File:Solar Dynamo Toroidal Poloidal Magnetic Fields.ogv

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Solar_Dynamo_Toroidal_Poloidal_Magnetic_Fields.ogv ‎(Ogg Theora video file, length 59 s, 400 × 226 pixels, 510 kbps, file size: 3.59 MB)

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Summary

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Description
English: This is the dynamo process, the net result being that part of the Sun's outflowing thermal convective energy from nuclear processes is used to create the magnetic field. In this visualization, the magnetic field lines (represented by the 'copper wire' structures) are 'snapshots' of the field structure constructed at each time step of the model.
Date
Source http://svs.gsfc.nasa.gov/vis/a000000/a003500/a003521/SolarDynamoFields_iPod.mov
Author NASA/Goddard Space Flight Center Scientific Visualization Studio

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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Date/TimeThumbnailDimensionsUserComment
current14:40, 11 March 201059 s, 400 × 226 (3.59 MB)Zetasurfer (talk | contribs){{Information |Description={{en|1=This is the dynamo process, the net result being that part of the Sun's outflowing thermal convective energy from nuclear processes is used to create the magnetic field. In this visualization, the magnetic field lines (re

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Format Bitrate Download Status Encode time
VP9 240P Not ready Unknown status
Streaming 240p (VP9) 264 kbps Completed 08:42, 16 December 2023 23 s
WebM 360P 255 kbps Completed 12:23, 2 December 2023 6.0 s
Streaming 144p (MJPEG) 1.02 Mbps Completed 12:30, 18 November 2023 2.0 s

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