Computation of the khaṇḍa, dhruva, etc. of the Moon
| 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.contributor.department | Dept. of Humanities and Social Sciences | 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.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.identifier.citation | Karaṇapaddhati of Putumana Somayājī. | en_US |
| dc.identifier.doi | https://doi.org/10.1007/978-981-10-6814-0_3 | en_US |
| dc.identifier.isbn | 978-981-13-3896-0 | en_US |
| dc.identifier.isbn | 978-981-10-6813-3 | en_US |
| dc.identifier.sourcetitle | Karaṇapaddhati of Putumana Somayājī | en_US |
| dc.identifier.uri | https://link.springer.com/chapter/10.1007/978-981-10-6814-0_3 | |
| dc.identifier.uri | http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7058 | |
| dc.language.iso | en | en_US |
| dc.publication.originofpublisher | Foreign | 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 |