File:SDO 20240707 1024 1600 (AIA).ogv

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Original file ‎(Ogg Theora video file, length 7.2 s, 1,024 × 1,024 pixels, 8.23 Mbps, file size: 7.06 MB)

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Description
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 7 July 2024
Source 20240707_1024_1600
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: 20240707_1024_1600.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
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Licensing

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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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current05:17, 8 July 20247.2 s, 1,024 × 1,024 (7.06 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2024/07/07/20240707_1024_1600.ogv via Commons:Spacemedia

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Format Bitrate Download Status Encode time
VP9 720P 1.54 Mbps Completed 05:35, 8 July 2024 1 min 20 s
Streaming 720p (VP9) 1.54 Mbps Completed 05:34, 8 July 2024 23 s
VP9 480P Not ready Added to Job queue 1 day, 3 hours, 5 minutes and 22 seconds ago
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