AMIP I/AMIP II Model Differences: Model JMA GSM9603 (T63
L30) 1998
AMIP II Model Designation
Most Similar AMIP I Model
AMIP I/AMIP II Model Differences
AMIP II Model
Designation
JMA GSM9603 (T63 L30) 1998
Most Similar AMIP
I Model
JMA GSM8911
(T42 L21) 1993
AMIP I/AMIP II Model Differences
Model Lineage
The JMA Global Spectral Model used in AMIP II first became operational
in March 1996 (hence its designation as GSM9603). It is the latest
version of a line of global spectral models first described by Kanamitsu
et al. (1983) [9] that also includes the AMIP I model GSM
8911.
Model Documentation
Key documentation of the AMIP II model characteristics is provided by
the JMA Numerical Prediction Division's 1997 Outline of the Operational
Numerical Weather Prediction at the Japan Meteorological Agency [10],
a different reference than for the AMIP
I model.
Horizontal Resolution
The AMIP II model's horizontal resolution is spectral triangular 63
(T63), roughly equivalent to 1.875 x 1.875 degrees latitude-longitude,
a finer resolution than the AMIP
I model.
Vertical Domain
The AMIP II model domain is from the surface to 1 hPa, a higher top
than for the AMIP
I model.
Vertical Resolution
For the AMIP II model, there are 30 unevenly spaced hybrid levels, a substantial
increase of the vertical resolution of the AMIP
I model. For a surface pressure of 1000 hPa, 6 levels are below 800
hPa and 16 levels are above 200 hPa.
Smoothing/Filling
The orography is truncated at spectral T63 resolution in the AMIP II model,
but at T42 in the AMIP I model.
Chemistry
The specified value of carbon dioxide concentration in the AMIP II model
(348 ppmv), differs from the AMIP
I value (345 ppmv). Monthly climatological zonal mean ozone profiles
of Wang et al. (1995) [1] are linearly
interpolated to obtain intermediate daily values in the AMIP II model,
while the AMIP
I model's ozone distributions are specified from another data set.
Radiation
The application of the delta-Eddington approximation in the near infrared
(0.7-5.0 microns) and the treatment of cloud-radiative interactions in
the AMIP II model are different from those of the AMIP
I model.
-
In the near-infrared, scattering/absorption are modeled by a two-stream
formulation using the delta-Eddington approximation (Joseph et al. 1976
[21] and Coakley et al. 1983 [22])
which is applied in the 10 spectral intervals, as described by Briegleb
(1992) [23]. These include 7 intervals
between 0.70 and 5.00 microns to capture oxygen A-band and water vapor
absorptions, and 3 intervals between 2.63 and 4.55 microns to capture carbon
dioxide absorption.
-
Shortwave scattering/absorption due to clouds are treated by the delta-Eddington
approximation. Cloud optical properties (optical depth, single-scattering
albedo and asymmetry factor) are linked to diagnostic cloud water and effective
droplet radius (specified differently for liquid droplets (Slingo 1989
[28]) and for ice particles (Ebert and
Curry1992 [29])). Clouds are treated
as graybodies in the longwave, and cloud absorption is modeled by an emissivity
formulation from cloud water path. For the radiation calculations, vertical
overlap of clouds is assumed to be mixed (changing from full to random
overlap with increasing vertical distance). See also Cloud
Formation.
Convection
The AMIP II model uses an economical version of Arakawa-Schubert (1974)
[30] scheme to simulate penetrative
(deep) convection, which is different from that of the AMIP
I model.
-
The vertical profile of upward mass flux is assumed to be a linear function
of height, as proposed by Moorthi and Suarez (1992) [31].
The mass flux at the cloud base (fixed near 950 hPa in the model) is determined
by the prognostic equation of Randall and Pan (1993) [32].
The major contributions of the cumulus clouds are made through compensating
downward motion, detrainment of mass and reevaporation of the convective
rainfall. See also Precipitation.
-
The effects of an ensemble of multiple-type cumuli are considered. Each
type is defined by the level of the cloud top, where the updraft cloud
mass loses its buoyancy and detrainment occurs. During the upward movement
of the cloud air mass, entrainment of the environment air mass is considered.
The lower limit of the entrainment rate is proposed by Tokioka et al. (1988)
[33].
-
The convective downdraft associated with the cumulus clouds affects the
environment by decreasing the net upward mass flux and detrainment of downdraft
in the subcloud layer. The downdraft mass flux at the cloud base is specified
so that the reevaporation of rainwater moistens the downward flux below
the cloud base to its saturation. In the extratropics, where moist convection
does not always initiate at the surface, the mass flux is determined so
that the large-scale moisture increase is spent by the convection. The
effect of the cumulus convection on the large-scale tendency is calculated
from a budget equation.
Cloud Formation
In the AMIP II model, cloud water content (not included in the AMIP
I model) is parameterized as a function of temperature after
Heymsfield (1977) [35]. All clouds form
completely as liquid clouds if the temperature is higher than 273.15 K,
and completely as ice clouds if the temperature is lower than 233.15 K.
In between, liquid/ice phase ratio of cloud water is linearly interpolated
by temperature. The effective radius of cloud liquid droplet is fixed at
15 microns, while the radius of an ice particle varies in the range 20-50
microns, according to the temperature. See Radiation
for the treatment of cloud-radiative interactions.
Precipitation
-
The treatment of convective precipitation and reevaporation of precipitation
is different from in the AMIP
I model. In the AMIP II model, all the condensed water in the
convective updraft is assumed to be carried to the cloud top. Here part
of the condensed water is converted from cloud droplets to raindrops, while
the remainder is evaporated, moistening the environment through the detrainment
process. See also Convection.
-
Subsequent evaporation of falling large-scale and convective precipitation
is simulated following the formula proposed by Ogura and Takahashi (1971)
[36] in the AMIP II model. The effect
of the wind shear, which is responsible for the vertical tilting of the
cumulus, is taken into account for reevaporation process using the Fritsch
and Chappel (1980) [37] relation between
the shear and the precipitation efficiency. The AMIP
I model does not simulate reevaporation of precipitation.
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Last update August 10, 1999. For questions or comments, contact
Tom Phillips (phillips@pcmdi.llnl.gov)
and/or the AMIP Representative(s).
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