File:PIA11237 - Churning Prominence.ogv

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Original file(Ogg Theora video file, length 17 s, 1,192 × 1,184 pixels, 9.6 Mbps, file size: 19.41 MB)

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English: A solar prominence rose up along the edge of the sun and twisted and churned for about two days before falling apart (Jan. 23-24, 2017). The dynamic action was generated by competing magnetic forces. The images were taken in a wavelength extreme ultraviolet light that observes activity close to the solar surface, perfect for capturing prominences, which are notoriously unstable clouds of plasma suspended above the sun. SDO is managed by NASA's Goddard Space Flight Center, Greenbelt, Maryland, for NASA's Science Mission Directorate, Washington. Its Atmosphere Imaging Assembly was built by the Lockheed Martin Solar Astrophysics Laboratory (LMSAL), Palo Alto, California.
Date 23 – 24 January 2017 (published )
Source Catalog page · Full-res (MP4)
Author NASA/GSFC/Solar Dynamics Observatory
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA11237.

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Solar Dynamics Observatory
Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current23:29, 30 January 201717 s, 1,192 × 1,184 (19.41 MB)PhilipTerryGraham (talk | contribs)User created page with UploadWizard

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VP9 1080P 4.78 Mbps Completed 10:02, 6 September 2018 1 min 17 s
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VP9 720P 2.34 Mbps Completed 10:01, 6 September 2018 1 min 5 s
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WebM 360P 506 kbps Completed 21:59, 17 March 2017 35 s
Streaming 144p (MJPEG) 854 kbps Completed 21:22, 17 November 2023 1.0 s

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