Characteristics of discrete VLF falling-tone chorus emissions observed at low latitude ground station Jammu

Singh, Ashutosh K.; Patel, R.P.; Singh, Rajesh; Singh, K.K.; Singh, A.K.

dc.contributor.author	Singh, Ashutosh K.
dc.contributor.author	Patel, R.P.
dc.contributor.author	Singh, Rajesh
dc.contributor.author	Singh, K.K.
dc.contributor.author	Singh, A.K.
dc.date.accessioned	2015-10-07T05:45:04Z
dc.date.accessioned	2021-02-12T09:25:27Z
dc.date.available	2015-10-07T05:45:04Z
dc.date.available	2021-02-12T09:25:27Z
dc.date.issued	2009
dc.identifier.citation	Earth Planets Space, v.61/10, p.1179–1183, 2009, doi: 10.1186/BF03352969	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/546
dc.description.abstract	The 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.iso	en	en_US
dc.subject	VLF emission	en_US
dc.subject	Whistler-mode waves	en_US
dc.subject	Geomagnetic storm	en_US
dc.subject	Jammu	en_US
dc.title	Characteristics of discrete VLF falling-tone chorus emissions observed at low latitude ground station Jammu	en_US
dc.type	Article	en_US
dc.identifier.accession	091062