सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)
Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary
भास्कराचार्य द्वितीय द्वारा
पृष्ठ 203, कुल 573 में से
संदर्भ में पढ़ें183
from the figure ÂPQ is the rising hour-angle = ÂPE + ÊPQ = ÂPE + 90° where 90° correspond to 15 nādīs. So we have to add ÂPE expressed in nādīs equal to the rising time of AE. Let us find the duration of the day for the place where s=3″ and when λ of s=44° ; the latitude of the place will be 14° (from tables) when λ 44°, we have found above that 42-20 Vinadis is the chara expressed in time. Hence half the day = 15-42-20 or duration of day 31-25 ; duration of night = 28-35. Note (1) In modern astronomy we have the formula cos h = — tan ϕ tan δ where h is the rising hour angle. Putting h = H + 90° where H stands for the arc EA of fig. 21 cos (90+H) = — sin h = — tan ϕ tan δ so that sin H = tan ϕ tan δ ie. R sin (Chara) = R tan ϕ tan δ which accords with the formula found before. The word chara used for EA means etymologically रविसञ्चारवशेन दिन- प्रमाणे विकारः i e. the variation in 15 ghatis of the eqiunoctial half-day on account of the Sun's variation in declination, (2) If ϕ = 0, Chara = 0 so that duration of half- day is 15 ghatis ie. on the terrestrial equator, whatever be the Sun's declination, the length of the day will be always 12 hours. (3) Let δ = 0 so that chara = 0 ie. whatever be the latitude (provided ϕ ≯ 90-δ as we shall see shortly). the day and night will be each of 12 hrs. (4) Let δ be negative, so that the arc connoting chara ie. EA will be above the horizon, and consequently the duration of half-day will be less than 6 hrs. by the time that is taken for EA to rise. This can be seen other- wise also as cos h = — tan ϕ tan δ = + ve so that h < 90° which means half-day is less than 6 hrs. (5) We could also treat the case when ϕ is negative, but as this case is not in the purview of Hindu Astro- nomers who had only India in their mind and as such were concerned primarily with positive latitudes. If, how- ever, we consider a negative latitude, when δ is + ve, cos h will be positive and if δ is — ve, cos b will be negative. This means that when the Sun is in northern latitudes, the southern latitudes will have their day less than 12 hours and when the Sun is in southern latitudes, their day will be greater than 12 hrs.