Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance

Lightning generated signals recorded at a low-latitude station, Suva (18.2° S, 178.3° E) Fiji, in the South Pacific region, during September 2003–July 2004, are used to study the propagation features and the reflection heights of tweek atmospherics in the waveguide forme...

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Main Authors: S. Kumar, A. Kishore, V. Ramachandran
Format: Article
Language:English
Published: Copernicus Publications 2008-06-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/26/1451/2008/angeo-26-1451-2008.pdf
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spelling doaj-aa617ca1d8ef4b2a9444409518c73b932020-11-25T00:12:21ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762008-06-01261451145910.5194/angeo-26-1451-2008Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distanceS. Kumar0A. Kishore1V. Ramachandran2School of Engineering and Physics, The University of the South Pacific, Suva, FijiSchool of Engineering and Physics, The University of the South Pacific, Suva, FijiSchool of Engineering and Physics, The University of the South Pacific, Suva, FijiLightning generated signals recorded at a low-latitude station, Suva (18.2&deg; S, 178.3&deg; E) Fiji, in the South Pacific region, during September 2003&ndash;July 2004, are used to study the propagation features and the reflection heights of tweek atmospherics in the waveguide formed by the Earth's surface and the lower ionosphere. Tweeks are observed only during the local night and the maximum harmonic (<I>n</I>) recorded is six. The occurrence of tweeks with higher <I>n</I> progressively decreases as <I>n</I> increases. The dispersed part of tweeks decreases as <I>n</I> increases. The attenuation factor has been calculated for tweeks with <I>n</I>=1&ndash;3. The ionospheric reflection heights obtained assuming the transverse magnetic mode of propagation for tweek signals vary from 83&ndash;92 km. A higher harmonic of the same tweek is reflected from about 2.0 km higher than the lower harmonic. For 90% of tweeks, propagation distances are estimated to be between 1000&ndash;5000 km. Tweeks with lower <I>n</I> propagate longer distances than the tweeks with higher <I>n</I>.https://www.ann-geophys.net/26/1451/2008/angeo-26-1451-2008.pdf
collection DOAJ
language English
format Article
sources DOAJ
author S. Kumar
A. Kishore
V. Ramachandran
spellingShingle S. Kumar
A. Kishore
V. Ramachandran
Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance
Annales Geophysicae
author_facet S. Kumar
A. Kishore
V. Ramachandran
author_sort S. Kumar
title Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance
title_short Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance
title_full Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance
title_fullStr Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance
title_full_unstemmed Higher harmonic tweek sferics observed at low latitude: estimation of VLF reflection heights and tweek propagation distance
title_sort higher harmonic tweek sferics observed at low latitude: estimation of vlf reflection heights and tweek propagation distance
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2008-06-01
description Lightning generated signals recorded at a low-latitude station, Suva (18.2&deg; S, 178.3&deg; E) Fiji, in the South Pacific region, during September 2003&ndash;July 2004, are used to study the propagation features and the reflection heights of tweek atmospherics in the waveguide formed by the Earth's surface and the lower ionosphere. Tweeks are observed only during the local night and the maximum harmonic (<I>n</I>) recorded is six. The occurrence of tweeks with higher <I>n</I> progressively decreases as <I>n</I> increases. The dispersed part of tweeks decreases as <I>n</I> increases. The attenuation factor has been calculated for tweeks with <I>n</I>=1&ndash;3. The ionospheric reflection heights obtained assuming the transverse magnetic mode of propagation for tweek signals vary from 83&ndash;92 km. A higher harmonic of the same tweek is reflected from about 2.0 km higher than the lower harmonic. For 90% of tweeks, propagation distances are estimated to be between 1000&ndash;5000 km. Tweeks with lower <I>n</I> propagate longer distances than the tweeks with higher <I>n</I>.
url https://www.ann-geophys.net/26/1451/2008/angeo-26-1451-2008.pdf
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AT akishore higherharmonictweeksfericsobservedatlowlatitudeestimationofvlfreflectionheightsandtweekpropagationdistance
AT vramachandran higherharmonictweeksfericsobservedatlowlatitudeestimationofvlfreflectionheightsandtweekpropagationdistance
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