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On the Progress of the Construction of the Sukharev Meridian Automatic Horizontal Instrument (MAHIS)

Published online by Cambridge University Press:  19 July 2016

R.I. Gumerov
Affiliation:
2Engelhardt Astronomical Observatory 422526 Kazan, USSR
V.B. Kapkov
Affiliation:
2Engelhardt Astronomical Observatory 422526 Kazan, USSR
T.R. Kirian
Affiliation:
1Central Astronomical Observatory (Pulkovo) 196140 Leningrad, USSR
N.S. Liadovoi
Affiliation:
3Nikolaev Branch, Pulkovo Observatory 327030 Nikolaev, USSR
G.I. Pinigin
Affiliation:
3Nikolaev Branch, Pulkovo Observatory 327030 Nikolaev, USSR
A.A. Pozhalov
Affiliation:
3Nikolaev Branch, Pulkovo Observatory 327030 Nikolaev, USSR
V.P. Sibilev
Affiliation:
3Nikolaev Branch, Pulkovo Observatory 327030 Nikolaev, USSR
A.W. Schumacher
Affiliation:
1Central Astronomical Observatory (Pulkovo) 196140 Leningrad, USSR
N.A. Shkutova
Affiliation:
1Central Astronomical Observatory (Pulkovo) 196140 Leningrad, USSR
O.E. Shornikov
Affiliation:
3Nikolaev Branch, Pulkovo Observatory 327030 Nikolaev, USSR

Abstract

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The MAHIS is the L.A. Sukharev meridian automatic horizontal instrument. It has all the advantages of the Pulkovo HMC and is devoid, or nearly devoid, of its disadvantages. A scheme of the MAHIS includes a flat mirror of D = 300 mm and two immovable horizontal tubes of D = 190 mm, focal length 8000 mm. There is a pavilion for the central unit and 2 roofed pavilions for eyepiece parts of the tubes. The MAHIS is provided with an automatic registering device, a system for meteorological data collection, and is computer controlled. The work on this telescope is being carried out at the Pulkovo, Kazan and Nikolaev observatories. The expected precision of the instrument is ±0.″05 in both coordinates with respect to systematic errors.

Type
Part 2: Pulkovo today
Copyright
Copyright © Kluwer 1990 

References

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