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Plasma Lensing Modeling of Substructures on Pulsar Scintillation Screens

  • Authors: Zhu Xu, Xun Shi

Zhu Xu and Xun Shi 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Scaled magnification ﹩{{\rm{log}}}_{10}(A\mu )﹩ as a function of normalized source position β/βouter for the dominant subimage in the Gaussian (h = 2) and top-hat (h = 8) models. Both models with various lens amplitudes A all exhibit similar functional shape well-described by a polynomial form of ﹩{{\rm{log}}}_{10}(A\mu )=58.25{(\beta /{\beta }_{{\rm{outer}}})}^{4}-182.64{(\beta /{\beta }_{{\rm{outer}}})}^{3}+231.48{(\beta /{\beta }_{{\rm{outer}}})}^{2}-151.79(\beta /{\beta }_{{\rm{outer}}})+55.77﹩ (gray dashed line) away from the caustics.

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