rad_bc_mixing_group_meeting_10_1_2014
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Group Meeting 10/1/14
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Characterizing the Radiative Effects of Black Carbon Internal Mixing Charles Li Group Meeting Presentation October 1, 2014
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Background Black Carbon (BC) Direct Radiative Forcing: • +0.71 W m-2 (+0.08, +1.27)
(1750-2005) Bond et al. [2013] • +0.60 W m-2 (+0.2, +1.1)
(1750-2010) IPCC-AR5
Large Uncertainties associated with direct radiative forcing of BC!
IPCC-AR5
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Background Absorption Aerosol Optical Depth (AAOD, τa)
MAC = Mass Absorption Coefficient nm
= mass concentration
Difference of BC AAOD between AERONET observations and AeroCom models. (Koch et al., 2009; Bond et al., 2013)
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Background
(Oshima et al., 2012; IPCC-AR5)
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Background
(Bond et al., 2013)
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Background • Internal mixing between black carbon (BC) and other aerosol
species, e.g. sulfate and organic carbon (OC)
Credit to Adachi et al. [2010]
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Background Particle-level observations, due to BC internal mixing, MAC is enhanced by • 1.8 ~ 2 for secondary organic aerosol (SOA) & BC (Schnaiter et al.,
2005) • 1.2 ~ 1.6 near large cities (Knox et al., 2009) • 1.4 in biomass burning plumes (Lack et al., 2012)
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Research Question How does black carbon internal mixing affect aerosol
climate forcing?
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Background Radiative forcing due to BC internal mixing from model results: Radiation
Internal Mixing II: Core Shell
Internal Mixing I: Homogeneous
•
+0.51 W m-2
•
+0.50 W m-2 (Lesins et al., 2002)
•
+0.39 W m-2 (Liao and Seinfeld, 2005)
+0.17 W m-2 (Chylek et al., 1995)
(Jacobson, 2001)
•
Internal Mixing III: Maxwell-Garnet (MG) Approximation
•
BC
+0.27 W m-2 (Jacobson, 2001) External Mixing
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Background • 2 × CO2 :
• 2 × Sulfate :
• 2 × BC (at different altitudes):
(Hansen et al., 2005)
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Specific Question and Aim I How does BC internal mixing influence surface forcing
and atmospheric absorption additional to top of the atmosphere (TOA) radiative forcing?
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Background
Mie Calculation
Radiative Transfer Module
AtmosphericChemistry Model
Particle-level Radiative Properties
Radiative Forcing
Aerosol distribution
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Specific Question and Aim II Is it possible to provide a more efficient framework to
study BC internal mixing with reduced complexities?
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Method Mie Theory Calculation
Comprehensive Radiative Transfer Model
Particle-level Radiative Properties
Layer-level Radiative Forcing
Simplified Radiative Transfer Model
• Captures major characteristics; • Saves computational cost; • Examines radiative forcing varied with variables e.g. mixing ratios/states, aerosol species, RH, hygroscopicity.
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I. DEFINING RADIATIVE FORCING DUE TO INTERNAL MIXING.
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Method: GFDL Standalone Radiative Transfer Model • Radiative Properties • Aerosol distribution • Meteorological condition
Standalone Radiative Transfer Model
Radiative Fluxes (RF)
Definition: RF(BC + Sulfate)
= RF(All) – RF(no BC & Sulfate)
RF(BC)
= RF(All) – RF(no BC)
RF(Sulfate)
= RF(All) – RF(no Sulfate)
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Radiative Fluxes: INT vs. EXT Global mean clear-sky radiative fluxes using aerosol climatology in 1999 : Surface Radiative Flux
TOA Radiative Forcing
BC+Sulfat BC e ≅
BC+Sulfat BC e ≅
Sulfat +e
EXT
-2.70
-0.94
-1.73
-1.72
INT
-3.20
-1.45
-2.22
-1.26
Atmospheric Sulfate Absorption
+ +0.2 -1.90 0 +0.6 6
-1.44
+0.98 +1.94
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Radiative Fluxes: INT vs. EXT Global mean clear-sky radiative fluxes using aerosol climatology in 1999 : Surface Radiative Flux
TOA Radiative Forcing
BC+Sulfat e
BC+Sulfat e
EXT
-2.70
INT
-3.20
BC
Sulfat e
≠ -0.94 + -1.73 -1.45
-2.22
RF(BC + Sulfate)
-1.72 -1.26
BC
Atmospheric Sulfate Absorption
≠ +0.2 + -1.90 0 +0.6 6
-1.44
+0.98 +1.94
= RF(All) – RF(no BC & Sulfate)
RF(BC)
= RF(All) – RF(no BC)
RF(Sulfate)
= RF(All) – RF(no Sulfate)
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Radiative Fluxes: INT vs. EXT Global mean clear-sky radiative fluxes using aerosol climatology in 1999 : Surface Radiative Flux
TOA Radiative Forcing
Atmospheric Sulfate Absorption
BC+Sulfat e
BC
Sulfat e
BC+Sulfat e
BC
EXT
-2.70
-0.94
-1.73
-1.72
+0.2 0
-1.90
+0.98
INT
-3.20
-1.45
-2.22
-1.26
+0.6 6
-1.44
+1.94
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Radiative Fluxes: INT vs. EXT Global mean clear-sky radiative fluxes using aerosol climatology in 1999 : Surface Radiative Flux
TOA Radiative Forcing
Atmospheric Sulfate Absorption
BC+Sulfat e
BC
Sulfat e
BC+Sulfat e
BC
EXT
-2.70
-0.94
-1.73
-1.72
+0.2 0
-1.90
+0.98
INT
-3.20
-1.45
-2.22
-1.26
+0.6 6
-1.44
+1.94
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Global mean clear-sky radiative fluxes using aerosol climatology in 1999 +0.46 Wm-2
Radiative Fluxes: INT vs. EXT
-0.50 Wm-2
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Nonlinear effect due to internal mixing • Previous studies:
α ≅ 2 (Jacobson, 2001) α ≅ 1.3 (Bond et al., 2011)
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Nonlinear effect due to internal mixing Clear-sky
TOA
Each color has 8 marks denoting RF based on model year 1860,1890,1910,1930,1950,1970,1990,1999.
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Nonlinear effect due to internal mixing • Assumption behind previous studies:
• Actually, in the case of BC and sulfate mixing:
nonlinear cross term!
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II. CHARACTERIZING INTERNAL MIXING ON PARTICLE LEVEL
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Mie Calculation: BC/Sulfate Mixing Simulations
Difference in Calculation
Ext. Mixing
Mix of radiative properties (BC, Sulfate+water) post MIE
Int. Mixing
Mix of Refractive Indices (BC, Sulfate+water) before MIE
Magnitude of estimations: External Spherical & Aggregated < Core/shell & MG < Homo. Internal Homogeneous Mixing
(Lesin et al., 2002; Bond et al., 2006; Jacobson, 2006)
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Radiative Properties Of The Particles MAC
MSC
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Radiative Properties Of The Particles Effect of internal mixing at the particle level: • Slight increase in
extincetion • Enhanced absorption • Reduced scattering • Forward scattering
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III. CHARACTERIZING INTERNAL MIXING ON LAYER LEVEL
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Relationship between particle-level and layer-level effects
Mie Calculation
λ—wavelength, RH—relative humidity, σ—mass ratio
Two-layer Simplified RTM
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Radiative Properties Of The Aerosol Layer
• Absorbance dominates the difference between layerlevel radiative properties of INT vs. EXT • MAC is the key particlelevel factor that determines this difference.
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Method: Simplified Radiative Transfer Model
Radiative Properties Mie Calculation
Radiative Fluxes Standalone Radiative Transfer Model
GFDL Climate Model • Aerosol distribution • Meteorological condition
Two-layer Simplified RTM Radiative Forcing
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Method: Simplified Radiative Transfer Model Top of Atmosphere F0—insolation
One Dimensional Two-layer Aerosol Radiative Transfer Model
… Ac—cloud fraction Ta—transmittance … Aerosol Layer Multi-scattering …
Surface Rs—surface albedo
Radiative properties of the aerosol layer:
t—transmittance a—absorbance r—reflectance. (Chylek and Wong, 1995)
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Simplified Radiative Transfer Model • Assumption I: eliminate high-order term
• Approximated radiative fluxes:
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Simplified Radiative Transfer Model • Radiative forcing due to internal mixing:
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Simplified Radiative Transfer Model • As was shown
• Then, effects of internal mixing will be
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Simplified vs. Comprehensive Model Clear-sky
Clear-sky
Each color has 8 marks denoting RF based on model year 1860,1890,1910,1930,1950,1970,1990,1999.
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Simplified vs. Comprehensive Model Assume Rs falls between 0.3 and 0.4,
• Simplified model well captured the relative magnitude of
radiative energy.
• Internal mixing evenly captures extra energy from TOA
(positive RF) and surface (negative RF), while retaining them in the atmosphere.
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Particle-level Absorption Enhancement
In most source regions, sulfate mass ratio is between 80% and 98%:
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Absorption Enhancement Comprehensive model:
Particle-level:
Simplified model:
Each color has 8 marks denoting RF based on model year 1860,1890,1910,1930,1950,1970,1990,1999.
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Radiative Fluxes due to internal mixing
F0 = 342 W m-2 Ta = 0.79 Rs = 0.45
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Important Role Of Water
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Missing role of OC Aerosol mass concentration over West Africa in model year 1999
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IV. THREE-SPECIES INTERNAL MIXING: BC, SULFATE AND OC
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Three-species internal mixing Mixing All EXT
Description BC, Sulfate(+water), and OC(+water) are all externally mixed
BCSUL INT
BC and Sulfate(+water) are internally mixed, while OC(+water) is externally mixed with them.
All INT
BC, Sulfate(+water), and OC(+water) are all internally mixed
σsul—mass
ratio of sulfate to BC σoc—mass ratio of OC to BC
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Three-species internal mixing: MAC
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Changing OC/BC Mixing Ratio
• When changing OC mixing ratio towards BC, normalized
RF calculated by BCSUL INT is a good approximation to All INT
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Changing BC/Sulfate Mixing Ratio
• The difference between BCSUL INT and All INT is susceptible to changing Sulfate/BC mixing ratio.
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Changing BC/Sulfate Mixing Ratio • Consider the global mean column density of the three
species together as about 7 mg m-2. • Then, if we assume σsul = 80%, the bias between All INT and
BCSUL INT is Unnegligible!
compared with the bias between BCSUL INT and All EXT
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Summary of current results • Internal mixing evenly captures extra energy from TOA and
surface, while retaining them in the atmosphere. • Enhancement of the absorbing ability (a factor of 2~3) is the
dominant factor in determining the difference between INT and EXT. • Effects of internal mixing is strongest at mass mixing ratio of 60%
sulfate, and has an important contribution from water. • Internal mixing significantly enhances and alters vertical heating
profile, that may result in hydrological response. • Three-species internal mixing has an important contribution,
especially for studying the changing sulfate/BC mixing ratio.
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V. LIMITATIONS
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Limitations From instantaneous radiative forcing to effective radiative forcing: • Fast feedbacks—semi-direct effects on clouds
• Missing component in the current framework: vertical heating
profile due to internal mixing
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Possible fast feedbacks Vertical heating rates
Forcing: • Strong atmospheric heating at
750mb and near surface Possible effects: • Enhanced convection near
surface • Prohibited convection beyond
750mb • Increased low cloud at 800 mb
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Follow-up work (current project) • Implement internal mixing between three aerosol species:
BC, sulfate and OC in the radiative module of the GFDL climate model.
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THANK YOU!
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