Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte

Detalhes bibliográficos
Autor(a) principal: Santos, Diego Dal Pozzolo dos
Data de Publicação: 2021
Tipo de documento: Dissertação
Idioma: por
Título da fonte: Manancial - Repositório Digital da UFSM
Texto Completo: http://repositorio.ufsm.br/handle/1/23530
Resumo: The Aeolian processes are key elements to understand the surfaces of celestial bodies with atmosphere. This paper performs an analysis of aeolian activity on Herschel crater, from two dune fields in different topographical settings. At East field, between small simple craters, and at West, the dune field is located inside a large impact crater near to uplifted central peak. As source of data will be employed high resolution images (spatial resolution 0,25 m/pixel) and digital terrain models (DTM), with 1m / pixel spatial resolution, generated by HiRISE sensor of orbital probe Mars Reconnaissance Orbiter (MRO) and Mars Climate Database (MCD) meteorological database data of direction and wind speed. Were measured horizontal parameters (Area,Azimuth length, width , and length/width ratio) and vertical parameters (height of crest (Hc), height of slipface (Hs),slipface slope, curvature)of 10 dunes in each field. Altimetry, slope and slope orientation maps of both fields were aslo prepared using the ENVI and QGIS softwares.The results indicates Herschel East dunes are fat,free, and in uphill. The taller and steepest dunes are located at side of impact craters, due to horseshoe vortex effect It is characterized by the unimodal wind regime in the predominant N-S axis, wind patterns of the Tsoar type at night and Bagnold during the day. It has little azimuth variation. Predominance of the slope between 5-10º. There is a predominance of NW, E, W (Windward) SE, (slip) orientations. Similar conditions have been identified in similar terrestrial environments such as, White Sands, (New Mexico), Wolfe Creek, (Australia) and Lagoa da Conceição (Santa Catarina).The dunes from Herschel West are slim, in downhill, some anchored by Yardangs. It presents acute bimodal wind patterns on the predominant axis W-E, Bagnold type wind pattern at night and Tsoar during the day. Predominance of orientations E, SE, NE (windward), W, NW (landslide). A lot of azimuth variation. Predominance of the 5-10º slope. As a terrestrial analogue, we have the Liwa Oasis (United Arab Emirates / Saudi Arabia).
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spelling Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, MarteGeomorphology and the planetary studies: thue use of hirise images and aeolian processes on Herschel crater, MarsGeomorfologia planetáriaMarteDunasVentoCraterasPlanetary geomorphologyMarsDunesWindCratersCNPQ::CIENCIAS HUMANAS::GEOGRAFIAThe Aeolian processes are key elements to understand the surfaces of celestial bodies with atmosphere. This paper performs an analysis of aeolian activity on Herschel crater, from two dune fields in different topographical settings. At East field, between small simple craters, and at West, the dune field is located inside a large impact crater near to uplifted central peak. As source of data will be employed high resolution images (spatial resolution 0,25 m/pixel) and digital terrain models (DTM), with 1m / pixel spatial resolution, generated by HiRISE sensor of orbital probe Mars Reconnaissance Orbiter (MRO) and Mars Climate Database (MCD) meteorological database data of direction and wind speed. Were measured horizontal parameters (Area,Azimuth length, width , and length/width ratio) and vertical parameters (height of crest (Hc), height of slipface (Hs),slipface slope, curvature)of 10 dunes in each field. Altimetry, slope and slope orientation maps of both fields were aslo prepared using the ENVI and QGIS softwares.The results indicates Herschel East dunes are fat,free, and in uphill. The taller and steepest dunes are located at side of impact craters, due to horseshoe vortex effect It is characterized by the unimodal wind regime in the predominant N-S axis, wind patterns of the Tsoar type at night and Bagnold during the day. It has little azimuth variation. Predominance of the slope between 5-10º. There is a predominance of NW, E, W (Windward) SE, (slip) orientations. Similar conditions have been identified in similar terrestrial environments such as, White Sands, (New Mexico), Wolfe Creek, (Australia) and Lagoa da Conceição (Santa Catarina).The dunes from Herschel West are slim, in downhill, some anchored by Yardangs. It presents acute bimodal wind patterns on the predominant axis W-E, Bagnold type wind pattern at night and Tsoar during the day. Predominance of orientations E, SE, NE (windward), W, NW (landslide). A lot of azimuth variation. Predominance of the 5-10º slope. As a terrestrial analogue, we have the Liwa Oasis (United Arab Emirates / Saudi Arabia).Os processos eólicos são elementos chave para entender as superfícies de corpos celestes com atmosfera. Este trabalho realizou uma análise da atividade eólica na cratera Herschel, a partir de dois campos de dunas com diferentes condições topográficas. No campo Leste entre pequenas crateras simples, e no Oeste, o campo de dunas localizado dentro de uma grande cratera de impacto, próximo ao pico central soerguido. Como fontes de dados foram empregadas imagens (resolução espacial de 0,25m) e modelos digitais de terreno (DTM) com resolução espacial de 1m/pixel, gerados pelo sensor HIRISE da sonda orbital Mars Reconnaissance Orbiter (MRO), além de dados de direção e velocidade do vento da base de dados meteorológica Mars Climate Database (MCD). Foram medidos parâmetros horizontais (área, azimute, comprimento, largura e a relação comprimento/largura), e parâmetros verticais (altura da crista (Hc), altura da face de escorregamento (Hs), declividade da face de escorregamento, curvatura) de 10 dunas em cada campo. Também foram elaborados mapas altimetria, declividade e orientação de vertentes de ambos os campos por meio dos Softwares ENVI e QGIS. Os resultados indicam que as dunas em Herschel Leste são gordas, livres e em aclive. As dunas mais altas e íngremes estão localizadas ao lado das crateras de impacto pelo efeito dos vórtices de ferradura que se caracteriza pelo regime de ventos unimodal no Eixo predominante N-S, por padrões de vento do tipo Tsoar durante a noite e Bagnold durante o dia. Ademais, possuem pouca variação de azimute; predomínio da declividade entre 5-10º e predomínio das orientações NW, E, W (Barlavento) SE, (escorregamento). Condições similares foram identificadas em ambientes análogos terrestres, como White Sands, (Novo México), Wolfe Creek, (Austrália) e Lagoa da Conceição (Santa Catarina). As dunas de Herschel Oeste são delgadas, em declive, algumas ancoradas por Yardangs. Possuem padrões de ventos bimodal agudo no Eixo predominante W-E, do Tipo Bagnold durante a noite e Tsoar durante o dia. Nessas dunas, há o predomínio das orientações E, SE, NE (barlavento), W, NW (escorregamento) e muita variação de azimute. Por fim, apresentam predomínio da declividade 5-10º. Como análogo terrestre, temos o Oasis de Liwa (Emirados Árabes Unidos /Arábia Saudita).Universidade Federal de Santa MariaBrasilGeografiaUFSMPrograma de Pós-Graduação em GeografiaCentro de Ciências Naturais e ExatasSouza, Bernardo Sayão Penna ehttp://lattes.cnpq.br/4162826845630069Pereira Filho, WaterlooRehbein, Moisés OrtemarSantos, Diego Dal Pozzolo dos2022-01-13T19:10:52Z2022-01-13T19:10:52Z2021-05-07info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/masterThesisapplication/pdfhttp://repositorio.ufsm.br/handle/1/23530porAttribution-NonCommercial-NoDerivatives 4.0 Internationalhttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessreponame:Manancial - Repositório Digital da UFSMinstname:Universidade Federal de Santa Maria (UFSM)instacron:UFSM2022-01-13T19:12:31Zoai:repositorio.ufsm.br:1/23530Biblioteca Digital de Teses e Dissertaçõeshttps://repositorio.ufsm.br/ONGhttps://repositorio.ufsm.br/oai/requestatendimento.sib@ufsm.br||tedebc@gmail.comopendoar:2022-01-13T19:12:31Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)false
dc.title.none.fl_str_mv Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
Geomorphology and the planetary studies: thue use of hirise images and aeolian processes on Herschel crater, Mars
title Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
spellingShingle Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
Santos, Diego Dal Pozzolo dos
Geomorfologia planetária
Marte
Dunas
Vento
Crateras
Planetary geomorphology
Mars
Dunes
Wind
Craters
CNPQ::CIENCIAS HUMANAS::GEOGRAFIA
title_short Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
title_full Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
title_fullStr Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
title_full_unstemmed Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
title_sort Geomorfologia e os estudos planetários: o uso das imagens hirise e os processos eólicos na cratera Herschel, Marte
author Santos, Diego Dal Pozzolo dos
author_facet Santos, Diego Dal Pozzolo dos
author_role author
dc.contributor.none.fl_str_mv Souza, Bernardo Sayão Penna e
http://lattes.cnpq.br/4162826845630069
Pereira Filho, Waterloo
Rehbein, Moisés Ortemar
dc.contributor.author.fl_str_mv Santos, Diego Dal Pozzolo dos
dc.subject.por.fl_str_mv Geomorfologia planetária
Marte
Dunas
Vento
Crateras
Planetary geomorphology
Mars
Dunes
Wind
Craters
CNPQ::CIENCIAS HUMANAS::GEOGRAFIA
topic Geomorfologia planetária
Marte
Dunas
Vento
Crateras
Planetary geomorphology
Mars
Dunes
Wind
Craters
CNPQ::CIENCIAS HUMANAS::GEOGRAFIA
description The Aeolian processes are key elements to understand the surfaces of celestial bodies with atmosphere. This paper performs an analysis of aeolian activity on Herschel crater, from two dune fields in different topographical settings. At East field, between small simple craters, and at West, the dune field is located inside a large impact crater near to uplifted central peak. As source of data will be employed high resolution images (spatial resolution 0,25 m/pixel) and digital terrain models (DTM), with 1m / pixel spatial resolution, generated by HiRISE sensor of orbital probe Mars Reconnaissance Orbiter (MRO) and Mars Climate Database (MCD) meteorological database data of direction and wind speed. Were measured horizontal parameters (Area,Azimuth length, width , and length/width ratio) and vertical parameters (height of crest (Hc), height of slipface (Hs),slipface slope, curvature)of 10 dunes in each field. Altimetry, slope and slope orientation maps of both fields were aslo prepared using the ENVI and QGIS softwares.The results indicates Herschel East dunes are fat,free, and in uphill. The taller and steepest dunes are located at side of impact craters, due to horseshoe vortex effect It is characterized by the unimodal wind regime in the predominant N-S axis, wind patterns of the Tsoar type at night and Bagnold during the day. It has little azimuth variation. Predominance of the slope between 5-10º. There is a predominance of NW, E, W (Windward) SE, (slip) orientations. Similar conditions have been identified in similar terrestrial environments such as, White Sands, (New Mexico), Wolfe Creek, (Australia) and Lagoa da Conceição (Santa Catarina).The dunes from Herschel West are slim, in downhill, some anchored by Yardangs. It presents acute bimodal wind patterns on the predominant axis W-E, Bagnold type wind pattern at night and Tsoar during the day. Predominance of orientations E, SE, NE (windward), W, NW (landslide). A lot of azimuth variation. Predominance of the 5-10º slope. As a terrestrial analogue, we have the Liwa Oasis (United Arab Emirates / Saudi Arabia).
publishDate 2021
dc.date.none.fl_str_mv 2021-05-07
2022-01-13T19:10:52Z
2022-01-13T19:10:52Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/masterThesis
format masterThesis
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://repositorio.ufsm.br/handle/1/23530
url http://repositorio.ufsm.br/handle/1/23530
dc.language.iso.fl_str_mv por
language por
dc.rights.driver.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
http://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Universidade Federal de Santa Maria
Brasil
Geografia
UFSM
Programa de Pós-Graduação em Geografia
Centro de Ciências Naturais e Exatas
publisher.none.fl_str_mv Universidade Federal de Santa Maria
Brasil
Geografia
UFSM
Programa de Pós-Graduação em Geografia
Centro de Ciências Naturais e Exatas
dc.source.none.fl_str_mv reponame:Manancial - Repositório Digital da UFSM
instname:Universidade Federal de Santa Maria (UFSM)
instacron:UFSM
instname_str Universidade Federal de Santa Maria (UFSM)
instacron_str UFSM
institution UFSM
reponame_str Manancial - Repositório Digital da UFSM
collection Manancial - Repositório Digital da UFSM
repository.name.fl_str_mv Manancial - Repositório Digital da UFSM - Universidade Federal de Santa Maria (UFSM)
repository.mail.fl_str_mv atendimento.sib@ufsm.br||tedebc@gmail.com
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