Although we certainly agree that the models should
be run at the resolution used in GCMs, we also feel that analysis of the
results is almost impossible on a low vertical resolution. One should note
that the lower resolution might benefit from the high resolution results,
as coding errors, numerical instabilities, and ``fawlty'' physics become
more apparent on high resolution. In addition, a gradual increase in vertical
resolution might be expected in the coming years.
Our approach can be summarized as follows: "first
understand the physics of the SCM on a rather high resolution (with small
numerical errors) and then investigate the degrading on lower resolution.''
We therefore request to run your model on (at least) two resolutions.
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``standard (low) 19 level resolution'' : 60 level
ECMWF resolution
This is actually not such a low resolution for
a GCM. It has about 20 levels in the lower 4 km of the atmosphere, but
most of the levels are concentrated in the lowest 1 km. In the cloud the
grid spacing is approx. 300 m, equivalent to 3 or 4 levels in the cloud.
This resolution should be considered as the minimum resolution needed to
take advantage of the ``advanced'' physics most SCMs use.
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``high 40 level resolution''
40 levels in the lowest 4 km. In the cloud the
resolution is 100-120 meters. The cloud layer is now rather well resolved
by 6-8 levels.
Initial profiles at these resolutions and
the grid can be found here. One may also choose
to replace the latter high-resolution by any other higher resolution (but
you will have to do the interpolation yourself; please check carefully).
The suggested resolution is the lower limit of what I call high resolution.
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if possible also run the model on your present operational
resolution. For this resolution one only needs to sent in setA (mean profiles)
and setE (time series).
Some model might not be able to run with half
an atmosphere (extending to only 4 km). If that is true the profiles should
be extrapolated. It is perhaps easiest to take a very stable, very dry
atmosphere above 4 km to rule out any interference.
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time resolution. Most
GCMs run with a large time step (order 5 minutes - 30 minutes). However,
if possible, please run you model with a relatively small time step of
order 1 min - 5 minutes. The reason is that numerical errors caused by
the time descretization are very unpredictable, thus making an analysis
of the results almost impossible. For your own interest you may also run
with larger time steps.
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requested output. The
original requested output was focussed on the LES models. We defined a
somewhat different set of output parameters more suitable for the SCMs.
In particular, more output is requested with respect to the turbulence
scheme and the massflux scheme. The list of output variables are here.
Please adhere the formatting requirements.
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surface fluxes. From
previous SCM intercomparisons it appears that in some models it is not
easy to prescribe the surface fluxes. In many models this means that the
surface routine has to be modified because the surface flux is implicitely
calculated in the turbulence scheme. Some small errors in the surface fluxes
are therefore acceptable, as long as these stay within 5 % of the actual
flux (so at most 25 W/m2 for the latent heat flux during day time).
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specific humidity or mixing ratio.In
the original case prescription there was some confusion between specific
humidity qv and mixing ratio rv. The initial profiles in the original case
description are in rv. We give both qv and rv. But don't worry too much
about this because differences are only of order 1%, as qv = rv / (1 +
rv) ,with rv order 0.01 kg/kg (10 g/kg). For the forcing tendencies (advection)
the difference between qv and rv can be neglected.
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radiation. Radiation
(both longwave and shortwave) should be switched off completely.