Hostname: page-component-7479d7b7d-qlrfm Total loading time: 0 Render date: 2024-07-12T09:28:12.453Z Has data issue: false hasContentIssue false

The Stability of Continental Blocks in Seismically Active Regions

Published online by Cambridge University Press:  14 August 2015

V. P. Shcheglov*
Affiliation:
Astronomical Observatory of Tashkent U.S.S.R.

Abstract

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.

In connection with the problem of continental drift some authors voice a supposition of the existence of progressive and rotational motion of continental blocks, particularly in seismically active regions. Azimuths of some terrestrial objects determined over long time intervals were used to investigate these motions. Naturally, the reliability of the result depends on the length of these intervals.

The axis of the meridian instrument of Uloug-Beg Observatory in Samarkand, installed 550 years ago (1420-30) is the most ancient meridian direction on the Earth. Using measurements made by the author in 1941, 1956, and present-day observations, it was found that the direction of the axis had moved through an angle of . Allowing for observational errors in the pre-optical period one can accept a change of 5′ or per year. To ascertain if the observed change is caused by rotation of the continental block or local deformation repeated measurements of azimuths of triangulation stations first measured forty years ago were made. The results show the absence of continental block rotation in the region of Middle Asia within a possible accidental error of .

Type
Part VIII: Geophysics
Copyright
Copyright © Reidel 1979