File:SDO 20221201 1024 1700 (AIA).ogv

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Original file (Ogg Theora video file, length 7.2 s, 1,024 × 1,024 pixels, 10.34 Mbps, file size: 8.88 MB)

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Description
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 1 December 2022
Source 20221201_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: 20221201_1024_1700.

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Public domain 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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current19:49, 2 September 20237.2 s, 1,024 × 1,024 (8.88 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2022/12/01/20221201_1024_1700.ogv via Commons:Spacemedia

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Format Bitrate Download Status Encode time
VP9 720P 1.86 Mbps Completed 19:50, 2 September 2023 15 s
VP9 480P 503 kbps Completed 19:50, 2 September 2023 8.0 s
VP9 360P 156 kbps Completed 19:50, 2 September 2023 4.0 s
VP9 240P 67 kbps Completed 19:49, 2 September 2023 2.0 s
WebM 360P 517 kbps Completed 19:49, 2 September 2023 2.0 s
QuickTime 144p (MJPEG) Not ready Unknown status

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