Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/36372
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dc.contributor.authorGhosh, S N-
dc.contributor.authorMidya, S K-
dc.date.accessioned2016-10-27T11:15:04Z-
dc.date.available2016-10-27T11:15:04Z-
dc.date.issued1989-02-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36372-
dc.description33-35en_US
dc.description.abstractFollowing Barth’s mechanism a theoretical curve of 5577 Å line emission at night with height is presented. An empirical relation between emission and height is then obtained from it. Experimental curve obtained by Kulkarni P V [J Geophys Res (USA), 81 (1976) 3740] gives intensity which agrees with that obtained from the curve of Barth’s mechanism. The intensity of 5577 Å line comes out to be 156 Rayleigh from the Chapman’s curve vis-à-vis 210 Rayleigh from the Barth’s mechanism, the latter value agrees with the accepted value 200 Rayleigh.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.18(1) [February 1989]en_US
dc.title5577 Å Night Airglow Emission from Barth’s and Chapman’s Mechanismsen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.18(1) [February 1989]

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