File:SDO 20130611 1024 0304 (AIA).ogv

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DescriptionSDO 20130611 1024 0304 (AIA).ogv	English: AIA 0304 channel is especially good at showing areas where cooler dense plumes of plasma (filaments and prominences) are located above the visible surface of the Sun. Many of these features either can't be seen or appear as dark lines in the other channels. The bright areas show places where the plasma has a high density. Where: Upper chromosphere and lower transition region Wavelength: 304 angstroms (0.0000000304 m) = Extreme Ultraviolet Primary ions seen: singly ionized helium (He II) Characteristic temperature: 50,000 K (90,000 F)
Date	Taken on 11 June 2013
Source	20130611_1024_0304
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: 20130611_1024_0304.

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	20:52, 17 March 2024		5.3 s, 1,024 × 1,024 (11.38 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2013/06/11/20130611_1024_0304.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	1.61 Mbps	Completed 20:52, 17 March 2024	27 s
Streaming 720p (VP9)	1.6 Mbps	Completed 20:52, 17 March 2024	28 s
VP9 480P	809 kbps	Completed 22:47, 17 March 2024	12 s
Streaming 480p (VP9)	807 kbps	Completed 22:47, 17 March 2024	13 s
VP9 360P	491 kbps	Completed 22:47, 17 March 2024	9.0 s
Streaming 360p (VP9)	491 kbps	Completed 22:46, 17 March 2024	9.0 s
VP9 240P	217 kbps	Completed 22:46, 17 March 2024	5.0 s
Streaming 240p (VP9)	217 kbps	Completed 22:46, 17 March 2024	5.0 s
WebM 360P	586 kbps	Completed 22:46, 17 March 2024	2.0 s
Streaming 144p (MJPEG)	996 kbps	Completed 22:46, 17 March 2024	1.0 s

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