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www.bsc.es
Enhancing the Barcelona Supercomputing Centre
chemical transport model with aerosol assimilation
Enza Di Tomaso1, Nick Schutgens2, Oriol Jorba1, George Markomanolis1
1 Earth Sciences Department, Barcelona Supercomputing Centre2 Atmospheric, Oceanic and Planetary Physics, University of Oxford
WWOSC 2014, Montreal, August 20, 2014
Our Dust Model
NMMB/BSC-CTM
NMMB
BSC-CTM
DUST
Pérez et al., ACP, 2011
CHEM
Jorba et al., JGR, 2012
SEA-SALT
Spada et al, ACP, 2013
Our Dust Model
NMMB/BSC-CTM
NMMB
BSC-CTM
DUST
Pérez et al., ACP, 2011
CHEM
Jorba et al., JGR, 2012
SEA-SALT
Spada et al, ACP, 2013
Our Dust Model
NMMB/BSC-CTM
NMMB
BSC-CTM
DUST
Pérez et al., ACP, 2011
CHEM
Jorba et al., JGR, 2012
SEA-SALT
Spada et al, ACP, 2013
Our Dust Model
NMMB/BSC-CTM
NMMB
BSC-CTM
DUST
Pérez et al., ACP, 2011
CHEM
Jorba et al., JGR, 2012
SEA-SALT
Spada et al, ACP, 2013
Current Operational Flow
model
00 IC +06 FC +12 FC +18 FC +24 FC
model
00 IC FC+06 +12 +18 +24
timeday 1 day 2 day 3 …
Data Assimilation Flow
model
00 IC +06 FC +12 FC +18 FC +24 FC
model
00 IC FC+06 +12 +18 +24
timeday 1 day 2 day 3 …
06 obs 12 obs 18 obs 24 obs
Data Assimilation Flow
model
00 IC +06 FC +12 FC +18 FC +24 FC
model
00 IC FC+06 +12 +18 +24
timeday 1 day 2 day 3 …
model
1
model
m
model
M
06 obs 12 obs 18 obs 24 obs
Data Assimilation Flow
model
00 IC +06 FC +12 FC +18 FC +24 FC
model
00 IC FC+06 +12 +18 +24
timeday 1 day 2 day 3 …
model
1
model
m
model
M
DA
model
1
model
m
model
M
06 obs 12 obs 18 obs 24 obs
DA DA
Data Assimilation Flow
model
00 IC +06 FC +12 FC +18 FC +24 FC
model
00 IC FC+06 +12 +18 +24
timeday 1 day 2 day 3 …
model
1
model
m
model
M
06 AN 12 AN 18 AN 24 AN
DA
model
1
model
m
model
M
06 obs 12 obs 18 obs 24 obs
DA DA
Local Ensemble Transform Kalman Filter
FUNCTION 𝐴𝑝𝑝𝑙𝑦𝐿𝐸𝑇𝐾𝐹 … , 𝐘𝑏 𝑛𝑜𝑏𝑠,𝑀 , 𝐒𝜀 , 𝐲 − 𝐻 𝐱𝑏 , … ,𝐖 𝑀,𝑀
(function and figure by Takemasa Miyoshi, Ott et al. 2004, Hunt et al. 2005)
{ 𝐱(𝑚)= 𝐱𝑏 + 𝐗𝑏 𝐰 𝑚 ∶ 𝑚 = 1,… ,𝑀}
Perturbations factor
Vertical mass flux of dust into a transport bin k
𝐹𝑘 = 𝐶 𝑆 1 − 𝑉 𝛼 𝐻
𝑖=0
3
𝑚𝑖 𝑀𝑖,𝑘 𝑘 = 1,⋯ , 8
Perturbations factor
Vertical mass flux of dust into a transport bin k
𝐹𝑘 = 𝐶 𝑆 1 − 𝑉 𝛼 𝐻
𝑖=0
3
𝑚𝑖 𝑀𝑖,𝑘 𝑘 = 1,⋯ , 8
Experiment setup
Experiment Assimilated Observations Perturbations
CTL none NA
Exp1 NRL MODIS 1 calibration factor
Exp2 selected NRL MODIS 1 calibration factor
Exp3 NRL MODIS calibration factors per bin
Exp4 NRL MODIS calibration factors per fine/coarse bin
Experiment setup
Experiment Assimilated Observations Perturbations
CTL none NA
Exp1 NRL MODIS 1 calibration factor
Exp2 selected NRL MODIS 1 calibration factor
Exp3 NRL MODIS calibration factors per bin
Exp4 NRL MODIS calibration factors per fine/coarse bin
vs
Experiment setup
Experiment Assimilated Observations Perturbations
CTL none NA
Exp1 NRL MODIS 1 calibration factor
Exp2 selected NRL MODIS 1 calibration factor
Exp3 NRL MODIS calibration factors per bin
Exp4 NRL MODIS calibration factors per fine/coarse bin
vs
Experiment setup
Experiment Assimilated Observations Perturbations
CTL none NA
Exp1 NRL MODIS 1 calibration factor
Exp2 selected NRL MODIS 1 calibration factor
Exp3 NRL MODIS calibration factors per bin
Exp4 NRL MODIS calibration factors per fine/coarse bin
vs
Experiment setup
Experiment Assimilated Observations Perturbations
CTL none NA
Exp1 NRL MODIS 1 calibration factor
Exp2 selected NRL MODIS 1 calibration factor
Exp3 NRL MODIS calibration factors per bin
Exp4 NRL MODIS calibration factors per fine/coarse bin
vs
Porting the DA code to OmpSs programming model
• Serial execution with various tasks (different colors, Paraver view)
• The usage of OmpSs on the ‘calcensstat’ subroutine (green color)
• By using two cores we improve two times the performance of the subroutine and we gain
17% of the total execution time
Dust optical depth: 2014 3 Apr FC+24
International Model Intercomparison: the Regional Domain
http://sds-was.aemet.es/forecast-products/dust-forecasts/compared-dust-forecasts
= data assimilation
Dust optical depth: 2014 3 Apr FC+24
International Model Intercomparison: the Regional Domain
http://sds-was.aemet.es/forecast-products/dust-forecasts/compared-dust-forecasts
= data assimilation
Conclusions
A correct characterisation of the ensemble perturbations
has a great potential to deal with our model uncertainties
Conclusions
Once we will have the complete aerosol family in the BSC
chemical transport model, the assimilation of satellite aerosol
products will be more meaningful
Thanks to:
All the Principal Investigators and their staff for establishing and maintaining the AERONET sites
used in this investigation (www.aeronet.gsfc.nasa.gov)
NRL-UND for the MODIS AOD and FF L3 product (Zhang et al. 2006, 2008, Shi et al. 2011,
Hyer et al. 2011) (http://usgodae.org/docs/modis_l3.html)
The MODIS mission scientists and associated NASA personnel for the production of the AOD and
AE data used in this investigation (www.disc.sci.gsfc.nasa.gov/Giovanni)
Takemasa Miyoshi (RIKEN Institute, Japan) who developed the core of the LETKF scheme
(Ott et al. 2004, Hunt et al. 2005)
Acknowledgments