  As an observer from within the Milky Way, it is difficult to determine its
global structure. Despite extensive observational data from surveys at
different wavelengths, we have no conclusive description of the structure of
our own Galaxy. For very-high-energy (VHE) $\gamma$ rays, the most
comprehensive catalogue of Galactic sources resulting from the H.E.S.S.
Galactic Plane Survey (HGPS) shows a striking asymmetry in the distribution of
the sources in the latitudinal direction. This could be the result of a local
feature in the spatial distribution of the sources or it could be due to the
position of the Sun above the Galactic plane. In this contribution, we estimate
the position of the Sun based on the latitudinal flux profile of VHE
$\gamma$-ray sources, assuming three mirror-symmetric models for the spatial
distribution of the sources in three-dimensional space and taking into account
the observational bias of the HGPS. We verify our method using simulations and
find values for $z_{\odot}$ between $-6\,\mathrm{pc}$ and $94\,\mathrm{pc}$
depending on the considered model. Our results show that the position of the
Sun has a significant impact on the observed source distribution and must
therefore be taken into account when modelling the population of Galactic VHE
$\gamma$ sources. However, it is not conclusive whether the Sun's offset from
the Galactic plane is the only factor leading to the asymmetry in the
latitudinal profile.
