brightness.temperature.total: Brightness temperature
In nobodyinperson/meteoRology: Basic meteorology functions
Description
Usage
Arguments
Value
See Also
Description
Calculate the brightness temperature from the total emitted radiation energy density.
Usage
1
brightness.temperature.total(I, epsilon = 1)
Arguments
I
total radiation energy density in [W*m-2]
epsilon
emissivity, in the range of c(0,1)
Value
The brightness temperature in Kelvin.
See Also
total.radiation 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
Calculate the brightness temperature from the total emitted radiation energy density.
Usage
1 | brightness.temperature.total(I, epsilon = 1)
|
Arguments
I |
total radiation energy density in [W*m-2] |
epsilon |
emissivity, in the range of c(0,1) |
Value
The brightness temperature in Kelvin.
See Also
total.radiation 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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