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THE PULSATING PULSAR MAGNETOSPHERE

  • Authors: K. H. Tsui

2015 The Astrophysical Journal 805 106.

  • Provider: AAS Journals

Caption: Figure 2.

With ﹩{{\kappa }^{2}}=5﹩ corresponding to ﹩a_{L}^{2}=8﹩ and ﹩{{m}^{2}}=3﹩, the axial function ﹩{{Z}_{a}}(\varsigma )﹩ with exponentially decaying profile is plotted as a function of the normalized axial distance ς.

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