Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/36532
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dc.contributor.authorRastogi, R G-
dc.date.accessioned2016-11-01T09:08:42Z-
dc.date.available2016-11-01T09:08:42Z-
dc.date.issued1986-02-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36532-
dc.description10-16en_US
dc.description.abstractThe comparison of the scintillations of VHF radio beacons from geostationary satellite Geos-1 (74.9°W) and the vertical incidence ionograms at Huancayo (75.3°W) have shown that the diffused echoes observed on the ionograms during late night or early morning hours are not due to oblique reflections from new ionization but due to in situ plasma irregularities (bubbles) present on the path of satellite-to-ground radio path. These events are preceded with rapid rise of the F-Iayer. Multi-satellite and multi-station radio scintillation records indicate the presence of a westward movement of the bubbles corresponding on eastward electric field during these not very normal post-midnight events.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.15(1) [February 1986]en_US
dc.titlePost-midnight Equatorial Spread-Fen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.15(1) [February 1986]

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