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Summary of data deficiencies in the operational archive |
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This section summarizes
all known data deficiencies (suspect or missing data) of the ECMWF/TOGA
Level III Data Sets from 1 January 1985 to the current date.
Total cloud cover Precipitation U- and V-Wind Components at the Poles (a) Surface data. The grid points at each of the poles will contain horizontal
wind components from the nearest neighbouring Gaussian latitude circle
interpolated to the required resolution. For the T213 model the nearest
latitude circle is ± 89.578132. (b) Upper air data. The grid points at each of the poles contain the
correct horizontal wind components derived from the spherical harmonics
coefficients, i.e. the values of the wind magnitude derived from the horizontal
wind components will be constant, while the u- and v- components oscillate
with a wave number 1 pattern around the poles. From 1 January 1992, all u- and v-wind components at the poles supplied
from the ECMWF/TOGA Advanced Data Sets will be in the format described
in (a) and (b) above. (N.B.) Prior to August 1998, data from the ECMWF/TOGA Basic Data Sets
for periods between 1985 and June 1991 will contour incorrect u and v
components at the pole as described in (a) and (b) above. The following paragraph contains a method for calculating wind components
at the poles using the values at a neighbouring latitude circle. This
is only one method that can be used. The user may wish to use another
method for calculating polar winds, for example by using a polar stereographic
projection. Calculation of wind at the pole from values at a neighbouring
latitude circle approximate wind at the pole for longitude i=l based on the wave number
1 components of U and V along the latitude.
* Gaussian latitude nearest to pole Humidity for the period 12/10/1999-10/04/2000 ECMWF has issued the following warning about upper air data between 12 October 1999 and 10 April 2000. During the operation of IFS Cycle 21r4 of the ECMWF model from 12 October 1999 to 10 April 2000 the humidity fields in the lower stratosphere both in the analysis and forecast were seriously affected by erroneous moisture. These fields should not be used for research and it is recommended that the model results from the operational archive are not used to provide initial conditions for numerical experiments during this period. The error is up to 1 to 2 orders of magnitude in a shallow layer just above the tropopause. This may have a slight affect on the temperature in some regions. Alternative analysis (but not forecast) data can be supplied for this period from research experiments which were run with the error corrected. However the pressure level data from these experiments does not include specific humidity WAM - Size of waves This problem is largely confined to enclosed or semi-enclosed seas such as the Mediterranean Sea, Black Sea, Baltic Sea, the Gulf of Mexico and the East China Sea. A partial correction for this problem was introduced on 11 April 2000 and further changes will be introduced shortly which should eliminate the problem. The spectral orography (parameter 129, archived in MARS on model level 1) and the Gaussian grid point orography (parameter 129, archived in MARS as a surface field) of the high resolution model T511 were not in agreement for the period 21 November 2000 - 26 November 2002. The discrepency between the two fields was introduced on 21
November 2000 with the introduction Differences between the two orography fields can be up to a couple of hundred metres in particular on the slopes of steep orography such as the Alps or the Pyrenees. The spectral orography field on model level 1 is the correct field. The surface Gaussian grid point orography is in error through the application of a wrong filter. |
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