Changes in the earth's rate of rotation between A.D. 1672 and 1806 as deduced from solar eclipse timings

Details Changes in the earth's rate of rotation between A.D. 1672 and 1806 as deduced from solar eclipse timings Changes in the earth's rate of rotation between A.D. 1672 and 1806 as deduced from solar eclipse timings

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...200..218s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 200, no. 1-2, July 1988, p. 218-224.

Astronomy and Astrophysics

Astrophysics

1

Earth Rotation, Ephemeris Time, Secular Variations, Solar Eclipses, Electromagnetic Coupling, Io, Time Response

Scientific paper

Solar eclipse timings measured between A.D. 1672 and 1806 are analyzed to study the variation of Delta T (= ET - UT) over this interval. These solar eclipse observations confirm the results of Brouwer (1952), Martin (1969), and Stephenson and Morrison (1969) which were obtained from the analysis of occultations in this period. It is believed that Goldstein's (1985) analysis inadequately represents the changes in Delta T.

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