ARTS
2.0.49
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Go to the source code of this file.
Functions | |
Numeric | dinvplanckdI (const Numeric &i, const Numeric &f) |
dinvplanckdI More... | |
void | fresnel (Complex &Rv, Complex &Rh, const Complex &n1, const Complex &n2, const Numeric &theta) |
fresnel More... | |
Numeric | invplanck (const Numeric &i, const Numeric &f) |
invplanck More... | |
Numeric | invrayjean (const Numeric &i, const Numeric &f) |
invrayjean More... | |
Numeric | number_density (const Numeric &p, const Numeric &t) |
number_density More... | |
Numeric | planck (const Numeric &f, const Numeric &t) |
planck More... | |
Numeric | rayjean (const Numeric &f, const Numeric &t) |
rayjean More... | |
This file contains declerations of functions of physical character.
Definition in file physics_funcs.h.
dinvplanckdI
Calculates the derivative of inverse-Planck with respect to intensity.
i | radiance |
f | frequency |
Definition at line 71 of file physics_funcs.cc.
References BOLTZMAN_CONST, PLANCK_CONST, and SPEED_OF_LIGHT.
Referenced by apply_y_unit2().
void fresnel | ( | Complex & | Rv, |
Complex & | Rh, | ||
const Complex & | n1, | ||
const Complex & | n2, | ||
const Numeric & | theta | ||
) |
fresnel
Calculates complex AMPLITUDE reflection coeffcients for a specular reflection
The properties of the two involved media are given as the complex refractive index, n. A dielectric constant, eps, is converted as n = sqrt( eps ). The power reflection coefficient, r, for one polarisation is r = abs(R)^2.
Rv | Out: Reflection coefficient for vertical polarisation |
Rh | Out: Reflection coefficient for vertical polarisation |
n1 | In: Refractive index of medium where radiation propagates |
n2 | In: Refractive index of reflecting medium |
theta | In: Propagation angle from normal of radiation to be reflected |
Definition at line 110 of file physics_funcs.cc.
References DEG2RAD.
Referenced by surfaceFlatRefractiveIndex().
invplanck
Converts a radiance to Plack brightness temperature.
i | radiance |
f | frequency |
Definition at line 142 of file physics_funcs.cc.
References BOLTZMAN_CONST, PLANCK_CONST, and SPEED_OF_LIGHT.
Referenced by apply_y_unit().
invrayjean
Converts a radiance to Rayleigh-Jean brightness temperature.
i | radiance |
f | frequency |
Definition at line 170 of file physics_funcs.cc.
References BOLTZMAN_CONST, and SPEED_OF_LIGHT.
Referenced by apply_y_unit(), apply_y_unit2(), doit_conv_flagAbsBT(), doit_conv_flagLsq(), iyMC(), MCGeneral(), and MCIPA().
number_density
Calculates the atmospheric number density.
p | pressure |
t | temperature |
Definition at line 195 of file physics_funcs.cc.
References BOLTZMAN_CONST.
Referenced by abs_coefCalcFromXsec(), calc_nd_field(), GasAbsLookup::Extract(), and vmrunitscf().
planck
Calculates the Planck function for a single temperature.
Note that this expression gives the intensity for both polarisations.
f | frequency |
t | temperature |
Definition at line 219 of file physics_funcs.cc.
References BOLTZMAN_CONST, PLANCK_CONST, and SPEED_OF_LIGHT.
Referenced by cloud_ppath_update1D_planeparallel(), cloud_RT_no_background(), emissionPlanck(), MatrixCBR(), MatrixPlanck(), MCGeneral(), MCIPA(), surface_specular_R_and_b(), surfaceBlackbody(), surfaceFlatReflectivity(), surfaceFlatVaryingEmissivity(), and surfaceLambertianSimple().
rayjean
Converts a Rayleigh-Jean brightness temperature to radiance
tb | RJ brightness temperature |
f | frequency |
Definition at line 252 of file physics_funcs.cc.
References BOLTZMAN_CONST, and SPEED_OF_LIGHT.
Referenced by iyInterpCloudboxField(), and iyInterpPolyCloudboxField().