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What’s seismology about?

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Presentation on theme: "What’s seismology about?"— Presentation transcript:

1 What’s seismology about?
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.

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3 Elastic Moduli Young’s Modulus Poisson Ratio Bulk Modulus
Shear Modulus Lamb’s constants Vp, Vs.

4 E = s = tensile stress = (F /A) e = tensional strain = (DL /L) s e
Young’s modulus s = tensile stress = (F /A) e = tensional strain = (DL /L) … for uniaxial tension or compression s e E =

5 E = s = tensile stress = (F /A) e = tensional strain = (DL /L) s e
Young’s modulus s = tensile stress = (F /A) e = tensional strain = (DL /L) … for uniaxial tension or compression s e E =

6 Poisson’s ratio = - (eyy / exx)
Under a stress (sxx) along the x-axis, longitudinal strain = exx = and transverse strain = eyy = DL L DW W Then, Poisson’s ratio = - (eyy / exx)

7 Bulk Modulus = (DP/Q) … where Q = dilatation = DV/V and P = pressure

8 m = shear stress = (DF /A) shear strain = (Dl /L) A shear stress
shear modulus shear stress = (DF /A) shear strain = (Dl /L) shear stress shear strain m =

9 Elastic Moduli and Densities of Some Common Materials
From Lay & Wallace (1995)

10 From Lay & Wallace (1995)

11 K + ( )m l + 2m V = a = = r m V = b = 2m n E l = k - =
p 4/3 V = b = m s Where m,l are the Lamé coefficients and l is l = k = 2m n E ( 1 + n ) ( 1 - 2n )

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13 Body Waves compressions P-wave dilatations S-wave amplitude wavelength

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21 Body wave Amp ~ 1/x Surface wave Amp ~ x-1/2

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29 Late homework policy Late homework will not be accepted one week after the deadline. Late homework will be penalized: 90% (1 day late), 80% (2 day late), 60% (3 day late), 40 % (4 day late) and 20% (5-7 day late).

30 Body Waves compressions P-wave dilatations S-wave amplitude wavelength

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35 Seismic Rays & Geometric Ray Theory
Rays are defined as the normal to the wave fronts and thus point in the direction of propagation. Connecting the these successive directions forms a ray paths. In the case of plane wave, rays are a family of straight lines; in the case of spherical wave, rays are spokes radiating out from the seismic source. They provide a convenient means of tracking an expanding wave front. The seismic rays corresponding to P and S waves behave very much as light does in traveling through materials of varying indices of refraction. This leads to many parallels with optics: rays bend, focus, and defocus depending on the velocity distribution. Although geometric ray theory is an approximation, it, however, simplifies the analysis and yet gives the correct answer or a good approximation.

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38 Fermat’s Principle Ray paths between two points are those for which travel time is an extremum, either a minimum or maximum, with respect to the nearby possible paths.

39 Snell’s Law and Fermat Principle
Fermat Principle: T(x) is either minimum or maximum

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44 Reynolds (1997)

45 Spherical Ray Parameter
R sin i = constant = p V

46 What control reflection and transmission?
Continuity of stress Continuity of displacement

47 I = 1 I = 2 Reynolds (1997)

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