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THE PULSATING PULSAR MAGNETOSPHERE

  • Authors: K. H. Tsui

2015 The Astrophysical Journal 805 106.

  • Provider: AAS Journals

Caption: Figure 7.

With ﹩{{a}_{0}}=1﹩ and ﹩{{a}_{1}}=-1.5﹩, and ﹩a_{\phi }^{2}=-17﹩ and ﹩a_{L}^{2}=7﹩, plus the condition  ﹩a_{z}^{2}=0﹩, the radial solution ﹩R(\xi )﹩ with a root within LC is plotted as a function of the normalized radial distance ξ.

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