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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/214202
Ver los metadatos del registro completo
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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 Técnicas2025-10-22T11:24:51Zoai: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:34982025-10-22 11:24:51.353CONICET 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 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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Society of Photo-Optical Instrumentation Engineers |
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Society of Photo-Optical Instrumentation Engineers |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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