Lecture 1 May 3rd 2006 Wednesday: 16:00-17:30 Rocco Malservisi: e-mail...
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Transcript of Lecture 1 May 3rd 2006 Wednesday: 16:00-17:30 Rocco Malservisi: e-mail...
Lecture 1 May 3rd 2006
Wednesday: 16:00-17:30
Rocco Malservisi: e-mail [email protected] 21804202
Class Web page: www.geophysik.lmu.de/~malservisi/TectGPS.html
Lecture 1 May 3rd 2006
“Geodesy is the branch of applied
mathematics concerned with the
determination of the size and shape of
the Earth, with the exact positions of
points on its surface, and with the
description of variations of its gravity
field.”International Association of Geodesy definition
From Greek: “ DIVIDING THE EARTH ”`
Lecture 1 May 3rd 2006
How big is the Earth?
Which is the shapeof the planet?
How tall is a mountain?
Where my property ends? How big is my property?
Where am I?
How far am I from a place?
In which direction should I go?
Lecture 1 May 3rd 2006
If we want to have a mathematical representation of a point (point’s coordinate) we need to have a reference surface we can refer to.
Knowing the shape of the Earth we can define this surface.
The gravity field gives the best representation of the shape of the Earth.
Lecture 1 May 3rd 2006
The Earth is “almost” a sphere with a circumference ~40000 km longThe meter was defined using this length.
Lecture 1 May 3rd 2006
Eratosthenes (215 BC)
R~ 6267 km
S=4400 stadia ~787kmC=39376km
Lecture 1 May 3rd 2006
XVII XVIII Century Discussion of Oblate-Prolate spheroid
Cassini meridian south of France shorter than in ParisPROLATE
British Pendulum slower at equator and Newton equationsOBLATE
XVIII Century (1730) Expedition of France Academy:Peru measurement: 6376.45 km (Equatorial Radius)Lapland measurement: 6355.88 km (Polar Radius)OBLATE!!Difference: 1350m in 111km!!!
Lecture 1 May 3rd 2006
The Earth is “almost” a sphere with a circumference ~40000 km longThe meter was defined using this length.
Better approximate by an oblate ellipsoid
Today accepted Value Equatorial Radius 6378 kmPolar Radius 6357 kmSphere of Equal Volume Radius 6371 kmFlattening 1/298.257223563
Lecture 1 May 3rd 2006
The “real” shape of the planet is approximated by the Geoid:THE EQUIPOTENTIAL SURFACE AT THE MEAN SEA LEVEL
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Lecture 1 May 3rd 2006
We can divide geodesy
Space Geodesyuse of extra-terrestrialobject as observable.
Terrestrial GeodesyUse of terrestrial toolsAnd observable
Global GeodesyDetermination of shape of the Earth, global references.Geodetic SurveyDetermination of positions,and references over a regionfor which the Earth’s curva-ture can have influences.Plane SurveyDetermination of positions and references on a local level.
According to method
OR
According to what we observe
Lecture 1 May 3rd 2006
TRADITIONAL SURVEY
Horizontal positioning Vertical positioning
TRIANGULATION
TRILATERATION
TRAVERSING
ASTRONOMICALPOSITIONING
GEODETIC LEVELING
TRIGONOMETRIC HEIGHTING
BAROMETRIC LEVELING
TILTING
Lecture 1 May 3rd 2006
TRADITIONAL SURVEY
Horizontal positioning
TRIANGULATION
Lecture 1 May 3rd 2006
TRADITIONAL SURVEY
Horizontal positioning
TRILATERATION
Lecture 1 May 3rd 2006
TRADITIONAL SURVEY
Horizontal positioning
TRAVERSE
EDM
Lecture 1 May 3rd 2006
TRADITIONAL SURVEY
Vertical positioning
GEODETIC LEVELING
TRIGONOMETRIC HEIGHTING
Lecture 1 May 3rd 2006
SPACE SURVEY
VLBI Very Long Baseline Interferometry
SLR Satellite Laser Ranging
GPS Global Positioning System Glonass Galileo
DORIS
InSAR Interferometric Synthetic Aperture Radar
Lecture 1 May 3rd 2006
Very Long Baseline Interferometry
VLBI is a geometric technique: • It measures the time difference
between the arrival at two Earth-based antennas of a radio wavefront emitted by a distant quasar.
• Using large numbers of time difference measurements from many quasars observed with a global network of antennas, VLBI determines the inertial reference frame defined by the quasars and simultaneously the precise positions of the antennas.
Lecture 1 May 3rd 2006
SLR Satellite Laser Ranging
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QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture.
Lecture 1 May 3rd 2006
The Global Positioning System• The Global Positioning System (GPS) is
a satellite-based navigation system.• GPS was originally intended for military applications, but in the
1980s, the government made the system available for civilian use.• GPS works in any weather conditions, anywhere in the world, 24
hours a day. There are no subscription fees or setup charges to use GPS
• Some civilian uses:– Navigation on land, sea, air
and space– Geophysics research– Guidance systems– Geodetic network densification– Hydrographic surveys
• The Global Positioning System (GPS) is a satellite-based navigation system.
• GPS was originally intended for military applications, but in the 1980s, the government made the system available for civilian use.
• GPS works in any weather conditions, anywhere in the world, 24 hours a day. There are no subscription fees or setup charges to use GPS
• Some civilian uses:– Navigation on land, sea, air
and space– Geophysics research– Guidance systems– Geodetic network densification– Hydrographic surveys
Lecture 1 May 3rd 2006
GlonassGlonass GLObal NAvigation Satellite System
Glonass is a Soviet space-based navigation system comparable
to the American GPS system.
The operational system contains 21 satellites in 3 orbital planes,
with 3 on-orbit spares.
Glonass provides 100 meters accuracy with its C/A
(deliberately degraded) signals and 10-20 meter accuracy with
its P (military) signals.
Lecture 1 May 3rd 2006
Doppler Orbitography and Radio positioning Integrated by Satellite
Precise orbit determination and location system using Doppler shift measurement techniques. A global network of 52 Doris orbitography beacons has been deployed. Doris was developed by Cnes, the French space agency, and is operated by CLS.
DORIS
Lecture 1 May 3rd 2006
• Two or more data acquisition of the same area from nearby location (< 1000 m)
• Enables detection of surface changes within cm level accuracy
InSAR
Lecture 1 May 3rd 2006