Description

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

Usage

Arguments

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