GLOBAL KNOWLEDGE ARK

Reference library

Foundations

Explore concepts, laws, equations and methods, with clear explanations of their use and sources. Choose an area of study or find a specific entry.

More filters

Reference entries

Showing 91–120 of 324 reference entries

Earth & cosmos · ChemistryMetamorphic assemblages and phase constraints

Metamorphism changes mineral assemblage and texture under changed pressure, temperature, fluid and deformation conditions without requiring bulk melting.

Model
Earth & cosmos · Chemistry · BiologyWeathering, soil formation and chemical export

Mechanical weathering changes fragment size; chemical weathering transforms or dissolves minerals through reactions such as hydrolysis and oxidation.

Model
Earth & cosmos · ChemistryGeochemical partition coefficients

A distribution coefficient relates one species' concentrations in two specified coexisting phases.

Model
Earth & cosmos · ChemistryBatch melting and fractional crystallization models

In homogeneous constant-D batch melting, mass balance and equilibrium give melt enrichment Cℓ/C₀=1/[D+F(1−D)].

Model
Earth & cosmosSediment entrainment, transport and deposition

Streams carry bed load, suspended material and dissolved solutes through different processes.

Model
Earth & cosmosAquifer storage, permeability and recharge

Porosity measures pore-space fraction, while hydraulic permeability/conductivity concerns connected flow under stated fluid conditions.

Model
Earth & cosmos · ChemistryGroundwater chemistry and transport context

Groundwater exchanges dissolved species with aquifer minerals and surfaces.

Model
Earth & cosmosGlacier mass balance and ice motion

Glacier accumulation and ablation determine a mass budget; an equilibrium line separates zones in the specified surface-balance picture.

Model
Earth & cosmosGlacial erosion and depositional evidence

Moving ice can abrade and pluck bedrock, while transported debris can be deposited directly as till or sorted by meltwater.

Model
Earth & cosmosGlobal and relative sea-level change

Relative sea level is water level measured against local land.

Model
Earth & cosmosAtmospheric and oceanic hydrostatic balance

When vertical acceleration is negligible, the vertical pressure gradient balances gravity: ∂p/∂z=−ρg for upward z.

Approximation
Earth & cosmosGeostrophic flow and Rossby-number scope

For sufficiently slowly varying large-scale flow away from strong friction, horizontal pressure-gradient and Coriolis accelerations can approximately balance.

Approximation
Earth & cosmosDry adiabatic motion and potential temperature

For an ideal dry gas with constant heat capacities, potential temperature θ=T(p₀/p)^(Rd/cp) is conserved in reversible adiabatic parcel motion.

Model
Earth & cosmosHumidity, condensation and clouds

Water-vapour amount and relative humidity are distinct; relative humidity compares vapour pressure with a specified saturation value at the current temperature.

Model
Earth & cosmosOcean density, stratification and mixing

Seawater density depends on temperature, salinity and pressure.

Model
Earth & cosmosWind stress and Ekman transport

In the steady idealized surface Ekman layer, vertically integrated mass transport is ME=τ×ẑ/f.

Approximation
Earth & cosmosWind-driven gyres and vorticity constraints

Spatially varying wind stress can cause Ekman convergence/divergence and force interior ocean circulation.

Model
Earth & cosmos · Chemistry · BiologyMarine carbonate speciation and exchange

Dissolved inorganic carbon includes aqueous CO₂/carbonic-acid convention, bicarbonate and carbonate.

Model
Earth & cosmosPalaeoclimate proxy and chronology inference

Natural archives such as ice, sediments, corals and tree rings record properties related to past environments.

Method
Earth & cosmosLTE excitation and ionization populations

For a classical gas in local thermodynamic equilibrium, level ratios within one ionization stage obey N_b/N_a=(g_b/g_a)exp[−(E_b−E_a)/(k_BT)].

Model
Earth & cosmosEquivalent width and spectral-line saturation

An absorption line's wavelength equivalent width is W_λ=∫[1−F_λ/F_{λ,c}]dλ, using the local continuum.

Method
Earth & cosmosDistances and lookback time in FLRW cosmology

In an expanding FLRW model with present scale factor one, the line-of-sight comoving distance is D_C=c∫₀ᶻ dz′/H(z′), and the lookback time is t_L=∫₀ᶻ dz′/[(1+z′)H(z′)].

Model
Earth & cosmosAngular and luminosity distance observables

For transparent geometrical photon propagation in FLRW cosmology, angular diameter distance is D_A=D_M/(1+z), and luminosity distance is D_L=(1+z)D_M=(1+z)²D_A.

Model
Earth & cosmosPulsation periods and stellar density

Radial stellar pulsation has a characteristic gravitational/acoustic period scale proportional to √[R³/(GM)].

Model
Earth & cosmosPlanetary equilibrium temperature model

A spherical planet intercepts stellar power over its projected disk and emits thermal power over its surface.

Model
Earth & cosmosJeans parameter and thermal escape

At an exobase radius r_ex and temperature T_ex, λ=GMm/(r_ex k_BT_ex) compares a species' binding energy with thermal energy.

Model
Earth & cosmosNewtonian tidal gradients and disruption scale

Tides arise from gravitational acceleration differences across an extended body.

Model
Earth & cosmosNearly circular galactic disk orbits

In a smooth stationary axisymmetric potential, expanding about a stable circular guiding radius R_g gives small radial oscillations at epicyclic frequency κ and vertical oscillations at ν.

Model
Earth & cosmosLocal gravitational stability of a gas disk

For a razor-thin rotating ideal fluid disk, local axisymmetric tightly wound perturbations have dispersion ω²=κ²−2πGΣ|k|+c_s²k².

Model
Earth & cosmosClosed-box galactic enrichment model

In a well-mixed closed gas-plus-star system with initially zero metallicity, instantaneous recycling and constant yield p per mass locked in long-lived stars, gas metallicity follows Z=p ln(1/μ), where μ=M_gas/M_total.

Model