Night-time anomalies in very low frequency propagation produced by a galactic X-ray source at centaurus

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dc.contributor.authorKaufmann P.
dc.contributor.authorDe Barros M.H.P.
dc.contributor.authorVianna E.N.
dc.date.accessioned2024-03-13T01:48:23Z
dc.date.available2024-03-13T01:48:23Z
dc.date.issued1970
dc.description.abstractNIGHT-TIME propagation of very low frequency (VLF) waves in the terrestrial ionosphere shows considerable variability, both in phase and in amplitude, in comparison with the relatively stable daytime conditions. The night-time anomalies are not yet well understood, a number of them being associated with the presence of energetic particles originating from solar proton events 1. The explanation of others remains obscure. © 1970 Nature Publishing Group.
dc.description.firstpage1080
dc.description.issuenumber5276
dc.description.lastpage1081
dc.description.volume228
dc.identifier.doi10.1038/2281080a0
dc.identifier.issn0028-0836
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38115
dc.relation.ispartofNature
dc.rightsAcesso Restrito
dc.titleNight-time anomalies in very low frequency propagation produced by a galactic X-ray source at centaurus
dc.typeArtigo
local.scopus.citations7
local.scopus.eid2-s2.0-36949055287
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=36949055287&origin=inward
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