Lecture 5 – Earth’s Gravity Field

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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

Transcript of Lecture 5 – Earth’s Gravity Field

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.

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

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.

Topics

• Definition of gravity

• Its importance to geodesy

• Measurement techniques

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).

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.

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.

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.

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

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.

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.

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).

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.

Absolute Gravity Meters

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

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).

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

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

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

Which model to use?

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

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

.

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.

Note the discontinuity at the shoreline.

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.

Gravity Recovery And Climate Experiment

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

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

GRACE 111 days of data

GRACE 363 days of data

Orbit inclination: 89.048 degrees

Eccentricity: 0.000775

Semi-major axis: 6,849,706.754m

Distance between satellites: 222,732.810 m

GRACE

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.

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