total.radiation: Total body radiation at temperature T after Stefan-Boltzmann.
In nobodyinperson/meteoRology: Basic meteorology functions
Description
Usage
Arguments
Value
See Also
Description
The total body radiation of a body with emissivity epsilon and temperature
T after Stefan-Boltzmann.
Usage
1
total.radiation(T, epsilon = 1)
Arguments
T
temperature in Kelvin [K]
epsilon
emissivity, in the range of c(0,1). Defaults to black body epsilon=1.
Value
The total body radiation energy density of a body with emissivity
epsilon and temperature T after Stefan-Boltzmann in [W*m-2].
See Also
brightness.temperature.total for the opposite.
nobodyinperson/meteoRology documentation built on May 23, 2019, 9:31 p.m.
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Description Usage Arguments Value See Also
Description
The total body radiation of a body with emissivity epsilon and temperature
T after Stefan-Boltzmann.
Usage
1 | total.radiation(T, epsilon = 1)
|
Arguments
T |
temperature in Kelvin [K] |
epsilon |
emissivity, in the range of c(0,1). Defaults to black body |
Value
The total body radiation energy density of a body with emissivity
epsilon and temperature T after Stefan-Boltzmann in [W*m-2].
See Also
brightness.temperature.total for the opposite.
R Package Documentation
Browse R Packages
We want your feedback!
Note that we can't provide technical support on individual packages. You should contact the package authors for that.
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