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Boundary Layer Clouds St & Sc Stratus and stratocumulus Transition Trade cumulus Intertropiccal Convergence Zone (ITCZ) SGP Low cloud coverage (ceilometer & MPL): 27.8% (Lazarus et al. 2000) Cooling effect Warming effect NASA: The Earth Radiation Budget Experiment (ERBE) It measures the energy budget at the top of the atmosphere. Energy budget at the top of atmosphere (TOA) Incoming solar radiation 340 W/m2 Reflected SW radiation Q1= 50 W/m2 Fictitious climate system No clouds Incoming solar radiation 340 W/m2 Reflected SW radiation Q= 100 W/m2 shortwave cloud forcing dQ=Q1-Q=-50 W/m2 (cooling) Emitted LW radiation F1= 270 W/m2 Emitted LW radiation F= 240 W/m2 longwave cloud forcing dF=F1-F=30 W/m2 (warming) Present climate system with clouds SW cloud forcing = clear-sky SW radiation – full-sky SW radiation LW cloud forcing = clear-sky LW radiation – full-sky LW radiation Net cloud forcing (CRF) = SW cloud forcing + LW cloud forcing Current climate: CRF = -20 W/m2 (cooling) But this does not mean clouds will damp global warming! The impact of clouds on global warming depends on how the net cloud forcing changes as climate changes. Direct radiative forcing due to doubled CO2, G = 4 W/m2 0 positive cloud feedback CRF G 0 zero cloud feedback 0 negative cloud feedback e.g. If the net cloud forcing changes from -20 W/m2 to -16 W/m2 due to doubling CO2, the change of net cloud forcing will add to the direct CO2 forcing. The global warming will be amplified by a fact ofCRF 2. - 16 - (-20) 4 W/m 2 Cloud radiative effects depend on cloud distribution, height, and optical properties. Low cloud High cloud Tc Tc Tg Tc Ta Tc Ta Tg SW cloud forcing dominates LW cloud forcing dominates In GCMs, clouds are not resolved and have to be parameterized empirically in terms of resolved variables. water vapor (WV) cloud surface albedo lapse rate (LR) WV+LR ALL Issues LS Forcing Cloud evolution and maintenance. Cloudiness . Radiation Turbulence Microphysics Radiative and microphysical properties. Cloud entraining processes and cloud mass transport. Cloud mesoscale organizations. Surface Processes Cloud-aerosol-drizzle interactions Mesoscale cellular convection (MCC) Pockets of open cell (POCS) Variations of MCCs and POCs are much larger than the individual variations within the structures (Jensen et al. 2008) Aerosol feedback Direct aerosol effect: scattering, reflecting, and absorbing solar radiation by particles. Primary indirect aerosol effect (Primary Twomey effect): cloud reflectivity is enhanced due to the increased concentrations of cloud droplets caused by anthropogenic cloud condensation nuclei (CNN). Secondary indirect aerosol effect (Second Twomey effect): 1. Greater concentrations of smaller droplets in polluted clouds reduce cloud precipitation efficiency by restricting coalescence and result in increased cloud cover, thicknesses, and lifetime. 2. Changed precipitation pattern could further affect CCN distribution and the coupling between diabatic processes and cloud dynamics. Parameterization Development and Testing Strategy GCM /NW P PAR CRMS LES OBS Hi-Res simulation s and 3-D Observations Traditional LES: idealized initial profiles and prescribed horizontal homogeneous large-scale forcings. Representativeness of clean cloud cases? Clouds Liquid water mixing ratio Liquid water density of clouds l wl air Cloud droplet distribution Number density N (D): the number of droplets per nit volume (concentration) in an interval D + ΔD wl mass liquid mass dry air l mass liquid volume of dry air mass of a droplet l 6 D 3 Liquid water content L 6 l N i ( Di ) Di3 Variables that are useful for cloud research Mixing ratio, saturated mixing ratio, liquid water mixing ratio, total mixing ratio r , rs , rl , rt v (1 0.608r rl ) e Lv r C pT l CLT rl p es Lv rs C pT Equivalent potential temperature Liquid water potential temperature Saturated quivalent potential temperature Instrumentation Latest version W-band (95 GHz)cloud radar Millimeter Wave Cloud Radar (35 GHz) X-band scanning ARM precipitation radar Vaisala Ceilometer Mechanisms of maintaining cloud-topped boundary layer 1. Surface forcing 2. Cloud top radiative cooling 3. Cloud top evaporative cooling Cloud parameterization 1. Cloud fraction parameterization Shallow cumulus parameterization: Mass-flux approach Fcu w M c (c e ) , M c (1 )(w c w e ), c (1 )c Entraining plume model c (c ) z 1 M c Mc z 1. How to close the system? 2. How to determine entrainment and detrainment rates? Stratocumulus parameterization Cloud top entrainment parameterization Eddy viscosity A1, A2: empirical coefficients. V: turbulent velocity scale. ΔF: cloud-top radiative flux divergence. ΔB: buoyance jump across the inversion.