smrt.emmodel.rayleigh module¶
Compute Rayleigh scattering. This theory requires the scatterers to be smaller than the wavelength and the medium to be sparsely populated (eq. very low density in the case of snow).
This model is only compatible with the Independent Sphere microstructure model

class
Rayleigh
(sensor, layer)¶ Bases:
object

basic_check
()¶

ft_even_phase_baseonUlaby
(m, mu_s, mu_i, npol=None)¶ # # Equations are from pg 11881189 Ulaby, Moore, Fung. Microwave Remote Sensing Vol III. # See also pg 157 of Tsang, Kong and Shin: Theory of Microwave Remote Sensing (1985)  can be used to derive # the Ulaby equations.

ft_even_phase_basedonJin
(m, mu_s, mu_i, npol=None)¶ Rayleigh phase matrix.
These are the Fourier decomposed phase matrices for modes m = 0, 1, 2. It is based on Y.Q. Jin
Coefficients within the phase function are:
 M = [Pvvp Pvhp]
 [Phvp Phhp]
Inputs are: :param m: mode for decomposed phase matrix (0, 1, 2) :param mu: vector of cosines of incidence angle
Returns P: phase matrix

ft_even_phase_tsang
(m, mu_s, mu_i, npol=None)¶ Rayleigh phase matrix.
These are the Fourier decomposed phase matrices for modes m = 0, 1, 2. Equations are from p128 Tsang Application and Theory 200 and sympy calculations
Coefficients within the phase function are:
 M = [PCvvp PCvhp PSvup]
 [PChvp PChhp PShup] [PSuvp PSuhp PCuup]
Inputs are: :param m: mode for decomposed phase matrix (0, 1, 2) :param mu: vector of cosines of incidence angle
Returns P: phase matrix

ft_even_phase
(m, mu_s, mu_i, npol=None)¶ # # Equations are from pg 11881189 Ulaby, Moore, Fung. Microwave Remote Sensing Vol III. # See also pg 157 of Tsang, Kong and Shin: Theory of Microwave Remote Sensing (1985)  can be used to derive # the Ulaby equations.

phase
(mu_s, mu_i, dphi, npol=2)¶

ke
(mu)¶ return the extinction coefficient

effective_permittivity
()¶
