File:SDO 20180405 1024 1600 (AIA).ogv

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DescriptionSDO 20180405 1024 1600 (AIA).ogv	English: AIA 1600 channel (as well as AIA 1700) often shows a web-like pattern of bright areas that highlight places where bundles of magnetic fields lines are concentrated. However, small areas with a lot of field lines will appear black, usually near sunspots and active regions. Where: Transition region and upper photosphere Wavelength: 1600 angstroms (0.00000016 m) = Far Ultraviolet Primary ions seen: thrice ionized carbon (C IV) and Continuum Characteristic temperatures: 6,000 K (11,000 F), and 100,000 K (180,000 F)
Date	Taken on 5 April 2018
Source	20180405_1024_1600
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: 20180405_1024_1600.

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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	06:10, 11 February 2024		4.8 s, 1,024 × 1,024 (8.32 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2018/04/05/20180405_1024_1600.ogv via Commons:Spacemedia

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Format	Bitrate	Download	Status	Encode time
VP9 720P	1.6 Mbps		Completed 06:10, 11 February 2024	11 s
VP9 480P	721 kbps		Completed 07:04, 11 February 2024	12 s
VP9 360P	285 kbps		Completed 07:04, 11 February 2024	8.0 s
VP9 240P	116 kbps		Completed 07:04, 11 February 2024	4.0 s
WebM 360P	239 kbps		Completed 07:04, 11 February 2024	2.0 s
QuickTime 144p (MJPEG)		Not ready	Unknown status

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