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Volumn 273, Issue 5271, 1996, Pages 100-104

Late proterozoic and paleozoic tides, retreat of the moon, and rotation of the earth

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; AUSTRALIA; CHRONOLOGY; MOON; PRIORITY JOURNAL; RHYTHM; SUN; SUNLIGHT; TIME; UNITED STATES;

EID: 0029663562     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.273.5271.100     Document Type: Article
Times cited : (93)

References (33)
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    • e); Earth has 1.23% of the total system angular momentum, and the moon has the remaining 98.8%. Thus, the moon's present-epoch share of orbital angular momentum must be reduced by 1.23%, the fraction belonging to Earth. For the earlier time periods, the barycenter shifts closer to Earth's center. For the Earth-sun barycenter, the sun is taken as infinitely massive and the moon's mass is ignored. The obliquity of the lunar orbit to Earth's equator is necessarily ignored here.
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    • In MLE computations, we assume noise is Gaussian (normally distributed). Additionally, as the frequency scale is based on neap-spring laminae count (index) rather than on true frequency, errors attributable to lost laminae can contract the time scale.
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    • note
    • In memoriam S. K. Runcorn. Supported in part by the NASA Innovative Research Program (to C.P.S.), the NSF Atmospheres program (to G. E. Williams and C.P.S.) for the Elatina data reduction, and NSF grant EAR-9315937 (to MAC. and E.P.K.) for the BCC data. We thank H. R. Johnson and A. Zawostoski for technical support.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.