Tectonophysics
A.Y. 2024/2025
Learning objectives
The course unit aims to make students acquire the ability to understand and describe mathematically the main physical processes that take place within our planet, from the Earth's surface to the core-mantle boundary, with particular regard to phenomena that modify the Earth on time scales of 102 - 106 years. The mathematization of these processes is also relevant to achieve the goal of making us understand the changes that our planet undergoes and that collectively take the name of global change. The student will be able to mathematically model the perturbations in radial and tangential displacements and gravitational potential, today monitored through different geophysical and geodetic techniques, due to a wide range of Solid Earth phenomena, from the redistribution of masses at the Earth's surface (changes in sea level, mass instability in the glacial compartment of the planet, earthquakes) and inside (convection of the mantle), to instability in the Earth's rotation.
Expected learning outcomes
At the end of the course unit the student will have acquired the following skills:
1) will be able to matematize a realistic model of the Earth, spherically symmetric, self-gravitating and viscoelastic, in which the fundamental equations of conservation of momentum of momentum, angular momentum and Poisson are expanded in spherical harmonics;
2) will be able to derive in a completely analytical way the Green functions, relating to the perturbation of gravitational potential and surface deformations of the Earth, for surface and internal loads as well as dislocations, for a spherical, self-gravitating and incompressible model, due to surface and internal mass and redistribution and earthquakes;
3) will be able to use the results of the previous two points to matematize the physics inherent in the global processes that the Earth undergoes, following the melting taking place in the glacial compartment interacting with the solid part of the Earth, the changes in the average sea level and following the earthquakes that occur both in the Pacific belt of fire and in Italy, targeted towards a modern control the territory in which we live;
4) will be able to model and interpret from a physical point of view the perturbations of the Earth's rotation and gravitational potential, traceable to point 3) above, aimed at the exploitation of satellite gravitational data and GNSS (Global Navigation Satellite System) data;
5) will be able to apply the acquired methodologies to other planets and satellites of the Solar System, in particular to Icy Moons, such as Europa, Ganymede and Callisto of Jupiter and Titan and Enceladus of Saturn.
1) will be able to matematize a realistic model of the Earth, spherically symmetric, self-gravitating and viscoelastic, in which the fundamental equations of conservation of momentum of momentum, angular momentum and Poisson are expanded in spherical harmonics;
2) will be able to derive in a completely analytical way the Green functions, relating to the perturbation of gravitational potential and surface deformations of the Earth, for surface and internal loads as well as dislocations, for a spherical, self-gravitating and incompressible model, due to surface and internal mass and redistribution and earthquakes;
3) will be able to use the results of the previous two points to matematize the physics inherent in the global processes that the Earth undergoes, following the melting taking place in the glacial compartment interacting with the solid part of the Earth, the changes in the average sea level and following the earthquakes that occur both in the Pacific belt of fire and in Italy, targeted towards a modern control the territory in which we live;
4) will be able to model and interpret from a physical point of view the perturbations of the Earth's rotation and gravitational potential, traceable to point 3) above, aimed at the exploitation of satellite gravitational data and GNSS (Global Navigation Satellite System) data;
5) will be able to apply the acquired methodologies to other planets and satellites of the Solar System, in particular to Icy Moons, such as Europa, Ganymede and Callisto of Jupiter and Titan and Enceladus of Saturn.
Lesson period: Second semester
Assessment methods: Esame
Assessment result: voto verbalizzato in trentesimi
Single course
This course can be attended as a single course.
Course syllabus and organization
Single session
Responsible
Lesson period
Second semester
Lectures and laboratory lessons could be carried out in synchronous mode using the TEAMS platform
Course syllabus
The course is aimed at allowing the students to acquire the ability to understand and mathematically describe the main physical processes that occur within our planet, from the Earth's surface to the core-mantle boundary, with particular regard to phenomena that modify the Earth on time scales of 102 - 106 years. The mathematization of these processes is also relevant to reach the goal of making the changes that our planet undergoes understandable and collectively called global change.The student will be able to mathematically model the perturbations in the radial and tangential displacements and in the gravitational potential, now monitored by different geophysical and geodetic techniques, due to a wide range of Solid Earth phenomena, from the redistribution of masses on the Earth's surface (variations ofsea level, instability of mass in the glacial compartment of the planet, earthquakes) and within it (mantle convection), instability in the Earth's rotation.
At the end of the course the student will have acquired the following skills:
1) will know how to mathematize a realistic model of the Earth with spherical symmetry, self-gravitating and viscoelastic, in which the fundamental equations of conservation of momentum, of angular momentum and Poisson equation are developed in spherical harmonics;
2) will be able to derive in a completely analytical way the Green functions related to the perturbation of the gravitational potential and to the superficial deformations for surface and internal loads and dislocations for a spherical, self-gravitating and incompressible model, due to surface and internal mass redistributions and earthquakes;
3) will be able to use the results of the two previous points to mathematize the physics inherent to the global processes that the Earth undergoes, following the fusion taking place in the glacial compartment interacting with the solid part of the Earth, the variations of the average sea level and the earthquakes that occur both in the Pacific belt of fire and in Italy, for the purpose of a modern control of the territory in which we live;
4) will be able to model and interpret from the physical point of view the perturbations of the terrestrial rotation and of the gravitational potential, ascribable to the previous point 3), with connections to the current gravitational missions of ESA (European Space Agency) and NASA (National Aeronautics and Space Administration);
5) will know how to apply the acquired methodologies also to other planets and satellites of the Solar System, in particular to the Icy Moons, such as Europa, Ganymede and Callisto of Jupiter and Titan and Enceladus of Saturn;
6) will be able to autonomously manage the problems related to the previous points, thanks to the use of the textbook: Global Dynamics of the Earth - Applications of viscoelastic relaxation theory to Solid and Earth Planetary Geophysics, Roberto Sabadini, Bert Vermeersen and Gabriele Cambiotti ( Authors), Springer (Editor), second edition 2016.
At the end of the course the student will have acquired the following skills:
1) will know how to mathematize a realistic model of the Earth with spherical symmetry, self-gravitating and viscoelastic, in which the fundamental equations of conservation of momentum, of angular momentum and Poisson equation are developed in spherical harmonics;
2) will be able to derive in a completely analytical way the Green functions related to the perturbation of the gravitational potential and to the superficial deformations for surface and internal loads and dislocations for a spherical, self-gravitating and incompressible model, due to surface and internal mass redistributions and earthquakes;
3) will be able to use the results of the two previous points to mathematize the physics inherent to the global processes that the Earth undergoes, following the fusion taking place in the glacial compartment interacting with the solid part of the Earth, the variations of the average sea level and the earthquakes that occur both in the Pacific belt of fire and in Italy, for the purpose of a modern control of the territory in which we live;
4) will be able to model and interpret from the physical point of view the perturbations of the terrestrial rotation and of the gravitational potential, ascribable to the previous point 3), with connections to the current gravitational missions of ESA (European Space Agency) and NASA (National Aeronautics and Space Administration);
5) will know how to apply the acquired methodologies also to other planets and satellites of the Solar System, in particular to the Icy Moons, such as Europa, Ganymede and Callisto of Jupiter and Titan and Enceladus of Saturn;
6) will be able to autonomously manage the problems related to the previous points, thanks to the use of the textbook: Global Dynamics of the Earth - Applications of viscoelastic relaxation theory to Solid and Earth Planetary Geophysics, Roberto Sabadini, Bert Vermeersen and Gabriele Cambiotti ( Authors), Springer (Editor), second edition 2016.
Prerequisites for admission
None
Teaching methods
Frontal lessons
Teaching Resources
Global Dynamics of the Earth - Applications of viscoelastic relaxation theory to Solid Earth and Planetary Geophysics, Roberto Sabadini, Bert Vermeersen and Gabriele Cambiotti (Authors), Springer (Editor), second edition 2016.
Assessment methods and Criteria
Oral examination
GEO/10 - SOLID EARTH GEOPHYSICS - University credits: 6
Practicals with elements of theory: 24 hours
Lessons: 32 hours
Lessons: 32 hours
Professor:
Cambiotti Gabriele
Shifts:
Turno
Professor:
Cambiotti GabrieleProfessor(s)