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  • 04.03. Geodesy  (2)
  • Polarized plate tectonics  (2)
  • 1
    Publication Date: 2019-03-26
    Description: Even if plate tectonics was a truly significant unifying theory that began to give sense to a series of different geological observations, plate motions were considered scattered. The advent of space geodesy confirmed and greatly refined the models of plate kinematics, allowing also to study the motion of the lithosphere with respect to the inner layers of the Earth. Switching from the no net rotation to the hotspot reference frames, plate motion assumes coherence with a mean global westward drift of the lithosphere with respect to the mantle. However, the driving forces of plate tectonics are still under investigation and space geodesy may provide fundamental tools to develop comprehensive models which can take into account the contributes of mantle density gradients and astronomical forces, as Earth’s rotation and tides. This paper is dedicated to Prof. Michele Caputo who was a pioneer in measuring the misalignment of the tidal bulge with respect to the Earth–Moon gravitational alignment. The misplaced mass in excess may account for the westerly directed torque of the lithosphere relative to the mantle. Local GPS networks and satellite observations are providing new insights on plate boundary tectonics and allow unravelling the evolution of the interplay between the shallow brittle upper crust and the underlying visco-plasticlower crust, which is deforming in a steady state regime without releasing relevant seismic waves. Along active tectonic areas, zones marked by low strain rates are suitable to store larger energy, subsequently dissipated during the coseismic stage. GPS and InSAR observations have widely increased the capability to monitor the spatial and temporal variations of deformation. The coseismic deformation pattern suggests a different mechanism of energy store and release, mainly gravitational in extensional tectonic settings and essentially elastic in strike-slip and contractional tectonic settings. The increasing details provided by future dense and low-cost geodetic networks will allow to detect reliable deformation transients and new insight on seismic precursors.
    Description: Published
    Description: 29-34
    Description: 1T. Struttura della Terra
    Description: JCR Journal
    Keywords: Space geodesy ; Plate motion ; Seismic cycle ; Strain rate ; 04.03. Geodesy
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 2
    Publication Date: 2019-12-13
    Description: We measured ground displacements before and after the 2009 L’Aquila earthquake using multitemporal InSAR techniques to identify seismic precursor signals. We estimated the ground deformation and its temporal evolution by exploiting a large dataset of SAR imagery that spans seventy-two months before and sixteen months after the mainshock. These satellite data show that up to 15 mm of subsidence occurred beginning three years before the mainshock. This deformation occurred within two Quaternary basins that are located close to the epicentral area and are filled with sediments hosting multi-layer aquifers. After the earthquake, the same basins experienced up to 12 mm of uplift over approximately nine months. Before the earthquake, the rocks at depth dilated, and fractures opened. Consequently, fluids migrated into the dilated volume, thereby lowering the groundwater table in the carbonate hydrostructures and in the hydrologically connected multi-layer aquifers within the basins. This process caused the elastic consolidation of the fine-grained sediments within the basins, resulting in the detected subsidence. After the earthquake, the fractures closed, and the deep fluids were squeezed out. The pre-seismic ground displacements were then recovered because the groundwater table rose and natural recharge of the shallow multi-layer aquifers occurred, which caused the observed uplift.
    Description: Published
    Description: 12035
    Description: 6T. Variazioni delle caratteristiche crostali e precursori
    Description: JCR Journal
    Keywords: InSAR ; earthquake ; L'Aquila ; precursor ; hydrogeology ; consolidation ; 04.04. Geology ; 04.03. Geodesy ; 04.07. Tectonophysics
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 3
    Publication Date: 2022-12-01
    Description: The processes occurring on the Earth are controlled by several gradients. The surface of the Planet is featured by complex geological patterns produced by both endogenous and exogenous phenomena. The lack of direct investigations still makes Earth interior poorly understood and prevents complete clarification of the mechanisms ruling geo- dynamics and tectonics. Nowadays, slab-pull is considered the force with the greatest impact on plate motions, but also ridge-push, trench suction and physico-chemical heterogeneities are thought to play an important role. However, several counterargu- ments suggest that these mechanisms are insufficient to explain plate tectonics. While large part of the scientific community agreed that either bottom-up or top-down driven mantle convection is the cause of lithospheric displacements, geodetic observations and geodynamic models also support an astronomical contribution to plate motions. Moreover, several evidences indicate that tectonic plates follow a mainstream and how the lithosphere has a roughly westerly drift with respect to the asthenospheric mantle. An even more wide-open debate rises for the occurrence of earthquakes, which should be framed within the different tectonic setting, which affects the spatial and temporal properties of seismicity. In extensional regions, the dominant source of energy is given by gravitational potential, whereas in strike-slip faults and thrusts, earthquakes mainly dissipate elastic potential energy indeed. In the present article, a review is given of the most significant results of the last years in the field of geodynamics and earthquake geology following the common thread of gradients, which ultimately shape our planet.
    Description: Published
    Description: 801–881
    Description: 1T. Struttura della Terra
    Description: JCR Journal
    Keywords: Earth’s gradients ; Forces driving plate motions ; Polarized plate tectonics ; Global scale geodynamics ; Earthquake geology ; The role of gradients in seismic dynamics
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 4
    Publication Date: 2023-06-05
    Description: Tidal forces are generally neglected in the discussion about the mechanisms driving plate tectonics despite a worldwide geodynamic asymmetry also observed at subduction and rift zones. The tidal drag could theoretically explain the westerly shift of the lithosphere relative to the underlying mantle. Notwithstanding, viscosity in the asthenosphere is apparently too high to allow mechanical decoupling produced by tidal forces. Here, we propose a model for global scale geodynamics accompanied by numer- ical simulations of the tidal interaction of the Earth with the Moon and the Sun. We provide for the first time a theoretical proof that the tidal drag can produce a westerly motion of the lithosphere, also com- patible with the slowing of the Earth’s rotational spin. Our results suggest a westerly rotation of the litho- sphere with a lower bound of x % ð0:1 0:2Þ /Myr in the presence of a basal effective shear viscosity g % 1016 Pa s, but it may rise to x 〉 1 /Myr with a viscosity of g K 3 1014 Pa s within the Low- Velocity Zone (LVZ) atop the asthenosphere. This faster velocity would be more compatible with the mainstream of plate motion and the global asymmetry at plate boundaries. Based on these computations, we suggest that the super-adiabatic asthenosphere, being vigorously convecting, may further reduce the viscous coupling within the LVZ. Therefore, the combination of solid Earth tides, ultra-low viscosity LVZ and asthenospheric polarized small-scale convection may mechanically satisfy the large-scale decoupling of the lithosphere relative to the underlying mantle. Relative plate motions are explained because of lat- eral viscosity heterogeneities at the base of the lithosphere, which determine variable lithosphere- asthenosphere decoupling and plate interactions, hence plate tectonics.
    Description: Published
    Description: 101623
    Description: 1T. Struttura della Terra
    Description: JCR Journal
    Keywords: Tidal drag ; Lithosphere-asthenosphere interaction ; Plate motions ; Polarized plate tectonics ; Geodynamics ; 04.04. Geology
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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