Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/124
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dc.contributor.authorRangarajan, G.K.
dc.date.accessioned2015-05-21T10:40:47Z
dc.date.accessioned2021-02-12T10:04:27Z-
dc.date.available2015-05-21T10:40:47Z
dc.date.available2021-02-12T10:04:27Z-
dc.date.issued1975
dc.identifier.citationProc. "Equatorial Geomagnetic Phenomena", IIG, Bombay, p.218-226, May 15-16, 1975.en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/124-
dc.description.abstractPower spectral estimates unbiased by noise of horizontal intensity observations from three low and middle latitude stations, well separated from each other, in the period range 8 to 60 days are obtained adopting a procedure described by Black (1970). Results confirm that amplitudes at different frequencies exhibit latitudinal dependence. A significantly determined peak corresponding to a period of 13.9 days and absence of its sub harmonic near 28 days indicates the tendency for equi-distant spacing of solar active regions. Several other significant periodicities are also detected.en_US
dc.language.isoenen_US
dc.subjectGeomagnetic spectrumen_US
dc.subjectGeomagnetic activityen_US
dc.subjectMagnetic fielden_US
dc.subjectNoiseen_US
dc.titleGeomagnetic spectrum unbiased by noise 8 to 60 daysen_US
dc.typeArticleen_US
dc.identifier.accession090632
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