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Proceedings - C-SRNWP Project

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either with a 1-dimensional observation operator which assumes local horizontal homogeneity<br />

for the radiative transfer calculations, or with a 2-dimensional observation operator which<br />

takes into account horizontal gradients along the limb-viewing plane.<br />

The first set of experiments assimilating CHAMP GPS radio occultation (GPSRO)<br />

measurements with 2-dimensional bending angle observation operators has been completed.<br />

The 2-dimensional operators improved the bending angle departure statistics in the lower<br />

troposphere by around ~5% compared with a 1-dimensional bending angle operator, although<br />

this did not translate into a clear, statistically significant improvement in the forecast scores.<br />

COSMIC data (which has been seen to be of high quality) have been received from August<br />

and should be used in operations soon.<br />

Green dots – COSMIC GPSRO locations over a 24 hour period. Red dots: radiosondes<br />

Observing System Experiments (OSEs) coordinated by EUCOS have been performed to<br />

examine the various components of the terrestrial Observing System, in the presence of the<br />

current satellite-based Observing System. Results from a summer period (46 days) are<br />

currently being assessed. The winter studies indicate a large impact of the radiosondes (wind<br />

and temperature) and aircraft (wind and temperature), a marginal impact of radiosonde<br />

humidity information, and a contrasted impact (with negative spells) from the wind profilers.<br />

REANALYSIS<br />

The ERA-interim reanalysis has started. It covers the period from 1989 and will be continued<br />

in near-real time when it reaches the present (“climate data assimilation mode”).<br />

• It uses Cycle 31r1 of the IFS 12-hour window 4D-Var and T255 resolution in the outer<br />

loops. Currently two versions exist: 60 and 91 levels. Only the best version will be<br />

continued in near-real time.<br />

• The set of observations and SST/ice information used is the same as in ERA-40 until 2002,<br />

then operational datasets will be used.<br />

• It also uses Meteosat AMV´s reprocessed by Eumetsat and ERS-1 and ERS-2 altimeter and<br />

scatterometer data reprocessed by ESA.<br />

• It uses 1dVar+4dvar assimilation of rain-affected SSMI radiances.<br />

• It uses variational bias correction of all clear sky satellite radiances and automated bias<br />

correction for surface pressure observations.<br />

20

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