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Geophysics & Earth models

Showing 1–30 of 48 reference entries

Earth & cosmosEarthquake slip, elastic rebound and aseismic deformation

A tectonic earthquake involves sudden slip on a fault and release of part of the surrounding rock's stored elastic energy, including energy radiated as seismic waves.

Empirical finding
Earth & cosmosEffective normal stress and a Coulomb slip threshold

In a compression-positive Coulomb model for a closed fault, effective normal traction is σ′_n=σ_n−p.

Model
Earth & cosmosScalar seismic moment and moment magnitude

For a planar shear-fault source with uniform shear modulus μ and consistently directed slip magnitude D, scalar moment is M₀=μAD̄, equivalently μ∫_A D dA.

Model
Earth & cosmosP and S speeds in an isotropic elastic solid

For a homogeneous isotropic linearly elastic solid of densityρ, P waves have vP²=(λ+2μ)/ρ=(K+4μ/3)/ρ and S waves have vS²=μ/ρ.

Model
Earth & cosmosSeismic rays, interface refraction and travel time

In a high-frequency ray model, travel time along a pathγ is t=∫_γ ds/v.

Model
Earth & cosmosDirect, reflected and head-wave travel-time models

For source and receiver on a flat surface a horizontal distance x apart above a uniform layer of depth h and speed v₁, direct travel time is x/v₁ and reflection from its horizontal base has time 2√(h²+x²/4)/v₁.

Method
Earth & cosmosReference gravity, elevation and Bouguer corrections

A gravity anomaly is an observed/modelled field difference relative to a stated reference and correction convention.

Model
Earth & cosmosGravity forward models for a buried line and strip

For an infinite line parallel to y at horizontal coordinate x₀ and depth b>0 with signed excess mass per lengthm_l, its downward surface anomaly is Δg=2Gm_lb/[(x−x₀)²+b²].

Method
Earth & cosmosNonuniqueness and resolution in gravity inference

Different subsurface density structures can yield the same external gravitational field.

Method
Earth & cosmosConductive heat diffusion and a thermal length scale

For stationary homogeneous material with constant positiveρ,c_p andk, no internal heat production and one-dimensional conduction, ρc_pT_t=kT_zz, with thermal diffusivityκ=k/(ρc_p).

Model
Earth & cosmosSteady geotherm with internal heat production

With depthz positive downward, constant conductivityk and uniform volumetric heat productionH, a stationary conductive slab obeys kT_zz+H=0.

Model
Earth & cosmosHalf-space cooling of an ideal lithosphere

For z>0 initially at uniform T_i and a surface held at T_s for t>0, constant-κ conduction gives T(z,t)=T_s+(T_i−T_s)erf[z/(2√(κt))].

Model
Earth & cosmosPassive and active Earth-observation signals

Passive sensors receive externally supplied or naturally emitted radiation; active radar/lidar supplies illumination and measures its return.

Method
Earth & cosmosDigital values, TOA radiance and reflectance

For the specified Landsat Level-1 product, metadata supplies band-specific rescaling L_λ=M_LQ_cal+A_L and uncorrected planetary reflectanceρ′=M_ρQ_cal+A_ρ.

Method
Earth & cosmosThermal brightness temperature and surface-temperature limits

A Landsat thermal-band TOA radianceL_λ>0 maps to product brightness temperature T_B=K₂/ln(K₁/L_λ+1), using its band-specific metadata constants.

Method
Earth & cosmosNDVI as a calibrated spectral ratio

For compatible near-infrared and red surface-reflectance bands, NDVI=(ρ_NIR−ρ_R)/(ρ_NIR+ρ_R).

Method
Earth & cosmosPulse ranging, elevation geometry and a DEM

For a monostatic pulse with corrected round-trip delayτ and constant propagation group speedv_g, one-way slant range is R=v_gτ/2.

Method
Earth & cosmosOcean colour and an empirical chlorophyll retrieval

Ocean-colour band-ratio models estimate near-surface chlorophyll-a from water-leaving remote-sensing reflectances.

Method
Earth & cosmosResolved fault traction and the Mohr construction

LetΣ be the symmetric compression-positive stress tensor, the negative of tensile-positive Cauchy stress.

Method
Earth & cosmosAndersonian stress regimes and faulting

In an Andersonian idealization, one principal stress axis is vertical and two are horizontal.

Model
Earth & cosmosEnergy balance for brittle crack extension

In a quasistatic elastic fracture model, crack extension releases mechanical potential energy at rateG=−∂Π/∂A per projected crack area.

Model
Earth & cosmosInduced/remanent magnetization and a total-field anomaly

A weak-field linear isotropic rock model separates magnetizationM=M_r+χH into retained remanence and an induced response to localH.

Method
Earth & cosmosBayesian geophysical inverse problems

An inverse solution is a posterior distribution conditioned on observations, a forward operator, likelihood and prior.

Method
Earth & cosmosEnsemble data assimilation

Ensemble assimilation estimates forecast-error covariances from model realizations and updates the state using observations and their error model.

Method
Earth & cosmosClimate detection, attribution and model evaluation

Fingerprinting compares observed patterns with simulated responses to specified forcing and internal-variability covariance.

Method
Earth & cosmosReal seawater thermodynamics and density

TEOS-10 seawater calculations distinguish Absolute Salinity, Conservative Temperature and sea pressure.

Method
Earth & cosmosNonlinear seawater mixing and cabbeling

Mixing waters can change density through nonlinear temperature/salinity dependence even when each source has the same density at the reference pressure.

Method
Earth & cosmosNonideal mineral phase equilibrium

A mineral assemblage at specified pressure, temperature and bulk composition minimizes Gibbs energy subject to component balance.

Method
Earth & cosmosMineral thermodynamic databases and elastic inference

Combining mineral phase fractions with elastic properties can predict seismic velocities, but equilibrium databases and shear-modulus data have separate calibration domains.

Method
Earth & cosmosIce enthalpy and thermal-rheological coupling

Ice thermal models combine advection, diffusion and deformation heating; enthalpy tracks sensible heat and liquid fraction at the pressure-melting boundary.

Method