Unlike the Standard Model (SM), supersymmetric models stabilize the
electroweak (EW) scale v at the quantum level and {\it predict} that v is a
function of the TeV-valued SUSY parameters (γα) of the UV
Lagrangian. We show that the (inverse of the) covariance matrix of the model in
the basis of these parameters and the usual deviation δχ2 (from
χmin2 of a model) automatically encode information about the
"traditional" EW fine-tuning measuring this stability, {\it provided that} the
EW scale v∼mZ is indeed regarded as a function v=v(γ). It is
known that large EW fine-tuning may signal an incomplete theory of soft terms
and can be reduced when relations among γα exist (due to GUT
symmetries, etc). The global correlation coefficient of this matrix can help
one investigate if such relations are present. An upper bound on the usual EW
fine-tuning measure ("in quadrature") emerges from the analysis of the
δχ2 and the s-standard deviation confidence interval by using
v=v(γ) and the theoretical approximation (loop order) considered for the
calculation of the observables. This upper bound avoids subjective criteria for
the "acceptable" level of EW fine-tuning for which the model is still
"natural".Comment: 13 pages. LaTeX, (v4: minor corrections