  As the only eclipsing asynchronous polar, V1432 Aql provides an excellent
laboratory to study the interaction between the accreted matter and the
magnetic field. Here, we report an analysis of the X-ray data from the
contemporaneous \nustar\ and \xrt\ observations. The X-ray data present a
profile with a low-intensity state for almost half an orbital period, a dip at
0.6 phase, and a peak at 0.75 phase, which suggests that there was only one
accretion region during the observation and the claim is supported by the
spectral analysis. The comparison with the previous data indicates that the
X-ray data have an orbital modulation, as the case in \sax, rather than a spin
one observed in \rosat. We attribute the orbit and spin modulations to the
different accretion geometries at work. The spectral analysis of the wide-band
data presents a significant reflection effect, a commonly observed soft X-ray
temperature, and the energy balance in V1432 Aql . Additionally, we obtained a
low total accretion rate of 1.3 $\times$ 10$^{-10}$ M$_{\odot}$ yr$^{-1}$ and a
high specific accretion rate of 3.8 g cm$^{-2}$ s$^{-1}$ which explains the
strong reflection from the surface of the white dwarf. However, due to its
complex emission, a more physical understanding of its accretion geometry is
still outstanding.
