lecture 5 – earth’s gravity field

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Lecture 5 – Earth’s Gravity Field GISC-3325

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Lecture 5 – Earth’s Gravity Field. GISC-3325. Schedule for next two weeks. You are responsible for material in Chapters 1-4 in text as well as all lectures and labs to date. I will miss class 6 February as well as 18 and 20 February. - PowerPoint PPT Presentation

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Page 1: Lecture 5 – Earth’s Gravity Field

Lecture 5 – Earth’s Gravity Field

GISC-3325

Page 2: Lecture 5 – Earth’s Gravity Field

Schedule for next two weeks• You are responsible for material in

Chapters 1-4 in text as well as all lectures and labs to date.

• I will miss class 6 February as well as 18 and 20 February.

• The first exam, open-book and “take-home,” will take place on either 18 or 20 February.

Page 3: Lecture 5 – Earth’s Gravity Field

Some comments on Lab 2

• It is expected that students will review the reference materials on the NGS toolkit pages and the lecture materials on the web.

• Using the XYZ Coordinate Conversion tool for question 8 is NOT correct. It computes on the ellipse NOT sphere with uniform radius.

• When transforming be aware of significant digits! We must be able to do the inverse with our answer to transform back.

Page 4: Lecture 5 – Earth’s Gravity Field
Page 5: Lecture 5 – Earth’s Gravity Field

Topics

• Definition of gravity

• Its importance to geodesy

• Measurement techniques

Page 6: Lecture 5 – Earth’s Gravity Field
Page 7: Lecture 5 – Earth’s Gravity Field

What is Geodesy?

• “Geodesy is the discipline that deals with the measurement and representation of the earth, including its gravity field, in a three-dimensional time varying space.” – definition adopted by the National Research

Council of Canada in 1973. (Vanicek, P.K. and Edward Krakiwsky, E.(1986) Geodesy: The Concepts. Elsevier).

Page 8: Lecture 5 – Earth’s Gravity Field

Another definition

• “The task of geodesy is the determination of the potential function W(x,y,z)” i.e. of the gravity potential of the Earth. – By Heinrich Bruns (1878)

• Both definitions indicate the linkages between positioning and gravity field determination.

Page 9: Lecture 5 – Earth’s Gravity Field

Integrated Geodesy

• Also called “Operational Geodesy”

• Integrated geodesy is a method in which a wide variety of surveying measurements are modeled in terms of geometric positions and the earth’s geopotential.– Both geometric and gravimetric data are

simultaneously estimated using Least Squares.

Page 10: Lecture 5 – Earth’s Gravity Field

The System of Natural Coordinates

• Axes are defined by meaningful directions: the gravity vector and of the spin axis of the Earth.

• Gravity vector defines the up-down direction– Orthogonal to a level

surface.

• There is a difference between the gravity vector and normal to ellipsoid.

Page 11: Lecture 5 – Earth’s Gravity Field

Universal Law of Gravitation

• Newton formulated the law (1687) to reflect the attraction of two point masses separated by a distance.

• f = G* [ (m*m’)/l2]– ( f is force, m and m’ are point masses, l is

distance and G is Newton’s gravitational constant)

• Currently accepted value for G – 6.67259 x 10-11m3kg-1s-2

Page 12: Lecture 5 – Earth’s Gravity Field

Gravity and Geodesy

• Defines a plumb line (local vertical) defined by gravity.

• Gravity also serves as an important reference surface. It is the level surface that is perpendicular to the plumb line at all points.

Page 13: Lecture 5 – Earth’s Gravity Field

Some unit issues

• Your textbook uses– g = 6.67259 x 10-11m3kg-1s-2

• A 1998 free-fall determination experiment (published in Science, 282, 2230-2234, 1998) determined a value for g of – (6.6873+/- 0.0094) x 10-11m3kg-1sec-2

• We will discuss the instrument used in this measurement.

Page 14: Lecture 5 – Earth’s Gravity Field

Unit of measurement

• Standard unit of measurement is the gal – named after Galileo Galilei – 1cm/sec-2

• Units are expressed as either gals or fractional parts (e.g. milligals or microgals).

Page 15: Lecture 5 – Earth’s Gravity Field

Gravitational Constant

• Geocentric gravitational constant (GM) is considered a constant.

• The value for GM accepted by the International Association of Geodesy (IAG) is:– 3 986 005 x 108m3s-2

• This equation assumes the Earth’s mass is located at a finite point (center of mass) and includes the atmosphere.

Page 16: Lecture 5 – Earth’s Gravity Field
Page 17: Lecture 5 – Earth’s Gravity Field

Absolute Gravity Meters

Mendenhall pendulum gravity meter Accuracy +/-0.6 to 5 mGals

Page 18: Lecture 5 – Earth’s Gravity Field

How does it work?

• Motion of a test mass free falling in a vacuum is interferometrically measured with respect an inertial reference.

• Controlled carriage assembly releases the test mass (a corner cube retroreflector mounted in an aluminum housing).

• The inertial reference is another corner cube retroreflector mounted on a force feedback long period (60sec) seismometer.

• Non-gravitational forces are minimized (air drag, electrostatics, and eddy current damping).

Page 19: Lecture 5 – Earth’s Gravity Field
Page 20: Lecture 5 – Earth’s Gravity Field
Page 21: Lecture 5 – Earth’s Gravity Field
Page 22: Lecture 5 – Earth’s Gravity Field
Page 23: Lecture 5 – Earth’s Gravity Field

Gravity change

• FG5 accuracy:

14

Instrument 1.1 Gals

Environmental: 1.5 Gals

Observational error: ~0.4 Gals

RMS of above at instrument height (131 cm): 1.9 Gals

RMS with relative transfer to mark or excenter: 3 to 8 Gals

• +3 Gals corresponds to -1 cm elevation change

+7½ foot rise in water-table

GPS to resolve ambiguity

• Can also measure magma insertion

sea level change (with tide record comparisons)

glacial ice mass change

Page 24: Lecture 5 – Earth’s Gravity Field

26

CHURCHILL, MANITOBA

-12

-8

-4

0

4

8

12

16

20

24

28

32

1986 1988 1990 1992 1994 1996 1998 2000 2002 2004

TIME (Yrs)

g - 9

8175

2800

µG

AL

Gravity Values

+ 95% Error Bound

- 95% Error Bound

Trend -1.91 ± 0.19 µGal/Yr

ICE-3G Theoretical (-1.11 Gal/yr)

2 cm uplift

Page 25: Lecture 5 – Earth’s Gravity Field
Page 26: Lecture 5 – Earth’s Gravity Field
Page 27: Lecture 5 – Earth’s Gravity Field
Page 28: Lecture 5 – Earth’s Gravity Field
Page 29: Lecture 5 – Earth’s Gravity Field
Page 30: Lecture 5 – Earth’s Gravity Field

Two models provide similar but not identical results. Difference is 1 mgal.

Page 31: Lecture 5 – Earth’s Gravity Field

Which model to use?

• NAVD88 - Modeled Gravity uses a model developed for the NAVD88 adjustment rather than current gravity values.

Page 32: Lecture 5 – Earth’s Gravity Field

Review of Height Systems• Helmert Orthometric• NAVD 88

• local gravity field ( )• single datum point• follows MSL

g

HC

g

C

g H

g gh

G H

0 0 4 2 41

23

.

Page 33: Lecture 5 – Earth’s Gravity Field

Earth’s Gravity Field from Space• Satellite data was

used for global models– Only useful at

wavelengths of 700 km or longer

• Lower wavelength data from terrestrial or marine gravity of varying vintage, quality and geographic coverage

Terrestrial and marine gravity data in NGS data base.

Page 34: Lecture 5 – Earth’s Gravity Field

Note the discontinuity at the shoreline.

Page 35: Lecture 5 – Earth’s Gravity Field

Gravity

• Static gravity field – Based on long-term average within Earth

system

• Temporally changing component– Motion of water and air– Time scale ranges from hours to decades.

• Mean and time variable gravity field affect the motion of all Earth space vehicles.

Page 36: Lecture 5 – Earth’s Gravity Field

Gravity Recovery And Climate Experiment

www.csr.utexas.edu/grace/gravity/

Page 37: Lecture 5 – Earth’s Gravity Field

Geoid Model from Earth Orbiting Space Vehicles (pre-GRACE)

Page 38: Lecture 5 – Earth’s Gravity Field

GRACE 111 days of data

Page 39: Lecture 5 – Earth’s Gravity Field

GRACE 363 days of data

Page 40: Lecture 5 – Earth’s Gravity Field

Orbit inclination: 89.048 degrees

Eccentricity: 0.000775

Semi-major axis: 6,849,706.754m

Distance between satellites: 222,732.810 m

Page 41: Lecture 5 – Earth’s Gravity Field
Page 42: Lecture 5 – Earth’s Gravity Field

GRACE

Page 43: Lecture 5 – Earth’s Gravity Field

How does GRACE work?

• Motion of two satellites differ because they are at different positions in space.

• When the lead SV approaches a higher gravity mass it accelerates as it moves beyond it decelerates.

• Distance changes between SVs is measured precisely.

Page 44: Lecture 5 – Earth’s Gravity Field

ITRF96/GRS-80 ellipsoid surface

global geopotential surface

NAVD 88 datum

G99

SS

S

G99

BM

Average of 52 cm

NAD 83 datum

GE

OID

99MSL

SS

T

NOTE: heights are not to scale

Page 45: Lecture 5 – Earth’s Gravity Field
Page 46: Lecture 5 – Earth’s Gravity Field