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Department of Earth SciencesKFUPM
Gravity Methods 3
Fc
Introduction to GeophysicsIn
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Previous Lecture
•Gravity Methods 2•Bouguer Correction •Bouguer Gravity Anomaly on Land •Bouguer Gravity Anomaly on Sea
•Mid-Term Exam
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0
20
40
60
80
100
1 2 3 4 5
MIDTERM
MIDTERM
Gra
de
Students
Grade Distribution in Mid-Term Exam
2043
17
2142
69
2227
36
2262
02
2343
45
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Mid-Term Exam Solutions
smV
smV
/100002.0
2000
/30004.0
1200
2
1
12
2112
VV
VVhxcr
300010000
10000300021200 1
h
7000
1300021200 1h
186.1
1200h mh 3.4401
h1? km
Bedrock = V2 = xxxx ft/sec
Alluvium = V1 = xxxx ft/sec ? km
Bedrock = V2 = xxxx ft/sec
Alluvium = V1 = xxxx ft/sec
XCR
h1
V 1
V2
1200 3200
0.4
0.6
Meters
Sec
ond
s
V1, V2, h1?
0.3
0.2
0.1
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Simplified version of Assignment 2
From Kearey, Brooks, and Hill, 2002
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For example, a double spike function, 2, 0, 1 convolved with an impulse response function 4, 3, 2, 1 .
It was class example of Lecture 9.2
34
pv
sv3
3
/2950
/95.2
mkg
cmg
GPamkgsmv s 04.43)/2950()/3820( 322
GPa
Pamkgsm
vk P
02.79
)10*304.4(3
4)/2950()/6800(
3
4
1032
2
Given that the P-velocity of a rock is 6.8 km/s, the S-velocity is 3.82 km/s, and density 2.95 g/cm3, calculate µ and k?
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Modified version asked in Quiz 1
?=2.08377.21.8258.4(c)
3.82?=55.332.5533.3(b)
3.272.54.36?=?(a)
V2 (km/sec)R (° )V1 (km/sec)I (°)Case
?=2.08377.21.8258.4(c)
3.82?=55.332.5533.3(b)
3.272.54.36?=?(a)
V2 (km/sec)R (° )V1 (km/sec)I (°)Case
Where possible, supply the missing quantity in each case in the following table, where: i = angle of incidence r = angle of refraction v1 = wave speed in upper layer, v2 = wave speed in lower layer. The wave originates in the upper layer.
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Modified version asked in Quiz 2
The same question solved in Class
21
11
2,
n
iii
n
iinrms ttvv v1=1500 m s-1
v2=2000 m s-1
v3=2345 m s-1
t1=2.14 s
t2=1.21 s
t3=1.13 s
vrms at the base of layer 3?
1-s m 064.1882
13.121.114.2
)13.12345()21.12000()14.21500( 21
222
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vrms at the base of layer 1?
1-s m150014.2
)14.21500( 21
2
1-s m 672.1697
21.114.2
)21.12000()14.21500( 21
22
vrms at the base of layer
2?
v1=2.5 km s-1
ρ1 =2.5 g/ cc
v2=1.7km s-1
ρ2 =2.02 g/ cc
v3=2.2 km s-1
ρ3 =2.27 g/ cc
Shale
Sand + gas
Sand + oil
v4=2.3 km s-1
ρ4 =2.28 g/ ccSand + oil
h1=100m
h2=200m
h3=150m
Explosion
v1=2.5 km s-1
ρ1 =2.5 g/ cc
v2=1.7km s-1
ρ2 =2.02 g/ cc
v3=2.2 km s-1
ρ3 =2.27 g/ cc
Shale
Sand + gas
Sand + oil
v4=2.3 km s-1
ρ4 =2.28 g/ ccSand + oil
h1=100m
h2=200m
h3=150m
Explosion
29.0)5.2(5.2)02.2(7.1
)5.2(5.2)02.2(7.1
1122
112212
vv
vvR
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v1=2.5 km s-1
ρ1 =2.5 g/ cc
v2=1.7km s-1
ρ2 =2.02 g/ cc
v3=2.2 km s-1
ρ3 =2.27 g/ cc
Shale
Sand + gas
Sand + oil
v4=2.3 km s-1
ρ4 =2.28 g/ ccSand + oil
h1=100m
h2=200m
h3=150m
Explosion
v1=2.5 km s-1
ρ1 =2.5 g/ cc
v2=1.7km s-1
ρ2 =2.02 g/ cc
v3=2.2 km s-1
ρ3 =2.27 g/ cc
Shale
Sand + gas
Sand + oil
v4=2.3 km s-1
ρ4 =2.28 g/ ccSand + oil
h1=100m
h2=200m
h3=150m
Explosion
19.0)02.2(7.1)27.2(2.2
)02.2(7.1)27.2(2.2
2233
223323
vv
vvR
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v1=2.5 km s-1
ρ1 =2.5 g/ cc
v2=1.7km s-1
ρ2 =2.02 g/ cc
v3=2.2 km s-1
ρ3 =2.27 g/ cc
Shale
Sand + gas
Sand + oil
v4=2.3 km s-1
ρ4 =2.28 g/ ccSand + oil
h1=100m
h2=200m
h3=150m
Explosion
v1=2.5 km s-1
ρ1 =2.5 g/ cc
v2=1.7km s-1
ρ2 =2.02 g/ cc
v3=2.2 km s-1
ρ3 =2.27 g/ cc
Shale
Sand + gas
Sand + oil
v4=2.3 km s-1
ρ4 =2.28 g/ ccSand + oil
h1=100m
h2=200m
h3=150m
Explosion
024.0)27.2(2.2)28.2(3.2
)27.2(2.2)28.2(3.2
3344
334434
vv
vvR
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Recall GradingIn
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Final Exam 35%Mid Term Exam 25%Quiz 15%Homework 15%Class Participation 10%
Homework StatusIn
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Homework StatusIn
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Homework StatusIn
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Summary of Equations for Free Air and Bouguer Gravity Anomalies
Standard parameters used to compute gravity anomalies on land and at sea.
•FAC =Free-Air Correction; BC =Bouguer Corrections;
•BCs =Bouguer correction at sea
•ρ =reduction density; h =elevation (m) and hw =water depth (m)In
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Bouguer Gravity Anomaly on SeaIn
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Δgfa= g – gt + FAC
ΔgB= Δgfa-BC BC= 0.419 ρ h
FAC= h x (0.308 mGal/m)
Terrain CorrectionIn
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ΔgBC= ΔgB+TC
terrain correction is no needed in areas of low relief but is required where changes in topography is significant and equation for a complete Bouguer anomaly is:
Terrain correction is needed in areas of high relief in order to account decrease of observed gravity due to
1. mountains above the slab (1),
2. and overcorrection due to valleys (2).
Terrain CorrectionIn
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ΔgBC= ΔgB+TC
Terrain Correction
For both situations, the terrain correction is positive, making the complete Bouguer anomaly higher than the simple Bouguer anomaly.
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Gravity MeasurementIn
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True gravitational acceleration (ρ)
Reflecting the difference in gravitational acceleration (Δρ) at one station (ρ1) compared to another (ρ2).
Measurement of relative gravity
A gravimeter measures the length of a spring (L), which is proportional to the gravitational acceleration (g).
+ΔL Increase in gravity-ΔL Decrease in gravity
Map of relative gravity survey. The traverse starts with a measurement at the base station, the each of the 16 stations, followed by re-measurement at the base station.In
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Microgravity surveys require that we measure g with
precision of better than 1 part in 40 million
• we measure either absolute gravity or more commonly, relative gravity (change in g between two stations)
Methods:
1. Falling body
2. Pendulums
3. Mass-spring gravimeters
Gravity MeasurementIn
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Gravitational acceleration can be measured directly by dropping an object and measuring its acceleration.
Free Fall Methods
• distance a body falls is proportional to the time it has fallen squared
z = ½gt2
g = 2z/t2
ginst = 2 ·50 m/(3.19 s)2
= 9.8 m/s2
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PendulumsGravity first measured by Pierre Bouguer in 1749
(257 years ago) using Pendulum: period of oscillation T of pendulum is inversely proportional to g
T = 2K/gK = constant related to pendulum design
T
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Gravity Units
212
E
E
sE
R
mG
m
Fg
Most of us are familiar with the units of g as feet/sec2 or meters/sec2, etc.
From Newton’s law of gravity g also has units of
kilogram
newtonsEg
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Using the metric system, we usually think of g as being 9.8 meters/sec2.This is an easy number to recall. If, however, we were on the Martian moon Phobos, gp is only about 0.0056meters/sec2 [m/sec2] might not be the most useful units to use on Phobos.
Some unit names you will hear when gravity applications are discussed include:
9.8 m/sec2
980 Gals (or cm/sec2)980000 milligals (i.e. 1000th of a Gal)
We experience similar problems in geological applications, because changes of g associated with subsurface density contrasts can be quite small.
Gravity Units
http://www.esa.int/SPECIALS/Mars_Express/SEM21TVJD1E_0.html
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1 mGal = 10 microns/sec2
1 milligal equals 10-5 m/sec2 or conversely
1 m/sec2 = 105 milligals.
The gravity on Phobos is 0.0056m/s2 or 560 milligals.
Are such small accelerations worth contemplating?
Can they even be measured?
GalGal = 1 cm/sec2= 0.01 m/sec2
1 mGal = 10-3 Gal
Istituto e Museo di Storia della Scienza
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1564-1642