File:SDO 20110115 1024 HMID (HMI).ogv

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Original file (Ogg Theora video file, length 3.7 s, 1,024 × 1,024 pixels, 37.37 Mbps, file size: 16.26 MB)

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Description
English: Sun's dopplergram as pictured by SDO HMI. Grays shades on the picture are associated with various speeds. Light areas are getting farther while dark ones are getting closer.
Français : Dopplergramme du soleil tel que représenté par l'observatoire SDO. Les tons de gris sur l'image représentent la vitesse. Les zones sombres s'approchent de nous et les zones claires s'éloignent.
Date Taken on 15 January 2011
Source 20110115_1024_HMID
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 Helioseismic and Magnetic Imager (HMI) 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: 20110115_1024_HMID.

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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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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current14:23, 30 April 20243.7 s, 1,024 × 1,024 (16.26 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2011/01/15/20110115_1024_HMID.ogv via Commons:Spacemedia

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Format Bitrate Download Status Encode time
VP9 720P 1.32 Mbps Completed 15:48, 30 April 2024 14 s
VP9 480P 808 kbps Completed 21:09, 30 April 2024 12 s
VP9 360P 457 kbps Completed 21:09, 30 April 2024 9.0 s
VP9 240P 187 kbps Completed 21:08, 30 April 2024 4.0 s
WebM 360P 496 kbps Completed 21:09, 30 April 2024 2.0 s
QuickTime 144p (MJPEG) 837 kbps Completed 07:11, 26 November 2024 1.0 s

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