Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/3994
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dc.contributor.authorSingh, D P-
dc.contributor.authorSingh, U P-
dc.date.accessioned2009-04-24T07:29:00Z-
dc.date.available2009-04-24T07:29:00Z-
dc.date.issued2006-02-
dc.identifier.issn0367-8393-
dc.identifier.urihttp://hdl.handle.net/123456789/3994-
dc.description22-25en_US
dc.description.abstractPossibility of sideband generation at low, middle and high latitudes is studied considering non-linear interaction between resonant electrons and very low frequency signals transmitted into the magnetosphere. It is shown that as L value increases, sideband spacing decreases and, at low L shells, frequency difference of 1500 Hz in interacting signals (i.e. from 2500 to 4000 Hz or from 4000 to 5500 Hz) produces insignificant spacing values. It is also shown that mean fractional spacing at low latitudes is more than maximum(observed) fractional spacing at L = 4, indicating that sideband generation at low latitudes has a remote possibility.en_US
dc.language.isoen_USen_US
dc.publisherCSIRen_US
dc.sourceIJRSP Vol.35(1) [February 2006]en_US
dc.subjectWave-particle interactionen_US
dc.subjectWhistler wavesen_US
dc.subjectWave propagationen_US
dc.titleProbability of sideband generation at low latitudesen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.35(1) [February 2006]

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