In the exercise we are given that the spectrum of a light source consists of two spectral lines, which both have wavelengths around $500 \text{ nm}$ and the separation between them - given in wavenumbers - is close to $0.1 \text{ cm}^{-1}$.
One part asks us to calculate the distance between the mirrors if we want the free spectral range of our Fabry-Perot etalon to satisfy $FSR(\text{in } \overline \nu) = 2.5(\overline \nu_2 - \overline \nu_1)$.
Now, I know that the free spectral range ($\theta = 0$, $n_{air} \approx 1$) is given by
$$FSR = \frac{c}{2d}$$
where $d$ is the distance between the mirrors and we have
$$\Delta\overline \nu = \frac{c}{\lambda_2} - \frac{c}{\lambda_1} = \frac{c}{2\pi}\Delta k $$
So shouldn't then
$$d = \frac{c}{2 FSR} = \frac{c}{2 \cdot 2.5c/(2\pi) \Delta k} = \frac{\pi}{2.5\Delta k} \approx 12.566 \text{ cm}$$
According to the solution this is wrong: They get $FSR = 0.25 \text{ cm}^{-1}$ and $d = \frac{1}{2 \cdot FSR} = 20 \text{ mm}$
I seem to be missing something. If they calculate the free spectral range in terms of the wavenumber, shouldn't they convert it to frequency by
$$FSR(k) \to FSR(\nu) = \frac{c}{2\pi} FSR(k)$$
instead of
$$FSR(k) \to FSR(\nu) = c \cdot FSR(k)$$
Does anybody see what's going on here (maybe the solution is simply wrong, but I'd like to know for sure)?