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DC Field | Value | Language |
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dc.contributor.author | PAI, VENKETESWARA R. | en_US |
dc.contributor.author | Ramasubramanian, K. | en_US |
dc.contributor.author | Sriram, M. S. | en_US |
dc.contributor.author | Srinivas, M. D. | en_US |
dc.date.accessioned | 2022-06-13T04:41:15Z | |
dc.date.available | 2022-06-13T04:41:15Z | |
dc.date.issued | 2018-03 | en_US |
dc.identifier.citation | Karaṇapaddhati of Putumana Somayājī. | en_US |
dc.identifier.isbn | 978-981-13-3896-0 | en_US |
dc.identifier.isbn | 978-981-10-6813-3 | en_US |
dc.identifier.uri | https://link.springer.com/chapter/10.1007/978-981-10-6814-0_3 | en_US |
dc.identifier.uri | http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7058 | |
dc.description.abstract | Let the heap of days (dharādinaugha), and the difference in the revolutions of the Moon and its apogee be mutually divided. Then, from these results, the guṇakāras and hārakas associated with the Moon’s anomaly (candra-kendra) are to be obtained as stated earlier. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Springer Nature | en_US |
dc.subject | Indian astronomy | en_US |
dc.subject | Mean planets | en_US |
dc.subject | Vallyupasaṃhāra technique | en_US |
dc.subject | Kendraphalas | en_US |
dc.subject | Hārakas | en_US |
dc.subject | Kalpādidhruvas | en_US |
dc.subject | Rsines | en_US |
dc.subject | Planetary longitudes | en_US |
dc.subject | Gnomonic shadow | en_US |
dc.subject | Meridian transit | en_US |
dc.subject | Right Ascension | en_US |
dc.subject | 2018 | en_US |
dc.title | Computation of the khaṇḍa, dhruva, etc. of the Moon | en_US |
dc.type | Book chapter | en_US |
dc.contributor.department | Dept. of Humanities and Social Sciences | en_US |
dc.identifier.doi | https://doi.org/10.1007/978-981-10-6814-0_3 | en_US |
dc.identifier.sourcetitle | Karaṇapaddhati of Putumana Somayājī | en_US |
dc.publication.originofpublisher | Foreign | en_US |
Appears in Collections: | BOOK CHAPTERS |
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