File:SDO 20111216 1024 0304 (AIA).ogv

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DescriptionSDO 20111216 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 16 December 2011
Source	20111216_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: 20111216_1024_0304.

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current	10:34, 23 July 2024		4.9 s, 1,024 × 1,024 (10.75 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2011/12/16/20111216_1024_0304.ogv via Commons:Spacemedia

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Format	Bitrate	Download	Status	Encode time
VP9 720P	1.6 Mbps		Completed 13:11, 23 July 2024	24 s
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VP9 360P	491 kbps		Completed 19:10, 23 July 2024	8.0 s
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