In this paper we present the scope of the Galactic Emission Mapping (GEM) project and its results at 2.3 GHz. Its observational program was conceived and developed to reveal the large scale properties of Galactic synchrotron radiation in total intensity and polarisation through a self-consistent set of radio continuum surveys between 408 MHz and 10 GHz. GEM's unique observational strategy and experimental design aim at the production of foreground templates in order to address the mutual inconsistencies between existing surveys and the role of Galactic emission as the main source of astrophysical contamination in measurements of the Cosmic Microwave Background radiation. The GEM experiment uses a portable and double-shielded 5.5-m radiotelescope on a rotating platform to map 60 deg wide declination bands, from different observational sites, by circularly scanning the sky at 30 deg from the Zenith. The observations at 2.3 GHz were accomplished with a total power receiver, whose front-end HEMT was matched directly to a cylindrical horn at the prime focus of a parabolic reflector. The Moon was used to calibrate the antenna temperature scale and the preparation of the map required direct subtraction and destriping algorithms to remove ground contamination as the most significant source of systematic error. For this first GEM survey, 484 hours of observations were used from two locations in Colombia and Brazil to yield a 69% sky coverage from DEC = -53 deg to DEC = +35 deg with a horizontal HPBW of 2.3 deg and a vertical HPBW 1.85 deg. The pointing accuracy was 8.6 arcmin and the RMS sensitivity was $9.8 +/- 1.6 mK. The zero-level uncertainty is 103 mK with a temperature scale error of 5% after direct correlation with the Rhodes/HartRAO survey at 2326 MHz on a T-T plot.