The new submillimeter-wave solar telescope

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dc.contributor.authorKaufmann P.
dc.contributor.authorCosta J.E.R.
dc.contributor.authorGimenez de Castro C.G.
dc.contributor.authorHadano Y.R.
dc.contributor.authorKingsley J.S.
dc.contributor.authorKingsley R.K.
dc.contributor.authorLevato H.
dc.contributor.authorMarun A.
dc.contributor.authorRaulin J.-P.
dc.contributor.authorRovira M.
dc.contributor.authorCorreia E.
dc.contributor.authorSilva A.V.R.
dc.date.accessioned2024-03-13T01:46:52Z
dc.date.available2024-03-13T01:46:52Z
dc.date.issued2001
dc.description.abstractA new and unique solar submillimeter telescope (SST) was installed in the EI Leoncito site, Argentina Andes. It has a 1.5 m radome-enclosed cassegrain antenna, and arrays of four 212 GHz and two 405 GHz radiometers placed in the focal plane. We present a brief technical description of the system, preliminary results on its performance, the atmospheric opacity measured at the site, and the first detection of solar flare submm-w emissions.
dc.description.firstpage439
dc.description.lastpage442
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38032
dc.relation.ispartofSBMO/IEEE MTT-S International Microwave and Optoelectronics Conference Proceedings
dc.rightsAcesso Restrito
dc.subject.otherlanguageAtmospheric opacity
dc.subject.otherlanguageRadio-telescopes
dc.subject.otherlanguageSolar flares
dc.subject.otherlanguageSubmm-w antennas
dc.subject.otherlanguageSubmm-w radiometers
dc.titleThe new submillimeter-wave solar telescope
dc.typeArtigo de evento
local.scopus.citations17
local.scopus.eid2-s2.0-0035757736
local.scopus.subjectAtmospheric opacity
local.scopus.subjectSolar flares
local.scopus.subjectSubmillimeter-wave antenna
local.scopus.subjectSubmillimeter-wave radiometers
local.scopus.subjectSubmillimeter-wave solar telescope
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=0035757736&origin=inward
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