I am trying to find the inverse of the metric
$$\mathrm ds^2 = \rho^2~\mathrm d\theta^2 -2a\sin^2\theta ~\mathrm dr~d\varphi + 2~\mathrm dr~\mathrm du + \rho^{-2}\left[\left(r^2+a^2\right)^2 -\Delta a^2\sin^2\theta\right]\sin^2\theta~\mathrm d\varphi^2-2a\rho^{-2}\left(2mr-e^2\right)\sin^2\theta~\mathrm d\varphi~\mathrm du-\left[1-\rho^{-2}\left(2mr-e^2\right)\right]~\mathrm du^2 $$
The inverse was given in Global Structure of the Kerr Family of Gravitational Fields as
$$(\partial/\partial s)^2 = \rho^{-2}(\partial/\partial\theta)^2+ 2\rho^{-2}\left(r^2+ a^2\right)(\partial/\partial r)(\partial/\partial u)+ 2\rho^{-2}a(\partial/\partial r)(\partial/\partial\varphi)+ 2\rho^{-2}a(\partial/\partial u)(\partial/\partial \varphi)+ \rho^{-2}\sin^2\theta(\partial/\partial u)^2 + \rho^{-2}\sin^2\theta(\partial/\partial \varphi)^2+ \rho^{-2}\Delta(\partial/\partial r)^2$$
I know how to find the inverse of the metric $g_{\mu\nu}$ but they seem to give different components to the components presented in the inverse metric. Does anyone know what method was used to find the inverse?