A model of equatorial and low latitude VHF scintillation in India

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dc.contributor.authorIyer, K.N.
dc.contributor.authorSouza, J.R.
dc.contributor.authorPathan, B.M.
dc.contributor.authorJivani, M.N.
dc.contributor.authorJoshi, H.P.
dc.contributor.authorAbdu, M.A.
dc.date.accessioned2015-09-22T09:57:25Z
dc.date.accessioned2021-02-12T09:25:01Z
dc.date.available2015-09-22T09:57:25Z
dc.date.available2021-02-12T09:25:01Z
dc.date.issued2006
dc.description.abstractUsing the observed VHF scintillations at equatorial and anomaly crest stations in India during the years 1987-1989, an empirical model is developed. The model employs the cubic spline technique to reproduce the variation of scintillation occurrence with local time, season, solar activity and latitude. The modelled values are compared with observed ones and the agreement is found to be quite good.en_US
dc.identifier.accession090970
dc.identifier.citationIndian Journal of Radio and Space Physics, v.35, p.98-104, 2006en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/464
dc.language.isoenen_US
dc.subjectIonospheric scintillationsen_US
dc.subjectCubic spline techniqueen_US
dc.subjectVHF scintillationsen_US
dc.subjectScintillationsen_US
dc.titleA model of equatorial and low latitude VHF scintillation in Indiaen_US
dc.typeArticleen_US

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