Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/37965
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dc.contributor.authorPandey, V. K.-
dc.contributor.authorMahajan, K. K.-
dc.date.accessioned2016-12-01T06:15:23Z-
dc.date.available2016-12-01T06:15:23Z-
dc.date.issued1973-06-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37965-
dc.description134-138en_US
dc.description.abstractElectron density profiles from the Alouctte-II satellite are used to study the latitudinal distribution of electrons to heights up to 3000 km in the topside ionosphere. The electron density in the topside decreases as one goes away from the equator, resulting in a trough at mid to high latitudes for both day and night conditions in the winter hemisphere and only for night conditions in other seasons. This trough, however, is not always seen at the F2 peak. On the dayside, while the trough is not observed for altitudes up to 1000 km, the higher altitudes indicate a tendency towards the formation of the trough. The plasma scale heights, obtained from the electron density profiles, show a sharp decrease at and above the trough latitudes, indicating the dominance of atomic oxygen ions and the depletion of lighter ions at these latitudes. These results are in agreement with the ion composition measurements on various satellites and the polar wind theory which predicts an upward plasma flow at the high latitudes.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.02(2) [June 1973]en_US
dc.titleLatitudinal Distribution of Electron Concentration from the Alouette-II Topside Sounderen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.02(2) [June 1973]

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