  We report the first high resolution, detailed abundances of 21 elements for
giants in the Galactic bulge/bar within $1^\circ$ of the Galactic plane, where
high extinction has rendered such studies challenging. Our high S/N and
high-resolution, near-infrared spectra of 7 M giants in the inner-bulge,
located at ($l,b$)=(0,+1$^{\circ}$), are observed using the IGRINS
spectrograph. We report the first multi-chemical study of the inner Galactic
bulge, by investigating relative to a robust new Solar Neighborhood sample, the
abundance trends of 21 elements, including the relatively difficult to study
heavy elements. The elements studied are: F, Mg, Si, S, Ca, Na, Al, K, Sc, Ti,
V, Cr, Mn, Co, Ni, Cu, Zn, Y, Ce, Nd, and Yb. We investigate bulge membership
of all seven stars using distances and orbital simulations, and find that the
most metal-poor star may be a halo interloper. Our investigation shows that the
inner-bulge also as close as $1^\circ$ North of the Galactic Center displays a
similarity to the inner disk sequence, following the high [$\alpha$/Fe]
envelope of the Solar vicinity metal-rich population, though no firm
conclusions for a different enrichment history are evident from this sample. We
find a small fraction of metal-poor stars (\feh$<-0.5$) but most of our stars
are mainly of super-solar metallicity. Fluorine is found to be enhanced at high
metallicity compared to the solar neighbourhood, but confirmation with a larger
sample is required. We will apply this approach to explore populations of the
Nuclear Stellar Disk and the Nuclear Star Cluster.
