File:SDO 20130423 1024 0335 (AIA).ogv

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DescriptionSDO 20130423 1024 0335 (AIA).ogv	English: AIA 0335 channel (as well as AIA 211) 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 - or 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: 335 angstroms (0.0000000335 m) = Extreme Ultraviolet Primary ions seen: 15 times ionized iron (Fe XVI) Characteristic temperature: 2.8 million K (5 million F)
Date	Taken on 23 April 2013
Source	20130423_1024_0335
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: 20130423_1024_0335.

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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	21:53, 17 March 2024		5.7 s, 1,024 × 1,024 (5.89 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2013/04/23/20130423_1024_0335.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	1.1 Mbps	Completed 21:53, 17 March 2024	11 s
VP9 480P	498 kbps	Completed 00:14, 18 March 2024	7.0 s
VP9 360P	195 kbps	Completed 00:14, 18 March 2024	4.0 s
VP9 240P	92 kbps	Completed 00:14, 18 March 2024	3.0 s
WebM 360P	185 kbps	Completed 00:14, 18 March 2024	2.0 s
QuickTime 144p (MJPEG)	818 kbps	Completed 08:46, 27 November 2024	1.0 s

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