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Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/602
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dc.contributor.authorBanola, S.
dc.contributor.authorMaurya, R.N.
dc.contributor.authorChandra, H.
dc.date.accessioned2015-10-14T12:06:37Z
dc.date.accessioned2021-02-12T09:34:40Z-
dc.date.available2015-10-14T12:06:37Z
dc.date.available2021-02-12T09:34:40Z-
dc.date.issued2010
dc.identifier.citationJ. Ind. Geophys. Union, v. 14/3, p.195-209, 2010en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/602-
dc.description.abstractA network of stations was operated monitoring amplitude scintillations of 244/251 MHz signal from FLEETSAT (73º E) in India for over a solar cycle. Latitudinal width of the equatorial belt of scintillation is higher during D-months and E-months compared to J-months. There is a positive correlation between the width of the belt and solar activity. Width of the belt decreases with magnetic activity. Equatorial scintillations are inhibited during magnetic disturbances with seasonal and solar cycle dependence. An analysis covering more than 200 geomagnetic storm events show scintillations at low latitudes can be either inhibited or triggered during storms depending on the phase of the storm and local time of occurrence.en_US
dc.language.isoenen_US
dc.subjectSolar activityen_US
dc.subjectGeomagnetic activityen_US
dc.subjectVHFen_US
dc.subjectScintillationsen_US
dc.subjectStormsen_US
dc.titleSolar and geomagnetic activity control on equatorial VHF Scintillations in the Indian regionen_US
dc.typeArticleen_US
dc.identifier.accession091100
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