Presentation is loading. Please wait.

Presentation is loading. Please wait.

Attributing direct radiative forcing to specific emissions using adjoint sensitivities Daven K Henze, Drew T. Shindell, Robert J. D. Spurr g-con.

Similar presentations


Presentation on theme: "Attributing direct radiative forcing to specific emissions using adjoint sensitivities Daven K Henze, Drew T. Shindell, Robert J. D. Spurr g-con."— Presentation transcript:

1 Attributing direct radiative forcing to specific emissions using adjoint sensitivities Daven K Henze, Drew T. Shindell, Robert J. D. Spurr g-con

2 Radiative Forcing Transfer Functions How to calculate the radiative forcing change for a given change in emissions? IPCC, 2007 Global contributions to aerosol direct RF

3 Radiative Forcing Transfer Functions How to calculate the radiative forcing change for a given change in emissions? Using transfer function T :

4 Radiative Forcing Transfer Functions How to calculate the radiative forcing change for a given change in emissions? Using transfer function T : Approximate T using adjoint: Calculated using GC adjoint (Henze et al., 2007 and LIDORT (Spurr, 2002)

5 Radiative Forcing Transfer Functions The % change in radiative forcing per change in BC emission: note: per change in any BC emission. This shows variation in efficiency of BC emissions forcing.

6 Radiative Forcing Transfer Functions The % change in radiative forcing per change in SO 2 emission:

7 Applying to MFR 2030 – 2000 inventories BC, Total SO 2, Total

8 Applying to MFR 2030 – 2000 inventories BC, Total SO 2, Total

9 Applying to CLE 2030 – 2000 inventories BC, Total SO 2, Total

10 Applying to CLE 2030 – 2000 inventories BC, RESALL SO 2, RESALL

11 Applying to CLE 2030 – 2000 inventories BC, POWER SO 2, POWER

12 Validation: BC CLE 2030 – 2000 perturbation Looks good

13 Validation: SO 2 CLE 2030 – 2000 perturbation Looks OK, but adjoint-approach biased?

14 Validation: SO 2 10% perturbationsCLE 2030 – 2000 perturbation Check: does reducing perturbation reduce nonlinearity? Yes. The adjoint code is accurate.

15 Validation: SO 2 RF E SO2 E 2000 E’ 2030 |ADJ| > |FD| E’’ 2030 |ADJ| < |FD| Can we anticipate bias?

16 Validation: SO 2 CLE 2030 – 2000 perturbation E 2030 > E 2000 (China, India) E 2030 < E 2000 (Europe ) Yes, bias can be anticipated. Also, overall ordering remains the same. Conclusion: adjoint sensitivities provide a rapid means of exploring the effect of specific emissions changes on aerosol DRF.

17 The end Thanks to: Columbia Univ. Earth Institute Fellowship Drew Shindell, Rob Spurr, Nadine Unger, John Seinfeld NASA GSFC: NCCS NASA JPL: SCC

18 Radiative Transfer Code Mie Code derivate mode GC Adj Weighting functions Henze et al., 2007 Following Martin et al., 2004, Drury et al., 2008 Radiative Forcing with GEOS-Chem GEOS-Chem Mie Code Grainger et al., 2004 [SIA], [BC], RH, D dry Radiative Transfer Code LIDORT (Spurr, 2002) TOA upward SW flux Forward model Sensitivity calculation:

19 Radiative Forcing with GEOS-Chem GEOS-Chem [SIA], RH 8.4Koch et al. (1999) 11Chin et al. (2002) 6.5-13.9Martin et al. (2004) 10.5current work Literature D dry N, D wet Mie Code Grainger et al., 2004 (tabulate as )

20 Validating Radiative Forcing Sensitivity ignore Phase function coefficients for SIA(D wet ) D max D min

21 Validating Radiative Forcing Sensitivity Mie results for extinction at discrete mode diameters:

22 Radiative Forcing (forward calculation) Chemical Transport Model Mie Code Aerosol concentrations optical properties

23 Radiative Forcing Sensitivity LIDORT Spurr, 2002 Jacobian calculation GEOS-Chem Adj Henze et al., 2007 Mie Derivative [SIA]*, [BC]* Grainger et al., 2004

24 Radiative Forcing (forward calculation) Chemical Transport Model Mie Code Aerosol concentrations optical properties Radiative Transfer Code TOA upward SW fluxes

25 Next Steps -Validate the transfer functions -Apply to various emissions perturbations of interest

26 Radiative Forcing Sensitivity Radiative Transfer Code LIDORT (Spurr 2002) Jacobian calculation GEOS-Chem Adj Mie Derivative [SIA]*, [BC]* 24 hr 1 week

27 Radiative Forcing with GEOS-Chem GEOS-Chem N, D wet Mie Code Grainger et al., 2004 [SIA], RH [BC] D dry (external mixture) Radiative Transfer Code LIDORT (Spurr, 2002) TOA upward SW flux Following Martin et al., 2004; Drury et al,. 2008

28 Following Martin et al., 2004, Drury et al., 2008 Radiative Forcing with GEOS-Chem GEOS-Chem Mie Code Grainger et al., 2004 [SIA], [BC], RH, D dry Radiative Transfer Code LIDORT (Spurr, 2002) TOA upward SW flux Forward model Radiative Transfer Code Mie Code derivate mode GEOS-Chem Adj Sensitivity calculation [SIA]*, [BC]* Weighting functions Henze et al., 2007 24 hr 1 wk

29 Applying to CLE 2030 inventories note: this takes about 10 seconds

30 Applying to MFR 2030 inventories


Download ppt "Attributing direct radiative forcing to specific emissions using adjoint sensitivities Daven K Henze, Drew T. Shindell, Robert J. D. Spurr g-con."

Similar presentations


Ads by Google