{ "id": 40507, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/", "page_type": "Gallery", "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.", "release_date": "2023-08-28T00:00:00-04:00", "update_date": "2025-03-20T00:00:00-04:00", "main_image": { "id": 399772, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a030900/a030998/1-SMD-FLEET_MASTER_11_23_2020_searchweb.png", "filename": "1-SMD-FLEET_MASTER_11_23_2020_searchweb.png", "media_type": "Image", "alt_text": "The full NASA Science Fleet", "width": 180, "height": 320, "pixels": 57600 }, "media_groups": [ { "id": 372263, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372263", "widget": "Basic text (large)", "title": "Overview", "caption": "", "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\"link 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.", "items": [], "extra_data": {} }, { "id": 372264, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372264", "widget": "Card gallery", "title": "Science Mission Directorate and General Heliophysics", "caption": "", "description": "General Heliophysics and visualizations that cross divisions", "items": [ { "id": 423443, "type": "details_page", "extra_data": null, "instance": { "id": 31162, "url": "https://svs.gsfc.nasa.gov/31162/", "page_type": "Hyperwall Visual", "title": "Operating and Future Science fleet", "description": "The current operational and future science fleet. || SMD_MASTER_FLEET_07_29_2024-hw_tweaks_print.jpg (1024x575) [267.6 KB] || SMD_MASTER_FLEET_07_29_2024-hw_tweaks.png (2667x1500) [5.9 MB] || SMD_MASTER_FLEET_07_29_2024-hw_tweaks_searchweb.png (320x180) [191.9 KB] || SMD_MASTER_FLEET_07_29_2024-hw_tweaks_thm.png (80x40) [98.2 KB] ||", "release_date": "2021-08-30T00:00:00-04:00", "update_date": "2026-06-04T10:22:37.914730-04:00", "main_image": { "id": 1203849, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a031100/a031162/SMD_FLEET_OPERATING_CROSS-DIRECTORATE_DEC_2025_1080p.jpg", "filename": "SMD_FLEET_OPERATING_CROSS-DIRECTORATE_DEC_2025_1080p.jpg", "media_type": "Image", "alt_text": "The current operational and future science fleet.", "width": 1920, "height": 1080, "pixels": 2073600 } } }, { "id": 413103, "type": "details_page", "extra_data": null, "instance": { "id": 30822, "url": "https://svs.gsfc.nasa.gov/30822/", "page_type": "Infographic", "title": "NASA's Heliophysics Fleet", "description": "The current Heliophysics fleet || hpd-fleet-chart-jan-2024_print.jpg (1024x576) [180.0 KB] || hpd-fleet-chart-jan-2024.png (3840x2160) [7.3 MB] || hpd-fleet-chart-jan-2024_searchweb.png (320x180) [91.3 KB] || hpd-fleet-chart-jan-2024_thm.png (80x40) [7.2 KB] || nasas-fleets-by-division-helio-jewel.hwshow [228 bytes] ||", "release_date": "2016-12-06T00:00:00-05:00", "update_date": "2026-05-13T17:20:13.717223-04:00", "main_image": { "id": 1153643, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a030800/a030822/helio-fleet-july-2024-1080p.png", "filename": "helio-fleet-july-2024-1080p.png", "media_type": "Image", "alt_text": "The current Heliophysics fleet", "width": 1920, "height": 1080, "pixels": 2073600 } } }, { "id": 413104, "type": "details_page", "extra_data": null, "instance": { "id": 4898, "url": "https://svs.gsfc.nasa.gov/4898/", "page_type": "Visualization", "title": "Heliophysics Sentinels 2022", "description": "There has been one significant change since the 2020 Heliophysics Fleet. SET has been decommissioned. As of Fall 2022, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "release_date": "2022-11-23T00:00:00-05:00", "update_date": "2025-02-02T00:15:53.838252-05:00", "main_image": { "id": 368244, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004800/a004898/Sentinels2022.Earth2Voyager.GSE.AU.clockSlate_EarthTarget.HD1080.00280_print.jpg", "filename": "Sentinels2022.Earth2Voyager.GSE.AU.clockSlate_EarthTarget.HD1080.00280_print.jpg", "media_type": "Image", "alt_text": "This visualization presents orbits of the current heliophysics satellites covering the space near Earth, through the solar system, and concluding with a view of the Voyagers, just outside the heliopause.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413105, "type": "media_group", "extra_data": null, "title": "Heliophysics Big Year Graphic Elements", "caption": "The Heliophysics Big Year is a NASA-led public engagement campaign designed to promote heliophysics broadly, make heliophysics science and information accessible to all, and showcase ongoing efforts to understand the Sun and all that it touches. We are challenging the public to participate in as many Sun science activities as possible from October 2023 to December 2024, leading up to and around solar maximum.

This page contains graphic elements for use in promotion and support of the Heliophysics Big Year. Anyone supporting the Heliophysics Big Year effort may use these resources in accordance with the guidance listed in the captions.", "instance": { "id": 859294, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014400/a014420/HBY_Identifier_Motion_ColorGlow_4kProres.00090_searchweb.png", "filename": "HBY_Identifier_Motion_ColorGlow_4kProres.00090_searchweb.png", "media_type": "Image", "alt_text": "The Heliophysics Big Year is a NASA-led public engagement campaign designed to promote heliophysics broadly, make heliophysics science and information accessible to all, and showcase ongoing efforts to understand the Sun and all that it touches. We are challenging the public to participate in as many Sun science activities as possible from October 2023 to December 2024, leading up to and around solar maximum.This page contains graphic elements for use in promotion and support of the Heliophysics Big Year. Anyone supporting the Heliophysics Big Year effort may use these resources in accordance with the guidance listed in the captions.", "width": 180, "height": 320, "pixels": 57600 } }, { "id": 413106, "type": "details_page", "extra_data": null, "instance": { "id": 30710, "url": "https://svs.gsfc.nasa.gov/30710/", "page_type": "Hyperwall Visual", "title": "Our Solar System", "description": "The 8 planets plus Pluto with planetary axis tilt || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_print.jpg (1024x576) [75.1 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_searchweb.png (320x180) [49.6 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_thm.png (80x40) [5.0 KB] || planets3x3_pluto_colorMercury_axis_tilt_720p.00001_web.png (320x180) [50.6 KB] || planets3x3_pluto_colorMercury_axis_tilt_720p.00001_thm.png (80x40) [5.0 KB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.mp4 (1920x1080) [9.2 MB] || planets3x3_pluto_colorMercury_axis_tilt_720p.mp4 (1280x720) [4.7 MB] || planets3x3_pluto_colorMercury_axis_tilt_1080p.webm (1920x1080) [2.7 MB] || planets3x3_pluto_colorMercury_axis_tilt_2160p.mp4 (3840x2160) [28.7 MB] || 3x3_pluto_tilt (4104x2304) [0 Item(s)] || 100-science-overview-001.hwshow || ", "release_date": "2016-03-15T12:00:00-04:00", "update_date": "2025-03-10T00:22:19.106978-04:00", "main_image": { "id": 427299, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a030700/a030710/planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_print.jpg", "filename": "planets3x3_pluto_colorMercury_axis_tilt_1080p.00001_print.jpg", "media_type": "Image", "alt_text": "The 8 planets plus Pluto with planetary axis tilt", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413107, "type": "details_page", "extra_data": null, "instance": { "id": 4469, "url": "https://svs.gsfc.nasa.gov/4469/", "page_type": "Visualization", "title": "Dynamic Earth-A New Beginning", "description": "The visualization 'Excerpt from \"Dynamic Earth\"' has been one of the most popular visualizations that the Scientific Visualization Studio has ever created. It's often used in presentations and Hyperwall shows to illustrate the connections between the Earth and the Sun, as well as the power of computer simulation in understanding those connections.There is one part of this visualization, however, that has always seemed a little clumsy to us. The opening shot is a pullback from the limb of the sun, where the sun is represented by a movie of 304 Angstrom images from the Solar Dynamics Observatory (SDO). It is difficult to pull back from the limb of a flat sun image and make the sun look spherical, and the problem was made more difficult because the original sun images were in a spherical dome show format. As a result, the pullback from the sun showed some odd reprojection artifacts.The best solution to this issue was to replace the existing pullout with a new one, one which pulled directly out from the center of the solar disk. For the new beginning, we chose a series of SDO images in the 171 Angstrom channel that show a visible coronal mass ejection (CME) in the lower right corner of the solar disk. Although this is not the specific CME that is seen affecting Venus and Earth later in this visualization, its presence links the SDO animation thematically to the later solar storm. The SDO images were also brightened considerably and tinted yellow to match the common perception of the Sun as a bright yellow object (even though it is actually white).Please go to the original version of this visualization to see the complete credits and additional details. || ", "release_date": "2016-06-16T15:00:00-04:00", "update_date": "2025-01-05T23:03:46.233808-05:00", "main_image": { "id": 423901, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004469/newsun.00000_print.jpg", "filename": "newsun.00000_print.jpg", "media_type": "Image", "alt_text": "This is the complete Dynamic Earth excerpt with a new beginning at 1080p and 4K resolution.This video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413108, "type": "gallery_page", "extra_data": null, "instance": { "id": 40455, "url": "https://svs.gsfc.nasa.gov/gallery/spacecraft-animations/", "page_type": "Gallery", "title": "Satellite Animations", "description": "A collection of spacecraft beauty pass animations for current missions.", "release_date": "2023-01-24T00:00:00-05:00", "update_date": "2025-02-12T00:00:00-05:00", "main_image": { "id": 369462, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020300/a020371/BurstCube_360Y_30fps_4444ProRes.00001_searchweb.png", "filename": "BurstCube_360Y_30fps_4444ProRes.00001_searchweb.png", "media_type": "Image", "alt_text": "A collection of spacecraft beauty pass animations for current missions.", "width": 180, "height": 320, "pixels": 57600 } } }, { "id": 413109, "type": "gallery_page", "extra_data": null, "instance": { "id": 40508, "url": "https://svs.gsfc.nasa.gov/gallery/launchesand-landingsonthe-hyperwall/", "page_type": "Gallery", "title": "Launches and Landings on the Hyperwall", "description": "Launches and Landings of missions across all 5 divisions", "release_date": "2023-10-04T00:00:00-04:00", "update_date": "2023-10-04T00:00:00-04:00", "main_image": { "id": 859592, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a031200/a031250/schulte-2023-egu-slide2_0015_searchweb.png", "filename": "schulte-2023-egu-slide2_0015_searchweb.png", "media_type": "Image", "alt_text": "Views of Mission Control and on Mars during Perseverance's descent", "width": 180, "height": 320, "pixels": 57600 } } }, { "id": 413110, "type": "media_group", "extra_data": null, "title": "Full Screen NASA Logo", "caption": "In order to study the Earth as a whole system and understand how it is changing, NASA develops and supports a large number of Earth observing missions. These missions provide Earth science researchers the necessary data to address key questions about global climate change. \n\n

Missions begin with a study phase during which the key science objectives of the mission are identified, and designs for spacecraft and instruments are analyzed. Following a successful study phase, missions enter a development phase whereby all aspects of the mission are developed and tested to insure it meets the mission objectives. Operating missions are those missions that are currently active and providing science data to researchers. Operating missions may be in their primary operational phase or in an extended operational phase.\n\n

Missions begin with a study phase during which the key science objectives of the mission are identified, and designs for spacecraft and instruments are analyzed. Following a successful study phase, missions enter a development phase whereby all aspects of the mission are developed and tested to insure it meets the mission objectives.", "instance": { "id": 858423, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a030000/a030065/nasalogo_searchweb.png", "filename": "nasalogo_searchweb.png", "media_type": "Image", "alt_text": "In order to study the Earth as a whole system and understand how it is changing, NASA develops and supports a large number of Earth observing missions. These missions provide Earth science researchers the necessary data to address key questions about global climate change. \n\nMissions begin with a study phase during which the key science objectives of the mission are identified, and designs for spacecraft and instruments are analyzed. Following a successful study phase, missions enter a development phase whereby all aspects of the mission are developed and tested to insure it meets the mission objectives. Operating missions are those missions that are currently active and providing science data to researchers. Operating missions may be in their primary operational phase or in an extended operational phase.\n\nMissions begin with a study phase during which the key science objectives of the mission are identified, and designs for spacecraft and instruments are analyzed. Following a successful study phase, missions enter a development phase whereby all aspects of the mission are developed and tested to insure it meets the mission objectives.", "width": 180, "height": 320, "pixels": 57600 } }, { "id": 423265, "type": "details_page", "extra_data": null, "instance": { "id": 5090, "url": "https://svs.gsfc.nasa.gov/5090/", "page_type": "Visualization", "title": "Map Projections Morph", "description": "Morphing between various map projections || projection_morph_comp.01000_print.jpg (1024x576) [139.0 KB] || projection_morph_comp.01000_searchweb.png (320x180) [77.1 KB] || projection_morph_comp.01000_thm.png (80x40) [6.6 KB] || comp (3840x2160) [0 Item(s)] || map_layer (3840x2160) [0 Item(s)] || overlay_layer (3840x2160) [0 Item(s)] || projection_morph_comp_2160p59.94_2.webm (3840x2160) [31.7 MB] || projection_morph_comp_2160p59.94_2.mp4 (3840x2160) [175.0 MB] || ", "release_date": "2023-06-07T16:00:00-04:00", "update_date": "2025-01-06T00:35:30.006918-05:00", "main_image": { "id": 855415, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005000/a005090/projection_morph_comp.01000_print.jpg", "filename": "projection_morph_comp.01000_print.jpg", "media_type": "Image", "alt_text": "Morphing between various map projections", "width": 1024, "height": 576, "pixels": 589824 } } } ], "extra_data": {} }, { "id": 372273, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372273", "widget": "Tile gallery", "title": "Eclipse", "caption": "", "description": "2023 Annular Eclipse, 2024 Total Eclipse, and beyond", "items": [ { "id": 413111, "type": "details_page", "extra_data": null, "instance": { "id": 14394, "url": "https://svs.gsfc.nasa.gov/14394/", "page_type": "Produced Video", "title": "Annular Eclipse Safety GIFs with Nicola Fox", "description": "On Oct. 14, 2023, an annular solar eclipse will cross North, Central, and South America. The Sun is never completely blocked by the Moon during an annular solar eclipse. Therefore, during an annular eclipse, it is never safe to look directly at the Sun without specialized eye protection designed for solar viewing.These GIFs, featuring Nicola Fox, associate administrator for NASA’s Science Mission Directorate, can be used as reminders for safe solar viewing this October.Learn more about how to safely watch the annular solar eclipse: https://solarsystem.nasa.gov/eclipses/2023/oct-14-annular/safety/ || ", "release_date": "2023-08-15T12:00:00-04:00", "update_date": "2023-08-11T16:44:20.013350-04:00", "main_image": { "id": 857660, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014300/a014394/14394_Instructions_4k.00060_print.jpg", "filename": "14394_Instructions_4k.00060_print.jpg", "media_type": "Image", "alt_text": "1. Put on your solar viewing or \"eclipse\" glasses.2. Marvel at the annular eclipse.3. Look down then take off your eclipse glasses.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 423826, "type": "details_page", "extra_data": null, "instance": { "id": 14557, "url": "https://svs.gsfc.nasa.gov/14557/", "page_type": "Produced Video", "title": "How to Photograph a Total Solar Eclipse", "description": "On April 8, 2024, a total solar eclipse will soar over the heads of more than 30 million people across North America. This astronomical event is a unique opportunity for scientists studying in the shadow of the Moon, but it’s also a perfect opportunity to capture unforgettable images. Whether you’re an amateur photographer or a selfie master, try out these tips for photographing the eclipse. To learn more about eclipses visit science.nasa.gov/eclipses || ", "release_date": "2024-03-21T10:00:00-04:00", "update_date": "2024-03-20T14:37:49.291960-04:00", "main_image": { "id": 1090339, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014557/14557_EclipsePhotoTips_Thumbnail.png", "filename": "14557_EclipsePhotoTips_Thumbnail.png", "media_type": "Image", "alt_text": "Music Credit: “Corals Instrumental” by Marc Burh [GEMA], Marek Nichel [GEMA] via Universal Production MusicAdditional photographs and footage: Unsplash, Videvo", "width": 1280, "height": 720, "pixels": 921600 } } }, { "id": 423827, "type": "details_page", "extra_data": null, "instance": { "id": 5219, "url": "https://svs.gsfc.nasa.gov/5219/", "page_type": "Visualization", "title": "2024 Path of Totality", "description": "This visualization closely follows the Moon's umbra shadow as it crosses North America during the April 8, 2024 total solar eclipse. It covers the one hour and 50 minutes between 10:57 a.m. Pacific Standard Time and 4:47 p.m. Atlantic Daylight Time. Annotations include a running clock and the location of the center of the shadow. Everyone within the dark oval sees totality. || flyover.2101_print.jpg (1024x576) [348.8 KB] || flyover.2101_searchweb.png (180x320) [129.1 KB] || flyover.2101_thm.png (80x40) [7.6 KB] || text (1920x1080) [0 Item(s)] || eclipse2024_flyover_720p30.mp4 (1280x720) [59.2 MB] || eclipse2024_flyover_1080p30.mp4 (1920x1080) [108.3 MB] || eclipse2024_flyover_360p30.mp4 (640x360) [24.3 MB] || text (3840x2160) [0 Item(s)] || eclipse2024_flyover_2160p30.mp4 (3840x2160) [360.5 MB] || eclipse2024_flyover_1080p30.mp4.hwshow [193 bytes] || ", "release_date": "2024-02-13T09:00:00-05:00", "update_date": "2025-01-13T00:17:02.265358-05:00", "main_image": { "id": 1089154, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005200/a005219/flyover.2101_print.jpg", "filename": "flyover.2101_print.jpg", "media_type": "Image", "alt_text": "This visualization closely follows the Moon's umbra shadow as it crosses North America during the April 8, 2024 total solar eclipse. It covers the one hour and 50 minutes between 10:57 a.m. Pacific Standard Time and 4:47 p.m. Atlantic Daylight Time. Annotations include a running clock and the location of the center of the shadow. Everyone within the dark oval sees totality.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413114, "type": "details_page", "extra_data": null, "instance": { "id": 5123, "url": "https://svs.gsfc.nasa.gov/5123/", "page_type": "Visualization", "title": "The 2024 Total Solar Eclipse", "description": "This page is also available in the following languages:Tagalog (Wikang Tagalog)Vietnamese (tiếng Việt)Simplified Chinese (汉语)Traditional Chinese (漢語)Arabic (بهاس ملايو)Korean (한국어) || ", "release_date": "2023-07-10T14:00:00-04:00", "update_date": "2025-01-12T22:59:22.920153-05:00", "main_image": { "id": 856401, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005100/a005123/eclipse_map_2024_QR_1920.png", "filename": "eclipse_map_2024_QR_1920.png", "media_type": "Image", "alt_text": "The path of totality and partial contours crossing the U.S. for the 2024 total solar eclipse occurring on April 8, 2024.", "width": 1920, "height": 960, "pixels": 1843200 } } }, { "id": 424113, "type": "details_page", "extra_data": null, "instance": { "id": 5248, "url": "https://svs.gsfc.nasa.gov/5248/", "page_type": "Visualization", "title": "Insolation during the 2024 Eclipse", "description": "Insolation (the amount of sunlight reaching the ground) is affected dramatically by the Moon's shadow during the April 8, 2024 total solar eclipse. || insol.0765_print.jpg (1024x576) [144.8 KB] || insol.0765_searchweb.png (320x180) [73.2 KB] || insol.0765_thm.png (80x40) [6.1 KB] || eclipse2024_insol_720p30.mp4 (1280x720) [10.4 MB] || eclipse2024_insol_1080p30.mp4 (1920x1080) [21.3 MB] || eclipse2024_insol_2160p30.mp4 (3840x2160) [66.1 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || eclipse2024_insol_360p30.mp4 (640x360) [3.2 MB] || ", "release_date": "2024-03-25T13:30:00-04:00", "update_date": "2024-03-26T12:36:59.301576-04:00", "main_image": { "id": 1090581, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005200/a005248/insol.0765_print.jpg", "filename": "insol.0765_print.jpg", "media_type": "Image", "alt_text": "Insolation (the amount of sunlight reaching the ground) is affected dramatically by the Moon's shadow during the April 8, 2024 total solar eclipse.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413112, "type": "details_page", "extra_data": null, "instance": { "id": 5073, "url": "https://svs.gsfc.nasa.gov/5073/", "page_type": "Visualization", "title": "The 2023 and 2024 Solar Eclipses: Map and Data", "description": "The map was updated on March 15, 2023, to correct times in Mexico along the total eclipse path. || ", "release_date": "2023-03-08T14:00:00-05:00", "update_date": "2024-08-30T11:48:34-04:00", "main_image": { "id": 806913, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005000/a005073/eclipse_map_full_print.jpg", "filename": "eclipse_map_full_print.jpg", "media_type": "Image", "alt_text": "A map showing where the Moon’s shadow will cross the U.S. during the 2023 annular solar eclipse and 2024 total solar eclipse. Available at 5400 x 2700, 10,800 x 5400, and 22,500 x 11,250.", "width": 1024, "height": 512, "pixels": 524288 } } }, { "id": 413113, "type": "details_page", "extra_data": null, "instance": { "id": 5124, "url": "https://svs.gsfc.nasa.gov/5124/", "page_type": "Visualization", "title": "The 2023 Annular Solar Eclipse", "description": "The path of annularity and partial contours crossing the U.S. for the 2023 annular solar eclipse occurring on October 14, 2023. || eclipse_map_2023_QR_1920.png (1920x960) [3.4 MB] || eclipse_map_2023_QR_10800.png (10800x5400) [77.3 MB] || eclipse_map_2023_QR_5400.png (5400x2700) [23.1 MB] || eclipse_map_2023_QR_1920_searchweb.png (320x180) [111.9 KB] || eclipse_map_2023_QR_1920_thm.png (80x40) [7.2 KB] || eclipse_map_2023_QR.png (22500x11250) [129.8 MB] || the-2023-annular-solar-eclipse.hwshow [302 bytes] || ", "release_date": "2023-07-10T14:00:00-04:00", "update_date": "2024-10-10T00:15:24.081640-04:00", "main_image": { "id": 856417, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005100/a005124/eclipse_map_2023_QR_1920.png", "filename": "eclipse_map_2023_QR_1920.png", "media_type": "Image", "alt_text": "The path of annularity and partial contours crossing the U.S. for the 2023 annular solar eclipse occurring on October 14, 2023.", "width": 1920, "height": 960, "pixels": 1843200 } } }, { "id": 423828, "type": "details_page", "extra_data": null, "instance": { "id": 5236, "url": "https://svs.gsfc.nasa.gov/5236/", "page_type": "Visualization", "title": "5000 Years of Total Solar Eclipses: The Movie", "description": "An animated heatmap showing the accumulation of total solar eclipse paths over the 5000 years from 2000 BCE to 3000 CE. || heatmap.0090_print.jpg (1024x576) [282.2 KB] || heatmap.0090_searchweb.png (320x180) [93.8 KB] || heatmap.0090_thm.png (80x40) [7.5 KB] || heatmap_720p30.mp4 (1280x720) [20.0 MB] || heatmap_1080p30.mp4 (1920x1080) [38.1 MB] || 3840x2160_16x9_30p (3840x2160) [64.0 KB] || heatmap_360p30.mp4 (640x360) [6.2 MB] || heatmap_2160p30.mp4 (3840x2160) [120.6 MB] || ", "release_date": "2024-03-13T17:30:00-04:00", "update_date": "2024-03-22T13:01:24.262835-04:00", "main_image": { "id": 1090194, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005200/a005236/heatmap.0090_print.jpg", "filename": "heatmap.0090_print.jpg", "media_type": "Image", "alt_text": "An animated heatmap showing the accumulation of total solar eclipse paths over the 5000 years from 2000 BCE to 3000 CE. ", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 423829, "type": "details_page", "extra_data": null, "instance": { "id": 5222, "url": "https://svs.gsfc.nasa.gov/5222/", "page_type": "Visualization", "title": "5000 Years of Total Solar Eclipses", "description": "A heatmap showing the frequency of total solar eclipses over the 5000 years from 2000 BCE to 3000 CE. Includes versions without the color key and without the continent outlines. || eclipse_freq_heatmap_print.jpg (1024x512) [323.0 KB] || eclipse_freq_heatmap_searchweb.png (320x180) [120.8 KB] || eclipse_freq_heatmap_thm.png (80x40) [17.8 KB] || eclipse_freq_heatmap.tif (5400x2700) [14.9 MB] || eclipse_freq_heatmap_nocbar.tif (5400x2700) [14.9 MB] || eclipse_freq_heatmap_noland.tif (5400x2700) [17.0 MB] || ", "release_date": "2024-02-20T12:07:00-05:00", "update_date": "2024-02-19T12:41:27.671167-05:00", "main_image": { "id": 1089333, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005200/a005222/eclipse_freq_heatmap_print.jpg", "filename": "eclipse_freq_heatmap_print.jpg", "media_type": "Image", "alt_text": "A heatmap showing the frequency of total solar eclipses over the 5000 years from 2000 BCE to 3000 CE. Includes versions without the color key and without the continent outlines.", "width": 1024, "height": 512, "pixels": 524288 } } }, { "id": 413115, "type": "details_page", "extra_data": null, "instance": { "id": 5086, "url": "https://svs.gsfc.nasa.gov/5086/", "page_type": "Visualization", "title": "A Tour of NASA’s Solar Eclipse Map for 2023 and 2024", "description": "The map was updated on March 15, 2023, to correct times in Mexico along the total eclipse path.Two solar eclipses will cross the United States in 2023 and 2024. On October 14, 2023, an annular solar eclipse will create a “ring of fire” in the sky from Oregon to Texas. On April 8, 2024, a total solar eclipse will darken the skies from Texas to Maine. On both dates, all 48 contiguous states in the U.S. will experience a partial solar eclipse. || ", "release_date": "2023-03-08T14:00:00-05:00", "update_date": "2025-01-06T00:35:28.062801-05:00", "main_image": { "id": 806950, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005000/a005086/eclipse_map_video_1920.png", "filename": "eclipse_map_video_1920.png", "media_type": "Image", "alt_text": "Watch a close-up tour of the new 2023 and 2024 solar eclipse map. \rMap Credits: Michala Garrison and the Scientific Visualization Studio (SVS), in collaboration with the NASA Heliophysics Activation Team (NASA HEAT), part of NASA’s Science Activation portfolio; eclipse calculations by Ernie Wright, NASA Goddard Space Flight Center\r", "width": 1920, "height": 1080, "pixels": 2073600 } } }, { "id": 413116, "type": "details_page", "extra_data": null, "instance": { "id": 5093, "url": "https://svs.gsfc.nasa.gov/5093/", "page_type": "Visualization", "title": "Solar Eclipse Animation Elements", "description": "Due to their relative scale and distances, the disks of the Sun and the Moon appear to be almost the same size in the sky when standing on Earth. This means that even though the Moon is much smaller than the Sun, it can block most or all of the Sun's light, resulting in a dark shadow over Earth called a solar eclipse.These videos are designed to help describe some of the dynamics that determine how solar eclipses work and why they are important for those of us living on Earth. || ", "release_date": "2023-04-14T09:00:00-04:00", "update_date": "2024-11-22T00:15:55.693541-05:00", "main_image": { "id": 854665, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005000/a005093/eclipseElements60fps_4-11-2023d_apogee_perigee.01080_print.jpg", "filename": "eclipseElements60fps_4-11-2023d_apogee_perigee.01080_print.jpg", "media_type": "Image", "alt_text": "The Moon travels in a not-quite-circular orbit around Earth, meaning that it is at times closer to us than others. We call the Moon's closest point to Earth \"perigee,\" and its farthest point from Earth is \"apogee.\"When the Moon passes between the Sun and Earth while near perigee, it completely blocks out the Sun causing a total eclipse. When the Moon passes between the Sun and Earth, and it is near apogee, it creates an annular eclipse that covers most of the Sun; the edges of the Sun remain visible and create a \"ring of fire.\"", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 426803, "type": "details_page", "extra_data": null, "instance": { "id": 14563, "url": "https://svs.gsfc.nasa.gov/14563/", "page_type": "Produced Video", "title": "Locations of Planets and Comet During Totality on April 8, 2024", "description": "During the total solar eclipse on April 8, 2024, sharp-eyed observers might spot some planets in the darkened sky near the eclipsed Sun.Jupiter and Venus, on opposite sides of the Sun, will be the brightest and easiest to spot. Jupiter will appear about 30 degrees to the upper left of the eclipsed Sun while Venus will appear about 15 degrees to the lower right of the eclipsed Sun.Fainter Mars and Saturn will appear next to one another about 35 degrees to the lower right of the eclipsed Sun, but they might be challenging for most to see. Mercury and Comet 12P/Pons-Brooks will also be in the sky to the upper left of the eclipsed Sun, but they will likely be too faint to see without binoculars or a telescope.For more information about safely watching the eclipse, either directly or with binoculars or a telescope, visit go.nasa.gov/Eclipse2024Safety. || ", "release_date": "2024-04-02T09:00:00-04:00", "update_date": "2024-04-01T17:16:56.276125-04:00", "main_image": { "id": 1090863, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014563/EclipsePlanets_Planets_No_Angles_D.png", "filename": "EclipsePlanets_Planets_No_Angles_D.png", "media_type": "Image", "alt_text": "Jupiter, Venus, Saturn, and Mars could be visible to the unaided eye during totality on April 8, 2024. Mercury (to the upper left of the eclipsed Sun) and Comet 12P/Pons-Brooks (to the right of Jupiter), not labeled here, will likely be too faint to see without binoculars or a telescope.Credit: NASA/JPL-Caltech", "width": 1690, "height": 951, "pixels": 1607190 } } } ], "extra_data": {} }, { "id": 372265, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372265", "widget": "Card gallery", "title": "The Solar Dynamics Observatory", "caption": "", "description": "SDO observations", "items": [ { "id": 413117, "type": "details_page", "extra_data": null, "instance": { "id": 4117, "url": "https://svs.gsfc.nasa.gov/4117/", "page_type": "Visualization", "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. || ", "release_date": "2013-12-17T10:00:00-05:00", "update_date": "2021-02-22T07:37:05-05:00", "main_image": { "id": 461378, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004117/SDOargoFD_rotorzoom_stand.HD1080i.01800.jpg", "filename": "SDOargoFD_rotorzoom_stand.HD1080i.01800.jpg", "media_type": "Image", "alt_text": "The movie opens with a full-disk view of the Sun in visible wavelengths. Then the filters are applied to small pie-shaped wedges of the Sun, starting with 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 let the set of filters sweep around the solar disk and then zoom and rotate the camera to rotate with the filters as the solar image is rotate underneath. This video is also available on our YouTube channel.", "width": 1920, "height": 1080, "pixels": 2073600 } } }, { "id": 413118, "type": "details_page", "extra_data": null, "instance": { "id": 4008, "url": "https://svs.gsfc.nasa.gov/4008/", "page_type": "Visualization", "title": "SDO Jewelbox: The Many Eyes of SDO", "description": "5x3 Layout view. This version has the imagery organized in order of increasing wavelength, from upper left to lower right for AIA. The HMI products occupy the bottom row. || SDOJewelbox_5x3.0100.jpg (2400x810) [317.7 KB] || SDOJewelbox_5x3.0100_web.png (320x108) [28.9 KB] || SDOJewelbox_5x3.0100_thm.png (80x40) [3.7 KB] || SDOJewelbox_5x3.0100_searchweb.png (320x180) [29.2 KB] || SDOJewelbox_5x3.webmhd.webm (960x540) [3.3 MB] || SDOJewelbox_5x3.mov (2400x810) [91.5 MB] || SDOJewelbox_5x3.mp4 (2400x810) [91.5 MB] || 2400x810_80x27_30p (2400x810) [0 Item(s)] || ", "release_date": "2012-11-20T09:00:00-05:00", "update_date": "2019-10-03T16:36:27-04:00", "main_image": { "id": 472810, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004008/SDOJewelbox_3x3.0100.jpg", "filename": "SDOJewelbox_3x3.0100.jpg", "media_type": "Image", "alt_text": "3x3 Layout view. This version is a subset of SDO filters. HMI imagery occupies the top row. EVE data is in the center. Selected AIA wavelengths other spots.", "width": 1920, "height": 1080, "pixels": 2073600 } } }, { "id": 413119, "type": "details_page", "extra_data": null, "instance": { "id": 3838, "url": "https://svs.gsfc.nasa.gov/3838/", "page_type": "Visualization", "title": "Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms)", "description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk.Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3839 (171 Ångstroms), 3840 (211 Ångstroms) and 3841 (1700 Ångstroms). || ", "release_date": "2011-07-01T10:00:00-04:00", "update_date": "2025-03-09T00:00:56.850075-05:00", "main_image": { "id": 484932, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003838/SDO304FullDisk_1080HD_web.png", "filename": "SDO304FullDisk_1080HD_web.png", "media_type": "Image", "alt_text": "These movies present the six hour interval around the event, a one minute per animation frame.", "width": 320, "height": 180, "pixels": 57600 } } }, { "id": 413120, "type": "details_page", "extra_data": null, "instance": { "id": 31213, "url": "https://svs.gsfc.nasa.gov/31213/", "page_type": "Hyperwall Visual", "title": "A Smiling Sun", "description": "Solar Dynamics Observatory image of the Sun from October, 2022 || 2022-agu-fox-slide5_print.jpg (1024x576) [144.3 KB] || 2022-agu-fox-slide5.png (3840x2160) [10.5 MB] || 2022-agu-fox-slide5_searchweb.png (320x180) [93.5 KB] || 2022-agu-fox-slide5_thm.png (80x40) [7.5 KB] || a-smiling-sun.hwshow [275 bytes] || ", "release_date": "2023-01-06T00:00:00-05:00", "update_date": "2024-10-11T00:31:07.664194-04:00", "main_image": { "id": 551798, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a031200/a031213/2022-agu-fox-slide5_print.jpg", "filename": "2022-agu-fox-slide5_print.jpg", "media_type": "Image", "alt_text": "Solar Dynamics Observatory image of the Sun from October, 2022", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413121, "type": "details_page", "extra_data": null, "instance": { "id": 5084, "url": "https://svs.gsfc.nasa.gov/5084/", "page_type": "Visualization", "title": "Several impressive filament eruptions leading up to an M 8.7 Flare at Active Region 13234 - February 27-28, 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.Some impressive filaments erupt on the solar limb (lower left and lower right) in the early part of this image series. Later (17:46:42 TAI), an active region in the upper right quadrant of the solar disk launches a mid-level M 8.7 class flare.Event Description || ", "release_date": "2023-06-06T00:00:00-04:00", "update_date": "2023-05-31T09:52:33.068028-04:00", "main_image": { "id": 855590, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005000/a005084/20230227_AR13234M86_AIA304_PSF_stamped.001120_print.jpg", "filename": "20230227_AR13234M86_AIA304_PSF_stamped.001120_print.jpg", "media_type": "Image", "alt_text": "Large filaments appear off the limb of the Sun (lower left and lower right) in this view from SDO/AIA 304 Angstrom filter. Note the lower right filament visible in this 304 Angstrom image is NOT visible in the 171 Angstrom filter.", "width": 1024, "height": 1024, "pixels": 1048576 } } }, { "id": 413122, "type": "details_page", "extra_data": null, "instance": { "id": 5103, "url": "https://svs.gsfc.nasa.gov/5103/", "page_type": "Visualization", "title": "Dancing on the Limb - May 1, 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.A large loop of solar plasma executes some interesting long-lived (15 hours in this series) gyrations on the lower solar limb. || ", "release_date": "2023-05-24T00:00:00-04:00", "update_date": "2023-05-19T09:20:23.150857-04:00", "main_image": { "id": 855383, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005100/a005103/20230501_LimbEvent_AIA171_PSF_stamped.002000_print.jpg", "filename": "20230501_LimbEvent_AIA171_PSF_stamped.002000_print.jpg", "media_type": "Image", "alt_text": "A view of a very active coronal plasma loop (lower solar limb) in this long view using the SDO AIA 171A filter.", "width": 1024, "height": 1024, "pixels": 1048576 } } }, { "id": 413123, "type": "details_page", "extra_data": null, "instance": { "id": 14263, "url": "https://svs.gsfc.nasa.gov/14263/", "page_type": "Produced Video", "title": "133 Days on the Sun", "description": "This 133-day time lapse of the Sun at 17.1nm shows brilliant active regions, dynamic loops of plasma and numerous solar eruptions.Music (in order): Concave Hexagon, Heptagon, Tetrahedron, Triangular Prism, Square-based Pyramid, Irregular Quadrilateral, Equilateral Triangle, Dodecahedron, Icosahedron, all from \"Geometric Shapes\" written and produced by Lars Leonhard.Credit: NASA's Goddard Space Flight Center/SDOWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Video Descriptive Text available. || 133DaysontheSun_StillSept15_print.jpg (1024x576) [134.4 KB] || 133DaysontheSun_StillSept15.png (3840x2160) [25.3 MB] || 133DaysontheSun_StillSept15.jpg (3840x2160) [1.1 MB] || 133DaysontheSun_StillSept15_searchweb.png (320x180) [74.6 KB] || 133DaysontheSun_StillSept15_thm.png (80x40) [6.8 KB] || 14263_133_Days_on_the_Sun_1080.mp4 (1920x1080) [4.3 GB] || 14263_133_Days_on_the_Sun_1080.webm (1920x1080) [470.3 MB] || 14263_133_Days_on_the_Sun_ProRes_3840x2160_2997.mov (3840x2160) [156.8 GB] || 14263_133_Days_on_the_Sun_4k_100mbps.mp4 (3840x2160) [41.5 GB] || 14263_133_Days_on_the_Sun_4k.mp4 (3840x2160) [10.5 GB] || 133_Days-on_the_Sun_SRT_Captions.en_US.srt [2.5 KB] || 133_Days-on_the_Sun_SRT_Captions.en_US.vtt [2.6 KB] || ", "release_date": "2023-01-05T11:00:00-05:00", "update_date": "2023-05-03T11:43:47.542342-04:00", "main_image": { "id": 551741, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014200/a014263/133DaysontheSun_StillSept15_print.jpg", "filename": "133DaysontheSun_StillSept15_print.jpg", "media_type": "Image", "alt_text": "This 133-day time lapse of the Sun at 17.1nm shows brilliant active regions, dynamic loops of plasma and numerous solar eruptions.Music (in order): Concave Hexagon, Heptagon, Tetrahedron, Triangular Prism, Square-based Pyramid, Irregular Quadrilateral, Equilateral Triangle, Dodecahedron, Icosahedron, all from \"Geometric Shapes\" written and produced by Lars Leonhard.Credit: NASA's Goddard Space Flight Center/SDOWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Video Descriptive Text available.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413124, "type": "details_page", "extra_data": null, "instance": { "id": 14126, "url": "https://svs.gsfc.nasa.gov/14126/", "page_type": "Produced Video", "title": "SDO Video Toolkit", "description": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files || New_Trebuchet_mkII.00300_print.jpg (1024x576) [336.5 KB] || New_Trebuchet_mkII.00300_print_searchweb.png (320x180) [95.4 KB] || New_Trebuchet_mkII.00300_print_thm.png (80x40) [6.2 KB] || New_Trebuchet_mkII.mp4 (1920x1080) [32.4 MB] || New_Trebuchet_mkII.webm (1920x1080) [3.7 MB] || New_Trebuchet_mkII.mov (1920x1080) [443.3 MB] || New_Trebuchet_mkII.mp4.hwshow [115 bytes] || ", "release_date": "2022-04-01T00:00:00-04:00", "update_date": "2024-10-21T14:41:30-04:00", "main_image": { "id": 372191, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/New_Trebuchet_mkII.00300_print.jpg", "filename": "New_Trebuchet_mkII.00300_print.jpg", "media_type": "Image", "alt_text": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files", "width": 1024, "height": 576, "pixels": 589824 } } } ], "extra_data": {} }, { "id": 372274, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372274", "widget": "Card gallery", "title": "Other Heliophysics Missions", "caption": "", "description": "Parker Solar Probe, SOHO, MMS, and others in the Heliophysics fleet", "items": [ { "id": 413125, "type": "details_page", "extra_data": null, "instance": { "id": 14055, "url": "https://svs.gsfc.nasa.gov/14055/", "page_type": "Produced Video", "title": "Parker Solar Probe's WISPR Images Inside The Sun's Atmosphere", "description": "For the first time in history, a spacecraft has touched the Sun. NASA’s Parker Solar Probe has now flown through the Sun’s upper atmosphere – the corona – and sampled particles and magnetic fields there. As Parker Solar Probe flew through the corona, its WISPR instrument captured images.The Wide-Field Imager for Parker Solar Probe (WISPR) is the only imaging instrument aboard the spacecraft. WISPR looks at the large-scale structure of the corona and solar wind before the spacecraft flies through it. About the size of a shoebox, WISPR takes images from afar of structures like coronal mass ejections, or CMEs, jets and other ejecta from the Sun. These structures travel out from the Sun and eventually overtake the spacecraft, where the spacecraft’s other instruments take in-situ measurements. WISPR helps link what’s happening in the large-scale coronal structure to the detailed physical measurements being captured directly in the near-Sun environment.To image the solar atmosphere, WISPR uses the heat shield to block most of the Sun’s light, which would otherwise obscure the much fainter corona. Specially designed baffles and occulters reflect and absorb the residual stray light that has been reflected or diffracted off the edge of the heat shield or other parts of the spacecraft.WISPR uses two cameras with radiation-hardened Active Pixel Sensor CMOS detectors. These detectors are used in place of traditional CCDs because they are lighter and use less power. They are also less susceptible to effects of radiation damage from cosmic rays and other high-energy particles, which are a big concern close to the Sun. The camera’s lenses are made of a radiation hard BK7, a common type of glass used for space telescopes, which is also sufficiently hardened against the impacts of dust.WISPR was designed and developed by the Solar and Heliophysics Physics Branch at the Naval Research Laboratory in Washington, D.C. (principal investigator Russell Howard), which will also develop the observing program. || ", "release_date": "2021-12-20T22:00:00-05:00", "update_date": "2023-05-03T13:43:36.490627-04:00", "main_image": { "id": 374325, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014000/a014055/wispr_lw_composite_enc08_20210428.00001_print.jpg", "filename": "wispr_lw_composite_enc08_20210428.00001_print.jpg", "media_type": "Image", "alt_text": "During Parker Solar Probe’s eighth orbit around the Sun, the spacecraft flew through structures in the corona called streamers. This movie shows that data from the WISPR instrument on Parker Solar Probe.Credit: NASA/Johns Hopkins APL/Naval Research Laboratory", "width": 1024, "height": 803, "pixels": 822272 } } }, { "id": 413126, "type": "details_page", "extra_data": null, "instance": { "id": 4970, "url": "https://svs.gsfc.nasa.gov/4970/", "page_type": "Visualization", "title": "The Many Eyes on the Parker Solar Probe Perihelion (February 2022)", "description": "This visualization opens with a top-down view, then transtions to an oblique view of the inner solar system with the various solar-observing missions conducting coordinated observations of the plasma environment. This version displays the imaging instrument camera frustums and solar magnetic field alignments - the 'glyph' version. A version with just the orbits, no 'glyphs' is available in the [Download Options] menu. || SolarSynergiesPlus.Encounter2022FebTop2Side.HAE.AU.glyphs_CRTT.HD1080.01300_print.jpg (1024x576) [123.3 KB] || SolarSynergiesPlus.Encounter2022FebTop2Side.HAE.AU.glyphs_CRTT.HD1080.01300_searchweb.png (320x180) [78.9 KB] || SolarSynergiesPlus.Encounter2022FebTop2Side.HAE.AU.glyphs_CRTT.HD1080.01300_thm.png (80x40) [5.2 KB] || Encounter2022FebTop2Side (1920x1080) [0 Item(s)] || Encounter2022FebTop2Side.glyphs (1920x1080) [0 Item(s)] || SolarSynergiesPlus.Encounter2022FebTop2Side.HD1080_p30.mp4 (1920x1080) [47.0 MB] || SolarSynergiesPlus.Encounter2022FebTop2Side.glyphs.HD1080_p30.mp4 (1920x1080) [60.7 MB] || SolarSynergiesPlus.Encounter2022FebTop2Side.HD1080_p30.webm (1920x1080) [9.7 MB] || Encounter2022FebTop2Side (3840x2160) [0 Item(s)] || Encounter2022FebTop2Side.glyphs (3840x2160) [0 Item(s)] || SolarSynergiesPlus.Encounter2022FebTop2Side.UHD2160_p30.mp4 (3840x2160) [143.6 MB] || SolarSynergiesPlus.Encounter2022FebTop2Side.glyphs.UHD2160_p30.mp4 (3840x2160) [176.4 MB] || SolarSynergiesPlus.Encounter2022FebTop2Side.HD1080_p30.mp4.hwshow [220 bytes] || ", "release_date": "2022-02-25T10:00:00-05:00", "update_date": "2025-01-06T00:19:45.634227-05:00", "main_image": { "id": 372784, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004900/a004970/SolarSynergiesPlus.Encounter2022FebTop2Side.HAE.AU.glyphs_CRTT.HD1080.01300_print.jpg", "filename": "SolarSynergiesPlus.Encounter2022FebTop2Side.HAE.AU.glyphs_CRTT.HD1080.01300_print.jpg", "media_type": "Image", "alt_text": "This visualization opens with a top-down view, then transtions to an oblique view of the inner solar system with the various solar-observing missions conducting coordinated observations of the plasma environment. This version displays the imaging instrument camera frustums and solar magnetic field alignments - the 'glyph' version. A version with just the orbits, no 'glyphs' is available in the [Download Options] menu.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413127, "type": "details_page", "extra_data": null, "instance": { "id": 4957, "url": "https://svs.gsfc.nasa.gov/4957/", "page_type": "Visualization", "title": "Parker Solar Probe: The Origins of Switchbacks", "description": "Most of the magnetic field measured at Parker during this time is directed sunward (blue field lines and vectors). A switchback occurs when the field changes direction almost 180 degrees for a short period of time. FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are represented as gold. || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_print.jpg (1024x576) [114.9 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_searchweb.png (320x180) [71.7 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_thm.png (80x40) [4.5 KB] || Switchbacks20181106A (1920x1080) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4 (1920x1080) [25.7 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.webm (1920x1080) [4.4 MB] || Switchbacks20181106A (3840x2160) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.UHD3840_2160p30.mp4 (3840x2160) [100.2 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4.hwshow [229 bytes] || ", "release_date": "2021-12-14T12:00:00-05:00", "update_date": "2025-01-06T00:19:27.633122-05:00", "main_image": { "id": 374848, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004900/a004957/BaleSwitchbacks.enc06.top.Overview.FIELDS.field.clockSlate_EarthTarget.HD1080.00690_print.jpg", "filename": "BaleSwitchbacks.enc06.top.Overview.FIELDS.field.clockSlate_EarthTarget.HD1080.00690_print.jpg", "media_type": "Image", "alt_text": "A top-down view from the ecliptic pole of the orbit of Parker Solar Probe for Encounter 6. FIELDS instrument magnetic vector data are projected from the spacecraft position with arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are the gold lines, representing the propagation of the average field measured at Parker, propagated back to the solar photosphere.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413128, "type": "details_page", "extra_data": null, "instance": { "id": 3504, "url": "https://svs.gsfc.nasa.gov/3504/", "page_type": "Visualization", "title": "Halloween 2003 Solar Storms: SOHO/EIT and SOHO/LASCO", "description": "Here is a view of the solar disk in 195 Å ultraviolet light (colored green in this movie) and the Sun's extended atmosphere, or corona, (blue and white in this movie). The corona is visible to the SOHO/LASCO coronagraph instruments, which block the bright disk of the Sun so the significantly fainter corona can be seen. In this movie, the inner coronagraph (designated C2) is combined with the outer coronagraph (C3). This movie covers a two week period in October and November 2003 which exhibited some of the largest solar activity events since the advent of space-based solar observing.As the movie plays, we can observe a number of features of the active Sun. Long streamers radiate outward from the Sun and wave gently due to their interaction with the solar wind. The bright white regions are visible due to their high density of free electrons which scatter the light from the photosphere towards the observer. Protons and other ionized atoms are there as well, but are not as visible since they do not interact with photons as strongly as electrons. Coronal Mass Ejections (CMEs) are occasionally observed launching from the Sun. Some of these launch particle events which can saturate the cameras with snow-like artifacts.Also visible in the coronagraphs are stars and planets. Stars are seen to drift slowly to the right, carried by the relative motion of the Sun and the Earth. The planet Mercury is visible as the bright point moving left of the Sun. The horizontal 'extension' in the image is called 'blooming' and is due to a charge leakage along the readout wires in the CCD imager in the camera.This movie is part of a series of movies with matching cadence designed to play synchronously with each other. The other movies in this series are Halloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 195 angstromHalloween 2003 Solar Storms: SOHO/EIT Ultraviolet, 304 angstromHalloween 2003 Solar Storms: SOHO/MDI Continuum Halloween 2003 Solar Storms: SOHO/MDI Magnetograms For more information, visit the SOHO project page.. || ", "release_date": "2008-04-02T00:00:00-04:00", "update_date": "2024-12-29T22:01:09.387297-05:00", "main_image": { "id": 506033, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003500/a003504/coronagraphs_stand.HD1080i.01000.jpg", "filename": "coronagraphs_stand.HD1080i.01000.jpg", "media_type": "Image", "alt_text": "This movie plays nearly two weeks of SOHO/EIT and SOHO/LASCO imagery from around Halloween 2003.", "width": 1920, "height": 1080, "pixels": 2073600 } } }, { "id": 413129, "type": "details_page", "extra_data": null, "instance": { "id": 5136, "url": "https://svs.gsfc.nasa.gov/5136/", "page_type": "Visualization", "title": "STEREO-A Returns by Earth", "description": "The Solar Terrestrial Relations Observatory (STEREO) mission was launched on October 25, 2006, with the purpose of tracing the flow of energy and matter from the Sun to Earth. The STEREO mission began with two spacecraft: STEREO-A and STEREO-B. Each was launched into Sun-orbiting trajectories - STEREO-A moving ahead of Earth, and STEREO-B moving behind Earth (STEREO's Routes to Solar Orbits). In mid-August 2023, the still-operational STEREO-A (STEREO-B went offline in October 2014) will pass Earth for the first time since its launch 17 years ago. Like race cars driving different speeds around a circular track, STEREO-A is traveling slightly faster than Earth around the Sun. After launch, STEREO-A pulled ahead of Earth and extended its lead a little bit more with each orbit. Now, STEREO-A’s lead is so great that it is catching up to Earth from behind and is about to “lap” Earth, having completed 18 circuits around the Sun while Earth completed just 17. || ", "release_date": "2023-08-22T00:00:00-04:00", "update_date": "2025-01-06T00:44:34.491471-05:00", "main_image": { "id": 857695, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005100/a005136/STEREOflyby.STEREOflybyZoom.GSE.AU.clockSlate_EarthTarget.HD1080.00500_print.jpg", "filename": "STEREOflyby.STEREOflybyZoom.GSE.AU.clockSlate_EarthTarget.HD1080.00500_print.jpg", "media_type": "Image", "alt_text": "A view of the orbit of STEREO-A relative to Earth from mid-June 2023 to mid-October 2023, as it passes Earth. The camera is anchored on the Earth-Sun line so Earth and the Sun appear fixed while the distant stars appear to move around the camera. This movie starts with a wide view of the inner solar system with STEREO-A and Earth marked. The camera then zooms in to a closer view of Earth showing Solar Dynamics Observatory (SDO) orbiting Earth, the heliophysics missions orbiting the L1 Lagrange Point (the green cross), and the orbit of the Moon.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413130, "type": "details_page", "extra_data": null, "instance": { "id": 4788, "url": "https://svs.gsfc.nasa.gov/4788/", "page_type": "Visualization", "title": "The Solar Polar Magnetic Field", "description": "From our single vantage point of Earth, our view of the Sun is never complete. While the far-side of the Sun eventually rotates into view, coverage of the Sun's polar regions is never satisfactory as perspective effects either completely block our view or create a distorted view. We must often resort to computer modeling of these solar polar regions.This visualization presents the Potential Field Source Surface (PFSS) magnetic field model based on solar observations covering the years 2017-2019. One version also presents the 'hole' in our measurements of the solar polar region. The region oscillates in size over the course of the year due to the changing perspective created by the tilt of Earth's orbital plane with the solar equator. In this region, researchers must resort to approximations to build a more complete view of the solar magnetic field.Why is the solar magnetic field in this region important? Because the combined with the outgoing flow of the solar wind, the magnetic field lines from the polar regions curve up, and then back down to near the Sun's equatorial plane, which is still fairly close to the orbital plane of Earth and other planets in our solar system. This gives the Sun's polar magnetic field a significant influence on the space weather impacting Earth and crewed and uncrewed assets around the solar system. || ", "release_date": "2020-02-04T12:00:00-05:00", "update_date": "2023-05-03T13:45:13.561169-04:00", "main_image": { "id": 387970, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004788/PFSSPolarTour_inertial.HD1080i.0240_print.jpg", "filename": "PFSSPolarTour_inertial.HD1080i.0240_print.jpg", "media_type": "Image", "alt_text": "This movie gives a view starting at equator and tipping to a view of the north heliographic pole (the blue axis) then dipping down to the south heliographic pole. Closed field lines are white/grey, green and violet lines represent field lines that are considered 'open'. Green represents positive magnetic polarity, and violet represents negative polarity. The dark rings around the blue polar axis show the region where the solar surface magnetic field must be generated from a model. This region grows and shrinks depending on SDOs position in its orbit around the Sun and Earth (above and below the solar equator, which is tilted by 7.25 degrees relative to Earth's orbital plane).", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413131, "type": "details_page", "extra_data": null, "instance": { "id": 4639, "url": "https://svs.gsfc.nasa.gov/4639/", "page_type": "Visualization", "title": "MMS Sees a New Type of Reconnection", "description": "The Magnetospheric Multiscale (MMS) mission consists of four identical satellites that traverse various regions of Earth's magnetosphere measuring the particles and electric and magnetic field which influence them.In the turbulent plasma between Earth's magnetopause and bow shock, a region called the magnetosheath, the MMS satellite constellation has measured multiple jets of energetic electrons between magnetic bubbles. This appears to be a new 'flavor' of magnetic reconnection based on electrons and occuring on smaller time and spatial scales than the standard model of magnetic reconnection with ions.In these data visualizations, the arrows represent the data collected by the spacecraft. To better comprehend changes as the spacecraft moves along, the data are allowed to 'echo' along the spacecraft trail. The length of the vectors represent the relative magnitude of the vector. However, the electron and proton vectors are scaled so equal velocities correspond to vectors of equal magnitude.Magenta represents the direction and magnitude of the magnetic field at the spacecraft position.Green represents the direction and magnitude of the net electric current created by the motion of the electrons and ions measured at the spacecraft position.The four MMS spacecraft are represented by colored spheres, corresponding to the plotted data lines in the lower graphicMMS1MMS2MMS3MMS4The clocks on MMS are synchronized for the TAI (International Atomic Time) system provided through the Global Positioning System (GPS) satellites. It provides a high-precision time reference for comparing MMS measurements to other datasets. || ", "release_date": "2018-05-09T13:00:00-04:00", "update_date": "2025-01-06T00:12:51.453633-05:00", "main_image": { "id": 404491, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004639/PhanNewReconnect_Fly2Pursuit2Drift_Dec09DataShort_RE_MMS.slate_CRTT.HD1080i.3000_print.jpg", "filename": "PhanNewReconnect_Fly2Pursuit2Drift_Dec09DataShort_RE_MMS.slate_CRTT.HD1080i.3000_print.jpg", "media_type": "Image", "alt_text": "From a wide view of the MMS orbit, this visualization zooms down to the four spacecraft as they move between the magnetopause and bow shock. Along the track of each spacecraft we see the measured magnetic field vectors (magenta arrows) and the measured current vectors (green arrows). The energetic event of interest occurs at clock time of 09:03:54.3 TAI.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413132, "type": "details_page", "extra_data": null, "instance": { "id": 3590, "url": "https://svs.gsfc.nasa.gov/3590/", "page_type": "Visualization", "title": "THEMIS/ASI Nights - High Resolution", "description": "A collection of ground-based All-Sky Imagers (ASI) makes an important component of the THEMIS mission in understanding the interaction of the magnetosphere and aurora. It is sometimes referred to as the sixth THEMIS satellite. Descriptions of the instruments are available on the THEMIS-Canada Home Page. Imagery from each camera is co-registered to the surface of the Earth and assembled into a view of the auroral events. This movie presents data from the first large auroral substorm since the THEMIS launch. The substorm reached its maximum between 6:00 and 7:00 UT. Note that the ASI data in this movie are assembled from significantly higher resolution datesets than the earlier version, THEMIS/ASI Nights. The higher resolution enables you to see much finer details in the aurora structure. In addition, one notices trees circling the horizon visible to the cameras located in western Canada. || ", "release_date": "2009-07-07T00:00:00-04:00", "update_date": "2025-01-05T22:01:59.525805-05:00", "main_image": { "id": 502226, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003500/a003590/ASInew.1000.jpg", "filename": "ASInew.1000.jpg", "media_type": "Image", "alt_text": "This movie zooms in on the Earth, revealing the placement of the ASI ground stations and their sky coverage. We observe the stations coming online as the night progresses.", "width": 1280, "height": 720, "pixels": 921600 } } } ], "extra_data": {} }, { "id": 372275, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372275", "widget": "Card gallery", "title": "Space Weather", "caption": "", "description": "Solar flares, coronal mass ejections, as well as their effects and interactions (needs a better description)", "items": [ { "id": 413133, "type": "details_page", "extra_data": null, "instance": { "id": 31248, "url": "https://svs.gsfc.nasa.gov/31248/", "page_type": "Hyperwall Visual", "title": "How Do Space Weather Effects & Solar Storms Affect Earth?", "description": "Technological and infrastructure affected by space weather events. || space-weather-effects_print.jpg (1024x953) [307.6 KB] || space-weather-effects.png (3480x3240) [8.3 MB] || space-weather-effects_searchweb.png (320x180) [77.3 KB] || space-weather-effects_thm.png (80x40) [6.2 KB] || how-do-space-weather-effects-solar-storms-affect-earth.hwshow [320 bytes] || ", "release_date": "2023-09-29T00:00:00-04:00", "update_date": "2024-10-11T00:31:41.612521-04:00", "main_image": { "id": 859455, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a031200/a031248/space-weather-effects_print.jpg", "filename": "space-weather-effects_print.jpg", "media_type": "Image", "alt_text": "Technological and infrastructure affected by space weather events.", "width": 1024, "height": 953, "pixels": 975872 } } }, { "id": 413134, "type": "details_page", "extra_data": null, "instance": { "id": 30179, "url": "https://svs.gsfc.nasa.gov/30179/", "page_type": "Hyperwall Visual", "title": "ISS Timelapse: Aurora Australis", "description": "The photographs used to make this video were taken on September 17, 2011 from 17:22:27 to 17:37:21 GMT from the International Space Station (ISS). This image sequence begins over the Indian Ocean halfway between Madagascar and Antarctica. Aurora Australis is present for the first 2/3rds of the video, then Australis comes into view. Yellow lights near the coast show the presence of cities, while interior oragne lights indicate brush fires.http://eol.jsc.nasa.gov || ", "release_date": "2013-10-17T12:00:00-04:00", "update_date": "2025-03-02T00:20:39.886218-05:00", "main_image": { "id": 429031, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a030100/a030179/iss029_aurora_20110917_print.jpg", "filename": "iss029_aurora_20110917_print.jpg", "media_type": "Image", "alt_text": "Time lapse photos of Aurora Australis", "width": 1024, "height": 574, "pixels": 587776 } } }, { "id": 413135, "type": "details_page", "extra_data": null, "instance": { "id": 20363, "url": "https://svs.gsfc.nasa.gov/20363/", "page_type": "Animation", "title": "Animation: Heliosphere", "description": "The sun sends out a constant flow of charged particles called the solar wind, which ultimately travels past all the planets to some three times the distance to Pluto before being impeded by the interstellar medium. This forms a giant bubble around the sun and its planets, known as the heliosphere. NASA studies the heliosphere to better understand the fundamental physics of the space surrounding us - which, in turn, provides information regarding space throughout the rest of the universe, as well as regarding what makes planets habitable.The solar wind is a gas of charged particles known as plasma, a state of matter governed by its own set physical laws just as the more common solids, liquids, and gases are. As the solar wind sweeps out into space, it creates a space environment filled with radiation as well as magnetic fields that trail all the way back to the sun. This space environment is augmented by interstellar cosmic rays and occasional concentrated clouds of solar material that burst off the sun, known as coronal mass ejections.This complex environment surrounds the planets and ultimately has a crucial effect on the formation, evolution, and destiny of planetary systems. For one thing, our heliosphere acts as a giant shield, protecting the planets from galactic cosmic radiation. Earth is additionally shielded by its own magnetic field, the magnetosphere, which protects us not only from solar and cosmic particle radiation but also from erosion of the atmosphere by the solar wind. Planets without a shielding magnetic field, such as Mars and Venus, are exposed to such processes and have evolved differently.NASA's studies of the heliosphere include research into: how the solar wind behaves near Earth; what causes and sustains magnetic and electric fields around other planets; how does the heliosphere interact with the interstellar medium; what do the boundaries of the heliosphere look like; what is the origin and evolution of the solar wind and the interstellar cosmic rays; and what contributes to the habitability of exoplanets.The field is, therefore, intensely cross-disciplinary. Heliospheric research often works hand in hand with planetary scientists, astrophysicists, astrobiologists, and space weather researchers.NASA heliophysics missions contributing to heliospheric research are: the Advanced Composition Explorer; NOAA's Deep Space Climate Observatory, the Interstellar Boundary Explorer, the Solar Terrestrial Relations Observatory; Voyager, and Wind. || ", "release_date": "2022-03-09T18:00:00-05:00", "update_date": "2025-06-23T00:18:39.136923-04:00", "main_image": { "id": 372595, "url": "https://svs.gsfc.nasa.gov/vis/a020000/a020300/a020363/H_0322_HeliopauseCycle_v01.00680_print.jpg", "filename": "H_0322_HeliopauseCycle_v01.00680_print.jpg", "media_type": "Image", "alt_text": "A conceptual animation showing the heliosphere — the vast bubble that is generated by the Sun’s magnetic field and envelops all the planets. ", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413136, "type": "details_page", "extra_data": null, "instance": { "id": 12249, "url": "https://svs.gsfc.nasa.gov/12249/", "page_type": "Produced Video", "title": "Earth's Magnetism In Action", "description": "Scientists make a breakthrough in observing the dynamic magnetic system surrounding our planet. || c-1024.jpg (1024x576) [385.4 KB] || c-1280.jpg (1280x720) [576.4 KB] || c-1024_print.jpg (1024x576) [403.6 KB] || c-1024_searchweb.png (320x180) [137.4 KB] || c-1024_web.png (320x180) [137.4 KB] || c-1024_thm.png (80x40) [24.5 KB] || ", "release_date": "2016-05-24T11:00:00-04:00", "update_date": "2023-05-03T13:48:35.815142-04:00", "main_image": { "id": 424052, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012200/a012249/c-1024_print.jpg", "filename": "c-1024_print.jpg", "media_type": "Image", "alt_text": "Scientists make a breakthrough in observing the dynamic magnetic system surrounding our planet.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 464089, "type": "details_page", "extra_data": null, "instance": { "id": 5435, "url": "https://svs.gsfc.nasa.gov/5435/", "page_type": "Visualization", "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm", "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ", "release_date": "2024-12-12T12:00:00-05:00", "update_date": "2025-06-11T19:45:38.611593-04:00", "main_image": { "id": 1139754, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a005400/a005435/multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg", "filename": "multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg", "media_type": "Image", "alt_text": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms", "width": 1024, "height": 576, "pixels": 589824 } } } ], "extra_data": {} }, { "id": 372276, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372276", "widget": "Card gallery", "title": "Carrington-Class Event", "caption": "", "description": "Visualizations relating to a very large and very fast coronal mass ejection in July 2012", "items": [ { "id": 413137, "type": "details_page", "extra_data": null, "instance": { "id": 4189, "url": "https://svs.gsfc.nasa.gov/4189/", "page_type": "Visualization", "title": "Comparative Magnetospheres: A Carrington-Class CME", "description": "In an effort to understand and predict the impact of space weather events on Earth, the Community-Coordinated Modeling Center (CCMC) at NASA Goddard Space Flight Center, routinely runs computer models of the many historical events. These model runs are then compared to actual data to determine ways to improve the model, and therefore forecasts of the impacts of future space weather events.But sometimes we don't have an actual event where we have lots of data for comparison. Extreme space weather events are one example where we must test models with a rather limited set of data.This is a model run used to examine the consequences if a large coronal mass ejection (CME) such as The Carrington-Class CME of 2012 had actual hit Earth. Such model runs allow us to estimate consequences of a large event hitting Earth so we can better protect power grids and satellites.Some of the conclusions from this model run are (documented in the paper linked below):The magnetopause is compressed to the point it is moved inside the orbits of our geosynchronous satellites.Large field-aligned currents are created on the night-side of Earth, generating large ionospheric potentials.At high latitudes, geo-electric fields of 26 volts per kilometer can be generated.For comparison, the geo-electric field of the March 1989 storm which generated an extensive power outage in Canada (Wikipedia) had a value of only about 6 volts per kilometer; and the 2003 Halloween solar storms (see Halloween Solar Storms 2003) generated a field of about 12 volts per kilometer. || ", "release_date": "2014-09-25T10:00:00-04:00", "update_date": "2024-12-29T22:16:09.811536-05:00", "main_image": { "id": 452497, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004189/Earth_CarringtonClass_Pullout.noslate_GSEmove.HD1080i.0001_print.jpg", "filename": "Earth_CarringtonClass_Pullout.noslate_GSEmove.HD1080i.0001_print.jpg", "media_type": "Image", "alt_text": "This movie opens with a close-up view of Earth with geo-magnetic field lines. The camera pulls out and fades in a profile slice of the plasma density data.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413138, "type": "details_page", "extra_data": null, "instance": { "id": 4188, "url": "https://svs.gsfc.nasa.gov/4188/", "page_type": "Visualization", "title": "Comparative Magnetospheres: A Noteworthy Coronal Mass Ejection", "description": "In an effort to understand and predict the impact of space weather events on Earth, the Community-Coordinated Modeling Center (CCMC) at NASA Goddard Space Flight Center, routinely runs computer models of the many historical events. These model runs are then compared to actual data to determine ways to improve the model, and therefore forecasts of the impacts of future space weather events.In mid-December of 2006, the Sun erupted with a bright flare and coronal mass ejection (CME) that launched particles Earthward. While not the brightest or largest event observed, its impact on Earth was substantial, requiring some effort to protect satellites (ESA: Reacting to a solar flare).The visualization presented here is a CCMC run of a BATS-R-US model simulating the impact of this event on Earth. Here, lines are used to represent the 'flow direction' of magnetic field of the solar wind impacting Earth, as well as the effects on Earth's geomagnetic field. A 'cut-plane' through the data illustrates the changes in the particle density in the solar wind and magnetosphere. The color of the data represents a logarithmic scaling of density, with red as the highest (1000 particles per cubic centimeter) down to blue (0.01 particles per cubic centimeter). In this simulation, each frame of the movie corresponds to two minutes of real time.In the movie, we see vertical field lines of magnetic field carried by the solar wind, coming in from the left. As this field, and the plasma carrying it, strike Earth's magnetic field, they bend and reconnect, around the Earth. Some field lines actually reconnect to the polar regions of the Earth, providing a ready flow-path for particles to reach the ionosphere and generate aurora. This interaction between the solar wind and the plasma trapped in Earth's magnetosphere also creates a density enhancement between Earth and the solar wind helping to shield Earth from some of the effects. A lower density wake forms behind Earth (the blue region). There is a circular 'hole' around the Earth which is a gap in the model. || ", "release_date": "2014-09-25T10:00:00-04:00", "update_date": "2025-01-05T22:31:29.713646-05:00", "main_image": { "id": 452471, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004188/Earth_December2006_Pullout.noslate_GSEmove.HD1080i.0300_print.jpg", "filename": "Earth_December2006_Pullout.noslate_GSEmove.HD1080i.0300_print.jpg", "media_type": "Image", "alt_text": "This movie opens with a close-up view of Earth with geo-magnetic field lines. The camera pulls out and fades in a profile slice of the plasma density data.This video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } } }, { "id": 413139, "type": "details_page", "extra_data": null, "instance": { "id": 4167, "url": "https://svs.gsfc.nasa.gov/4167/", "page_type": "Visualization", "title": "The Big CME that Missed Earth", "description": "July of 2012 witnessed the eruption of a very large and fast solar coronal mass ejection (CME) (see NASA STEREO Observes One of the Fastest CMEs On Record and Carrington-class CME Narrowly Misses Earth ). While not directed at Earth, it was sufficiently large that it could have seriously disrupted the global electrical infrastructure. The event did impact STEREO-A of NASA's heliophysics fleet which provided a host of measurements (see Sentinels of the Heliosphere).One of the conditions which contributed to the high speed of this event is that two smaller CMEs were launched a little earlier, and these events cleared out much of the solar wind material, leaving little to slow the outflow of the July 23 event (UTC).In the visualizations below, generated from the Enlil space weather model, green represents particle density, usually protons and other ions. In green, we see the Parker spiral moving out from the sun generated by the sun's current sheet (Wikipedia). Red represents particles at high temperatures and shows the CME is hotter than the usual solar wind flow. Large changes in density are represented in blue. These three colors sometimes combine to tell us more about the characteristics of the event (noted in the 3-color Venn diagram below).However, if this CME had struck Earth's magnetosphere, which has a much stronger magnetic field, the changing magnetic field would induce much larger voltages in systems with long electrical conductors, such as power lines that run over long distances. These significantly higher voltages can damage power transformers. || ", "release_date": "2014-07-23T00:00:00-04:00", "update_date": "2025-01-04T00:05:05.071417-05:00", "main_image": { "id": 455573, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004167/2012July_high2AU.full.0327.jpg", "filename": "2012July_high2AU.full.0327.jpg", "media_type": "Image", "alt_text": "Enlil model run of the July 23, 2012 CME and events leading up to it. This movie provides a better view of the inner solar system for the CME event. The density color table has been altered accordingly. This view includes a 'top-down' view in the plane of Earth's orbit, as well as a slice perpendicular to the orbit which passes through Earth. We see the previous CME pass Earth, but not the July 23 event.", "width": 1920, "height": 1080, "pixels": 2073600 } } } ], "extra_data": {} }, { "id": 372277, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/#media_group_372277", "widget": "Card gallery", "title": "Transits", "caption": "", "description": "", "items": [ { "id": 413140, "type": "details_page", "extra_data": null, "instance": { "id": 4763, "url": "https://svs.gsfc.nasa.gov/4763/", "page_type": "Visualization", "title": "Mercury Transit, 2019 (SDO 4K imagery)", "description": "Mercury transit visible through the 171 angstrom filter on SDO. || AIA171_00025_print.jpg (1024x1024) [108.7 KB] || AIA171_00025_searchweb.png (320x180) [65.6 KB] || AIA171_00025_thm.png (80x40) [5.2 KB] || AIA171_2048p30.mp4 (2048x2048) [19.2 MB] || AIA171_1024p30.mp4 (1024x1024) [3.7 MB] || AIA171-Frames (4096x4096) [0 Item(s)] || AIA171-Time (4096x4096) [0 Item(s)] || AIA171_4096p30_h265.mp4 (4096x4096) [13.6 MB] || AIA171_4096p30_h265.webm (4096x4096) [2.7 MB] || ", "release_date": "2019-11-11T16:30:00-05:00", "update_date": "2025-02-02T22:42:44.095832-05:00", "main_image": { "id": 391227, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004763/AIA171_00025_print.jpg", "filename": "AIA171_00025_print.jpg", "media_type": "Image", "alt_text": "Mercury transit visible through the 171 angstrom filter on SDO.", "width": 1024, "height": 1024, "pixels": 1048576 } } } ], "extra_data": {} } ] }