STRAY-LIGHT SUPPRESSION IN A REFLECTING WHITE-LIGHT CORONAGRAPH

An analysis of stray-light suppression in the white-light channel of t he Ultraviolet Coronagraph Spectrometer experiment for the Solar and H eliospheric Observatory is reported. The white-light channel consists of a reflecting telescope with external and internal occultation and a polarimeter section. Laboratory tests and analytical methods are used to perform the analysis. The various stray-light contributions are cl assified in two main categories: the contribution from sunlight that p asses directly through the entrance aperture and the contribution of s unlight that is diffracted by the edges of the entrance aperture. Valu es of the stray-light contributions from various sources and the total stray-light level for observations at heliocentric heights from 1.4 t o 5 solar radii are derived. Anticipated signal-to-stray-light ratios are presented together with the effective stray-light rejection by the polarimeter, demonstrating the efficacy of the stray-light suppressio n design.