File:SDO Venus Transit 2012.ogv

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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.
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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 667 kbps Completed 09:16, 18 October 2018 1 min 2 s
Streaming 720p (VP9) Not ready Unknown status
VP9 480P 316 kbps Completed 09:16, 18 October 2018 45 s
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VP9 360P 171 kbps Completed 09:16, 18 October 2018 27 s
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VP9 240P 97 kbps Completed 09:16, 18 October 2018 21 s
Streaming 240p (VP9) 98 kbps Completed 04:27, 6 December 2023 1.0 s
WebM 360P 507 kbps Completed 16:57, 13 November 2012 50 s
Streaming 144p (MJPEG) 1.05 Mbps Completed 15:46, 15 November 2023 3.0 s

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