METO 621 Lesson 15. Prototype Problem #1 Semi-infinite slab.

Slides:



Advertisements
Similar presentations
Using a Radiative Transfer Model in Conjunction with UV-MFRSR Irradiance Data for Studying Aerosols in El Paso-Juarez Airshed by Richard Medina Calderón.
Advertisements

Variational Methods Applied to the Even-Parity Transport Equation
METO621 Lesson 18. Thermal Emission in the Atmosphere – Treatment of clouds Scattering by cloud particles is usually ignored in the longwave spectrum.
Lesson 3 METO 621. Basic state variables and the Radiative Transfer Equation In this course we are mostly concerned with the flow of radiative energy.
Atmospheric effect in the solar spectrum
Self-consistency of the RT solutions. Self-consistent solution of RT Take into account the intensity part of the source function (scattering) Construct.
Radiative Transfer Model Vijay Natraj. Welcome-2 Why RADIANT? Standard methods for multiple scattering RT calculations are: Standard methods for multiple.
METO 621 Lesson 9. Solution for Zero Scattering If there is no scattering, e.g. in the thermal infrared, then the equation becomes This equation can be.
Atmospheric scatterers
Page 1 Vijay Natraj Polarization November 9, 2007.
Radiative Transfer Model Vijay Natraj. Welcome-2 Why RADIANT? The optical depth sensitivity of doubling The optical depth sensitivity of doubling The.
METO 621 Lesson 13. Separation of the radiation field into orders of scattering If the source function is known then we may integrate the radiative transfer.
METO 621 Lesson 19. Role of radiation in Climate We will focus on the radiative aspects of climate and climate change We will use a globally averaged.
METO 621 Lesson 10. Upper half-range intensity For the upper half-range intensity we use the integrating factor e -  In this case we are dealing with.
METO 621 Lesson 11. Azimuthal Dependence In slab geometry, the flux and mean intensity depend only on  and . If we need to solve for the intensity.
METO 621 Lesson 16. Transmittance For monochromatic radiation the transmittance, T, is given simply by The solution for the radiative transfer equation.
METO 621 Lesson 14. Prototype Problem I: Differential Equation Approach In this problem we will ignore the thermal emission term First add and subtract.
Introduction to radiative transfer
Page 1 1 of 100, L2 Peer Review, 3/24/2006 Level 2 Algorithm Peer Review Polarization Vijay Natraj.
A 21 F A 21 F Parameterization of Aerosol and Cirrus Cloud Effects on Reflected Sunlight Spectra Measured From Space: Application of the.
Radiant 2.0: An Introduction Mick Christi OCO Science Meeting March 2004.
Solar Radiation Processes on the East Antarctic Plateau Stephen Hudson General Examination 7 June 2005.
METO 621 Lesson 12. Prototype problems in Radiative Transfer Theory We will now study a number of standard radiative transfer problems. Each problem assumes.
Light Scattering Rayleigh Scattering & Mie Scattering.
LESSON 4 METO 621. The extinction law Consider a small element of an absorbing medium, ds, within the total medium s.
4.8 Quadratic Formula and Discriminant
Ch. 5 - Basic Definitions Specific intensity/mean intensity Flux
Radiative Transfer Theory at Optical and Microwave wavelengths applied to vegetation canopies: part 2 UoL MSc Remote Sensing course tutors: Dr Lewis
CSE 872 Dr. Charles B. Owen Advanced Computer Graphics1 BSSRDF – Bidirectional surface scattering reflectance distribution function Radiance theory BRDF.
02/25/05© 2005 University of Wisconsin Last Time Meshing Volume Scattering Radiometry (Adsorption and Emission)
Multiple Scattering in Vision and Graphics Lecture #21 Thanks to Henrik Wann Jensen.
1 EE 543 Theory and Principles of Remote Sensing Derivation of the Transport Equation.
A discussion of Radiative Transfer Models Thomas J. Kleespies NOAA/NESDIS.
Ch. 5 - Basic Definitions Specific intensity/mean intensity Flux
1-1 Lesson 1 Objectives Objectives of Course Objectives of Course Go over syllabus Go over syllabus Go over course Go over course Overview of Course Overview.
Coherent backscattering and opposition phenomena exhibited by some atmosphere- less solar system bodies Janna M. Dlugach Main Astronomical Observatory.
1 Atmospheric Radiation – Lecture 9 PHY Lecture 10 Infrared radiation in a cloudy atmosphere: approximations.
Louie Grasso Daniel Lindsey A TECHNIQUE FOR COMPUTING HYDROMETEOR EFFECITVE RADIUS IN BINS OF A GAMMA DISTRIBUTION M anajit Sengupta INTRODUCTION As part.
DMRT-ML Studies on Remote Sensing of Ice Sheet Subsurface Temperatures Mustafa Aksoy and Joel T. Johnson 02/25/2014.
Computation of Polarized Subsurface BRDF for Rendering Charly Collin – Sumanta Pattanaik – Patrick LiKamWa Kadi Bouatouch.
Lesson 4: Computer method overview
1 Grey Atmosphere (Mihalas 3) Eddington Approximation Solution Temperature Stratification Limb Darkening Law Λ-iteration, Unsőld iteration Method of Discrete.
The Configuration Factors between Ring Shape Finite Areas in Cylinders and Cones Cosmin DAN, Gilbert DE MEY.
Green's function solution to subsurface light transport for BRDF computation Charly Collin – Ke Chen – Ajit Hakke-Patil Sumanta Pattanaik – Kadi Bouatouch.
Numerical Analysis. Numerical Analysis or Scientific Computing Concerned with design and analysis of algorithms for solving mathematical problems that.
1 Analytical Relations for the Transfer Equation (Mihalas 2) Formal Solutions for I, J, H, K Moments of the TE w.r.t. Angle Diffusion Approximation.
1 EEE 431 Computational Methods in Electrodynamics Lecture 7 By Dr. Rasime Uyguroglu
The Finite Element Method A self-study course designed for engineering students.
1 Atmospheric Radiation – Lecture 9 PHY Lecture 9 Infrared radiation in a cloudy atmosphere.
Radar Bands Letters chosen during WWII. X-band so-named b/c it was kept secret during the war.
Retrieval of cloud parameters from the new sensor generation satellite multispectral measurement F. ROMANO and V. CUOMO ITSC-XII Lorne, Victoria, Australia.
Solve Equations With Variables on Both Sides. Steps to Solve Equations with Variables on Both Sides  1) Do distributive property  2) Combine like terms.
1 Equation of Transfer (Mihalas Chapter 2) Interaction of Radiation & Matter Transfer Equation Formal Solution Eddington-Barbier Relation: Limb Darkening.
Martin-Gay, Developmental Mathematics 1 Warm-Up #28 (Thursday, 11/12)
Basic Definitions Specific intensity/mean intensity Flux
(A) Future of Radiation Parameterizations in CAM Bill Collins National Center for Atmospheric Research
Hanyang University 1/18 Seminar on Microwave and Optical Communication Wonhong Jeong
Visualization Techniques for Discrete Ordinates Method Radiation Transport Cornelius Toole Lawrence Berkeley National Laboratory Jackson State University.
Lecture 8: Stellar Atmosphere 3. Radiative transfer.
Slide 1 Robin Hogan, APRIL-CLARA-DORSY meeting 2016 ©ECMWF Towards a fast shortwave radiance forward model for exploiting MSI measurements Robin Hogan.
Spatial treatment in 1D Slab Discrete Ordinates
Recap and iteration practice Reduction of B.E. to 1D 1D Quadratures
Class Notes 19: Numerical Methods (2/2)
The Finite Element Method
The GIFTS Fast Model: Clouds, Aerosols, Surface Emissivity
Investigators Tony Johnson, T. V. Hromadka II and Steve Horton
Solving Multi-Step Equations
Analytical Relations for the Transfer Equation (Hubeny & Mihalas 11)
The Transport Equation
Distribute and combine like terms
Presentation transcript:

METO 621 Lesson 15

Prototype Problem #1 Semi-infinite slab

Prototype Problem #1 Angular distribution of the Intensity

Adding-Doubling Techniques Consider two layers in the atmosphere with the same reflectance and transmittance. Then the combined reflectance and transmittance of the two layers can be written as

Adding-Doubling Techniques

The advantage of the technique is that one can start with thin layers – small optical depths – which are easier to handle mathematically. There is no limit as to how many of the layers one eventually adds. If the two layers are dissimilar, then we must take into account that the transmittance and reflectance will be different for illumination from above and below. The equations for the combined reflectance and transmittance can also be determined.

Adding-Doubling Techniques From above From below

Adding-Doubling Techniques

Discrete Ordinate Method – Isotropic Scattering The solution of the isotropic scattering problem involves the following integral over angle In the two stream method we replaced the integration over  with the simple formula

Discrete Ordinate Method – Isotropic Scattering This is obviously a crude approximation. We can improve the accuracy by including more points in a numerical quadrature formula Where w’ j is a quadrature weight, and u j is the discrete ordinate Most commonly used radiative transfer computer codes is DISORT – DIScreteOrdinateRadiativeTransfer