It is also possible to set CAM to predict sulfate aerosols. These aerosols can be run as passive (non-interacting) constituents, or the model can be set to allow sulfate to interact with the radiative transfer formulation. The CAM 3.0 release of the model allows only the direct radiative effect of the aerosols, although it is a straightforward modification of the model to allow indirect effects as well.
The formulation for the parameterization follows closely that described in Barth et al. [12] and Rasch et al. [143]. The module was used to examine the influence of sulfate aerosols on the atmospheric radiation budget in [92] The standard emission inventory used for prognostic aerosols is not the same as that used to produce the climatological prescribed sulfate aerosols described in section 4.8.3.
The sulfur chemistry represented in the model includes emissions,
transport, gas and aqueous reactions, and wet and dry deposition of
DMS, SO, SO
, and H
O
. Sources and sinks
represented in the description of the sulfur cycle include emissions
of DMS and anthropogenic sulfur, gas-phase oxidation of DMS and
SO
, gas-phase production and destruction of
H
O
, aqueous-phase oxidation of S(IV) by
H
O
and O
, dry deposition of H
O
,
SO
, and aerosol sulfate, and wet deposition of
H
O
, SO
, and aerosol sulfate.
Transport processes of trace gases and aerosols include resolved-scale advection and subgrid-scale convection and diffusion. The convective transport of trace gases and aerosols is performed on the interstitial fraction of these species in the cloudy volume and the fraction of dissolved material in the cloud drops that do not undergo microphysical transformation to precipitation. The species can be can be detrained at higher levels in the model by the convective processes.
Emissions of sulfur species in the model include anthropogenic emissions
of SO and SO
and oceanic emissions of DMS;
volcanic and biomass burning sources currently are excluded.
Anthropogenic emissions come from the [162] inventory.
The seasonally averaged emissions data were provided at the
surface and at 100 m and above to accommodate emissions from industry stacks
The anthropogenic emissions are assumed to be 98% by mole SO and 2% SO
.
Since the emissions inventory supplied data at two levels
and the height of the interface between the bottom two model levels was
generally above 100 m (average height was
120 m), we apportioned
a fraction of the emissions data from
above 100 m to the bottom level of the model. The fraction into the
bottom level was determined as
where is the height of the top of the lowest level of the model and
is the height of the top of the second lowest level of the model.
The emissions of DMS were obtained from the biogenic sulfur emissions inventory of [86].
The order of the chemistry calculations is as follows. The aqueous
chemistry is performed after the cloud water mixing ratio is determined.
The new HO
, SO
, and SO
concentrations are then used for the gas
chemistry calculations. The modified H
O
, SO
, and SO
concentrations
then are used
in the wet deposition calculation. After the chemistry and wet deposition are calculated,
transport through subgrid convective cores is determined for the interstitial
fraction of each species (because of their high solubility, sulfate aerosols are
not convectively transported). Because a centered time step is used, a
time filter couples the concentrations from the odd and even time
step integrations.
Then the emissions and dry deposition calculations are performed.
The reactions used for the sulfur cycle are described in Table 4.7.
![]() |
![]() |
Reference4.2 | ||||
Gas Chemistry | ||||||
(R1) | SO![]() |
![]() |
SO![]() |
k![]() ![]() ![]() |
NASA97 | |
k![]() ![]() |
||||||
(R2) | DMS + OH |
![]() |
![]() ![]() ![]() |
Y90 | ||
(R3) | DMS + NO![]() |
![]() |
SO![]() ![]() |
1.0
![]() |
500. | NASA97 |
(R4) | HO![]() ![]() |
![]() |
H![]() ![]() ![]() |
8.6
![]() |
-590. | NASA97 |
(R5) | H![]() ![]() ![]() |
![]() |
2OH | see text | ||
(R6) | H![]() ![]() |
![]() |
HO![]() ![]() |
1.7
![]() |
160. | NASA97 |
Aqueous Chemistry | ||||||
(R7) | HSO![]() ![]() ![]() |
![]() |
SO![]() ![]() ![]() |
2.7
![]() |
4750. | HC85 |
(R8) | HSO![]() ![]() |
![]() |
SO![]() ![]() ![]() |
3.7
![]() |
5300. | HC85 |
(R9) | SO![]() ![]() |
![]() |
SO![]() ![]() |
1.5
![]() |
5280. | HC85 |
Equilibrium Reactions | ||||||
(R10) | H![]() ![]() |
![]() |
H![]() ![]() |
7.4
![]() |
-6621. | LK86 |
(R11) | O![]() |
![]() |
O![]() |
1.15
![]() |
-2560. | NBS65 |
(R12) | SO![]() |
![]() |
SO![]() |
1.23 | -3120. | NBS65 |
(R13) | H![]() ![]() |
![]() |
HSO![]() ![]() |
1.3
![]() |
-2015. | M82 |
(R14) | HSO![]() |
![]() |
SO![]() ![]() |
6.3
![]() |
-1505. | M82 |
Oxidation of SO to form sulfate, oxidation of DMS to form SO
, and
production and destruction of H
O
are represented in the model.
In R1, it is assumed that the SO + OH reaction is the
rate-limiting step of the multistep process of forming aerosol sulfate.
Concentrations of short-lived radicals OH, NO
, and HO
are prescribed using three-dimensional, monthly averaged concentrations
obtained from the Intermediate Model of Global Evolution of Species (IMAGES)
[130].
The diurnal variation of these oxidants is not included in our
calculations, but instead, the diurnally averaged value is used at
each time step.
The rate coefficient for (R2) follows Benkovitz et al. [16],
who followed the work of Yin et al. [195,194].
The rate of H
O
photolysis is determined via a look-up table method
where the photolysis rate depends on the diurnally averaged zenith
angle and the height of the grid point, assuming that the albedo for
ultraviolet radiation is 0.3. Because R4 is nonlinear and
the diurnally averaged rate of reaction does not equal the reaction
rate of diurnally averaged HO
mixing ratios, the HO
mixing
ratios are adjusted by the amount of daylight at any given latitude.
The rates of the sulfur reactions are determined by the effective
first-order rate coefficient and using a quasi-steady state approximation
[70]. The H
O
concentration determined
from the gas-phase reactions is calculated using an Euler forward
approximation.
Oxidation of aqueous SO by O
and H
O
to form SO
aerosol is
included in the model (Table 4.7). The concentrations of
O
are prescribed using three-dimensional, monthly averaged
concentrations obtained from the IMAGES model. Prescribed species
(O
, OH, HO
, and NO
) are set according to the linearly
interpolated concentration for the location of the grid point and the
time of year.
The pH of the drops is determined diagnostically assuming an
NH to
SO
molar ratio of 1.0.
The liquid water content in a grid cell is determined by combining
the resolved-scale cloud water mixing ratio that is predicted, the
subgrid-scale deep convective and shallow convective cloud water
mixing ratios, and the resolved-scale rain mixing ratio that is
diagnosed from the precipitation rate using a mass-weighted fall speed,
which is determined assuming a Marshall Palmer
size distribution for rain. SO and
H
O
are depleted and SO
is produced only in the cloudy region of
the grid box. The grid box concentration of these species is found
by multiplying the cloudy region concentration times the cloud fraction
and the clear air concentration times the fraction of clear air in the
grid box.
Because the rate of S(IV) (= SO
H
O + HSO
+ SO
)
oxidation by O
depends on the pH of the drops, the aqueous-phase reactions are evaluated
using a 2-min time step with an Euler forward numerical approximation.
At the end of each 2-min time step the hydrogen ion concentration is
recalculated so that the influence of pH on S(IV) oxidation is captured.
The wet deposition rates are calculated separately for gases and aerosols. Cloud water and rain mixing ratios from both the resolved clouds and the subgrid-scale clouds are determined for the cloudy volume in each grid column. Trace gases are scavenged only by the liquid hydrometeors, whereas aerosols can also be scavenged by snow.
The fraction of a trace gas that is in the liquid water is determined through each species' Henry's law coefficient, which is temperature- and/or pH-dependent. At any particular level in the model the flux of the dissolved trace gas in the precipitation entering the grid cell from above is found. The trace gas is reequilibrated with the current model level's properties. Then the flux of the dissolved trace gas exiting the model level is determined. The rate of wet deposition is found from the flux divergence, maintaining mass conservation.
The wet deposition of aerosols is performed in a similar flux method. Any layer in the model can undergo both below-cloud and in-cloud scavenging.
The below-cloud scavenging follows Dana and Hales [47] and Balkanski et al. [10]. It is assumed that both rain and snow, which has graupel-like characteristics (and therefore characteristics similar to rain), scavenge the aerosol below cloud. Removal is assumed to take place by a first-order loss process. That is,
In-cloud scavenging is performed assuming that the some fraction (currently 30%) of the aerosol reside in the cloud water. That fraction is then removed in proportion to the fraction of cloud water that is converted to rain through coalescence and accretion processes. This fraction of the aerosol is removed through wet deposition.
Evaporation of rain is accounted for in the wet deposition rate calculation by releasing a proportionate mass of aerosol to the atmosphere (i.e., if 10% of the precipitation evaporates, then 10% of the sulfate aerosol is released back to the air). This last assumption could lead to an overestimate of sulfate mixing ratios in the air [11] because the number of drops that completely evaporate (and therefore the amount of sulfate aerosol released from the drop to the air) is not necessarily proportional to the mass of rain that evaporates.
In [12] we used of dry deposition similar to that described
by Benkovitz et al. [16]. The deposition velocity of
SO is determined following the series resistance method
outlined by Wesely [180] where the deposition
velocity is inversely proportional to the sum of the aerodynamic
resistance, the resistance to transport across the atmospheric
sublayer in contact with surface elements, and the surface resistance.
The aerodynamic and sublayer resistances are determined using boundary
layer meteorological parameters. The surface resistance is found
through a parameterization outlined by
Wesely [180].
We are in the process of integrating this calculation with the surface process characterization produced by the Common Land Model (CLM). When complete, the internal consistency of the parameterization will be much improved.
In the meantime, we have chosen to prescribe our deposition velocities
following [58]. For SO we use
0.6 cm/s for land, 0.8 cm/s over ocean, and 0.1 cm/s over ice and
snow. Deposition velocities for SO
are set to 0.2cm/s
everywhere.