Abstract

The great flexibility of the 200-inch mirror required the development of new and elaborate support systems to maintain the figure in all orientations. New methods had, therefore, to be devised for testing the mirror in the telescope while on these supports. The final figuring was done on the mountain on the basis of these tests.

To increase the effectiveness of the instrument, corrector lenses were designed by Ross greatly to enlarge the field of the main mirror. Likewise the method of evaporating a reflecting coat of aluminum was developed by Strong to replace the old silvering procedures. Several new optical designs were introduced in the spectrographs to make optimum use of the light collected. These included the use of (1) a composite of four “blazed” gratings to permit a collimator aperture of 12 inches; (2) Schmidt cameras with half-strength corrector plate placed practically in contact with the grating, the light passing through the plate twice (this eliminates many vignetting problems and permits higher speeds and larger fields); and (3) a combination of a quartz aplanatic sphere with a Schmidt camera for the shortest focal-length camera to obtain a much higher speed (F/D = 0.7) than would otherwise have been possible.

© 1952 Optical Society of America

A Fixed-Focus Broad-Range Echelle Spectrograph of High Speed and Resolving Power*

George R. Harrison, James E. Archer, and Jean Camus
J. Opt. Soc. Am. 42(10) 706-712 (1952)

The Optical Properties of a Compound Liquid Prism Suitable for Studies of the Raman Effect

H. J. V. Tyrrell and G. K. T. Conn
J. Opt. Soc. Am. 42(2) 106-113 (1952)

A Collimator with Variable Focal Length and Tilted Test Plate for Testing Cameras

Per J. Lindberg
J. Opt. Soc. Am. 42(10) 748-751 (1952)

Successive Diffractions by a Concave Grating

F. A. Jenkins and L. W. Alvarez
J. Opt. Soc. Am. 42(10) 699-705 (1952)

An Infrared Spectrograph for Use in the 40–150-Micron Spectral Region*

R. A. Oetjen, W. H. Haynie, W. M. Ward, R. L. Hansler, H. E. Schauwecker, and E. E. Bell
J. Opt. Soc. Am. 42(8) 559-566 (1952)