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________________ JANUARY, 1984 Differentiating both sides w.r.t time t, we have d(RMB) = d (Radius of Meru's base on flat earth remains constant.) Thus the rate of variation of radii of the solar mandalas is in toto the same as the rate of variation of their north polar distances (NPD) from periphery of the mount Meru's base on flat earth. So using Eq. No. (3), we have from Eq. No. (12) that 48 Y/day (day and night) (RMB) Mn 61 Using Eq. No. (11), we have &(DM2) Mn C or Mn (13) i.e. diameters of the solar mandalas vary as 535 yojanas per day (day 61 and night). = (NPD of Mn)+0........ = 2 The circumference of any solar mandala has verily been computed in an alike manner as R.C. Gupta1 has shown in his paper 'Circumference of Jambudvipa in Jaina Comography' that circumference of Jambudvipa had been computed from its diameter by using only approximate values of π. They had commonly employed the following formula CM2 = = 5 535Y/days 61 √ 10 D2 Jain Education International 95 Mn = √10 D1 where CM=Circumference of Mn (nth solar mandala). But they did not use the correct value of the square root of ten but instead, for finding out the square root of a non-square positive number N, the following bionominal approximation was frequently used during the ancient and medieval times; ..(12) Mn For Private & Personal Use Only 14 Gupta, R. C. (1974), 'Circumference of Jambudvipa in Jaina Cosmography', IJHS, Vol 10, No. 1, pp. 38-46. (14) www.jainelibrary.org
SR No.520073
Book TitleJain Journal 1984 01
Original Sutra AuthorN/A
AuthorJain Bhawan Publication
PublisherJain Bhawan Publication
Publication Year1984
Total Pages49
LanguageEnglish
ClassificationMagazine, India_Jain Journal, & India
File Size3 MB
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