Core Modeling Concepts

The fundamental principles that make climate models work

How Models Represent Climate

1. Spatial Resolution: The Climate Grid

Climate models divide Earth into a 3D grid of cells. Each cell represents averages over that area - temperature, wind, humidity, etc. Higher resolution (smaller cells) captures more detail but requires exponentially more computing power.

Interactive: Adjust Model Resolution

Grid Cells: 8×8
Higher Resolution
More detail, slower computation
Lower Resolution
Less detail, faster runs

2. Temporal Resolution: Time Steps

Models advance in small time increments (typically 15-30 minutes for atmosphere, hours for ocean). At each step, they calculate how conditions change based on physics laws. Running 100 years of simulation can take months of supercomputer time.

Interactive: Watch Time Steps

Time Step: 1 / 24
Each step = 1 hour

Models calculate atmospheric conditions hour by hour, updating temperature, wind, humidity, and other variables at each step based on physics equations.

3. Physics-Based Equations

Fundamental Laws

  • • Conservation of energy
  • • Conservation of momentum
  • • Conservation of mass
  • • Thermodynamic principles

Climate Processes

  • • Radiation transfer
  • • Fluid dynamics
  • • Phase changes (ice/water)
  • • Chemical reactions

⚙️Parameterization: Representing Small-Scale Processes

Some processes (clouds, turbulence) happen at scales smaller than grid cells. Models use "parameterization" - simplified representations based on larger-scale conditions. This is a major source of uncertainty.