  We report on results of two years of INTEGRAL/SPI monitoring of the Galactic
microquasar GRS 1915+105. From September 2004 to May 2006, the source has been
observed twenty times with long (approx 100 ks) exposures. We present an
analysis of the SPI data and focus on the description of the high-energy (> 20
keV) output of the source. We found that the 20 - 500 keV spectral emission of
GRS 1915+105 was bound between two states. It seems that these high-energy
states are not correlated with the temporal behavior of the source, suggesting
that there is no direct link between the macroscopic characteristics of the
coronal plasma and the the variability of the accretion flow. All spectra are
well fitted by a thermal comptonization component plus an extra high-energy
powerlaw. This confirms the presence of thermal and non-thermal electrons
around the black hole.
