# JE3: Testing the radiation transport equation solver in a homogeneous slab¶

Contents

## Problem formulation and Fourier decomposition¶

In this entry I test the solver for the radiation transport equation (RTE) in a homogeneous slab. In addition to stand-alone use this solver can be used as a building block for solving the RTE in an inhomogeneous slab.

Although it might seem that the problem of the RTE in a slab is only of academic interest, it finds applications in understanding the radiation in the Earth’s (and other planetary) atmosphere and oceans. To an excellent approximation the atmosphere and the ocean can be treated as horizontally uniform with optical properties varying only with depth. See, for example, [Mobley1994] and [Thomas1999]. The key difficulty in solving the RTE for such applications is highly anisotropic scattering with a strong forward component. This requires the use of special algorithms to accurately handle the angular dependence of the radiation field.

The systematic study of the RTE was initiated by Subrahmanyan Chandrasekhar. He wrote a now-classic monograph [ChandraRT] (based on a series of his papers) in which he developed very elegant analytical methods to solve the RTE (including the effects of polarization) in homogeneous slabs. Chandra’s book is a tour de force in mathematical physics and has inspired several algorithms now in common use.

The RTE is a linear integro-differential equation and is written as

where

- \(L(\tau,\mu,\phi)\) is the radiance in units of Watt \(\mathrm{m}^{-2}\) \(\mathrm{sr}^{-1}\) \(\mathrm{nm}^{-1}\),
- \(0 < \tau < \tau_0\) is the optical depth,
- \(\varpi\) is the albedo of single scattering,
- \(\mu\) is the cosine of the polar angle measured with the positive \(Z\)-axis and \(\phi\) is the azimuthal angle,
- \(p(\cos\Theta) = \sum_{l=0}^L\beta_lP_l(\cos\Theta)\) is the phase function, where \(\Theta\) is the scattering angle and \(\beta_0=1\).

The boundary conditions are a directed beam incident at \(\tau=0\) and a “black” boundary at \(\tau=\tau_0\)

for \(\mu\in [0,1]\), and where

- \(\tau_0\) is the optical depth of the slab,
- \(\mu_0\) and \(\phi_0\) are the cosine of the polar angle and azimuthal angle of incident beam,
- \(\mu_0\pi F\) is the total downward irradiance incident on the slab.

The singular component of the radiance is removed using the decomposition

Where \(L_*(\tau,\mu,\phi)\) is the diffuse (scattered at least once) component of the radiance. Further, the addition theorem of spherical harmonics is used to write

where

are the normalized Legendre functions. The diffuse radiance is expanded in a Fourier cosine series as

Using these definitions the RTE becomes a set of equations for each Fourier component \(L^m(\tau,\mu)\)

and

The boundary conditions on each Fourier component become

The algorithm implemented in Lucee is described in full detail in a paper by Siewert [Siewert2000].

## Test Problems and Results¶

The test problems solved in this note are taken from [Garcia1985] that also lists very accurate benchmark results for these problem. For each problem the results computed with Lucee are plotted against the tabulated data in Garcia and Siewert.

### Problem 1¶

Mie scattering with \(L=8\) case for slab with \(\tau_0=1\), \(\mu_0 = 0.5\) and \(\varpi=0.95\).

Lucee results are compared to Garcia and Siewert results for Fourier modes \(m=0\) and \(m=1\).

### Problem 2¶

Haze-L phase-function case with \(L=82\) for slab with
\(\tau_0=1\), \(\mu_0 = 1.0\) and \(\varpi=0.9\). The
expansion coefficients of the phase function are available
`here`

.

### Problem 3¶

Same as Problem 2 except \(\mu_0=0.5\). 64 Fourier modes are used to compute the azimuthal dependence of the radiance.

### Problem 4¶

Same as Problem 2 except \(\varpi=1.0\). Note that Lucee can not actually handle this case of conservative scattering as the eigensystem is not complete when \(m=0\) and \(\varpi=1.0\). Hence, a modification of the algorithm is required to handle this by adding an eigenvector to complete the system. However, this modification is not implemented in Lucee. To overcome this we simply set \(\varpi=1-1\times 10^{-6}\).

## References¶

[Mobley1994] | C.D. Mobley, Light and Water. Radiative Transfer in
Natural Waters, Academic, New York, 2004. |

[Thomas1999] | G.E. Thomas and K. Stamnes, Radiative Transfer in the
Atmosphere and Ocean, Cambridge University Press, Cambridge UK,
1999. |

[ChandraRT] | S. Chandrasekhar, Radiative Transfer, Dover
Publications, 1960. |

[Siewert2000] | C.E. Siewert, “A concise and accurate solution to
Chandrasekhar’s basic problem in radiative transfer”, Journal of
Quantitative Spectroscopy & Radiative Transfer, 64,
Pg. 109-130, 2000. pdf. |

[Garcia1985] | R.D.M. Garcia and C.E. Siewert, “Benchmark Results in
Radiative Transfer”, Transport Theory and Statistical Physics,
14, No. 4 Pg. 437-483, 1985. pdf |