The relative position of the Moon to the Sun at the 1970 March 7 eclipse.
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Date
1976
Metadata
Show full item recordAbstract
The reduction of the contact time observation for the 1970 Mexico solar eclipse is revised employing the solar ephemeris in the IAU 1964 system, the lunar ephemeris j=2 and a refined geocentric position of the telescope, all of which have become available after the first report was presented. Assuming ET- AT to be 32.s0, the observed positions minus phemerides become Δ (Lmoon-Lsun) =ー0."12土0."02 (m.e.) , Δ (βmoon-βsun)=+0."19土0."07(m.e.)Journal
Report of Hydrographic and Oceanographic ResearchesIssue/Article Nr
11Page Range
pp.39-41Resource/Dataset Location
https://www1.kaiho.mlit.go.jp/GIJUTSUKOKUSAI/KENKYU/report/rhr11/rhr11-02.pdf