  The advent of the new class 8 meters telescopes allows for the first time the
detailed study of numerous stars of galaxies other than our own. The Large
Magellanic Cloud is one of the most interesting targets due to its proximity
and its relatively face-on disk, permitting to separate populations pertaining
to the different structures of the galaxy. We have used FLAMES (the Fibre Large
Array Multi Element Spectrograph) at the VLT-UT2 telescope to obtain spectra of
a large sample of stars from the Inner Disk of the LMC, $\sim$2 kpc from the
center of the galaxy. We investigate the chemical abundances of iron-peak
elements, heavy and light $s$-process elements, Cu, Na, Sc and
$\alpha$-elements for a sample of red giant stars. Metallicities for the sample
stars range from [Fe/H] = $-$1.76 to $-$0.02. LMC inner disk stars show a
definitely different chemical pattern when compared to galactic stars of the
same metallicity.
