published an integral formula for the relative intensities to be expected in the diffraction orders of an echelette grating. On performing the integration, we obtain a formula (after correcting for two typographical errors) which differs from that obtained by Rowland in his third term. On the basis of this formula, conditions can be obtained so that a given wavelength can be in the blaze in a certain order. It will be shown that these conditions are not sufficient to determine the incident and diffracted rays uniquely, and further that a variety of blaze conditions exists. This leads to the possibility of several grating mountings which permit the operator to work in the blaze over a range of wavelengths. Two of these possibilities have previously been published by Greig and and .
Description
H. A. Rowland, The Physical Papers of Henry A. Rowland, Johns Hopkins University Press, 1902, p. 525 J. H. Greig and W. F. C. Ferguson, J. O. S. A. 40:504 (1950) N. Finkelstein, J. O. S. A. 41:179 (1951)