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This function gives the result of integrating spectral data over wavelengths and dividing the result by the spread or span of the wavelengths.

Usage

average_spct(spct)

Arguments

spct

generic_spct

Value

One or more numeric values with no change in scale factor: e.g. [W m-2 nm-1] -> [W m-2 nm-1]. Each value in the returned vector corresponds to a variable in the spectral object, except for wavelength.

Examples


average_spct(sun.spct)
#>      e.irrad      q.irrad 
#> 5.175479e-01 2.414142e-06