Frequency dependence of equtorial electrojet effect on geomagnetic micropulsations

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dc.contributor.author Roy, M.
dc.contributor.author Rao, D.R.K.
dc.date.accessioned 2015-05-13T10:21:38Z
dc.date.accessioned 2021-02-12T09:22:48Z
dc.date.available 2015-05-13T10:21:38Z
dc.date.available 2021-02-12T09:22:48Z
dc.date.issued 1998
dc.identifier.citation Earth Planet Space, v.50, p.847-851, 1998, doi: 10.1186/BF03352178 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/70
dc.description.abstract The 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.iso en en_US
dc.subject Earth planet space en_US
dc.subject Equatorial electrojet en_US
dc.subject Micropulsation en_US
dc.subject Magnetic field en_US
dc.title Frequency dependence of equtorial electrojet effect on geomagnetic micropulsations en_US
dc.type Article en_US
dc.identifier.accession 090560


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