Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7214
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dc.contributor.authorPAI, VENKETESWARA R.en_US
dc.contributor.authorSriram, M. S.en_US
dc.contributor.authorSrinivas, M. D.en_US
dc.contributor.editorPAI, VENKETESWARA K.en_US
dc.contributor.editorRamasubramanian, K.en_US
dc.contributor.editorSriram, M. S.en_US
dc.contributor.editorSrinivas, M. D.en_US
dc.date.accessioned2022-06-24T11:02:47Z
dc.date.available2022-06-24T11:02:47Z
dc.date.issued2018-03en_US
dc.identifier.citationKaraṇapaddhati of Putumana Somayājī , 101–132.en_US
dc.identifier.isbn978-981-10-6813-3en_US
dc.identifier.isbn978-981-10-6814-0en_US
dc.identifier.urihttps://link.springer.com/chapter/10.1007/978-981-10-6814-0_4en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7214
dc.description.abstractThe above verse defines the mandakendrahārakas of the planets. It may be recalled that the mandakendra is the difference between the planet and its mandocca (apogee). The mandakendra-guṇakāras and the mandakendrahārakas determine the successive approximations to the rate of motion of the mandakendra.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectHumanities and Social Sciencesen_US
dc.subject2018en_US
dc.titleObtaining the hārakas for the planetsen_US
dc.typeBook chapteren_US
dc.contributor.departmentDept. of Humanities and Social Sciencesen_US
dc.title.bookKaraṇapaddhati of Putumana Somayājīen_US
dc.identifier.doihttps://doi.org/10.1007/978-981-10-6814-0_4en_US
dc.identifier.sourcetitleKaraṇapaddhati of Putumana Somayājīen_US
dc.publication.originofpublisherForeignen_US
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