Book contents
- Frontmatter
- Contents
- Preface to the first edition
- Preface to the second edition
- Introduction to the first edition
- 1 Background of thermodynamics of solids
- 2 Elastic moduli
- 3 Lattice vibrations
- 4 Equations of state
- 5 Melting
- 6 Transport properties
- 7 Earth models
- Appendix PREM model (1s) for the mantle and core
- Bibliography
- Index
Preface to the first edition
Published online by Cambridge University Press: 05 June 2012
- Frontmatter
- Contents
- Preface to the first edition
- Preface to the second edition
- Introduction to the first edition
- 1 Background of thermodynamics of solids
- 2 Elastic moduli
- 3 Lattice vibrations
- 4 Equations of state
- 5 Melting
- 6 Transport properties
- 7 Earth models
- Appendix PREM model (1s) for the mantle and core
- Bibliography
- Index
Summary
Not so long ago, Geophysics was a part of Meteorology and there was no such thing as Physics of the Earth's interior. Then came Seismology and, with it, the realization that the elastic waves excited by earthquakes, refracted and reflected within the Earth, could be used to probe its depths and gather information on the elastic structure and eventually the physics and chemistry of inaccessible regions down to the center of the Earth.
The basic ingredients are the travel times of various phases, on seismograms recorded at stations all over the globe. Inversion of a considerable amount of data yields a seismological earth model, that is, essentially a set of values of the longitudinal and transverse elastic-wave velocities for all depths. It is well known that the velocities depend on the elastic moduli and the density of the medium in which the waves propagate; the elastic moduli and the density, in turn, depend on the crystal structure and chemical composition of the constitutive minerals, and on pressure and temperature. To extract from velocity profiles self-consistent information on the Earth's interior such as pressure, temperature, and composition as a function of depth, one needs to know, or at least estimate, the values of the physical parameters of the high-pressure and high-temperature phases of the candidate minerals, and relate them, in the framework of thermodynamics, to the Earth's parameters.
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- Information
- Introduction to the Physics of the Earth's Interior , pp. ix - xiPublisher: Cambridge University PressPrint publication year: 2000