Zinc Phosphate Cement: Variations in proportioning affects dimetral tensile strength

Objectives: To quantify variability in hand proportioning of zinc phosphate cement among a cohort of dental undergraduates and to determine the effect of any such variability on the diametral tensile strength (DTS) of the set cement. The null hypothesis was that such variability has no effect on DTS. 
Methods: Thirty-four operators dispensed a zinc phosphate cement [Fleck's® Cement] according to the manufacturers' instructions. The mass of powder and liquid dispensed was recorded. Cylindrical specimens (n = 2 x 34) of dimensions 6mm x 3mm were prepared using a stainless steel split mould. The maximum mass of powder and the minimum volume of liquid were used as one extreme ratio and the minimum mass of powder and the maximum volume of liquid used on the other extreme. The manufacturers' recommended ratio was also tested (n=34).The samples were left to set for one hour before being transferred into distilled water for 48 hours. Compression across a diameter was carried out using a universal testing machine, H10KS [Tinius Olsen], at a constant crosshead speed of 0.75 ±0.25 mm/min. Statistical analyses (α = 0.05) were by Student's t-test for the powder/liquid ratio and one-way ANOVA and Tukey HSD for for pair-wise comparisons of mean DTS. Tests were carried out for normality and constant variability. 
Results: The mean (range) amount of powder dispensed was 0.863g (0.531-1.216)g. The mean (range) amount of liquid dispensed was 0.341ml (0.265-0.394)ml. The manufacturer's recommended amounts were 0.8g of powder and 0.3ml of liquid. The mean powder/liquid ratio was not significantly different from the manufacturer's recommended value (p=0.64). Mean (SD) DTS were (MPa) max: 7.19(1.50), min: 2.65(1.01), manufacturer: 6.01(1.30). All pair-wise comparisons were significantly different (p<0.001). 
Conclusions: Variability exists in the hand proportioning powder and liquid components of zinc phosphate cement. This variability can affect the DTS of zinc phosphate cement.

Transit timing variations in WASP-10b induced by stellar activity

The hot-JupiterWASP-10bwas reported by Maciejewski et al. to showtransit timing variations (TTVs) with an amplitude of ~3.5 min. These authors proposed that the observed TTVs were caused by a 0.1M_Jup perturbing companion with an orbital period of ~5.23 d, and hence, close to the outer 5:3 mean-motion resonance with WASP-10b. To test this scenario, we present eight new transit light curves of WASP-10b obtained with the Faulkes Telescope North and the Liverpool Telescope. The new light curves, together with 22 previously published ones, were modelled with a Markov Chain Monte Carlo transit fitting code. Transit depth differences reported forWASP-10b are thought to be due to starspot-induced brightness modulation of the host star. Assuming the star is brighter at the activity minimum, we favour a small planetary radius. We find Rp = 1.039^+0.043 _-0.049R_Jup in agreement with Johnson et al. and Maciejewski et al. Recent studies find no evidence for a significant eccentricity in this system. We present consistent system parameters for a circular orbit and refine the orbital ephemeris ofWASP-10b. Our homogeneously derived transit times do not support the previous claimed TTV signal, which was strongly dependent on two previously published transits that have been incorrectly normalized. Nevertheless, a linear ephemeris is not a statistically good fit to the transit times of WASP-10b. We show that the observed transit time variations are due to spot occultation features or systematics. We discuss and exemplify the effects of occultation spot features in the measured transit times and show that despite spot occultation during egress and ingress being difficult to distinguish in the transit light curves, they have a significant effect in the measured transit times. We conclude that if we account for spot features, the transit times of WASP-10b are consistent with a linear ephemeris with the exception of one transit (epoch 143) which is a partial transit. Therefore, there is currently no evidence for the existence of a companion to WASP-10b. Our results support the lack of TTVs of hot-Jupiters reported for the Kepler sample. 

Variations in the Processing of DNA Double-Strand Breaks Along 60-MeV Therapeutic Proton Beams

PURPOSE: To investigate the variations in induction and repair of DNA damage along the proton path, after a previous report on the increasing biological effectiveness along clinically modulated 60-MeV proton beams.

METHODS AND MATERIALS: Human skin fibroblast (AG01522) cells were irradiated along a monoenergetic and a modulated spread-out Bragg peak (SOBP) proton beam used for treating ocular melanoma at the Douglas Cyclotron, Clatterbridge Centre for Oncology, Wirral, Liverpool, United Kingdom. The DNA damage response was studied using the 53BP1 foci formation assay. The linear energy transfer (LET) dependence was studied by irradiating the cells at depths corresponding to entrance, proximal, middle, and distal positions of SOBP and the entrance and peak position for the pristine beam.

RESULTS: A significant amount of persistent foci was observed at the distal end of the SOBP, suggesting complex residual DNA double-strand break damage induction corresponding to the highest LET values achievable by modulated proton beams. Unlike the directly irradiated, medium-sharing bystander cells did not show any significant increase in residual foci.

CONCLUSIONS: The DNA damage response along the proton beam path was similar to the response of X rays, confirming the low-LET quality of the proton exposure. However, at the distal end of SOBP our data indicate an increased complexity of DNA lesions and slower repair kinetics. A lack of significant induction of 53BP1 foci in the bystander cells suggests a minor role of cell signaling for DNA damage under these conditions.

Young Stellar Object VARiability (YSOVAR): Long Timescale Variations in the Mid-infrared

The YSOVAR (Young Stellar Object VARiability) Spitzer Space Telescope observing program obtained the first extensive mid-infrared (3.6 and 4.5 μm) time series photometry of the Orion Nebula Cluster plus smaller footprints in 11 other star-forming cores (AFGL 490, NGC 1333, Mon R2, GGD 12-15, NGC 2264, L1688, Serpens Main, Serpens South, IRAS 20050+2720, IC 1396A, and Ceph C). There are ~29,000 unique objects with light curves in either or both IRAC channels in the YSOVAR data set. We present the data collection and reduction for the Spitzer and ancillary data, and define the "standard sample" on which we calculate statistics, consisting of fast cadence data, with epochs roughly twice per day for ~40 days. We also define a "standard sample of members" consisting of all the IR-selected members and X-ray-selected members. We characterize the standard sample in terms of other properties, such as spectral energy distribution shape. We use three mechanisms to identify variables in the fast cadence data—the Stetson index, a χ2 fit to a flat light curve, and significant periodicity. We also identified variables on the longest timescales possible of six to seven years by comparing measurements taken early in the Spitzer mission with the mean from our YSOVAR campaign. The fraction of members in each cluster that are variable on these longest timescales is a function of the ratio of Class I/total members in each cluster, such that clusters with a higher fraction of Class I objects also have a higher fraction of long-term variables. For objects with a YSOVAR-determined period and a [3.6]-[8] color, we find that a star with a longer period is more likely than those with shorter periods to have an IR excess. We do not find any evidence for variability that causes [3.6]-[4.5] excesses to appear or vanish within our data set; out of members and field objects combined, at most 0.02% may have transient IR excesses.

Time-lapse monitoring of fluid induced geophysical property variations within an unstable earthwork using P-wave refraction

A significant portion of the UK’s transportation system relies on a network of geotechnical earthworks (cuttings and embankments) that were constructed more than 100 years ago, whose stability is affected by the change in precipitation patterns experienced over the past few decades. The vulnerability of these structures requires a reliable, cost- and time-effective monitoring of their geomechanical condition. We have assessed the potential application of P-wave refraction for tracking the seasonal variations of seismic properties within an aged clay-filled railway embankment, located in southwest England. Seismic data were acquired repeatedly along the crest of the earthwork at regular time intervals, for a total period of 16 months. P-wave first-break times were picked from all available recorded traces, to obtain a set of hodocrones referenced to the same spatial locations, for various dates along the surveyed period of time. Traveltimes extracted from each acquisition were then compared to track the pattern of their temporal variability. The relevance of such variations over time was compared with the data experimental uncertainty. The multiple set of hodocrones was subsequently inverted using a tomographic approach, to retrieve a time-lapse model of VPVP for the embankment structure. To directly compare the reconstructed VPVP sections, identical initial models and spatial regularization were used for the inversion of all available data sets. A consistent temporal trend for P-wave traveltimes, and consequently for the reconstructed VPVP models, was identified. This pattern could be related to the seasonal distribution of precipitation and soil-water content measured on site.

Methodological variations in estimating apparent progressive visual field loss in clinical trials of glaucoma treatment.

OBJECTIVES:

To compare methods to estimate the incidence of visual field progression used by 3 large randomized trials of glaucoma treatment by applying these methods to a common data set of annually obtained visual field measurements of patients with glaucoma followed up for an average of 6 years.

METHODS:

The methods used by the Advanced Glaucoma Intervention Study (AGIS), the Collaborative Initial Glaucoma Treatment Study (CIGTS), and the Early Manifest Glaucoma Treatment study (EMGT) were applied to 67 eyes of 56 patients with glaucoma enrolled in a 10-year natural history study of glaucoma using Program 30-2 of the Humphrey Field Analyzer (Humphrey Instruments, San Leandro, Calif). The incidence of apparent visual field progression was estimated for each method. Extent of agreement between the methods was calculated, and time to apparent progression was compared.

RESULTS:

The proportion of patients progressing was 11%, 22%, and 23% with AGIS, CIGTS, and EMGT methods, respectively. Clinical assessment identified 23% of patients who progressed, but only half of these were also identified by CIGTS or EMGT methods. The CIGTS and the EMGT had comparable incidence rates, but only half of those identified by 1 method were also identified by the other.

CONCLUSIONS:

The EMGT and CIGTS methods produced rates of apparent progression that were twice those of the AGIS method. Although EMGT, CIGTS, and clinical assessment rates were comparable, they did not identify the same patients as having had field progression.

Modeling the Rossiter-McLaughlin Effect: Impact of the Convective Center-to-limb Variations in the Stellar Photosphere

bservations of the Rossiter–McLaughlin (RM) effect provide information on star–planet alignments, which can inform planetary migration and evolution theories. Here, we go beyond the classical RM modeling and explore the impact of a convective blueshift that varies across the stellar disk and non-Gaussian stellar photospheric profiles. We simulated an aligned hot Jupiter with a four-day orbit about a Sun-like star and injected center-to-limb velocity (and profile shape) variations based on radiative 3D magnetohydrodynamic simulations of solar surface convection. The residuals between our modeling and classical RM modeling were dependent on the intrinsic profile width and v sin i; the amplitude of the residuals increased with increasing v sin i and with decreasing intrinsic profile width. For slowly rotating stars the center-to-limb convective variation dominated the residuals (with amplitudes of 10 s of cm s−1 to ~1 m s−1); however, for faster rotating stars the dominant residual signature was due a non-Gaussian intrinsic profile (with amplitudes from 0.5 to 9 m s−1). When the impact factor was 0, neglecting to account for the convective center-to-limb variation led to an uncertainty in the obliquity of ~10°–20°, even though the true v sin i was known. Additionally, neglecting to properly model an asymmetric intrinsic profile had a greater impact for more rapidly rotating stars (e.g., v sin i = 6 km s−1) and caused systematic errors on the order of ~20° in the measured obliquities. Hence, neglecting the impact of stellar surface convection may bias star–planet alignment measurements and consequently theories on planetary migration and evolution.

M Dwarf Flare Continuum Variations on One-second Timescales: Calibrating and Modeling of ULTRACAM Flare Color Indices

We present a large data set of high-cadence dMe flare light curves obtained with custom continuum filters on the triple-beam, high-speed camera system ULTRACAM. The measurements provide constraints for models of the near-ultraviolet (NUV) and optical continuum spectral evolution on timescales of ≈1 s. We provide a robust interpretation of the flare emission in the ULTRACAM filters using simultaneously obtained low-resolution spectra during two moderate-sized flares in the dM4.5e star YZ CMi. By avoiding the spectral complexity within the broadband Johnson filters, the ULTRACAM filters are shown to characterize bona fide continuum emission in the NUV, blue, and red wavelength regimes. The NUV/blue flux ratio in flares is equivalent to a Balmer jump ratio, and the blue/red flux ratio provides an estimate for the color temperature of the optical continuum emission. We present a new “color-color” relationship for these continuum flux ratios at the peaks of the flares. Using the RADYN and RH codes, we interpret the ULTRACAM filter emission using the dominant emission processes from a radiative-hydrodynamic flare model with a high nonthermal electron beam flux, which explains a hot, T ≈ 104 K, color temperature at blue-to-red optical wavelengths and a small Balmer jump ratio as observed in moderate-sized and large flares alike. We also discuss the high time resolution, high signal-to-noise continuum color variations observed in YZ CMi during a giant flare, which increased the NUV flux from this star by over a factor of 100. Based on observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium, based on observations made with the William Herschel Telescope operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofsica de Canarias, and observations, and based on observations made with the ESO Telescopes at the La Silla Paranal Observatory under programme ID 085.D-0501(A).

SHORT-TERM EFFECTS OF SALINITY ON SOME PHYSIOLOGICAL PARAMETERS OF YOUNG OLIVE TREES OF ARBEQUINA, COBRANÇOSA AND GALEGA VARIETIES

SHORT-TERM EFFECTS OF SALINITY ON SOME PHYSIOLOGICAL PARAMETERS OF YOUNG OLIVE TREES OF ARBEQUINA, COBRANÇOSA AND GALEGA VARIETIES Ana Elisa Rato1,4, Renato Coelho1, Margarida Vaz1, Teresa Carola2, Dália Barbosa2, Nádia Silva1, José dos Santos2, Lourenço Machado2, João Godinho2, Luzia Ruas2, Margarida Barradas2, Hernani Pereira2, Sara Porfírio4 1 ICAAM, Universidade de Évora, Apartado 94, 7002-554 Évora, Portugal 2 Master students, Universidade de Évora, Apartado 94, 7002-554 Évora, Portugal 3 Ph.D. student, Universidade de Évora, Apartado 94, 7002-554 Évora, Portugal 4 aerato@uevora.pt Due to the desertification in some regions, the interest in plant’s tolerance to salinity has been increasing, as this response is determining for plant survival in stress conditions. This work reports the investigation of tolerance to salt in two year-old olive trees (Olea europaea L.) of three varieties, Arbequina, Cobrançosa and Galega vulgar. Plants were grown in 10 L plastic pots containing approximately 9 Kg of a sandy granitic soil, on a greenhouse. For 3 months (from the beginning of February to the end of April 2012), they were subjected to three levels of salinity in the irrigation water, 0 mM, 80 mM and 200 mM NaCl (6 plants per salinity level in a total of 18 plants of each variety),. Stomatal conductance (gs) and relative leaf chlorophyll content were assessed on each plant in February, March and April. Mid-day leaf water potential () and soil salinity were measured at the end of the experiment (April). On average, concerning all treatments and dates of determination, stomatal conductance of Arbequina and Galega vulgar was quite similar, around 40 mmol m-2 s-1, but Cobrançosa had a value of gs 36% higher, almost 50% higher (61 mmol m-2 s-1) when compared with the controls (0 mM salt) of the other two varieties. In percentage of controls, there was little difference in gs between varieties and between salinities during February and March. In contrast, in April, after about 90 days of exposure to salt, there was a clear decrease in gs with salt irrigation, proportional to salt concentration. Compared with controls, plants irrigated with 200 mM salt showed around 80% (Arbequina) or 85% (Cobrançosa and Galega vulgar) decrease in gs. Chlorophyll content of leaves showed less than 5% difference between varieties on the average of all treatments and dates of determination. During the course of this experiment, the salinity levels used did not show any relevant effect on chlorophyll content. Overall, at the end of the experimental period (April), leaf water potential () at midday was significantly higher in Cobrançosa (-1,4 MPa) than in Galega vulgar (-1,7 MPa) or Arbequina (-1,8 MPa), and salt decreased  of control plants (-1,25 MPa) by an average 30% (with 80 mM) and 65% (with 200 mM). At the end of the experiment, salinity in the soil irrigated with 0 mM, 80 mM or 200 mM NaCl was, on average of all varieties, 0,2 mS, 1,0 mS or 2,0 mS, respectively. Soil salinity was quite similar in Arbequina and Galega vulgar but about 35% lower in the pots of Cobrançosa, on average of all salt-irrigation levels. Plants of Cobrançosa had higher stomatal conductance, however they showed higher water potential and lower salinity in the soil. These apparently contradictory results seem to suggest that Cobrançosa responds to salt differently from the other two varieties. This issue needs further investigation.

Salinity-induced effects on transpiration rate, stomatal conductance and leaf area of three olive (Olea europaea L.) varieties

Transpiration of two year-old olive trees of three different varieties, Arbequina, Cobrançosa and Galega (18 trees per variety), irrigated with three levels of salt (0, 80 or 200 mM NaCl) for about 90 days, was measured by a gravimetric method. To determine leaf area, each tree was photographed from the side against a white background and the total area of each projected image was determined with ImageJ software. To calibrate these area determinations, one tree of each variety was subsequently stripped of all its leaves and its total leaf area was accurately measured. A correlation was then obtained between the area on the photograph of this particular tree and the total area of the detached leaves of the same tree. Using the leaf area determined by this procedure, transpiration rates of the trees could be calculated. Knowing leaf and air temperatures and RH, it was possible to determine the difference in molar fraction of water between the leaf and the air. Using this and the values of the transpiration rate, stomatal conductance could be calculated (gs calc) and compared with the conductance measured on the same trees with a porometer (gs). Actual leaf area of a plant was 1,40 (Arbequina), 1,42 (Cobrançosa) or 1,24 (Galega) times the area measured with ImageJ on the photograph of the same plant. Leaf area of the trees, on average of all salt irrigations, was significantly higher on Arbequina (0,187 m2) then on the other two varieties (0,138 m2 or 0,148 m2, for Cobrançosa or Galega, respectively), but did not differ significantly in percentage of controls (0 salt). On average of all three varieties, leaf area was also higher on plants irrigated without salt (0,181 m2) than on plants exposed to 80 or 200 mM NaCl (0,152 m2 or 0,140 m2, respectively), which did not differ between them. The same significant difference was observed when leaf area was expressed as percentage of controls. Transpiration rate was significantly higher on Cobrançosa (1,17 mmol m-2 s-1), on average of all treatments, but there were no significant differences between Arbequina (1,08 mmol m-2 s-1) and Galega (0,82 mmol m-2 s-1). In percentage of controls, there were no significant differences between varieties. Salt reduced significantly the transpiration rate in all varieties, both the actual and percentual values, to about 50% or 30% of controls when exposed to 80 mM or 200 mM NaCl, respectively. Stomatal conductance (gs), assessed by porometry, was significantly higher in control plants, mainly in Cobrançosa (102 mmol m-2 s-1), then in Arbequina (77 mmol m-2 s-1) and the lower values were found in Galega (51 mmol m-2 s-1). Salt reduced gs, on average of the three varieties to 30% or 10% of controls on exposure to 80 mM or 200 mM NaCl, respectively. Calculated (gs calc) and measured (gs) values of stomatal conductance showed a close relation between them (0,967, R2 = 0,837) which indicates this non-destructive method to determine whole-plant leaf area to be reasonably accurate.

Response to salinity in young olive trees of three Iberian varieties

Soil salinization is a problem in the Mediterranean region. This paper reports a research on the response to salt in two year-old olive trees (Olea europaea L.) of three Iberian varieties: Arbequina, Cobrançosa and Galega Vulgar. Plants were grown in plastic pots containing approximately 9 Kg of a sandy granitic soil, on a greenhouse at the University of Évora since February 2010. The experiment went from February to April 2012. As a rule, plants were watered every other day alternating salt solution (0 mM, 80 mM or 200 mM NaCl) or tap water. After three months irrigation with the different NaCl solutions, soil electric conductivity and soil water content were significantly higher on salt-irrigated pots. Salt also decreased significantly stomatal conductance (gs) and mid-day leaf water potential (), Cobrançosa having in general higher gs and but lower SLA than the two other varieties. Chlorophyll content of leaves was not affected by salt after this three months exposure to NaCl but was significantly higher on Arbequina and lower on Cobrançosa. In general, hyperspectral reflectance indexes did not show significant correlations with salt irrigation, except for the Photochemical Reflectance Index (PRI) which was clearly lower on plants of all three varieties irrigated with salt. Interestingly, Cobrançosa showed frequently vegetation indexes different from the other two varieties.

Determinant factors for the use of imposex in TBT pollution monitoring

Os compostos de tributilestanho (TBT) foram utilizados como biocidas em tintas antivegetativas (AV) e amplamente aplicados, durante décadas, de forma a evitar a bioincrustação em superfícies submersas, principalmente em cascos de embarcações. Os seus efeitos deletérios em organismos não-alvo tornaram-se evidentes após o aparecimento de gastrópodes prosobrâquios com imposex – sobreposição de caracteres sexuais masculinos sobre o tracto reprodutivo das fêmeas. Desde então, a expressão do imposex em prosobrânquios tem sido amplamente utilizada como biomarcador da poluição por TBT. Um dos objectivos da presente tese é avaliar se as mais recentes restrições legais na utilização das tintas AV com compostos organoestânicos (OTs) resultaram numa redução da poluição pelos mesmos na costa continental Portuguesa. Para tal, foi levada a cabo a análise da variação temporal do imposex como biomarcador dos níveis ambientais de TBT e a validação de procedimentos, de modo a seguir de forma precisa a evolução da intensidade deste fenómeno ao longo do tempo. O trabalho de investigação teve início no momento em que a ineficácia da legislação anterior (Directiva 89/677/CEE) na redução da poluição por TBT no litoral Português era reportada na literatura e quando estavam já agendados instrumentos decisivos para a diminuição definitiva deste tipo de poluição: o Regulamento (CE) N.º 782/2003 do Parlamento e do Conselho da União Europeia (UE) que bania as tintas AV baseadas em TBT na sua frota a partir de 1 de Julho de 2003; a "Convenção Internacional sobre o Controlo de Sistemas Antivegetativos Nocivos em Navios” (Convenção AFS), adoptada em 2001 pela Organização Marítima Internacional (OMI), que procurava erradicar os OTs da frota mundial até 2008. Os níveis de imposex e as concentrações de OTs nos tecidos de fêmeas de Nucella lapillus foram medidos em 17 locais de amostragem ao longo da costa Portuguesa em 2003, a fim de se avaliarem os impactos do TBT nas populações desta espécie e de se criar uma base de dados para seguir a sua evolução futura. O índice da sequência do vaso deferente (VDSI), o índice do tamanho relativo do pénis (RPSI) e a percentagem de fêmeas afectadas por imposex (%I) foram utilizados na medição da intensidade deste fenómeno em cada local de amostragem e os seus valores variaram entre 0,20-4,04, 0,0- 42,2% e 16,7-100,0%, respectivamente. Foram encontradas fêmeas estéreis em 3 locais de amostragem, com percentagens a variar entre 4,0 e 6,2%. As concentrações de TBT e dibutilestanho (DBT) nas fêmeas variaram respectivamente entre 23-138 e <10-62 ng Sn.g-1 de peso seco, e o conteúdo em TBT nos tecidos revelou-se significativamente correlacionado com o imposex (nomeadamente com o RPSI e o VDSI). Os níveis de expressão do fenómeno e o conteúdo em OTs nos tecidos, foram superiores na proximidade de portos, confirmando as conclusões obtidas anteriormente por outros autores de que os navios e a actividade dos estaleiros são as principais fontes destes compostos no litoral Português. As infra-estruturas associadas ás principais fontes de OTs – portos, estaleiros e marinas – estão geralmente localizadas no interior de estuários, motivo pelo qual estas áreas têm vindo a ser descritas como as mais afectadas por estes poluentes. Por esta razão, foi levado a cabo o estudo pormenorizado da poluição por TBT na Ria de Aveiro, como caso de estudo representativo da poluição por estes compostos num sistema estuarino em Portugal continental. N. lapillus foi usada como bioindicador para avaliar a tendência temporal da poluição por TBT nesta área entre 1997 e 2007. Foi registada uma diminuição da intensidade do imposex após 2003, embora as melhorias mais evidentes tenham sido observadas entre 2005 e 2007, provavelmente devido à implementação do Regulamento (CE) N.º 782/2003 que proibiu a aplicação de tintas AV com TBT em navios com a bandeira da UE. Apesar desses progressos, as análises ao conteúdo em OTs nos tecidos de fêmeas de N. lapillus e em amostras de água colhidas em 2006 indicaram contaminação recente por TBT na área de estudo, evidenciando assim a permanência de fontes de poluição. A utilização de N. lapillus como bioindicador da poluição por TBT na Ria de Aveiro apresenta algumas limitações uma vez que a espécie não ocorre nas áreas mais interiores da Ria e não vive em contacto com sedimentos. Assim, a informação obtida a partir da sua utilização como bioindicador é fundamentalmente relativa aos níveis de TBT na coluna de água. Foi então necessário recorrer a um bioindicador complementar – Hydrobia ulvae – para melhor avaliar a evolução temporal da poluição por TBT no interior deste sistema estuarino e estudar a persistência de TBT nos sedimentos. Não foi registada uma diminuição dos níveis de imposex em H. ulvae na Ria de Aveiro entre 1998 e 2007, apesar da aplicação do Regulamento (CE) N.º 782/2003. Pelo contrário, houve um aumento global significativo da percentagem de fêmeas afectadas por imposex e um ligeiro aumento do VDSI, contrastando com o que tem sido descrito para outros bioindicadores na Ria de Aveiro no mesmo período. Estes resultados mostram que a diferente biologia/ecologia das espécies indicadoras determina vias distintas de acumulação de TBT, apontando a importância da escolha do bioindicador dependendo do compartimento a ser monitorizado (sedimento versus água). A ingestão de sedimento como hábito alimentar em H. ulvae foi discutida como sendo a razão para a escolha da espécie como indicadora da contaminação dos sedimentos por TBT. Foram também estudados os métodos mais fiáveis para reduzir a influência de variáveis críticas na medição dos níveis de imposex em H. ulvae. As comparações de parâmetros do imposex baseados em medições do pénis devem ser sempre realizadas sob condições de narcotização bem standardizadas uma vez que este procedimento provoca um aumento significativo do comprimento do pénis (PL) em ambos os sexos. O VDSI, a % e o PL em ambos os sexos revelaram ser fortemente influenciados pelo tamanho dos espécimes: a utilização de fêmeas mais pequenas conduz à subestimação do VDSI, da %I e do PL, enquanto que diferenças no tamanho dos machos provocam variações no índice do comprimento relativo do pénis (RPLI), independentemente dos níveis de poluição por TBT. Existe, portanto, a necessidade de controlar algumas variáveis envolvidas na análise do imposex que mostraram afectar a fiabilidade dos resultados. Uma vez que N. lapillus é o principal bioindicador dos efeitos biológicos específicos do TBT para a área da OSPAR, foi também estudada a influência de algumas variáveis na avaliação dos níveis de imposex nesta espécie, especificamente as relacionadas com o ciclo reprodutor e o tamanho dos espécimes. O estudo do ciclo reprodutor e a variação sazonal/espacial do comprimento do pénis do macho (MPL) incidiu num único local no litoral Português (Areão – região de Aveiro) de forma a avaliar se o RPSI varia sazonal e espacialmente na mesma estação de amostragem e se tais variações influenciam os resultados obtidos em programas de monitorização do imposex. Nos meses de Dezembro de 2005 a Junho de 2007, foram encontrados espécimes de N. lapillus sexualmente maturos e potencialmente aptos para a reprodução. Contudo, foi também evidente um padrão sazonal do ciclo reprodutor – o estado de desenvolvimento da gametogénese nas fêmeas variou sazonalmente e ocorreu uma diminuição do volume da glândula da cápsula e do factor de condição no final do Verão / início do Outono. Contrariamente, a gametogénese nos machos não apresentou variação sazonal significativa, embora os valores mais baixos do factor de condição, do comprimento do pénis e dos volumes de esperma e da próstata tenham também sido registados no final do Verão / início do Outono. Além disso, o MPL mostrou variar, no mesmo local de amostragem, inversamente com a distância aos ninhos de cápsulas ovígeras; um aumento dos valores do MPL foi também observado em espécimes de maior tamanho. Todas estas variações no MPL introduzem desvios nos resultados da avaliação do imposex quando é usado o RPSI. A magnitude do erro envolvido foi quantificada e revelou-se superior em locais com níveis mais elevados de poluição por TBT. Apesar do RPSI ser um índice que fornece informação importante sobre os níveis de poluição por TBT, a sua interpretação deve ser cuidadosa e realizada complementarmente com os outros índices, destacando-se o VDSI como índice mais fiável e com significado biológico mais expressivo. Novas campanhas de monitorização do imposex em N. lapillus foram realizadas ao longo da costa Portuguesa em 2006 e 2008, e os resultados subsequentemente comparados com a base de dados criada em 2003,de forma a avaliar a evolução da poluição por TBT no litoral Português naquele período. Nestes estudos foram aplicados novos procedimentos na monitorização e tratamento dos dados, de forma a minimizar a variação nos índices de avaliação do imposex induzida pelos factores acima descritos, para seguir com maior consistência a tendência da poluição por TBT entre 2003 e 2008. Foi observado um declínio global significativo na intensidade de imposex na área de estudo durante o referido período e a qualidade ecológica da costa Portuguesa, segundo os termos definidos pela Comissão OSPAR, revelou melhorias notáveis após 2003 confirmando a eficácia do Regulamento (CE) N.º 782/2003. Não obstante, as populações de N. lapillus revelaram-se ainda amplamente afectadas por imposex, tendo sido detectadas emissões de TBT na água do mar ao longo da costa em 2006, apesar da restrição anteriormente referida. Estes inputs foram atribuídos principalmente aos navios que à data ainda circulavam com tintas AV com TBT aplicadas antes de 2003, uma vez que a sua utilização nas embarcações foi apenas proibida em 2008. Considerando que o Regulamento (CE) N.º 782/2003 constitui uma antecipação da proibição global da OMI que entrou em vigor em Setembro de 2008, prevê-se, por analogia, que haja uma rápida diminuição da poluição por TBT à escala mundial num futuro próximo. Na sequência desta previsão, é apresentada uma discussão teórica preliminar relativamente ás possíveis estratégias usadas por N. lapillus na recolonização de locais onde, no passado, as populações terão aparentemente sido extintas devido a níveis extremamente elevados de TBT. Estes locais são tipicamente zonas abrigadas junto de infra-estruturas portuárias, cuja recolonização por esta espécie será provavelmente muito lenta dada a mobilidade reduzida dos adultos e o ciclo de vida não apresentar fase larvar pelágica. Foram então equacionadas duas hipotéticas vias de recolonização de zonas abrigadas por espécimes provenientes de populações de costa aberta/exposta: a migração de adultos e/ou a dispersão de juvenis. No entanto, em ambos os casos, estaria implicada a transposição de um problema amplamente descrito na bibliografia: as populações de N. lapillus de costa aberta podem apresentar um fenótipo muito diferente das de zonas abrigadas, podendo inclusivamente variar no número de cromossomas. A recolonização pode portanto não ter sucesso pelo simples facto dos novos recrutas não estarem bem adaptados aos locais a recolonizar. Para analisar este problema, foram estudados tanto a forma da concha de espécimes de N. lapillus ao longo da costa Portuguesa como o respectivo número de cromossomas. Embora a forma da concha tenha revelado diferenças, de acordo com o grau de hidrodinamismo entre as populações de N. lapillus avaliadas, o cariótipo 2n = 26, típico de zonas expostas, foi registado em todos os locais amostrados. Por outro lado, foi também testada em laboratório a possível mortalidade de juvenis em dispersão no interior menos salino dos estuários. Foi então verificada a ocorrência de mortalidade elevada de juvenis expostos a salinidades baixas (=100% após 1 hora a salinidades ≤9 psu), o que também pode comprometer a recolonização de zonas estuarinas menos salinas por esta via. Mesmo assim, os juvenis mostraram um comportamento de flutuação à superfície da água em condições laboratoriais, que pode ser considerado um benefício específico na colonização de áreas mais internas dos estuários, se tal facto vier a ser confirmado em estudos de campo. As conclusões deste estudo contribuem certamente para a descrição do final da “história do TBT” dado que, uma vez controlados alguns factores determinantes no uso do imposex como biomarcador, a avaliação do declínio da poluição por estes compostos, agora esperado à escala global, se torna mais rigorosa.