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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[edit]DescriptionSolar Dynamo Toroidal Poloidal Magnetic Fields.ogv |
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 |
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[edit]Public domainPublic domainfalsefalse |
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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current | 14:40, 11 March 2010 | 59 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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