HR: 1330h
AN: A43A-08 [Abstracts]
TI: Implementation of NASA/GSFC GCE Ice Schemes into WRF
AU: * Shi, J J
EM: shi@agnes.gsfc.nasa.gov
AF: Science Applications International Corp, Maryland Corporate Center
Bldg 1, Suite 103
7501 Forbe Bldg, Seabrook, MD 20771
AU: Tao, W
EM: tao@agnes.gsfc.nasa.gov
AF: NASA/GSFC, Code 613.1
NASA/GSFC, Greenbelt, MD 20771
AB:
WRF is a next-generation mesoscale forecast model and assimilation system, which started with a blank sheet almost seven
years ago. The model has since incorporated modern advanced dynamics, numeric and data assimilation techniques, a multiple
relocatable nesting capability, and improved physical packages. WRF also adopted an advanced software framework to allow
incremental and reasonably rapid development towards full-functionality while maintaining overall consistency on its own
architecture and interface. The WRF model can be used for a wide range of applications, from idealized research to
operational forecasting, with an emphasis on horizontal grid sizes in the range of 1-10 km. The WRF is a prime candidate to
replace existing research and forecast models as MM5 users being strongly encouraged to begin transitioning to it. WRF
v2.0.3.1 was recently released in December 2004 with one-way/two-way interactive nesting, Eulerian mass coordinate, WRFSI
v2.0 and WRF 3DVAR v2.0. Several improvement are also undergoing among many WRF developer groups.
The current WRF includes 1) Lin et al. (1983), Kessler, and Ferrier microphysics schemes; 2) Kain-Fritsch, and
Betts-Miller-Janjic cumulus parameterization schemes; 3) Mellor-Yamada-Janjic PBL scheme; 4) GFDL, and Goddard (Chou)
shortwave radiation; 5) GFDL, and RRTM long-wave radiation and many other optional physical packages. Our group will
implement several ice schemes based on Tao et al. (2003), Goddard radiation (including explicitly calculated cloud optical
properties), LIS (including the CLM and NOAH land surface models), rainfall and bogus vortex assimilation techniques and
diagnostics into the WRF. We will perform benchmark cases from real case studies. In this meeting, we will present the
impact of the first phase of our endeavor resulted from adding several ice schemes (Tao et al. 2003) into WRF.
DE: 0300 ATMOSPHERIC COMPOSITION AND STRUCTURE
DE: 0320 Cloud physics and chemistry
SC: Atmospheric Sciences [A]
MN: 2005 Joint Assembly