Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6982
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dc.contributor.authorRavindra, B-
dc.contributor.authorJavaraiah, J-
dc.date.accessioned2020-11-12T15:22:38Z-
dc.date.available2020-11-12T15:22:38Z-
dc.date.issued2018-02-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 340, pp. 259-260en_US
dc.identifier.isbn978-1-108-47109-1-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6982-
dc.descriptionRestricted Access © International Astronomical Union https://doi.org/10.1017/S1743921318001187en_US
dc.description.abstractSunspot activity exhibits hemispheric asymmetry. We study the long-term variations in the hemispheric sunspot area from Kodaikanal white-light data during 1921 – 2011. The results on the presence or absence of double peak in an individual solar cycle, dominant hemispheric activity, and phase lag between the activities of northern and southern hemispheres, etc., are presented.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.titleStudy of long-term variations in hemispheric asymmetry of solar activityen_US
dc.typeArticleen_US
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