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Climate model

From Wikipedia, the free encyclopedia
Quantitative methods used to simulate climate
This article is about the theories and mathematics of climate modeling. For computer-driven prediction of Earth's climate, seeGeneral circulation model.

For broader coverage of this topic, seeAtmospheric model andOceanic model.
Climate models apply knowledge in varioussciences to process extensive sets of input climate data, executingdifferential equations among grid elements in a three-dimensional model of Earth'sclimate system. The models produce simulated climates having an array of climatic and weather elements, such as heatwaves and storms. Each element may be described by several attributes, including intensity, frequency, and impacts. Climate models supportadaptation to projectedclimate change, and enableextreme event attribution to explain specific weather events.

Numericalclimate models (orclimate system models) aremathematical models that can simulate the interactions of important drivers ofclimate. These drivers are theatmosphere,oceans,land surface andice. Scientists use climate models to study the dynamics of theclimate system and to make projections of future climate and ofclimate change. Climate models can also be qualitative (i.e. not numerical) models and contain narratives, largely descriptive, of possible futures.[1]

Climate models take account of incomingenergy from the Sun as well as outgoing energy from Earth. An imbalance results in achange in temperature. The incoming energy from the Sun is in the form of short waveelectromagnetic radiation, chieflyvisible and short-wave (near)infrared. The outgoing energy is in the form of long wave (far)infrared electromagnetic energy. These processes are part of thegreenhouse effect.

Climate models vary in complexity. For example, a simpleradiant heat transfer model treats the Earth as a single point and averages outgoing energy. This can be expanded vertically (radiative-convective models) and horizontally. More complex models are the coupled atmosphere–ocean–sea iceglobal climate models. These types of models solve the full equations for mass transfer,energy transfer and radiant exchange. In addition, other types of models can be interlinked. For exampleEarth System Models include alsoland use as well asland use changes. This allows researchers to predict the interactions between climate andecosystems.

Climate models are systems ofdifferential equations based on the basic laws ofphysics,fluid motion, andchemistry. Scientists divide the planet into a 3-dimensional grid and apply the basic equations to those grids.Atmospheric models calculatewinds,heat transfer,radiation,relative humidity, and surfacehydrology within each grid and evaluate interactions with neighboring points. These are coupled withoceanic models to simulateclimate variability and change that occurs on different timescales due to shiftingocean currents and the much largerheat storage capacity of the global ocean.External drivers of change may also be applied. Including anice-sheet model better accounts for long term effects such assea level rise.

Uses

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Climate models divide the planet into a 3-dimensional grid and applydifferential equations to each grid. Climate model equations are based on the basic laws ofphysics,fluid motion, andchemistry.

Complex climate models enableextreme event attribution, which is the science of identifying and quantifying the role that human-causedclimate change plays in the frequency, intensity and impacts ofextreme weather events.[2][3] Attribution science aims to determine the degree to which such events can be explained by or linked to human-caused global warming, and are not simply due torandom climate variability[4] or naturalweather patterns.[5]

There are three major types of institution where climate models are developed, implemented and used:

Big climate models are essential but they are not perfect. Attention still needs to be given to the real world (what is happening and why). The global models are essential to assimilate all the observations, especially from space (satellites) and produce comprehensive analyses of what is happening, and then they can be used to make predictions/projections. Simple models have a role to play that is widely abused and fails to recognize the simplifications such as not including a water cycle.[6][7]

General circulation models (GCMs)

[edit]
This section is an excerpt fromGeneral circulation model.[edit]
Climate models are systems ofdifferential equations based on the basic laws ofphysics,fluid motion, andchemistry. To "run" a model, scientists divide the planet into a 3-dimensional grid, apply the basic equations, and evaluate the results. Atmospheric models calculatewinds,heat transfer,radiation,relative humidity, and surfacehydrology within each grid and evaluate interactions with neighboring points.[8]

Ageneral circulation model (GCM) is a type of climate model. It employs amathematical model of the general circulation of a planetaryatmosphere or ocean. It uses theNavier–Stokes equations on a rotating sphere withthermodynamic terms for various energy sources (radiation,latent heat). These equations are the basis for computer programs used tosimulate the Earth's atmosphere or oceans. Atmospheric and oceanic GCMs (AGCM andOGCM) are key components along withsea ice andland-surface components.

GCMs and global climate models are used forweather forecasting, understanding theclimate, and forecastingclimate change.

Atmospheric GCMs (AGCMs) model the atmosphere and imposesea surface temperatures as boundary conditions. Coupled atmosphere-ocean GCMs (AOGCMs, e.g.HadCM3,EdGCM,GFDL CM2.X, ARPEGE-Climat)[9] combine the two models. The first general circulation climate model that combined both oceanic and atmospheric processes was developed in the late 1960s at theNOAAGeophysical Fluid Dynamics Laboratory[10] AOGCMs represent the pinnacle of complexity in climate models and internalise as many processes as possible. However, they are still under development and uncertainties remain. They may be coupled to models of other processes, such as thecarbon cycle, so as to better model feedback effects. Such integrated multi-system models are sometimes referred to as either "earth system models" or "global climate models."

Versions designed for decade to century time scale climate applications were created bySyukuro Manabe andKirk Bryan at theGeophysical Fluid Dynamics Laboratory (GFDL) inPrinceton, New Jersey.[8] These models are based on the integration of a variety of fluid dynamical, chemical and sometimes biological equations.

Energy balance models (EBMs)

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Simulation of the climate system in full 3-D space and time was impractical prior to the establishment of large computational facilities starting in the 1960s. In order to begin to understand which factors may have changed Earth'spaleoclimate states, the constituent and dimensional complexities of the system needed to be reduced. A simple quantitative model that balanced incoming/outgoing energy was first developed for the atmosphere in the late 19th century.[11] Other EBMs similarly seek an economical description of surface temperatures by applying theconservation of energy constraint to individual columns of the Earth-atmosphere system.[12]

Essential features of EBMs include their relative conceptual simplicity and their ability to sometimes produceanalytical solutions.[13]: 19  Some models account for effects of ocean, land, or ice features on the surface budget. Others include interactions with parts of thewater cycle orcarbon cycle. A variety of these and other reduced system models can be useful for specialized tasks that supplement GCMs, particularly to bridge gaps between simulation and understanding.[14][15]

Zero-dimensional models

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Zero-dimensional models consider Earth as a point in space, analogous to thepale blue dot viewed byVoyager 1 or an astronomer's view of very distant objects. Thisdimensionless view while highly limited is still useful in that the laws of physics are applicable in a bulk fashion to unknown objects, or in an appropriatelumped manner if some major properties of the object are known. For example, astronomers know that most planets in our own solar system feature some kind of solid/liquid surface surrounded by a gaseous atmosphere.

Model with combined surface and atmosphere

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A very simple model of theradiative equilibrium of the Earth is

(1a)Sπr2=4πr2ϵσT4{\displaystyle (1-a)S\pi r^{2}=4\pi r^{2}\epsilon \sigma T^{4}}

where

  • the left hand side represents the total incoming shortwave power (in Watts) from the Sun
  • the right hand side represents the total outgoing longwave power (in Watts) from Earth, calculated from theStefan–Boltzmann law.

The constant parameters include

The constantπr2{\displaystyle \pi \,r^{2}} can be factored out, giving a nildimensional equation for the equilibrium

(1a)S=4ϵσT4{\displaystyle (1-a)S=4\epsilon \sigma T^{4}}

where

  • the left hand side represents the incoming shortwave energy flux from the Sun in W·m−2
  • the right hand side represents the outgoing longwave energy flux from Earth in W·m−2.

The remaining variable parameters which are specific to the planet include

This very simple model is quite instructive. For example, it shows the temperature sensitivity to changes in the solar constant, Earth albedo, or effective Earth emissivity. The effective emissivity also gauges the strength of the atmosphericgreenhouse effect, since it is the ratio of the thermal emissions escaping to space versus those emanating from the surface.[19]

The calculated emissivity can be compared to available data. Terrestrial surface emissivities are all in the range of 0.96 to 0.99[20][21] (except for some small desert areas which may be as low as 0.7). Clouds, however, which cover about half of the planet's surface, have an average emissivity of about 0.5[22] (which must be reduced by the fourth power of the ratio of cloud absolute temperature to average surface absolute temperature) and an average cloud temperature of about 258 K (−15 °C; 5 °F).[23] Taking all this properly into account results in an effective earth emissivity of about 0.64 (earth average temperature 285 K (12 °C; 53 °F)).[citation needed]

Models with separated surface and atmospheric layers

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One-layer EBM with blackbody surface

Dimensionless models have also been constructed with functionally distinct atmospheric layers from the surface. The simplest of these is thezero-dimensional, one-layer model,[24] which may be readily extended to an arbitrary number of atmospheric layers. The surface and atmospheric layer(s) are each characterized by a corresponding temperature and emissivity value, but no thickness. Applying radiative equilibrium (i.e conservation of energy) at the idealized interfaces between layers produces a set of coupled equations which are solvable.[25]

These multi-layered EBMs are examples ofmulti-compartment models. They can estimate average temperatures closer to those observed for Earth's surface and troposphere.[26] They likewise further illustrate the radiativeheat transfer processes which underlie the greenhouse effect. Quantification of this phenomenon using a version of the one-layer model was first published bySvante Arrhenius in year 1896.[11]

Radiative-convective models

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See also:radiative-convective equilibrium

Water vapor is a main determinant of the emissivity of Earth's atmosphere. It both influences the flows of radiation and is influenced by convective flows of heat in a manner that is consistent with its equilibrium concentration and temperature as a function of elevation (i.e.relative humidity distribution). This has been shown by refining the zero dimension model in the vertical to a one-dimensional radiative-convective model which considers two processes of energy transport:[27]

  • upwelling and downwelling radiative transfer through atmospheric layers that both absorb and emit infrared radiation
  • upward transport of heat by air and vapor convection, which is especially important in the lowertroposphere.

Radiative-convective models have advantages over simpler models and also lay a foundation for more complex models.[28] They can estimate both surface temperature and the temperature variation with elevation in a more realistic manner. They also simulate the observed decline in upper atmospheric temperature and rise in surface temperature whentrace amounts of other non-condensible greenhouse gases such ascarbon dioxide are included.[27]

Other parameters are sometimes included to simulate localized effects in other dimensions and to address the factors that move energy about Earth. For example, the effect of ice-albedo feedback on globalclimate sensitivity has been investigated using a one-dimensional radiative-convective climate model.[29][30]

Higher-dimension models

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The zero-dimensional model may be expanded to consider the energy transported horizontally in the atmosphere. This kind of model may well bezonally averaged. This model has the advantage of allowing a rational dependence of local albedo and emissivity on temperature – the poles can be allowed to be icy and the equator warm – but the lack of true dynamics means that horizontal transports have to be specified.[31]

Early examples include research ofMikhail Budyko andWilliam D. Sellers who worked on theBudyko-Sellers model.[32][33] This work also showed the role ofpositive feedback in the climate system and has been considered foundational for the energy balance models since its publication in 1969.[12][34]

Earth systems models of intermediate complexity (EMICs)

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Main article:Earth systems model of intermediate complexity

Depending on the nature of questions asked and the pertinent time scales, there are, on the one extreme, conceptual, more inductive models, and, on the other extreme,general circulation models operating at the highest spatial and temporal resolution currently feasible. Models of intermediate complexity bridge the gap. One example is the Climber-3 model. Its atmosphere is a 2.5-dimensional statistical-dynamical model with 7.5° × 22.5° resolution and time step of half a day; the ocean is MOM-3 (Modular Ocean Model) with a 3.75° × 3.75° grid and 24 vertical levels.[35]

Box models

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See also:multi-compartment model andconceptual model
Schematic of a simple box model used to illustratefluxes in geochemical cycles, showing a source(Q), sink(S) and reservoir(M)

Box models are simplified versions of complex systems, reducing them to boxes linked by fluxes. The boxes contain reservoirs (i.e.inventories) of species of matter and energy that are assumed to be mixed homogeneously. The concentration of any species is therefore uniform at any time within a box. However, the abundance of a species within a given box may vary as a function of time due to input flows or output flows; and may also vary due to the production, consumption or transformation of a species within the box.[36][37]

Simple box models, i.e. box model with a small number of boxes whoseextensive properties (e.g. their volume) do not change with time, are often useful to deriveanalytical formulas describing the dynamical and steady-state abundances of a species. The formulae are calledgoverning equations and are derived fromconservation laws (e.g. conservation of energy, conservation of mass, etc.). Larger sets of interacting species and equations are evaluated with numerical techniques to describe behavior of the system.[38]

Box models are used extensively to simulate environmental systems and ecosystems. In 1961Henry Stommel was the first to use a simple2-box model to study the stability of large-scaleocean circulation.[39] A more complex model has examined interactions between ocean circulation and thecarbon cycle.[40]

History

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See also:History of climate change science
This section is an excerpt fromAtmospheric model § Climate modeling.[edit]

In 1956, Norman Phillips developed a mathematical model that realistically depicted monthly and seasonal patterns in the troposphere. This was the first successful climate model.[41][42] Several groups then began working to creategeneral circulation models.[43] The first general circulation climate model combined oceanic and atmospheric processes and was developed in the late 1960s at theGeophysical Fluid Dynamics Laboratory, a component of the U.S.National Oceanic and Atmospheric Administration.[44]

By 1975, Manabe and Wetherald had developed a three-dimensionalglobal climate model that gave a roughly accurate representation of the current climate. Doubling CO2 in the model's atmosphere gave a roughly 2 °C rise in global temperature.[45] Several other kinds of computer models gave similar results: it was impossible to make a model that gave something resembling the actual climate and not have the temperature rise when the CO2 concentration was increased.

By the early 1980s, the U.S.National Center for Atmospheric Research had developed the Community Atmosphere Model (CAM), which can be run by itself or as the atmospheric component of theCommunity Climate System Model. The latest update (version 3.1) of the standalone CAM was issued on 1 February 2006.[46][47][48] In 1986, efforts began to initialize and model soil and vegetation types, resulting in more realistic forecasts.[49] Coupled ocean-atmosphere climate models, such as theHadley Centre for Climate Prediction and Research'sHadCM3 model, are being used as inputs forclimate change studies.[43] Meta-analyses of past climate change models show that they have generally been accurate, albeit conservative, under-predicting levels of warming.[50][51]

Increase of forecasts confidence over time

[edit]
The pattern correlation between global climate models and observations has improved over sequential CMIP phases 3, 5, and 6.[52]

TheCoupled Model Intercomparison Project (CMIP) has been a leading effort to foster improvements in GCMs and climate change understanding since 1995.[53][54]

The IPCC stated in 2010 it has increased confidence in forecasts coming from climate models:

"There is considerable confidence that climate models provide credible quantitative estimates of future climate change, particularly at continental scales and above. This confidence comes from the foundation of the models in accepted physical principles and from their ability to reproduce observed features of current climate and past climate changes. Confidence in model estimates is higher for some climate variables (e.g., temperature) than for others (e.g., precipitation). Over several decades of development, models have consistently provided a robust and unambiguous picture of significant climate warming in response to increasing greenhouse gases."[55]

Coordination of research

[edit]

TheWorld Climate Research Programme (WCRP), hosted by theWorld Meteorological Organization (WMO), coordinates research activities on climate modelling worldwide.

A 2012U.S. National Research Council report discussed how the large and diverse U.S. climate modeling enterprise could evolve to become more unified.[56] Efficiencies could be gained by developing a common software infrastructure shared by all U.S. climate researchers, and holding an annual climate modeling forum, the report found.[57]

Issues

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Electricity consumption

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Cloud-resolving climate models are nowadays run on high intensitysuper-computers which have a high power consumption and thus cause CO2 emissions.[58] They requireexascale computing (billion billion – i.e., a quintillion – calculations per second). For example, theFrontier exascale supercomputer consumes 29 MW.[59] It can simulate a year’s worth of climate at cloud resolving scales in a day.[60]

Techniques that could lead to energy savings, include for example: "reducing floating point precision computation; developing machine learning algorithms to avoid unnecessary computations; and creating a new generation of scalable numerical algorithms that would enable higher throughput in terms of simulated years per wall clock day."[58]

Parametrization

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This section is an excerpt fromParametrization (atmospheric modeling).[edit]
Parametrization (or parameterization) in anatmospheric model (eitherweather model or climate model) is a method of replacing processes that are too small-scale or complex to be physically represented in the model by a simplified process. This can be contrasted with other processes—e.g., large-scale flow of the atmosphere—that are explicitly resolved within the models. Associated with these parametrizations are variousparameters used in the simplified processes. Examples include the descent rate of raindrops, convective clouds, simplifications of the atmosphericradiative transfer on the basis ofatmospheric radiative transfer codes, andcloud microphysics. Radiative parametrizations are important to both atmospheric and oceanic modeling alike. Atmospheric emissions from different sources within individual grid boxes also need to be parametrized to determine their impact onair quality.

See also

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References

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