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dc.contributor.authorRoy, M.
dc.contributor.authorRao, D.R.K.
dc.date.accessioned2015-05-13T10:21:38Z
dc.date.accessioned2021-02-12T09:22:48Z-
dc.date.available2015-05-13T10:21:38Z
dc.date.available2021-02-12T09:22:48Z-
dc.date.issued1998
dc.identifier.citationEarth Planet Space, v.50, p.847-851, 1998, doi: 10.1186/BF03352178en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/70-
dc.description.abstractThe micropulsation data (Pc3–Pc4 range) from off-equatorial and equatorial stations Alibag (ABG) and Tirunelvelli (TIR) in the Indian zone during 1991 are analysed for delineating the electrojet effect. The ratios of the spectral amplitudes at significant frequency bands the horizontal component of the magnetic field at TIR to that at ABG are worked out as a function of frequency. The results show that the lower frequencies undergo larger equatorial amplification. However, above a certain frequency the pulsation signal is found to attenuate rather than exhibit the general enhancement. The ratio becomes minimum around the period, 18 to 24 sec. At further higher frequencies, there is again the normal electrojet amplification. The explanation of such a behaviour of the electrojet on the pulsation amplitude is rather difficult at the present stage and to some extent becomes controversial even if it is offered.en_US
dc.language.isoenen_US
dc.subjectEarth planet spaceen_US
dc.subjectEquatorial electrojeten_US
dc.subjectMicropulsationen_US
dc.subjectMagnetic fielden_US
dc.titleFrequency dependence of equtorial electrojet effect on geomagnetic micropulsationsen_US
dc.typeArticleen_US
dc.identifier.accession090560
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