Title: CO2 variability simulated with daily fluxes
1CO2 variability simulated with daily fluxes
- Shamil Maksyutov, Misa Ishizawa
- Frontier Research System for Global Change,
Yokohama Japan
Transcom workshop Tsukuba 2004
2Should one simulate the high frequency
variability
- Pro
- Inverse models relying on snapshot observations
(flask data) have to deal with observation noise
translated directly into noise in fluxes
(interannual or monthly). ? Perfect forward model
simulation is supposed to reduce this source of
noise - Compared to monthly average data use, more
uncertainty reduction can be expected with the
same data, by applying different weight
(observation error) to each measurement, avoiding
conservative error estimate for aggregated data.
Kind of data aggregation error or bias
3Should one simulate the high frequency
variability
4Should one simulate the high frequency
variability
- Contra
- Forward model simulation errors are even more
evident in high frequency time series, including - Transport model error (limited model resolution
in time and space, numerical diffusion, imperfect
physics, etc) - Emission field errors
- Terrestrial ecosystem flux simulation with
ecosystem models daily flux simulation often
fails even at flux tower sites with well known
hydrology, phenology, vegetation type, when
global/regional gridded meteo data sets are used
as forcing for process based models.
5Multiyear simulation of atmospheric CO2
variability in global scale
- Atmospheric tracer transport NIES transport
model with NCEP wind interpolated to 2.5 or 1
degree resolution. Modification increased
tropospheric mixing by prescribed turbulence. - Fossil fuel emission (CDIAC)
- Oceanic flux (Takahashi, 1999, 2002), as in T3
protocol - Terrestrial biosphere
- a) CASA Randerson 1997 (Transcom)
- b) Biome BGC (Fujita et al 2003)
6Biospheric model fluxes at daily resolution
- Biome-BGC model (S. Running, P. Thornton) v. 4.12
- Ecosystem type map (derived from Matthews by R.
Hunt, 1996) 1x1 deg. - 1x1 deg Zobler soil data set ( clay, sand, silt
for water holding capacity simulation) - 1.8 deg 6hourly NCEP reanalysis data set (tmin,
tmax, temp, precip, short wave radiation)
interpolated to 1x1 deg. - 2 versions of SWR algorithm tried a) - Mtclim
processor, b) NCEP reanalysis
7Model vs. observations simulating spikes
8Model vs. observations simulating spikes
9Simulating continuous observations at Hateruma
- Observations hourly data interpolated to daily
average. Hourly data show much larger variability
as compared to model simulation - Model simulation (6hourly output) performed with
CASA (monthly) and Biome-BGC (daily) fluxes. - Surprisingly, monthly CASA fluxes are sufficient
in many cases for simulating the synoptic scale
variability, while dailiy Biome-BGC fluxes do not
have much advantage.
10Short term variability at marine site Hateruma
11Extracting short term variability
- Seasonal cycle fit curve is subtracted from both
observations and simulations respectively.
12Short term variability at marine site Hateruma
Comparison shows better correlation in winter
13Short term variability at marine site Hateruma
Breakdown into components show anti-correlation
of biospheric and fossil fuel components in
summer may be a reason for difficulty to
simulate In winter similar magnitude and sign.
14Short term variability at land site ITN
1997-98
15Short term variability breakdown into
components ITN
In summer dominated by biospheric flux
contribution In winter biospheric and fossil
fuel are of similar order of magnitude
1997-98
16Data selection issue for land site
- Preferable treatment is to select well mixed
(usually afternoon condition) - Selecting afternoon values at low towers may
still lead to significant difference vs 500m
level in winter - For tall towers (500 m LEF, ITN) difference
between daily and afternoon is small, compared to
short term variability.
17Short term variability breakdown into
components LEF
1995-96
18Correlation as a measure of the forward model
performance (LEF)
- Better correlation in winter, CASA vs Biome BGC
19Few formulas
- Objective function for optimization
- Data uncertainty in Globalview based analysis
defined as observation error (variability plus
analysis error including calibration offset
uncertainty) - In Bayesian inversion (as in Tarantola) flux is a
linear function of (observation-model) mismatch,
so it makes sense reducing mismatch at synoptic
scale too. However posterior flux uncertainty is
not influenced by the mismatch.
20Summary
- Taking into account high frequency variability
may improve inverse modeling performance, reduce
actual flux noise. - Even simple model setup with relatively crude
resolution shows good correlation at time scales
of 3-5 days most of the year - Improvements in the inverse model theory are
needed to incorporate model error and
observation-model mismatch into the flux error
estimate.