Geodesy Class
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Transcript of Geodesy Class
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Geodesy
Geodesist
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Geodesy
Geodesist
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Geodesy
Geodesist
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Space Space Geodesy
NASA (NationalAeronautics and Space
Administration)
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(Space Geodesy)
Satellite tracking ()
Satellite laser ranging
Very-Long Baseline Interferometry VLBI
GPS/Glonass/Galileo
Satellite altimetry
Imaging lidar
Satellite-satellite tracking
Synthetic aperture radar SAR
Interferometric SAR (InSAR)
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An early space geodesy
experiment by Eratosthenes (2200
years ago) to measure the Earth:
Spherical Earth assumption
Gravity (vertical/radial)
Astronomical reference (sunlight)
Time synchronism
Terrestrial distance
Mathematics
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Humans first satellite,
Sputnik I,
USSR,
October 4, 1957
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Sputnik 1, 1957
Satellite nodal precession
(around an oblate Earth)
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GEO
LEOMEO
A Snapshot of the hundreds of Earths artificial satellites:
LEO = low Earth orbit; MEO = medium Earth orbit; GEO = geosynchronous
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QuickTime and adecompressor
are needed to see this picture.
Satellitestracked by theLaser Ranging
network (inaddition to theMoon)
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BASELINE
Distant quasar
VLBI: very-long-baseline interferometry
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Tectonic Plate motion Velocity Fielddetermined by 2 decades of space geodesy measurements
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Earth Rotation
Orientation
Nutations (w.r.t. space)
Polar motion (w.r.t. Earth) Speed
Length-of-day/UT1
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10-DAY MISSION; 159 ORBITS
(NOT INCLUDING CALIBRATION OCEAN DATATAKES)Objective: Digital terrain data of the EarthLandmass.
One arc-sec (30 meter) posting
10 meter relative height resolution
16 meter absolute height resolution
Mosaickable terrain-corrected geocoded
images
QuickT ime and aGIF decompressor
are needed to see this picture.
QuickTime and a
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QuickTime and a
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Venus:
run-away
greenhouseeffect
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Venus Orbiting
Imaging Radar
on Magellan,19901994 (burnt
in atmosphere)
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QuickTime and adecompressor
are needed to see this picture.
THE TOPOGRAPHY OF MARS (MOLA data)
MOLA SCIENCE & INSTRUMENT TEAMS
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QuickTime and adecompressor
are needed to see this picture.
ICESAT LASER ALTIMETER
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ICESat first days work (2/20/2003)
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TOPEX/Poseidon
(NASA/CNES; 1992-2005)
Jason-1 / Jason II(CNES/NASA; 2002 - )
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Sea Level Variations
= geoid (gravitational equi-potential surface)
+ more water (melting of land ice/glaciers, dams, etc.)
+ steric effects (thermal+salinity effects)
+ tides
+ dynamic height (wind-driven and thermohaline-drivencurrents)
+ inverted barometer & loading (pressure-driven effects )
+ waves (wind-driven, planetary, tsunami, )
Everywhere
On all time scales
For a variety of reasons
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Satellite ocean altimetry derived Gravity Field
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Surface Ocean Currents
(driven by prevailing wind field and under geostrophy)
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El Nio (11/1997) La Nia (10/1998)
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QuickTime and adecompressor
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M2 Lunar Tide in the Ocean
(GOT99, courtesy R. Ray)
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2007IPCC
mm
IPCC 2007
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Global Sea Level Rise From Topex/Poseidon(courtesy S. Nerem)
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GRACE (Gravity Recovery And Climate Experiment)
St ti G it A l
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4 Decades of tracking to geodetic satellites 111 days of GRACE data
13 months of GRACE data
Static Gravity Anomaly
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COSMIC
constellation:
6 satellites
6 orbits:
800 km altitude
71 inclination
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P
GPS
GPS
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Interferometric SAR Observations
Earthquakes
Operational Constellations
for Plate Boundary ScaleVector Measurements
PBO
Northridge, CA
Site-specific, Irregular
Scalar Measurements
Hector Mine, CA
Greenland
Volcanoes
Long Valley, CA
Stress Change
Ice Sheets
GEODETIC IMAGING LIDAR Canopy Top Digital Surface Bald Earth Digital Terrain
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CANOPY HEIGHT CANOPY TOP
BALD EARTH USGS 10m DEM
GEODETIC IMAGING LIDARat a variety of scales
GLOBAL REGIONAL LOCAL
Canopy Top Digital Surface, Bald Earth Digital TerrainModels compared to USGS DEM
Terrapoint 1 8m Shaded Relief
Tacoma
Terrapoint 1.8m Shaded Relief
Mapping Mount Rainier Hazards withHigh Resolution LIDAR
500 m pixels 20 m pixels 2 m pixels
MOLA/MGS VCL Simulation SENH Airborne
Tacoma is downslope from Mount Ranierand inline for possible lahars triggeredb l i lti f k