The relative position of the Moon to the Sun at the 1970 March 7 eclipse.
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.)
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| Main Authors: | , |
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| Format: | Journal Contribution biblioteca |
| Language: | Japanese |
| Published: |
1976
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| Online Access: | http://hdl.handle.net/1834/16320 |
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