Image:Bennett Pinch graph.png
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[edit] Summary
The Bennett Pinch showing the total current (I) versus the number of particle per unit length (N). The chart illustrates four physically distinct regions. The plasma temperature is 20 K, the mean particle mass 3×10-27 kg, and ΔWBz is the excess magnetic energy per unit length due to the axis magnetic field Bz. The plasma is assumed to be non-rotational, and the kinetic pressure at the edges is much smaller than inside.
Redrawn by Ian Tresman after Carlqvist, Per, "Cosmic electric currents and the generalized Bennett relation" (1988) Astrophysics and Space Science (ISSN 0004-640X), vol. 144, no. 1-2, May 1988, p. 73-84
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15:51:50, 1 June 2006 . . Iantresman (Talk | Contribs) . . 1053x878 (78,496 bytes) (The [[Bennett Pinch]] showing the total current (I) versus the number of particle per unit length (N). The chart illustrates four physically distinct regions. The plasma temperature is 20 K, the mean particle density 3x10<sup>-27</sup>kg, and ΔW<sub>Bz</)
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- (del) (cur) 05:37, 15 February 2007 . . PNG crusade bot (Talk | contribs) . . 1053×878 (47,682 bytes) (__NOTOC__ == Summary == The Bennett Pinch showing the total current (I) versus the number of particle per unit length (N). The chart illustrates four physically distinct regions. The plasma temperature is 20 K, the mean particle mass 3×10<sup>-27</su)
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