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THE PULSATING PULSAR MAGNETOSPHERE

  • Authors: K. H. Tsui

2015 The Astrophysical Journal 805 106.

  • Provider: AAS Journals

Caption: Figure 8.

With ﹩{{\kappa }^{\prime 2}}=5﹩ (﹩{{\kappa }^{2}}=-5﹩) corresponding to ﹩a_{L}^{2}=7﹩ and ﹩{{m}^{2}}=12﹩, the axial function ﹩Z_{a}^{\prime }(\varsigma )﹩ with cosine profile is plotted as a function of the normalized axial distance ς.

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