Geomagnetic spectrum unbiased by noise 8 to 60 days

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dc.contributor.author Rangarajan, G.K.
dc.date.accessioned 2015-05-21T10:40:47Z
dc.date.accessioned 2021-02-12T10:04:27Z
dc.date.available 2015-05-21T10:40:47Z
dc.date.available 2021-02-12T10:04:27Z
dc.date.issued 1975
dc.identifier.citation Proc. "Equatorial Geomagnetic Phenomena", IIG, Bombay, p.218-226, May 15-16, 1975. en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/124
dc.description.abstract Power 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.iso en en_US
dc.subject Geomagnetic spectrum en_US
dc.subject Geomagnetic activity en_US
dc.subject Magnetic field en_US
dc.subject Noise en_US
dc.title Geomagnetic spectrum unbiased by noise 8 to 60 days en_US
dc.type Article en_US
dc.identifier.accession 090632


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