RESUMO
The interferometer and viewing optics that are the main optical components of an automated surface mapping system used to characterize the surface topography and the wall thickness uniformity of opaque and transparent spherical shells are described. To characterize surface finish or wall thickness of spherical shells with an accuracy of 10 nm and a resolution of 1 microm, the differential phase shift between two beams of orthogonal polarizations is measured before and after the probe beam has interacted with the test object.
RESUMO
Ruby lasers in large, fixed installations are being used by groups in France, Japan, the Soviet Union, and the U.S. for measuring distances to retroreflectors on the moon. This paper describes a transportable transmitting unit that can be installed at any astronomical observatory where a large telescope is available to detect the received signal. The transmitter consists of a high radiance, frequency-doubled, neodymium-glass laser and a coudé optical system of moderate size. It has been installed, but is not yet in operation, at the Agassiz Observatory, Harvard, Massachusetts.
