File:SDO 20121104 1024 0193 (AIA).ogv

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DescriptionSDO 20121104 1024 0193 (AIA).ogv	English: AIA 0193 channel highlights the outer atmosphere of the Sun - called the corona - as well as hot flare plasma. Hot 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: Corona and hot flare plasma Wavelength: 193 angstroms (0.0000000193 m) = Extreme Ultraviolet Primary ions seen: 11 times ionized iron (Fe XII) Characteristic temperature: 1.25 million K (2.25 million F)
Date	Taken on 4 November 2012
Source	20121104_1024_0193
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: 20121104_1024_0193.

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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	14:25, 21 April 2024		5.7 s, 1,024 × 1,024 (1.51 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2012/11/04/20121104_1024_0193.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	882 kbps	Completed 14:40, 21 April 2024	10 s
VP9 480P	369 kbps	Completed 16:29, 21 April 2024	7.0 s
VP9 360P	188 kbps	Completed 16:28, 21 April 2024	6.0 s
VP9 240P	102 kbps	Completed 16:28, 21 April 2024	4.0 s
WebM 360P	209 kbps	Completed 16:28, 21 April 2024	2.0 s
QuickTime 144p (MJPEG)	964 kbps	Completed 04:16, 27 November 2024	0.0 s

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