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सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)

सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)

Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary

भास्कराचार्य द्वितीय द्वारा

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पृष्ठ 164, कुल 573 में से

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पृष्ठ 164

144 Comm. As per the formulation. Bhujaphala = (H sin m × c) / 360 = (H sin m × r) / R Kotiphala = (H cos m × c) / 360 = (H cos m × r) / R in the case of Mandaphala or Sīghraphala where c = peri- phery of the Manda or Sīghra periphery, r=Antyaphalajyā defined above R = 3438' and m stands for the Manda or Sīghra anomaly. These Bhujaphala and Kotiphala will be used in their respective contexts. Verses 27, 28, 29. Calculation of what is known as Sīghrakarṇa. (H Cos m ± r)² + H Sin² m = K² (1) (R ± Kotiphala)² + Bhujaphala² = K² (2) R² + r² ± 2 R × Kotiphala = K² (3) R² + r² ± 2 r × H Cos m = K² (4) The arc of the H Sine of the equation of centre is called the Mandaphala. Comm. Ref. fig. 9. From triangle E₁M₁M₂ (E₁M₁ + M₁N₂)² + M₂N₂² = E₁M₂² = K². But M₁N₂ = Kotiphala and M₂N₂ = Bhujaphala defined previously so that we have the second formula for K enunciated above. From the similarity of the triangles E₁M₁Q₁ and M₁M₂N₂ we have M₂N₂ / M₁Q₁ = M₁M₂ / E₁M₁ so that M₂N₂ = r / R × M₁Q₁ ; Since M₁Q₁ is called the Bhuja, the corresponding M₂N₂ in the Antya- phalajyā triangle is called the Bhujaphala. Similarly M₁N₂ is called the Kotiphala. Again (E₁Q₁ + Q₁Q₂)² + M₂Q₂² = E₁M₂² where E₁Q₁ = H Cos m, Q₁Q₂ = M₁N₂ = r and M₂Q₂ = M₁Q₁ = H Sin m. From this we have the first formula enunciated.

सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक) · पृष्ठ 164, कुल 573 में से · BharatKosha