1 / 9

Radiative Transfer Model Vijay Natraj

Radiative Transfer Model Vijay Natraj. Why RADIANT?. The optical depth sensitivity of doubling The necessity of re-computing the entire RT solution if using a code such as DISORT if only a portion of the atmosphere changes

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? • The optical depth sensitivity of doubling • The necessity of re-computing the entire RT solution if using a code such as DISORT if only a portion of the atmosphere changes • Goal: Employ the strengths of both while leaving the undesirable characteristics behind

  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 for improved efficiency • 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. Obtaining Radiances at TOA RT Solution: I+(z*) = {T(0,z*)Rg[E-R(0,z*) Rg] -1T(z*,0) + R(z*,0) } I-(z*) + {T(0,z*)Rg[E-R(0,z*) Rg] –1R(0,z*) + T(0,z*)}agfoe-/o + T(0,z*)Rg[E-R(0,z*) Rg] –1S(z*,0) + S(0,z*)

  8. Numerical Efficiency: Eigenmatrix vs. Doubling

  9. Numerical Efficiency: RADIANT vs. DISORT

More Related