FIRB 2010: Il paesaggio di una grande strada romana
FIRB 2010: Il paesaggio di una grande strada romana
The Via Appia archaeological site is affected by an elevated hydrogeological risk due to active rockfall processes from the carbonate slopes flanking the route track, which are particularly evident south of the St. Andrea stronghold, towards Itri (Fig.1). More than 80 rock blocks were documented on the route, with a volume ranging from 0.5 to 1.5 m³ (Figs.2a,b). Structural analysis of the rock scarps evidenced potential unstable rock wedges of about 3.3. m³.
Gravity-driven processes causing instability have been simulated by a stochastic model and using software Rotomap® and RotoMap GIs®. Initial motion condition (free-fall phase) were constrained to the geomorphological characteristics of rock scarps (elevation, length etc). Motion along rock slope was modelled by adopting literature values for dynamic parameters such as normal and tangential restitution coefficients (Kn and Kt) and friction angle (Φd) which control the rebound and roto-translation phases, respectively. Calibration of dynamic parameters was set with a back-analysis procedure on modelling results and considering constraints from fallen rock blocks inventory.
Simulations consider falling of a dimensionless rock blocks. For blocks detaching from 4,6 and 10 meters-high rock scarps, modelling result showed: the probabilistic distribution of possible trajectories; arrest points of rock blocks; the specific kinetic energies distribution (Fig.4a); the bouncing heights distribution (Fig.4b).
Finally, different design blocks were inferred and an hazard mitigation plane was defined which provides for placement and dimensioning of elastic barriers (Fig.5) capable to absorb impact energies between 2000 and 3000 KJ (considering design blocks of 1.56 and 3.32 m³, respectively).