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Radiative feedbacks from stochastic variability in temperature and - - PowerPoint PPT Presentation

Radiative feedbacks from stochastic variability in temperature and radiative imbalance in a hierarchy of CESM simulations Cristian Proistosescu JISAO, University of Washington NCAR May 10, 2018 Collaborators: Kyle Armour - University of


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SLIDE 1

Radiative feedbacks from stochastic variability in temperature and radiative imbalance in a hierarchy of CESM simulations

Cristian Proistosescu

JISAO, University of Washington NCAR May 10, 2018

Collaborators: Kyle Armour - University of Washington Aaron Donohoe - University of Washington Gerard Roe - University of Washington Malte Stuecker - University of Washington Cecilia Bitz - University of Washington

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SLIDE 2

1976 “Understanding the origin of climatic variability in the entire spectral range, from extreme ice age changes to seasonal anomalies, is a primary goal of climate research. Yet [...] there exists today (1976) no generally accepted, simple explanation for the observed structure of climate variance spectra […] A persistent difficulty is that the input response relationships are not

  • bvious upon on inspection of the appropriate time series “
  • K. Hasselmann

2018 A lot more time series, still no simple explanation.

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SLIDE 3

Hansen 1985, Soden and Held 2006, Roe 2008

Energy Balance:

Q = F + R(T)

Energy Budget

kT

= F

TOA

Q

R(T) =

= F

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SLIDE 4

Energy Balance:

Q = F + R(T)

R(T) = −λT R(T) = −λPlanckT + λwvT + λcloudsT + . . .

Linear feedbacks: Linear feedbacks:

Linear Feedbacks

Q = λ · T + F

kT

= F

TOA

Q

R(T) = λT

= F

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SLIDE 5

Equilibrium Sensitivity:

Teq = F λ

Hansen 1985, Soden and Held 2006, Roe 2008

Energy Balance:

Q = F + R(T)

R(T) = −λT

Linear feedbacks:

Q = 0

Net feedback determines equilibrium Climate Sensitivity

Q = λ · T + F

kT

= F

TOA

Q

R(T) = λT

= F

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SLIDE 6

CERES GISTEMP TOA (W/m2) T (K)

Observations of Energy Budget

Donohoe et al 2013

kT

= F

TOA

Q

R(T) = λT

= F

Q = λ · T + F

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SLIDE 7

CERES GISTEMP TOA (W/m2) T (K)

  • Two possible sources of stochastic forcing
  • Ocean forcing only impacts TOA through

changing T

Energy fluxes in the coupled system

Q = −λT + Frad + Focn

TOA

− λT

TOA

+ Frad

+ Focn

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SLIDE 8

CERES GISTEMP TOA (W/m2) T (K)

− λT

TOA

+ Frad

+ Focn

ENSO assumption Oceanic forcing dominates

TOA = −λT

Q = −λT + Frad + Focn

TOA

Assuming oceanic forcing…

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SLIDE 9

CERES GISTEMP TOA (W/m2) T (K)

Assuming oceanic forcing… feedback can be regressed

2 1

  • 1
  • 2
  • 0.4

0.4 0.2

  • 0.2

TOA (W/m2) T (K)

(Forster 2016)

λ = 1.2 (W/m2/K)

(Forster & Gregory 2006, Murphy 2009, Trenberth et al 2010, Dessler 2010, Stevens & Schwartz 2012, Tsushima & Manabe 2013, Zhou et al 2015)

λ = 1.2 (W/m2/K)

TOA = −λT

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SLIDE 10

CERES GISTEMP TOA (W/m2) T (K)

Choices, choices, choices….

TOA (W/m2) T (K)

Monthly Annual Monthly, lag 4 TOA

(Forster 2016)

Sensitive to

  • averaging
  • lag
  • record length
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SLIDE 11

Lagged Regression

TOA (W/m2) T (K)

Monthly Annual Monthly, lag 4 TOA

(Forster 2016)

Sensitive to

  • averaging
  • lag
  • record length
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SLIDE 12

#GOALS

Sensitive to

  • averaging
  • lag
  • record length

We cannot use feedback estimates from variability until we understand the temporal structure. (Forster 2016) Results are sensitive to assumptions about

  • forcing. (Spencer and Braswell, 2010,2011)

Q = −λT + Frad + Focn

TOA

− λT

TOA

+ Frad

+ Focn

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SLIDE 13

CESM1

Reproduces salient feature

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SLIDE 14

CESM1

Reproduces salient feature

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SLIDE 15

Physics is separated by frequency, not lag

  • Carl Wunsch
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SLIDE 16

We need a dynamical model

TOA

− λT

TOA

+ Frad

+ Focn

Q = −λT + Frad + Focn

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SLIDE 17

Hasselmann Model

TOA

− λT

TOA

+ Frad

+ Focn

C dT dt = −λT + Frad + Focn

white noise

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SLIDE 18

Phase fingerprints forcing: ocean forcing

TOA

− λT

TOA

+ Frad

+ Focn

C dT dt = −λT + Frad + Focn

(in phase)

TOA = −λT

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SLIDE 19

TOA

− λT

TOA

+ Frad

+ Focn

C dT dt = −λT + Frad + Focn

TOA = C dT dt

(quadrature)

Phase fingerprints forcing: radiative forcing

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SLIDE 20

Physics is separated by frequency, not lag

  • Carl Wunsch

Physics is separated by model hierarchy

  • Isaac Held (paraphrased)
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SLIDE 21

CESM1 model hierarchy

  • OCN: CESM1 (CAM5)
  • SOM: CAM5 + slab ocean model
  • fSST: CAM5 + fixed SSTs

Unforced, pre-industrial control runs

Atmosphere(Y), Slab(Y), ENSO(Y) Atmosphere(Y), Slab(Y), ENSO(N) Atmosphere(Y), Slab(N), ENSO(N)

  • Energy Balance Model
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SLIDE 22

Fixed SST simulation

− λT

TOA

+ Frad

+ Focn

C dT1 dt = −λ1T1 + Frad + Focn TOA1

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SLIDE 23

Fixed SST simulation: ocean forced

− λT

TOA

+ Frad

+ Focn

(in phase)

C dT1 dt = −λ1T1 + Frad + Focn TOA1 TOA1 = −λ1T1

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SLIDE 24

Slab Ocean Model

− λT

TOA

+ Frad

+ Focn

C dT2 dt = −λ2T2 + Frad + Focn TOA2

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SLIDE 25

Slab Ocean Model: radiatively forced slow mode

− λT

TOA

+ Frad

+ Focn

Q

C dT2 dt = −λ2T2 + Frad + Focn TOA2

(in quadrature)

TOA2 = −C2 dT2 dt

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SLIDE 26

On fast time scales Air-Sea fluxes provide both forcing and damping − λT

TOA

+ Frad Q

H

Ocean-atmosphere exchanges Can be separated into

H ∝ U(To − T) H ∝ U(To − T)0 + U 0(To − T)

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SLIDE 27

On fast time scales Air-Sea fluxes provide both forcing and damping

Ocean-atmosphere exchanges Wind-driven term acts as forcing. Temperature driven term acts as damping term (feedback) Can be separated into

− λT

TOA

+ Frad

+ Focn

H ∝ U(To − T) H ∝ U(To − T)0 + U 0(To − T) H = λaoT + Focn = λaoT +

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SLIDE 28

Coupled atmosphere-ocean model

− λT

TOA

+ Frad

+ Focn

= λaoT

TOA SHF

(Barsugli and Battisti 1998, Cronin and Emanuel, 2013)

  • Atmosphere & land warming may excite different

radiative feedbacks vs mixed layer warming (Proistosescu & Huybers 2017)

Ca dTa dt = −λrad,aTa + Frad,l − λao(Ta − To) + Focn Co dTo dt = −λrad,oTo + Frad,o + λao(Ta − To) − Focn

  • The system evolves along two eigenmodes, each

equivalent to a Hasselmann model (1) (2)

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SLIDE 29

Fast time-scales equivalent to fixed SST − λT

TOA

+ Frad

+ Focn

= λaoT

TOA SHF

(Cronin and Emanuel, 2013)

Co dTo dt = −λrad,oTo + Frad,o + λao(Ta − To) − Focn Ca dTa dt = −λrad,aTa + Frad,l − λao(Ta − To) + Focn

  • On fast time-scales mixed-layer

variability is small

  • (1) is a good approximation for

the first eigenmode

εCa dT1 dt = −λrad,aT1 + εFocn

(1) (2)

ε = λrad,o λrad,o + λao TOA1 = −λrad,aT1

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SLIDE 30

Fast time-scales equivalent to fixed SST

TOA SHF

(Cronin and Emanuel, 2013)

Co dTo dt = −λrad,oTo + Frad,o + λao(Ta − To) − Focn Ca dTa dt = −λrad,aTa + Frad,l − λao(Ta − To) + Focn (1)

(2)

ε = λrad,o λrad,o + λao C1 dT1 dt = −λ1T1 + εFocn

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SLIDE 31

Spectral structures of SHF and TOA support ocean driver

SHF1 = −λaoT1 + Focn + Frad

fSST TOA SHF

C1 dT1 dt = −λ1T1 + εFocn TOA1 = −λ1T1 + Frad

Frequency [1/yr] PSD

εFocn

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SLIDE 32

Filter to high frequencies

SHF1 = −λaoT1 + Focn + Frad

fSST TOA SHF

C1 dT1 dt = −λ1T1 + εFocn TOA1 = −λ1T1 + Frad

Frequency [1/yr] PSD

εFocn

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SLIDE 33

High Frequency heat fluxes (fSST)

Fsurf ≈ cU 0(Ta − To)

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SLIDE 34

Slow time scales, ocean and atmosphere are in near equilibrium

TOA SHF

(Cronin and Emanuel, 2013)

Co dTo dt = −λrad,oTo + Frad,o + λao(Ta − To) − Focn Ca dTa dt = −λrad,aTa + Frad,l − λao(Ta − To) + Focn

  • On slow time-scales atmosphere

and ocean are equilibrated (1) (2)

Ta ≈ To ≈ T2

− λT

+ Frad

+ Focn

= λaoT TOA

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SLIDE 35

Slow time scales, the system coevolves

TOA SHF

(Cronin and Emanuel, 2013)

Co dTo dt = −λrad,oTo + Frad,o + λao(Ta − To) − Focn Ca dTa dt = −λrad,aTa + Frad,l − λao(Ta − To) + Focn (1)

(2)

(Ca + Co)dT2 dt = λ2T2 + Frad Ca dT1 dt = −(λrad,a + λao)T1 + Focn TOA

− λT

+ Frad

+ Focn

= λaoT

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SLIDE 36

Slow time scales, the system coevolves

(Cronin and Emanuel, 2013)

(Ca + Co)dT2 dt = λ2T2 + Frad Ca dT1 dt = −(λrad,a + λao)T1 + Focn

− λT

+ Frad

+ Focn

= λaoT TOA

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SLIDE 37

T1, T2 are eigenmodes of a coupled atmosphere-slab model

On fast time scales

  • Atmosphere equilibrating with ocean
  • Strong forcing, very strong damping

On slow time scales

  • Joint system equilibrating with space
  • Weak forcing,
  • Very weak radiative damping leads to
  • large response, slow equilibration

− λT

+ Frad

+ Focn

= λaoT TOA

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SLIDE 38

Additional ENSO mode

  • TOA and T constant phase lag

fE dT 2 dt2 + 2τ dT dt + λT = ηocn

  • Damped linear oscillator

TOA(t) = −λT(t − θ)

− λT

TOA

+ Frad

+ Focn

= λaoT

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SLIDE 39

Spectral solution Cross Spectrum Wiener-Khinchin Theorem Lagged Covariance Lagged Regression

We can model the lagged regression

We have an analytical stochastic linear model

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SLIDE 40

Fixed SST

Lag (years) Slope (W/m2/K)

T1

— CESM 1 — EBM

TOA1 TOA1 = −λ1T1 + Frad

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SLIDE 41

Slab Ocean Model

TOA1 = −λ1T1 + Frad

Lag (years) Slope (W/m2/K)

T1 + T2 +

— CESM 1 — EBM

TOA1 + TOA2 TOA2 = −λ2T + Frad ∝ dT2 dt

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SLIDE 42

Regression dillution

Lag (years) Slope (W/m2/K)

T1 + T2 +

— CESM 1 — EBM

TOA1 + TOA2

r(lag) = X λi ✓ σTi σtotal ◆ acf(lag)

(timescale)

  • Net feedback

✦average of distinct feedbacks, ✦ weighted by relative variance & ✦ weighted by lag

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SLIDE 43

Regression dilution

r(lag) = X λi ✓ σTi σtotal ◆ acf(lag)

(timescale)

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SLIDE 44

Fully Coupled model

r(lag) = X λi ✓ σTi σtotal ◆ acf(lag)

(timescale)

T1 + T2 + T3

Lag (years) Slope (W/m2/K) — CESM 1 — EBM

TOA1 + TOA2 + TOA3

Understanding previous results

  • Net feedback

✦average of distinct feedbacks, ✦ weighted by relative variance & ✦ weighted by lag

  • Multiple source of forcing
  • Changing fractional variances & acf

explains sensitivity to lag, sampling, & smoothing

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SLIDE 45

Variance fraction is dependent on sampling and record length

r(lag) = X λi ✓ σTi σtotal ◆ acf(lag)

Annual averaging preferentially eliminates fast, air-sea forced mode

Understanding previous results

  • Net feedback

✦average of distinct feedbacks, ✦ weighted by relative variance & ✦ weighted by lag

  • Multiple source of forcing
  • Changing fractional variances & acf

explains sensitivity to lag, sampling, & smoothing

T1 + T2 + T3

Lag (years) Slope (W/m2/K) — CESM 1 — EBM

TOA1 + TOA2 + TOA3

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SLIDE 46

λ1 = 1.2 λ2 = 0.9 λ3 = 2.7 r(0) = 0.8 r(τ) = 1.1 λGHG = 0.9

Air-sea forced Radiatively forced ENSO Zero-lag Peak regression (NOT ENSO) Global-warming

So what does it mean?

r(lag) = X λi ✓ σTi σtotal ◆ acf(lag)

Dynamics are well separated by time-scale. However, variance and covariance (regression) amalgamate across time scales

Understanding previous results

  • Net feedback

✦average of distinct feedbacks, ✦ weighted by relative variance & ✦ weighted by lag

  • Multiple source of forcing
  • Changing fractional variances & acf

explains sensitivity to lag, sampling, & smoothing

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SLIDE 47

Time scale structure of feedbacks

r(lag) = X λi ✓ σTi σtotal ◆ acf(lag)

Stochastic variations in energy budget Conclusions (a)Mechanistic model for joint variability (b)System can be understood as superposition of linear modes (i) atmosphere & land (ii) Mixed Layer (iii) Coupling to deep ocean (c)We can model and understand interannual feedback Proistosescu et al 2018, in press (GRL) Understanding previous results

  • Net feedback

✦average of distinct feedbacks, ✦ weighted by relative variance & ✦ weighted by lag

  • Multiple source of forcing
  • Changing fractional variances & acf

explains sensitivity to lag, sampling, & smoothing