Summary
of the POET kick-off meeting
March,
7 2000
Paris
Attended
the meeting:
Stig
B., University of Oslo (stigbd@geofysikk.uio.no)
Inga
floisand, NILU (inga@nilu.no)
John
Burrows, University of Bremen (john.burrows@gome5.physik.uni-bremen.de)
Andreas
Richter, University of Bremen (andreas.richter@gome5.physik.uni-bremen.de)
Nick
Savage, University of Cambridge (nick.savage@atm.ch.cam.ac.uk)
Kathy
Law, University of Cambridge (kathy@atm.ch.cam.ac.uk)
Carl
Brenninkmeijer, Max Planck Institut for Chemistry (carlb@mpch-mainz.mpg.de)
Valerie
Gros (vgros@mpch-mainz.mpg.de)
Jos
Olivier, RIVM (jos.olivier@rivm.nl)
Jean-François
Müller (jfm@oma.be)
Philippe
Ciais (ciais@lsce.saclay.cea.fr)
Cathy
Clerbaux (ccl@aero.jussieu.fr)
Juliette
Hadji-Lazaro (jha@aero.jussieu.fr)
During
the meeting, each of the participants presented the work which has already been
done and the work everyone is planning to do within each workpackage.
Workpackage
1: Distribution of ozone precursors from satellite data
John
Burrows and Andreas Richter showed examples of
distributions of NO2 tropospheric columns measured by GOME in
1997. He discussed the strategy for comparing observations and model results:
should we calculate the slant columns directly in the models for better
comparisons?
The
work planned in Bremen for the first year of the project will concern the
improvement of the tropospheric NO2 columns retrieval techniques,
more specifically on the air mass factors. The data for 1997 should be ready for
inclusion into the POET data base by the end of 2000.
The
modellers should think about it, and tell the Bremen group what they would like
to have in the data base. In 2001, the Bremen group will work on the ozone and
CH2O retrievals.
Cathy
Clerbaux discussed the first CO tropospheric columns retrieved from the
IMG/ADEOS satellite instrument. The measurements cover the June 16-19, 1997
period. In 2000, she and Juliette Hadji-Lazaro will concentrate on the retrieval
of CO for April and January 1997, and will start the retrieval of tropospheric
ozone columns from the same instrument.
Workpackage
2: Emission inventories
Jos
Olivier discussed the development of the new EDGAR v3.0 data base, which will
provide anthropogenic emissions for year 1995. The emissions factors used in the
EDGAR v2.0 (1990 emissions) will be improved, when possible, and the new ship
emissions inventory will be included. Lightning and aircraft emissions will also
be updated.
The
current Edgar v2.0 data base can be found at the following Web site:
http://www.rivm.nl/env/int/coredata/edgar
His
group will start to work on time profile for the emissions, on a monthly or
daily basis for specific days.
The
data base provides currently emissions of kg hydrocarbons per time unit.
However, most models need additional data to convert these numbers into
molecules. Jos and Jean-Francois Müller will provide during the first year
speciation factors for the hydrocarbons, and they will work together on the time
profiles of the anthropogenic emissions.
Jos
has written several papers describing the data base and its improvements. People
interested by the papers can send him an email to receive these publications.
Jean-François
described the work he recently started to update the algorithms used to
calculate the global emissions of natural hydrocarbons, with a focus on isoprene
and terpenes.
Stig
described the emissions set used in the Oslo model, and focused primarily on
biomass burning emissions.
Jos
also noted that he would like to have a wish list provided by the modellers for
emissions that are not yet available from EDGAR.
Jos
proposed to have a small meeting of people working more particularly on biomass
burning emissions (Jos, Jean-Francois, Stig, Claire, and Martin Schultz from
Hamburg), who could meet in June to agree on a common distribution for biomass
burning emissions to be used in the 4 models.
Workpackage
3: Intercomparison of CTMs
4
models are participating in POET: TOMCAT from Cambridge, OSLO-CTM2 from the
University of Oslo, MOZART from CNRS in Paris, and IMAGES from BISA, Brussels.
Nick
Savage presented the strategy for the intercomparison:
All
models will first perform a first set of runs where the distribution of
long-lived species such as radon will be calculated. Cambridge will send to the
modeling groups the emissions to be used in all models, as well as the
meteorological fields everybody should use. This first set of runs should be
done before the summer, and a 2-days meeting will take place in Cambridge in
July or in September to analyze the model results.
We
will have to discuss more the way the comparisons will be done:
-
which set of data should we use
-
what diagnostics will we use for the intercomparison
-
what definition of tropopause will we use
-
what will be the best period to do accurate comparisons: data, spin up,
El Nino, ...
-
how to define a common emission database: speciation of hydrocarbons,
diurnal/weekly/seasonal variation
-
What informations should we put in the model database
We
should also work on a description of the models, which should be sent to all the
participants (or be included in the POET data base).
Inga
Floisand gave us detailed informations of the POET data base. The ftp address
will be:
zardoz.nilu.no
(128.39.104.1)
directory:
/nadir/projects/poet
NILU
will send us a standard protocol, and we will have to discuss and agree about
the conditions of access to the POET database.
The
format we will use in the database is the CDF format, defined in the Web site:
http://nssdc.gsfc.nasa.gov/cdf/cdf_home.html
This
format is binary format and platform independent.
We
will have to define one person who is responsible for each topic.
We
have defined for now 4 directories:
-
à
Observations
-
à
Isotopes
-
à
Models
-
à
Documents
Note :
Just after the meeting, Inga sent a note indicating that the format used in the
NILU
data base will become HDF. This will be discussed in more details at the next
meeting.
Workpackage
4: Inverse modeling
Philippe
Ciais detailed what he has already done with Jean-François on the inverse
modeling of methane, and he proposed to continue this work by looking at the
interannual changes in methane sources. This will also include an impact of OH
changes with sensitivity studies.
Different
models would be used, and data from the Aerocarb network, which provides regular
measurements of CO2, CH4 and CO, could be used.
Claire
showed preliminary results obtained for the inverse modeling of CO using the
IMAGES model and data from the CMDL network.
The
strategy for the development of the adjoints of IMAGES and MOZART was discussed
by Claire and Jean-François. The adjoint generator TAMC will be used for these
developments, which will start in May in collaboration with Thomas Kaminski (Max
Planck Institut, Hamburg) who participated in the development of TAMC.
Workpackage
5: Isotopes
Carl
Brenninkmeijer gave an overview of the CO and CH4 isotopes
measurements made by different groups. These data will be collected and will be
made available in the POET data base. No systematic work has ever been done on
the analysis of all the available data, and, during the first year of POET, the
data will be analyzed more critically, in order to better understand what we can
learn from isotopic data.
Not
all the sources are known, and the missing parameters will have to be
identified.
Carl
should have a first database by September, and he will discuss the format with
NILU.
Workpackage
6: OH/ozone precursors
Stig
discussed the use of the Oslo model in this study. The Oslo group will define a
strategy for establishing the emissions used in this workpackage.
Paul
Monks (UK) has contacted us before the POET meeting. He is the coordinator of
the TROTREP project: the goals of TROTREP are to understand the trends of
CO, methane and ozone during the 2-3 previous decades. The work performed
within WP 6 is very close to what will be done in TROTREP. John and Carl, who
are going to the Eurotrac meeting will talk to Paul Monks in order to see how we
could cooperate.
Workpackage
7: tagging of ozone
Nick
showed how the tagging of stratospheric ozone has been performed in the TOMCAT
model. The tagging of ozone formed by photochemical production is not
straightforward: different possibilities were discussed. Everybody should think
about it, and bring possible ideas at the meeting in Cambridge.
Summary
by Nick: Think, think and think!
Workpackages
8 and 9:
These
WP will start later. Stig said a few words on the definition of future
scenarios, that will be based on IPCC scenarios.
Jos
proposed to couple the IMAGES CTM with the emission model IMAGE developed at
RIVM. This will be discussed in more details in a year from now.
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