comparison of ritter-geleyn radiaton code to lbl model rtx
DESCRIPTION
7th COSMO General Meeting 20-23 september 2005, Zurich (CH). COMPARISON OF RITTER-GELEYN RADIATON CODE TO LBL MODEL RTX. PRELIMINARY RESULTS. Alessio Bozzo – ADGB Phys. dep. Univ. of Bologna ARPA-SIM. MOTIVATIONS. - PowerPoint PPT PresentationTRANSCRIPT
COMPARISON OF RITTER-GELEYN RADIATON CODE
TO LBL MODEL RTXPRELIMINARY RESULTS
Alessio Bozzo – ADGB Phys. dep. Univ. of Bologna
ARPA-SIM
7th COSMO General Meeting
20-23 september 2005, Zurich (CH)
MOTIVATIONS
• test the fast -two stream radiation code GRAALS with the LbL-multiple scattering model RTX
• particolar attention is paid to the comparison between the treatement of gases, clouds and aerosols optical properties
MODELS OVERVIEW: RTX
• Benchmark model: RTX
– LbL radiation code.
– Spectroscopic database based on HITRAN2000 from FIR to 0.4 m
– cirrus cloud single scattering optical properties for spherical, hexagonal and aggregate crystals
– “exact” multiple scattering computation of cloud and Rayleigh layers via adding-and-doubling method
MODELS OVERVIEW:GRAALS
• GRAALS (General Radiative Algorithm Adapted to Linear-type Solutions, Ritter/Geleyn 1991)– fast -two stream radiation code with
treatement of partial cloudiness– optical properties of clouds and gases
parameterized over 8 wide spectral intervals from VIS (0.2m) to FIR (104.5m) based on AFGL ’84 database
COMPARISON SETTINGS
• Surface type: Lambertian• Gaseous absorption: CO2, H2O, O3, N2O, O2, CO, CH4
for both models. RTX consider also trace gases as CFCs (F11, F12, CCl4), NO, NO2, SO2, N2.
• Monocromatic RTX fluxes grouped in GRAALS bands. Spectroscopic database of RTX extend from FIR to 0.4m. In solar region the comparison covers only 2 of the 3 GRAALS solar bands (i.e. the VIS range 0.2-0.7m is not taken into account for now)
SCENARIO-1: CLEAR
standard tropical profile
solar zenith angles: 0°, 45°, 60°
H2O mixing ratio (g/kg)
O3 mixing ratio (g/kg)
Solar spectrum in GRAALS is all
distributed from 0.2 to 4.5m
CO2
CO2,H2O
O3
H2O
Sun zenith angle=60°
TOA and SURFACE NET Fluxes RTX-GRAALS (%)
TOA FLUXES
SURFACE FLUXES
Solar spectrum (0.7-4.6um)
Thermal spectrum (4.6-104.5um)
UP- FLUX -12.3% -4.6%
DOWN - FLUX -4.4%
Solar spectrum (0.7-4.6um)
Thermal spectrum (4.6-104.5um)
UP - FLUX 12.9% -0.8%
DOWN - FLUX -8.8% 0.7%
Contribute due to FIR H2O band (20-104m)
Contribute due to CO2 band (12-20m)
Contribute due to O3 band (9-10m)
VIS and UV O3 band: work in progress...
– standard tropical profile with different cloud types at various heights (overcast homogeneus layers)
– solar zenith angle 0°, 45°, 60°
• low-level thick water cloud– 850-715hPa (1500m thick); LWC=0.5 g/m3,
re=9.3m
• medium-level water cloud– 672-633 hPa (500m thick); LWC=0.129 g/m3,
re=5.2m
• high-level cloud– 266-247 hPa (500m thick); LWC=0.013 g/m3,
re=4.1m
SCENARIO-2: CLOUDY
Sun zenith angle=60°
FURTHER WORK• Improve the parameterization of ice clouds with
the most advanced particle shapes (aggregate, columns, hex. plates) (collaboration with UK Met Office)
• Re-compute the gaseous optical properties using the last HITRAN2004 spectroscopic database (work in progress by F.Geleyn)
• Compare the treatement of aerosol in GRAALS with the latest OPAC database in RTX (Hess, Koepke, and Schult, 1998)