File:420px-Magnetic-rope.png

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420px-Magnetic-rope.png(420 × 600 pixels, file size: 27 KB, MIME type: image/png)

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Summary[edit]

The self-constricting magnetic field lines and current paths in a Birkeland current (or magnetic rope). The current is strongest at the axis and becomes weaker further away. Currents flow parallel to the magnetic field, and derives partly from an external axial field and partly from the toroidal field produced by the current itself.

Image credit: http://history.nasa.gov/SP-345/ch15.htm#250 (and arrows coloured by myself)

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Licensing[edit]

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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Original upload log[edit]

Date/Time Dimensions User Comment
1 November 2005, 02:31:45 420 × 600 (23359 bytes) Perpetual (talk · contribs) The self-constricting magnetic field lines and current paths in a Birkeland current (or magnetic rope). The current is strongest at the axis and becomes weaker further away. Currents flow parallel to the magnetic field, and derives partly from an external

File history

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Date/TimeThumbnailDimensionsUserComment
current17:06, 23 July 2014Thumbnail for version as of 17:06, 23 July 2014420 × 600 (27 KB)GifTagger (talk | contribs)Bot: Converting file to superior PNG file. (Source: 420px-Magnetic-rope.gif). This GIF was problematic due to non-greyscale color table.

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