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Geology 5640/6640Introduction to Seismology
12 Jan 2015
© A.R. Lowry 2015Read for Wed 14 Jan: S&W 29-52 (§2.1-2.3)
Last time: Course overview
Seismology is used as a tool to investigate:
• Seismic sources: Earthquake physics, magma transfer in volcanic systems, “icequakes”, storms, nuclear test verification, …
• Seismic velocity & impedance structure: Seismic reflection imaging (oil & gas industry), site investigation (construction, environmental, hydro resources), virtually all fundamental research into processes in the Earth’s interior
SourcePulse
Seismogram
Source
Medium
Receiver
Origintime
Traveltime
Arrivaltime
A seismogram is a time-record of motion of an inertial mass…
… that contains information about the source, Earth response, and seismometer response.
(After S&WFig. 1.1-1)
11 km/s
8-10 km/s
8-14 km/s
Most of what we know about the Earth’s interior comes from seismology.
And not justEarth!Apollo-eraseismic datademonstratethe lunar interior has similaritiesto Earth’s…
How to use these powerpoints:
• Review them often: Before each class, while doing exercises, and in preparing your projects
• The most important points of each lecture (in my opinion) are summarized on the first slide of the next lecture
• Note the notation! Arial Black, italic means Important, pay attention… Arial Black, italic, red font means Critically Important concept or terminology that I expect you to understand intimately for exercises and projects Times New Roman, italic, black font means this is an equation or an algebraic variable
A Red Box with Grey Background means this is an especially important concept or equation
Seismology (A brief review ofthings you “already know”)
Four Types of Seismic Waves:
(1) P (primary) wave (Velocity Vp = 4 to 14 km/s)
(2) S (secondary) wave (Vs = 2/5 to 3/5 Vp, or 0)
(3) Surface Waves (Love, Rayleigh) V slightly < Vs
(4) Normal Modes (Resonant “Tones”, like a bell…) continue for months after largest earthquakes periods of hours or days “standing waves”
Body Waves}
P
S
Surface (Love)
Surface (Rayleigh)
Seismic waves are strain wavesthat propagate in a medium…
Common analogies use ripples in a pond, or light. There aresimilarities in that all three are described by the wave equation.Ripples & seismic waves similarly involve stress & displacements that propagate as individual particles in themedium oscillate between potential and kinetic energy states…
But, a major difference is rheology. Stress, displacement &strain in a solid continuum are governed by Hooke’s Law.
Despite differences, similarities inherent in the wave equation many important principles can be borrowed from optics.
One of these is Huygen’s Principle:
Every point on a wavefront can be treated as a point source for the next generation of wavelets. The wavefront at a timet later is a surfacetangent to thefurthest point oneach of thesewavelets. This isbecause extremalpoints of propagationhave the greatest constructiveinterference…
Another is Fermat’s Principle (or the principle ofleast time):
The propagation path (or raypath) between any two pointsis that for which travel-time is the least of all possible paths.
(Here a ray is the normal to a wavefront at any given time):
A key principle because most of our applications will involvea localized source and observation at a point (seismometer).
•
•
V = fast V = slow
least time in slow
least time in fast
Fermat’s principle leads to Snell’s Law:
Travel-time is minimized whenwhen the ratio of sines of theangle of incidence (anglefrom the normal) to a velocity boundary is equal to the ratio of the velocities, i.e.,
straight line
least time
€
sinθ1
sinθ2
=V1
V2
Aboriginal spear-fishers understand Snell’s law intuitively, after learning to always aim below the visual location of the fish!
Important terminology: Refractions are transmitted rays that bend at a change in medium; Reflections are bounces off an interface that remain within the original medium.
Refraction
Reflection
Reflections & Refractions:
Consider that when a seismic wave meets a layer boundarybetween solid media with different velocities V (= f = /T),• Energy E must be conserved• Stress must be continuous (i.e. the same on both sides)• Displacement u must be continuousThis is achieved by “partitioning” the energy between reflections & refractions, and in most cases by convertingpart of the energy from one type of wave to the other!
incoming P
reflected Preflected Srefracted P
refracted S