Book contents
- Frontmatter
- Contents
- Preface
- 1 Origin and history of the Solar System
- 2 Composition of the Earth
- 3 Radioactivity, isotopes and dating
- 4 Isotopic clues to the age and origin of the Solar System
- 5 Evidence of the Earth's evolutionary history
- 6 Rotation, figure of the Earth and gravity
- 7 Precession, wobble and rotational irregularities
- 8 Tides and the evolution of the lunar orbit
- 9 The satellite geoid, isostasy, post-glacial rebound and mantle viscosity
- 10 Elastic and inelastic properties
- 11 Deformation of the crust: rock mechanics
- 12 Tectonics
- 13 Convective and tectonic stresses
- 14 Kinematics of the earthquake process
- 15 Earthquake dynamics
- 16 Seismic wave propagation
- 17 Seismological determination of Earth structure
- 18 Finite strain and high-pressure equations of state
- 19 Thermal properties
- 20 The surface heat flux
- 21 The global energy budget
- 22 Thermodynamics of convection
- 23 Thermal history
- 24 The geomagnetic field
- 25 Rock magnetism and paleomagnetism
- 26 ‘Alternative’ energy sources and natural climate variations: some geophysical background
- Appendix A General reference data
- Appendix B Orbital dynamics (Kepler's laws)
- Appendix C Spherical harmonic functions
- Appendix D Relationships between elastic moduli of an isotropic solid
- Appendix E Thermodynamic parameters and derivative relationships
- Appendix F An Earth model: mechanical properties
- Appendix G A thermal model of the Earth
- Appendix H Radioactive isotopes
- Appendix I A geologic time scale
- Appendix J Problems
- References
- Name Index
- Subject Index
26 - ‘Alternative’ energy sources and natural climate variations: some geophysical background
Published online by Cambridge University Press: 05 July 2013
- Frontmatter
- Contents
- Preface
- 1 Origin and history of the Solar System
- 2 Composition of the Earth
- 3 Radioactivity, isotopes and dating
- 4 Isotopic clues to the age and origin of the Solar System
- 5 Evidence of the Earth's evolutionary history
- 6 Rotation, figure of the Earth and gravity
- 7 Precession, wobble and rotational irregularities
- 8 Tides and the evolution of the lunar orbit
- 9 The satellite geoid, isostasy, post-glacial rebound and mantle viscosity
- 10 Elastic and inelastic properties
- 11 Deformation of the crust: rock mechanics
- 12 Tectonics
- 13 Convective and tectonic stresses
- 14 Kinematics of the earthquake process
- 15 Earthquake dynamics
- 16 Seismic wave propagation
- 17 Seismological determination of Earth structure
- 18 Finite strain and high-pressure equations of state
- 19 Thermal properties
- 20 The surface heat flux
- 21 The global energy budget
- 22 Thermodynamics of convection
- 23 Thermal history
- 24 The geomagnetic field
- 25 Rock magnetism and paleomagnetism
- 26 ‘Alternative’ energy sources and natural climate variations: some geophysical background
- Appendix A General reference data
- Appendix B Orbital dynamics (Kepler's laws)
- Appendix C Spherical harmonic functions
- Appendix D Relationships between elastic moduli of an isotropic solid
- Appendix E Thermodynamic parameters and derivative relationships
- Appendix F An Earth model: mechanical properties
- Appendix G A thermal model of the Earth
- Appendix H Radioactive isotopes
- Appendix I A geologic time scale
- Appendix J Problems
- References
- Name Index
- Subject Index
Summary
Preamble
Solid Earth geophysics offers assessments of energy sources alternative to fossil fuels. We gain some insight on the accessibility and geophysical effects of exploiting any particular energy source by comparing the contemplated scale of its use with the corresponding natural dissipation. The analyses and discussions of earlier chapters are used to address these issues. We consider also the astronomically induced climate variations that must be distinguished from the consequences of fossil fuel use. This is background material to the environmental questions that are primarily problems for atmospheric science and to the resource question of fossil fuel exhaustion that is a central problem for exploration geophysicists. Energy sources considered are solar, wind, tidal, ocean wave, hydroelectric and geothermal, but not nuclear. We neglect also the possibilities of biofuel, merely noting that if it is to make a major contribution it will require a large fraction of the land area to be devoted to appropriate crops.
The energy dissipations by various natural processes (Section 26.2), give an indication of their availability for exploitation, and especially the magnitudes of their potential contributions. The comparison with the human use of energy draws attention to the fact that human activity is a global geophysical scale phenomenon. This means that major adjustments to it cannot be made easily in a controlled way. But major adjustments to energy use are inevitable and if they are uncontrolled they are likely to be painful.
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- Chapter
- Information
- Physics of the Earth , pp. 438 - 447Publisher: Cambridge University PressPrint publication year: 2008