Modelling study of the impact of deep convection on the utls air composition - Part I: Analysis of ozone precursors

The aim of this work is to study the local impact on the upper troposphere/lower stratosphere air composition of an extreme deep convective system. For this purpose, we performed a simulation of a convective cluster composed of many individual deep convective cells that occurred near Bauru (Brazil). The simulation is performed using the 3-D mesoscale model RAMS coupled on-line with a chemistry model. The comparisons with meteorological measurements show that the model produces meteorological fields generally consistent with the observations. The present paper (part I) is devoted to the analysis of the ozone precursors (CO, NO x and non-methane volatile organic compounds) and HO x in the UTLS. The simulation results show that the distribution of CO with altitude is closely related to the upward convective motions and consecutive outflow at the top of the convective cells leading to a bulge of CO between 7 km altitude and the tropopause (around 17km altitude). The model results for CO are consistent with satellite-borne measurements at 700 hPa. The simulation also indicates enhanced amounts of NO x up to 2 ppbv in the 7-17 km altitude layer mainly produced by the lightning associated with the intense convective activity. For insoluble non-methane volatile organic compounds, the convective activity tends to significantly increase their amount in the 7-17km layer by dynamical effects. During daytime in the presence of lightning NO x, this bulge is largely reduced in the upper part of the layer for reactive species (e.g. isoprene, ethene) because of their reactions with OH that is increased on average during daytime. Lightning NO x also impacts on the oxydizing capacity of the upper troposphere by reducing on average HO x, HO 2, H 2O 2 and organic hydroperoxides. During the simulation time, the impact of convection on the air composition of the lower stratosphere is negligible for all ozone precursors although several of the simulated convective cells nearly reach the tropopause. There is no significant transport from the upper troposphere to the lower stratosphere, the isentropic barrier not being crossed by convection. The impact of the increase of ozone precursors and HO x in the upper troposphere on the ozone budget in the LS is discussed in part II of this series of papers.

Aspectos observacionais e numéricos da interação floresta-atmosfera na Amazônia oriental: fenômenos turbulentos noturnos

Este estudo identificou dois fenômenos turbulentos noturnos sobre a região de Caxiuanã, na Amazônia Oriental, durante a estação seca: jatos de baixos níveis (JBNs) e rajadas de ventos, utilizando dados das campanhas de coleta de dados CiMeLA (estação seca de 2003) e COBRA-PARÁ (estação seca de 2006). Ambos foram analisados observacionalmente, no que diz respeito aos seus horários de ocorrência, intensidade, altura e duração, bem como a evolução noturna destas ocorrências. Verificou-se que a maioria dos eventos de JBNs observados foi acompanhada de queda na temperatura potencial equivalente e que as rajadas de vento exerceram uma importante influência sobre as trocas floresta-atmosfera. A gênese dos dois fenômenos também foi investigada. Notou-se, através do modelo de mesoescala BRAMS, que a origem dos jatos está possivelmente associada à brisa marítima e à intensificação dos ventos alísios de nordeste, baseado em resultados de testes de sensibilidade, que incluíram a retirada dos rios, da interface oceano-atmosfera, dos efeitos de downdrafts e do desflorestamento da região. Observou-se também que o processo de formação das rajadas está associado à existência da baía de Caxiuanã, cuja forma se assemelha a um lago, e à atividade convectiva local. Verificou-se que os dois fenômenos não existiram simultaneamente, exceto em uma única noite, o que pode ser explicado por efeitos de blindagem por cisalhamento, que impedem a propagação de turbulência para baixo, em direção à superfície, gerados pela presença de JBNs muito fortes. Esta pesquisa reflete a importância e complexidade dos fenômenos atmosféricos próximos à costa paraense.

Lightning and precipitation produced by severe weather systems over Belém, Brazil

Eventos de raios nuvem-solo registrados pela rede de detecção do SIPAM, integrada por 12 sensores VAISALA LPATS IV, distribuídos no leste da Amazônia, foram analisados durante 4 tempestades com ocorrência de precipitação intensa em Belém-PA-Brasil, em 2006-2007. Esses casos selecionados, correspondem a eventos de chuva com mais de 25 mm/hora ou 40 mm/ 2 horas, de precipitação registrada por um pluviômetro instalado em 1º 47' 53" and 48º 30' 16" O. Com centro nessa localização, um círculos de 30, 10 e 5 km de raio foram traçados através de um sistema de informação geográfica e os dados de eventos de raios nessas áreas foram separados para analise. Durante essas tempestades, os eventos de raios ocorreram de maneira quase aleatória, sobre a área maior que já havia sido previamente coberta por sistemas convectivos de mesoescala, em todos os casos. Esse trabalho também mostrou a grande influencia dos sistemas de larga escala nas condições de tempo que levaram às tempestades severas estudadas. Adicionalmente, foi observado que, quando existe interação entre sistemas de larga e meso escalas, tanto a precipitação como o numero de relâmpagos aumentaram significativamente e a atividade elétrica nos círculos maiores pode anteceder a chuva no ponto central.

Complexo Convectivo de Mesoescala observado em 27/11/2002 no nordeste da Argentina

Neste trabalho foram analisadas as condições sinóticas associadas à atuação de um Complexo Convectivo de Mesoescala (CCM), ocorrido no dia 27/11/02, no nordeste da Argentina. Para tal foram utilizadas imagens no canal infravermelho do satélite meteorológico GOES-8 e campos simulados pelo modelo regional BRAMS. A simulação feita com o modelo, com saídas de três em três horas, permitiu detalhar o comportamento das variáveis meteorológicas em grande escala que afetam o ciclo de vida do CCM, reproduzindo as condições favoráveis para sua iniciação, manutenção e dissipação. Os resultados mostraram que o CCM estudado apresentou características similares às observadas por diversos autores.

Características e distribuição das descargas atmosféricas e dos sistemas precipitantes produtores de raios na Amazônia Oriental

Este trabalho analisou 10 anos de distribuição espacial e temporal dos raios, dos sistemas precipitantes e suas características, como refletividade, temperatura de brilho e altura dos sistemas precipitantes amostrados pelo satélite Tropical Rainfall Measuring Mission (TRMM) através dos sensores Lightning Imaging Sensor (LIS), Precipitation Radar (PR) e TRMM Microwave Imager (TMI). Estes dados foram organizados e armazenados pelo grupo de pesquisa da convecção tropical da University of Utah no período de dezembro de 1997 a fevereiro de 2009. Também foram analisados dados de focos de queimadas detectadas pelo Instituto Nacional de Pesquisas Espaciais (INPE), no período de 1998 a 2008. Foi selecionada uma área delimitada entre 60ºW a 45ºW de longitude e 10ºS a 5ºN de latitude, a qual, posteriormente, foi dividida em nove sub-áreas para um melhor detalhamento dasinformações. Para verificar a possível influência das queimadas no número de raios, selecionaram-se oito áreas, sendo 4 com o maior número de focos de queimadas e 4 com o menor número de focos de queimadas. Os sistemas precipitantes foram classificados seguindo a metodologia de Nesbitt et. al. 2000 e obedecendo a nova definição dos dados realizado por Liu (2007). Os sistemas precipitantes amostrados pelo satélite TRMM utilizados neste trabalho são denominados ALLPFS e são definidos como aqueles que apresentam pixel de chuva estimado pelo algoritmo 2A25. Estes são classificados em PFS e OTHPFS, que respectivamente, são aqueles que apresentam e não apresentam informação de temperatura de brilho. Os PFS são sub-classificados em sistemas sem assinatura de gelo (NOICE), com assinatura de gelo (WICE) e sistemas convectivos de mesoescala (MCS), sendo que os sistemas mais intensos, dentre estes últimos, são sistemas que recebem a denominação de IMCS. Os resultados mostram que as regiões do sul do Estado do Pará, município de Belém e Ilha do Marajó foram as que apresentaram as maiores ocorrências de raios na Amazônia Oriental, com valores superiores a 20 a 35 raios/km^²/ano. Os NOICEs foram os sistemas mais frequentes em todas as regiões e os sistemas precipitantes da categoria WICE e MCS são aqueles que mais contribuem com a produção de raios sobre essas regiões. Os sistemas eletrificados apresentam grande contribuição no volume de chuva estimada sobre as áreas CENTRO e SUL, com percentuais superiores a 50% nas áreas SUL. A variação mensal dos raios na área de estudo mostrou que as maiores ocorrências de raios sobre o município de Belém são nos meses de janeiro a junho, com um pico no mês de janeiro. As maiores ocorrências no setor SUL da Amazônia Oriental concentram-se nos meses de setembro a dezembro. Nas análises sobre a interação entre os raios e as queimadas não se observou coerência, dentro das áreas de maior número de queimadas, na correlação mensal entre os raios e as queimadas, evidenciando que, apesar do grande número de queimadas observado sobre essas áreas, outros fatores interferem na produção de raios.

A Multiple-Vortex Tornado in Southeastern Brazil

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Long-term rainfall trends in Serra da Mantiqueira Environmental Protection Area, southeast Brazil

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Stability of Order in Solvent-Annealed Block Copolymer Thin Films

ABSTRACT: One way to produce high order in a block copolymer thin film is by solution casting a thin film and slowly evaporating the solvent in a sealed vessel. Such a solvent-annealing process is a versatile method to produce a highly ordered thin film of a block copolymer. However, the ordered structure of the film degrades over time when stored under ambient conditions. Remarkably, this aging process occurs in mesoscale thin films of polystyrene-polyisoprene triblock copolymer where the monolayer of vitrified 15 nm diameter polystyrene cylinders sink in a 20 nm thick film at 22 °C. The transformation is studied by atomic force microscopy (AFM). We describe the phenomena, characterize the aging process, and propose a semiquantitative model to explain the observations. The residual solvent effects are important but not the primary driving force for the aging process. The study may lead to effective avenue to improve order and make the morphology robust and possibly the solvent-annealing process more effective.

Is the Brazil Current eddy-dominated to the north of 20 degrees S?

The Brazil Current (BC) originates with the arrival and bifurcation of the southernmost branch of the South Equatorial Current (sSEC) between 10-20 degrees S. Previous climatological studies showed a stratified sSEC bifurcation and that the resulting southern branch formed a shallow BC - a weak western boundary current. The analysis of three recent synoptic surveys and global model outputs challenge the description of a continuous BC. The sSEC bifurcation signal near the continental margin was unclear in the analyses, and the velocity fields were dominated by mesoscale eddies. Recurrent anticyclones that seemed to be related to the meandering BC led us to construct a picture of a flow strongly influenced by topography and probably very unstable. Given this new emerging scenario, we hypothesize that the Brazil Current is eddy-dominated to the north of 20 degrees S. Citation: Soutelino, R. G., I. C. A. da Silveira, A. Gangopadhyay, and J. A. Miranda (2011), Is the Brazil Current eddy-dominated to the north of 20 S?, Geophys. Res. Lett., 38, L03607, doi:10.1029/2010GL046276.

A two-layer approximation to the Brazil Current-Intermediate Western Boundary Current System between 20 degrees S and 28 degrees S

It has been shown that the vertical structure of the Brazil Current (BC)-Intermediate Western Boundary Current (IWBC) System is dominated by the first baroclinic mode at 22 degrees S-23 degrees S. In this work, we employed the Miami Isopycnic Coordinate Ocean Model to investigate whether the rich mesoscale activity of this current system, between 20 degrees S and 28 degrees S, is reproduced by a two-layer approximation of its vertical structure. The model results showed cyclonic and anticyclonic meanders propagating southwestward along the current axis, resembling the dynamical pattern of Rossby waves superposed on a mean flow. Analysis of the upper layer zonal velocity component, using a space-time diagram, revealed a dominant wavelength of about 450 km and phase velocity of about 0.20 ms(-1) southwestward. The results also showed that the eddy-like structures slowly grew in amplitude as they moved downstream. Despite the simplified design of the numerical experiments conducted here, these results compared favorably with observations and seem to indicate that weakly unstable long baroclinic waves are responsible for most of the variability observed in the BC-IWBC system. (C) 2009 Elsevier Ltd. All rights reserved.

Submesoscale activity over the Argentinian shelf

Submesoscale activity over the Argentinian shelf is investigated by means of high resolution primitive equation numerical solutions. These reveal energetic turbulent activity (visually similar to the one occasionally seen in satellite images) at scales O(5 km) in fall and winter that is linked to mixed layer baroclinic instability. The air-sea heat flux responsible for (i) deepening the upper ocean boundary layer (at these seasons) and (ii) maintaining a cross-shelf background density gradient is the key environmental parameter controlling submesoscale activity. Implications of submesoscale turbulence are investigated. Its mixing efficiency estimated by computing a diffusivity coefficient is above 30 m(2) s(-1) away from the shallowest regions. Aggregation of surface buoyant material by submesoscale currents occurs within hours and is presumably important to the ecosystem.

Global interannual trends and amplitude modulations of the sea surface height anomaly from the TOPEX/Jason-1 altimeters

This study uses the global Ocean Topography Experiment (TOPEX)/Jason-1 altimeters` time series to estimate the 13-yr trend in sea surface height anomaly. These trends are estimated at each grid point by two methods: one fits a straight line to the time series and the other is based on the difference between the average height between the two halves of the time series. In both cases the trend shows large regional variability, mostly where the intense western boundary currents turn. The authors hypothesize that the regional variability of the sea surface height trends leads to changes in the local geostrophic transport. This in turn affects the instability-related processes that generate mesoscale eddies and enhances the Rossby wave signals. This hypothesis is verified by estimates of the trend of the amplitude of the filtered sea surface height anomaly that contains the spectral bands associated with Rossby waves and mesoscale eddies. The authors found predominantly positive tendency in the amplitude of Rossby waves and eddies, which suggests that, on average, these events are becoming more energetic. In some regions, the variation in amplitude over 13 yr is comparable to the standard deviation of the data and is statistically significant according to both methods employed in this study. It is plausible that in this case, the energy is transferred from the mean currents to the waves and eddies through barotropic and baroclinic instability processes that are more pronounced in the western boundary current extension regions. If these heat storage patterns and trends are confirmed on longer time series, then it will be justified to argue that the warming trend of the last century provides the energy that amplifies both Rossby waves and mesoscale eddies.

Influence of salinity on the interannual heat storage trends in the Atlantic estimated from altimeters and Pilot Research Moored Array in the Tropical Atlantic data

Changes in the oceanic heat storage (HS) can reveal important evidences of climate variability related to ocean heat fluxes. Specifically, long-term variations in HS are a powerful indicator of climate change as HS represents the balance between the net surface energy flux and the poleward heat transported by the ocean currents. HS is estimated from sea surface height anomaly measured from the altimeters TOPEX/Poseidon and Jason 1 from 1993 to 2006. To characterize and validate the altimeter-based HS in the Atlantic, we used the data from the Pilot Research Moored Array in the Tropical Atlantic (PIRATA) array. Correlations and rms differences are used as statistical figures of merit to compare the HS estimates. The correlations range from 0.50 to 0.87 in the buoys located at the equator and at the southern part of the array. In that region the rms differences range between 0.40 and 0.51 x 10(9) Jm(-2). These results are encouraging and indicate that the altimeter has the precision necessary to capture the interannual trends in HS in the Atlantic. Albeit relatively small, salinity changes can also have an effect on the sea surface height anomaly. To account for this effect, NCEP/GODAS reanalysis data are used to estimate the haline contraction. To understand which dynamical processes are involved in the HS variability, the total signal is decomposed into nonpropagating basin-scale and seasonal (HS(l)) planetary waves, mesoscale eddies, and small-scale residual components. In general, HS(l) is the dominant signal in the tropical region. Results show a warming trend of HS(l) in the past 13 years almost all over the Atlantic basin with the most prominent slopes found at high latitudes. Positive interannual trends are found in the halosteric component at high latitudes of the South Atlantic and near the Labrador Sea. This could be an indication that the salinity anomaly increased in the upper layers during this period. The dynamics of the South Atlantic subtropical gyre could also be subject to low-frequency changes caused by a trend in the halosteric component on each side of the South Atlantic Current.

Quantum Mechanics Insight into the Microwave Nucleation of SrTiO3 Nanospheres

An extensive investigation of strontium titanate, SrTiO3 (STO), nanospheres synthesized via a microwave-assisted hydrothermal (MAH) method has been conducted to gain a better insight into thermodynamic, kinetic, and reaction phenomena involved in STO nucleation and crystal growth processes. To this end, quantum chemical modeling based on the density functional theory and periodic super cell models were done. Several experimental techniques were employed to get a deep characterization of structural and optical features of STO nanospheres. A possible formation mechanism was proposed, based on dehydration of titanium and strontium clusters followed by mesoscale transformation and a self-assembly process along an oriented attachment mechanism resulting in spherical like shape. Raman and XANES analysis renders a noncentrosymmetric environment for the octahedral titanium, while infrared and first order Raman modes reveal OH groups which are unsystematically incorporated into uncoordinated superficial sites. These results seem to indicate that the key component is the presence of distorted TiO6 clusters to engender a luminescence property. Analysis of band structure, density Of states, and charge map shows that there is a close relationship among local broken symmetry, polarization, and energy split of the 3d orbitals of titanium. The interplay among these electronic and structural features provides necessary conditions to evaluate its luminescent properties under two energy excitation.