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Lecture 8 Climate Feedback Processes

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Lecture 8 Climate Feedback Processes GEU 0136 Forcing, Response, and Sensitivity Consider a climate forcing (e.g., a change in TOA net radiation balance, dQ) and a ... – PowerPoint PPT presentation

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Title: Lecture 8 Climate Feedback Processes


1
Lecture 8Climate Feedback Processes
  • GEU 0136

2
Forcing, Response, and Sensitivity
  • Consider a climate forcing
  • (e.g., a change in TOA net radiation balance, dQ)
  • and a climate response
  • (e.g., a resulting change in the globally
    averaged annual mean surface air temperature,
    dTs)
  • We can define a climate sensitivity parameter
  • To know (i.e., forecast) expected climate change
    resulted from a forcing of DQ, simply multiply by
    lR
  • Then the central question of know how
  • What determine the magnitude of lR?

3
Response, Sensitivity, and Feedback
  • Sensitivity parameter depends on direct and
    indirect effects of forcing
  • Changes in TS will also affect
  • Outgoing longwave (sTe4)
  • Planetary albedo (ice, snow, clouds)
  • Water vapor absorption
  • Total sensitivity must take all these indirect
    effects into account
  • Some will amplify sensitivity, and some will damp
    sensitivity

S0 solar constant yj yj(S0)
DS0
4
3 Basic Radiative Feedback Processes
5
Stefan-Boltzmann Feedback
  • Simplest possible model of planetary radiative
    equilibrium
  • Outgoing longwave radiation will increase to
    partly offset any increase in incoming radiation

6
Water Vapor Feedback
  • As surface warms, equilibrium vapor pressure will
    increase (Clausius-Clapeyron)
  • Increasing q increases LWdown (higher e), so Ts
    warms even more
  • Air is not always saturated, but we can assume
    relative humidity remains fixed as Ts increases,
    and calculate new Ts from radiative-convective
    equilibrium

7
Water Vapor Feedback (contd)
  • Water vapor is a positive feedback mechanism
  • OLR is only linear wrt TS, not quartic as
    predicted by BB curves

lR)FRH 2 lR)BB
8
Ice-Albedo Feedback
  • Cold temperatures make the surface turn white due
    to increased sea ice and snow cover on land
  • White (high-albedo) surfaces reflect more SWdown,
    decrease energy absorbed , leading to colder
    surface temperatures
  • Warmer temperatures tend to reduce planetary
    albedo, allowing more energy to be absorbed
  • Positive feedback tends to amplify changes in
    TS resulting from any forcing

9
Ice-Albedo Feedback
  • SH ice sheet at pole, sea-ice from 50º to 80º
  • NH sea-ice at pole, seasonal snow from 40 º
    northward

10
Ice Age Changes
  • Ice age surface albedo was much higher than
    present!

11
Budyko Ice-Albedo Climate Model
  • Solar rad is distribted according to latitude
  • Energy transport is diffusive
  • OLR is linear with TS
  • Albedo switches between two values, depending on
    ice or no ice

12
Budyko Ice-Albedo Climate Solutions
  • Stronger sun causes ice edge to retreat to higher
    lat, vice versa
  • Below 97 of current value, model produces a
    white Earth!

13
Budyko Feedback Sensitivities, 1
  • Ratio of meridional energy transport to longwave
    cooling
  • Budyko used 2.6 modern measurements suggest 1.7
  • Less sensitive using recent data

d g/B
14
Budyko Feedback Sensitivities, 2
  • Ice-free albedo decreases toward the poles to
    account for cloud masking of surface
  • Ice transition makes less difference

15
Tropical SST and LW Feedback
  • Tropical SSTs didnt vary much during ice ages
    why?
  • Near 300 K, LW cooling decreases very fast with
    increasing SST
  • Positive feedback should make tropical SSTs
    sensitive and variable
  • but theyre not!

16
Longwave and Evaporation Feedbacks
  • Tropical SST energy balance
  • SWdown LWup H LE
    DF
  • (200 W m-2) - (60 W m-2)
    (10 W m-2 ) (120 W m-2) (20 W m-2)

17
Compensating Tropical SST Feedbacks
  • Changes in LE with SST balance positive feedback
    with respect to longwave down

18
Biophysical Feedback Daisyworld
  • Consider a planet populated by two kinds of
    plants white daisies and black daisies.
  • Write an energy balance for the planet, assuming
  • (1) it emits as a blackbody
  • (2) the albedo is an area-weighted average of the
    albedos of bare ground, white, and black daisies
  • The daisies grow at temperature-dependent rates
    (optimum at 22.5º C, zero at 5 º and 40º), and
    also proportional to the fraction of bare ground
  • The daisies also die at a specified rate c
  • Solve for areas Ai and temperatures Ti of each
    surface (white daisies, black daisies, and bare
    ground)

19
Daisyworld
h 0 transport is perfect
More generally,
h (S0/4) transport is zero
20
Biophysical Feedback Daisyworld
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