File:SDO 20170529 1024 0304 (AIA).ogv

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DescriptionSDO 20170529 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 29 May 2017
Source	20170529_1024_0304
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

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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: 20170529_1024_0304.

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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	05:48, 13 February 2024		4.8 s, 1,024 × 1,024 (6.02 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2017/05/29/20170529_1024_0304.ogv via Commons:Spacemedia

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Format	Bitrate	Download	Status	Encode time
VP9 720P	1.6 Mbps		Completed 06:42, 13 February 2024	16 s
VP9 480P	771 kbps		Completed 10:39, 13 February 2024	10 s
VP9 360P	403 kbps		Completed 10:39, 13 February 2024	21 s
VP9 240P	177 kbps		Completed 10:39, 13 February 2024	5.0 s
WebM 360P	419 kbps		Completed 10:39, 13 February 2024	2.0 s
QuickTime 144p (MJPEG)		Not ready	Unknown status

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