File:SDO 20210325 1024 0211 (AIA).ogv

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DescriptionSDO 20210325 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 25 March 2021
Source	20210325_1024_0211
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

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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: 20210325_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	11:14, 17 January 2024		7.0 s, 1,024 × 1,024 (1.99 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2021/03/25/20210325_1024_0211.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	960 kbps	Completed 11:14, 17 January 2024	6.0 s
VP9 480P	446 kbps	Completed 11:14, 17 January 2024	4.0 s
VP9 360P	210 kbps	Completed 11:14, 17 January 2024	2.0 s
VP9 240P	111 kbps	Completed 11:14, 17 January 2024	2.0 s
WebM 360P	194 kbps	Completed 11:14, 17 January 2024	2.0 s
QuickTime 144p (MJPEG)	871 kbps	Completed 15:08, 1 December 2024	0.0 s

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