New telescopes for ground-based solar observations at submillimeter and mid-infrared

Autores
Kaufmann, Pierre; Levato, Orlando Hugo; Cassiano, Marta M.; Correia, Emilia; Costa, Joaquim E.R.; De Castro, C. Guillermo Giménez; Godoy, Rodolfo Alfredo; Kingsley, Robert K.; Kingsley, Jeffrey S.; Kudaka, Amauri S.; Marcon, Rogério; Martin, Robert; Marun, Adolfo Hector; Melo, Arline M.; Pereyra, Pablo Florencio; Raulin, JeanPierre; Rose, Thomas; Valio, Adriana Silva; Walber, Achim; Wallace, Patrick; Yakubovich, Azriel; Zakia, Maria Beny
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The solar submillimeter-wave telescope (SST) is the only one of its kind dedicated to solar continuous observations. Two radiometers at 0.740 mm (405 GHz), and four at 1.415 mm (212 GHz) are placed in the Cassegrain focal plane of the 1.5-m dish at El Leoncito high altitude site, San Juan, Argentina. The aperture efficiencies are close to design predictions: 20% and 35% for 2 and 4 arcminutes beam sizes at 405 and 212 GHz, respectively. The positioner absolute pointing accuracy is 10 arcseconds. Spectral coverage is complemented by ground-based mid-infrared telescopes developed for high cadence observations in the continuum 10 micron band (30 THz), using small apertures and roomtemperature microbolometer cameras. Using the system, a new solar burst spectral component was discovered, exhibiting fluxes increasing for smaller wavelengths, separated from the well known microwave component. Rapid subsecond pulsations are common for all bursts. The pulsations onset times of appear to be connected to the launch times of CMEs. Active regions are brighter for shorter submillimeter-waves. Mid-IR bright regions are found closely associated with calcium plages and magnetic structures near the solar photosphere. Intense and rapid 10 micron brightening was detected on active centers in association with weak flares. These results raise challenging difficulties for interpretation.
Fil: Kaufmann, Pierre. Universidade Estadual de Campinas; Brasil. Universidade Presbiteriana Mackenzie; Brasil
Fil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Cassiano, Marta M.. Universidade Presbiteriana Mackenzie; Brasil
Fil: Correia, Emilia. Universidade Presbiteriana Mackenzie; Brasil. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Costa, Joaquim E.R.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: De Castro, C. Guillermo Giménez. Universidade Presbiteriana Mackenzie; Brasil
Fil: Godoy, Rodolfo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Kingsley, Robert K.. University of Arizona; Estados Unidos
Fil: Kingsley, Jeffrey S.. University of Arizona; Estados Unidos
Fil: Kudaka, Amauri S.. Universidade Presbiteriana Mackenzie; Brasil
Fil: Marcon, Rogério. “Bernard Lyot” Solar Observatory; Brasil. Universidade Estadual de Campinas; Brasil
Fil: Martin, Robert. Composite Mirror Applications, Inc.; Estados Unidos
Fil: Marun, Adolfo Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Melo, Arline M.. Universidade Presbiteriana Mackenzie; Brasil. Universidade Estadual de Campinas; Brasil
Fil: Pereyra, Pablo Florencio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Raulin, JeanPierre. Universidade Presbiteriana Mackenzie; Brasil
Fil: Rose, Thomas. Rpg-radiometer Physics Gmbh; Alemania
Fil: Valio, Adriana Silva. Universidade Presbiteriana Mackenzie; Brasil
Fil: Walber, Achim. Rpg-radiometer Physics Gmbh; Alemania
Fil: Wallace, Patrick. Rutherford Appleton Laboratory; Reino Unido
Fil: Yakubovich, Azriel. Orbit Advanced Technologies Ltd.; Israel
Fil: Zakia, Maria Beny. Universidade Estadual de Campinas; Brasil
Materia
MID-IR SOLAR PHOTOMETERS
SOLAR FLARES
SUBMM-WAVES TELESCOPES
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/214202

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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling New telescopes for ground-based solar observations at submillimeter and mid-infraredKaufmann, PierreLevato, Orlando HugoCassiano, Marta M.Correia, EmiliaCosta, Joaquim E.R.De Castro, C. Guillermo GiménezGodoy, Rodolfo AlfredoKingsley, Robert K.Kingsley, Jeffrey S.Kudaka, Amauri S.Marcon, RogérioMartin, RobertMarun, Adolfo HectorMelo, Arline M.Pereyra, Pablo FlorencioRaulin, JeanPierreRose, ThomasValio, Adriana SilvaWalber, AchimWallace, PatrickYakubovich, AzrielZakia, Maria BenyMID-IR SOLAR PHOTOMETERSSOLAR FLARESSUBMM-WAVES TELESCOPEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The solar submillimeter-wave telescope (SST) is the only one of its kind dedicated to solar continuous observations. Two radiometers at 0.740 mm (405 GHz), and four at 1.415 mm (212 GHz) are placed in the Cassegrain focal plane of the 1.5-m dish at El Leoncito high altitude site, San Juan, Argentina. The aperture efficiencies are close to design predictions: 20% and 35% for 2 and 4 arcminutes beam sizes at 405 and 212 GHz, respectively. The positioner absolute pointing accuracy is 10 arcseconds. Spectral coverage is complemented by ground-based mid-infrared telescopes developed for high cadence observations in the continuum 10 micron band (30 THz), using small apertures and roomtemperature microbolometer cameras. Using the system, a new solar burst spectral component was discovered, exhibiting fluxes increasing for smaller wavelengths, separated from the well known microwave component. Rapid subsecond pulsations are common for all bursts. The pulsations onset times of appear to be connected to the launch times of CMEs. Active regions are brighter for shorter submillimeter-waves. Mid-IR bright regions are found closely associated with calcium plages and magnetic structures near the solar photosphere. Intense and rapid 10 micron brightening was detected on active centers in association with weak flares. These results raise challenging difficulties for interpretation.Fil: Kaufmann, Pierre. Universidade Estadual de Campinas; Brasil. Universidade Presbiteriana Mackenzie; BrasilFil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Cassiano, Marta M.. Universidade Presbiteriana Mackenzie; BrasilFil: Correia, Emilia. Universidade Presbiteriana Mackenzie; Brasil. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; BrasilFil: Costa, Joaquim E.R.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; BrasilFil: De Castro, C. Guillermo Giménez. Universidade Presbiteriana Mackenzie; BrasilFil: Godoy, Rodolfo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Kingsley, Robert K.. University of Arizona; Estados UnidosFil: Kingsley, Jeffrey S.. University of Arizona; Estados UnidosFil: Kudaka, Amauri S.. Universidade Presbiteriana Mackenzie; BrasilFil: Marcon, Rogério. “Bernard Lyot” Solar Observatory; Brasil. Universidade Estadual de Campinas; BrasilFil: Martin, Robert. Composite Mirror Applications, Inc.; Estados UnidosFil: Marun, Adolfo Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Melo, Arline M.. Universidade Presbiteriana Mackenzie; Brasil. Universidade Estadual de Campinas; BrasilFil: Pereyra, Pablo Florencio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Raulin, JeanPierre. Universidade Presbiteriana Mackenzie; BrasilFil: Rose, Thomas. Rpg-radiometer Physics Gmbh; AlemaniaFil: Valio, Adriana Silva. Universidade Presbiteriana Mackenzie; BrasilFil: Walber, Achim. Rpg-radiometer Physics Gmbh; AlemaniaFil: Wallace, Patrick. Rutherford Appleton Laboratory; Reino UnidoFil: Yakubovich, Azriel. Orbit Advanced Technologies Ltd.; IsraelFil: Zakia, Maria Beny. Universidade Estadual de Campinas; BrasilSociety of Photo-Optical Instrumentation Engineers2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/214202Kaufmann, Pierre; Levato, Orlando Hugo; Cassiano, Marta M.; Correia, Emilia; Costa, Joaquim E.R.; et al.; New telescopes for ground-based solar observations at submillimeter and mid-infrared; Society of Photo-Optical Instrumentation Engineers; Spie; 7012; 12-2008; 19-250277-786XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2008SPIE.7012E..0LK/abstractinfo:eu-repo/semantics/altIdentifier/url/https://www.spiedigitallibrary.org/conference-proceedings-of-spie/7012/1/New-telescopes-for-ground-based-solar-observations-at-submillimeter-and/10.1117/12.788889.shortinfo:eu-repo/semantics/altIdentifier/doi/10.1117/12.788889info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:55:42Zoai:ri.conicet.gov.ar:11336/214202instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:55:42.985CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv New telescopes for ground-based solar observations at submillimeter and mid-infrared
title New telescopes for ground-based solar observations at submillimeter and mid-infrared
spellingShingle New telescopes for ground-based solar observations at submillimeter and mid-infrared
Kaufmann, Pierre
MID-IR SOLAR PHOTOMETERS
SOLAR FLARES
SUBMM-WAVES TELESCOPES
title_short New telescopes for ground-based solar observations at submillimeter and mid-infrared
title_full New telescopes for ground-based solar observations at submillimeter and mid-infrared
title_fullStr New telescopes for ground-based solar observations at submillimeter and mid-infrared
title_full_unstemmed New telescopes for ground-based solar observations at submillimeter and mid-infrared
title_sort New telescopes for ground-based solar observations at submillimeter and mid-infrared
dc.creator.none.fl_str_mv Kaufmann, Pierre
Levato, Orlando Hugo
Cassiano, Marta M.
Correia, Emilia
Costa, Joaquim E.R.
De Castro, C. Guillermo Giménez
Godoy, Rodolfo Alfredo
Kingsley, Robert K.
Kingsley, Jeffrey S.
Kudaka, Amauri S.
Marcon, Rogério
Martin, Robert
Marun, Adolfo Hector
Melo, Arline M.
Pereyra, Pablo Florencio
Raulin, JeanPierre
Rose, Thomas
Valio, Adriana Silva
Walber, Achim
Wallace, Patrick
Yakubovich, Azriel
Zakia, Maria Beny
author Kaufmann, Pierre
author_facet Kaufmann, Pierre
Levato, Orlando Hugo
Cassiano, Marta M.
Correia, Emilia
Costa, Joaquim E.R.
De Castro, C. Guillermo Giménez
Godoy, Rodolfo Alfredo
Kingsley, Robert K.
Kingsley, Jeffrey S.
Kudaka, Amauri S.
Marcon, Rogério
Martin, Robert
Marun, Adolfo Hector
Melo, Arline M.
Pereyra, Pablo Florencio
Raulin, JeanPierre
Rose, Thomas
Valio, Adriana Silva
Walber, Achim
Wallace, Patrick
Yakubovich, Azriel
Zakia, Maria Beny
author_role author
author2 Levato, Orlando Hugo
Cassiano, Marta M.
Correia, Emilia
Costa, Joaquim E.R.
De Castro, C. Guillermo Giménez
Godoy, Rodolfo Alfredo
Kingsley, Robert K.
Kingsley, Jeffrey S.
Kudaka, Amauri S.
Marcon, Rogério
Martin, Robert
Marun, Adolfo Hector
Melo, Arline M.
Pereyra, Pablo Florencio
Raulin, JeanPierre
Rose, Thomas
Valio, Adriana Silva
Walber, Achim
Wallace, Patrick
Yakubovich, Azriel
Zakia, Maria Beny
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv MID-IR SOLAR PHOTOMETERS
SOLAR FLARES
SUBMM-WAVES TELESCOPES
topic MID-IR SOLAR PHOTOMETERS
SOLAR FLARES
SUBMM-WAVES TELESCOPES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The solar submillimeter-wave telescope (SST) is the only one of its kind dedicated to solar continuous observations. Two radiometers at 0.740 mm (405 GHz), and four at 1.415 mm (212 GHz) are placed in the Cassegrain focal plane of the 1.5-m dish at El Leoncito high altitude site, San Juan, Argentina. The aperture efficiencies are close to design predictions: 20% and 35% for 2 and 4 arcminutes beam sizes at 405 and 212 GHz, respectively. The positioner absolute pointing accuracy is 10 arcseconds. Spectral coverage is complemented by ground-based mid-infrared telescopes developed for high cadence observations in the continuum 10 micron band (30 THz), using small apertures and roomtemperature microbolometer cameras. Using the system, a new solar burst spectral component was discovered, exhibiting fluxes increasing for smaller wavelengths, separated from the well known microwave component. Rapid subsecond pulsations are common for all bursts. The pulsations onset times of appear to be connected to the launch times of CMEs. Active regions are brighter for shorter submillimeter-waves. Mid-IR bright regions are found closely associated with calcium plages and magnetic structures near the solar photosphere. Intense and rapid 10 micron brightening was detected on active centers in association with weak flares. These results raise challenging difficulties for interpretation.
Fil: Kaufmann, Pierre. Universidade Estadual de Campinas; Brasil. Universidade Presbiteriana Mackenzie; Brasil
Fil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Cassiano, Marta M.. Universidade Presbiteriana Mackenzie; Brasil
Fil: Correia, Emilia. Universidade Presbiteriana Mackenzie; Brasil. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Costa, Joaquim E.R.. Centro de Previsao de Tempo e Estudos Climáticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: De Castro, C. Guillermo Giménez. Universidade Presbiteriana Mackenzie; Brasil
Fil: Godoy, Rodolfo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Kingsley, Robert K.. University of Arizona; Estados Unidos
Fil: Kingsley, Jeffrey S.. University of Arizona; Estados Unidos
Fil: Kudaka, Amauri S.. Universidade Presbiteriana Mackenzie; Brasil
Fil: Marcon, Rogério. “Bernard Lyot” Solar Observatory; Brasil. Universidade Estadual de Campinas; Brasil
Fil: Martin, Robert. Composite Mirror Applications, Inc.; Estados Unidos
Fil: Marun, Adolfo Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Melo, Arline M.. Universidade Presbiteriana Mackenzie; Brasil. Universidade Estadual de Campinas; Brasil
Fil: Pereyra, Pablo Florencio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Raulin, JeanPierre. Universidade Presbiteriana Mackenzie; Brasil
Fil: Rose, Thomas. Rpg-radiometer Physics Gmbh; Alemania
Fil: Valio, Adriana Silva. Universidade Presbiteriana Mackenzie; Brasil
Fil: Walber, Achim. Rpg-radiometer Physics Gmbh; Alemania
Fil: Wallace, Patrick. Rutherford Appleton Laboratory; Reino Unido
Fil: Yakubovich, Azriel. Orbit Advanced Technologies Ltd.; Israel
Fil: Zakia, Maria Beny. Universidade Estadual de Campinas; Brasil
description The solar submillimeter-wave telescope (SST) is the only one of its kind dedicated to solar continuous observations. Two radiometers at 0.740 mm (405 GHz), and four at 1.415 mm (212 GHz) are placed in the Cassegrain focal plane of the 1.5-m dish at El Leoncito high altitude site, San Juan, Argentina. The aperture efficiencies are close to design predictions: 20% and 35% for 2 and 4 arcminutes beam sizes at 405 and 212 GHz, respectively. The positioner absolute pointing accuracy is 10 arcseconds. Spectral coverage is complemented by ground-based mid-infrared telescopes developed for high cadence observations in the continuum 10 micron band (30 THz), using small apertures and roomtemperature microbolometer cameras. Using the system, a new solar burst spectral component was discovered, exhibiting fluxes increasing for smaller wavelengths, separated from the well known microwave component. Rapid subsecond pulsations are common for all bursts. The pulsations onset times of appear to be connected to the launch times of CMEs. Active regions are brighter for shorter submillimeter-waves. Mid-IR bright regions are found closely associated with calcium plages and magnetic structures near the solar photosphere. Intense and rapid 10 micron brightening was detected on active centers in association with weak flares. These results raise challenging difficulties for interpretation.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/214202
Kaufmann, Pierre; Levato, Orlando Hugo; Cassiano, Marta M.; Correia, Emilia; Costa, Joaquim E.R.; et al.; New telescopes for ground-based solar observations at submillimeter and mid-infrared; Society of Photo-Optical Instrumentation Engineers; Spie; 7012; 12-2008; 19-25
0277-786X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/214202
identifier_str_mv Kaufmann, Pierre; Levato, Orlando Hugo; Cassiano, Marta M.; Correia, Emilia; Costa, Joaquim E.R.; et al.; New telescopes for ground-based solar observations at submillimeter and mid-infrared; Society of Photo-Optical Instrumentation Engineers; Spie; 7012; 12-2008; 19-25
0277-786X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://ui.adsabs.harvard.edu/abs/2008SPIE.7012E..0LK/abstract
info:eu-repo/semantics/altIdentifier/url/https://www.spiedigitallibrary.org/conference-proceedings-of-spie/7012/1/New-telescopes-for-ground-based-solar-observations-at-submillimeter-and/10.1117/12.788889.short
info:eu-repo/semantics/altIdentifier/doi/10.1117/12.788889
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Society of Photo-Optical Instrumentation Engineers
publisher.none.fl_str_mv Society of Photo-Optical Instrumentation Engineers
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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