Uplifts, with elevations of up to 2000 m and short wavelengths (30-35
km), flank three major grabens in central Greece: the Rio, Sparta, and
Atalanti grabens. They are bordered on their landward sides by narrow
basins oriented parallel to the graben axes: the Manesi and Trichonis
basins at the Rio graben and Copais and Istiea basins at the Atalanti
graben. The flexural origin of these uplift profiles is investigated
here by using thin, broken plate models. It is demonstrated that the o
bserved topography of the graben flanks is consistent with the upward
deflection of elastic and viscoelastic plates in response to upward di
rected forces applied at the graben flanks. In order to evaluate to ap
plicability of each model, their predictions are checked against the o
bservations. The elastic predictive modeling fits well with the observ
ed flexural wavelengths and the flanking seismicity. However, it fails
to predict the graben widths and the inferred elastic layer thickness
. In contrast, the viscoelastic model successfully explains the graben
widths and the ''back'' basins as flexural hinterland basins and matc
hes the seismological data and the time constraints of rifting. It is
therefore suggested that flexural uplift with viscoelastic relaxation
accounts, for the building of the graben flanks. The invoked viscoelas
tic models constrain the effective elastic thickness of the plates at
10 km for the Rio graben and 15 km for the Sparta and Atalanti grabens
, suggesting a low-viscosity lower crust. Furthermore, they predict lo
w rates of tectonic uplift of the order of 0.1 mm a(-1) for the Atalan
ti graben, intermediate rates of 0.24-0.37 mm a(-1) for the Rio graben
, and high rates of 0.7-0.9 mm a(-1) for the Sparta graben. The latter
are quite possibly overestimated since napping events, capable of pro
ducing high local relief, are traced normal to the modeled profiles.