Instrumental equation

from Wikipedia, the free encyclopedia

In astrometry and geodesy, the instrumental equation is the effect of small systematic errors in a measuring instrument or a measuring method, which remain almost constant in their overall effect on the determination of time , plumbness and location .

The name was created by analogy with the term " personal equation " when, around 1930, the observer began to reduce the effects of time and target errors through (partial) automation .

Just like the personal equation , the instrumental equation can only be determined by reference measurements at a precisely known reference point .

causes

The instrumental equation is mainly caused by the following effects:

Sometimes meteorological effects such as zenith or side refraction are also included in the instrumental errors, provided that they have a systematic component (e.g. due to the slope of the terrain ). They arise from thermal layer inclinations in the lower troposphere . A pillar rotation caused by cooling also has a systematic effect .

See also

literature

  • Karl Ramsayer : Geodetic Astronomy ( Handbook of Surveying Volume 2a). 10th, completely revised and restructured edition. JB Metzler-Verlag, Stuttgart 1970.
  • Joachim Höpfner: Astronomical differences in length and latitude of the basic observatories Potsdam, Irkutsk and Simeiz . Astronom. News 304/5, p. 265-275, Berlin 1983.

supporting documents

  1. Gottfried Gerstbach : For the azimuth measurement with second theodolites . Austrian Magazine for surveying 64/2, p. 53-68, Vienna 1977
  2. ^ Rudolf Sigl : The influence of systematic .. observation errors on the Laplace equation , Bull.Géod. 44/1, doi: 10.1007 / BF02526434 .