1 / 8

Radiative Transfer Model Vijay Natraj

Radiative Transfer Model Vijay Natraj. Why RADIANT?. Standard methods for multiple scattering RT calculations are: Eigenmatrix (e.g. DISORT) Doubling-adding Doubling methods are inefficient for optically thick layers

fola
Download Presentation

Radiative Transfer Model Vijay Natraj

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Radiative Transfer Model Vijay Natraj

  2. Why RADIANT? • Standard methods for multiple scattering RT calculations are: • Eigenmatrix (e.g. DISORT) • Doubling-adding • Doubling methods are inefficient for optically thick layers • Eigenmatrix methods re-compute entire atmosphere even if properties change only in one layer (e.g., computing PDs) • Goal: Remove above weaknesses

  3. RADIANT: Overview • Plane-parallel, multi-stream RT model • Allows for computation of radiances for user-defined viewing angles • Includes effects of absorption, emission, and multiple scattering • Can operate in a solar only, thermal only, or combined fashion • Allows stipulation of multiple phase functions due to multiple constituents in individual layers • Allows stipulation of the surface reflectivity and surface type (lambertian or non-lambertian)

  4. RADIANT: Solution Methodology • Convert solution of the RTE (a boundary value problem) into a initial value problem • Using the interaction principle • Applying the lower boundary condition for the scene at hand • Build individual layers (i.e. determine their global scattering properties) via an eigenmatrix approach • Combine layers of medium using adding to build one “super layer” describing entire medium • Apply the radiative input to the current scene to obtain the RT solution for that scene The Interaction Principle I+(H) = T(0,H)I+(0) + R(H,0)I-(H) + S(0,H) Lower Boundary Condition: I+(0) = RgI-(0) + agfoe-/o

  5. Operational Modes: Normal

  6. Operational Modes: Layer Saving

  7. Numerical Efficiency: Eigenmatrix vs. Doubling Send to first page

  8. Numerical Efficiency: RADIANT vs. DISORT2 Show new figure

More Related