GLOBAL KNOWLEDGE ARK

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Showing 1–30 of 324 reference entries

Physics · Earth & cosmosNewtonian gravitation

An inverse-square force models attraction between point masses.

Model
Earth & cosmosRock cycle and geological transformation

Rock materials can change through multiple geological pathways.

Model
Earth & cosmosPlate tectonics

Moving lithospheric plates organize many large-scale geological processes.

Model
Earth & cosmosEarth's water cycle

Water moves among reservoirs above, on and below Earth's surface.

Model
Earth & cosmos · Biology · ChemistryEarth's carbon cycle

Carbon moves through biological, oceanic, atmospheric and geological reservoirs.

Model
Earth & cosmosPlanetary radiative energy balance

Earth's energy storage changes when incoming and outgoing energy differ.

Model
Earth & cosmosAtmospheric greenhouse effect

Infrared absorption and emission affect how Earth loses heat to space.

Model
Earth & cosmosWeather, climate and their time scales

Weather describes short-term conditions; climate describes their longer-term patterns.

Definition
Earth & cosmosOrbits as gravitational motion

An orbiting body can remain in continuous gravitational free fall.

Model
Earth & cosmosStellar fusion and evolution

Main-sequence stars release energy by fusing hydrogen into helium.

Model
Earth & cosmosHot Big Bang and the cosmic microwave background

Expansion and relic radiation support an earlier hot, dense Universe.

Model
Physics · Earth & cosmosFriedmann cosmological evolution

Homogeneity and isotropy reduce gravitational expansion to two balances.

Model
Physics · Earth & cosmosNuclear binding energy

A bound nucleus has less rest mass than its separated nucleons.

Model
Physics · Earth & cosmosExponential radioactive decay

A fixed decay probability per time gives a population timescale.

Model
Physics · Earth & cosmosFission, fusion and reaction energy

Nuclear rearrangement can release or require energy.

Model
Earth & cosmosMinerals, structure and diagnostic properties

Mineral identification combines structural and physical evidence.

Method
Earth & cosmosRadiometric ages and sample history

Isotopic measurements estimate an age only with a suitable geological model.

Method
Earth & cosmosSeismic constraints on Earth's interior

Wave travel, refraction and transmission constrain an interior model.

Method
Earth & cosmosThe geodynamo model

Fluid motion in the outer core maintains much of Earth's magnetic field.

Model
Earth & cosmosWater budgets and storage change

A defined area's water storage changes with total inflow and outflow.

Model
Earth & cosmosDarcy flux and hydraulic conductivity

Groundwater flow is often approximately linear in hydraulic-head gradient.

Approximation
Earth & cosmosOcean circulation and overturning

Wind, buoyancy changes and mixing contribute to ocean transport.

Model
Earth & cosmosGlobal atmospheric circulation

Unequal heating and rotation organize broad circulation patterns.

Model
Earth & cosmosClimate forcing and energy-budget perturbations

External changes can disturb climate's radiation budget.

Definition
Earth & cosmosClimate feedback mechanisms

Climate responses can amplify or damp a change.

Model
Earth & cosmosClimate detection and attribution methods

Attribution compares observed changes with plausible drivers and variability.

Method
Earth & cosmosStellar evolution and fuel stages

Stellar structure changes as core fuel and conditions change.

Model
Earth & cosmosWhite dwarfs, neutron stars and stellar black holes

Different evolutionary outcomes leave different compact remnants.

Model
Earth & cosmosAnnual stellar parallax and distance

Changing observing position permits geometric distance inference.

Method
Earth & cosmosCosmological redshift and distance inference

Spectral stretching carries expansion information but is not one universal distance ruler.

Method
ModelSource checked

Global atmospheric circulation

Earth & cosmos

Unequal heating and rotation organize broad circulation patterns.

Key knowledge

Unequal solar heating and Earth's rotation help organize atmospheric circulation. Tropical rising motion and subtropical descent form a broad Hadley circulation, while prevailing winds and other circulation patterns redistribute heat and moisture. Storms and regional geography modify the broad pattern.

Conditions and scope

  • A three-cell diagram describes a broad average, not three steady closed loops present everywhere.
  • Coriolis deflects moving air in a rotating frame; circulation also requires pressure gradients and energy exchanges.
Sources · 1

References

Sources retain their recorded scope. A source link alone does not establish verification of every statement.

  1. A Global Look at Moving Air: Atmospheric CirculationUniversity Corporation for Atmospheric Research (UCAR), Center for Science EducationTeaching resourcescied.ucar.eduRead source

Evidence and review

UCAR uneven-heating, rotating-Earth and circulation-cell explanation.

2026-10-10 · Checked conceptual large-scale scope without a local weather prediction.

Entry detailsPermanent link to this entry ↗
Record identity
earth-atmospheric-circulation
Revision
university-reference.1
Structured reference record
University reference