Chapter 1 Introduction
The Earth is composed of silicate and iron-alloy materials with the remarkable property that, over the wide range of pressure and temperature conditions existing within the planet, the materials respond nearly elastically under the application of small-magnitude transient forces but viscously under the application of long-duration forces. This time dependence of the material properties means that Earth ârings like a bellâ when short-term forces, such as sudden slip of rock across a fault surface or detonation of a buried explosion, are applied, even while the fluid-like flow of global convection continually reshapes the surface and interior of the planet over geological time scales. The mechanical vibrations result from the quasi-elastic behavior, which involves excitation and propagation of elastic waves in the interior. These waves are physical motions that ground-motion recording instruments called seismometers can preserve for scientific analysis. This text describes the nature of these elastic waves and the analysis of their recordings. It demonstrates how the elastic properties of the Earth reveal many characteristics of the present state of the Earth as well as of the long-term processes occurring in the global dynamic system. We hope that it will also provide insight into the processes producing destructive earthquakes, such as the January 17, 1994, Northridge, California event, which caused more than $20 billion in damage to Los Angeles.
Seismology is the study of the generation, propagation, and recording of elastic waves in the Earth (and other celestial bodies) and of the sources that produce them. Both natural and human-made sources of deformational energy can produce seismic waves, elastic disturbances that expand spherically outward from the source as a result of transient stress imbalances in the rock. The properties of seismic waves are governed by the physics of elastic solids, which is fully described by the theory of elastodynamics. Basic elastodynamics is presented in chapters 2, 3, 4, and 8. This body of theory, rooted in continuum mechanics, linear elasticity, and applied mathematics dating back to the early 1800s, provides a quantitative framework for analysis of elastic waves in the Earth.
Seismological procedures provide the highest resolution of internal Earth structure of any geophysical method. This is because elastic waves have the shortest wavelengths of any âgeophysical wave,â and the physics that governs them localizes their sensitivity spatially and temporally to the precise path traveled by the energy.
These localization properties provide far higher resolution than obtainable with electrical, gravitational, magnetic, or thermal fields, which average large regions and times.
Recordings of ground motion as a function of time, or seismograms, provide the basic data that seismologists use to study elastic waves as they spread throughout the planet. An example of a modern seismic recording is shown in Figure 1.1. Three orthogonal components of ground motions (upâdown, northâsouth, and eastâwest) are shown, as are needed to record the total (vector) ground displacement history, at station HRV (Harvard, Massachusetts). The source that produced these motions was a distant large earthquake that struck central Chile in 1985. The ground motions at HRV commenced about 10 min after the fault rupturing began, the length of time it took for the fastest seismic waves to travel through the Earth from the Chilean source region to the station. A complex sequence of slower wave arrivals caused ground motions at the station to continue for several hours. These recorded motions are quite tiny, with ground displacements of less than 0.7 mm and ground velocities of less than 60 ÎŒm/s. Such motions were imperceptible at HRV other than by sensitive instrumentation, but the waves were much stronger near the source and caused extensive damage and building collapse in Chile. Every wiggle on the seismogram has significance and contains information about the source and the Earth structure through which the waves have traveled. Seismologists strive to extract all possible information from the seismogram by understanding each wiggle.
A tremendous range in scales is considered in seismology, for both the many types of sources and the diverse seismic waves that result. The smallest detectable microearthquake has a seismic moment (an important physical quantity equal to the product of the fault surface area, the rigidity of the rock, and the average displacement on the fault) on the order of 105 N m, and great earthquakes have moments as large as 1023 N m. The amplitudes of seismic-wave motions are directly proportional to the seismic moments; thus seismic-wave displacements span an enormous range. Seismic waves commonly used in exploration seismology have frequencies as high as 200 Hz, while the longest-period standing waves excited by great earthquakes have frequencies around 3 Ă 10â4 Hz and solid Earth tide frequencies are around 2.0 Ă 10â5 Hz. Thus, transient ground motions spanning a frequency range of 107 Hz are of interest. In fact, the study of seismic sources further extends the range of interest to zero frequency, or static deformations, near faults and explosions, even while new, very high resolution shallow-imaging techniques are utilizing kilohertz frequencies. A local crustal survey may use waves that are traveling only tens of meters, while analysis of global structure may involve waves such as R7, which travel more than 108 m along the Earthâs surface.
One of the major challenges posed by the huge frequency range (bandwidth) and amplitude range (dynamic range) of interest for seismic observations has been to build seismometers capable of registering all useful signals against a background of ambient noise. No single instrument can record the full spectrum of motions with a linear response, so a suite of different seismic instruments that record limited portions of the seismic spectrum has been developed. However, great advances have been made in the last 10 years in developing seismic recording systems that provide remarkable bandwidth and dynamic range for the applications of global seismology to be emphasized in this text. The recording in Figure 1.1 was produced by such a system, and chapter 5 describes the remarkable instrument technology involved in the field of seismometry, or recording of ground motion.
The global distribution of earthquake sources, along with the requirement of extensive surface coverage with seismometers for the unraveling and interpretation of complex seismic signals, has made global seismology a truly international discipline, with unprecedented international collaboration, seismometer development, and data exchange over its 119+-year instrumental history. Over 3000 seismological observatories are in operation around the world today, with nearly every nation participating in the effort to record seismic waves continuously. The most recent efforts to upgrade the global network instrumentation by incorporating technological advances have involved countries such as Australia, Canada, China, England, France, Germany, Holland, Italy, Japan, Norway, Russia, Switzerland, and the United States, in keeping with the historic tradition of broad international collaboration. chapter 5 provides an overview of these efforts.
The fault that generated the 1985 Chile earthquake ruptured for about 100 km, with sliding motions on the fault lasting for only about 50 s. Thus, much of the prolonged nature of the vibrations in Figure 1.1 is due to wave interactions with the transmitting medium, which are manifested as a sequence of impulsive arrivals and longer-period oscillatory motions, including waves that repeatedly circle the globe. Most of these ground motions can now be interpreted quantitatively in the light of current knowledge of Earth structure, as shown in chapter 6. It is the fundamental simplicity of elastic waves, which transmit disturbances over great distances through the Earth wit...