Optic projection : principles, installation and use of the magic lantern, projection microscope, reflecting lantern, moving picture machine, fully illustrated with plates and with over 400 text-figures (1914)

Record Details:

Something wrong or inaccurate about this page? Let us Know!

Thanks for helping us continually improve the quality of the Lantern search engine for all of our users! We have millions of scanned pages, so user reports are incredibly helpful for us to identify places where we can improve and update the metadata.

Please describe the issue below, and click "Submit" to send your comments to our team! If you'd prefer, you can also send us an email to mhdl@commarts.wisc.edu with your comments.




We use Optical Character Recognition (OCR) during our scanning and processing workflow to make the content of each page searchable. You can view the automatically generated text below as well as copy and paste individual pieces of text to quote in your own work.

Text recognition is never 100% accurate. Many parts of the scanned page may not be reflected in the OCR text output, including: images, page layout, certain fonts or handwriting.

CH. VI] HELIOSTATS FOR THE MAGIC LANTERN 159 FIG. 84. LENS AND PRISM HELIOSTAT OF ALFRED M. MAYER. (From the Catalogue of Optical Instruments by R. Fuess), The figure has been modified by extending the clock-shaft above and below. As here shown the instrument is suitable for any latitude. It uses a mirror instead of a second prism as in the original of Mayer (fig. 83). U Clock-work. N P, L° The clock-shaft extended to indicate the direction of the celestial north pole above, and below the angle of elevation corresponding to the latitude of the place where the instrument is used. P D Z Three divided scales; P for the latitude, D for the Sun's declination, Z for the time of day. S, k and Pr. The convex and the concave lens, and the prism as shown in fig 83. Sp Mirror to take the place of the prism (L) in fig. 83.