An upper bound on the solar radar cross section at 50 MHz

Descripción del Articulo

We have made 16 unsuccessful attempts, in February and October 2003, and February 2004, to observe solar echoes using the 50 MHz radar at Jicamarca in Peru. The upper bound that we have determined on the solar cross section is significantly lower than the average of earlier reported observations. In...

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Detalles Bibliográficos
Autores: Coles, W.A., Harmon, J. K., Sulzer, M. P., Chau Chong Shing, Jorge Luis, Woodman Pollitt, Ronald Francisco
Formato: artículo
Fecha de Publicación:2006
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/1884
Enlace del recurso:http://hdl.handle.net/20.500.12816/1884
https://doi.org/10.1029/2005JA011416
Nivel de acceso:acceso abierto
Materia:Radar
Solar
Echoes
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv An upper bound on the solar radar cross section at 50 MHz
title An upper bound on the solar radar cross section at 50 MHz
spellingShingle An upper bound on the solar radar cross section at 50 MHz
Coles, W.A.
Radar
Solar
Echoes
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short An upper bound on the solar radar cross section at 50 MHz
title_full An upper bound on the solar radar cross section at 50 MHz
title_fullStr An upper bound on the solar radar cross section at 50 MHz
title_full_unstemmed An upper bound on the solar radar cross section at 50 MHz
title_sort An upper bound on the solar radar cross section at 50 MHz
author Coles, W.A.
author_facet Coles, W.A.
Harmon, J. K.
Sulzer, M. P.
Chau Chong Shing, Jorge Luis
Woodman Pollitt, Ronald Francisco
author_role author
author2 Harmon, J. K.
Sulzer, M. P.
Chau Chong Shing, Jorge Luis
Woodman Pollitt, Ronald Francisco
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Coles, W.A.
Harmon, J. K.
Sulzer, M. P.
Chau Chong Shing, Jorge Luis
Woodman Pollitt, Ronald Francisco
dc.subject.none.fl_str_mv Radar
Solar
Echoes
topic Radar
Solar
Echoes
http://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.none.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
description We have made 16 unsuccessful attempts, in February and October 2003, and February 2004, to observe solar echoes using the 50 MHz radar at Jicamarca in Peru. The upper bound that we have determined on the solar cross section is significantly lower than the average of earlier reported observations. In this paper we will describe the observations, discuss the noise and interference from solar bursts, and suggest possible reasons why the echo might be weaker than expected.
publishDate 2006
dc.date.accessioned.none.fl_str_mv 2018-07-16T15:54:17Z
dc.date.available.none.fl_str_mv 2018-07-16T15:54:17Z
dc.date.issued.fl_str_mv 2006-04
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Coles, W. A., Harmon, J. K., Sulzer, M. P., Chau, J. L., & Woodman, R. F. (2006). An upper bound on the solar radar cross section at 50 MHz.==$Journal of Geophysical Research: Space Physics, 111$==(A4), A04102. https://doi.org/10.1029/2005JA011416
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/1884
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1029/2005JA011416
identifier_str_mv Coles, W. A., Harmon, J. K., Sulzer, M. P., Chau, J. L., & Woodman, R. F. (2006). An upper bound on the solar radar cross section at 50 MHz.==$Journal of Geophysical Research: Space Physics, 111$==(A4), A04102. https://doi.org/10.1029/2005JA011416
index-oti2018
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/1884
https://doi.org/10.1029/2005JA011416
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:2169-9380
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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eu_rights_str_mv openAccess
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dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
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 Coles, W.A.Harmon, J. K.Sulzer, M. P.Chau Chong Shing, Jorge LuisWoodman Pollitt, Ronald Francisco2018-07-16T15:54:17Z2018-07-16T15:54:17Z2006-04Coles, W. A., Harmon, J. K., Sulzer, M. P., Chau, J. L., & Woodman, R. F. (2006). An upper bound on the solar radar cross section at 50 MHz.==$Journal of Geophysical Research: Space Physics, 111$==(A4), A04102. https://doi.org/10.1029/2005JA011416index-oti2018http://hdl.handle.net/20.500.12816/1884Journal of Geophysical Research: Space Physicshttps://doi.org/10.1029/2005JA011416We have made 16 unsuccessful attempts, in February and October 2003, and February 2004, to observe solar echoes using the 50 MHz radar at Jicamarca in Peru. The upper bound that we have determined on the solar cross section is significantly lower than the average of earlier reported observations. In this paper we will describe the observations, discuss the noise and interference from solar bursts, and suggest possible reasons why the echo might be weaker than expected.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/RadarSolarEchoeshttp://purl.org/pe-repo/ocde/ford#1.05.01An upper bound on the solar radar cross section at 50 MHzinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALA0014-63.pdfA0014-63.pdfapplication/pdf276675https://repositorio.igp.gob.pe/bitstreams/151e9618-c7e8-4f10-8901-c9d67539c21b/download3581888db43ce50127c6656566a34746MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/7a54e4ba-ceaf-43c0-99b1-81b31abdd306/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILA0014-63.pdf.jpgA0014-63.pdf.jpgIM Thumbnailimage/jpeg102672https://repositorio.igp.gob.pe/bitstreams/c842c6d9-8aa0-4f94-b8bd-88cfa345644d/downloadf4f40cee4235d8a061a91400c030f3f8MD53TEXTA0014-63.pdf.txtA0014-63.pdf.txtExtracted texttext/plain35075https://repositorio.igp.gob.pe/bitstreams/7971b151-9031-40c8-a208-1913e552c91f/download66534785bcaaaa9354ee0ad44c957a37MD5420.500.12816/1884oai:repositorio.igp.gob.pe:20.500.12816/18842024-10-12 22:18:10.202https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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