Jyeshtadeva was a Kerala astronomer who helped in the calculation of longitudes, when there is latitudinal deflection. In his Yukti Bhasa, he calculates correctly the cos l, the cosine of latitude, which is important in the Reduction to the Ecliptic.
There is a separate section in the Yukti Bhasa, which deals with the effects of the inclination of a planet’s orbit on its latitude. He describes how to find the true longitude of a planet, Sheegra Sphutam, when there is latitudinal deflection.
“Now calculate the Vikshepa Koti, cos l, by subtracting the square of the Vikshepa from the square of the Manda Karna Vyasardha and calculating the root of the difference.”
In the above diagram,
N is the Ascending Node
P is the planet on the Manda Karna Vritta, inclined to the Ecliptic
Vikshepa Koti = OM = SQRT( OP^2 – PM^2 )
Taking this Vikshepa Koti and assuming it to be the Manda Karna, sheegra sphuta, the true longitude, has to be calculated as before.