# Solar Spectrum¶

utility.solar_spectrum.convolved_solar_spectrum(wavelengths, psf_wavelengths, psf, spectrum='SAO2010')
Parameters: wavelengths: numpy array An array of wavelenghts in nanometers at which the solar spectrum will be calculated psf_wavelengths: numpy array An array of wavelengths in nanometers at which the point spread function is specified. The output wavelenghts are linearly interpolated from this array. psf: numpy array An array of wavelengths in nanometers defining the spectral point spread function. The PSF is assumed be gaussian with a standard deviation given by psf spectrum: ‘string’ options argument specifying which solar spectrum to use. Currenlty supported options are ‘SAO2010’ and ‘’. Default is ‘SAO2010’. convovled_irradiance: numpy.array The solar spectrum in units of photons/m^2/sec/nm at the resolution specified

Examples

>>> import utility.solar_spectrum as sol