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"https://svs.gsfc.nasa.gov/11460/", "page_type": "Produced Video", "title": "SDO: Year 4", "description": "The sun is always changing and NASA's Solar Dynamics Observatory is always watching. Launched on Feb. 11, 2010, SDO keeps a 24-hour eye on the entire disk of the sun, with a prime view of the graceful dance of solar material coursing through the sun's atmosphere, the corona. SDO's fourth year in orbit was no exception: NASA is releasing a movie of some of SDO's best sightings of the year, including massive solar explosions and giant sunspot shows. SDO captures images of the sun in 10 different wavelengths, each of which helps highlight a different temperature of solar material. Different temperatures can, in turn, show specific structures on the sun such as solar flares, which are giant explosions of light and x-rays, or coronal loops, which are streams of solar material traveling up and down looping magnetic field lines. The movie shows examples of both, as well as what's called prominence eruptions, when masses of solar material leap off the sun. The movie also shows a sunspot group on the solar surface. This sunspot, a magnetically strong and complex region appearing in mid-January 2014, was one of the largest in nine years. Scientists study these images to better understand the complex electromagnetic system causing the constant movement on the sun, which can ultimately have an effect closer to Earth, too: Flares and another type of solar explosion called coronal mass ejections can sometimes disrupt technology in space. Moreover, studying our closest star is one way of learning about other stars in the galaxy. NASA's Goddard Space Flight Center in Greenbelt, Md. built, operates, and manages the SDO spacecraft for NASA's Science Mission Directorate in Washington, D.C.SDO: Year One here.SDO: Year 2 here.SDO: Year 3 here.Information about the individual clips used in this video is here. || ", "release_date": "2014-02-11T12:00:00-05:00", "update_date": "2023-05-03T13:51:12.304065-04:00", "main_image": { "id": 458587, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011400/a011460/304_Year_4_blend_FINAL_16x9_1080.jpg", "filename": "304_Year_4_blend_FINAL_16x9_1080.jpg", "media_type": "Image", "alt_text": "Massive solar flares, graceful eruptions of solar material, and an enormous sunspot make up some of the imagery captured by NASA's Solar Dynamics Observatory during its fourth year in orbit. 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In the past two years, the sun generated more than 1,000 outbursts, including solar flares, coronal mass ejections and energetic particles that travel to the edge of the solar system. By recording these events in multiple wavelengths, scientists can unravel the process by which the roiling magnetic fields inside and around the sun cause it to erupt. For example, the above image showing light at 171 Angstroms and colorized in gold reveals the looping arcs of particles that coalesce around magnetic field lines in the sun's atmosphere during intense periods of solar activity. Other wavelengths make different features more readily visible to the human eye. Watch the video below highlighting some of the most amazing moments witnessed by SDO in its second year of operation. || ", "release_date": "2012-05-10T00:00:00-04:00", "update_date": "2023-05-03T13:53:05.147180-04:00", "main_image": { "id": 476425, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010900/a010972/COVER_sun_1024x576.jpg", "filename": "COVER_sun_1024x576.jpg", "media_type": "Image", "alt_text": "A breathtaking compilation of solar views you don't want to miss.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 3922, "url": "https://svs.gsfc.nasa.gov/3922/", "page_type": "Visualization", "title": "Growing Active Regions: January 2012", "description": "A group of active regions appear during the rise of solar cycle 25. 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"Visualization", "title": "Launching Filament: November 14, 2011", "description": "A large filament launches from the Sun in this sequence of 304 Ångstrom imagery from Solar Dynamics Observatory. || ", "release_date": "2012-03-31T00:00:00-04:00", "update_date": "2025-02-02T22:06:28.207119-05:00", "main_image": { "id": 477362, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003900/a003931/AIA304filament.00500_web.png", "filename": "AIA304filament.00500_web.png", "media_type": "Image", "alt_text": "Full resolution 4Kx4K frames", "width": 320, "height": 320, "pixels": 102400 } }, { "id": 3932, "url": "https://svs.gsfc.nasa.gov/3932/", "page_type": "Visualization", "title": "Survivor 2011: Comet Lovejoy vs. The Sun", "description": "Comet Lovejoy makes a close pass to the Sun, and survives.The Solar Dynamics Observatory (SDO) is actually repointed to better observe the comet's approach to the Sun. || ", "release_date": "2012-03-31T00:00:00-04:00", "update_date": "2025-03-10T00:02:02.274996-04:00", "main_image": { "id": 477376, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003900/a003932/LovejoyCloseup_stand.HD1080i.00600.jpg", "filename": "LovejoyCloseup_stand.HD1080i.00600.jpg", "media_type": "Image", "alt_text": "This movie zooms in for the comet approach and departure.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 3933, "url": "https://svs.gsfc.nasa.gov/3933/", "page_type": "Visualization", "title": "Sunspots on the Move: August 22, 2011", "description": "SDO/HMI movie of sunspots evolving across the solar disk. || HMI_IcChangingSpots.00300.jpg (4096x4096) [3.3 MB] || HMI_IcChangingSpots.00300_web.png (320x320) [89.7 KB] || HMI_IcChangingSpots.00300_thm.png (80x40) [3.8 KB] || HMI_IcChangingSpots.00300_searchweb.png (320x180) [57.8 KB] || HMI_Ic_ChangingSpots_1Kx1K.mov (1024x1024) [28.6 MB] || HMI_Ic_ChangingSpots_4Kx4K.webmhd.webm (960x540) [3.0 MB] || HMI_Ic_ChangingSpots_2Kx2K.mov (2048x2048) [168.7 MB] || 4096x4096_1x1_30p (4096x4096) [0 Item(s)] || HMI_Ic_ChangingSpots_4Kx4K.mov (4096x4096) [17.8 GB] || ", "release_date": "2012-03-31T00:00:00-04:00", "update_date": "2025-02-02T22:06:31.734231-05:00", "main_image": { "id": 477113, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003900/a003933/HMI_IcChangingSpots.00300_web.png", "filename": "HMI_IcChangingSpots.00300_web.png", "media_type": "Image", "alt_text": "SDO/HMI movie of sunspots evolving across the solar disk.", "width": 320, "height": 320, "pixels": 102400 } }, { "id": 3904, "url": "https://svs.gsfc.nasa.gov/3904/", "page_type": "Visualization", "title": "An X-class Flare of Solar Cycle 24 as Seen by SDO", "description": "An X1.1 flare was seen by SDO on March 5, 2012. This is the view from the 171 Angstrom filter. || ", "release_date": "2012-03-13T00:00:00-04:00", "update_date": "2025-02-02T22:05:12.149173-05:00", "main_image": { "id": 478444, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003900/a003904/SDO_2012-03_171_Flare.00400_web.png", "filename": "SDO_2012-03_171_Flare.00400_web.png", "media_type": "Image", "alt_text": "These are full-view frames and movies of the X-class flare event.", "width": 320, "height": 320, "pixels": 102400 } }, { "id": 3920, "url": "https://svs.gsfc.nasa.gov/3920/", "page_type": "Visualization", "title": "The Rising Solar Cycle: X5.4 Flare ('W' sunspot group) seen by SDO", "description": "Sunspot group 1429 of solar cycle 24 has launched an X5.4 flare can coronal mass ejection (CME) that is forecast to impact the EarthThis visualization has the full 4Kx4K frames from the 17.1 nm and 13.1 nm filters on the Solar Dynamics Observatory. 2Kx2K MPEG-4 movies are also available. || ", "release_date": "2012-03-07T14:00:00-05:00", "update_date": "2025-02-02T22:05:54.010075-05:00", "main_image": { "id": 478377, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003900/a003920/SDO_2012-03-07_171_X5Flare.00400_web.png", "filename": "SDO_2012-03-07_171_X5Flare.00400_web.png", "media_type": "Image", "alt_text": "The solar flare in the 171A (17.1nm) filter", "width": 320, "height": 320, "pixels": 102400 } }, { "id": 3918, "url": "https://svs.gsfc.nasa.gov/3918/", "page_type": "Visualization", "title": "Solar Flare & CME from January 2012", "description": "A solar flare and coronal mass ejection (CME) observed by SDO in January 2012. || ", "release_date": "2012-03-07T00:00:00-05:00", "update_date": "2025-02-02T22:05:43.598932-05:00", "main_image": { "id": 478575, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003900/a003918/SDO_Flare_171_Jan2012.01000_web.png", "filename": "SDO_Flare_171_Jan2012.01000_web.png", "media_type": "Image", "alt_text": "A movie of the solar flare event.", "width": 320, "height": 320, "pixels": 102400 } }, { "id": 3839, "url": "https://svs.gsfc.nasa.gov/3839/", "page_type": "Visualization", "title": "Incredible Solar Flare, Prominence Eruption and CME Event (171 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 3838 (304 Ångstroms), 3840 (211 Ångstroms) and 3841 (1700 Ångstroms). || ", "release_date": "2011-07-01T10:00:00-04:00", "update_date": "2025-02-02T00:01:24.120933-05:00", "main_image": { "id": 484965, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003839/SDO171Full_stand.HD1080i.00100.jpg", "filename": "SDO171Full_stand.HD1080i.00100.jpg", "media_type": "Image", "alt_text": "These movies present the six hour interval around the event, a one minute per animation frame.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 3840, "url": "https://svs.gsfc.nasa.gov/3840/", "page_type": "Visualization", "title": "Incredible Solar Flare, Prominence Eruption and CME Event (211 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), 3838 (304 Ångstroms) and 3841 (1700 Ångstroms). || ", "release_date": "2011-07-01T10:00:00-04:00", "update_date": "2025-02-02T22:02:50.495232-05:00", "main_image": { "id": 484994, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003840/SDO211Full_stand.HD1080i.00100.jpg", "filename": "SDO211Full_stand.HD1080i.00100.jpg", "media_type": "Image", "alt_text": "These movies present the six hour interval around the event, a one minute per animation frame.", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "sources": [ { "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 } } ], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }