Novos métodos de síntese de 4-quinolonas e benzo[b]acridonas

As 4-quinolonas e as acridonas são duas importantes famílias de compostos heterocíclicos azotados naturais que apresentam uma variedade de importantes aplicações biológicas. As 4-quinolonas têm sido objecto de extensos estudos devido às suas potenciais aplicações como fortes agentes citotóxicos, antimitóticos e anti-plaquetários e como protectores cardiovasculares, mas o seu uso é principalmente como antibióticos de largo espectro. As acridonas são conhecidas por apresentarem importante actividade antiviral, antiparasitária, contra a leishmania e a malária, e anticancerígena. A variedade de importantes aplicações biológicas das 4-quinolonas e das acridonas e a contínua procura pela comunidade científica de novas substâncias com actividades biológicas atractivas destaca estes compostos como alvos interessantes para a preparação de novos derivados e/ou para o desenvolvimento de novos métodos de síntese destas duas famílias de compostos. No primeiro capítulo desta dissertação descreve-se a síntese dos compostos de partida que tiveram de ser previamente preparados para o desenvolvimento das novas rotas de síntese apresentadas nos capítulos seguintes. A 4-cloro-3- formilquinolina foi obtida através da reacção de Vilsmeier-Haack da 2’-aminoacetofenona enquanto que a 3-formilquinolin-4(1H)-ona foi facilmente preparada por hidrólise ácida da anterior. Foi necessário proteger o grupo amina da quinolin-4(1H)-ona para evitar reacções secundárias e foram descritas as reacções de protecção com o grupo metilo, etoxicarbonilo e ptoluenossulfonilo. Os 2,2-dióxidos de 1,3-di-hidrobenzo[c]tiofeno, necessários para o estudo das reacções de Diels-Alder, não se encontram disponíveis comercialmente e a sua síntese é também descrita. No segundo capítulo reporta-se uma nova e eficiente rota de síntese de (Z)- e (E)-3-estirilquinolin-4(1H)-onas a partir da reacção de Wittig da 4-cloro-3- formilquinolina e de 3-formilquinolin-4(1H)-onas com benzilidenotrifenilfosforanos. As (Z)-3-estirilquinolin-4(1H)-onas foram obtidas com elevada diastereoselectividade a partir da reacção das 3-formilquinolin- 4(1H)-onas N-protegidas enquanto que as (E)-3-estirilquinolin-4(1H)-onas foram preparadas através da reacção de Wittig da 4-cloro-3-formilquinolina seguida da hidrólise ácida das respectivas (Z)- e (E)-4-cloro-3-estirilquinolinas obtidas. Ambas as rotas sintéticas são eficientes, independentemente dos substituintes dos benzilidenotrifenilfosforanos. No terceiro capítulo, descreve-se um novo método de síntese de novas benzo[b]acridonas a partir da reacção de Diels-Alder de 3-formilquinolin-4(1H)- onas N-protegidas, que actuam como dienófilos, com dienos altamente reactivos, os orto-benzoquinodimetanos, preparados in situ através da extrusão térmica do dióxido de enxofre dos respectivos 2,2-dióxidos de 1,3-dihidrobenzo[ c]tiofeno. A reacção de cicloadição das 3-formilquinolin-4(1H)-onas N-protegidas com orto-benzoquinodimetanos origina as benzo[b]-1,6,6a,12atetra- hidroacridin-12(7H)-onas esperadas, que são o resultado da referida cicloadição seguida de desformilação in situ, e mostrou ser eficiente apenas quando o grupo amina está derivatizado com um grupo sacador de electrões. A desidrogenação destas benzo[b]-1,6,6a,12a-tetra-hidroacridin-12(7H)-onas em dimetilsulfóxido utilizando uma quantidade catalítica de iodo foi também descrita e originou como produto principal as benzo[b]acridin-12(7H)-onas N-desprotegidas. Todos os compostos novos sintetizados foram caracterizados por diversas técnicas analíticas, especialmente por estudos espectroscópicos de ressonância magnética nuclear (RMN), incluindo espectros de 1H e 13C, bidimensionais de correlação espectroscópica homonuclear e heteronuclear e de efeito nuclear de Overhauser (NOESY). Foram também efectuados, sempre que possível, espectros de massa (EM) e análises elementares ou espectros de massa de alta resolução (EMAR) para todos os compostos novos sintetizados. O tautomerismo da 3-formil- e 3-estirilquinolin-4(1H)-onas e as isomerizações (E) (Z) e rotacional das 3-estirilquinolin-4(1H)-onas e das 4-cloro-3-estirilquinolinas foram estudados através de ressonância magnética nuclear experimental (RMN 1H e 13C) e teórica [B3LYP/6-311++G(d,p)].

Levantamento ambiental de uma indústria conserveira nos Açores

Dissertação de Mestrado em Ambiente, Saúde e Segurança.

Hospitalisation pour problèmes respiratoires et exposition aux émissions d’une aluminerie chez l’enfant

L’exposition quotidienne aux polluants atmosphériques tels que le dioxyde de soufre, les particules fines (PM2.5) et l’ozone en milieu urbain sont associés à des effets néfastes sur la santé respiratoire des enfants. Des études épidémiologiques transversales rapportent des associations entre la pollution atmosphérique et des problèmes de santé respiratoires chez les enfants en milieu industriel telles que la prévalence de l’asthme et de l'hyperréactivité bronchique. Ces études épidémiologiques transversales ne permettent pas d’évaluer les effets sur la santé d’une exposition de courte durée. Peu d’études ont évalué les effets respiratoires des expositions aiguës chez les enfants à la pollution atmosphérique d’émissions industrielles. Dans ce mémoire, nous avons analysé l’association entre l’exposition journalière aux émissions d’une aluminerie et l’hospitalisation pour problèmes respiratoires (asthme, bronchiolite) chez les enfants de Shawinigan. Pour étudier ces effets des expositions aiguës, nous avons utilisé le devis épidémiologique de type « case-crossover » qui compare l’exposition lors des jours « cas » (jour d’hospitalisation) avec l’exposition lors des jours « contrôle » (exposition du même individu, les mêmes jours de la semaine, durant le même mois). Les variables d’exposition suivantes ont été calculées pour les enfants vivants dans un rayon de 7.5 km de l’industrie et pour ceux habitant à moins de 2.5 km de la station de mesure de polluants près de l’industrie : i) le nombre d’heures par jour durant lesquelles la résidence de chaque enfant recevait le panache de fumée de l’industrie. ii) les concentrations journalières de PM2.5 et de SO2 (moyenne et maximales) de la station de mesure des polluants localisée près de l’industrie. Des régressions logistiques conditionnelles ont été utilisées pour estimer les rapports de cotes (OR) et leurs intervalles de confiance à 95% (IC95%). Au total, 429 hospitalisations d’enfants pour asthme et bronchiolite ont été recensées pendant la période d’étude allant de 1999 à 2008. Le risque d’hospitalisations pour asthme et bronchiolite a augmenté avec l’augmentation du nombre d’heures d’exposition aux fumées de l’industrie, chez les enfants de moins de 5 ans. Pour les enfants de 2-4 ans, cette association était : OR : 1.27, pour un interquartile de 4.8 heures/jour; intervalle de confiance à 95%: 1.03-1.56. Des tendances moins prononcées sont notées avec les niveaux de SO2 et de PM2.5. Cette étude suggère que l’exposition journalière aux émissions industrielles identifiées par l’exposition horaire des vents venant de l’usine pourrait être associée à une exacerbation des problèmes respiratoires chez les jeunes enfants. De plus, l’effet plus prononcé avec la variable d’exposition basée sur les vents suggère un effet découlant des polluants autres que ceux mesurés (SO2 et PM2.5), possiblement comme les hydrocarbures aromatiques polycycliques (HAP).

Problèmes respiratoires et exposition aux émissions d’industries au Saguenay

La majorité des études qui ont examiné les effets respiratoires d’une exposition de courte durée à la pollution de l’air ont été réalisées en milieu urbain. En milieu pollué par des sources industrielles, la nature de l’exposition diffère de celle en milieu urbain. Le premier objectif de ce mémoire visait une recension des études traitant de l’association entre les effets respiratoires chez l’enfant et l’exposition aux émissions de polluants industriels. La majorité des études suggèrent que l’exposition aux émissions de polluants émis par des industries est associée à un accroissement des problèmes respiratoires. Dans ces études, l’effet de l’exposition de courte durée a rarement été étudié. L’autre objectif du mémoire était d’évaluer l’association entre une exposition journalière aux émissions de pollution atmosphérique d’un complexe industriel (deux fonderies et une usine de raffinage de l’alumine) du Saguenay, Québec, et les hospitalisations pour problèmes respiratoires des enfants de 0 à 4 ans vivant près de celles-ci (<7.5 km), à l’aide d’une étude épidémiologique de type cas-croisé. Le pourcentage d’heures où le domicile de l’enfant était sous les vents provenant de la direction du complexe industriel et les maxima et moyennes journalières des concentrations de dioxyde de soufre (SO2) et de particules fines (PM2.5) ont été recueillis du 1er janvier 2001 au 31 décembre 2010 afin d’estimer l’exposition. Des régressions logistiques conditionnelles ont été employées pour estimer les rapports de cotes (OR) et les intervalles de confiance à 95%. Les hospitalisations pour asthme et bronchiolite chez les jeunes enfants étaient associées à l’augmentation de l’exposition journalière aux émissions, estimée par le pourcentage d’heures sous les vents. Les résultats de ce mémoire suggèrent que l’exposition aux émissions industrielles de polluants de l’air est associée à des effets respiratoires chez les enfants.

Caracterización de la exposición ocupacional a los gases, dióxido de azufre (so2), sulfuro de hidrógeno (h2s), y monóxido de carbono (co), y la percepción de salud de los trabajadores, en una empresa del sector hidrocarburo en Colombia

En el proceso de extracción de petróleo (crudo) deben realizarse tratamientos físicos y químicos en estaciones de recolección del hidrocarburo con el fin de garantizar su calidad antes de su entrega para el transporte y comercialización. Para la realización de esta actividad el personal operativo requerido (operadores) debe realizar diferentes actividades, tales como ronda operacional, verificación de sistemas de almacenamiento del crudo, agua residual del proceso e insumos químicos utilizados en su tratamiento y manipulación de facilidades en las estaciones de recolección, entre otras. Como resultados de las actividades rutinarias los operadores están expuestos a factores de riesgo químico asociados a gases y vapores orgánicos generados en los procesos de tratamiento del crudo. En el presente trabajo se realizaron mediciones de calidad de aire e higiene industrial en diferentes estaciones tratamiento de crudo, con el propósito de evaluar los niveles de exposición de los operadores a gases y vapores de hidrocarburos durante el proceso de tratamiento de crudo y dar respuesta a la siguiente pregunta: ¿existe relación entre la exposición ocupacional, las emisiones atmosféricas de gases (SO2, CO, H2S) y la percepción de afectación de la salud de los trabajadores que se encuentran expuestos durante la actividad laboral, en una empresa del sector de hidrocarburos? Se realizó un estudio de corte transversal, mediante la aplicación de cuestionarios sobre las condiciones de trabajo y de salud a 30 trabajadores que laboran en una estación de tratamiento de crudo de una compañía del sector de hidrocarburos. Los operadores objeto de estudio laboran en turnos rotativos, han estado vinculados con la compañía por más de dos años y tienen contrato directo, adicionalmente, se identificaron los factores de riesgos ambientales y ocupacionales para el grupo de trabajadores y se realizó una revisión de los informes de medición de higiene industrial y de calidad de aire de las estaciones donde labora el personal seleccionado con el fin de establecer si los resultados se relacionan. Los resultados obtenidos indican que el 100% de los trabajadores son de género masculino y se desempeñan en cargos de operadores, recorredores de pozos de crudo y supervisores. El 97% de los operadores tiene más de cuarenta años de edad y el 80% de los mismos ha laborado por más de 6 años en la compañía. Acerca de la percepción de los trabajadores sobre su estado de salud el 90% afirma que su salud es buena, el 97% respondió que no presenta problemas respiratorios, el 23% manifiesta que presenta trastornos dermatológicos y el 27% indican que presenta dolor de cabeza constante. De la revisión de los informes de calidad de aire disponibles se encontró que las mediciones de Dióxido de Azufre SO2, Monóxido de Carbono CO se encuentran dentro del rango definido como el de menor impacto para la salud humana. De los datos del informe se puede concluir que la calidad del aire es buena en el 100% de las áreas de influencia de las estaciones de tratamiento de crudo. Según los informes de higiene industrial el 34% de las instalaciones presenta concentraciones de Sulfuro de Hidrógeno (H2S) en el límite permisible para exposiciones crónicas en un promedio ponderado de tiempo (TLV-TWA) y el límite permisible para exposiciones agudas en un límite de exposición a corto plazo (TLV-STEL). Solo el 37% de los trabajadores objeto de este estudio percibe el riesgo por la exposición a factores de riesgo químicos y son claramente consientes que se encuentran expuestos a estos riesgos por la manipulación de productos químicos y exposición a sustancias químicas producto de sus actividades rutinarias, el 73% no percibe el riesgo de exposición por su actividad laboral. Se recomienda que la compañía fortalezca su esquema de vigilancia para generar alternativas que eleven los niveles de consciencia del riesgo del trabajador. Los factores de riesgo ambiental y ocupacional, de los gases y vapores generados se deben al proceso de tratamiento de crudo, están mutuamente relacionados dado que al generarse una emisión y/o escape no controlado como consecuencia se tiene una afectación directa al medio ambiente y a los trabajadores.

Combined Analysis of the Short-Term Effects of Photochemical Air Pollutants on Mortality within the EMECAM Project

In recent years, some epidemiologic studies have attributed adverse effects of air pollutants on health not only to particles and sulfur dioxide but also to photochemical air pollutants (nitrogen dioxide and ozone). The effects are usually small, leading to some inconsistencies in the results of the studies. Furthermore, the different methodologic approaches of the studies used has made it difficult to derive generic conclusions. We provide here a quantitative summary of the short-term effects of photochemical air pollutants on mortality in seven Spanish cities involved in the EMECAM project, using generalized additive models from analyses of single and multiple pollutants. Nitrogen dioxide and ozone data were provided by seven EMECAM cities (Barcelona, Gijón, Huelva, Madrid, Oviedo, Seville, and Valencia). Mortality indicators included daily total mortality from all causes excluding external causes, daily cardiovascular mortality, and daily respiratory mortality. Individual estimates, obtained from city-specific generalized additive Poisson autoregressive models, were combined by means of fixed effects models and, if significant heterogeneity among local estimates was found, also by random effects models. Significant positive associations were found between daily mortality (all causes and cardiovascular) and NO2, once the rest of air pollutants were taken into account. A 10 μg/m3 increase in the 24-hr average 1-day NO2 level was associated with an increase in the daily number of deaths of 0.43% [95% confidence interval(CI), –0.003–0.86%] for all causes excluding external. In the case of significant relationships, relative risks for cause-specific mortality were nearly twice as much as that for total mortality for all the photochemical pollutants. Ozone was independently related only to cardiovascular daily mortality. No independent statistically significant relationship between photochemical air pollutants and respiratory mortality was found. The results in this study suggest that, given the present levels of photochemical pollutants, people living in Spanish cities are exposed to health risks derived from air pollution

Report of the 2010 assessment of the scientific assessment panel: future ozone and its impact on surface UV

SCIENTIFIC SUMMARY Globally averaged total column ozone has declined over recent decades due to the release of ozone-depleting substances (ODSs) into the atmosphere. Now, as a result of the Montreal Protocol, ozone is expected to recover from the effects of ODSs as ODS abundances decline in the coming decades. However, a number of factors in addition to ODSs have led to and will continue to lead to changes in ozone. Discriminating between the causes of past and projected ozone changes is necessary, not only to identify the progress in ozone recovery from ODSs, but also to evaluate the effectiveness of climate and ozone protection policy options. Factors Affecting Future Ozone and Surface Ultraviolet Radiation • At least for the next few decades, the decline of ODSs is expected to be the major factor affecting the anticipated increase in global total column ozone. However, several factors other than ODS will affect the future evolution of ozone in the stratosphere. These include changes in (i) stratospheric circulation and temperature due to changes in long-lived greenhouse gas (GHG) abundances, (ii) stratospheric aerosol loading, and (iii) source gases of highly reactive stratospheric hydrogen and nitrogen compounds. Factors that amplify the effects of ODSs on ozone (e.g., stratospheric aerosols) will likely decline in importance as ODSs are gradually eliminated from the atmosphere. • Increases in GHG emissions can both positively and negatively affect ozone. Carbon dioxide (CO2)-induced stratospheric cooling elevates middle and upper stratospheric ozone and decreases the time taken for ozone to return to 1980 levels, while projected GHG-induced increases in tropical upwelling decrease ozone in the tropical lower stratosphere and increase ozone in the extratropics. Increases in nitrous oxide (N2O) and methane (CH4) concentrations also directly impact ozone chemistry but the effects are different in different regions. • The Brewer-Dobson circulation (BDC) is projected to strengthen over the 21st century and thereby affect ozone amounts. Climate models consistently predict an acceleration of the BDC or, more specifically, of the upwelling mass flux in the tropical lower stratosphere of around 2% per decade as a consequence of GHG abundance increases. A stronger BDC would decrease the abundance of tropical lower stratospheric ozone, increase poleward transport of ozone, and could reduce the atmospheric lifetimes of long-lived ODSs and other trace gases. While simulations showing faster ascent in the tropical lower stratosphere to date are a robust feature of chemistry-climate models (CCMs), this has not been confirmed by observations and the responsible mechanisms remain unclear. • Substantial ozone losses could occur if stratospheric aerosol loading were to increase in the next few decades, while halogen levels are high. Stratospheric aerosol increases may be caused by sulfur contained in volcanic plumes entering the stratosphere or from human activities. The latter might include attempts to geoengineer the climate system by enhancing the stratospheric aerosol layer. The ozone losses mostly result from enhanced heterogeneous chemistry on stratospheric aerosols. Enhanced aerosol heating within the stratosphere also leads to changes in temperature and circulation that affect ozone. • Surface ultraviolet (UV) levels will not be affected solely by ozone changes but also by the effects of climate change and by air quality change in the troposphere. These tropospheric effects include changes in clouds, tropospheric aerosols, surface reflectivity, and tropospheric sulfur dioxide (SO2) and nitrogen dioxide (NO2). The uncertainties in projections of these factors are large. Projected increases in tropospheric ozone are more certain and may lead to reductions in surface erythemal (“sunburning”) irradiance of up to 10% by 2100. Changes in clouds may lead to decreases or increases in surface erythemal irradiance of up to 15% depending on latitude. Expected Future Changes in Ozone Full ozone recovery from the effects of ODSs and return of ozone to historical levels are not synonymous. In this chapter a key target date is chosen to be 1980, in part to retain the connection to previous Ozone Assessments. Noting, however, that decreases in ozone may have occurred in some regions of the atmosphere prior to 1980, 1960 return dates are also reported. The projections reported on in this chapter are taken from a recent compilation of CCM simulations. The ozone projections, which also form the basis for the UV projections, are limited in their representativeness of possible futures since they mostly come from CCM simulations based on a single GHG emissions scenario (scenario A1B of Emissions Scenarios. A Special Report of Working Group III of the Intergovernmental Panel on Climate Change, Cambridge University Press, 2000) and a single ODS emissions scenario (adjusted A1 of the previous (2006) Ozone Assessment). Throughout this century, the vertical, latitudinal, and seasonal structure of the ozone distribution will be different from what it was in 1980. For this reason, ozone changes in different regions of the atmosphere are considered separately. • The projections of changes in ozone and surface clear-sky UV are broadly consistent with those reported on in the 2006 Assessment. • The capability of making projections and attribution of future ozone changes has been improved since the 2006 Assessment. Use of CCM simulations from an increased number of models extending through the entire period of ozone depletion and recovery from ODSs (1960–2100) as well as sensitivity simulations have allowed more robust projections of long-term changes in the stratosphere and of the relative contributions of ODSs and GHGs to those changes. • Global annually averaged total column ozone is projected to return to 1980 levels before the middle of the century and earlier than when stratospheric halogen loading returns to 1980 levels. CCM projections suggest that this early return is primarily a result of GHG-induced cooling of the upper stratosphere because the effects of circulation changes on tropical and extratropical ozone largely cancel. Global (90°S–90°N) annually averaged total column ozone will likely return to 1980 levels between 2025 and 2040, well before the return of stratospheric halogens to 1980 levels between 2045 and 2060. • Simulated changes in tropical total column ozone from 1960 to 2100 are generally small. The evolution of tropical total column ozone in models depends on the balance between upper stratospheric increases and lower stratospheric decreases. The upper stratospheric increases result from declining ODSs and a slowing of ozone destruction resulting from GHG-induced cooling. Ozone decreases in the lower stratosphere mainly result from an increase in tropical upwelling. From 1960 until around 2000, a general decline is simulated, followed by a gradual increase to values typical of 1980 by midcentury. Thereafter, although total column ozone amounts decline slightly again toward the end of the century, by 2080 they are no longer expected to be affected by ODSs. Confidence in tropical ozone projections is compromised by the fact that simulated decreases in column ozone to date are not supported by observations, suggesting that significant uncertainties remain. • Midlatitude total column ozone is simulated to evolve differently in the two hemispheres. Over northern midlatitudes, annually averaged total column ozone is projected to return to 1980 values between 2015 and 2030, while for southern midlatitudes the return to 1980 values is projected to occur between 2030 and 2040. The more rapid return to 1980 values in northern midlatitudes is linked to a more pronounced strengthening of the poleward transport of ozone due to the effects of increased GHG levels, and effects of Antarctic ozone depletion on southern midlatitudes. By 2100, midlatitude total column ozone is projected to be above 1980 values in both hemispheres. • October-mean Antarctic total column ozone is projected to return to 1980 levels after midcentury, later than in any other region, and yet earlier than when stratospheric halogen loading is projected to return to 1980 levels. The slightly earlier return of ozone to 1980 levels (2045–2060) results primarily from upper stratospheric cooling and resultant increases in ozone. The return of polar halogen loading to 1980 levels (2050–2070) in CCMs is earlier than in empirical models that exclude the effects of GHG-induced changes in circulation. Our confidence in the drivers of changes in Antarctic ozone is higher than for other regions because (i) ODSs exert a strong influence on Antarctic ozone, (ii) the effects of changes in GHG abundances are comparatively small, and (iii) projections of ODS emissions are more certain than those for GHGs. Small Antarctic ozone holes (areas of ozone <220 Dobson units, DU) could persist to the end of the 21st century. • March-mean Arctic total column ozone is projected to return to 1980 levels two to three decades before polar halogen loading returns to 1980 levels, and to exceed 1980 levels thereafter. While CCM simulations project a return to 1980 levels between 2020 and 2035, most models tend not to capture observed low temperatures and thus underestimate present-day Arctic ozone loss such that it is possible that this return date is biased early. Since the strengthening of the Brewer-Dobson circulation through the 21st century leads to increases in springtime Arctic column ozone, by 2100 Arctic ozone is projected to lie well above 1960 levels. Uncertainties in Projections • Conclusions dependent on future GHG levels are less certain than those dependent on future ODS levels since ODS emissions are controlled by the Montreal Protocol. For the six GHG scenarios considered by a few CCMs, the simulated differences in stratospheric column ozone over the second half of the 21st century are largest in the northern midlatitudes and the Arctic, with maximum differences of 20–40 DU between the six scenarios in 2100. • There remain sources of uncertainty in the CCM simulations. These include the use of prescribed ODS mixing ratios instead of emission fluxes as lower boundary conditions, the range of sea surface temperatures and sea ice concentrations, missing tropospheric chemistry, model parameterizations, and model climate sensitivity. • Geoengineering schemes for mitigating climate change by continuous injections of sulfur-containing compounds into the stratosphere, if implemented, would substantially affect stratospheric ozone, particularly in polar regions. Ozone losses observed following large volcanic eruptions support this prediction. However, sporadic volcanic eruptions provide limited analogs to the effects of continuous sulfur emissions. Preliminary model simulations reveal large uncertainties in assessing the effects of continuous sulfur injections. Expected Future Changes in Surface UV. While a number of factors, in addition to ozone, affect surface UV irradiance, the focus in this chapter is on the effects of changes in stratospheric ozone on surface UV. For this reason, clear-sky surface UV irradiance is calculated from ozone projections from CCMs. • Projected increases in midlatitude ozone abundances during the 21st century, in the absence of changes in other factors, in particular clouds, tropospheric aerosols, and air pollutants, will result in decreases in surface UV irradiance. Clear-sky erythemal irradiance is projected to return to 1980 levels on average in 2025 for the northern midlatitudes, and in 2035 for the southern midlatitudes, and to fall well below 1980 values by the second half of the century. However, actual changes in surface UV will be affected by a number of factors other than ozone. • In the absence of changes in other factors, changes in tropical surface UV will be small because changes in tropical total column ozone are projected to be small. By the middle of the 21st century, the model projections suggest surface UV to be slightly higher than in the 1960s, very close to values in 1980, and slightly lower than in 2000. The projected decrease in tropical total column ozone through the latter half of the century will likely result in clear-sky surface UV remaining above 1960 levels. Average UV irradiance is already high in the tropics due to naturally occurring low total ozone columns and high solar elevations. • The magnitude of UV changes in the polar regions is larger than elsewhere because ozone changes in polar regions are larger. For the next decades, surface clear-sky UV irradiance, particularly in the Antarctic, will continue to be higher than in 1980. Future increases in ozone and decreases in clear-sky UV will occur at slower rates than those associated with the ozone decreases and UV increases that occurred before 2000. In Antarctica, surface clear-sky UV is projected to return to 1980 levels between 2040 and 2060, while in the Arctic this is projected to occur between 2020 and 2030. By 2100, October surface clear-sky erythemal irradiance in Antarctica is likely to be between 5% below to 25% above 1960 levels, with considerable uncertainty. This is consistent with multi-model-mean October Antarctic total column ozone not returning to 1960 levels by 2100. In contrast, by 2100, surface clear-sky UV in the Arctic is projected to be 0–10% below 1960 levels.

Bounding the role of black carbon in the climate system: a scientific assessment

Black carbon aerosol plays a unique and important role in Earth’s climate system. Black carbon is a type of carbonaceous material with a unique combination of physical properties. This assessment provides an evaluation of black-carbon climate forcing that is comprehensive in its inclusion of all known and relevant processes and that is quantitative in providing best estimates and uncertainties of the main forcing terms: direct solar absorption; influence on liquid, mixed phase, and ice clouds; and deposition on snow and ice. These effects are calculated with climate models, but when possible, they are evaluated with both microphysical measurements and field observations. Predominant sources are combustion related, namely, fossil fuels for transportation, solid fuels for industrial and residential uses, and open burning of biomass. Total global emissions of black carbon using bottom-up inventory methods are 7500 Gg yr�-1 in the year 2000 with an uncertainty range of 2000 to 29000. However, global atmospheric absorption attributable to black carbon is too low in many models and should be increased by a factor of almost 3. After this scaling, the best estimate for the industrial-era (1750 to 2005) direct radiative forcing of atmospheric black carbon is +0.71 W m�-2 with 90% uncertainty bounds of (+0.08, +1.27)Wm�-2. Total direct forcing by all black carbon sources, without subtracting the preindustrial background, is estimated as +0.88 (+0.17, +1.48) W m�-2. Direct radiative forcing alone does not capture important rapid adjustment mechanisms. A framework is described and used for quantifying climate forcings, including rapid adjustments. The best estimate of industrial-era climate forcing of black carbon through all forcing mechanisms, including clouds and cryosphere forcing, is +1.1 W m�-2 with 90% uncertainty bounds of +0.17 to +2.1 W m�-2. Thus, there is a very high probability that black carbon emissions, independent of co-emitted species, have a positive forcing and warm the climate. We estimate that black carbon, with a total climate forcing of +1.1 W m�-2, is the second most important human emission in terms of its climate forcing in the present-day atmosphere; only carbon dioxide is estimated to have a greater forcing. Sources that emit black carbon also emit other short-lived species that may either cool or warm climate. Climate forcings from co-emitted species are estimated and used in the framework described herein. When the principal effects of short-lived co-emissions, including cooling agents such as sulfur dioxide, are included in net forcing, energy-related sources (fossil fuel and biofuel) have an industrial-era climate forcing of +0.22 (�-0.50 to +1.08) W m-�2 during the first year after emission. For a few of these sources, such as diesel engines and possibly residential biofuels, warming is strong enough that eliminating all short-lived emissions from these sources would reduce net climate forcing (i.e., produce cooling). When open burning emissions, which emit high levels of organic matter, are included in the total, the best estimate of net industrial-era climate forcing by all short-lived species from black-carbon-rich sources becomes slightly negative (�-0.06 W m�-2 with 90% uncertainty bounds of �-1.45 to +1.29 W m�-2). The uncertainties in net climate forcing from black-carbon-rich sources are substantial, largely due to lack of knowledge about cloud interactions with both black carbon and co-emitted organic carbon. In prioritizing potential black-carbon mitigation actions, non-science factors, such as technical feasibility, costs, policy design, and implementation feasibility play important roles. The major sources of black carbon are presently in different stages with regard to the feasibility for near-term mitigation. This assessment, by evaluating the large number and complexity of the associated physical and radiative processes in black-carbon climate forcing, sets a baseline from which to improve future climate forcing estimates.

Observations of the eruption of the Sarychev volcano and simulations using the HadGEM2 climate model

In June 2009 the Sarychev volcano located in the Kuril Islands to the northeast of Japan erupted explosively, injecting ash and an estimated 1.2 ± 0.2 Tg of sulfur dioxide into the upper troposphere and lower stratosphere, making it arguably one of the 10 largest stratospheric injections in the last 50 years. During the period immediately after the eruption, we show that the sulfur dioxide (SO2) cloud was clearly detected by retrievals developed for the Infrared Atmospheric Sounding Interferometer (IASI) satellite instrument and that the resultant stratospheric sulfate aerosol was detected by the Optical Spectrograph and Infrared Imaging System (OSIRIS) limb sounder and CALIPSO lidar. Additional surface‐based instrumentation allows assessment of the impact of the eruption on the stratospheric aerosol optical depth. We use a nudged version of the HadGEM2 climate model to investigate how well this state‐of‐the‐science climate model can replicate the distributions of SO2 and sulfate aerosol. The model simulations and OSIRIS measurements suggest that in the Northern Hemisphere the stratospheric aerosol optical depth was enhanced by around a factor of 3 (0.01 at 550 nm), with resultant impacts upon the radiation budget. The simulations indicate that, in the Northern Hemisphere for July 2009, the magnitude of the mean radiative impact from the volcanic aerosols is more than 60% of the direct radiative forcing of all anthropogenic aerosols put together. While the cooling induced by the eruption will likely not be detectable in the observational record, the combination of modeling and measurements would provide an ideal framework for simulating future larger volcanic eruptions.

Effect of SO(2) on the Transport Properties of an Imidazolium Ionic Liquid and Its Lithium Solution

Transport coefficients have been measured as a function of the concentration of sulfur dioxide, SO(2), dissolved in 1-butyl-2,3-dimethylimidazolium bis(trifluoromethylsulfonyl)-imide, [BMMI][Tf(2)N], as well as in its lithium salt solution, Li[Tf(2)N]. The SO(2) reduces viscosity and density and increases conductivity and diffusion coefficients in both the neat [BMMI] [Tf(2)N] and the [BMMI][Tf(2)N]-Li[Tf(2)N] solution. The conductivity enhancement is not assigned to a simple viscosity effect; the weakening of ionic interactions upon SO(2) addition also plays a role. Microscopic details of the SO(2) effect were unraveled using Raman spectroscopy and molecular dynamics (MD) simulations. The Raman spectra suggest that the Li(+)-[Tf(2)N] interaction is barely affected by SO(2), and the SO(2)-[Tf(2)N] interaction is weaker than previously observed in an investigation of an ionic liquid containing the bromide anion. Transport coefficients calculated by MD simulations show the same trend as the experimental data with respect to SO(2) content. The MD simulations provide structural information on SO(2) molecules around [Tf(2)N], in particular the interaction of the sulfur atom of SO(2) with oxygen and fluorine atoms of the anion. The SO(2)-[BMMI] interaction is also important because the [BMMI] cations with above-average mobility have a larger number of nearest-neighbor SO(2) molecules.

Detailed analysis of the charge transfer complex N,N-dimethylaniline-SO(2) by Raman spectroscopy and density functional theory calculations

Although the amine sulfur dioxide chemistry was well characterized in the past both experimentally and theoretically, no systematic Raman spectroscopic study describes the interaction between N,N-dimethylaniline (DMA) and sulfur dioxide (SO(2)). The formation of a deep red oil by the reaction of SO(2) with DMA is an evidence of the charge transfer (CT) nature of the DMA-SO(2) interaction. The DMA -SO(2) normal Raman spectrum shows the appearance of two intense bands at 1110 and 1151 cm(-1), which are enhanced when resonance is approached. These bands are assigned to nu(s)(SO(2)) and nu(phi-N) vibrational modes, respectively, confirming the interaction between SO(2) and the amine via the nitrogen atom. The dimethyl group steric effect favors the interaction of SO(2) with the ring pi electrons, which gives rise to a pi-pi* low-energy CT electronic transition, as confirmed by time-dependent density functional theory (TDDFT) calculations. In addition, the calculated Raman DMA-SO(2) spectrum at the B3LYP/6-311++g(3df,3pd) level shows good agreement with the experimental results (vibrational wavenumbers and relative intensities), allowing a complete assignment of the vibrational modes. A better understanding of the intermolecular interactions in this model system can be extremely useful in designing new materials to absorb, detect, or even quantify SO(2). Copyright (C) 2009 John Wiley & Sons, Ltd.

The effects of hydrogen sulfide on the polymer electrolyte membrane fuel cell anode catalyst: H(2)S-Pt/C interaction products

The performance of a polymer electrolyte membrane fuel cell (PEMFC) operating on a simulated hydrocarbon reformate is described. The anode feed stream consisted of 80% H(2),similar to 20% N(2), and 8 ppm hydrogen sulfide (H(2)S). Cell performance losses are calculated by evaluating cell potential reduction due to H(2)S contamination through lifetime tests. It is found that potential, or power, loss under this condition is a result of platinum surface contamination with elemental sulfur. Electrochemical mass spectroscopy (EMS) and electrochemical techniques are employed, in order to show that elemental sulfur is adsorbed onto platinum, and that sulfur dioxide is one of the oxidation products. Moreover, it is demonstrated that a possible approach for mitigating H(2)S poisoning on the PEMFC anode catalyst is to inject low levels of air into the H(2)S-contaminated anode feeding stream. (C) 2011 Elsevier B.V. All rights reserved.

Avaliação da genotoxicidade induzida por emissões de veículos automotores - Ctenomys minutus como organismo bioindicador

Existe um número crescente de componentes químicos lançados ao meio ambiente, muitos dos quais são capazes de induzir efeitos danosos adversos à saúde de animais e humanos, representando uma causa importante de preocupação por seus possíveis efeitos a longo prazo. O impacto ecológico e os riscos a saúde dos organismos associados com a exposição a poluentes ambientais são extremamente difíceis de se avaliar devido a muitos desses componentes serem parte de misturas complexas. Os gases produzidos pelos motores dos veículos à combustão contém diversos poluentes sabidamente genotóxicos, como óxidos de nitrogênio (NOX), monóxido de carbono (CO), óxidos de enxofre (SOx), hidrocarbonetos (HC) e seus derivados, bem como particulados, e metais (cádmio, cromo, cobre, níquel, vanádio, zinco e chumbo). Todos esses compostos isolados ou associados a outros elementos são tóxicos ou de efeito danoso aos organismos, de forma não totalmente esclarecida. Este estudo teve como objetivo verificar o possível efeito genotóxico das emissões dos automóveis em roedor nativo Ctenomys minutus cronicamente exposto, através do Ensaio Cometa (EC), comparando os resultados com o Teste de Micronúcleos (MN), ambos em sangue periférico. Levando em consideração alguns fatores que pudessem influenciar os resultados dos testes de genotoxicidade, este trabalho ainda teve como objetivos: identificar a presença de alguns agentes envolvidos na poluição gerada pelos veículos; verificar possíveis diferenças sazonais, como temperatura e ventos; e se existe influência da idade e sexo dos roedores. Os C. minutus (Octodontidae-Rodentia), foram capturados em dois campos diferentes, ambos ao lado da estrada RS/030, na cidade de Osório, Estado do Rio Grande do Sul (RS): (a) Amaral, e (b) Weber. Animais para controle externo foram capturados no Campo Maribo à cerca de 3 km de distância de outra estrada (RS/389-Osório/RS), conseqüentemente afastada das emissões dos veículos. No final do período desse estudo, foram capturados 123 animais (73 fêmeas e 50 machos).

Avaliação de quitosana, aplicada em pós-colheita, na proteção de uva 'Itália' contra Botrytis cinerea

Perdas significativas ocorrem durante o armazenamento e a comercialização de uvas de mesa devido, principalmente, à ocorrência do mofo cinzento (Botrytis cinerea Pers.:Fr.) e, para o controle de patógenos emprega-se, geralmente, o dióxido de enxofre (SO2). Diante da restrição crescente ao uso de produtos químicos em pós-colheita, tem ocorrido considerável interesse em métodos alternativos de controle. Este trabalho teve como principal objetivo avaliar os efeitos da quitosana, na proteção pós-colheita de uva 'Itália' contra B. cinerea. In vivo, avaliou-se o efeito direto e indireto da quitosana pelo tratamento dos cachos de uva, antes e após a inoculação com o patógeno. Utilizou-se quitosana nas concentrações de 0,00; 0,25; 0,50; 1,00; 1,50 e 2,00 % (v/v). Para inoculação, em 10 bagas de cada cacho de uva foram feitos ferimentos de ±2 mm de profundidade, procedendo-se em seguida, a aspersão da suspensão de conídios (±10(5) conídios.mL-1) de B. cinerea. Após os tratamentos, os cachos foram mantidos a 25±1 °C / 80-90 % UR e avaliados diariamente quanto à incidência e severidade da podridão. Avaliações in vitro do efeito do produto sobre o patógeno também foram realizadas analisando-se o crescimento micelial e a germinação dos conídios de B. cinerea. A solução de quitosana, nas concentrações de 1,5 e 2,0 % (v/v), quando empregada após a inoculação com B cinerea, reduziu significativamente o índice de doença no entanto, quando os cachos foram tratados antes da inoculação, não houve efeito significativo do tratamento sobre o desenvolvimento da doença. Nos ensaios in vitro, a solução de quitosana, nas maiores concentrações, suprimiu o crescimento micelial do patógeno e retardou a germinação dos conídios.

Avaliação do efeito de gases poluentes na corrosão metálica: um experimento para o ensino da corrosão

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)