Statistical study of equatorial scintillations at Ancon, Peru

Descripción del Articulo

13 p.
Detalles Bibliográficos
Autores: Tisnado, G., Woodman Pollitt, Ronald Francisco, Pomalaza, J.
Formato: otro
Fecha de Publicación:1970
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/573
Enlace del recurso:http://hdl.handle.net/20.500.12816/573
Nivel de acceso:acceso abierto
Materia:Scintillation
Interferometry
Fluctuations
Ionosphere
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.es_ES.fl_str_mv Statistical study of equatorial scintillations at Ancon, Peru
title Statistical study of equatorial scintillations at Ancon, Peru
spellingShingle Statistical study of equatorial scintillations at Ancon, Peru
Tisnado, G.
Scintillation
Interferometry
Fluctuations
Ionosphere
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Statistical study of equatorial scintillations at Ancon, Peru
title_full Statistical study of equatorial scintillations at Ancon, Peru
title_fullStr Statistical study of equatorial scintillations at Ancon, Peru
title_full_unstemmed Statistical study of equatorial scintillations at Ancon, Peru
title_sort Statistical study of equatorial scintillations at Ancon, Peru
author Tisnado, G.
author_facet Tisnado, G.
Woodman Pollitt, Ronald Francisco
Pomalaza, J.
author_role author
author2 Woodman Pollitt, Ronald Francisco
Pomalaza, J.
author2_role author
author
dc.contributor.author.fl_str_mv Tisnado, G.
Woodman Pollitt, Ronald Francisco
Pomalaza, J.
dc.subject.es_ES.fl_str_mv Scintillation
Interferometry
Fluctuations
Ionosphere
topic Scintillation
Interferometry
Fluctuations
Ionosphere
http://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.es_ES.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
description 13 p.
publishDate 1970
dc.date.accessioned.none.fl_str_mv 2016-11-07T21:11:58Z
2017-12-21T19:41:46Z
dc.date.available.none.fl_str_mv 2016-11-07T21:11:58Z
2017-12-21T19:41:46Z
dc.date.issued.fl_str_mv 1970
dc.type.es_ES.fl_str_mv info:eu-repo/semantics/other
format other
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/573
url http://hdl.handle.net/20.500.12816/573
dc.language.iso.es_ES.fl_str_mv eng
language eng
dc.rights.es_ES.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.uri.es_ES.fl_str_mv https://creativecommons.org/licences/by/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licences/by/4.0/
dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv Instituto Geofísico del Perú
dc.source.none.fl_str_mv reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
institution IGP
reponame_str IGP-Institucional
collection IGP-Institucional
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spelling Tisnado, G.Woodman Pollitt, Ronald FranciscoPomalaza, J.2016-11-07T21:11:58Z2017-12-21T19:41:46Z2016-11-07T21:11:58Z2017-12-21T19:41:46Z1970http://hdl.handle.net/20.500.12816/57313 p.The 136 MHz interferometric system at the past NASA Satellite Track­ing Station in Ancón, Perú, consists of two orthogonal baselines aligned along the North-South and East-West directions. A sizable number of interferometric records intended far operation­al tracking was spoiled by large amplitude and phase fluctuations. Ir - regularities In the ionosphere, those associated with the spread-F phenomena, are the cause of these fluctuations (scintillations). In most of the distorted records the North-South baseline inter­ferometer shows only a slight distort(on from the expected satellite graph whlle in the East-West interferometer the distortions are severe. This clearly shows the anisotropy of the irregularities and that they are elongated and aligned the magnetic field lines(Z) as have been found by other authors. The absence of North-South phase distortions when East­West distortions are present facilitates the detection of weak scintillations against the background noise. Far the purpose of this report the East-West baseline interferometric distortion was taken as an indication of scintillations.application/pdfengInstituto Geofísico del Perúinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/ScintillationInterferometryFluctuationsIonospherehttp://purl.org/pe-repo/ocde/ford#1.05.01Statistical study of equatorial scintillations at Ancon, Peruinfo:eu-repo/semantics/otherreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALStatistical study of equatorial scintillations at Ancon, Peru-1970.PDFapplication/pdf68630https://repositorio.igp.gob.pe/bitstreams/6f74fcde-1410-43cb-8c2a-304ec45a1f17/download5a525b7df1ce6146f2279382546ea486MD51LICENSElicense.txttext/plain1748https://repositorio.igp.gob.pe/bitstreams/6123a9c5-ceb9-47a9-b6bb-6f5f85f27263/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILStatistical study of equatorial scintillations at Ancon, Peru-1970.PDF.jpgStatistical study of equatorial scintillations at Ancon, Peru-1970.PDF.jpgIM Thumbnailimage/jpeg75953https://repositorio.igp.gob.pe/bitstreams/a2b7d450-3e96-4e51-869a-83eceb89faf0/downloaddb4538bdcc55d3d82ca0576b96308ffcMD53TEXTStatistical study of equatorial scintillations at Ancon, Peru-1970.PDF.txtStatistical study of equatorial scintillations at Ancon, Peru-1970.PDF.txtExtracted texttext/plain13https://repositorio.igp.gob.pe/bitstreams/560565f8-0612-4581-87dd-3e781507291f/download67e866c735744ec6037b77b623ee022dMD5420.500.12816/573oai:repositorio.igp.gob.pe:20.500.12816/5732024-10-13 23:50:38.592https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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Statistical study of equatorial scintillations at Ancon, Peru
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