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THE PULSATING PULSAR MAGNETOSPHERE

  • Authors: K. H. Tsui

2015 The Astrophysical Journal 805 106.

  • Provider: AAS Journals

Caption: Figure 9.

A set of poloidal flux functions ﹩{\Psi }(\xi ,\varsigma )﹩ for the equatorial region ion closed field lines is illustrated with contour values ﹩C=0.03,\;0.04,\;0.05﹩ with the same ordering. These field lines extend to an intermediate range of ξ to ensure ﹩{{B}_{z}}\lt 0﹩ as required by the space-charge density.

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