Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/36594
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dc.contributor.authorChauhan, N S-
dc.contributor.authorGurm, H S-
dc.date.accessioned2016-11-02T05:45:54Z-
dc.date.available2016-11-02T05:45:54Z-
dc.date.issued1985-02-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36594-
dc.description13-16en_US
dc.description.abstractThe monthly values of production and loss rate have been inferred by fitting the computed and observed total electron contents (TEC) from A TS-6 transmissions at six closely spaced low-latitude stations. A sunrise model of the low-latitude ionosphere is constructed by solving the plasma continuity equation. Comparison between the computed and the observed values of TEC yields the best fit average production rate of atomic oxygen at sunrise as 1.26 x 1013m-2sec-1 and average loss coefficient at 300km as 1.13 x 10-5-sec-1. The production rates for all the stations show semi-annual variations with maxima in equinoxes and minima in solstices. Latitudinally, it exhibits an increasing trend in its values towards the equator. The summer-to-winter ratio in loss coefficient is 1:2 at Patiala and it diminishes towards the equator. The stormtime production rate is found to exceed the quiettime value.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.14(1) [February 1985]en_US
dc.titleQuiet & Stormtime Production & Loss Rates: Smith's Techniqueen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.14(1) [February 1985]

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