The effect of a total solar eclipse on long path VLF transmission

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dc.contributor.authorKaufmann P.
dc.contributor.authorSchaal R.E.
dc.date.accessioned2024-05-08T14:04:43Z
dc.date.available2024-05-08T14:04:43Z
dc.date.issued1968
dc.description.abstractThe effects of the total solar eclipse of 12 November 1966 on VLF transmissions at 26·1 kHz transmitted from NPM, Hawaii, and received at São Paulo, are presented. The eclipse occurred during the sunrise transition period, making the data interpretation rather difficult. There was a clearly-marked change of phase, corresponding to a maximum delay of 12·3 sec. © 1968.
dc.description.firstpage469
dc.description.issuenumber3
dc.description.lastpage471
dc.description.volume30
dc.identifier.doi10.1016/0021-9169(68)90119-0
dc.identifier.issn0021-9169
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38703
dc.relation.ispartofJournal of Atmospheric and Terrestrial Physics
dc.rightsAcesso Restrito
dc.titleThe effect of a total solar eclipse on long path VLF transmission
dc.typeArtigo
local.scopus.citations23
local.scopus.eid2-s2.0-0004075460
local.scopus.updated2024-03-12
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=0004075460&origin=inward
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