The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds so each second in this video corresponds to 6 minutes of real time. The video covers 4:30 UTC on July 19th to 2:00 UTC on July 20th, a period of 21 hours and 30 minutes.
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"Heliophysics", "Hyperwall", "SDO", "Solar Activity", "Solar Dynamics Observatory", "Solar Flares", "Solar Ultraviolet", "Solar Wind", "Space Weather", "Sun-earth Interactions" ], "recommended_pages": [], "related": [ { "id": 11198, "url": "https://svs.gsfc.nasa.gov/11198/", "page_type": "Produced Video", "title": "Raindrops Falling On The Sun", "description": "On July 19, 2012, million-degree plasma in the sun's atmosphere began to cool and fall to the surface, resulting in a dazzling magnetic display known as coronal rain. Because the plasma is charged, it's strongly influenced by the sun's magnetic field. As it rained down, it condensed along twisted magnetic field lines close to the surface and formed giant streaming arcs, some as tall as five Earths stacked high. An ultra high-definition telescope aboard NASA's Solar Dynamics Observatory (SDO) captured images of the display, which lasted hours and was initiated by two eruptive events on the sun: a solar flare and coronal mass ejection. Scientists used a 304-angstrom-wavelength filter to see the plasma downpour. Watch the video to see it for yourself. || ", "release_date": "2013-03-28T00:00:00-04:00", "update_date": "2023-05-03T13:52:17.060149-04:00", "main_image": { "id": 466939, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011100/a011198/cover-1920.jpg", "filename": "cover-1920.jpg", "media_type": "Image", "alt_text": "A NASA spacecraft records a plasma downpour in ultra HD.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 11168, "url": "https://svs.gsfc.nasa.gov/11168/", "page_type": "Produced Video", "title": "SDO Sees Fiery Looping Rain on the Sun", "description": "Eruptive events on the sun can be wildly different. Some come just with a solar flare, some with an additional ejection of solar material called a coronal mass ejection (CME), and some with complex moving structures in association with changes in magnetic field lines that loop up into the sun's atmosphere, the corona. On July 19, 2012, an eruption occurred on the sun that produced all three. A moderately powerful solar flare exploded on the sun's lower right hand limb, sending out light and radiation. Next came a CME, which shot off to the right out into space. And then, the sun treated viewers to one of its dazzling magnetic displays — a phenomenon known as coronal rain. Over the course of the next day, hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, themselves, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 angstroms, which highlights material at a temperature of about 50,000 Kelvin. This plasma acts as a tracer, helping scientists watch the dance of magnetic fields on the sun, outlining the fields as it slowly falls back to the solar surface. The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds, and the movie plays at 30 frames per second, so each second in this video corresponds to 6 minutes of real time. The video covers 12:30 a.m. EDT to 10:00 p.m. EDT on July 19, 2012.Watch this video on YouTube. || ", "release_date": "2013-02-20T10:00:00-05:00", "update_date": "2023-05-03T13:52:23.303233-04:00", "main_image": { "id": 469204, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011100/a011168/Raining_Loops_Still_2.jpg", "filename": "Raining_Loops_Still_2.jpg", "media_type": "Image", "alt_text": "On July 19, 2012, an eruption occurred on the sun that produced a moderately powerful solar flare and a dazzling magnetic display known as coronal rain. Hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 angstroms, and outlining the fields as it slowly falls back to the solar surface.Music: \"Thunderbolt\" by Lars Leonhard, courtesy of artist.For complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 11203, "url": "https://svs.gsfc.nasa.gov/11203/", "page_type": "Produced Video", "title": "SDO: Year 3", "description": "On Feb. 11, 2010, NASA launched an unprecedented solar observatory into space. The Solar Dynamics Observatory (SDO) flew up on an Atlas V rocket, carrying instruments that scientists hoped would revolutionize observations of the sun. If all went according to plan, SDO would provide incredibly high-resolution data of the entire solar disk almost as quickly as once a second. When the science team released its first images in April of 2010, SDO's data exceeded everyone's hopes and expectations, providing stunningly detailed views of the sun. In the three years since then, SDO's images have continued to show breathtaking pictures and movies of eruptive events on the sun. Such imagery is more than just pretty, they are the very data that scientists study. By highlighting different wavelengths of light, scientists can track how material on the sun moves. Such movement, in turn, holds clues as to what causes these giant explosions, which, when Earth-directed, can disrupt technology in space. SDO is the first mission in a NASA's Living With a Star program, the goal of which is to develop the scientific understanding necessary to address those aspects of the sun-Earth system that directly affect our lives and society. 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.Information about the individual clips used in this video is here.Watch this video on YouTube. || ", "release_date": "2013-02-11T10:00:00-05:00", "update_date": "2025-02-02T00:20:19.989382-05:00", "main_image": { "id": 468557, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011203/Flux_Rope_Blend_Still.jpg", "filename": "Flux_Rope_Blend_Still.jpg", "media_type": "Image", "alt_text": "Blended 131 angstrom and 171 angstrom images of July 19, 2012 flare and CME.", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }