Abstract
The influence of sequential analysis rate on measurements of Michelson fringes is examined on a theoretical basis, sh whilst considering the special case where the elementary telescope pupils are small in comparison with Fried's parameter ( r 0). As a result of this investigation it seems that the principal effect due to an insufficient scanning rate is a degradation of the spectral analysis window employed in the calculation of spatial energy spectra. This effect is related to Fried's parameter and to the wind speed. Taylor's hypothesis is employed in the calculation. The results obtained appear to be consistent with experimental observations.
Full Text
Published Version
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call