File:SDO 20130604 1024 0171 (AIA).ogv

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DescriptionSDO 20130604 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 4 June 2013
Source	20130604_1024_0171
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: 20130604_1024_0171.

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	21:00, 17 March 2024		5.6 s, 1,024 × 1,024 (2.69 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2013/06/04/20130604_1024_0171.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	1.2 Mbps	Completed 21:00, 17 March 2024	15 s
Streaming 720p (VP9)	1.2 Mbps	Completed 21:00, 17 March 2024	10 s
VP9 480P	580 kbps	Completed 22:58, 17 March 2024	7.0 s
Streaming 480p (VP9)	582 kbps	Completed 22:58, 17 March 2024	8.0 s
VP9 360P	307 kbps	Completed 22:58, 17 March 2024	6.0 s
Streaming 360p (VP9)	307 kbps	Completed 22:58, 17 March 2024	6.0 s
VP9 240P	146 kbps	Completed 22:58, 17 March 2024	4.0 s
Streaming 240p (VP9)	146 kbps	Completed 22:58, 17 March 2024	3.0 s
WebM 360P	296 kbps	Completed 22:58, 17 March 2024	2.0 s
Streaming 144p (MJPEG)	973 kbps	Completed 22:58, 17 March 2024	1.0 s

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