  We perform an empirical synthesis of the blue integrated spectrum of the
metal-rich globular cluster 47 Tucanae, based directly on the color-magnitude
diagram of the cluster coupled to a moderately high-resolution spectral
library. Freed from any significant dependence on theory, we are able to
perform a fundamental test of the adequacy of the spectral library and its
associated stellar parameters. Excellent fits are achieved for almost all
absorption-line indices studied, provided the computations are corrected for
two limitations of the spectral library, namely, the lack of a representative
set of metal-poor giants and the absence of CN-strong stars. The latter effect
is corrected by means of spectrum synthesis from model photospheres,
considering the abundance pattern of CN-strong and CN-normal stars. We also
need to perform a slight correction of the metallicity of the cluster (by
--0.05 dex in relation to the standard value [Fe/H]=-0.7) in order to match the
metal-line index measurements in the cluster spectrum. After these relatively
small adjustments, the overall spectral agreement is good. Good fits are
achieved for Hbeta, Hgamma, Mgb, <Fe>, Ca4227 and Fe4383, and only Hdelta_F is
overpredicted. Thus, ages inferred from Hdelta_F are slightly older than the
ages based on the other Balmer lines, by ~ 3 Gyrs. The success of this exercise
suggests that previous failures to synthesize the spectrum of 47 Tuc must have
arisen from inadequacies in the theoretical evolutionary isochrones and/or
luminosity functions. Such a possibility is considered in a companion paper.
