A finite volume unstructured mesh approach to dynamic fluid–structure interaction: an assessment of the challenge of predicting the onset of flutter

Computational modelling of dynamic fluid–structure interaction (DFSI) is a considerable challenge. Our approach to this class of problems involves the use of a single software framework for all the phenomena involved, employing finite volume methods on unstructured meshes in three dimensions. This method enables time and space accurate calculations in a consistent manner. One key application of DFSI simulation is the analysis of the onset of flutter in aircraft wings, where the work of Yates et al. [Measured and Calculated Subsonic and Transonic Flutter Characteristics of a 45° degree Sweptback Wing Planform in Air and Freon-12 in the Langley Transonic Dynamic Tunnel. NASA Technical Note D-1616, 1963] on the AGARD 445.6 wing planform still provides the most comprehensive benchmark data available. This paper presents the results of a significant effort to model the onset of flutter for the AGARD 445.6 wing planform geometry. A series of key issues needs to be addressed for this computational approach. • The advantage of using a single mesh, in order to eliminate numerical problems when applying boundary conditions at the fluid-structure interface, is counteracted by the challenge of generating a suitably high quality mesh in both the fluid and structural domains. • The computational effort for this DFSI procedure, in terms of run time and memory requirements, is very significant. Practical simulations require even finer meshes and shorter time steps, requiring parallel implementation for operation on large, high performance parallel systems. • The consistency and completeness of the AGARD data in the public domain is inadequate for use in the validation of DFSI codes when predicting the onset of flutter.

Architecture in Cinema: A Relation of Representation Based on Space

Architecture, whether in the foreground or background, is an intrinsic part of any film, and cinema holds a position as a transformative reference in contemporary architecture. This book addresses the role of architecture in cinema, and through a focus on the use of space, it presents a critical overview of the relation between the two. Through framing, flattening and editing, cinematic space, as the representation of architectural space, focuses on its certain qualities, while eliminating others. Thus, cinema emphasizes individual aspects of space that may be overlooked when the whole context is considered. Space 'acts' in the foreground rather than simply filling the background in the films of Peter Greenaway and Wim Wenders, which are used to analyze two significant cinematic approaches to space, space as form and space as symbol. The detailed analysis of Greenaway's The Belly of an Architect and Wenders' Der Himmel über Berlin (Wings of Desire) offers an innovative and original perspective on space to those interested in both fields of architecture and film studies.

Validation study for prediction of iced aerofoil aerodynamics

Ice accretions can significantly change the aerodynamic performance of wings and rotor blades. Significant performance degradation can occur when ice accreations cause regions of separated flow, to predict this change implies, at a minimum, the solution of the Reynolds-Averaged Navier-Stokes equations. This paper presents validation for two generic cases involving the flow over aerofoil sections with added synthetic ice shapes. Results were obtained for two aerofoils, namely the NACA 23012 and a generic multi-element configuration. These results are compared with force and pressure coefficient measurements obtained in the NASA LTPT wind-tunnel for the NACA 23012, and force, PIV and boundary-layer measurements obtained at DNW for the multi-clement case. The level of agreement is assessed in the context of industrial requirements.

Multidimensional modelling of X-ray spectra for AGN accretion disc outflows

We use a multidimensional Monte Carlo code to compute X-ray spectra for a variety of active galactic nucleus (AGN) disc-wind outflow geometries. We focus on the formation of blueshifted absorption features in the Fe K band and show that line features similar to those which have been reported in observations are often produced for lines of sight through disc-wind geometries. We also discuss the formation of other spectral features in highly ionized outflows. In particular, we show that, for sufficiently high wind densities, moderately strong Fe K emission lines can form and that electron scattering in the flow may cause these lines to develop extended red wings. We illustrate the potential relevance of such models to the interpretation of real X-ray data by comparison with observations of a well-known AGN, Mrk 766. Journal compilation © 2008 RAS.

Mimicking the colourful wing scale structure of the Papilio blumei butterfly

The brightest and most vivid colours in nature arise from the interaction of light with surfaces that exhibit periodic structure on the micro- and nanoscale. In the wings of butterflies, for example, a combination of multilayer interference, optical gratings, photonic crystals and other optical structures gives rise to complex colour mixing. Although the physics of structural colours is well understood, it remains a challenge to create artificial replicas of natural photonic structures(1-3). Here we use a combination of layer deposition techniques, including colloidal self-assembly, sputtering and atomic layer deposition, to fabricate photonic structures that mimic the colour mixing effect found on the wings of the Indonesian butterfly Papilio blumei. We also show that a conceptual variation to the natural structure leads to enhanced optical properties. Our approach offers improved efficiency, versatility and scalability compared with previous approaches(4-6).

Electrostatic supersolitons in three-species plasmas

Superficially, electrostatic potential profiles of supersolitons look like those of traditional solitons. However, their electric field profiles are markedly different, having additional extrema on the wings of the standard bipolar structure. This new concept was recently pointed out in the literature for a plasma model with five species. Here, it is shown that electrostatic supersolitons are not an artefact of exotic, complicated plasma models, but can exist even in three-species plasmas and are likely to occur in space plasmas. Further, a methodology is given to delineate their existence domains in a systematic fashion by determining the specific limiting factors. © 2013 American Institute of Physics.

Ellerman Bombs - Evidence for Magnetic Reconnection in the Lower Solar Atmosphere

The presence of photospheric magnetic reconnection has long been thought to give rise to short and impulsive events, such as Ellerman bombs (EBs) and Type II spicules. In this article, we combine high-resolution, high-cadence observations from the Interferometric BIdimensional Spectrometer and Rapid Oscillations in the Solar Atmosphere instruments at the Dunn Solar Telescope, National Solar Observatory, New Mexico, with co-aligned Solar Dynamics Observatory Atmospheric Imaging Assembly and Hinode Solar Optical Telescope (SOT) data to observe small-scale events situated within an active region. These data are then compared with state-of-the-art numerical simulations of the lower atmosphere made using the MURaM code. It is found that brightenings, in both the observations and the simulations, of the wings of the Hα line profile, interpreted as EBs, are often spatially correlated with increases in the intensity of the Fe I λ6302.5 line core. Bipolar regions inferred from Hinode/SOT magnetic field data show evidence of flux cancellation associated, co-spatially, with these EBs, suggesting that magnetic reconnection could be a driver of these high-energy events. Through the analysis of similar events in the simulated lower atmosphere, we are able to infer that line profiles analogous to the observations occur co-spatially with regions of strong opposite-polarity magnetic flux. These observed events and their simulated counterparts are interpreted as evidence of photospheric magnetic reconnection at scales observable using current observational instrumentation.

The Influence of Structural Modeshape Variability on Limit Cycle Oscillation Behaviour

Modal analysis is a popular approach used in structural dynamic and aeroelastic problems due to its efficiency. The response of a structure is compo
sed of the sum of orthogonal eigenvectors or modeshapes and corresponding modal frequencies. This paper investigates the importance of modeshapes on the aeroelastic response of the Goland wing subject to structural uncertainties. The wing undergoes limit cycle oscillations (LCO) as a result of the inclusion of polynomial stiffness nonlinearities. The LCO computations are performed using a Harmonic Balance approach for speed, the modal properties of the system are extracted from MSC NASTRAN. Variability in both the wing’s structure and the store centre of gravity location is investigated in two cases:- supercritical and subcritical type LCOs. Results show that the LCO behaviour is only sensitive to change in modeshapes when the nature of the modes are changing significantly.

The NOTCH signaling pathway in normal and malignant blood cell production

The NOTCH pathway is an evolutionarily conserved signalling network, which is fundamental in regulating developmental processes in invertebrates and vertebrates (Gazave et al. in BMC Evol Biol 9:249, 2009). It regulates self-renewal (Butler et al. in Cell Stem Cell 6:251–264, 2010), differentiation (Auderset et al. in Curr Top Microbiol Immunol 360:115–134, 2012), proliferation (VanDussen et al. in Development 139:488–497, 2012) and apoptosis (Cao et al. in APMIS 120:441–450, 2012) of diverse cell types at various stages of their development. NOTCH signalling governs cell-cell interactions and the outcome of such responses is highly context specific. This makes it impossible to generalize about NOTCH functions as it stimulates survival and differentiation of certain cell types, whereas inhibiting these processes in others (Meier-Stiegen et al. in PLoS One 5:e11481, 2010). NOTCH was first identified in 1914 in Drosophila and was named after the indentations (notches) present in the wings of the mutant flies (Bigas et al. in Int J Dev Biol 54:1175–1188, 2010). Homologs of NOTCH in vertebrates were initially identified in Xenopus (Coffman et al. in Science 249:1438–1441, 1990) and in humans NOTCH was first identified in T-Acute Lymphoblastic Leukaemia (T-ALL) (Ellisen et al. in Cell 66:649–61, 1991). NOTCH signalling is integral in neurogenesis (Mead and Yutzey in Dev Dyn 241:376–389, 2012), myogenesis (Schuster-Gossler et al. in Proc Natl Acad Sci U S A 104:537–542, 2007), haematopoiesis (Bigas et al. in Int J Dev Biol 54:1175–1188, 2010), oogenesis (Xu and Gridley in Genet Res Int 2012:648207, 2012), differentiation of intestinal cells (Okamoto et al. in Am J Physiol Gastrointest Liver Physiol 296:G23–35, 2009) and pancreatic cells (Apelqvist et al. in Nature 400:877–881, 1999). The current review will focus on NOTCH signalling in normal and malignant blood cell production or haematopoiesis.

The Dynamics of Rapid Redshifted and Blueshifted Excursions in the Solar Hα Line

We analyze high temporal and spatial resolution time-series of spectralscans of the Hα line obtained with the CRisp Imaging SpectroPolarimeter instrument mounted on the Swedish Solar Telescope.The data reveal highly dynamic, dark, short-lived structures known asRapid Redshifted and Blueshifted Excursions (RREs, RBEs) that areon-disk absorption features observed in the red and blue wings ofspectral lines formed in the chromosphere. We study the dynamics of RREsand RBEs by tracking their evolution in space and time, measuring thespeed of the apparent motion, line of sight (LOS) Doppler velocity, andtransverse velocity of individual structures. A statistical study oftheir measured properties shows that RREs and RBEs have similaroccurrence rates, lifetimes, lengths, and widths. They also displaynon-periodic, nonlinear transverse motions perpendicular to their axesat speeds of 4-31 km s-1. Furthermore, both typesof structures either appear as high speed jets and blobs that aredirected outwardly from a magnetic bright point with speeds of50-150 km s-1, or emerge within a few seconds. Astudy of the different velocity components suggests that the transversemotions along the LOS of the chromospheric flux tubes are responsiblefor the formation and appearance of these redshifted/blueshiftedstructures. The short lifetime and fast disappearance of the RREs/RBEssuggests that, similar to type II spicules, they are rapidly heated totransition region or even coronal temperatures. We speculate that theKelvin-Helmholtz instability triggered by observed transversemotions of these structures may be a viable mechanism for their heating.

Statistical Analysis of Small Ellerman Bomb Events

The properties of Ellerman bombs (EBs), small-scale brightenings in the Hα line wings, have proved difficult to establish because their size is close to the spatial resolution of even the most advanced telescopes. Here, we aim to infer the size and lifetime of EBs using high-resolution data of an emerging active region collected using the Interferometric BIdimensional Spectrometer (IBIS) and Rapid Oscillations of the Solar Atmosphere (ROSA) instruments as well as the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO). We develop an algorithm to track EBs through their evolution, finding that EBs can often be much smaller (around 0.3″) and shorter-lived (less than one minute) than previous estimates. A correlation between G-band magnetic bright points and EBs is also found. Combining SDO/HMI and G-band data gives a good proxy of the polarity for the vertical magnetic field. It is found that EBs often occur both over regions of opposite polarity flux and strong unipolar fields, possibly hinting at magnetic reconnection as a driver of these events.The energetics of EB events is found to follow a power-law distribution in the range of a nanoflare (1022-25 ergs).

On the progenitor of the Type Ic SN 2013dk in the Antennae galaxies

We report the results of our search for the progenitor candidate of SN 2013dk, a Type Ic supernova (SN) that exploded in the Antennae galaxy system. We compare pre-explosion Hubble Space Telescope (HST) archival images with SN images obtained using adaptive optics at the ESO Very Large Telescope. We isolate the SN position to within 3σ uncertainty radius of 0.02 arcsec and show that there is no detectable point source in any of the HST filter images within the error circle. We set an upper limit to the absolute magnitude of the progenitor to be MF555W ≳ -5.7, which does not allow Wolf-Rayet (WR) star progenitors to be ruled out. A bright source appears 0.17 arcsec away, which is either a single bright supergiant or compact cluster, given its absolute magnitude of MF555W = -9.02 ± 0.28 extended wings and complex environment. However, even if this is a cluster, the spatial displacement of SN 2013dk means that its membership is not assured. The strongest statement that we can make is that in the immediate environment of SN 2013dk (within 10 pc or so), we find no clear evidence of either a point source coincident with the SN or a young stellar cluster that could host a massive WR progenitor.

Bursaphelenchus pinophilus Brzeski & Baujard, 1997 (Nematoda: Parasitaphelenchinae) associated with nematangia on Pityogenes bidentatus (Herbst, 1783) (Coleoptera: Scolytinae), from the Czech Republic

The occurrence of Bursaphelenchus species in the Czech Republic is poorly known, the first report of the genus being made by Kubátová et al. (2000) who reported the association of B. eremus with the hyphomycetous microfungus, Esteya vermicola, and the bark beetle, Scolytus intricatus, collected from Quercus robur, in central Bohemia. To date, four other species have been reported from the country, namely B. fungivorus (Braasch et al., 2002), B. hofmanni (see Braasch, 2001), B. mucronatus (see Braasch, 2001) and B. vallesianus (Gaar et al., 2006). More recently, a survey for Bursaphelenchus species associated with bark- and wood-boring insects in the Czech Republic identified B. pinophilus Brzeski & Baujard, 1997 from the Moravia region. Although this represents a new country record, it was also associated with nematangia on the hind wings of a new insect vector. A total of 404 bark- and wood-boring insects were collected from declining or symptomatic trees and screened for the presence of Bursaphelenchus. Bark and longhorn beetles were captured manually after debarking parts of the trunk displaying symptoms of insect attacks. Longhorn beetle larvae were also collected together with logs cut from the trunk. Logs were kept at room temperature in the laboratory until insect emergence. Each adult insect was individually dissected in water and examined for nematodes. All nematodes resembling dauer juveniles of Bursaphelenchus were collected and identified by molecular characterisation using a region of ribosomal DNA (rDNA) containing the internal transcribed spacer regions ITS1 and ITS2. ITS-RFLP analyses using five restriction enzymes (AluI, HaeIII, HinfI, MspI, RsaI) were performed to generate the species-specific profile according to Burgermeister et al. (2009). Species identification was also confirmed by morphological data after culture of the dauers on Botrytis cinerea Pers. ex Ft., growing in 5% malt extract agar. During this survey, only species belonging to the Curculionidae, subfamily Scolytinae, revealed the presence of nematodes belonging to Bursaphelenchus. Dauers of this genus were found aggregated under the elytra in nematangia formed at the root of the hind wings (Fig. 1). The dauers were identified from 12 individuals of Pityogenes bidentatus (Herbst, 1783) (Coleoptera: Scolytinae) collected under the bark of Pinus sylvestris trunks. Each insect carried ca 10-100 dauers. The ITS-RFLP patterns of the dauers so obtained confirmed the identification of B. pinophilus associated with this insect species. Bursaphelenchus pinophilus has been found mainly in Europe and has been reported from various countries such as Poland (Brzeski & Baujard, 1997), Germany (Braasch, 2001), and Portugal (Penas et al., 2007). The recent detection of this species associated with dead P. koraiensis in Korea (Han et al., 2009) expands its geographical distribution and potential importance. It has been found associated only with Pinus species, but very little is known about the insect vector. The bark beetle, Hylurgus ligniperda, was initially suggested as the insect vector by Pe-nas et al. (2006), although the nematode associated with this insect was later reclassified as B. sexdentati by morphological and molecular analysis (Penas et al., 2007). According to the literature, P. bidentatus has been cited as a vector of Ektaphelenchus sp. (Kakuliya, 1966) in Georgia, and an unidentified nematode species in Spain (Roberston et al., 2008). Interestingly, B. pinophilus was found in the nematangia formed at the root of the hind wings of P. bidentatus. Although this phenomenon is not so common in other Bursaphelenchus species, B. rufipennis has been found recently in such a structure on the hind wings of the insect Dendroctonus rufipennis (Kanzaki et al., 2008). Although other nematode species (e.g., Ektaphelenchus spp.) are frequently found associated within the same nematangia (see Kanzaki et al., 2008), in this particular case, only dauers of B. pinophilus were identified. The association between B. pinophilus and P. bidentatus represents the first report of this biological association and the association with the Scolytinae strengthens the tight and specific links between this group of Bursaphelenchus species and members of the Scolytinae (Ryss et al., 2005).

Morphobiometric and molecular characterization of Bursaphelenchus Fuchs, 1937 (Nematoda: Aphelenchoididae) species associated with Pinus pinaster Ainton in Portugal

Abstract - The genus Bursaphelenchus comprises almost 100 species mainly from the northern hemisphere, with conifers as the most important hosts. Among the various nematode species, the pine wood nematode (PWN), Bursaphelenchus xylophilus, is the casual agent of pine wilt disease (PWD), and the most important forest pest for pines worldwide, classified as an A1 quarantine organism within the European Union. In 1999 this nematode was detected for the first time in Portugal and Europa associated with maritime pine, Pinus pinaster. Following detection, a national program denominated "Programa Nacional de Luta contra o Nemátodo da Madeira do Pinheiro" (PROLUNP) was created to, among other objectives, determine the distribution of the PWN and its associated vector(s) and host(s), and therefore intensive surveys covering the entire country were conducted with thousands of wood samples and suspected insects being analyzed. This thesis presents the listing, distribution, frequency and the insects associated with Bursaphelenchus species found associated with maritime pine in Portugal, identifying and characterizing the various species by morphological, biometrical and molecular biology (ITS-RFLP and rDNA sequencing analysis) techniques. To achieve the objectives, a total of 4813 maritime pine wood samples and 3294 insects from 22 species and six families were individually analyzed. A total of nine Bursaphelenchus species were found, namely: B. antoniae, B. hellenicus, B. leoni, B. mucronatus, B. pinasteri, B. sexdentati, B. teratospicularis, B. tusciae and B. xylophilus, all of them (with the exception of B. xylophilus) being new records for Portugal. Some of the species appear to have a widespread distribution, such as B. leoni, B. teratospicularis and B. tusciae while others were very rarely found and apparently have a localized distribution range within the country, namely B. antoniae and B. mucronatus. The majority of the species is characteristic of the Mediterranean region and can also be found in countries such as Spain, Italy and Greece, reflecting the affinity of our fauna with those locations. The association of B. hellenicus and B. tusciae with maritime pine is here reported for the first time. Six of the Bursaphelenchus species were also found associated with insects, mainly from the family Scolytidae (Coleoptera). Some of these interactions were described for the first time, namely: B. hellenicus with both Ips sexdentatus and Hylurgus ligniperda, B. sexdentati with both H. ligniperda and Orthotomicus erosus and B. tusciae with H. ligniperda. The exclusive association of B. xylophilus with the cerambycid Monochamus galloprovincialis was also confirmed. The nematode's dauer juveniles were usually found in low numbers in the insect vectors (ca 10-100 per insect), although for B. xylophilus a few thousand specimens per insect were sometimes found. The location of the dauer juveniles differed according to the species, although they were more common under the elytra and wings of the adult insects. A species new to science was detected and formally described as B. antoniae, associated with Hylobius sp. (Coleoptera; Curculionidae) beetles. Morphologically, this new species is very similar to B. hylobianum, although it's distinct ITS-RFLP molecular pattern (with only the enzyme Haelll producing comparable restriction bands) and the failure of hybridization supported the two species as distinct entities. Additional phylogenetic analysis of the 18S rDNA sequence further supported the taxonomical proximity of B. antoniae with B. hylobianum. Concerning the PWN, detailed studies on the development and morphology of B. xylophilus were conducted, and comparative measurements of field-collected and laboratory-maintained populations demonstrated that nematodes from the second group displayed larger size in all morphometric parameters, which could derive from more adequate conditions of nourishment and/or temperature. Taxonomical studies on the development stages of B. xylophilus confirmed the existence of four propagative juvenile stages (J1,J2,J3 and J4), an adult stage with both sexes and two dispersal stages (jIII e jIV), with the measurements of the gonad length allowing the separation of the propagative stages. It is hoped that the acquired knowledge will be useful on future surveys of nematodes of the Bursaphelenchus genus collected from either wood material or insect vectors, and facilitate the correct distinction and identification of the various species which are now known to occur. ### Resumo - 0 género Bursaphelenchus compreende quase 100 espécies, distribuídas sobretudo nos países do hemisfério norte do globo terrestre. Embora algumas espécies já tenham sido detectadas em plantas herbáceas, os hospedeiros vegetais mais comuns deste género são as coníferas, particularmente pinheiros. 0 nemátode da madeira do pinheiro (NMP), Bursaphelenchus xylophilus, é considerado a espécie mais importante deste género uma vez que é o agente causal da doença da murchidão dos pinheiros ("pine wilt disease"). Originário dos Estados Unidos, onde não causa grande impacte, o NMP foi introduzido em alguns países da Ásia (China, Japão, Coreia e Taiwan) e mais recentemente na Europa (Portugal). Nestas regiões é responsável pela destruição de milhares de hectares de coníferas, assumindo uma elevada importância económica. Em Portugal, depois da sua detecção em 1999, associado a Pinus pinaster, foi implementado um programa nacional "Programa Nacional de Luta contra o Nemátodo da Madeira do Pinheiro" (PROLUNP) que permitiu determinar a área afectada pela praga (a sul do rio Tejo, península de Setúbal) bem como definir e implementar estratégias de controlo e prevenção da disseminação do NMP a outras zonas de Portugal. Recentemente, em Junho de 2008, foi confirmada a presença de B. xylophilus em outras regiões de Portugal levando as autoridades oficiais a definir todo o território continental como zona afectada e de restrição. As prospecções intensivas realizadas nos últimos anos incluíram a recolha e análise de milhares de amostras de madeira de pinheiro bem como de insectos associados ao pinheiro bravo conduzindo à identificação de várias espécies de Bursaphelenchus. Assim, os estudos conduzidos neste trabalho tiveram como objectivos efectuar uma caracterização morfológica, biométrica e molecular das espécies associadas a P. pinaster em Portugal bem como a sua distribuição geográfica e abundância. Os estudos biométricos foram realizados com populações extraídas directamente do meio natural. Foi ainda realizada uma pesquisa que permitiu identificar os insectos a que estão associadas essas espécies, os seus possíveis vectores. Foram analisadas no total 4813 amostras de P. pinaster e 3294 insectos (22 espécies pertencentes a seis famílias diferentes). Foram identificadas um total de nove espécies: B. antoniae n. sp., B. hellenicus, B. leoni, B. mucronatus, B. pinasteri, B. sexdentati, B. teratospicularis, B. tusciae e B. xylophilus. Foram realizados estudos morfológicos e biométricos de todas as espécies com excepção de B. mucronatus; o reduzido número de exemplares encontrados em apenas uma amostra foram utilizados para efectuar o diagnóstico molecular desta espécie (ITS-RFLP). Apesar de ter havido, sempre que possível, a confirmação molecular, na maioria dos casos a caracterização morfológica e biométrica permitiu a correcta identificação das espécies. Contudo, foi imprescindível a análise molecular em algumas amostras, nomeadamente para a identificação de B. xylophilus e B. sexdentati; dada a grande semelhança entre B. xylophilus e B. mucronatus e tendo sido encontradas algumas populações de B. xylophilus que possuíam fêmeas com cauda mucronada, foi necessária a realização da confirmação molecular. Com excepção de B. xylophilus, todas as outras espécies foram reportadas pela primeira vez em Portugal. Juntamente com B. xylophilus, B. pinasteri foi a espécie encontrada nas amostras de madeira de pinheiro com maior frequência. Algumas destas espécies como B. leoni, B. teratospicularis e B. tusciae foram reportadas em diferentes localidades do norte, centro e sul de Portugal, apresentando uma vasta distribuição geográfica; este resultado está em consonância com a forte associação destas espécies a climas mediterrânicos tal como acontece em Espanha, França, Itália e Grécia. Em oposição, espécies como B. antoniae e B. mucronatus foram encontradas apenas numa ocasião na região centro (Leiria) e norte (Figueira da Foz) do país, respectivamente. Bursaphelenchus mucronatus é igualmente pouco frequente em Espanha onde ocorre sobretudo na região norte, na Galiza. Esta espécie preferirá climas mais frios, ocorrendo com uma maior frequência nas regiões de latitude norte; esta análise é corroborada pela presença constante em países como Alemanha, Finlândia, França, Noruega, Rússia e Suécia. A nível mundial são descritas neste trabalho pela primeira vez as associações das espécies B. hellenicus e B. tusciae ao hospedeiro vegetal P. pinaster.

Non-linear analysis of piezolaminated structures

In the recent years the study of smart structures has attracted significant researchers, due to their potential benefits in a wide range of applications, such as shape control, vibration suppression, noise attenuation and damage detection. The applications in aerospace industry are of great relevance, such as in active control of airplane wings, helicopter blade rotor, space antenna. The use of smart materials, such as piezoelectric materials, in the form of layers or patches embedded and/or surface bonded on laminated composite structures, can provide structures that combine the superior mechanical properties of composite materials and the capability to sense and adapt their static and dynamic response, becoming adaptive structures. The piezoelectric materials have the property of generate electrical charge under mechanical load or deformation, and the reverse, applying an electrical field to the material results in mechanical strain or stresses.