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We calibrate the spectrometer by using light sources with well-known emission spectra such as mercury lines and sodium double-D lines. The accuracy in the calibration of the spectrometer is high enough within the allowed experimental error.
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We calibrate the spectrometer by using light sources with well-known emission spectra such as mercury lines and sodium double-D lines. The accuracy in the calibration of the spectrometer is high enough within the allowed experimental error.
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N. Since some nonfactors may become indistinguishable from the values of the maxima in the interferogram, we have to check if they actually divide N.
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