भारतकोश
पञ्चसिद्धान्तिका (आचार्य वराहमिहिर - सूर्य, रोमक, पौलिश, वासिष्ठ एवं पितामह सिद्धान्त)

पञ्चसिद्धान्तिका (आचार्य वराहमिहिर - सूर्य, रोमक, पौलिश, वासिष्ठ एवं पितामह सिद्धान्त)

Panchasiddhantika of Acharya Varahamihira with Commentary

आचार्य वराहमिहिर द्वारा

DevanagariHindipublished419 पृष्ठ

पृष्ठ 140, कुल 419 में से

संदर्भ में पढ़ें
पृष्ठ 140

114 PAÑCASIDDHĀNTIKĀ IV. 40 The arc of 84' 30" is 44° 46'. Therefore the Sun rises at a point 44° 46' north of the east point, and sets at a point 44° 46" north of the west point, (assuming that the declination has not changed). The formula for amplitude is got thus: See Fig. 12. Take S₁ as the Sun on the diurnal circle north of equator. Then S₁S₂ is the declination of the Sun, D₁D₂ is the amplitude of sunrise. From the figure it can be seen, D₁D₂ = 90° − ND₁ Therefore sin D₁D₂ = Cos ND₁. From the right angled triangle ND NP in the figure, Cos ND can be got thus: By the fundamental formula I, Cos ND₁ = 120' × Cos D₁ NP ÷ Cos N NP. But, Cos D₁ NP = Cos S₁ NP = Cos (90° − S₁S₂) = sin S₁S₂ = sin S₁S₂ Cos N NP = sin (90° − N NP) = sin colat. ∴ Sin amplitude = 120' × sin dec ÷ sin colat. When the Sun is south of the celestial equator, (e.g. S₃ in the figure), D₃ is the rising point, and D₂D₃ is the amplitude. Its sine is got thus, from the triangle, D₂D₃E, right-angled at E. By the funda- mental formula II, Sin D₂D₃ = sin ED₃ × radius ÷ sin angle D₃D₂E, Here, ED₃ is the declination. D₃D₂E = 90° − ED₂Z = 90° − lat. ∴ sin amplitude = sin declination × radius ÷ sin (90° − lat) = sin dec × radius ÷ sin co-lat., which is the formula given. [अग्राया अक्षानयनम्] तेन हता ऽखार्कऽघ्नी क्रान्तिज्या लम्बकोऽस्य [य] (च्चा) पम् | तेन नवतिर्विहीना (यच्छेषं) तेऽक्षभागाः स्युः || ४० || Latitude from Agrā 40. Multiply sine declination by 120 and divide by the sine of amplitude. The sine of co-latitude is got. Find its arc in degrees. Deduct the degrees from 90. The remainder are the degrees of latitude. Now, sin co-lat = 120' × sin dec. ÷ sin amplitude. From this, the arc, co-lat is got. 90° − colatitude = latitude, as already stated in (IV. 28). From the formula of the previous verse, Sin amp = radius × sin dec ÷ sin co-lat, Sin colat = radius × sin dec ÷ sin amp. = 120' × sin dec ÷ sin amp. From the amplitude of the setting Sun also, the latitude can thus be found. The amplitude can be marked on a circle with the directions already marked by the observation of sunrise or sunset. 40a. A. हृता. A. खार्कघ्नी b. A1. कोस्य श्रापम्; (A2. स्प corrected to स्य) c-d. A. हीना छयेघतेक्षभागाः