Hostname: page-component-745bb68f8f-hvd4g Total loading time: 0 Render date: 2025-01-11T01:58:45.233Z Has data issue: false hasContentIssue false
  • English
  • Français

Fortnightly Nutation from the ILS Data

Published online by Cambridge University Press:  14 August 2015

A. A. Korsun'  and
V. K. Taradij
A. A. Korsun'
Affiliation:
Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev, USSR
V. K. Taradij
Affiliation:
Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev, USSR

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

There are two reasons why the study of fortnightly nutation is important. First, it provides an opportunity to investigate some peculiarities of the Earth's structure; second, it permits us to calculate more precisely the apparent locations of stars.

Type
Session II
Information
Symposium - International Astronomical Union , Volume 78: Nutation and the Earth's Rotation , 1980 , pp. 41 - 46
Copyright
Copyright © Reidel 1980 

References

Atkinson, R.d'E.: 1973, Astron. J., 78, 147.CrossRefGoogle Scholar
Fedorov, E.P.: 1963, Nutation and Forced Motion of the Earth's Pole (Pergamon Press).Google Scholar
Kakuta, C.: 1970, Publ. Astron. Soc. Japan, 22, 199.Google Scholar
McCarthy, D.D.: 1976, Astron. J., 81, 6, 482.CrossRefGoogle Scholar
McClure, P.: 1973, Diurnal Polar Motion (NASA, Washington, DC), NASA-TM-X-70470.Google Scholar
O'Hora, N.P.J.: 1973, Astron. J., 78, 1115.CrossRefGoogle Scholar
Oppolzer, T.R.V.: 1880, Bahnbestimmung der Kometen und Planeten (Englemann, Leipzig Union), 2nd ed., 1, 154–155.Google Scholar
Woolard, E.W.: 1953, Astronomical Papers for the American Ephemeris and Nautical Almanac, XV, p. 1.Google Scholar