File:SDO 20150620 1024 0171 (AIA).ogv

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DescriptionSDO 20150620 1024 0171 (AIA).ogv	English: AIA 0171 channel is especially good at showing coronal loops - the arcs extending off of the Sun where plasma moves along magnetic field lines. The brightest spots seen here are locations where the magnetic field near the surface is exceptionally strong. Where: Quiet corona and upper transition region Wavelength: 171 angstroms (0.0000000171 m) = Extreme Ultraviolet Primary ions seen: 8 times ionized iron (Fe IX) Characteristic temperature: 1 million K (1.8 million F)
Date	Taken on 20 June 2015
Source	20150620_1024_0171
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: 20150620_1024_0171.

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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	06:25, 18 February 2024		4.8 s, 1,024 × 1,024 (2.13 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2015/06/20/20150620_1024_0171.ogv via Commons:Spacemedia

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Format	Bitrate	Download	Status	Encode time
VP9 720P	1.24 Mbps		Completed 06:25, 18 February 2024	7.0 s
VP9 480P	579 kbps		Completed 06:42, 18 February 2024	7.0 s
VP9 360P	322 kbps		Completed 06:42, 18 February 2024	4.0 s
VP9 240P	153 kbps		Completed 06:41, 18 February 2024	4.0 s
WebM 360P	334 kbps		Completed 06:42, 18 February 2024	2.0 s
QuickTime 144p (MJPEG)		Not ready	Unknown status

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