Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/36991
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dc.contributor.authorDabas, R S-
dc.contributor.authorTyagi, T R-
dc.contributor.authorSomayajulu, Y V-
dc.contributor.authorLal, J B-
dc.date.accessioned2016-11-09T09:45:13Z-
dc.date.available2016-11-09T09:45:13Z-
dc.date.issued1980-12-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36991-
dc.description234-241en_US
dc.description.abstractUsing the theoretical modelling of diffraction patterns produced by isolated ionospheric irregularities at E-region height, the scale sizes and maximum electron density enhancements are determined for the events observed at Delhi (lat., 28.6° N; long., 77.2°E) on 140 MHz radio beacon transmission from ATS-6 geostationary satellite. Some model calculations are done to see the effect of scale size and electron density on the characteristics of observed diffraction pattern. Simulation of some of the events observed on 140 MHz radio beacon transmission by isolated ionospheric irregularities at the E-region heights suggests that these are produced by the one dimensional Gaussian fluctuations in electron density. The scale sizes and maximum electron density enhancements of the isolated irregularities determined are found to vary from 30 to 300 m and 4.3 x 1011 to 1.4 X 1012 eI./m3, respectively. The results are compared with those of other workers.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.09(6) [December 1980]en_US
dc.titleDiffraction of 140 MHz ATS-6 Signal by Lenslike Ionospheric Irregularitiesen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.09(6) [December 1980]

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