Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/57444
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dc.contributor.authorAdhikari, Binod-
dc.contributor.authorPandit, Drabindra-
dc.contributor.authorBaruwal, Prashrit-
dc.contributor.authorThapa, Opendra-
dc.contributor.authorAdhikari, Niraj-
dc.contributor.authorKaphle, Bidur-
dc.contributor.authorBhattarai, Pratik-
dc.contributor.authorChapagain, Narayan P.-
dc.contributor.authorAdhikari, Sarala-
dc.date.accessioned2021-06-07T09:52:31Z-
dc.date.available2021-06-07T09:52:31Z-
dc.date.issued2020-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/57444-
dc.description128-138en_US
dc.description.abstractThis paper has been performed to study the Alfvenic Mach number (M­A) in relation to Field Aligned Currents (FACs), Polar Cap Potential (PCV), Dawn Dusk Electric Field (Ey) during different geomagnetic conditions. The relations of M­A with FACs, PCV and interplanetary electric field (IEF)-EY not solely dependent on any solar wind parameter but also associate with prior, main, and post conditions of geomagnetic storms. This study has shown that Prior to the arrival of interplanetary shock (IS),  and  show good relationship with FAC, PCV, EFY, and solar wind parameters, as the space weather seems unperturbed. The positive correlations among the various parameters have obtained due to the merging of two different interplanetary coronal mass ejections (ICMEs) driven solar storms and consequential intense southward interplanetary magnetic field. The negative relationships among the selected parameters may have been due to the slow recovery of the IMF-Bz component. This study indicate that the preceding solar winds could be associatedon the variance of M­A of a geomagnetic event, in turn might have its effects on FACs, PCV, Ey and in other solar wind parameters.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.49(3) [September 2020]en_US
dc.subjectGeomagnetic conditionsen_US
dc.subjectField aligned currentsen_US
dc.subjectPolar cap potentialen_US
dc.subjectDawn dusk electric fielden_US
dc.subjectAlfven Mach numberen_US
dc.titleCorrelation of Alfvén Mach number with field aligned current, polar cap potential and dawn dusk electric field during Quiet and extreme solar wind conditionsen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.49(3) [September 2020]

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