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THE PULSATING PULSAR MAGNETOSPHERE

  • Authors: K. H. Tsui

2015 The Astrophysical Journal 805 106.

  • Provider: AAS Journals

Caption: Figure 1.

With ﹩{{a}_{0}}=1﹩ and ﹩{{a}_{1}}=0﹩, and ﹩a_{\phi }^{2}=20﹩ and ﹩a_{L}^{2}=8﹩, the radial solution ﹩R(\xi )﹩ with monotonically increasing profile is plotted as a function of the normalized radial distance ξ.

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