VLF Emissions observed at the low latitude Indian station Varanasi

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dc.contributor.author Patel, R.P.
dc.contributor.author Singh, A.K.
dc.contributor.author Singh, S.
dc.contributor.author Singh, Rajesh
dc.contributor.author Singh, K.
dc.contributor.author Singh, R.P.
dc.date.accessioned 2015-09-10T09:45:36Z
dc.date.accessioned 2021-02-12T09:24:17Z
dc.date.available 2015-09-10T09:45:36Z
dc.date.available 2021-02-12T09:24:17Z
dc.date.issued 2008
dc.identifier.citation Advances in Space Research, v.41, p.1699-1703, 2008, doi: 10.1016/j.asr.2007.05.014 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/376
dc.description.abstract VLF 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.iso en en_US
dc.subject VLF Emissions en_US
dc.subject Whistler-Mode waves en_US
dc.subject Magnetosphere en_US
dc.subject Wave propagation en_US
dc.subject Low latitude en_US
dc.subject Varanasi en_US
dc.title VLF Emissions observed at the low latitude Indian station Varanasi en_US
dc.type Article en_US
dc.identifier.accession 090869


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