Ozone screening heights deduced from sunrise effects at very low frequencies

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dc.contributor.authorSchaal R.E.
dc.contributor.authorAnanthakrishnan S.
dc.date.accessioned2024-03-13T01:48:28Z
dc.date.available2024-03-13T01:48:28Z
dc.date.issued1970
dc.description.abstractDuring the period August-September of any year, the entire NAA-São Paulo path is illuminated almost simultaneously at sunrise, resulting in a sharp drop in the phase of the received signal. Using sunrise phase transitions and an assumed night-time reflection height of 90 km, an ozone screening height of 58 km was deduced. A calculation of the wavelength of the photo-detaching radiation, using this value of the screening height yielded a value of λ = 3015 A ̊. © 1970.
dc.description.firstpage1831
dc.description.issuenumber11
dc.description.lastpage1834
dc.description.volume32
dc.identifier.doi10.1016/0021-9169(70)90140-6
dc.identifier.issn0021-9169
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38119
dc.relation.ispartofJournal of Atmospheric and Terrestrial Physics
dc.rightsAcesso Restrito
dc.titleOzone screening heights deduced from sunrise effects at very low frequencies
dc.typeArtigo
local.scopus.citations3
local.scopus.eid2-s2.0-49849109961
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=49849109961&origin=inward
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