983 resultados para Equatorial Aeronomy


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A further progress has been made in defining the ionosonde deduced equator (IDE) which characterises a latitudinal transition from the northern to southern hemisphere. It is now possible to define the global IDE location as the locus of the average position between geographic and geomagnetic equators. A more complete insight to the phenomenon of the third equator (i.e. after geographic and geomagnetic equators) was made possible due to availability of ionospheric height (h'F) data from three stations positioned close to the IDE in the American and the far-east sectors. The IDE ionospheric signature (or E-type signature), detected at these stations, consists of bi-annual h'F height increases. This signature however is not consistently observed during solar cycle and at times, particularly at sunspot minimum, a weak hemispheric signature is observed (i.e. the northern or southern hemisphere signature). In general, the height increase at the IDE are considerably smaller (by a factor of 4) than at other equatorial locations, indicating that the ionosphere at the IDE location becomes less disturbed. It is suggested that the equatorial longitudinal regions which can be associated with more consistent E-type signature are located in the central Pacific and at the east coast of America, close to the intersection points of the geographic and geomagnetic equators. (C) 2003 Elsevier Ltd. All rights reserved.

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The General Ocean Turbulence Model (GOTM) is applied to the diagnostic turbulence field of the mixing layer (ML) over the equatorial region of the Atlantic Ocean. Two situations were investigated: rainy and dry seasons, defined, respectively, by the presence of the intertropical convergence zone and by its northward displacement. Simulations were carried out using data from a PIRATA buoy located on the equator at 23º W to compute surface turbulent fluxes and from the NASA/GEWEX Surface Radiation Budget Project to close the surface radiation balance. A data assimilation scheme was used as a surrogate for the physical effects not present in the one-dimensional model. In the rainy season, results show that the ML is shallower due to the weaker surface stress and stronger stable stratification; the maximum ML depth reached during this season is around 15 m, with an averaged diurnal variation of 7 m depth. In the dry season, the stronger surface stress and the enhanced surface heat balance components enable higher mechanical production of turbulent kinetic energy and, at night, the buoyancy acts also enhancing turbulence in the first meters of depth, characterizing a deeper ML, reaching around 60 m and presenting an average diurnal variation of 30 m.

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The virtual (or minimum) height of the F-region (h'F), recorded over a number of solar cycles for I I equatorial and mid-latitude ionosonde stations, was used to deduce the hemispheric (i.e. southern or northern hemisphere) character of equatorial stations. The semi-annual median monthly height (h'F) variations consist of two components: major local summer maximum and winter sub-maximum (about 5 percent of the summer maximum). This hemispheric pattern was most consistently observed for equatorial stations (within 5degrees of the geomagnetic equator) in a period centred on the local midnight (21-03 LT) but was also present, to a lesser extent, at mid-latitude stations and at other time intervals. It is evident that the physical parameter h'F defines the hemispheric character of an equatorial station which has different (sometimes opposite) geographic and geomagnetic latitudes. There is a sharp transition in the latitudinal character of the stations on both sides of the equator leading to hypothesis that the equal maxima in h'F in December and June solstices are observed at a near-equator position labelled as ionosonde deduced equator (IDE). Such a signature was observed for an American equatorial (both geographic and geomagnetic) station Talara (Peru) which is an experimental support of the hypothesis. The IDE can be another useful parameter characterising the equatorial ionosphere. This finding reveals a new application of the standard ionosonde data in defining the geophysical character of equatorial stations, being an important contribution to space climatology. (C) 2002 Elsevier Science Ltd. All rights reserved.

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Analisam a estrutura da floresta equatorial úmida próxima a Manaus, introduzindo a qualidade de fuste na. análise. Utilizam 8 amostras de 20m x 500m para indivíduos com DAP > 20cm, 24 subamostras de 10m x 100m para. indivíduos com DAP entre 5cm e 20cm e 120 subamostras de 2m x 10m para indivíduos com DAP < 5cm. Determinam valores mínimos de 2,6 e 22 amostras para composição florística é de 6,18 e 80 para a abundância em cada fração da floresta. Concluem que a floresta é muito heterogênea, com 324 espécies, 173 gêneros e 57 fiamílias e com grande diferença entre a regeneração e o povoamento adulto. Eschweilera odora, Corythophora alta., Protium apiculatum e Radlkoferella sp. são as espécies mais importantes. A floresta em geral apresenta a estrutura diamétrica regular esperada para florestas nativas devido às espécies do estrato inferior e sub-bosque.

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Analisa as variações florísticas em uma floresta equatorial de terra-firme, próximo de Manaus, através do índice de Expansão Florística (IEF), obtido através da taxa de regeneração natural, ponderada pela abundância relativa das espécies, concluindo que existe um grupo de cinqüenta e quatro espécies que ampliaram sua representatividade na composição florística, ocupando os espaços deixados por outro grupo de cinqüenta e uma espécies que reduziram sua representatividade florística. Sendo esses dois grupos responsáveis pelas variações florísticas na área, estudada. Um outro grupo de cento e vinte e três espécies, representando cerca de 30% dos indivíduos e mais 50% das espécies, é responsável pela manutenção da fisionomia estrutural da floresta.

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RESUMOAnalisa a distribuição espacial das espécies arbóreas com DAP maior ou igual a 20 cm em uma floresta equatorial de terra-firme, propondo um novo índice de dispersão ID = FrAB%, onde ID é o índice de dispersão, Fr é a frequência absoluta e AB% é a abundância relativa das espécies, concluindo que existem 39 espécies com distribuição aleatória e 108 espécies com distribuição regular, o que contraria alguns autores que afirmam ser muito rara a ocorrência desse último tipo de distribuição em florestas naturais.

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Analisa a relação entre a abundância e a frequência absoluta através de análise de regressão a partir dos resultados de Jardim Hosohawa (1986/87), concluindo que existe uma proporcionalidade direta entre as duas variáveis, expressa pela equação Y = 3,14785 X 1,12292 onde Y é a abundância relativa e X é a frequência absoluta, de cada espécie.

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Os impactos de eventos anômalos no oceano Pacífico associados ao El Niño-Oscilação Sul (ENOS) na precipitação da região norte e nordeste da América do Sul foram avaliados para o período de 1900 a 2007, fazendo-se uso de análise de composições. Os eventos El Niño (La Niña) no Pacífico que juntamente com um Modo Equatorial no Atlântico (MEA) frio (quente) formam um gradiente interbacias entre o Pacífico e Atlântico foram analisados considerando, separadamente, aqueles para os quais o gradiente se forma na fase inicial do ENOS daqueles em que o gradiente se forma na fase de decaimento do ENOS. Os resultados mostram que o padrão de precipitação na região norte e nordeste da América do Sul é reforçado mediante a configuração do gradiente interbacias durante a fase inicial do ENOS. Nesse caso, uma possível explicação é que o MEA de sinal contrário ao ENOS durante sua fase inicial cria condições favoráveis para o desenvolvimento de um gradiente inter-hemisférico no Atlântico Tropical atuando no mesmo sentido do gradiente interbacias, e colaborando para fortalecer o efeito do El Niño (La Niña) na precipitação. Por outro lado, para os eventos ENOS em que o gradiente se forma em sua fase de decaimento, o impacto na precipitação é mais significativo na região norte e centro-oeste da bacia. Uma possível explicação para essas diferenças está associada às mudanças que ocorrem na circulação atmosférica leste-oeste associada ao gradiente leste-oeste de anomalias da TSM. Os resultados deste estudo podem ser úteis, principalmente, para fins de monitoramento climático.

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OBJECTIVE: Studies conducted mainly in countries located in the Northern Hemisphere have shown that season of birth influences mood seasonality. Greater mood seasonality has been observed for individuals born during spring/summer months than those born during autumn/winter months. Expanding past research to the Southern Hemisphere, in this study we examine the influence of season of birth on mood seasonality in a sample of 1,247 healthy young Brazilians. METHOD: The Seasonal Pattern Assessment Questionnaire was used to compute a global seasonality score as a measure of mood seasonality in a cross-sectional study. RESULTS: Analysis of covariance was conducted to examine the effects of month of birth and gender on mood seasonality, with age entered as a covariate. A main effect of gender was observed, F (1, 1197) = 17.86, p < .01; partial Eta-squared = .02, with mood seasonality being higher for females (M = 8) than for males (M = 7). Contradicting previous findings, no significant main effect for month of birth was observed, F (1, 1197) = 0.65, p > .05. CONCLUSION: The unexpected finding is tentatively explained by differences in geographic location and weather fluctuations between the sampling location in Brazil and other countries where season of birth has been found to influence mood seasonality. Additional studies with larger samples from the Southern Hemisphere are necessary to shed additional light on the possible significant influence of season of birth on mood.

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The present study is a further contribution to the systematic knowledge of the shallow water marine ostracodes from the Brazilian oceanic islands. A total of 14 species belonging to 10 genera and eight families is herein identified. One new genus and species are described and illustrated: Berguecythere insularis gen. nov., sp. nov. In addition to this new taxon, the abundant species Loxocorniculum tricornatum Krutak, 1971, widely distributed in recent sediments in the Gulf of Mexico, Caribbean, north and northeast of Brazil and the Rocas Atoll, along with the cosmopolitan tropical ostracode Triebelina sertata Triebel, 1948, were also identified at specific level. The remaining 11 species were left at the genus level, and should provide new species. Ecological, zoo- and paleozoogeographical aspects were also briefly discussed.

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Two new species of Xestoleberididae: Xestoleberis brasilinsularis sp. nov. and Xestoleberis machadoae sp. nov., both endemic to Archipelago of São Pedro and São Paulo, are described. The record of these shallow marine waters species from Brazilian oceanic islands represents an important contribution to the knowledge of the evolutionary history the species inhabit areas.