Localizing the impact of satellite radiance observations using a global group ensemble filter

Results from an idealized simulation with known background error covariances show that the GGF localization function is superior to the optimal Gaspari and Cohn (GC) localization function. When the GGF is applied to the AMSU-A radiances, it can provide different localization functions for different channels, which indicates the complexity and large computational cost of tuning the localization scales for radiance observations.

The GC, GGF, and fitted GGF (FGGF) localization functions are compared using experiments with the NCEP GFS and the NOAA operational EnKF. Verifications relative to the conventional observations, AMSU-A radiances, and the ECMWF analyses show that the GGF and FGGF have smaller errors than GC except in the tropics, and the advantages of the GGF and FGGF persist through 120 h forecast lead time.