File:SDO 20180606 1024 1700 (AIA).ogv

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DescriptionSDO 20180606 1024 1700 (AIA).ogv	English: AIA 1700 channel (as well as AIA 1600) 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: Temperature minimum and photosphere Wavelength: 1700 angstroms (0.00000017 m) = Far Ultraviolet Primary ions seen: Continuum Characteristic temperature: 6,000 K (11,000 F)
Date	Taken on 6 June 2018
Source	20180606_1024_1700
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

This media is a product of the
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: 20180606_1024_1700.

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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	04:02, 11 February 2024		4.8 s, 1,024 × 1,024 (5.87 MB)	OptimusPrimeBot (talk \| contribs)	#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2018/06/06/20180606_1024_1700.ogv via Commons:Spacemedia

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Format	Bitrate	Status	Encode time
VP9 720P	1.51 Mbps	Completed 04:02, 11 February 2024	17 s
VP9 480P	671 kbps	Completed 04:29, 11 February 2024	11 s
VP9 360P	245 kbps	Completed 04:29, 11 February 2024	6.0 s
VP9 240P	97 kbps	Completed 04:29, 11 February 2024	4.0 s
WebM 360P	216 kbps	Completed 04:29, 11 February 2024	2.0 s
QuickTime 144p (MJPEG)	544 kbps	Completed 21:05, 13 October 2024	1.0 s

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