Fig. 1. 3D view of the Timpa di San Lorenzo structure (center) with the Pollino range at the West (left). View from NE, Google Earth maps. |
One quite spectacular geological structure in Southern Italy that can be
visualized in 3D terrain browsers such as Google Earth is the Timpa di
San Lorenzo (TSL) carbonatic structure, outcropping at the border
between Basilicata and Calabria near San Lorenzo Bellizzi (Fig. 1).
If you play for instance with Google Earth, you would note a well
exposed, planar fault surface cutting through limestones in the
footwall. This fault is dissected by other faults, the main one
being a NW-SE high-angle fault. North of it the TSL fault has a WNW-ESE
trend, while to the South it is NNW-SSE (Fig. 2).
Fig. 2. Geological sketch representing the Timpa di San Lorenzo structure (center), subdivided into two segments by a NW-SE trending fault. The Mt. Pollino range is at the West (left). |
In Alberti (2019) the two main segments were analyzed with GIS tools,
namely the qgSurf plugin for QGIS, in order to derive the best-fitting
planes to the various fault segments.
For the northern segment the
geological plane fitting the traces has an attitude of 072°/39° (dip
direction/dip angle), i.e., a medium-angle fault dipping to the ENE.
In
the southern segment the best-fitting plane attitude is 082°/40°, i.e. a
10° trend rotation in a clockwise manner with respect to the northern
sector.
In order to help visualize these inferred geological
planes directly within geological profiles, I am adding in the pygsf
and gst Python modules a new GIS tool that uses line traces with attitudes,
intersect them with profiles and plot the intersected attitude in the
profiles. This tool is still in development.
To analyse the
geological situation for the studied zone, I used the two previous
geological attitudes in order to derive, using the ‘Plane-DEM
intersections’ tool of the QGIS qgSurf plugin, their expected
topographic traces. These line traces were clipped to the appropriate
spatial domain and then merged together into a single line shapefile.
Using pygsf, gst and spatdata modules in development mode within Jupyter Notebook, the Timpa di San Lorenzo data were imported from the spatdata module, maps with faults (both mapped and theoretical traces) and profiles traces were created (Fig. 3).
The final product is represented by the geological profiles (Fig. 4), always produced within Jupyter Notebook using the three mentioned modules. The produced profiles highlights the carbonatic structures, while the pelagic sediments and meta-sediments units are not mapped.
As you can see in the profiles, the theoretical planes approximate quite well the attitude of the outcropping TSL fault slickensides (profiles 1 to 8, with the exception of profile 3, where the TSL fault is masked by other units).
In the southern segment, the slickenside is visible mainly in profile 8 and also profile 9.Moving soutwards, both the fault slickenside and the footwall is more and more eroded, due to the deep incision of the Torrente Raganello (profiles 10-13).
The Jupyter Notebook document used to create these (and more) analyses is available here.
To replicate the analysis you
have to clone the gsf, gst and spatdata repositories, install the
modules (for instance in development mode) and then run the notebook.
References
Alberti M. 2019. GIS analysis of geological surfaces orientations: the qgSurf plugin for QGIS. PeerJ Preprints 7:e27694v1 https://doi.org/10.7287/peerj.preprints.27694v1
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