Reading microscope

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Reading microscope; after William A. Norton (1867)

Reading microscopes are short, weakly magnifying microscopes with which graduated circles can be read precisely. They have been used since around 1800 for all precise angle measurements , as they are necessary in astronomy for meridian circles or in geodesy for theodolites and total stations .

Older measuring instruments still have open reading microscopes, which are attached in pairs at opposite points on the measuring circle. Modern theodolites only have a reading microscope directly next to the telescope, in whose field of view the diagonal points of the partial circles are reflected together by a folded beam path. This means that the measurement can be carried out very quickly and with only a low error rate. Since the 1990s, however, opto-electronic reading with immediate digital storage has become increasingly popular .

With large universal and passage instruments , the reading can be accommodated in a closed, moisture-proof and dust-proof housing, while with large astronomical telescopes the beam path is often directed to a fixed point, comparable to the placement of a Coude focus .

Individual evidence

  1. ^ William A. Norton: A treatise on astronomy, spherical and physical; with astronomical problems, and solar, lunar, and other astronomical tables. For the use of colleges and scientific schools . 4th edition. J. Wiley & Son, New York 1867, OCLC 6332896 .