File:SDO 20100525 1024 0304 (AIA).ogv

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DescriptionSDO 20100525 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 25 May 2010
Source	20100525_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: 20100525_1024_0304.

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current	22:36, 5 May 2024		4.8 s, 1,024 × 1,024 (11.98 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2010/05/25/20100525_1024_0304.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	1.61 Mbps	Completed 00:30, 6 May 2024	21 s
Streaming 720p (VP9)	1.6 Mbps	Completed 00:30, 6 May 2024	17 s
VP9 480P	805 kbps	Completed 09:49, 6 May 2024	19 s
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