title: Stray-light suppression in a reflecting white-light coronagraph.
abstract: An analysis of stray-light suppression in the white-light channel of the Ultraviolet Coronagraph Spectrometer experiment for the Solar and Heliospheric 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 classified in two main categories: the contribution from sunlight that passes directly through the entrance aperture and the contribution of sunlight that is diffracted by the edges of the entrance aperture. Values of the stray-light contributions from various sources and the total stray-light level for observations at heliocentric heights from 1.4 to 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 suppression design.
authors.forename: M
authors.initials: M
authors.lastname: Romoli
authors.forename: H
authors.initials: H
authors.lastname: Weiser
authors.forename: L D
authors.initials: LD
authors.lastname: Gardner
authors.forename: J L
authors.initials: JL
authors.lastname: Kohl