For a particular day, once the day count has been determined, the 
Surya Siddhanta describes how to determine the celestial longitude 
(measured along the ecliptic) of the particular body (Sun, Moon, or 
planet) in question. The longitude is calculated by first calculating 
the mean longitude for the particular body; this is the longitude 
that the body would have if it were moving around the celestial 
sphere at a constant rate. (It has the same meaning in modern 
calculations of positions of the Sun, Moon, and planets.) Then a 
correction is calculated based on the assumption that the body is 
sometimes ahead and sometimes behind the mean longitude. The 
correction amounts to assuming that the body moves on a smaller 
circle and the center of this circle is at the mean longitude. At 
times the body is at the leading edge of the smaller circle, and thus 
ahead of the mean longitude; later, as the body moves around the 
smaller circle it is near the trailing edge of the circle and thus 
behind the mean longitude. This is exactly the same as described by 
Ptolemy (150 A.D.) in his Almagest; the smaller circle is called an 
epicycle by Ptolemy. The Hindus apparently did not believe the body 
actually traveled around the epicycle however, instead they believe 
there was some sort of force which at times drew the body ahead in 
its motion, and at other times pulled it back in its motion. 


http://www.salagram.net/eclipse-suryasiddhanta.html






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