fig. 8.00 earthquakes and earthquake hazards. 3 seismic waves allow us to look inside the earth

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Fig. 8.00 Earthquakes and Earthquake Hazards

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Page 1: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Fig. 8.00

Earthquakes and Earthquake Hazards

Page 2: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 3: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

3

Seismic waves allow us to look inside the Earth

Page 4: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 5: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 6: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 7: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Vp =k + 4 3μ

ρ

Vs =μ

ρ

κ = compressibility

μ = rigidity

ρ = density

Seismic Waves

Page 8: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 9: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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QuickTime™ and aGIF decompressor

are needed to see this picture.

www.eas.purdue.edu/~braile

Page 10: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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QuickTime™ and aGIF decompressor

are needed to see this picture.

www.eas.purdue.edu/~braile

Page 11: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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QuickTime™ and aGIF decompressor

are needed to see this picture.

www.eas.purdue.edu/~braile

Page 12: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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QuickTime™ and aGIF decompressor

are needed to see this picture.

www.eas.purdue.edu/~braile

Page 13: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Fig. 8.12ab

W. W. Norton

Page 14: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Fig. 8.13ab

W. W. Norton

Page 15: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Fig. 8.13c

W. W. Norton

Page 16: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Fig. 8.15

Page 17: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 18: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Seismic Refraction

i’

i

sin(i)

sin(i’)=

Velocity of AVelocity of B

A

B

Page 19: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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Refraction

Page 20: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 21: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 22: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Seismic wave tomography — a CAT-scan of the interior

Colors are seismic wave velocity anomalies

Page 23: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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Red = slow (hot)

Blue = fast (cold)

Here is a slice through North America showing the now-subducted Farallon Plate, sinking to the bottom of the mantle.

Heating reduces rigidity more than it reduces density, so hotter material have slower seismic velocities

Page 24: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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How Faults Work — the Mechanics of Earthquakes

Page 25: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Static Friction with a spring

Fn

Fs=kx

At time of sliding τ =μs σ , where μs is the static coefficient of friction

σ = Fn/A(A= area of base)

τ = Fs/A

Why Earthquakes (stick-slip behavior)?

Page 26: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Fn

Fs=kx

Fs

Displacement

If friction was this simple — and if the applied forces, coming from plate motions, were constant — would we have stick-slip behavior?

μs

Page 27: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Of course, friction is NOT so simple — the coefficient of friction changes once sliding begins, and if μd < μs, then we should see the idealized stick-slip behavior

slip

Page 28: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

τ

Displacement

μs σ

μd σ

slope is -k (spring constant)

Idealized Stick-Slip Behavior

μs = μstatic

μd = μdynamic

Page 29: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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EQ Slip Model

Page 30: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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Page 31: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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As the rupture grows, more energy is released and a larger magnitude earthquake results. If a big segment of the fault is right near the limit, a small rupture can take off and grow into a huge rupture and a huge earthquake

Page 32: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

τ

Displacement

μs σ

μd σ

Idealized Stick-Slip Behavior

This is equivalent to the “re-loading” timeif we assume that the tectonic driving forces are applied at a steady rate

Page 33: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Time

Dis

pla

cem

en

t

Plate tectonic rate and friction along fault determine recurrence time and average size of earthquakes

Earthquake event

Time between earthquake — re-loading time

plate tecto

nic rate

Page 34: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Time

Dis

pla

cem

en

t

Same plate tectonic rate, but low friction (weaker fault plane), so shorter recurrence time and smaller earthquakes

Earthquake event

Time between earthquake

plate tecto

nic rate

Page 35: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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rocks in the circles were formerly right next to each other

The San Andreas Fault is the plate boundary between NAM and PAC

Page 36: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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4 cm/yr x 100 yr = 4 m (avg slip for M8 EQ)

Slip on the fault occurs in small segments, but over time, every part of the fault has to accommodate the 4 cm/yr plate tectonic rate

Page 37: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

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QuickTime™ and aSorenson Video 3 decompressorare needed to see this picture.

Page 38: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
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Page 40: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth
Page 41: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

Normal Fault Surface Scarp

Borah Peak, Idaho M 7.3 October 28, 1983

Page 42: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

1964 Alaskan Earthquake (M~9.2)

This side moved up about 6 m

Page 43: Fig. 8.00 Earthquakes and Earthquake Hazards. 3 Seismic waves allow us to look inside the Earth

M~8