Climate model
Numerical climate models use quantitative methods to simulate the interactions of the important drivers of climate, including atmosphere, oceans, land surface and ice. They are used for a variety of purposes from study of the dynamics of the climate system to projections of future climate. Climate models may also be qualitative models and also narratives, largely descriptive, of possible futures.
Quantitative climate models take account of incoming energy from the sun as short wave electromagnetic radiation, chiefly visible and short-wave infrared, as well as outgoing long wave infrared electromagnetic. Any imbalance results in a change in temperature.
Quantitative models vary in complexity:
- A simple radiant heat transfer model treats the earth as a single point and averages outgoing energy
- This can be expanded vertically and/or horizontally
- Finally, atmosphere–ocean–sea ice global climate models solve the full equations for mass and energy transfer and radiant exchange.
- Box models can treat flows across and within ocean basins.
- Other types of modelling can be interlinked, such as land use, allowing researchers to predict the interaction between climate and ecosystems.
Box models
Simple box models, i.e. box model with a small number of boxes whose properties do not change with time, are often useful to derive analytical formulas describing the dynamics and steady-state abundance of a species. More complex box models are usually solved using numerical techniques.
Box models are used extensively to model environmental systems or ecosystems and in studies of ocean circulation and the carbon cycle.
They are instances of a multi-compartment model.
Zero-dimensional models
A very simple model of the radiative equilibrium of the Earth iswhere
- the left hand side represents the incoming energy from the Sun
- the right hand side represents the outgoing energy from the Earth, calculated from the Stefan-Boltzmann law assuming a model-fictive temperature, T, sometimes called the 'equilibrium temperature of the Earth', that is to be found,
- S is the solar constant – the incoming solar radiation per unit area—about 1367 W·m−2
- ' is the Earth's average albedo, measured to be 0.3.
- r is Earth's radius—approximately 6.371×106m
- π is the mathematical constant
- ' is the Stefan-Boltzmann constant—approximately 5.67×10−8 J·K−4·m−2·s−1
- is the effective emissivity of earth, about 0.612
Solving for the temperature,
This yields an apparent effective average earth temperature of. This is because the above equation represents the effective radiative temperature of the Earth.
This very simple model is quite instructive. For example, it easily determines the effect on average earth temperature of changes in solar constant or change of albedo or effective earth emissivity.
The average emissivity of the earth is readily estimated from available data. The emissivities of terrestrial surfaces are all in the range of 0.96 to 0.99. Clouds, however, which cover about half of the earth's surface, have an average emissivity of about 0.5 and an average cloud temperature of about. Taking all this properly into account results in an effective earth emissivity of about 0.64.
This simple model readily determines the effect of changes in solar output or change of earth albedo or effective earth emissivity on average earth temperature. It says nothing, however about what might cause these things to change. Zero-dimensional models do not address the temperature distribution on the earth or the factors that move energy about the earth.
Radiative-convective models
The zero-dimensional model above, using the solar constant and given average earth temperature, determines the effective earth emissivity of long wave radiation emitted to space. This can be refined in the vertical to a one-dimensional radiative-convective model, which considers two processes of energy transport:- upwelling and downwelling radiative transfer through atmospheric layers that both absorb and emit infrared radiation
- upward transport of heat by convection.
Effect of ice-albedo feedback on global sensitivity in a one-dimensional radiative-convective climate model.
Higher-dimension models
The zero-dimensional model may be expanded to consider the energy transported horizontally in the atmosphere. This kind of model may well be zonally 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.EMICs (Earth-system models 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 with a 3.75° × 3.75° grid and 24 vertical levels.GCMs (global climate models or general circulation models)
General Circulation Models discretise the equations for fluid motion and energy transfer and integrate these over time. Unlike simpler models, GCMs divide the atmosphere and/or oceans into grids of discrete "cells", which represent computational units. Unlike simpler models which make mixing assumptions, processes internal to a cell—such as convection—that occur on scales too small to be resolved directly are parameterised at the cell level, while other functions govern the interface between cells.Atmospheric GCMs model the atmosphere and impose sea surface temperatures as boundary conditions. Coupled atmosphere-ocean GCMs combine the two models. The first general circulation climate model that combined both oceanic and atmospheric processes was developed in the late 1960s at the NOAA Geophysical Fluid Dynamics Laboratory 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 the carbon 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."
Research and development
There are three major types of institution where climate models are developed, implemented and used:- National meteorological services. Most national weather services have a climatology section.
- Universities. Relevant departments include atmospheric sciences, meteorology, climatology, and geography.
- National and international research laboratories. Examples include the National Center for Atmospheric Research, the Geophysical Fluid Dynamics Laboratory, Los Alamos National Laboratory, the Hadley Centre for Climate Prediction and Research, the Max Planck Institute for Meteorology in Hamburg, Germany, or the Laboratoire des Sciences du Climat et de l'Environnement, France, to name but a few.
A 2012 U.S. National Research Council report discussed how the large and diverse U.S. climate modeling enterprise could evolve to become more unified. 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.
Climate models on the web
- — plot and download model data referenced by the Fourth Assessment Report of the Intergovernmental Panel on Climate Change.
- with a user-friendly interface for PCs and Macs
- CM2 global climate model info and model output data files
- based on above GFDL CM2
- : based on GFDL CM2. Complexity in-between dry models and full GCMs
- , free for download. Leading researcher was a contributing author to an IPCC report on climate change.