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Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/546
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dc.contributor.authorSingh, Ashutosh K.
dc.contributor.authorPatel, R.P.
dc.contributor.authorSingh, Rajesh
dc.contributor.authorSingh, K.K.
dc.contributor.authorSingh, A.K.
dc.date.accessioned2015-10-07T05:45:04Z
dc.date.accessioned2021-02-12T09:25:27Z-
dc.date.available2015-10-07T05:45:04Z
dc.date.available2021-02-12T09:25:27Z-
dc.date.issued2009
dc.identifier.citationEarth Planets Space, v.61/10, p.1179–1183, 2009, doi: 10.1186/BF03352969en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/546-
dc.description.abstractThe discrete VLF chorus emissions recorded at low latitude ground station Jammu (geomag. lat. = 22°26′N, L = 1.17) are reported and their characteristics based on spectral analysis have been carried out. These discrete chorus emissions are falling tone emissions which are rarely observed at low latitude ground stations. These discrete chorus emissions are generated during a strong geomagnetic storm period of 2–7 May, 1998. We have computed the frequency sweep rate, repetition period and source region of the individual chorus elements. It is observed that the sweep rate increases with time.en_US
dc.language.isoenen_US
dc.subjectVLF emissionen_US
dc.subjectWhistler-mode wavesen_US
dc.subjectGeomagnetic stormen_US
dc.subjectJammuen_US
dc.titleCharacteristics of discrete VLF falling-tone chorus emissions observed at low latitude ground station Jammuen_US
dc.typeArticleen_US
dc.identifier.accession091062
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