Seâdet-i Ebediyye Endless Bliss Fourth Fascicle by Huseyin Hilmi Isik - HTML preview

Appendix VI

Sun’s Altitudes at Time of Late Afternoon Prayer for Any Latitude

For instance, the Sun’s declination on February 2 is -16.48^o in Istanbul; hence, ghâyat irtifâ’ (point of solar culmination, the Sun’s maximum altitude) is -16.48^o +49^o = 32.12^o; fay-izawâl (the shortest shadow) of a one-metre-long perpendicular rod is 1.58m.; and the length of its late-afternoon shadow is 2.58m.; and the Sun’s late-afternoon altitude is 21.20^o. The fadli-dâir (temporal value of the arc of complement of the Sun’s true altitude) is 2 hours and 41 minutes, which will be found by using a calculator. Thereby the time of late afternoon will be found to be 9.42 hours, adhânî, and 3.09 hours, in standard time, since the equation of time is -13.39; (please see Appendix IV.) A method to be used in the absence of the chart above is to get a privileg calculator, touch the buttons for the computation: 90-32.12 --> _o,,,= tan + 1 = arc tan MS 90-MR = --> _o,,, , and find the Sun’s altitude at the time of ’asr-i awwal (the earlier time of late afternoon) to be 21.08^o. There is yet another method: The Rub-i-dâira (quadrant). Its khayt, (thread that represents the daily rotation,) is brought over the number representing theghâyat irtifâ’; the number on the arc of zill-i-mebsût and crossed by the khayt shows the length of the shortest shadow termed fay-i-zawâl.