The lag-1 autocorrelation of the annual time series shows the degree of predictability from one year...

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The lag-1 autocorrelation of the annual time series shows the degree of predictability from one year to the next. It shows the importance of the long-term climate modes, and is also important for quantifying the uncertainty in time- series quantities. Red = AE, Blue = UE, black = control, black-dash = UE10x(fixedCH 4 ), thin colored lines are Monte Carlo realizations with control statistics, to indicate confidence. The three methane runs show decreased predictability in southern ocean. The Impact of Methane Clathrate Emissions on the Earth System Warming may release methane from large Arctic reservoirs Location of emission has some effect on climate Methane emissions may change variability Methane emissions change interannual autocorrelation We acknowledge the contribution of our collaborators, who have primary responsibility for the ocean model (S.Elliott & M.Maltrud, LANL) and sediment model (M.Reagan & G. Moridis, LBNL). We also acknowledge J.Stolaroff (LLNL) for including us in a review for technical mitigation measures for methane. This research used resources of the National Energy Research Scientific Philip Cameron-Smith 1 , Subarna Bhattacharyya 1 , Daniel Bergmann 1 , Matthew Reagan 2 , Scott Elliott 3 and George Moridis 2 1 Lawrence Livermore National Laboratory, 2 Lawrence Berkeley National Laboratory, 3 Los Alamos National Laboratory Future plans Couple our atmospheric methane model to ocean and permafrost methane codes. Determine emission amplification factors, ie the amount of extra methane released due to the warming from the original methane emission (cross- amplification between reservoirs will also occur). Assess the likelihood of runaway warming (aka, the clathrate gun). Participate in future methane related model intercomparisons (we participated in the Atmospheric Chemistry-Climate Model Intercomparison Project (ACCMIP), which helped confirm and debug our model chemical behavior, and resulted in several papers). Acknowledgements Clathrates are methane locked in a water ice structure. ESAS = East Siberian Arctic Shelf (methane under submerged permafrost) SPARC Meeting, Queenstown, 2014 Expected methane sources due to warming Onset of Clathrate emissions expected to be abrupt Fraction of methane that passes through ocean is uncertain, but could be large Stolaroff, et al., 2012 Reagan, et al., 2011 This is the sediment response to a temperature ramp of 5K for 100 years. This emission rate is ~20% of global methane emissions. Most of the emission comes from 300-400m depth. Methane is consumed in the ocean by methanotrophs. But, bubble plumes may inject methane to upper ocean levels which will allow faster release to the atmosphere. 50 m depth 150 m depth Sea - flo or % methane released to atmosphere (no methanotrophs) Months since start of simulation Methane conc. increases non-uniformly Note that methane suppresses the specie that destroys it, so a 3x increase in total methane emissions (10x clathrates) produces 6-8x methane concentration increase over our control (present-day). We added a fast chemical mechanism to CESM that is designed to handle methane . We simulated over 600 years (after spinup) under present-day conditions with 1x and10x expected clathrate emissions (AE), and the same amount of extra emission spread uniformly over the globe (UE). We used an active ocean to see the coupled chemistry-climate response. Temperature increase is modestly dependent on Emission location LEFT: Zonal mean surface temperature increase over control (AE=Red, UE=Blue, UE10x(fixedCH 4 )=Green, 2xCO 2 =Cyan, 4xCO 2 CMIP=Magenta). RIGHT: same data, but expressed as %difference for AE over UE for different regions (GL=globe, SP=south pole, LL=low latitudes, NP=north pole). The error bars are the uncertainty in the mean. The UE simulation is slightly warmer than the AE scenario for almost all latitudes except the Arctic. The modest difference in the Arctic seems to be a compensation between increased warming from extra methane in AE, with greater poleward heat transport in UE. Ozone increases most in polluted regions Annual-mean surface ozone increase due to clathrate emission (vmr) Methane is an important precursor for chemical smog, and the 1x and 10x clathrate emissions increase ozone concentrations by ~5ppb and ~35ppb in polluted regions, respectively. The ozone increase is likely to be even greater during pollution events. We developed a chemistry-climate version of CESMThere appears to be difference the interannual variability between AE, UE, and control The increased methane variability in AE over UE (from the effect of synoptic weather patterns on the clathrate plumes) seems to affect the PDFs of the annual temperature. The effect on the Arctic isn’t as noticeable because it is already a highly variable region. Note that the mean, std. dev., and skewness all seem to be affected. Interannual variability in zonal-mean temperature changes Variability decreases for El Nino and Sea-ice The spatial pattern of the change in the standard deviation of the annual mean surface temperatures looks like it is mostly a function of the radiative forcing in the scenario. The year-to-year auto correlation in southern ocean seems to be reduced Elliott, et al., 2010, 2011 10x scenar ios 10x sce nar io 10x scen ario Arct ic PDF of annual temperatures Annual temperature (K) 10x scena rios Glob al There seem to be changes roughly proportional to the level of global radiative forcing at several latitudes (indicated by arrows). In many cases the decreases are clearly related to sea-ice. In the zonal means, the difference between AE and UE is hard to distinguish from the uncertainty (1 sigma ~ 0.04). Note: the various 4xCO 2 runs are very short, so their variability is much more uncertain. Lag-1 autocorrelation coefficient Lattitude 10x scena rios 10x scena rios AE10x UE10x UE10x(fixed CH 4 ) 4xCO 2 CMIP 2xCO 2 Ratio of standard deviations of zonal-mean surface temperatures to control Latitude A E 1 0 x U E 1 0 x UE1 0x( fix ed) The dots are the variability in the means of each time window of the specified length within the 400 year simulations (with different starting years when possible). The circles are the standard error formula without any autocorrelation correction. The difference is due to auto-correlation. Auto-correlation important for uncertainty Red Dots: Arctic Emission Black Dots: Control Length of time-window (years) Uncertainty in surface temperature (K)

Transcript of The lag-1 autocorrelation of the annual time series shows the degree of predictability from one year...

Page 1: The lag-1 autocorrelation of the annual time series shows the degree of predictability from one year to the next. It shows the importance of the long-term.

The lag-1 autocorrelation of the annual time series shows the degree of predictability from one year to the next. It shows the

importance of the long-term climate modes, and is also important for quantifying the uncertainty in time-series quantities. Red = AE,

Blue = UE, black = control, black-dash = UE10x(fixedCH 4), thin colored lines are Monte Carlo realizations with control statistics, to

indicate confidence. The three methane runs show decreased predictability in southern ocean.

The Impact of Methane Clathrate Emissions on the Earth System

Warming may release methane from large Arctic reservoirs

Location of emission has some effect on climate

Methane emissions may change variability

Methane emissions change interannual autocorrelation

We acknowledge the contribution of our collaborators, who have primary responsibility for the ocean model (S.Elliott & M.Maltrud, LANL) and sediment model (M.Reagan & G. Moridis, LBNL). We also acknowledge J.Stolaroff (LLNL) for including us in a review for technical mitigation measures for methane.

This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science (BER) of the U.S. Dept. of Energy under Contract No. DE-AC02-05CH11231

Philip Cameron-Smith1, Subarna Bhattacharyya1, Daniel Bergmann1, Matthew Reagan2, Scott Elliott3 and George Moridis2

1 Lawrence Livermore National Laboratory, 2 Lawrence Berkeley National Laboratory, 3Los Alamos National Laboratory

Future plans• Couple our atmospheric methane model to ocean and

permafrost methane codes.• Determine emission amplification factors, ie the amount of

extra methane released due to the warming from the original methane emission (cross-amplification between reservoirs will also occur).

• Assess the likelihood of runaway warming (aka, the clathrate gun).

• Participate in future methane related model intercomparisons (we participated in the Atmospheric Chemistry-Climate Model Intercomparison Project (ACCMIP), which helped confirm and debug our model chemical behavior, and resulted in several papers).

Acknowledgements

Clathrates are methane locked in a water ice structure.ESAS = East Siberian Arctic Shelf (methane under submerged

permafrost)

SPARC Meeting, Queenstown, 2014

Expected methane sources due to warming

Onset of Clathrate emissions expected to be abrupt

Fraction of methane that passes through ocean is uncertain, but could be large

Stolaroff, et al., 2012

Reagan, et al., 2011

This is the sediment response to a temperature ramp of 5K for 100 years.

This emission rate is ~20% of global methane emissions.Most of the emission comes from 300-400m depth.

Methane is consumed in the ocean by methanotrophs.But, bubble plumes may inject methane to upper ocean levels which

will allow faster release to the atmosphere.

50 m depth

150 m depth

Sea-floor

% m

etha

ne re

leas

ed to

atm

osph

ere

(no

met

hano

trop

hs)

Months since start of simulation

Methane conc. increases non-uniformly

Note that methane suppresses the specie that destroys it, so a 3x increase in total methane emissions (10x clathrates) produces 6-8x

methane concentration increase over our control (present-day).

We added a fast chemical mechanism to CESM that is designed to handle methane . We simulated over 600 years (after spinup) under present-day conditions with 1x and10x expected clathrate emissions (AE), and the same amount of extra emission spread uniformly over

the globe (UE). We used an active ocean to see the coupled chemistry-climate response.

Temperature increase is modestly dependent onEmission location

LEFT: Zonal mean surface temperature increase over control (AE=Red, UE=Blue, UE10x(fixedCH4)=Green, 2xCO2=Cyan, 4xCO2CMIP=Magenta). RIGHT: same data, but expressed as %difference for AE over UE for different regions (GL=globe,

SP=south pole, LL=low latitudes, NP=north pole). The error bars are the uncertainty in the mean. The UE simulation is slightly warmer

than the AE scenario for almost all latitudes except the Arctic. The modest difference in the Arctic seems to be a compensation

between increased warming from extra methane in AE, with greater poleward heat transport in UE.

Ozone increases most in polluted regions

Annual-mean surface ozone increase due to clathrate emission (vmr)

Methane is an important precursor for chemical smog, and the 1x and 10x clathrate emissions increase ozone concentrations by

~5ppb and ~35ppb in polluted regions, respectively. The ozone increase is likely to be even greater during pollution events.

We developed a chemistry-climate version of CESM There appears to be difference the interannual variability between AE, UE, and control

The increased methane variability in AE over UE (from the effect of synoptic weather patterns on the clathrate plumes) seems to affect the PDFs of the annual temperature. The effect on the Arctic isn’t

as noticeable because it is already a highly variable region.Note that the mean, std. dev., and skewness all seem to be

affected.

Interannual variability in zonal-mean temperature changes

Variability decreases for El Nino and Sea-ice

The spatial pattern of the change in the standard deviation of the annual mean surface temperatures looks like it is mostly a function

of the radiative forcing in the scenario.

The year-to-year auto correlation in southern ocean seems to be reduced

Elliott, et al., 2010, 2011

10x scenario

s

10x scena

rio

10x scena

rio

Arctic

PDF

of a

nnua

l tem

pera

ture

s

Annual temperature (K)

10x scenario

s

Global

There seem to be changes roughly proportional to the level of global radiative forcing at several latitudes (indicated by arrows). In many

cases the decreases are clearly related to sea-ice. In the zonal means, the difference between AE and UE is hard to distinguish

from the uncertainty (1 sigma ~ 0.04). Note: the various 4xCO 2 runs are very short, so their variability is much more uncertain.

Lag-

1 au

toco

rrela

tion

coef

ficie

nt

Lattitude

10x scenari

os

10x scenari

os

AE10x UE10x UE10x(fixedCH4)

4xCO2CMIP2xCO2

Ratio

of s

tand

ard

devia

tions

of

zona

l-mea

n su

rface

tem

pera

ture

s to

con

trol

Latitude

AE10x

UE10x

UE10x(fixe

d)

The dots are the variability in the means of each time window of the specified length within the 400 year simulations (with different

starting years when possible). The circles are the standard error formula without any autocorrelation correction. The difference is

due to auto-correlation.

Auto-correlation important for uncertainty

Red Dots: Arctic EmissionBlack Dots: Control

Length of time-window (years)

Unce

rtain

ty in

sur

face

te

mpe

ratu

re (K

)

https://www.google.ca/search?q=sparc+poster+pjc+2014+methane+hydrate&oq=sparc+poster+pjc+2014+methane+hydrate&aqs=chrome..69i57.17768j0j8&sourceid=chrome&es_sm=93&ie=UTF-8#q=The+Impact+of+Methane+Clathrate+Emissions++Los+Alamos+National+Laboratory

Page 2: The lag-1 autocorrelation of the annual time series shows the degree of predictability from one year to the next. It shows the importance of the long-term.

June 2014

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Climate Action Network calls for phasing out all fossil fuel emissions and phasing in a 100% renewable energy future with sustainable energy access for all, as early as possible, but not later than 2050.

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