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Radiative Properties of Clouds ENVI3410 : Lecture 9 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds Cloud microphysics and precipitation Clouds and radiation Clouds and climate: forced changes to clouds Clouds and climate: cloud response to climate change
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Content of Lecture 9 Global radiation balance and the role of clouds Radiation interaction with cloud particles Shortwave radiation (Cloud albedo) Longwave radiation (emissivity) Net effect of clouds
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Atmospheric Radiation Streams Blackbody emission spectrum E= T 4 Sun’s shortwave energy arriving at Earth Earth’s emitted longwave (infrared) energy at the top of the atmosphere
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 strong IR absorption (GH effect) weak IR absorption at 8-14 m no visible light absorption weak near-IR absorption
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Global Energy Budget ~75% by clouds
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Problems to Solve How much solar SW radiation is reflected by a cloud and what physical properties of the cloud control the albedo? Is any solar radiation absorbed by a cloud? How much terrestrial (Earth) LW radiation is absorbed by clouds? What is the net effect of clouds on Earth’s energy balance and future changes to that balance?
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Radiation Interaction With Clouds Rays A-D are scattered (no loss of radiative energy) Ray E is absorbed (converted to heat) Scattering + absorption = extinction Scattered light gives cloud white appearance Intensity of direct beam progressively reduced inside cloud scattering absorption
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Microphysical Factors Affecting Scattering Scattering cross-section defined as Q sca = scattering efficiency (fraction of light scattered relative to shadow area) Q sca depends on –size of particle relative to wavelength of light –Index of refraction (real component)
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Scattering Efficiency, Q sca Q sca ~ 2 for cloud drops in visible light Q sca ~ variable for cloud drops in near IR Typical cloud droplets (visible light) Typical cloud droplets (terrestrial radiation) From Mie calculation
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Scattering Versus Drop Size for Constant LWC Assume single droplet size, Q sca = constant If LWC is constant, then Total light scattered in a thin cloud depends on Therefore, scattering efficiency of a cloud depends on Therefore, doubling N increases albedo by 25%, but thickness is also important
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Cloud Reflectivity in Solar Spectrum (SW) Visible light absorption negligible Some weak absorption in near-IR part of solar spectrum Cloud drop size and number is important in global energy balance 10 100 1000 0 20 40 60 80 100 2 4 8 16 liquid water path (g m -2 ) Reflectivity (%) 10 100 1000 0 20 40 60 80 100 cloud drop concentration (cm -3 ) Reflectivity (%) 50 100 500 1500 drop radius ( m) cloud thickness (m) LWC = 0.3 g m -3 16 2 Absorptivity (%)
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Mean Liquid Water Path
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Solar Radiation Intensity Through a Cloud Upward and downward SW radiation streams through a cloud above a surface of albedo = 0 0 200 400 600 800 1000 0 200 400 600 800 1000 SW intensity (W m -2 ) Height (m) SS SS Note rather slow decrease: Clouds need to be fairly thick to have a high albedo
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Clouds and LW Radiation Measured infrared spectrum of Earth from above a cloudless Sahara Desert 25 15 10 8 Wavelength / m blackbody curves for different temperatures Clouds absorb in the atmospheric window
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Cloud Absorptivity of IR Radiation 0 10 100 1000 0 0.2 0.4 0.6 0.8 1.0 liquid water path (g m -2 ) Absorptivity Some scattering remains, but cloud becomes close to a perfect emitter/absorber at low LWP Clouds are very efficient absorbers of LW across the entire terrestrial spectrum
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Solar (SW) and Terrestrial (LW) Radiation Intensity Through a Cloud 0 200 400 600 800 1000 0 200 400 600 800 1000 SW intensity (W m -2 ) Height (m) SS SS 280 300 320 340 360 380 0 200 400 600 800 1000 LW intensity (W m -2 ) Height (m) LL LL L and L in balance high LW downward flux below cloud strong LW cooling at cloud top
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Consequences of Different SW and LW Behaviours Clouds need to be relatively thick to have an albedo approaching 1.0 Even relatively thin clouds are good absorbers of LW radiation Thin cirrus clouds are effective LW absorbers but poor SW reflectors
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Consequences 290 280 250 210 Clear sky OLR through atmospheric window Ci: Small effect on albedo, large effect on OLR Sc: Large effect on albedo, small effect on OLR Cb: Large effect on albedo, large effect on OLR
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Albedo and OLR From ERBE ERBE = Earth Radiation Budget Experiment satellite low ScDeep Cb Ocean surface low Sc Deep Cb
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Net Radiation Balance
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Cloud Forcing low Sc cool in summer and Warm in winter Deep Cb small net radiative effect (SW cooling, LW heating)
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Net Effect of Clouds SW cooling LW heating Not complete cancellation, and depends on cloud type and season Next effect is global mean 15-20 Wm -2 cooling About 4-5 times radiative effect of CO 2 doubling Changes in cloud type/cover/properties have potential to affect climate
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ENVI3410 : Coupled Ocean & Atmosphere Climate Dynamics1 Reading/Further Investigation Read a description of ERBE Examine and understand further images http://cimss.ssec.wisc.edu/wxwise/homerbe.html
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