": 40245, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/", "result_type": "Gallery", "release_date": "2015-07-30T00:00:00-04:00", "title": "Hyperwall Sun", "description": "Heliophysics related hyperwall ready visualizations\nReturn to Main Hyperwall Gallery.", "hits": 9 }, { "id": 30499, "url": "https://svs.gsfc.nasa.gov/30499/", "result_type": "Hyperwall Visual", "release_date": "2014-05-13T00:00:00-04:00", "title": "Ocean Salinity and Daily Argo Coverage", "description": "Salinity has been measured at sea for centuries, first using buckets to collect samples, and later (within the past few decades) with instruments known as “CTDs,” which simultaneously measure conductivity (as a proxy for salinity), temperature, and ocean depth (based on pressure). This technology is used to provide single point samples throughout the ocean. The Argo program has over 3500 profiling floats with CTDs currently deployed in all ocean basins. The Argo array of profiling floats is the first attempt to monitor the global subsurface (upper 2000 meters) ocean temperature and salinity fields in real time. The first floats were deployed in late 1999 and it took another 8 years to reach the global target of 3000 operating floats delivering data every 10 days. While ~3500 floats seem like a lot, on a daily basis the ocean is still very undersampled.This visualization shows ocean salinity at 150 meters as derived by an eddy-resolving ocean model. The gray dots represent the daily locations of Argo floats from January 1993 to December 2010. Ocean salinity and temperature data from Argo floats have proved extremely useful, and can be used in combination with data from other sources (such as from NASA’s Aquarius mission and other satellite missions) to observe and model long-term ocean signals related to climate change. || ", "hits": 139 }, { "id": 4128, "url": "https://svs.gsfc.nasa.gov/4128/", "result_type": "Visualization", "release_date": "2013-12-24T00:00:00-05:00", "title": "Solar Dynamics Observatory - Argo view - Slices of SDO", "description": "Argos (or Argus Panoptes) was the 100-eyed giant in Greek mythology (wikipedia).While the Solar Dynamics Observatory (SDO) has significantly less than 100 eyes, (see \"SDO Jewelbox: The Many Eyes of SDO\"), seeing connections in the solar atmosphere through the many filters of SDO presents a number of interesting challenges. This visualization experiment illustrates a mechanism for highlighting these connections. This visualization is a variation of the original Solar Dynamics Observatory - Argo view. In this case, the different wavelength filters are presented in three sets around the Sun at full 4Kx4K resolution. This enables monitoring of changes in time over all wavelengths at any location around the limb of the Sun. The wavelengths presented are: 617.3nm optical light from SDO/HMI. From SDO/AIA we have 170nm (pink), then 160nm (green), 33.5nm (blue), 30.4nm (orange), 21.1nm (violet), 19.3nm (bronze), 17.1nm (gold), 13.1nm (aqua) and 9.4nm (green).We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear in different wavelengths.Filaments extending off the limb of the Sun which are bright in 30.4 nanometers, appear dark in many other wavelengths.Sunspots which appear dark in optical wavelengths, are festooned with glowing ribbons in ultraviolet wavelengths.small flares, invisible in optical wavelengths, are bright ribbons in ultraviolet wavelengths.if we compare the visible light limb of the Sun with the 170 nanometer filter on the left, with the visible light limb and the 9.4 nanometer filter on the right, we see that the 'edge' is at different heights. This effect is due to the different amounts of absorption, and emission, of the solar atmosphere in ultraviolet light.in far ultraviolet light, the photosphere is dark since the black-body spectrum at a temperature of 5700 Kelvin emits very little light in this wavelength. || ", "hits": 69 }, { "id": 4117, "url": "https://svs.gsfc.nasa.gov/4117/", "result_type": "Visualization", "release_date": "2013-12-17T10:00:00-05:00", "title": "Solar Dynamics Observatory - Argo view", "description": "Argos (or Argus Panoptes) was the 100-eyed giant in Greek mythology (wikipedia).While the Solar Dynamics Observatory (SDO) has significantly less than 100 eyes, (see \"SDO Jewelbox: The Many Eyes of SDO\"), seeing connections in the solar atmosphere through the many filters of SDO presents a number of interesting challenges. This visualization experiment illustrates a mechanism for highlighting these connections.The wavelengths presented are: 617.3nm optical light from SDO/HMI. From SDO/AIA we have 170nm (pink), then 160nm (green), 33.5nm (blue), 30.4nm (orange), 21.1nm (violet), 19.3nm (bronze), 17.1nm (gold), 13.1nm (aqua) and 9.4nm (green).We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear in different wavelengths.Filaments extending off the limb of the Sun which are bright in 30.4 nanometers, appear dark in many other wavelengths.Sunspots which appear dark in optical wavelengths, are festooned with glowing ribbons in ultraviolet wavelengths.Small flares, invisible in optical wavelengths, are bright ribbons in ultraviolet wavelengths.If we compare the visible light limb of the Sun with the 170 nanometer filter on the left, with the visible light limb and the 9.4 nanometer filter on the right, we see that the 'edge' is at different heights. This effect is due to the different amounts of absorption, and emission, of the solar atmosphere in ultraviolet light.In far ultraviolet light, the photosphere is dark since the black-body spectrum at a temperature of 5700 Kelvin emits very little light in this wavelength. || ", "hits": 88 }, { "id": 11385, "url": "https://svs.gsfc.nasa.gov/11385/", "result_type": "Produced Video", "release_date": "2013-12-17T10:00:00-05:00", "title": "Jewel Box Sun", "description": "Telescopes help distant objects appear bigger, but this is only one of their advantages. Telescopes can also collect light in ranges that our eyes alone cannot see, providing scientists ways of observing a whole host of material and processes that would otherwise be inaccessible. A new NASA movie of the sun based on data from NASA's Solar Dynamics Observatory, or SDO, shows the wide range of wavelengths – invisible to the naked eye – that the telescope can view. SDO converts the wavelengths into an image humans can see, and the light is colorized into a rainbow of colors. As the colors sweep around the sun in the movie, viewers should note how different the same area of the sun appears. This happens because each wavelength of light represents solar material at specific temperatures. Different wavelengths convey information about different components of the sun's surface and atmosphere, so scientists use them to paint a full picture of our constantly changing and varying star.Yellow light of 5800 angstroms, for example, generally emanates from material of about 10,000 degrees F (5700 degrees C), which represents the surface of the sun. Extreme ultraviolet light of 94 angstroms, which is typically colorized in green in SDO images, comes from atoms that are about 11 million degrees F (6,300,000 degrees C) and is a good wavelength for looking at solar flares, which can reach such high temperatures. By examining pictures of the sun in a variety of wavelengths – as is done not only by SDO, but also by NASA's Interface Region Imaging Spectrograph, NASA's Solar Terrestrial Relations Observatory and the European Space Agency/NASA Solar and Heliospheric Observatory — scientists can track how particles and heat move through the sun's atmosphere. || ", "hits": 106 }, { "id": 40083, "url": "https://svs.gsfc.nasa.gov/gallery/aquarius/", "result_type": "Gallery", "release_date": "2010-11-30T00:00:00-05:00", "title": "Aquarius Mission", "description": "During its nominal three-year mission, Aquarius will map the\rsalinity at the ocean surface to improve our understanding of\rEarth's water cycle and ocean circulation. Aquarius will help\rscientists see how freshwater moves between the ocean and\rthe atmosphere. It will monitor changes in the water cycle due\rto rainfall, evaporation, ice melting, and river runoff.", "hits": 101 }, { "id": 40043, "url": "https://svs.gsfc.nasa.gov/gallery/hurricane-resources/", "result_type": "Gallery", "release_date": "2010-03-08T00:00:00-05:00", "title": "Hurricane Resources", "description": "No description available.", "hits": 150 }, { "id": 20146, "url": "https://svs.gsfc.nasa.gov/20146/", "result_type": "Animation", "release_date": "2008-07-22T12:00:00-04:00", "title": "ARGO Buoy Animations", "description": "The ARGO buoy: it works in conjunction with many others of its kind (in an array) to collect data about ocean currents. || ", "hits": 17 }, { "id": 3205, "url": "https://svs.gsfc.nasa.gov/3205/", "result_type": "Visualization", "release_date": "2005-07-29T00:00:00-04:00", "title": "ARGO Float Animation #2", "description": "This visualization shows the locations of the ARGO buoy array over time. When the buoys above water, the lines are brighter; when the buoys are under water, the lines are fainter. The ARGO buoys measure ocean salinity, column temperature, and current velocities. This version of the visualization uses a faster camera move than version #1 (animation 3204). || ", "hits": 33 }, { "id": 3204, "url": "https://svs.gsfc.nasa.gov/3204/", "result_type": "Visualization", "release_date": "2005-07-28T11:00:00-04:00", "title": "ARGO Float Animation #1", "description": "This visualization shows the locations of the ARGO buoy array over time. When the buoys are above water, the lines are brighter; when the buoys are under water, the lines are fainter. The ARGO buoys measure ocean salinity, column temperature, and current velocities. This version of the visualization uses a slow camera move. || ", "hits": 75 } ] }