Earth science
Earth’s magnetic field
The dynamo, the dipole, inclination and declination, paleomagnetism and seafloor stripes.
Basics
The geodynamo
Liquid iron in the outer core moves with convection and rotation and sustains current and field — a dynamo. Internal heat and buoyancy of light elements drive the flow. Intensity wanders over millennia; poles sometimes reverse. A bar-magnet Earth is only a first sketch; real fields have higher multipoles and a westward drift.
Dipole and inclination
At the surface the main part is a tilted dipole. Inclination is the angle of field lines to the horizontal: steep near the magnetic poles, near 0 at the magnetic equator. Declination is the offset between true north and magnetic north. Navigation and field geology use local declination charts. Regions such as the South Atlantic Anomaly are weaker than a pure dipole.
Paleomagnetism
Magnetic minerals can lock the field as lava cools or sediment settles. Ancient inclination hints at the latitude of that continent. Seafloor stripes record normal and reversed field as crust is born at a ridge. That is independent evidence that plates move. Remagnetisation and tilt corrections keep interpretations honest.
Magnetosphere
The solar wind compresses Earth’s field on the dayside and stretches a tail on the night side. Charged particles are trapped in the Van Allen belts; spilling into the polar atmosphere makes aurora. Strong solar storms shake field and ionosphere and can disturb radio, satellites, and grids. A world such as Mars, with a weak global field, leaves more atmosphere exposed to the solar wind. For space-weather advice, follow official alerts.
Formulas
Dipole field (on axis, sketch)
Moment μ, distance r. Earth’s dipole is tilted and slightly offset.
Symbols
-
μmagnetic moment -
rdistance from the centre
Dipole inclination
Magnetic latitude λ_m. I → 90° at the magnetic pole.
Symbols
-
Iinclination -
λ_mmagnetic latitude
Cyclotron frequency
Gyrofrequency of a charge in B. Van Allen sketch.
Symbols
-
qcharge -
Bmagnetic field -
mmass
Key table
| Surface |B| | roughly 25–65 μT, larger toward the poles |
|---|---|
| Magnetic north | not true north; wanders year to year |
| Brunhes | present normal chron; last major reversal ~0.78 Ma |
In this field
Rocks and plate tectonics
Rock cycle, earthquakes, volcanoes, plate boundaries.
Atmosphere and weather
Layers, wind, clouds, fronts.
Oceans, climate, time
Currents, carbon, climate vs weather, relative and absolute age.
Minerals and water
Minerals and Mohs, water cycle, groundwater, soil.
Hazards and resources
Volcanoes, slides, storms; fuels and ores.
Geologic time and carbon
Relative and absolute ages, the carbon cycle.
Weathering, soil, and the water cycle
Weathering, erosion, soil profiles, and the water cycle.
Glaciers and sea level
Glacier budget, isostasy, sea level, and glacial deposits.
Groundwater
Porosity, permeability, water table, Darcy, aquifers and aquitards.
Seismic waves
P, S, and surface waves, travel-time curves, magnitude, and Earth’s interior sketch.