Osmium atomic-oxygen protection by an iridium overcoat for increased extreme-ultraviolet grating efficiency.
The deposition of a 30-A-thick layer of iridium upon a 250-A-thick osmium reflective layer for use as a diffraction grating in the Cosmic Hot Interstellar Plasma Spectrometer (CHIPS) satellite observatory has provided sufficient protection from an expected maximum orbital atomic-oxygen fluence of 1 x 10(16) atoms/cm2. The grating parameters of groove constant and depth, efficiencies of zeroth-order, first and second inside orders, and first inside-order efficiency positional uniformity as well as stray light near the first inside order of the Ir-Os-coated grating were measured within a CHIPS spectral bandpass of 90-260 A. Stray-light measurements were also made near the first inside spectral order at 304, 584, and 1216 A. The results make the Ir-Os coat an acceptable grating reflectivity layer for CHIPS and other spaceborne extreme-ultraviolet spectrometers that employ grazing-incidence reflection optics.
Hemphill
Richelieu
R
Space Sciences Laboratory, University of California, Berkeley, Berkeley, California 94720, USA. rhemp@ssl.berkeley.edu
Hurwitz
Mark
M
Pelizzo
Maria G
MG