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Use the Blackbody/Graybody assumption and set a value for the Initial temperature T, to define I=Ib(T). This option is only available in the Radiation in Participating Media interface.
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Set a User defined value for the Initial radiative intensity I. The default is 0 in the Radiation in Absorbing-Scattering Media interface, and rpm.Ibinit in the Radiation in Participating Media interface.
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When Initial value is set to Blackbody/Graybody, enter a value for the Initial temperature T, to define I=Ib(T). This option is only available in the Radiation in Participating Media interface.
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When Initial value is set to User defined for each band, enter a value for the Initial radiative intensity for each spectral band in the table displayed underneath. Within a spectral band, each value is assumed to be independent of wavelength.
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When Initial value is set to User defined distribution, enter a value or expression for the Initial radiative intensity distribution Iλ. The wavelength may be accessed through the rpm.lambda or rasm.lambda variable. This distribution is integrated on each spectral band to obtain the radiative intensity Ii,k for each spectral band.
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Use the Blackbody/Graybody assumption and set a value for the Initial temperature T, to define G = 4πIb(T). This option is only available in the Radiation in Participating Media interface.
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Set a User defined value for the Initial incident radiation G. The default is 0 in the Radiation in Absorbing-Scattering Media interface, and (4*pi)*rpm.Ibinit in the Radiation in Participating Media interface.
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When Initial value is set to Blackbody/Graybody, enter a value for the Initial temperature T, to define G = 4πIb(T). This option is only available in the Radiation in Participating Media interface.
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When Initial value is set to User defined for each band, enter a value for the Initial incident radiation for each spectral band in the table displayed underneath. Within a spectral band, each value is assumed to be independent of wavelength.
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When Initial value is set to User defined distribution, enter a value or expression for the Initial incident radiation distribution Gλ. The wavelength may be accessed through the rpm.lambda or rasm.lambda variable. This distribution is integrated on each spectral band to obtain the incident radiation Gk for each spectral band.
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