Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/36815
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dc.contributor.authorGoyal, R K-
dc.contributor.authorMitra, S N-
dc.date.accessioned2016-11-07T07:19:15Z-
dc.date.available2016-11-07T07:19:15Z-
dc.date.issued1982-10-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36815-
dc.description195-198en_US
dc.description.abstractThe methods of calculating the effective recombination coefficient (ɑ) of lower D-region, namely, (a) post-sunset decay and (b) post-flare decay of integrated field strength on 27 kHz atmospherics have been described. Both the methods give nearly the same values of ɑ. Data on ɑ at different heights have been collected and plotted against height on log log scale. The relationship is found to be linear. A simple formula has been developed to indicate this linear relationship.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.11(5) [October 1982]en_US
dc.titleEstimation of Effective Recombination Coefficient & Its Variation with Height for D-regionen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.11(5) [October 1982]

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