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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 4.

The location of the outer caustic βouter vs. the maximum gradient of the lens potential ﹩{\psi ^{\prime} }_{{\rm{\max }}}﹩. The approximate equivalence of the two quantities indicates that a measurement of βouter can probe the sharpness of the corresponding IISM structure. Shown are Gaussian (green crosses) and top-hat (blue stars) models with amplitudes A = 10, 102, …, 106 from left to right, respectively. The point mass model also obeys this relation since it has a diverging ﹩{\psi ^{\prime} }_{{\rm{\max }}}﹩ at its center and thus no finite βouter.

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