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eo_handbook
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Capabilities of Earth Observation Satellites
  Atmospheric Chemistry Instruments
  Atmospheric Temperature and Humidity Sounders  
  Cloud Profile and Rain Radars  
  Earth Radiation Budget Radiometers  
  High Resolution Optical Imagers  
  Hyperspectral Imagers  
  Imaging Multi-Spectral Radiometers (vis/IR)  
  Imaging Multi-Spectral Radiometers (Passive Microwave)
  Imaging Microwave Radars  
  Lidars  
  Lightning Instruments  
  Multiple Direction/Polarisation Instruments  
  Ocean Colour Instruments  
  Radar Altimeters  
  Scatterometers  
  Gravity, Magnetic Field and Geodynamic Instruments  
Earth Observation Plans: by Measurement
 
Catalogue of Satellite Missions
 
Catalogue of Satellite Instruments
 
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Gravity, Magnetic Field and Geodynamic Instruments

Description

This category of instruments is used here to describe a variety of sensors and supporting systems used to derive information on Earth’s gravity field, magnetic field or geodynamic activity.

Gravity field measurements from space rely on one of three techniques:

— Use of single or multiple accelerometers on one or more satellites to derive gravity or gravity-gradient information;

— Precise satellite orbit determination (using satellite-to-ground navigation systems such as GPS and satellite laser ranging systems), and separation of satellite motion, induced by Earth’s gravitational force alone, from other forces (such as solar radiation and aerodynamic drag);

— Satellite-to-satellite tracking (e.g. by GPS or microwave link) to measure relative speed variations of two satellites induced by gravitational forces.

Satellite-borne magnetometers provide information on the strength and direction of Earth’s internal and external magnetic field and its time variations.

Applications

Gravity field measurements from space provide the most promising advances for improved measurement of the ‘geoid’ and its time variations. The geoid (the surface of equal gravitational potential at mean sea level) reflects the irregularities in the Earth’s gravity field at the surface due to the inhomogeneous mass and density distribution in the planet’s interior.

More accurate models of the static mean geoid and its temporal variability are vital for:

— A precise marine geoid, needed for the quantitative determination, in combination with satellite altimetry, of absolute ocean currents, their transport of heat and other properties;

— A unified global height reference system for the study of topographic processes, including the evolution of ice sheets and land surface topography;

— New understanding of the physics of Earth’s interior;

— Estimates of the thickness of the polar ice sheets and their variations through a combination of bedrock topography derived from gravity measurements and ice sheet surface topography from altimetry;
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Current & planned instruments

Gravity Precision orbit
EFI ACC
EGG DORIS-NG
GRACE instrument DORIS-NG (SPOT)
LRI EGG
MWI GOLPE
  GPS (ESA)
Magnetic field GPS Receiver (Swarm)
Advanced GGAK-M GPSP
ASM GRAS
CSC FVM INES
GGAK-E IST
GGAK-M Laser Reflectors
Magnetometer (NOAA) Laser Reflectors (ESA)
MMP LCCRA
Overhauser Magnetometer LRA
SSJ/4 LRA (LAGEOS)
SSJ/5 LRR
SSM ROSA
VFM RRA
SI
SSTI
STR
TDP



— Estimates of the mass/volume redistribution of fresh water in order to further understand the hydrological cycle;

— Improved understanding of post-glacial rebound processes on a global scale.

Magnetic field measurements are also valuable in a range of applications, including navigation systems, resource exploration drilling, spacecraft attitude control systems, assessments of the impact of ‘space weather’ caused by cosmic particles and earthquake prediction studies.

The precision location capabilities of satellite laser ranging and other systems (such as DORIS and GPS), sometimes in combination with interferometric SAR (INSAR), are applied in support of studies of crustal deformation, tectonic movements and Earth’s spin rate.


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The Swarm constellation will study the dynamics of Earth's magnetic field and its interactions with the Earth system.
   


Prior to GRACE, the long-wavelength part of Earth’s gravity field from space was determined from various tracking measurements of satellites. Only the broad geophysical features of Earth’s structure could be detected. The lower image shows the final detail available after just 1 year of GRACE data.
 
   
 
  Further Information

CHAMP: op.gfz-potsdam.de/champ/
Demeter: smsc.cnes.fr/DEMETER/index.htm
DORIS: smsc.cnes.fr/DORIS/index.htm, www.aviso.oceanobs.com/en/doris/index.html,
ids-doris.org/welcome.html
GRACE: www.csr.utexas.edu/grace
GOCE: www.esa.int/esaLP/LPgoce.html
Swarm: www.esa.int/esaLP/ESA3QZJE43D_LPswarm_0.html