  We have developed techniques to extract true iron abundances and surface
gravities from spectra of the type provided by the multiple-object fibre-fed
spectroscopic radial-velocity surveys underway with 2dF, HYDRA, NESSIE, and the
forthcoming Sloan survey. Our method is optimised for low S/N, intermediate
resolution blue spectra of G stars. Spectroscopic indices sensitive to iron
abundance and gravity are defined from a set of narrow (few Angstrom)
wavelength intervals, and calibrated using synthetic spectra. We have also
defined a single abundance indicator which is able to provide useful iron
abundance information from spectra having S/N ratios as low as 10 per Angstrom.
The theoretical basis and calibration using synthetic spectra are described in
this paper. The empirical calibration of these techniques by application to
observational data is described in Jones, Wyse and Gilmore (PASP July 1995).
The technique provides precise iron abundances, with zero-point correct to
$\sim 0.1$ dex, and is reliable, with typical uncertainties being $\approxle
0.2$ dex. A derivation of the {\it in situ\/} thick disk metallicity
distribution using these techniques is presented by Gilmore, Wyse and Jones (AJ
1995 v109 p1095).
