Gravity, Magnetic And Geodynamic Measurements Measurements

Measurements > Gravity and Magnetic Fields > Gravity, Magnetic and Geodynamic measurements
The geoid is the surface of equal gravitational potential at mean sea level, and reflects the irregularities in the Earth’s gravity field at the planet’s surface caused by the inhomogeneous mass and density distribution in the interior. Such measurements are vital for quantitative determination – in combination with satellite altimetry – of ocean currents, improved global height references, estimates of the thickness of the polar ice sheets and its variations, and estimates of the mass/volume redistribution of fresh water in order to better understand the hydrological cycle.
Detailed MeasurementDescriptionInstrumentsTimeline
Auroral EmissionsA highly sensitive camera that collects photons radiated by auroral processes.
3 instruments
Timeline for Auroral Emissions
Crustal MotionChanges in time of the position and height of the Earth’s plates. Indicative of the lithosphere dynamics, thus useful for earthquake prediction - Physical unit: [ mm/y ] - Accuracy unit: [ mm/y ].
9 instruments
Timeline for Crustal Motion
Crustal plates positioningBasic for monitoring the evolution of the lithosphere dynamics - Physical unit: [ cm ] - Accuracy unit: [ cm ].
4 instruments
Timeline for Crustal plates positioning
Electric Field (vector)An instrument that measures the intensity and direction of the electric field.
1 instrument
Timeline for Electric Field (vector)
Electron density profileVertical profile of the electron density in the ionosphere and plasmasphere - Physical unit: [ electrons/m3] - Accuracy unit: [ % ].
4 instruments
Timeline for Electron density profile
Electron Energy and Pitch Angle DistributionElectrons spiral around magnetic field lines, and their motion is described by their velocity along the local magnetic field and perpendicular to it. The pitch angle is derived from the ratio of those two velocities and can predict which electrons will precipitate in the ionosphere to produce the aurora and which will be reflected back along the magnetic field line.
2 instruments
Timeline for Electron Energy and Pitch Angle Distribution
GeoidEquipotential surface which would coincide exactly with the mean ocean surface of the Earth, if the oceans were in equilibrium, at rest, and extended through the continents (such as with very narrow channels) - Physical unit: [ cm ] - Accuracy unit: [ cm ].
7 instruments
Timeline for Geoid
Gravity fieldIndicative of the statics and dynamics of the lithosphere and the mantle - Physical unit: [ mGal ] (1 Gal = 0.01 m/s2. i.e. 1 mGal ≈ 10-6 g0 . “Gal” stands for Galileo) - Accuracy unit: [ mGal ].
14 instruments
Timeline for Gravity field
Gravity gradientsGradient of the Earth’s gravity field measured at the satellite orbital height - Physical unit: [ E ] , Eötvös (1 E = 1 mGal / 10 km) - Accuracy unit: [ E ].
4 instruments
Timeline for Gravity gradients
Ion Density, Drift Velocity, and TemperatureAn instrument that measures the amount of ions encountered by the spacecraft, and attempts to deflect them to assess their velocity and temperature.
4 instruments
Timeline for Ion Density, Drift Velocity, and Temperature
Magnetic field (scalar)[Unit of measurement – n tesla]
7 instruments
Timeline for Magnetic field (scalar)
Magnetic field (vector) [Unit of measurement - n tesla]
12 instruments
Timeline for Magnetic field (vector)
Neutral Particle Composition and Flow VelocityA directional instrument that measures the amount of neutrals encountered by the spacecraft.
1 instrument
Timeline for Neutral Particle Composition and Flow Velocity
Total electron content (TEC)Number of electrons in between two points. Observed under more viewing angles so as to generate profiles by tomography - Physical unit: [ electrons/m2 ]; practical unit: TECU = 1016 electrons/m2 - Accuracy unit: [ % ].
6 instruments
Timeline for Total electron content (TEC)
ULF-HF Electromagnetic WavesRadio receiver instrument, recording the wave received from the ground or other spacecraft, to determine how it was modified by its travel through the ionosphere.
1 instrument
Timeline for ULF-HF Electromagnetic Waves