Stefan-Boltzmann equation

get.Stefan_Boltzmann computes the total radiant exitance of a blackbody at a given temperature, using the Stefan-Boltzmann law (\(H = \sigma T^4\)).

Usage

get.Stefan_Boltzmann(T_C)

Arguments

T_C

numeric vector. Temperature(s) of the emitting surface, in degrees Celsius.

Value

numeric vector. Blackbody radiant exitance H (W m^-2) at each temperature in T_C.

Author

Carlos Camino

Examples

if (FALSE) { # \dontrun{
H <- get.Stefan_Boltzmann(T_C = 20)
} # }