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Critical Curves for The SIE Lens

The SIE lens is defined by the convergence

κ(ξ1,ξ2)=fξ02ξ12+f2ξ22,\kappa(\xi_1,\xi_2)=\frac{\sqrt{f}\xi_0}{2\sqrt{\xi_1^2+f^2\xi_2^2}},

where ff is the ratio between the minor and major axes.

According to Kormann 1994 (TODO Check specific paper) the magnification matrix for SIE now becomes

A(θ)=[12κsin2ϕκsin(2ϕ)κsin(2ϕ)12κcos2ϕ]\mathcal{A}(\boldsymbol{\theta}) = \begin{bmatrix} 1 - 2\kappa\sin^2\phi & \kappa\sin(2\phi) \\\\\\\\ \kappa\sin(2\phi) & 1 - 2\kappa\cos^2\phi & \end{bmatrix}

where (ξ,ϕ)(\xi,\phi) are the polar coordinates of the normalised screen space point x\mathbf{x}. Now the critical curve is given as the points (ξcrit,ϕ)(\xi_{\mathrm{crit}},\phi) given as

ξcrit=fξ0cos2ϕ+f2sin2ϕ,\xi_{\mathrm{crit}} = \frac{\sqrt{f}\xi_0}{\sqrt{\cos^2\phi+f^2\sin^2\phi}},