  We present results of a decade of X-ray observations of the gamma-ray loud
binary HESS J0632+057, and interpret the available broadband data in view of
the system geometry and emission mechanisms. We have performed an analysis of
all X-ray data available to date from Swift, XMM-Newton, Chandra, NuSTAR and
Suzaku. We refine the orbital period of the system to be
$316.8^{+2.6}_{-1.4}$~d (95% c.l.), consistent with previous studies but
measured with significantly better accuracy. We report on a hydrogen column
density and spectral slope variation along the orbit. We argue that the
observed variability can be explained within an "inclined disk" model in which
the orbit of the compact object is inclined to the disk of the Be star. We show
that the observed X-ray to TeV emission can originate from a broken cut-off
power-law population of electrons and describe a way in which future X-ray/TeV
observations can distinguish between the proposed model and the alternative
flip-flop emission scenario of this system.
