Abstract:
Land surface (or 'skin') temperature (LST) lies at the heart of the surface
energy balance and is a key variable in weather and climate models. Here we
assimilate LST retrievals from the International Satellite Cloud Climatology
Project (ISCCP) into the Noah and Catchment (CLSM) land surface models
using an ensemble-based, off-line land data assimilation system. LST is
described very differently in the two models. A priori scaling and dynamic
bias estimation approaches are applied because satellite and model LST
typically exhibit different mean values and variability. Performance is
measured against 27 months of in situ measurements from the Coordinated
Energy and Water Cycle Observations Project at 48 stations. LST estimates
from Noah and CLSM without data assimilation ('open loop') are comparable
to each other and superior to that of ISCCP retrievals. For LST, RMSE
values are 4.9 K (CLSM), 5.5 K (Noah), and 7.6 K (ISCCP), and anomaly
correlation coefficients (R) are 0.61 (CLSM), 0.63 (Noah), and 0.52
(ISCCP). Assimilation of ISCCP retrievals provides modest yet statistically
significant improvements (over open loop) of up to 0.7 K in RMSE and 0.05
in anomaly R. The skill of surface turbulent flux estimates from the
assimilation integrations is essentially identical to the corresponding open
loop skill. Noah assimilation estimates of ground heat flux, however, can be
significantly worse than open loop estimates. Provided the assimilation
system is properly adapted to each land model, the benefits from the
assimilation of LST retrievals are comparable for both models.