Abstract
The theory of radiative transfer in turbid media was developed well enough for solving problems in astrophysics, nuclear physics and atmospheric physics (Davison 1958; Marchuk 1961 on the process of neutron transfer; Chandrasekhar 1950; Sobolev 1963 on astrophysical problems; Vladimirov 1961; Case and Zweifel 1967 for a mathematical description of transport theory). A formal way of developing radiative transfer theory in leaf canopies using the analogy of a turbid layer can be found in Shifrin (1953). Ross and colleagues further developed the theory in the mid 1960s (Ross 1962, 1964; Ross and Nilson 1963, 1965, 1967, 1968a, b: Nilson 1968a, b; Niilisk and Ross 1969).
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Abbreviations
- as(z, Ω′̱ → Ω̱):
-
new scattering cross-section
- g(z, Ω̱·Ω̱′):
-
any rotationally invarianted scattering phase function
- G1(L, Ω′̱):
-
diffuse component of area scattering cross-section Ψ(L, Ω′̱)
- G2(L, Ω′̱):
-
specular component of area scattering cross-section Ψ(L, Ω′̱)
- I′0 :
-
constant denoting the direct radiation attenuated by the atmosphere
- In(z, Ω̱):
-
n-th approximation to the solution of the transfer equation
- Iun(L, Ω̱):
-
uncollided radiation
- Iun 1(L, Ω̱):
-
incident diffuse radiation stream that has not undergone any interactions in the canopy
- Iun 2(L, Ω̱):
-
incident direct radiation stream that has not undergone any interactions in the canopy
- Ic(L, Ω̱):
-
radiance of photons which have been scattered one or more times in the canopy
- Ic 1(L, Ω̱):
-
first-order scattering radiance when a monodirectional stream of photons escapes the source
- Ic M(L, Ω̱):
-
radiance of multiply scattered photons
- Jk(z, Ω̱):
-
radiance of the photons scattered k times
- lL :
-
length of the mean chord of the leaf
- l*L = lL/H:
-
parameter characterizing the leaf dimensions
- rΩ0,Ω :
-
correlation function
- R(Ω̱′, Ω̱):
-
canopy bidirectional reflectance factor
- Ra(Ω̱′, Ω̱):
-
bidirectional reflectance factor of the atmosphere
- Rs(Ω̱′, Ω̱):
-
bidirectional reflectance factor of the soil
- SOSA:
-
successive orders of scattering approximation
- t1 :
-
computer time needed for calculating one iteration
- t2 :
-
computer time spent on additional operations
- y(L, Ω̱):
-
solution of the integral transfer equation
- Z:
-
geometrical depth of the atmosphere
- α:
-
angle between the leaf normal and the photon incident direction
- α′:
-
angle between the leaf normal and the photon exit direction
- ΓD, (L, Ω̱′ → Ω̱):
-
diffuse component of the area scattering phase function
- ΓS, (L, Ω̱′ → Ω̱):
-
specular component of the area scattering phase function
- δ2 (Ω̱·Ω̱′):
-
surface delta function
- εn :
-
parameter characterizing convergence of the iterative process
- η1, η2 :
-
given accuracies
- λ(r, Ω̱):
-
analogy of albedo for single scattering
- μ*L :
-
cos θ*L
- ρc :
-
rate of convergence of the iterative process
- σ′(L, Ω̱0, Ω̱):
-
new total interaction cross-section
- τ(z′, z, Ω̱):
-
optical depth between the points z′ and z along the direction Ω̱
- T :
-
optical depth of the atmosphere
- Ω̱*:
-
direction of specular reflection
- Ω̱± :
-
part of the hemisphere in which ± (Ω̱′ Ω̱L)(Ω̱ Ω̱L) - 0
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Knyazikhin, Y., Marshak, A. (1991). Fundamental Equations of Radiative Transfer in Leaf Canopies, and Iterative Methods for Their Solution. In: Myneni, R.B., Ross, J. (eds) Photon-Vegetation Interactions. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-75389-3_2
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DOI: https://doi.org/10.1007/978-3-642-75389-3_2
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