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 |
|