In Polar Co-ordinates¶
\begin{aligned} \frac{\partial\psi^{\mathrm{R}}}{\partial x} &= C_0\frac{\sqrt{f}}{f’}\cdot \left( \cos\theta\cdot\sinh^{-1}\left(\frac{f’}{f}\cdot(\cos\phi\cos\theta+\sin\phi\sin\theta)\right) -\sin\theta\cdot\sin^{-1}\left(f’\cdot(-\cos\phi\sin\theta+\sin\phi\cos\theta)\right) \right) \\\\ \frac{\partial\psi^{\mathrm{R}}}{\partial y} &= C_0\frac{\sqrt{f}}{f’}\cdot \left( \sin\theta\cdot\sinh^{-1}\left(\frac{f’}{f}\cdot(\cos\phi\cos\theta+\sin\phi\sin\theta)\right) +\cos\theta\cdot\sin^{-1}\left(f’\cdot(-\cos\phi\sin\theta+\sin\phi\cos\theta)\right) \right) \end{aligned}
Since these expression are constant in , we can write \begin{aligned} \frac{\partial f}{\partial x} &= - \big(\frac{\sin\phi}{R}\big)\frac{\partial f}{\partial\phi} \\\\ \frac{\partial f}{\partial y} &= \big(\frac{\cos\phi}{R}\big)\frac{\partial f}{\partial\phi} \end{aligned} where .
Amplitudes for arbitrary orientation¶
The deflection is given as the vector , in a Cartesian co-ordinate system with axes aligned with the axes of the lens. We call this the lens frame. We are interested in the deflection vector in a global frame, which shares the origin with the lens frame, but is rotated clockwise by an angle . In other words, the lens is oriented at an angle (counterclockwise) in the global frame.
We will let denote the point in the global frame, and the same point in the lens frame. Hence \begin{aligned}
&=
\cdot
\end{aligned} In other words, the coordinates are rotated clockwise. Similarly the deflection is given as in the lens frame, and in the global frame. Thus, has to be rotated counterclockwise, as \begin{aligned} \vec{\alpha}(x,y) &=
\cdot \nabla\psi^{\mathrm{R}}(x’,y’) \end{aligned} This gives \begin{aligned} \vec{\alpha}(x,y) = C_0\frac{\sqrt{f}}{f’}\cdot
\end{aligned}