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Climate Change: An Inter-disciplinary Approach to Problem Solving��How do I build a climate model?

Richard B. Rood

rbrood@umich.edu

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Winter 2021

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Modeling Resources

  • Modeling is hard to teach and hard to communicate.
  • However, we use models all the time. Sometimes we don’t even realize that. It is how we understand things, how we think about things.
  • Please refer to other resources provided on modeling for more introductory material.

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What do we do?

  • We develop climate models based on the conservation of energy and mass and momentum, the fundamental ideas of classical physics. (Budget equations)
    • We are going to identify the sources (production) and the sinks (losses)
      • Things that absorb and things that reflect

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What do we do?

  • We develop climate models based on the conservation of energy and mass and momentum, the fundamental ideas of classical physics. (Budget equations)
    • We are going to identify the sources (production) and the sinks (loss)

Source, Production: Water comes in

Sink, Loss: Water goes out

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What do we do?

  • We develop climate models based on the conservation of energy and mass and momentum, the fundamental ideas of classical physics. (Budget equations)
    • We are going to identify the sources (production) and the sinks (losses).
    • Sources and sinks will be related to those things that can alter, for example, heating and cooling – the “forcing.”
      • Greenhouse gases
      • Aerosols
      • Transfer
      • Transport by Motion
      • Feedbacks

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The Earth System

CLOUD-WORLD

ATMOSPHERE

ICE

(cryosphere)

OCEAN

LAND

SUN

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Symbolic Energy Balance Equation

Eat+Δt = Eat + Δt((Pa – LaEa) + (Tra🡨🡪oil + Ma ))

Atmosphere:

Symbols

E = “Energy”

P = Production

L = Loss rate

Tr = Transfer

M = Motion (Transport)

Superscripts

a is for atmosphere

o is for ocean

i is for ice

l is for land

Variables

t = time

Δt = time increment

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What do we do? – An Example

  • We determine the characteristics of production and loss from theory and observations.
    • Example: the eruption of a major volcano and the temperature response as measured by the global observing system.

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What do we do? – An Example

  • We determine the characteristics of production and loss from theory and observations.
    • Example: the eruption of a major volcano and the temperature response as measured by the global observing system.

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What do we do? – An Example

  • We determine the characteristics of production and loss from theory and observations.
    • Example: the eruption of a major volcano and the temperature response as measured by the global observing system.
    • For this problem we would emphasize
      • Aerosols
      • Transport by Motion
      • Feedbacks
      • Transfer

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The Earth System

CLOUD-WORLD

ATMOSPHERE

ICE

(cryosphere)

OCEAN

LAND

SUN

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Symbolic Energy Balance Equation�(Earth System)

Eat+Δt = Eat + Δt((Pa – LaEa) + (Tra🡨🡪oil + Ma ))

Atmosphere:

Eot+Δt = Eot + Δt((Po – LoEo) + (Tro🡨🡪ail + Mo ))

Ocean:

Eit+Δt = Eit + Δt((Pi – LiEi) + (Tri🡨🡪oal + Mi ))

Ice:

Elt+Δt = Elt + Δt((Pl – LlEl) + (Trl🡨🡪oia + Ml ))

Land:

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A point

  • With this model we are now existing inside of the climate system rather than sitting out in space looking at the global balance.
    • Inside – we are especially interested in what goes on at the surface of the Earth
    • Inside – we must worry about the climate every day, we don’t have the benefit of the average
    • Inside – we must deal with the complexity

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  • This is your point of view or frame of reference.

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A point, continued

  • Conservation is still true, but you must think about being embedded in the system, not a distant observer of the system.
    • Open versus isolated versus closed systems

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  • In your design of the model and model experiment, you are often trying to ”isolate” a system so you can study it.

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Consider just the Production and Loss Rate�(We call this forcing.)

Pa – LaEa

We can divide this, conceptually, into two:

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  • That in absence of the influence of the “industry” of humans (natural)
  • That which includes the influence of the “industry” of humans (anthropogenic)
  • Variability of the sun
  • What volcanoes put in the atmosphere
  • Greenhouse gases prior to industrial revolution
  • Aerosols from, for instance, sea salt and desert dust
  • Changes in greenhouse gases due to burning of fuel
  • Aerosols from “industrial” emissions
  • Changes in gases due to changes in what is growing
  • Change in absorption and reflection due to land use change
  • More?

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More points

  • Models are how we organize our knowledge.
  • The model is a world that you control, you make the decisions. Therefore, you can design experiments.
  • A model is designed for purpose, for an application.
    • Without an application, it is difficult to make decisions of model design.
  • We, naturally, seek to apply models to problems for which they were not designed.
    • We need to remember this.

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Finally: How we can design an experiment?

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  • We look at some historical observations of, for example, temperature.
  • We attempt to predict the temperature response. (What does the “Energy” do.)
  • We evaluate (“validate”) how well we did, characterize the quality of the prediction relative to the observations, and determine, sometimes with liberal interpretation, whether we can establish cause and effect.

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What do we do?

  • We attempt to predict the temperature (“Energy”) response.
  • We evaluate (validate) how well we did, characterize the quality of the prediction relative to the observations, and determine, sometimes with liberal interpretation, whether we can establish cause and effect.

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For example, can we explain the last 1000 years?

Surface temperature and CO2 data from the past 1000 years. Temperature is a northern hemisphere average. Temperature from several types of measurements are consistent in temporal behavior.

  • Medieval warm period
  • “Little ice age”
  • Temperature starts to follow CO2 as CO2 increases beyond approximately 300 ppm, the value seen in the ice-age cycles as the upper range of variability in the past 350,000 years.

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