File:SDO Venus Transit 2012.ogv

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Original file (Ogg Theora video file, length 38 s, 1,280 × 720 pixels, 1.99 Mbps, file size: 9.06 MB)

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Description
English: The 2012 Venus transit as seen in the 171 Å wavelength, imaged by the Solar Dynamics Observatory. This channel is especially good at showing coronal loops - the arcs extending off of the Sun where plasma moves along magnetic field lines. The brightest spots seen here are locations where the magnetic field near the surface is exceptionally strong.
Esperanto: Pasado de Venuso vidita en la ondolongo 171, bildigita de Solar Dynamics Observatory. Tiu ĉi kanalo estas speciale taŭga por vidi koronajn maŝojn - la arkojn etenditajn de Suno kie plasmo moviĝas laŭ magnetaj fortolinioj. La plej malhelaj makuloj ĉi tie estas lokoj kie estas surfaca magneta kampo ekstreme forta.
Date
Source YouTube: NASA SDO - The Venus Transit – View/save archived versions on archive.org and archive.today
Author NASA/Solar Dynamics Observatory

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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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Date/TimeThumbnailDimensionsUserComment
current10:20, 6 June 201238 s, 1,280 × 720 (9.06 MB)Huntster (talk | contribs)== {{int:filedesc}} == {{Information |Description={{en|1=The 2012 Venus transit as seen in the 171 wavelength, imaged by the {{w|Solar Dynamics Observatory}}. This channel is especially good at showing coronal loops - the arcs extending off of the Sun ...

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VP9 720P 1.46 Mbps Completed 16:23, 26 June 2024 3 min 41 s
VP9 480P 733 kbps Completed 03:19, 28 June 2024 1 min 10 s
VP9 360P 324 kbps Completed 03:17, 28 June 2024 28 s
VP9 240P 142 kbps Completed 03:16, 28 June 2024 21 s
WebM 360P 242 kbps Completed 03:18, 28 June 2024 12 s
QuickTime 144p (MJPEG) Not ready Unknown status

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