Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/376
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dc.contributor.authorPatel, R.P.
dc.contributor.authorSingh, A.K.
dc.contributor.authorSingh, S.
dc.contributor.authorSingh, Rajesh
dc.contributor.authorSingh, K.
dc.contributor.authorSingh, R.P.
dc.date.accessioned2015-09-10T09:45:36Z
dc.date.accessioned2021-02-12T09:24:17Z-
dc.date.available2015-09-10T09:45:36Z
dc.date.available2021-02-12T09:24:17Z-
dc.date.issued2008
dc.identifier.citationAdvances in Space Research, v.41, p.1699-1703, 2008, doi: 10.1016/j.asr.2007.05.014en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/376-
dc.description.abstractVLF emissions such as hiss, chorus, pulsing hiss, triggered emissions observed at Varanasi (geom. lat. = 14° 55′ N, long. = 153° 55′ E) are reported. An attempt has been made to explain the dynamic spectra in terms of the generation mechanism and propagation through the inhomogeneous magnetoplasma. It is noted that the reported events have propagated along different L-values in the magnetosphere, although they have been recorded at the same station. The ULF waves propagating along geomagnetic field lines modulate the growth rate of VLF waves, which results in the pulsation of VLF hiss intensity. The pulsating growth rate has been computed.en_US
dc.language.isoenen_US
dc.subjectVLF Emissionsen_US
dc.subjectWhistler-Mode wavesen_US
dc.subjectMagnetosphereen_US
dc.subjectWave propagationen_US
dc.subjectLow latitudeen_US
dc.subjectVaranasien_US
dc.titleVLF Emissions observed at the low latitude Indian station Varanasien_US
dc.typeArticleen_US
dc.identifier.accession090869
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