  The measurement of large scale patterns or anisotropies in the arrival
direction of high energy cosmic rays is an important step towards the
understanding of their origin. Such measurements rely on an accurate estimation
of the detector relative exposure in each direction on the sky : the coverage
map. To reach an accuracy on the determination of this map below the one
percent level one must properly identify and correct for all the environmental
effects that may induce variations in the detector exposure as a function of
time. In an approach, similar to the one used in anti-sidereal time analysis,
we propose a method to empirically estimate and correct for those effects under
the hypothesis that seasonal and diurnal variations can be factorized. We
tested this method using a model ground detector of cosmic ray air showers,
whose aperture varies due to the dependence of the air shower development on
the atmospheric conditions.

Astrophysics