The reflectance of a W-B4C multilayer mirror, with a period thickness
that increased with depth into the multilayer, was measured at near-no
rmal incidence with synchrotron radiation and at grazing incidence wit
h Cu K alpha radiation. The period thickness increased linearly from 1
7.9 Angstrom at the top of the multilayer structure to 21.9 Angstrom a
t the substrate while the same ratio of nodal layer to period thicknes
s was maintained. For a grazing angle of 80 degrees (10 degrees from n
ormal incidence), the peak reflectance was 1.1% at a wavelength of 36
Angstrom, and the reflectance profile was 1 Angstrom wide. For Cu K al
pha radiation the reflectance peaked at a grazing angle of 2.4 degrees
and was 0.4 degrees wide. Compared with a W-B4C multilayer mirror wit
h a constant period thickness, the depth-graded multilayer mirror has
wider reflectance profiles at near-normal and grazing incidences, resu
lting in larger integrated reflectances and wider fields of view. (C)
1996 Optical Society of America