Page 27 - Guidelines for Training/ Orientation of Faculty on IKS
P. 27

Guidelines for Training/ Orientation of Faculty on IKS


                         Explain the concept of cara as outlined in the Indian astronomical texts that captures the
                         variation  in  the  duration  of  the  day  at  a  given  location.  Present  the  formula  for
                         determining the local time using shadow measurements. Also outline how cara plays a
                         role in determining this local time. Bring out the distinction between this local time and
                         the standard time that we are generally familiar with and generally keep track of.
                     12.  Lagna and its computation
                       Introduce the  concept  of  lagna,  and  how  non-trivial  a  problem  it  is  to  determine  it
                         precisely. Also point out how this is deeply connected with fixing times for various social
                         and  religious  functions  such  as  marriage,  etc.  Bring  out  the  connection  between  its
                         computation  and  the  computation  of  declination,  cara  etc.  that  would  have  been
                         discussed  before.  Explain  how this  can  be  determined  ‘reasonably’  accurately  using
                         interpolation.  Also  outline  more  precise  formulations  that  have  been  given  by  later
                         astronomers by introducing the notion of kālalagna.
                     13.  Eclipses and their computation
                       Briefly explain the phenomenon of lunar and solar eclipses, and the crucial role played
                         by the position of the lunar nodes in their computation. Also bring out how difficult it is
                         to  precisely  determine  the  position  of  the  nodes—as  they  are  not  physical  objects
                         available for observation. Explain how the latitude of the moon is computed, and then
                         outline the procedure for the determination of the semi-diameters of the eclipsing and
                         the eclipsed bodies. Derive the simple formula for determining the duration of eclipses
                         as  well  as  the  obscuration.  Also  mention  that  iterative  procedures  are  followed  to
                         improve accuracy. Point out the role of parallax in the determination of solar eclipses.


                     References:
                                                                             nd
               1.  S. N. Sen and K. S. Shukla, History of Astronomy in India, 2  Ed., INSA, Delhi, 2001.
               2.  S. Balachandra Rao, Indian Astronomy An Introduction, Universities Press, Hyderabad, 2000
               3.  History of  Astronomy: A Handbook, Edited  by K. Ramasubramanian, Aniket Sule and
                   Mayank Vahia, SandHI, IIT Bombay, and  T.I.F.R. Mumbai, 2016.
               4.  B.V.  Subbarayappa  and  K.V.  Sarma,  Indian  Astronomy:  A  Source  Book,  Nehru  Centre,
                   Bombay, 1985.
               5.  Tantrasaṅgraha of Nīlakaṇṭha Somayājī, Translation and Notes, K. Ramasubramanian and M.
                   S. Sriram, Hindustan Book Agency, New Delhi 2011.
























                                                                25
   22   23   24   25   26   27   28   29   30   31   32