Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area

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We describe the results of the study of aerosol optical depth (AOD) and Direct Radiative Forcing (DRF) in Top Of Atmosphere (TOA), obtained from the measurement and monitoring campaign carried out during the XXI Antarctic Peruvian Expedition in the months of January and February 2013 and in the Metr...

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Detalles Bibliográficos
Autores: Angeles Suzao, Julio Miguel, Suarez Salas, Luis, Huaman De La Cruz, Alex Rubén, Angeles Vasquez, Roberto, Rosales Aylas, Georgynio, Rocha Condor, Alicia, Requena Rojas, Edilson, Muñoz Ccuro, Felipa, Flores Rojas, Jose Luis, Abi Karam, Hugo
Formato: artículo
Fecha de Publicación:2020
Institución:Universidad Tecnológica del Perú
Repositorio:UTP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.utp.edu.pe:20.500.12867/3461
Enlace del recurso:https://hdl.handle.net/20.500.12867/3461
http://dx.doi.org/10.11137/2020_4_404_412
Nivel de acceso:acceso abierto
Materia:Aerosol
Radiative forcing
Antarctic
https://purl.org/pe-repo/ocde/ford#1.05.09
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dc.title.es_PE.fl_str_mv Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
dc.title.alternative.es_PE.fl_str_mv Forçamento radiativo direto devido a propriedades de aerossóis na estação antártica peruana e na área metropolitana de Huancayo
title Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
spellingShingle Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
Angeles Suzao, Julio Miguel
Aerosol
Radiative forcing
Antarctic
https://purl.org/pe-repo/ocde/ford#1.05.09
title_short Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
title_full Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
title_fullStr Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
title_full_unstemmed Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
title_sort Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo area
author Angeles Suzao, Julio Miguel
author_facet Angeles Suzao, Julio Miguel
Suarez Salas, Luis
Huaman De La Cruz, Alex Rubén
Angeles Vasquez, Roberto
Rosales Aylas, Georgynio
Rocha Condor, Alicia
Requena Rojas, Edilson
Muñoz Ccuro, Felipa
Flores Rojas, Jose Luis
Abi Karam, Hugo
author_role author
author2 Suarez Salas, Luis
Huaman De La Cruz, Alex Rubén
Angeles Vasquez, Roberto
Rosales Aylas, Georgynio
Rocha Condor, Alicia
Requena Rojas, Edilson
Muñoz Ccuro, Felipa
Flores Rojas, Jose Luis
Abi Karam, Hugo
author2_role author
author
author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Angeles Suzao, Julio Miguel
Suarez Salas, Luis
Huaman De La Cruz, Alex Rubén
Angeles Vasquez, Roberto
Rosales Aylas, Georgynio
Rocha Condor, Alicia
Requena Rojas, Edilson
Muñoz Ccuro, Felipa
Flores Rojas, Jose Luis
Abi Karam, Hugo
dc.subject.es_PE.fl_str_mv Aerosol
Radiative forcing
Antarctic
topic Aerosol
Radiative forcing
Antarctic
https://purl.org/pe-repo/ocde/ford#1.05.09
dc.subject.ocde.es_PE.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.05.09
description We describe the results of the study of aerosol optical depth (AOD) and Direct Radiative Forcing (DRF) in Top Of Atmosphere (TOA), obtained from the measurement and monitoring campaign carried out during the XXI Antarctic Peruvian Expedition in the months of January and February 2013 and in the Metropolitan Huancayo Area in the months of June and July 2019. In the Scientific Peruvian Station at Antarctic “Machu Picchu” our used a SP02-L sun photometer, which is within the instrumental framework of the International Polar Year. This instrument has 4 channels: 412 nm, 500 nm, 675 nm and 862 nm, thus allowing direct radiation spectra measurements. And in the MHA we used the BF5 sensor. This instrument measured Direct, Diffuse and Global Radiation in low wavelength. The results calculated of AOD in polar latitudes varied between 0.0646 to 0.1061, in relation to AOD in MHA, presents the value maximum that is 0.58 (11 of June) and minimum that is 0.19 (12 June). The Angstrom coefficient was determined have values ranging from 0 to 0.07, these values also indicates the presence of big particles. Also to the MHA presents the mean value varied from 0 to 1.8, that indicated the presence the aerosols types biomass burning and industrial. Recorded optical properties used to estimate the direct aerosol radiative forcing (DARF) at the top of the atmosphere. The results indicates that on King George Island site the DARF is between [-2 4] W/m2; also, the direct aerosol radiative forcing in MHA is between [0 20] W/m2.
publishDate 2020
dc.date.accessioned.none.fl_str_mv 2020-12-30T16:29:04Z
dc.date.available.none.fl_str_mv 2020-12-30T16:29:04Z
dc.date.issued.fl_str_mv 2020
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dc.identifier.journal.es_PE.fl_str_mv Anuario do Instituto de Geociencias
dc.identifier.doi.none.fl_str_mv http://dx.doi.org/10.11137/2020_4_404_412
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http://dx.doi.org/10.11137/2020_4_404_412
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dc.publisher.es_PE.fl_str_mv Universidade Federal do Rio de Janeiro
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spelling Angeles Suzao, Julio MiguelSuarez Salas, LuisHuaman De La Cruz, Alex RubénAngeles Vasquez, RobertoRosales Aylas, GeorgynioRocha Condor, AliciaRequena Rojas, EdilsonMuñoz Ccuro, FelipaFlores Rojas, Jose LuisAbi Karam, Hugo2020-12-30T16:29:04Z2020-12-30T16:29:04Z20200101-9759https://hdl.handle.net/20.500.12867/3461Anuario do Instituto de Geocienciashttp://dx.doi.org/10.11137/2020_4_404_412We describe the results of the study of aerosol optical depth (AOD) and Direct Radiative Forcing (DRF) in Top Of Atmosphere (TOA), obtained from the measurement and monitoring campaign carried out during the XXI Antarctic Peruvian Expedition in the months of January and February 2013 and in the Metropolitan Huancayo Area in the months of June and July 2019. In the Scientific Peruvian Station at Antarctic “Machu Picchu” our used a SP02-L sun photometer, which is within the instrumental framework of the International Polar Year. This instrument has 4 channels: 412 nm, 500 nm, 675 nm and 862 nm, thus allowing direct radiation spectra measurements. And in the MHA we used the BF5 sensor. This instrument measured Direct, Diffuse and Global Radiation in low wavelength. The results calculated of AOD in polar latitudes varied between 0.0646 to 0.1061, in relation to AOD in MHA, presents the value maximum that is 0.58 (11 of June) and minimum that is 0.19 (12 June). The Angstrom coefficient was determined have values ranging from 0 to 0.07, these values also indicates the presence of big particles. Also to the MHA presents the mean value varied from 0 to 1.8, that indicated the presence the aerosols types biomass burning and industrial. Recorded optical properties used to estimate the direct aerosol radiative forcing (DARF) at the top of the atmosphere. The results indicates that on King George Island site the DARF is between [-2 4] W/m2; also, the direct aerosol radiative forcing in MHA is between [0 20] W/m2.Descrevemos os resultados do estudo da profundidade ótica do aerossol (POA) e do Forçamento Radiativo Direto (FRD) no topo da atmosfera (TOA), obtidos durante a campanha de medição e monitoramento, XXI Expedição Antártica do Peru, entre os meses de janeiro e fevereiro de 2013, e na área metropolitana de Huancayo (AMH) entre os meses de junho e julho de 2019. Na Estação Antártica Peruana Machu Picchu utilizou-se um fotômetro solar SP02-L. Tal instrumento possui 4 canais: 412 nm, 500 nm, 675 nm e 862 nm, permitindo realizar medições diretas do espectro de radiação visível. Na AMH usamos o sensor BF5, que mede a radiação direta, difusa e global em comprimento de onda curta. Os cálculos de AOD em latitudes polares variaram entre 0,0646 e 0,1061. Na AMH apresenta valor máximo de 0,58 (11 de junho) e mínimo de 0,19 (12 de junho). Determinou-se o coeficiente de Angstrom variando de 0 a 0,07, esses valores indicam a presença de partículas grandes. Na AMH varia de 0 a 1,8, que indica a presença de aerossóis de fonte de queima de biomassa e industrial. As propriedades óticas observadas foram usadas para estimar a forçante radiativa direta por aerossóis (FRDA) no topo da atmosfera. Os resultados indicam que no King George Island, o FRDA, está entre -2 e 4 W/m2; já para a AMH a forçante radiativa direta de aerossol está entre 0 e 20 W/m2.Revisión por paresRevisión por paresCampus Huancayoapplication/pdfengUniversidade Federal do Rio de Janeirourn:isnn:0101-9759info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/4.0/Repositorio Institucional - UTPUniversidad Tecnológica del Perúreponame:UTP-Institucionalinstname:Universidad Tecnológica del Perúinstacron:UTPAerosolRadiative forcingAntarctichttps://purl.org/pe-repo/ocde/ford#1.05.09Direct radiative forcing due to aerosol properties at the Peruvian antarctic station and metropolitan Huancayo areaForçamento radiativo direto devido a propriedades de aerossóis na estação antártica peruana e na área metropolitana de Huancayoinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionTHUMBNAILJulio Miguel Angeles Suazo_Luis Suarez_Alex Huaman_et. al._Articulo_Anuario do Instituto de Geociencias_spa_2020.pdf.jpgJulio Miguel Angeles Suazo_Luis Suarez_Alex Huaman_et. al._Articulo_Anuario do Instituto de Geociencias_spa_2020.pdf.jpgGenerated Thumbnailimage/jpeg37494https://repositorio.utp.edu.pe/backend/api/core/bitstreams/22045b78-0e67-43d5-aa96-33e45dca11f3/download84fcbd1f33f14b4cb42e7fafd44e6f8bMD58ORIGINALJulio Miguel Angeles Suazo_Luis Suarez_Alex Huaman_et. al._Articulo_Anuario do Instituto de Geociencias_spa_2020.pdfJulio Miguel Angeles Suazo_Luis Suarez_Alex Huaman_et. al._Articulo_Anuario do Instituto de Geociencias_spa_2020.pdfapplication/pdf741268https://repositorio.utp.edu.pe/backend/api/core/bitstreams/fe06cc15-420c-4430-bfeb-ef860abfc4eb/downloadf3079342a2728ee10477585379686551MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.utp.edu.pe/backend/api/core/bitstreams/e24fa10c-ab00-4279-bf82-14efcdc68822/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTJulio Miguel Angeles Suazo_Luis Suarez_Alex Huaman_et. al._Articulo_Anuario do Instituto de Geociencias_spa_2020.pdf.txtJulio Miguel Angeles Suazo_Luis Suarez_Alex Huaman_et. al._Articulo_Anuario do Instituto de Geociencias_spa_2020.pdf.txtExtracted texttext/plain34878https://repositorio.utp.edu.pe/backend/api/core/bitstreams/ca8733e3-1d71-40bf-894f-2642e7886ae2/download8b633c8a8eaf2324c0e79aebccf13366MD5720.500.12867/3461oai:repositorio.utp.edu.pe:20.500.12867/34612025-11-30 17:43:15.013https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.utp.edu.peRepositorio de la Universidad Tecnológica del Perúrepositorio@utp.edu.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