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gfdl's home page > people > John Dunne >
Notes from May 11 and 18, 2005
The purpose of these meetings was to present a preliminary analysis of our current 1860 run, and more clearly define the guiding philosophy for ESM development and implementation through a discussion of the various potential physical initialization strategies, carbon initialization strategies and potential carbon system "show stoppers".
A) Preminary Analysis of 60 year ESM2.1 1860 control run:
-
Anand Gnanadesikan presented the model results. In the global
scale, results were surprisingly good. However, the Amazon is
drying out considerably, much more than in CM2.1U. His
presentation can be downloaded here
-
Result - LMDT will take on the issue of the
desertification of the Amazon to diagnose where the problem
lies, and hopefully how to improve it.
B) EM2.1 Initialization procedure
- This run was performed with the radiation configuration of Jan 1,
1860 (CO2 = 285.97865 ppmv), but with the land and ocean
biogeochemistry "feeling" 276 ppmv CO2 for equilibration.
- Issues:
- In this run, we are attempting to accomplish three separate goals:
- Spinning up land and ocean carbon cycle
- Assessing the fidelity of the model solution by
comparing with present-day obs.
- Assessing biospheric feedbacks/impacts to the
fidelity of the model solution by compare directly to
CM2.1U results
- Analysis of the 1860 control run is non-ideal because it makes it
difficult to do a direct comparison with "present day" data.
- Analysis of the 1990 control run is non-ideal because the model
and real-world systems are both out of radiative, ocean nutrient, and
carbon balance
-
Lessons from CM2.1 configuration for initialization, development and
spinup:
- All configurations with first initialized from data, and then spun-up as component models with data boundary conditions (AMIP/CORE) then further spun up in the intermediate coupled model configurations, before the final runs were performed.
- Ocean - Levitus temp and salt was run for 1 year with CORE forcing to spin up currents while retaining large scale temp/salt structure.
- Ice - climatology
- Atmosphere and Land - A cold start (isothermal, stationary
atmosphere) was done with the
atmosphere AMIP was then run for 1979-1986
- Control_1860_D4 - 1860 greenhouse gases i.e. CO2 = 286
ppm) were run for 241 years, then restarted in testing (and
final) configuration
- Control_1990_E1 - 1990 greenhouse gases (i.e. CO2 = 353
ppm) were run for 241 years, then restarted in testing (and
final) configuration
- Historical run (1860_2000_H2) - Time-varying greenhouse
gases were run from year 41 of Control_1860_D4.
- Even in the case of the physics-only CM2.1U,
many steps were required for initialization. In particular,
efforts were made to assure that each component was both
stable and as close to observations as possible in it's
interface with other models - e.g. allowing the ocean to have
currents but not let it change SST too much before coupling
with the atmosphere. Ron Stouffer commented that, in
retrospect, the physics spin-up should have been given at
least 500 years to decrease drift, but that time-pressure did not allow it.
- ESM2.1 greenhouse gas configuration options:
- 1750 - undisturbed vegetation, CO2 = 278 ppmv - the benefit is
that this scenario allows us to cleanly spin up the carbon system
before anthropogenic impacts. The liabilities are that there is no
data to establish fidelity, we do not know how how adversely the CO2
will impact vegetation, the CO2 level from the middle ages with more
like 283 ppm, so 278 may be overextending the industrial change, and
there is not currently a CM2.1U run for these
exact conditions available for direct comparison with the ESM... perhaps we should run
a Control_1750 in order to do these comparisons?
- 1860 - beginning of the industrial revolution, CO2 286 ppmv - the
benefit is in comparability to the CM2.1U control run. The liability
is that land use and CO2 have some
anthropogenic impacts, such that the total CO2 change from full
"preindustrial" to 1990 is
diminished by 11%.
- 1990 - Present day, CO3 = 353 ppmv - the benefit is that these are
the current conditions of the Earth system under which most of the
observations were taken. The liabilities are that the spin-up result
would not be applicable as an initial condition for the pre-industrial
era and that, at the present
time, the earth system is
currently out of balance in terms of radiation, CO2, and land use, all
of which are increasing. Since it takes on the order of 100 years for
the vegetation and surface ocean biogeochemistry to come into balance,
the conditions would be difficult to interpret, since the observations
have their own time-scale of response embedded within them.
- Fixed to historical concentrations - the benefit of this would be
that it would follow the real forcing. The liability is that the
system would not be in steady state, and so temporal changes would be
impossible to attribute uniquely to model drift versus climate response.
- Result - Until we get through the development, initialization and
spin-up and phases, all ESM runs will be in the 1860 configuration -
this means that BOTH RADIATION AND BIOGEOCHEMICAL CO2 will need to be equilibrated to the Jan 1, 1860
value (285.97865 ppmv) to avoid shock after spin-up. The previous run
had used 276 ppmv as the biogeochemical CO2. As we assess the
fidelity of this run, we will be comparing results to present day data
for land and ocean biogeochemistry with the implicit assumption that
large-scale features have not changed.
- The central question is whether we need to establish strict
fidelity criteria that determine when model development is complete...
- CM2 analogy - CMDT established the following three
criteria that the model development was forced to satisfy before
it could be considered viable and complete:
- Modeled sea surface temperatures everywhere < 10 deg. C from
Levitus on the annual mean
- North Atlantic Deep Water formation rates had to be at least
10 Sverdrups.
- The model had to exhibit some form of El Nino - where El
Nino was somewhat loosely defined as a tropical variability with
a period between 1 and 5 years with an intensity of the same
order as that observed.
- Most of the physics driving the biogeochemistry has already been optimized for
the particular configuration, so simple physical improvements are unlikely
- The ESM is more complex than a climate model alone as it includes both physical and
biogeochemical components with potentially much more sophisticated
representation of the role of and impact on humans. Thus, it
behooves us to charge ahead and not get too bogged down in details
which may prove irrelevant.
- We don't have nearly the kind of experience with
the ESM class of models as with do with climate models, so we have
much less idea as to what features and defects of the model the
results will be most sensitive.
- The experience we do have tells us that some of the biogeochemical time
scales are much longer because of terrestrial soil processes and
ocean interior sources and sinks of tracers.
- Result: For now, the only target that we will consider
absolutely necessary is that both the land and ocean models spin
up to an equilibration criterion wherein the net flux to/from the
atmosphere - which we will specify as having to be less than 2.0
Pg C / decade - is dwarfed by the
anthropogenic increase which will be applied (2 Pg C / yr).
- Other targets we will consider aiming for are:
- total land biomass (600PgC)
- total land soil carbon (2000 PgC)
- average surface nitrate concentration (5 uM)
- average 1000m nitrate concentration(34 uM)
- This discussion brought up the larger question of whether or not we even attempt to tune in the ESM, or simply incorporate tunings from component models?
- Result: Tuning within the ESM should be avoided as much as
possible. When problems are suspected in the simulation, they should
be worked out in the component models wherever possible.
D) Plans for next two months/continuing action items.
- 1) Achieve frozen rts checkout based on Lima that is capable
of reproducing CM2.1
- 2) Finalization of ocean carbon system initialization plan.
