Abstract

The camera which has been developed consists of a spherical mirror and a corrector lens with spherical surfaces. The equivalent focal length is about 900 mm and the relative aperture is f/4. The design is based on the theory by Argentieri and becomes a camera of the nonconcentric type. The useful range of the camera is from 2500 A to 12 000 A. Some details of the construction and results obtained are shown.

© 1954 Optical Society of America

Cine Spectrograph

Donald J. Lovell, Harold S. Stewart, and Seymour Rosin
J. Opt. Soc. Am. 44(10) 799-803 (1954)

Schmidt Systems as Spectrograph Cameras*

R. Minkowski
J. Opt. Soc. Am. 34(2) 89-92 (1944)

Calculation of Integrated Intensities in Spectrographic Microanalysis*

J. K. Hurwitz
J. Opt. Soc. Am. 44(1) 30-34 (1954)

Effect of Stray Light in Prism and Grating Spectrographs on Emulsion Calibration Curves and Its Significance in Spectrographic Analysis*

Richard N. Kniseley and Velmer A. Fassel
J. Opt. Soc. Am. 44(5) 390-393 (1954)

Monochromatic Camera for Photography in the Far Ultraviolet

W. E. Behring, J. M. Jackson, S. C. Miller, and William A. Rense
J. Opt. Soc. Am. 44(3) 229-231 (1954)