948 research outputs found
Tectonic escape of Sicily micro plate in the framework of the Tyrrhenian-Apennine system evolution.
The opening of the Tyrrhenian basin and the contemporary formation of the Apennine chain are
described through the application of techniques of deformable plate kinematics and modeled with
several dedicated software (Chapter 1). These methods have proven to be suitable to describe
complex tectonic processes, such as those observed along the Africa–Europe collision belt,
characterized by passive subduction processes. These results from the subduction of the residual
Alpine Tethys and the Ionian lithosphere, and from the fragmentation of the Adriatic plate.
As a first step, described in Chapter 2, the area of the Apennine Chain and of the Tyrrhenian basin
have been divided into deformable polygons through a careful observation of the regional
structures. The polygons are distinguished on the basis of sets of extensional structures that are
coherent with unique Euler pole grids. The boundaries between these polygons coincide with large
tectonic lineaments that characterize the Tyrrhenian–Apennine area. The tectonic style along
these structures reflects the variability of relative velocity vectors between two adjacent blocks.
The deformation of tectonic elements is accomplished, allowing different rotation velocities of
lines that compose these blocks about the same stable stage poles. The angular velocities of
extension are determined on the basis of the stratigraphic records of syn-rift sequences, while the
finite rotation angles are obtained by crustal balancing. From north to south, the polygons are: (1)
Northern Apennine; (2) Umbria–Marche Apennine Arc; (3) Southern Apennine; (4) Calabrian Arc;
(5) Sicilian Chain.
Then, to understand the geodynamic processes that guided the opening of Tyrrhenian back-arc
basin, the geometry of the Adriatic-Ionian slab has been reconstructed and presented in Chapter
3. The slab is constituted by Liguride and Ionian oceans and by the Apulian-Adriatic continental
margin. It is segmented by STEP faults, propagated along the COB of the Liguride and Ionian
oceans and along the fracture zones of the Apulian-Adriatic margin, formed during the Triassic-
Jurassic rifting. The continental lithosphere begins to subduct starting from the North and
proceeds to the South with time intervals determined by the articulation of the Adriatic COB line.
To the South, where the continental lithosphere is absent or scarce, the slab segments keep
sinking into the upper mantle; on the contrary, the northernmost segments progressively decrease
their sinking with the incoming of continental lithosphere into the subduction zone, until the
buoyancy equilibrium is reached. A strong relationship between upper plate evolution and
asynchronous subduction has been considered in the proposed kinematic model.
Chapter 4 is dedicated to the specific aim of this PhD thesis: reconstruct the kinematic evolution
of Sicily, considered as an independent plate starting from 4.5 Ma ago, and its role in the
framework of the Tyrrhenian-Apennine System. Sicily is involved in a process of escape towards
east-southeast induced by the African plate acting as an intender pushing toward north, during its
convergence with the European plate, and by the Malta escarpment STEP fault, due to the retreat
of the African-Ionian slab that created space toward east.
The plates and microplates that I consider involved during the evolution of the last 4.5 Ma are
Europe, Africa, Calabria and Tunisia. This last microplate is strictly related to the evolution of Sicily.
The boundaries of the Sicily and Tunisia microplates are lithospheric structures known from the
literature and identifiable from geological and geophysical datasets: high resolution bathymetric
maps, seismic sections, geodetic data, focal mechanism of recent earthquakes, gravimetric maps,
Moho depth maps and so on.
The margin between Sicily and Europe is along the Drepano-Elimi chain (Ustica ridge), a E-W
trending morpho-structure with a general transpressive kinematics; the margin with the Calabrian
microplate is along the right-lateral Taormina line first and then along the ‘‘Aeolian-Tindari-
Letojanni” line; the margin with Africa is expressed along part of the Malta Escarpment and along
the Sicily Channel, where a series of troughs (Pantelleria, Linosa and Malta) were interpreted in
literature as rift basins or as pull-apart basins related to a dextral shear zone. The margins of
Tunisia instead follow the N-S and NE-SW structures that characterize the Central Atlas.
Several attempts have been tried to obtain the Euler pole of rotation between Sicily and Africa,
starting from the structures in the Sicily Channel and using the GPlates software. Then, also Sicily-
Europe, Sicily-Calabria and Sicily-Tunisia poles and the respective velocity vectors have been
derived and compared with the geological data.
Finally, the proposed kinematic model of the Tyrrhenian-Apennine system, including Sicily and
Tunisia, is shown in Appendix 1 and Movie 1, and described in 5 phases in Chapter 5. Briefly,
during the first phase (19–12 Ma), an extension strip divided the proto-Apennine chain from
Sardinia while a northern Apennine arc and a central Apennine arc were separated from an
extensional area, in transverse direction, covered by top-wedge sediments. The Calabrian arc was
divided in north Calabria and south Calabria–Peloritani mounts, separated by the Catanzaro
Trough. The second phase (12–7 Ma) is marked by the separation of the Western Sicily chain from
the Calabrian arc and the beginning of extension in the Caltanissetta basin; this, is still active in
phase 3, for the whole Messinian age. Phase 3 (7–4.5 Ma) was characterized by the formation of
the Vavilov basin, which records major changes in the Ionian slab-retreat process. A new nascent
sector, the Southern Apennine Sector, including the Lazio–Abruzzi platform, was separated from
the Apennine Arc by the Ancona–Anzio Line and rotated around a very close pole, located at the
northern tip of the Vavilov Basin. During phase 4 (4.5-2.5 Ma) Sicily and Tunisia start to rotate
around their poles: Tunisia is pushed upward while Sicily starts a clockwise rotation that produces
extension in the northernmost part of the Sicily Channel. At this time the Taormina line is active as
the boundary between Sicily and Calabria. At the beginning of the last phase (2.5-0 Ma) extension
jumped eastwards of the Vavilov basin and the southern branch of the triple junction of the
Southern Tyrrhenian rifts started to form the Marsili basin. A dextral shear zone is active in the
Sicily channel and the movement between Sicily and Calabria jumps from the Taormina line to the
‘‘Aeolian-Tindari-Letojanni” line. At the end of this phase the Ionian STEP fault intersected the
Malta Escarpment and the tear fault began to propagate along this structure
The Unstoppable Intrusion: The Unique Effect of Online Harassment and What the United States Can Ascertain from Other Countries\u27 Attempts to Prevent It
The United States must provide some solution to deal with online harassment. Looking at its fellow nations may be a good way to provide a foundation for changes that need to be mad
The Unstoppable Intrusion: The Unique Effect of Online Harassment and What the United States Can Ascertain from Other Countries\u27 Attempts to Prevent It
The United States must provide some solution to deal with online harassment. Looking at its fellow nations may be a good way to provide a foundation for changes that need to be mad
Line ratios and temperature structure in the deep photosphere
A program to monitor solar cycle variations of the solar flux by using suitable spectral line ratios is going on at Kitt Peak since 1976;the most sensitive to Teff variations are the ratios involving the C I 538.032 nm, whose formation
depth is almost coincident with that of the continuum, and either the Fe I 537.958 or the Ti II 538.103. The temperature sensitivities of those line ratios have been
empirically calibrated by observing the spectra of several solar-like stars by Gray and Livingston, while several attempts to obtain the same calibration theoretically,
through Kurucz’s models of stellar atmospheres, showed difficulty in reproducing quantitatively the experimental results. Because the observed/computed ratio was
approximately the same for both couples of lines, we argued that the problem was in the behaviour of C line, that is more affected than the others by the temperature structure of the deep photosphere, where it is formed. As, in these layers, the gradients of the average temperature are sensibly affected by different treatments of the convection, we compared, first of all, several theoretical models, distinguished from each other in including or not convective overshooting. Then we explored the effects due to variations of the value of the free parameter (α =�/HP ) and those ensued by different versions of the mixing-length theory
SAW RFID-Tags for Mass-Sensitive Detection of Humidity and Vapors
One-port surface acoustic wave (SAW) devices with defined reflector patterns give characteristic signal patterns in the time domain making them identifiable and leading to so-called RFID-Tags. Each sensor responds with a burst of signals, their timed positions giving the identification code, while the amplitudes can be related to the analyte concentration. This paper presents the first combination of such a transducer with chemically sensitive layer materials. These include crosslinked polyvinyl alcohol for determining relative humidity and tert-butylcalix[4]arene for detecting solvent vapors coated on the free space between the reflectors. In going from the time domain to the frequency domain by Fourier transformation, changes in frequency and phase lead to sensor responses. Hence, it is possible to measure the concentration of tetrachloroethene in air down to 50 ppm, as well as 1% changes in relative humidity
Development of a surgical stereo endoscopic image dataset for validating 3D stereo reconstruction algorithms
In the last decades, endoscopic stereo images have been exploited to retrieve tissue surface information of the surgical site using 3D reconstruction algorithms. The application of such algorithms in Computer Assisted Surgery (CAS) tools for Minimally Invasive Surgery (MIS) requires a robust validation process in order to guarantee reliability and safety. 3D reconstruction algorithms are commonly evaluated comparing their result with respect to a reference Ground Truth (GT). However, few datasets providing endoscopic images and GT are openly available.
Considering the increasing necessity of surgical datasets, the aim of this work is the generation of an Endoscopic Abdominal Stereo (EndoAbS) dataset composed of stereo-images with associated GT for 3D stereo-reconstruction algorithm validation. To recreate the surgical scenario, a polyurethane surgical phantom abdomen was built. Images were captured with a stereo-endoscope, while for acquiring the GT a laser scanner (calibrated with respect to the stereoendoscope) was used. This dataset is openly available on-line for the benefit of the CAS community
The correlation of synthetic UV color vs Mg II index along the solar cycle
Modeling of planets' climate and habitability requires as fundamental input
the UV emission of the hosting star. \citet{lovric2017} employed SORCE/SOLSTICE
solar observations to introduce a UV color index which is a descriptor of the
UV radiation that modulates the photochemistry of planets atmospheres. After
correcting the SOLSTICE data for residual instrumental effects that produced
asymmetric signals during different phases of the cycles analyzed, the authors
found that the UV color index is linearly correlated with the Mg II index.In
this paper we employ an irradiance reconstruction technique to synthetize the
UV color and Mg II index with the purpose of investigating whether the
correction applied by \citet{lovric2017} to SORCE/SOLSTICE data might have
compensated for solar variations, and to investigate the physical mechanisms
that produce such a strong correlation between the UV color index and the solar
activity. Reconstructed indices reproduce very well the observations and
present the same strong linear dependence. Moreover our reconstruction, which
extends back to 1989, shows that the UV color - Mg II index relation can be
described by the same linear relation for almost three cycles, thus ruling out
an overcompensation of SORCE/SOLTICE data in the analysis of
\citet{lovric2017}. We suggest that the strong correlation between the indices
results from the fact that most of the Far- and Middle- UV radiation originates
in the chromosphere, where atmosphere models of quiet and magnetic features
present similar temperature and density gradients.Comment: Accepted in Ap
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