File:SDO 20101212 1024 0211 (AIA).ogv

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DescriptionSDO 20101212 1024 0211 (AIA).ogv	English: AIA 0211 channel (as well as AIA 335) highlights the active region of the outer atmosphere of the Sun - the corona. Active regions, solar flares, and coronal mass ejections will appear bright here. The dark areas - called coronal holes - are places where very little radiation is emitted, yet are the main source of solar wind particles. Where: Active regions of the corona Wavelength: 211 angstroms (0.0000000211 m) = Extreme Ultraviolet Primary ions seen: 13 times ionized iron (Fe XIV) Characteristic temperature: 2 million K (3.6 million F)
Date	Taken on 12 December 2010
Source	20101212_1024_0211
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

This media is a product of the
Solar Dynamics Observatory
Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory

This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: 20101212_1024_0211.

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	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/Time	Thumbnail	Dimensions	User	Comment
current	13:28, 3 May 2024		5.7 s, 1,024 × 1,024 (1.99 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2010/12/12/20101212_1024_0211.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	1.03 Mbps	Completed 13:38, 3 May 2024	13 s
VP9 480P	426 kbps	Completed 15:20, 3 May 2024	6.0 s
VP9 360P	204 kbps	Completed 15:19, 3 May 2024	4.0 s
VP9 240P	106 kbps	Completed 15:19, 3 May 2024	2.0 s
WebM 360P	226 kbps	Completed 15:20, 3 May 2024	2.0 s
QuickTime 144p (MJPEG)	893 kbps	Completed 18:20, 12 October 2024	1.0 s

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