Determination of correction to the standard solar radius.

Details Determination of correction to the standard solar radius. Determination of correction to the standard solar radius.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acasn..30..355w&link_type=abstract

Acta Astron. Sin., Vol. 30, No. 4, p. 355 - 366

Astronomy and Astrophysics

Astronomy

Sun: Diameter, Solar Eclipses: 1987September 23

Scientific paper

During the annular solar eclipse of Sept. 23, 1987 Baily beads were observed at two locations near both southern and northern edges of the path. The observations were analysed to identify the features of the lunar profile which gave rise to the beads observed. They were then reduced to derive the corrections to the ecliptic longitude and latitude of the Sun and to the standard solar radius. The corrections obtained are: Δr = -0″11±0″03 m.e., Δl = +0″57±0″09 m.e., Δb = +0″02±0″02 m.e.

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