In powder spectrometers of modern design the `vertical' divergence of the beam is limited by Soller slits, and has little influence on the position and shape of the diffraction maxima. `Horizontal' divergence cannot be considered apart from absorption and thickness of specimen. These three effects shift the centre of gravity of the maximum toward lower values of θ. 2A is the illuminated length of the specimen, t is its thickness, R is the spectrometer radius, and μ is the linear absorption coefficient of the specimen. In most spectrometers A is limited by slits to αR csc θ, where 2α is the horizontal divergence of the incident beam, but in some the specimen is irradiated over its full length L, and A is constant at ½L. The shift of the peak is more complicated, and requires a consideration of the line profile. In the limiting case of theta large a first approximation gives the same displacement for the peak as for the centre of gravity; in the limiting case of θ small the peak displacement is the smallest of the three expressions A2sin 2θ/2R2, 0.214 sin 2θ/µR, t cos θ/R No simple expression has been found for intermediate values of theta, Except for weakly absorbing substances and low Bragg angles the displacements are very small. The error in the spacings calculated from high-angle lines is discussed; there seems to be no reason why Geiger-counter spectrometry should not reach the same accuracy as the powder camera in the measurement of spacings.
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