सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)
Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary
भास्कराचार्य द्वितीय द्वारा
पृष्ठ 325, कुल 573 में से
संदर्भ में पढ़ें305
projections of the rising points of the Sun on the same
plane. Let perpendiculars be dropped from S₁, S₂, S₃ on
the plane of the horizon. Let o be the centre of the
sphere. Let ns be the north-south line. In position S₁,
S₁C = Śanku-Bhujā, KA = Śankutala, oA = Agrā, so
that A = S + B (1) In the position S₂. S₂D = Śanku-Bhuja,
LA = Śanku-tala, oA = Agrā, so that B + A = S; but
here B is negative, a the azimuth being south so that writ-
ing - B for B, - B + A = S ∴ A = S + B again. In
position S₃, OB = A, MB = S, OM = B so that A + S = B;
but here A is +ve, δ being south and B is negative a
being south; hence writing - A and - B for A and B
A + S = - B or A = S + B again. This shows that
with the convention cited above A = S + B holds good
universally.
Now let us consider the situation with respect to
the Karnāgrā. Each of the three quantities a, b, s have
now opposite directions. If δ be north, the Sun will be on
the north of Equator, but the extremity of the shadow will
now be on the south of the Equinoctial shadow line
(E.S.L.) ie. the line which is parallel to the East-west
line at a distance of the equinoctial shadow s, and which
is tbe locus of the extremity of the shadow on the
equinoctial day; thus when the Agrā is considered to be
positive being on the north of the East point, the
Karnāgrā, though it is on fhe south will have to be
considered positive. Similarly when the azimuth of the
Sun a is on the north of the prime-vertical and is so
considered to be positive, the extremity of the shadow
being on the south of the East-west line and has a
negative azimuth, the bhuja is still to be considered
positive. Again the Śankutala being always south of
the Udayāsta Sūtra being considered south and positive,
the corresponding quantity into which it gets converted
on the horizontal dial namely the equinoctial shadow s
will be north of the East-west line and will be considered
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