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Fig. 1.

image

Difference between the declination δh computed from the altitude with Eqs. (7)–(9) and the declination δW listed in Manuscript for ϕG = 51° 19′. With few excaptions, the computations are exact for superior and southern culminations. The values δh from inferior culmination are systematically too high for low altitudes. Values for which δh ≠ δW are labelled with W for those entries for which only one altitude is listed, and for W 9. The solid curve gives the refraction RR according to Rothmann. Stars to the right of the vertical dashed line have R = 0, according to Rothmann.

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