सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)
Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary
भास्कराचार्य द्वितीय द्वारा
पृष्ठ 254, कुल 573 में से
संदर्भ में पढ़ें234 Fig. 33 Fig. 34 cos (90 — δ) = cos ϕ cos (90 — A) ie. sin δ / cos ϕ = sin A or in the Hindu form H sin A = R (sin δ / cos ϕ) = Agrajyā (5). This Agrajyā is in a circle of radius R, and if it be re- duced to a circle whose radius is K, is will be (K / R) × (R sin δ / cos ϕ) = (K sin δ / cos ϕ) which is called Karṇāgrā. Hence we have Karṇāgrā = s + b which we shall write as a = b + s (6). This is an important formula which is going to be formulated later in verses 72, 73. In the above formula, s being constant, by differentiating δa = δb which means that the variation in the bhuja is on account of the variation in the Karṇāgrā. If in Fig. 35, Cω', CE″ be morning and evening shadows when they are equal as per the verse under comment, Mω' = b the morning bhuja, NE″ = b', the evening bhuja dE' is the variation in the bhuja ie. b — b' = δb which is formulated and equal to δa. But δa = δ(K sin δ / cos ϕ) = K δ (sin δ) / cos ϕ, ϕ being con- stant and K also being constant because the shadow S is constant and K = √(S² + 12²) = constant on both the occasions. ∴ δb = δK = (K / cos ϕ) (sin δ₁ — sin δ₂) as stated by Bhāskara.