Super Cluster Expolsion

Objective Analysis for TOGA-COARE IOP

by Baode Chen (1996)


* About the Figure: GMS-4 Infrared Image (by courtesy of Dr. T. Nakazawa, MRI) and 200 HPa Divergent Wind of UCLA TOGA-COARE Analysis. 00UTC, Nov. 11, 1992


Using the NCEP/NCAR reanalysis as the first guess, we have performed objective analysis (successive correction method) of the final validated, high resolution (~5 hPa) sounding data (see the Priority Sounding Stations) for the Intensive Observation Period (IOP) (November 1992 - February 1993) of TOGA COARE. The product has two versions: (1) Large-domain analysis; the domain ranges from 90E to 170W and 30S to 30N on a 2.5 X 2.5 grid mesh, with a vertical resolution of 50 hPa from 1000 hPa to 50 hPa twice daily at 00 UTC and 12 UTC. (2) Small-domain analysis; the region is from 140E to 180E and 10S to 10N on a 1 X 1 grid mesh and the vertical resolution is 25 hPa with total of 39 levels from 1000 hPa to 50 hPa daily at 00, 06, 12, 18 UTC. Judged with OLR data and GMS brightness temperature, and compared with the grid data from the analyses of NCEP/NCAR, JMA(Japan Meteorological Agency) and ECMWF, which did not include all PSS data in their analyses, UCLA analysis provides a better representation of the atmospheric kinematic and thermodynamic characteristics during the COARE-IOP. However, the moisture field and the moisture budget residual Q2 appear to have some problems. The differences among the four different analyses become clearer for the derived quantities such as horizontal divergence.

 


Acknowledgements:

All figures displayed are produced with the Grid Analysis and Display System (GrADS), which is developed at the Center for Ocean-Land-Atmosphere Interaction, University of Maryland.

Please send your comments, suggestions, and questions to Baode Chen <baode@candor.gsfc.nasa.gov>