effective transport kernels for spatially correlated media, application to cloudy atmospheres...

Download Effective Transport Kernels for Spatially Correlated Media, Application to Cloudy Atmospheres Anthony B. Davis Los Alamos National Laboratory Space & Remote

If you can't read please download the document

Upload: gloria-lucas

Post on 13-Dec-2015

216 views

Category:

Documents


4 download

TRANSCRIPT

  • Slide 1

Effective Transport Kernels for Spatially Correlated Media, Application to Cloudy Atmospheres Anthony B. Davis Los Alamos National Laboratory Space & Remote Sensing Sciences Group (ISR-2) with help from many others LA-UR-04-6228 Slide 2 Key References 1.Davis, A., and A. Marshak, L vy kinetics in slab geometry: Scaling of transmission probability, in Fractal Frontiers, M. M. Novak and T. G. Dewey (eds.), World Scientific, Singapore, pp. 63-72 (1997). 2.Pfeilsticker, K., First geometrical pathlength distribution measurements of skylight using the oxygen A-band absorption technique - II, Derivation of the L vy-index for skylight transmitted by mid-latitude clouds, J. Geophys. Res., 104, 4101-4116 (1999). 3.Buldyrev, S. V., S. Havlin, A. Ya. Kazakov, M. G. E. da Luz, E. P. Raposo, H. E. Stanley, and G. M. Viswanathan, Average time spent by L vy flights and walks on an interval with absorbing boundaries, Phys. Rev. E, 64, 41108-41118 (2001). 4.Kostinski, A. B., On the extinction of radiation by a homogeneous but spatially correlated random medium, J. Opt. Soc. Am. A, 18, 1929-1933 (2001). 5.Davis, A. B., and A. Marshak, Photon propagation in heterogeneous optical media with spatial correlations: Enhanced mean-free-paths and wider-than-exponential free-path distributions, J. Quant. Spectrosc. Rad. Transf., 84, 3-34 (2004). 6.Davis, A. B., and H. W. Barker, Approximation methods in three-dimensional radiative transfer, in Three-Dimensional Radiative Transfer for Cloudy Atmospheres, A. Marshak and A. B. Davis (eds.), Springer-Verlag, Heidelberg (Germany), to appear (2004). and others, as we proceed Slide 3 Outline Motivation & Background (atmospheric radiation science only) Mean-field transport kernels Heuristic scattering-translation factorization Directional diffusion: Transport MFP revisited Spatial impact: Non-exponential tails Implications for effective medium theories (homogenization) Anomalous photon diffusion: The basic boundary-value problem Time-dependent (first, then ) Steady-state Observational corroborations Time-domain lightning observations Fine spectroscopy in oxygen absorption lines/bands Summary & Outlook Slide 4 Ren Magritte, 1929 Motivation, 1: Surrealism Slide 5 Motivation, 2: State-of-the-Art Conceptual Models inside operational cloud remote sensing schemes (chez NASA et Co.), and inside any Global Climate Models radiation module This is a cloud. Slide 6 Motivation, 3: Reality! from Space Shuttle archive (courtesy Bob Cahalan) Slide 7 Approximation theory in atmospheric radiative transfer: Needs assessment Variability: Resolved or not? in computational grid in observations (pixels) Slide 8 Large-scale radiation budget estimation: Unresolved variability effects Clear-cloudy separation (70s - 80s) The cloud fraction enters A correlation scale enters: Stochastic RT in Markovian binary media The Independent-Column Approximation (ICA) limit for very large aspect ratios Cloudy part gets variable Stephens closure-based effective medium theory (1988) Davis et al.s parameterization with power-law rescaling (1991) Cahalans ICA-based effective medium theory (1994) Barkers Gamma-weighted/2-stream ICA (1996) More effective medium theories Cairns et al.s renormalization theory (2000) Pettys cloudets (2002): large clumps as scattering entities Recent numerical solutions for GCM consumption And what about cloud overlap (vertical correlation)? The McICA Project (2003-) Slide 9 Some definitions in 3D Radiative Transfer Slide 10 Directional diffusion Slide 11 Directional diffusion: Spatial impact After n* (1g) 1 scatterings, directional memory is lost. Slide 12 Directional diffusion and its spatial impact illustrated in 2D Slide 13 Effective (i.e., mean) transport kernels: the actual photon free-path distributions Slide 14 Need for long-range spatial correlations! Slide 15 Synthetic scale-invariant media that are turbulence-like Slide 16 Three remarkable properties of effective free-path distributions For 2.-3., using a very different approach, see: Kostinski, A. B., 2001: On the extinction of radiation by a homogeneous but spatially correlated random medium, J. Opt. Soc. Am. A, 18, 1929-1933. Slide 17 Variability scales of 3D-transport interest? Consider extinction (x) or local (pseudo-)MFP 1/ (x). How much does it typically change, on a relative scale, between two discrete transport events (emission or injection, scattering, absorption or escape)? N.B. Extreme cases are well-known in stochastic RT theory for binary Markovian media, respectively, the limits of: a. atomistic mixing (i.e. optical homogeneity using mean values); c. linear mixing by volume fraction (a.k.a. the ICA/IPA in atmospheric work). Slide 18 An illustration with binary media: Implications for effective medium theories: * will all fail at large-enough scales; * watch for correlations over the (actual) MFP. Slide 19 Expectations for Earths cloudy atmosphere, 1: Barker et al.s (1996) LandSat Analysis From: Gamma distributions capture many cloud optical depth scenarios. Slide 20 Expectations for Earths cloudy atmosphere, 2: Effective transport kernels are power-law Assuming s = H (thickness) in previous slide: Slide 21 Solar photons multiply scattering in the cloudy atmosphere Slide 22 Anomalous diffusion through a finite medium: Time-dependence for transmission from free space to a finite slab (thickness H): Slide 23 Anomalous diffusion through a finite medium: Steady-state transmission from a half-space to a finite slab (thickness H): For a more rigorous approach: Slide 24 Observations, 1a: Differential absorption spectroscopy at very high resolution From: Min Q.-L., L. C. Harrison, P. Kiedron, J. Berndt, and E. Joseph, 2004: A high-resolution oxygen A-band and water vapor band spectrometer, J. Geophys. Res., 109, D02202, doi:10.1029/2003JD003540. x-section density pathlength Slide 25 Observations, 1b: Ground-based Oxygen Spectroscopy Cases near the =2 line are very overcast, and those near =1 are for sparse clouds, as expected from model. A single cloud layer ( =2) with variable thickness H the slope of the linear path vs optical depth plot. A complex cloud situation (1<