22
Ali Oncel [email protected] .sa Department of Earth Sciences KFUPM Gravity Methods 1 F c Introduction to Geophysics troduction to Geophysics-KFUP

Gravity Methods 1

Embed Size (px)

Citation preview

Page 1: Gravity Methods 1

Ali [email protected]

Department of Earth SciencesKFUPM

Gravity Methods 1

Fc

Introduction to GeophysicsIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 2: Gravity Methods 1

Field Trip: Refraction Seismology

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 3: Gravity Methods 1

Field Trip: Refraction Seismology

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 4: Gravity Methods 1

Field Trip: Refraction Seismology

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 5: Gravity Methods 1

Field Trip: Refraction Seismology

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 6: Gravity Methods 1

Field Application by Gravimeter

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

This Wednesday, Mid Term

Next Wednesday, May 10

Page 7: Gravity Methods 1

a. The gravity field is symmetric. Force vectors (arrows) have approximately equal magnitude and point toward the center of the Earth.

Earth’s Gravity Potential FieldIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 8: Gravity Methods 1

b. The magnitude and direction of the magnetic field is governed by positive (south) and negative (north) poles. Magnitude varies by a factor of two from equator to pole.

Earth’s Magnetic Potential FieldIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 9: Gravity Methods 1

Differences in Earth’s Potential Fields

Earth’s gravity field is simply compared to the magnetic field. Lines of the force for the gravity field are directed toward the center of the Earth while magnetic field strength and direction depend on the Earth’s positive and negative poles.

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 10: Gravity Methods 1

c. The acceleration due to gravity (a=g) of a body depends only the mass of attracting body (m2=M) and the distance to the center of that mass ( r=R ).

g=GM/R2

a. The gravitational force between two objects is directly proportional to their masses (m1, m2), and inversely proportional to the square of their distance ( r ).

b. The mass (m1), times the acceleration (a) due to mass (m2), determines the

gravitational force (F). F=m1 a

212

2112 r

mmGF

EARTH’S GRAVITY FIELDIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 11: Gravity Methods 1

212

E

E

sE

R

mG

m

Fg

The variation of g across the earth’s surface provides information about the distribution of density contrasts in the subsurface since m = V (i.e. density x volume).

ms spring mass, mE mass of the earth = 5.967 x 1024 kgRE radius of the earthLike apparent conductivity and resistivity, the acceleration of

gravity (g) is a basic physical property we measure, and from which, we infer the distribution of subsurface density contrast.

Earth’s Gravitational Acceleration

For perfectly spherical and non-rotating Earth with uniform mass distribution, gE represents the acceleration of gravity at a particular point on the earth’s surface: RE

mS

mE

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 12: Gravity Methods 1

a. The mass (M) of the Earth and radius ( r ) to the Earth’s center determine the gravitational acceleration (g) of objects and above Earth’s surface.

b. The acceleration is the same (g), regardless of the mass of the object.

c. Objects at Earth’s surface (radius R1) have greater acceleration than objects some distance above the surface (radius R2).

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 13: Gravity Methods 1

The main factors responsible for the difference in gravitational acceleration at the equator compared to the poles.

Gravity increases from 978,000 mGal at the equator, to about 983,000 mGal at the poles.Variation in gravity from equator to pole, according to 1967 Reference Gravity formula.In

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 14: Gravity Methods 1

Theoretical Gravity

2 42978.03185 1 0.005278895sin 0.000023463sinn

cmgs

The average value of gravity for a given latitude is approximated by the International Association of Geodesy in 1967.

gn =Normal Gravity: Gravitational acceleration

expected for a rotating ellipsoidal earth without any geologic complications and no surface features.

Ф=latitudeGravitation increase from the equator (Ф =0)

=978,03185 mGal to the pole (Ф =0)=983,217.72 mGalIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 15: Gravity Methods 1

dg/dR≈-0.308 mGal/m

dg/dR≈ average value for the change in gravity with increasing elevation

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 16: Gravity Methods 1

Free Air Gravity Correction

Rising upward from Earth’s surface, gravitational acceleration decreases by about 0.308 mGal for every meter of height.

A gravity station at high elevation tends to have a lower gravitational acceleration (g) than a station at lower elevation

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 17: Gravity Methods 1

Free Air Gravity Correction

•The free air correction (FAC) accounts for the extended radius to an observation point, elevated h meters above a sea level datum.

• The above equation illustrates that, for every 3 m (about 10 feet) upward from the surface of the Earth, the acceleration due to gravity decreases by about 1 mGal.

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 18: Gravity Methods 1

Gravity Anomaly

• What is an anomaly?• Difference between observed gravity and

International Gravity Formula (IGF) for same location or relative to local base

station, termed the gravity anomaly, Dg

Dg = gobs - gn

• difference is the result of density contrasts in the subsurface below the measurement point

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 19: Gravity Methods 1

Free Air Gravity Anomaly

Δgfa= g – gt + FAC

Δgfa = free gravity anomaly

g = gravitational acceleration observed at stationgt= theoretical gravity

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 20: Gravity Methods 1

Bouguer Correction

a

•The extra mass of mountains results in higher gravity relative to areas near sea level.

• The Bouguer Correction (BC) accounts for the gravitational attraction of the mass above the sea-level datum.

Intr

od

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 21: Gravity Methods 1

Bouguer Correction

•Thus, to account for the excess mass above a sea level datum, the Bouguer correction assumes an infinite slab of density (ρ), with thickness (h) equal to the station’s elevation.

BC= 2 π ρ G hG=Universal Gravitational Constant (6,367,000 m)

H= thickness of the slab (station elevation)

Substituting the values of G and 2 π yields:

BC= 0.419 ρ h

bIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM

Page 22: Gravity Methods 1

a

b

Bouguer CorrectionIn

trod

uct

ion t

o G

eop

hysi

cs-K

FUPM