The Delta–MMethod: Rapid Yet Accurate Radiative Flux Calculations for Strongly Asymmetric Phase Functions
- 1 September 1977
- journal article
- Published by American Meteorological Society in Journal of the Atmospheric Sciences
- Vol. 34 (9) , 1408-1422
- https://doi.org/10.1175/1520-0469(1977)034<1408:tdmrya>2.0.co;2
Abstract
The delta–M method represents a natural extension of the recently proposed delta–Eddington approximation to all orders M of angular approximation. It relies essentially on matching the first 2M phase function moments and using a Dirac delta–function representation of forward scattering. Computed fluxes are remarkably accurate at very low orders M of approximation, even when the phase function is strongly asymmetric; thus the associated M × M matrix computations remain small and manageable. Flux is automatically conserved, making phase function “renormalization” unnecessary. Phase function truncation is effected in a much more attractive manner than in the past; furthermore, truncation tends to zero as M → ∞. Errors are shown to oscillate with (roughly) exponentially decreasing amplitude as M increases; which has the curious consequence that increasing M by small amounts does not necessarily reduce error. Mie computations associated with the δ–M method can be considerably reduced, based on a simpl... Abstract The delta–M method represents a natural extension of the recently proposed delta–Eddington approximation to all orders M of angular approximation. It relies essentially on matching the first 2M phase function moments and using a Dirac delta–function representation of forward scattering. Computed fluxes are remarkably accurate at very low orders M of approximation, even when the phase function is strongly asymmetric; thus the associated M × M matrix computations remain small and manageable. Flux is automatically conserved, making phase function “renormalization” unnecessary. Phase function truncation is effected in a much more attractive manner than in the past; furthermore, truncation tends to zero as M → ∞. Errors are shown to oscillate with (roughly) exponentially decreasing amplitude as M increases; which has the curious consequence that increasing M by small amounts does not necessarily reduce error. Mie computations associated with the δ–M method can be considerably reduced, based on a simpl...Keywords
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