Secular trend of geomagnetic elements in the Indian region

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dc.contributor.author Bhardwaj, S.K.
dc.contributor.author Subbarao, P.B.V.
dc.date.accessioned 2015-11-27T06:42:54Z
dc.date.accessioned 2021-02-12T09:21:06Z
dc.date.available 2015-11-27T06:42:54Z
dc.date.available 2021-02-12T09:21:06Z
dc.date.issued 2013
dc.identifier.citation Earth Planets Space, v.65/12, p.1515-1523, 2013, doi: 10.5047/eps.2013.09.001 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/710
dc.description.abstract In the present study, secular trends and jerks in the geomagnetic elements D, H and Z are investigated at the six Indian magnetic observatories using annual and monthly mean values for all days, quiet days and night base (night time mean). The residuals of all-day annual and monthly means are computed by removing a polynomial fit from their best fitting curves. The residuals of D, H and Z curves do not show any parallelism with the 11-year sunspot cycle. At Alibag, the D residual shows a periodicity of 2 solar cycles, whereas the H and Z residuals indicate a quasi-periodicity of 3 solar cycles for the period 1921–2009. At the Indian stations, an in-phase solar cycle component is observed for 2 of the solar cycles in the D and Z residuals, while the H residual shows out-of-phase variations with the sunspot cycle for the period 1958–2009. Two geomagnetic jerks, 1970 and 1991, are well reflected in the monthly and annual mean values in the Indian region, as observed globally. en_US
dc.language.iso en en_US
dc.subject Secular variation en_US
dc.subject Core-mantle en_US
dc.subject Geomagnetic jerks en_US
dc.subject Solar cycle en_US
dc.subject Polynomial fit en_US
dc.subject Indian region en_US
dc.title Secular trend of geomagnetic elements in the Indian region en_US
dc.type Article en_US
dc.identifier.accession 091374


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