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Home > Research > Ifsdocs > PHYSICS >  
   

Chapter 6. Clouds and large-scale precipitation

IFS documentation Front Page


Table of contents



Chapter 1. Overview

Chapter 2. Radiation

Chapter 3. Turbulent diffusion and interactions with the surface

Chapter 4. Subgrid-scale orographic drag

Chapter 5. Convection

Chapter 6. Clouds and large-scale precipitation

Chapter 7. Land suface parametrization

Chapter 8. Methane oxidation

Chapter 9. Climatological data

REFERENCES


 
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6.2 Numerics




6.2.1 Integration of the equations for cloud water/ice and cloud cover




As cloud processes are rapidly varying in time, care must be taken when Eq. (6.9) and Eq. (6.10) are integrated over the relatively large model time steps. Therefore terms that depend linearly on and are integrated analytically. Eq. (6.9) and Eq. (6.10) can be written as

 
(6.57)


where C is defined by Eq. (6.13), Eq. (6.17), Eq. (6.21), Eq. (6.25), Eq. (6.27) and Eq. (6.29) and D is defined by Eq. (6.48) or Eq. (6.49) respectively, and

 
(6.58)


with , , and defined by Eq. (6.14), Eq. (6.18), Eq. (6.24), Eq. (6.28) and Eq. (6.31). Analytical integration of Eq. (6.57) and Eq. (6.58) yields

 
(6.59)


and

 
(6.60)


Since there are terms in Eq. (6.57) that depend on and terms in Eq. (6.58) that depend on the following method to solve the two equations is adopted. First Eq. (6.59) is solved using the values for at time . Then a time-centred value for the cloud fraction, is calculated as

 
.
(6.61)


Then Eq. (6.60) is divided by and solved yielding a new value for the in-cloud value which is converted into the grid-mean value by re-multiplying with .


6.2.2 Calculation of




Special care has to be taken in the numerical calculation of from Eq. (6.19). Since the saturation water vapour pressure depends exponentially on temperature, straightforward numerical integration of Eq. (6.19) would produce large truncation errors. Therefore the average of over the time step is determined by the means of moist adjustment (e.g. Haltiner and Williams 1980). This is achieved by first extrapolating the cloud temperature to time-level and then adjust temperature and moisture toward saturation conditions.


6.2.3 Convective cloud source




The vertical discretization of equations (6.13) and (6.14) is achieved with a simple upstream scheme, i.e.,

 
(6.62)


and

 
.
(6.63)


Although two of the terms in equation (6.62) depend linearly on it was decided to treat the convective source (like any other source of condensate) fully explicitely, i.e., (6.62) is added into (6.57) as a contribution to only. For cloud fraction it is obvious that the first term on the right hand side of (6.63) can be added to in equation (6.58) wheras the second term can be split into a contribution to and .


6.2.4 Stratiform cloud source




It is evident from (6.24) that the stratiform source of cloud cover is quadratically dependent on and can therefore not easily be integrated analytically following (6.58). To overcome this problem one factor of is integrated into , i.e., treated explicitely, before carrying out the analytic integration of (6.58), i.e.,

 
.
(6.64)


6.2.5 Precipitation fractions




The method to determine and is as follows. If precipitation is generated in a level through the processes of autoconversion or ice sedimentation, it is assumed to be generated at all portions of the cloud uniformly and thus at the base of level k, . The precipitation generated in this cloudy region is given by:

 
,
(6.65)


and the cloudy precipitation flux at the base of level k is given by , where the twiddle symbol indicates the value of at the top of level k. Because the cloud is assumed to be internally homogenous, (6.65) simplifies to , where is the generation rate of precipitation inside the cloud. If only accretion occurs in the clouds of level k, equals , the fractional area that contains cloudy precipitation flux at the top of level k.


Because the clear precipitation flux is assumed to be horizontally uniform, evaporation does not alter the area containing clear precipitation flux such that . Only in the case that all of the clear precipitation flux evaporates in level k does . The clear-sky precipitation flux at the base of level k is given by , where is the clear-sky precipitation flux at the top of level k, and

 
,
(6.66)


where represents precipitation evaporation. Note that precipitation evaporation is a function of guaranteeing that precipitation generated in a level cannot evaporate in the same level. This will guarantee consistency with the assumption that clouds where present fill the vertical extent of the grid cell and that horizontal transfer of precipitation mass from cloudy to clear regions of the grid cell is not possible.


At the interfaces between levels, precipitation mass that is in cloud of the upper level may fall into clear air of the lower level, or precipitation mass that is in clear air of the upper level may fall into cloud of the lower level. Thus at level interfaces an algorithm is needed to transfer precipitation and its area between the cloudy and clear portions of the grid box. The algorithm is constructed by determining the amount of area associated with each transfer and then transferring precipitation fluxes between clear and cloudy components according to the assumption that the precipitation flux is horizontally uniform but with different values in the clear and cloudy regions containing precipitation.


There are four possible areas to be defined (see schematic in Figure ??): the area in which cloudy precipitation flux falls into cloud of the lower level, the area in which cloudy precipitation flux falls into clear air of the lower level, the area in which clear precipitation flux falls into clear air of the lower level, and the area in which clear precipitation flux falls into cloud of the lower level. To determine these areas, the cloud overlap assumption is applied to determine the relative horizontal placements of clouds in the upper and lower levels. For the ECMWF model, the cloud overlap assumption is expressed in terms of an equation which relates the total horizontal area C covered by clouds in levels 1 to k (where k = 1 is the top level of the model), to the total horizontal area cover by clouds in levels 1 to k-1:

 
,
(6.67)


where is a tiny number set to 10-6. Equation (6.67) gives maximum overlap for clouds in adjacent levels and random overlap for clouds separated by clear levels. From this equation, one can determine the portion of clouds of the lower level which is unoverlapped by clouds at all higher levels; this area, , cannot have any precipitation falling into it. Using this assumption, the area for which cloudy precipitation flux falls into clear air of the level below is given by:

 
.
(6.68)


Equation (6.68) makes the further assumption that there is maximum overlap between the area covered by cloudy precipitation at the base of the upper level and the portion of the lower level cloud which lies beneath clouds in higher levels, . With the assumption that the precipitation flux is horizontally uniform, the amount of cloudy precipitation flux of the upper level that falls into clear air of the level below is:

 
.
(6.69)


The area in which clear precipitation flux of the upper level falls into cloud of the level below is:

 
,
(6.70)


which assumes maximum overlap between the portion of the cloud in the lower level k which has cloud at some higher level other than k-1, and the area covered by the clear precipitation flux. Again, with the assumption that the precipitation flux is horizontally uniform, the amount of clear precipitation flux of the upper level that falls into cloud of the level below is:

 
.
(6.71)


Finally, the areas and fluxes at the top of level k can be related to those at the base of level k-1 by:

 
,
(6.72)

 
,
(6.73)

 
,
(6.74)

 
.
(6.75)


From these equations it is obvious that total precipitation area, , and precipitation flux, , are conserved at level interfaces.


6.2.6 Precipitation sources







After the integration of Eq. (6.60) the fallout of condensate (represented by the term in Eq. (6.57)) out of model level is determined as

 
.
(6.76)


The condensate falling out of model level is then distributed into rain, snow or cloud ice in the level below using the following assumptions:
(i)   Pure water clouds. In the case of pure water clouds ( ) all condensate falling out of a model level is converted into rain, i.e.,

 
.
(6.77)
(ii)   Mixed phase clouds. In the case of mixed phase clouds ( ) all condensate falling out of a model level is converted into rain or snow whereby the partitioning between the two phases is determined using Eq. (6.6), i.e.,

 
(6.78)
  and

 
.
(6.79)
(iii)   Pure ice clouds. In the case of pure ice clouds ( ) the condensate falling out of a model level is partitioned into a source of cloud ice in the level below and snow. There are two sources of snow from falling cloud ice; i) all ice content in particles larger than 100 µm is converted into snow, and ii) of the falling cloud ice in particles smaller than 100 µm, ice falling into clear sky is converted into snow, while ice in falling into cloud remains cloud ice. This is implemented in the code as follows. First (6.44) is solved to determine the ice water content in particles smaller than 100 µm. Then (6.60) is solved for layer using

 
(6.80)
  and

 
,
(6.81)
  where

 
.
(6.82)
  represents all sources and sinks of cloud ice not related to precipitation processes, whereas is the source of cloud ice through settling of particles from the layer above (for definition see below). Then (6.76) is solved to determine the fallout of ice out of layer , . Of the ice water content falling into layer in particles smaller than 100 µm, i.e., , the part falling into overlapping cloud area is treated as source of cloud ice, . The area of cloud overlap is determined as

 
,
(6.83)
  where is the change of total cloud cover from layer to layer as described above. Hence,

 
.
(6.84)
  With these defintions the generation of snow in level becomes

 
.
(6.85)
  After the definitions above the precipitation at the surface can be written as

 
.
(6.86)


6.2.7 Evaporation of precipitation




Since the evaporation of precipitation has a threshold value of relative humidity at which the process should cease to exist (see quation (6.55)) an implicit treatment is applied when solving (6.54). If (6.54) is written as

 
(6.87)


the implicit solution becomes

 
,
(6.88)


where refers to the time level at the beginning of timestep . (6.88) ensures that evaporation of precipitation never leads to . To ensure the maximum relative humidity after evaporation does not exceed the threshold value defined in (6.55) the maximum change in specific humidity is calculated as

 
.
(6.89)


The smaller of the values given by (6.88) and (6.89) is then chosen as the true value of evaporation of precipitation.


6.2.8 Cloud top entrainment




After parametrizing the entrainment flux as in Eq. (6.32) and the entrainment velocity as in Eq. (6.33) the tendency equations for the two levels involved in the entrainment process are solved simultaneously using an implicit formulation.


The tendency equation for the cloudy model level, , can be written as

 
,
(6.90)


where is the flux of taken at half-level . A similar equation can be written for the level immediately above the cloud, . Since only the transport between levels and are considered only the flux at half level is non-zero. The solution for at both model levels for time given the values at time can then be found by solving the system of two linear equations

 
(6.91)


and

 
.
(6.92)


6.2.9 Final moist adjustment




After the calculation of the liquid water/ice tendency and the corresponding tendencies of temperature and moisture a final test for supersaturation is performed. If any supersaturation is found the grid box is re-adjusted to saturation (using the moist adjustment formulation) and the moisture excess is converted into precipitation.


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