File:SDO 20101117 1024 HMID (HMI).ogv

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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 17 November 2010
Source 20101117_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: 20101117_1024_HMID.

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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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current12:15, 6 May 20245.7 s, 1,024 × 1,024 (24.41 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://sdo.gsfc.nasa.gov/assets/img/dailymov/2010/11/17/20101117_1024_HMID.ogv via Commons:Spacemedia

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