 Fourier-Hankel normalization for an isotropic spectrum

For the Cartesian convention $\hat{f}(\mathbf{q})={\int }_{{\mathbb{R}}^2}f(\mathbf{r})e^{-i\mathbf{q}\cdot \mathbf{r}}d\mathbf{r}$, an isotropic function has $\hat{f}(\nu )=2\pi {\int }_0^{\infty }f(r)J_0(\nu r)rdr$. Its inverse is $f(r)=(2\pi {)}^{-1}{\int }_0^{\infty }\hat{f}(\nu )J_0(\nu r)\nu d\nu$. The self-reciprocal Hankel transform instead uses $F_H=\hat{f}/(2\pi )$. In particular $f(0)=\int F_H(\nu )\nu d\nu$. Mixing these spectral conventions changes attenuation coefficients by $2\pi$.