{ "id": 40245, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/", "page_type": "Gallery", "title": "Hyperwall Sun", "description": "Heliophysics related hyperwall ready visualizations\nReturn to Main Hyperwall Gallery.", "release_date": "2015-07-30T00:00:00-04:00", "update_date": "2015-11-18T00:00:00-05:00", "main_image": { "id": 858868, "url": "https://svs.gsfc.nasa.gov/images/gallery/Hyperwall/a011912_s3-1024_searchweb.png", "filename": "a011912_s3-1024_searchweb.png", "media_type": "Image", "alt_text": "Heliophysics encompasses science that improves our un­derstanding of fundamental physical processes throughout the solar system, and enables us to understand how the Sun, as the major driver of the energy throughout the solar system, impacts our technological society.", "width": 180, "height": 320, "pixels": 57600 }, "media_groups": [ { "id": 370922, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/#media_group_370922", "widget": "Basic text (large)", "title": "Overview", "caption": "", "description": "Heliophysics related hyperwall ready visualizations\n

Return to Main Hyperwall Gallery.", "items": [], "extra_data": {} }, { "id": 370923, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/#media_group_370923", "widget": "Card gallery", "title": "Overview", "caption": "", "description": "", "items": [ { "id": 407466, "type": "details_page", "extra_data": null, "instance": { "id": 4288, "url": "https://svs.gsfc.nasa.gov/4288/", "page_type": "Visualization", "title": "The 2015 Earth-Orbiting Heliophysics Fleet", "description": "Movie showing the heliosphysics missions from near Earth orbit out to the orbit of the Moon.This video is also available on our YouTube channel. || Helio2015A.MMStour.slate_RigRHS.HD1080i.0500_print.jpg (1024x576) [112.6 KB] || Helio2015A.MMStour.HD1080.webm (1920x1080) [6.7 MB] || WithoutTimeStamp (1920x1080) [128.0 KB] || Helio2015A.MMStour.HD1080.mov (1920x1080) [196.3 MB] || Helio2015_4288.pptx [198.6 MB] || Helio2015_4288.key [201.3 MB] || ", "release_date": "2015-06-10T00:00:00-04:00", "update_date": "2024-12-15T22:20:35.001660-05:00", "main_image": { "id": 443168, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004200/a004288/Helio2015A.MMStour.slateHR_RigRHS.HD1080i.0364_print.jpg", "filename": "Helio2015A.MMStour.slateHR_RigRHS.HD1080i.0364_print.jpg", "media_type": "Image", "alt_text": "Moving out further, we see SDO as we pass geosynchronous orbit.", "width": 1024, "height": 576, "pixels": 589824 } } } ], "extra_data": {} }, { "id": 370924, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/#media_group_370924", "widget": "Card gallery", "title": "Heliosphere", "caption": "", "description": "Plasmas and their embedded magnetic fields affect the formation, evolution and destiny of planets and planetary systems. The heliosphere shields the solar system from galactic cosmic radiation. Our habitable planet is shielded by its magnetic fi eld, protecting it from solar and cosmic particle radiation and from erosion of the atmosphere by the solar wind. Planets without a shielding magnetic field, such as Mars and Venus, are exposed to those processes and evolve differently. And on Earth, the magnetic field changes strength and configuration during its occasional polarity reversals, altering the shielding of the planet from external radiation sources.", "items": [ { "id": 407467, "type": "media_group", "extra_data": null, "title": "Solar Dynamics Observatory - Argo view", "caption": "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. ", "instance": { "id": 461370, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004117/SDOargoFD_rotorzoom_stand.HD1080i.01800_web.png", "filename": "SDOargoFD_rotorzoom_stand.HD1080i.01800_web.png", "media_type": "Image", "alt_text": "Views of the Sun from multiple wavelengths (mostly ultraviolet not visible from the ground) taken by Solar Dynamics Observatory (SDO).", "width": 180, "height": 320, "pixels": 57600 } }, { "id": 407468, "type": "media_group", "extra_data": null, "title": "NuSTAR Sun", "caption": "Blue-White areas in composite image with NuSTAR data show most energetic spots. ", "instance": { "id": 433232, "url": "https://svs.gsfc.nasa.gov/vis/a030000/a030700/a030726/nustar_sun_PIA19821_searchweb.png", "filename": "nustar_sun_PIA19821_searchweb.png", "media_type": "Image", "alt_text": "Blue-White areas in composite image with NuSTAR data show most energetic spots. ", "width": 180, "height": 320, "pixels": 57600 } }, { "id": 407469, "type": "details_page", "extra_data": null, "instance": { "id": 11868, "url": "https://svs.gsfc.nasa.gov/11868/", "page_type": "Produced Video", "title": "NASA's SDO Observes a Cinco de Mayo Solar Flare", "description": "Video of May 5, 2015 X2.7 flare.Credit: NASA/GSFC/SDO || May_5_2015_Flare_Still_304-171.png (1920x1080) [8.1 MB] || May_5_2015_Flare_Still_304-171.jpg (1920x1080) [415.9 KB] || May_5_2015_Flare_Still_304-171_print.jpg (1024x576) [145.7 KB] || May_5_2015_Flare_Still_304-171_web.png (320x180) [83.3 KB] || 11868_May_5_X_Flare_MPEG4_1920X1080_2997.mp4 (1920x1080) [42.2 MB] || 11868_May_5_X_Flare_H264_Good_1920x1080_2997.webm (1920x1080) [4.8 MB] || 11868_May_5_X_Flare_1280x720.wmv (1280x720) [23.1 MB] || 11868_May_5_X_Flare_appletv.m4v (960x540) [19.0 MB] || 11868_May_5_X_Flare_appletv_subtitles.m4v (960x540) [19.0 MB] || 11868_May_5_X_Flare_ipod_lg.m4v (640x360) [7.1 MB] || 11868_May_5_X_Flare_ipod_sm.mp4 (320x240) [3.6 MB] || 11868_May_5_X_Flare_SRT_Captions.en_US.srt [230 bytes] || 11868_May_5_X_Flare_SRT_Captions.en_US.vtt [243 bytes] || 11868_May_5_X_Flare_ProRes_1920x1080_2997.mov (1920x1080) [674.9 MB] || 11868_May_5_X_Flare_H264_Best_1920x1080_2997.mov (1920x1080) [682.7 MB] || 11868_May_5_X_Flare_H264_Good_1920x1080_2997.mov (1920x1080) [219.1 MB] || ", "release_date": "2015-05-06T09:45:00-04:00", "update_date": "2024-10-06T23:38:49.781474-04:00", "main_image": { "id": 443402, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011800/a011868/May_5_2015_Five_Across_no_Labels_print.jpg", "filename": "May_5_2015_Five_Across_no_Labels_print.jpg", "media_type": "Image", "alt_text": "NASA's Solar Dynamics Observatory captured these images of a solar flare – as seen in the bright flash on the left – on May 5, 2015. Each image shows a different wavelength of extreme ultraviolet light that highlights a different temperature of material on the sun. By comparing different images, scientists can better understand the movement of solar matter and energy during a flare. From left to right, the wavelengths are: visible light, 171 angstroms, 304 angstroms, 193 angstroms and 131 angstroms. Each wavelength has been colorized. Unlabeled.Credit: NASA/GSFC/SDO", "width": 1024, "height": 576, "pixels": 589824 } } } ], "extra_data": {} }, { "id": 370925, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/#media_group_370925", "widget": "Card gallery", "title": "Magnetospheres", "caption": "", "description": "Determine changes in the Earth's magnetosphere, ionosphere, and upper atmosphere in order to enable specification, prediction, and mitigation of their effects. Heliophysics seeks to develop an understanding of the response of the near-Earth plasma regions to space weather. This complex, highly coupled system protects Earth from the worst solar disturbances while redistributing energy and mass throughout.", "items": [ { "id": 407470, "type": "media_group", "extra_data": null, "title": "NASA Observes Auroras Across Canada", "caption": "These aurora images were taken from the ground looking up with a network of all-sky cameras spread across Canada, studying auroras in collaboration with NASA’s Time History of Events and Macroscale Interactions during Substorms, or THEMIS, mission. Taking images of aurora from the ground in conjunction with satellite data taken from above the atmosphere gives scientists a more comprehensive picture of how and why the aurora form. The ground-based camera network is also observing this week’s auroras.

The aurora data is provided courtesy of S. Mende at University California Berkeley and E. Donovan at the University of Calgary, logistical support in fielding and data retrieval from the ground-based stations is provided by the Canadian Space Agency. The array of aurora images is funded by NSF in support of GIMNAST through grant AGS-1004736.

Credit: NASA/CSA/University of California, Berkeley/University of Calgary/NSF", "instance": { "id": 438145, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012000/a012040/Storm_0386_searchweb.png", "filename": "Storm_0386_searchweb.png", "media_type": "Image", "alt_text": "These aurora images were taken from the ground looking up with a network of all-sky cameras spread across Canada, studying auroras in collaboration with NASA’s Time History of Events and Macroscale Interactions during Substorms, or THEMIS, mission. Taking images of aurora from the ground in conjunction with satellite data taken from above the atmosphere gives scientists a more comprehensive picture of how and why the aurora form. The ground-based camera network is also observing this week’s auroras. The aurora data is provided courtesy of S. Mende at University California Berkeley and E. Donovan at the University of Calgary, logistical support in fielding and data retrieval from the ground-based stations is provided by the Canadian Space Agency. The array of aurora images is funded by NSF in support of GIMNAST through grant AGS-1004736.Credit: NASA/CSA/University of California, Berkeley/University of Calgary/NSF", "width": 180, "height": 320, "pixels": 57600 } } ], "extra_data": {} }, { "id": 370926, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-sun/#media_group_370926", "widget": "Card gallery", "title": "Space Environment", "caption": "", "description": "Understand the causes and subsequent evolution of solar activity that affects Earth's space climate and environment. The climate and space environment of Earth are significantly determined by the impact of plasma, particle, and radiative outputs from the Sun. Therefore, it is essential to understand the Sun, determine how predictable solar activity truly is, and develop the capability to forecast solar activity and the evolution of disturbances as they propagate to Earth.", "items": [ { "id": 407471, "type": "media_group", "extra_data": null, "title": "The Big CME that Missed Earth", "caption": "Enlil model run of the July 23, 2012 CME and events leading up to it. 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.", "instance": { "id": 455555, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004167/2012July_high6AU.full.0327_web.png", "filename": "2012July_high6AU.full.0327_web.png", "media_type": "Image", "alt_text": "Enlil model run of the July 23, 2012 CME and events leading up to it. This view includes a 'top-down' view in the plane of Earth's orbit, but rotated so STEREO-A is the focus of the event. The slice perpendicular to the orbit passes through STEREO-A so we can see the July 23 event hit STEREO-A.", "width": 180, "height": 320, "pixels": 57600 } } ], "extra_data": {} } ] }