Single-Scattering Stuff + petty chap 12 intro April 27-29, 2015.

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Presentation transcript:

Single-Scattering Stuff + petty chap 12 intro April 27-29, 2015

Reminders Project 2 due this Friday – Rob laid up but will answer s, or come see me! ( first) Homework 4 will be handed out soon, due Friday May 8. Course evals likely Friday may 8 also. Final Thursday May 14

Upwelling Radiance At TOA: Downwelling Radiance at Surface: In the limit of τ * << 1: direct beam Singly-scattered radiance direct beam Singly-scattered radiance direct beam

Limits of the approximation? Thin aerosol layers, rayleigh atmosphere, optically thin clouds. If the sun is too low on horizon, it will break. If the view angle is too close to horizon, it will break. If ωτ * >~ 0.5, it will break: i.e., most cloudy situations.

Single-Scattering Approximation: Behavior vs. Optical depth of scattering layer

Application Let’s attempt to determine the clear-sky flux reflectivity of the atmosphere, due to Rayleigh-scattering of gas molecules in the atmopshere. Result will depend strongly on wavelength, but we can solve it generally… Will not worry about photons scattered off surface (just atmosphere).

Pieces to think about How is F defined?: integral over a hemisphere of F mu. How is flux reflectivity defined?: Fout/Fin

Back to Phase Function “Asymmetry Parameter” Equivalent to:

Useful phase function: “Henyey-Greenstein Phase Function” Function of g only Not a “real” phase function – but can be useful in certain applications when the real phase function is too hard to deal with

Useful phase function: “Henyey-Greenstein Phase Function” Function of g only Not a “real” phase function – but can be useful in certain applications when the real phase function is too hard to deal with Forward Scattering Backward Scattering

Phase Function of water spheres (Mie theory) Low Asymmetry Parameter High Asymmetry Parameter

The range of atmospheric scatterers

Scattering by particles: clouds, precip, aerosols, air Intrinsic properties: Extinction efficiency single scattering albedo phase function Extrinsic properties: Scattering optical depth Emissivity Spherical albedo Transmissivity

Rayleigh Scattering: Geometry & Polarization Very small scatterer acts like a pure dipole!

Vertical Incoming Polarization Horizontal Incoming Polarization Incoming Light Unpolarized Scattered electric field (polar plot)

Rayleigh Optical Properties of a small sphere (x<<1) (slightly more accurate equation in book)

The Rayleigh-regime Single Scattering Albedo If imag(m) > 0, then there will be almost no scattering. However, if imag(m) is tiny (<~ 1e-7), then there can be appreciable scattering. For molecular (rayleigh scattering), it is in the “window” regime by definition – absorption is treated separated because they have such different wavelength-dependence – so ssa=1.

“Absorbing Rayleigh” (e.g., cloud droplets in the microwave) Cloud droplet radii: r = 10 μm (4-25 μm) Microwave Wavelength: λ = 1 cm (0.2 – 5 cm) x = 2πr/λ= So τ cloud = k a  (Cloud Liquid water Path in kg m -2 )

Mie Theory Input – Size parameter x of particle – Relative index of refraction m (real, imaginary) Output – Qe, Qs, Qa, single-scattering Albedo – 6x6 “Phase Matrix” with 4 independent elements – P(1,1) function is the Intensity phase function P(Θ)

Phase Function of water spheres (Mie theory) Low Asymmetry Parameter High Asymmetry Parameter

Mie Theory Results Exact Qs, Qa for spheres of some x, m. a, b coefficients are called “Mie Scattering coefficients”, functions of x & m. Easy to program up. “bhmie” is a standard code to calculate Q-values in Mie theory. Need to keep approximately x + 4x 1/3 + 2 terms for convergence

Q e for NON- ABSORBING SPHERES

Mie Theory Results for ABSORBING SPHERES

Variations of SSA with wavelength Non- Absorbing! Somewhat Absorbing

Satellite retrieve of cloud optical depth & effective radius Non-absorbing Wavelength (SSA~1): Reflectivity is mainly a function of optical depth. Absorbing Wavelength (SSA < 1): Reflectivity is mainly a function of cloud droplet size (for thicker clouds).

Distributions of Particles

Radar Bands Letters chosen during WWII. X-band so-named b/c it was kept secret during the war.