Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/38083
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dc.contributor.authorPradhan, S.M.-
dc.contributor.authorTiwari, R. S.-
dc.contributor.authorSingh, B.-
dc.contributor.authorSrivastava, S. K.-
dc.contributor.authorTantry, B. A. P.-
dc.date.accessioned2016-12-02T07:02:25Z-
dc.date.available2016-12-02T07:02:25Z-
dc.date.issued1972-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/38083-
dc.description218-220en_US
dc.description.abstractThe plasma instability mechanisms previously discussed by G. C. Reid [J. geophys. Res., 73 (1968), 1627] and S. Kato [Rep. Ionosph. Space Res., Japan, 13 (1959), 62] have been applied to obtain the variation of the size of ionospheric irregularities due to changes in altitude as well as latitude. The variation of the size of the irregularities with altitude has been computed and is found to be in good agreement with the recent satellite observations. The latitude variation of the size of the irregularities in E-region is also calculated and successfully correlated with the experimental observations.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.01(3) [September 1972]en_US
dc.titleIonospheric Irregularities & Plasma Instabilityen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.01(3) [September 1972]

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