Não-extensividade no contexto da atividade magnética solar: o problema da assimetria hemisférica

Solar activity indicators, each as sunspot numbers, sunspot area and flares, over the Sun’s photosphere are not considered to be symmetric between the northern and southern hemispheres of the Sun. This behavior is also known as the North-South Asymmetry of the different solar indices. Among the different conclusions obtained by several authors, we can point that the N-S asymmetry is a real and systematic phenomenon and is not due to random variability. In the present work, the probability distributions from the Marshall Space Flight Centre (MSFC) database are investigated using a statistical tool arises from well-known Non-Extensive Statistical Mechanics proposed by C. Tsallis in 1988. We present our results and discuss their physical implications with the help of theoretical model and observations. We obtained that there is a strong dependence between the nonextensive entropic parameter q and long-term solar variability presents in the sunspot area data. Among the most important results, we highlight that the asymmetry index q reveals the dominance of the North against the South. This behavior has been discussed and confirmed by several authors, but in no time they have given such behavior to a statistical model property. Thus, we conclude that this parameter can be considered as an effective measure for diagnosing long-term variations of solar dynamo. Finally, our dissertation opens a new approach for investigating time series in astrophysics from the perspective of non-extensivity.

Análise wavelet e modelo de manchas em curvas de luz estelares dos telescópios espaciais Kepler e CoRoT

Analogous to sunspots and solar photospheric faculae, which visibility is modulated by stellar rotation, stellar active regions consist of cool spots and bright faculae caused by the magnetic field of the star. Such starspots are now well established as major tracers used to estimate the stellar rotation period, but their dynamic behavior may also be used to analyze other relevant phenomena such as the presence of magnetic activity and its cycles. To calculate the stellar rotation period, identify the presence of active regions and investigate if the star exhibits or not differential rotation, we apply two methods: a wavelet analysis and a spot model. The wavelet procedure is also applied here to study pulsation in order to identify specific signatures of this particular stellar variability for different types of pulsating variable stars. The wavelet transform has been used as a powerful tool for treating several problems in astrophysics. In this work, we show that the time-frequency analysis of stellar light curves using the wavelet transform is a practical tool for identifying rotation, magnetic activity, and pulsation signatures. We present the wavelet spectral composition and multiscale variations of the time series for four classes of stars: targets dominated by magnetic activity, stars with transiting planets, those with binary transits, and pulsating stars. We applied the Morlet wavelet (6th order), which offers high time and frequency resolution. By applying the wavelet transform to the signal, we obtain the wavelet local and global power spectra. The first is interpreted as energy distribution of the signal in time-frequency space, and the second is obtained by time integration of the local map. Since the wavelet transform is a useful mathematical tool for nonstationary signals, this technique applied to Kepler and CoRoT light curves allows us to clearly identify particular signatures for different phenomena. In particular, patterns were identified for the temporal evolution of the rotation period and other periodicity due to active regions affecting these light curves. In addition, a beat-pattern vii signature in the local wavelet map of pulsating stars over the entire time span was also detected. The second method is based on starspots detection during transits of an extrasolar planet orbiting its host star. As a planet eclipses its parent star, we can detect physical phenomena on the surface of the star. If a dark spot on the disk of the star is partially or totally eclipsed, the integrated stellar luminosity will increase slightly. By analyzing the transit light curve it is possible to infer the physical properties of starspots, such as size, intensity, position and temperature. By detecting the same spot on consecutive transits, it is possible to obtain additional information such as the stellar rotation period in the planetary transit latitude, differential rotation, and magnetic activity cycles. Transit observations of CoRoT-18 and Kepler-17 were used to implement this model.

Em busca de um novo indicador Espectroscópico do período de rotação das Estrelas do tipo solar

The study of sunspots consistently contributed to a better understanding of magnetic phenomena of the Sun, as its activity. It was found with the dynamics of sunspots that the Sun has a rotation period of twenty-seven days around your axis. With the help of Project Sun-As-A-Star that solar spectra obtained for more than thirty years we observed oscillations of both the depth of the spectral line and its equivalent width, and analysis of the return information about the characteristics of solar magnetism. It also aims to find patterns of solar magnetic activity cycle and the average period of rotation of the Sun will indicate the spectral lines that are sensitive to magnetic activity and which are not. Sensitive lines how Ti II 5381.0 Å stands as the best indicator of the solar rotation period and also shows different periods of rotation cycles of minimum and maximum magnetic activity. It is the first time we observe clearly distinct rotation periods in the different cycles. The analysis also shows that Ca II 8542.1 Å and HI 6562.0 Å indicate the cycle of magnetic activity of eleven years. Some spectral lines no indicated connection with solar activity, this result can help us search for programs planets using spectroscopic models. Data analysis was performed using the Lomb-Scargle method that makes the time series analysis for unequally spaced data. Observe different rotation periods in the cycles of magnetic activity accounts for a discussion has been debated for many decades. We verified that spectroscopy can also specify the period of stellar rotation, thus being able to generalize the method to other stars

Análise wavelet em curvas de luz estelares de sistemas binários da missão espacial CoRoT

Binary systems are key environments to study the fundamental properties of stars. In this work, we analyze 99 binary systems identified by the CoRoT space mission. From the study of the phase diagrams of these systems, our sample is divided into three groups: those whose systems are characterized by the variability relative to the binary eclipses; those presenting strong modulations probably due to the presence of stellar spots on the surface of star; and those whose systems have variability associated with the expansion and contraction of the surface layers. For eclipsing binary stars, phase diagrams are used to estimate the classification in regard to their morphology, based on the study of equipotential surfaces. In this context, to determine the rotation period, and to identify the presence of active regions, and to investigate if the star exhibits or not differential rotation and study stellar pulsation, we apply the wavelet procedure. The wavelet transform has been used as a powerful tool in the treatment of a large number of problems in astrophysics. Through the wavelet transform, one can perform an analysis in time-frequency light curves rich in details that contribute significantly to the study of phenomena associated with the rotation, the magnetic activity and stellar pulsations. In this work, we apply Morlet wavelet (6th order), which offers high time and frequency resolution and obtain local (energy distribution of the signal) and global (time integration of local map) wavelet power spectra. Using the wavelet analysis, we identify thirteen systems with periodicities related to the rotational modulation, besides the beating pattern signature in the local wavelet map of five pulsating stars over the entire time span.

Análise wavelet em curvas de luz estelares de sistemas binários da missão espacial CoRoT

Binary systems are key environments to study the fundamental properties of stars. In this work, we analyze 99 binary systems identified by the CoRoT space mission. From the study of the phase diagrams of these systems, our sample is divided into three groups: those whose systems are characterized by the variability relative to the binary eclipses; those presenting strong modulations probably due to the presence of stellar spots on the surface of star; and those whose systems have variability associated with the expansion and contraction of the surface layers. For eclipsing binary stars, phase diagrams are used to estimate the classification in regard to their morphology, based on the study of equipotential surfaces. In this context, to determine the rotation period, and to identify the presence of active regions, and to investigate if the star exhibits or not differential rotation and study stellar pulsation, we apply the wavelet procedure. The wavelet transform has been used as a powerful tool in the treatment of a large number of problems in astrophysics. Through the wavelet transform, one can perform an analysis in time-frequency light curves rich in details that contribute significantly to the study of phenomena associated with the rotation, the magnetic activity and stellar pulsations. In this work, we apply Morlet wavelet (6th order), which offers high time and frequency resolution and obtain local (energy distribution of the signal) and global (time integration of local map) wavelet power spectra. Using the wavelet analysis, we identify thirteen systems with periodicities related to the rotational modulation, besides the beating pattern signature in the local wavelet map of five pulsating stars over the entire time span.

Estudo sistemático de estrelas variáveis na era dos grandes surveys

The interest in the systematic analysis of astronomical time series data, as well as development in astronomical instrumentation and automation over the past two decades has given rise to several questions of how to analyze and synthesize the growing amount of data. These data have led to many discoveries in the areas of modern astronomy asteroseismology, exoplanets and stellar evolution. However, treatment methods and data analysis have failed to follow the development of the instruments themselves, although much effort has been done. In present thesis, we propose new methods of data analysis and two catalogs of the variable stars that allowed the study of rotational modulation and stellar variability. Were analyzed the photometric databases fromtwo distinctmissions: CoRoT (Convection Rotation and planetary Transits) and WFCAM (Wide Field Camera). Furthermore the present work describes several methods for the analysis of photometric data besides propose and refine selection techniques of data using indices of variability. Preliminary results show that variability indices have an efficiency greater than the indices most often used in the literature. An efficient selection of variable stars is essential to improve the efficiency of all subsequent steps. Fromthese analyses were obtained two catalogs; first, fromtheWFCAMdatabase we achieve a catalog with 319 variable stars observed in the photometric bands Y ZJHK. These stars show periods ranging between ∼ 0, 2 to ∼ 560 days whose the variability signatures present RR-Lyrae, Cepheids , LPVs, cataclysmic variables, among many others. Second, from the CoRoT database we selected 4, 206 stars with typical signatures of rotationalmodulation, using a supervised process. These stars show periods ranging between ∼ 0, 33 to ∼ 92 days, amplitude variability between ∼ 0, 001 to ∼ 0, 5 mag, color index (J - H) between ∼ 0, 0 to ∼ 1, 4 mag and spectral type CoRoT FGKM. The WFCAM variable stars catalog is being used to compose a database of light curves to be used as template in an automatic classifier for variable stars observed by the project VVV (Visible and Infrared Survey Telescope for Astronomy) moreover it are a fundamental start point to study different scientific cases. For example, a set of 12 young stars who are in a star formation region and the study of RR Lyrae-whose properties are not well established in the infrared. Based on CoRoT results we were able to show, for the first time, the rotational modulation evolution for an wide homogeneous sample of field stars. The results are inagreement with those expected by the stellar evolution theory. Furthermore, we identified 4 solar-type stars ( with color indices, spectral type, luminosity class and rotation period close to the Sun) besides 400 M-giant stars that we have a special interest to forthcoming studies. From the solar-type stars we can describe the future and past of the Sun while properties of M-stars are not well known. Our results allow concluded that there is a high dependence of the color-period diagram with the reddening in which increase the uncertainties of the age-period realized by previous works using CoRoT data. This thesis provides a large data-set for different scientific works, such as; magnetic activity, cataclysmic variables, brown dwarfs, RR-Lyrae, solar analogous, giant stars, among others. For instance, these data will allow us to study the relationship of magnetic activitywith stellar evolution. Besides these aspects, this thesis presents an improved classification for a significant number of stars in the CoRoT database and introduces a new set of tools that can be used to improve the entire process of the photometric databases analysis

Efeitos de tempestades magnéticas em sinais de gps, em Natal, Brasil

Satellites signals present disturbances (scintillations), due to presence of irregularities in the ionospheric plasma. In the present work, we dedicate to the study of the attenuation of these scintillations that is, an improvement in the signal, during the main magnetic storm phase during the period of October 2006 to February 2007. Using amplitude of scintillation 1.5GHz (L1) data of the net of satellites GPS, in the ionospheric station of Natal (5.84o S, 35.20o O, -20o dip) and geomagnetic indices, during the minimum solar cycle (referred to as cycle 23), demonstrating its anti-correlation between magnetic activity (Kp) and index of scintillation () (Bonelli2005 method, that works for solar maximum, Bonelli(2005)). These results show that these storms correspond to category I of Aarons (1991). The magnetic storms can generate irregularities when the electric feld of penetration eastward on the pre-reversal hour intensificating that and can too generate irregularities on midnight and sunlight period. The limitation of the method applied here is that it is not considering some storms that had also occurred during equinox and summer in the Brazilian region. For this reason, we will use additional data of the stations of São João de Cariri (Imager and Photometer) and of the station at Fortaleza (Digissonde data), as aid to analyze these storms. The storms that had been left out by the applied method, fit in the other two categories of Aarons, with one only exception (storm of January, 02). We show that in the day of the main phase of the magnetic storm, and with presence of bubbles (according to data of the Imager and Photometer), the speed of vertical drift ~E ~B (hF=t) is below 20m/s, that is the threshold found for Anderson al., (2004) (>20m/s as condition favorable to the formation of irregularities and increase in the scintillation index). This reduction of the speed is due to solar minimum

Investigando o campo magnético das estrelas análogas e gêmeas solares através da espectropolarimetria

This study proposes an observing program focused on the investigation of the stellar magnetism and dynamo evolution in cool active solar-like stars. More mainly in the solar analogs and twins. Observations of stars of our base were carried out with two spectropolarimeter (ESPaDOnS@CFHT and NARVAL@TBL). The analyse of stars in stage different allows an understanding of the dependence of magnetic activity on basic stellar parameters such as rotation, mass, age and depth of the convection zone. This study provides measures necessary for testing dynamo theories. The 65 targets for this project are solar type stars with mass spanning from 0:9 M=Mfi 1:075 solar masses and at different evolutionary stages. Our two main science objectives were, (i) To determine how the magnetic field evolved from the ZAMS to the TO (turn off) for stars with 0:9 M=Mfi 1:075; (ii) To determine the impact of convective depth and rotation on magnetic of cool stars of solar type. The main result from this study was the characterization of the dependence of magnetic field intensity as function of age, Rossby number and the convective zone deepening. This context, the availability of ESPaDOnS and NARVAL opens an exceptional possibility to study the magnetic properties of Sun-like stars by means of spectropolarimetric observations

Estudo fitoquímico e atividade antiplasmódica em Plasmodium falciparum (W2) de Himatanthus articulatus (Vahl) Woodson (Apocynaceae)

O presente trabalho descreve a análise fitoquímica e avaliação da atividade antiplasmódica em Plasmodium falciparum (W2) de Himatanthus articulatus (Vahl) Woodson. O extrato etanólico (EEHS) obtido por percolação do pó das cascas, após concentração, forneceu um precipitado (EEHSP) e um resíduo pastoso que foi submetido a liofilização (EEHS). Fracionou-se este por: re-extração sob refluxo, partição ácido-base e coluna cromatográfica de sílica gel. Além disso, submeteu-se o pó das cascas a extração com ácido clorídrico 1 N para separação de alcalóides. A prospecção fitoquímica, em CCD, foi realizada com EEHS e EEHSP, enquanto que EEHS, frações (FrDCM EEHS, FrAcOET EEHS e FrMeOH EEHS) e FAHS2 DCM foram analisadas por cromatografia líquida de alta eficiência acoplada a DAD (arranjo de diiodo-CLAE-DAD). FrAcOET EEHS foi fracioanda por coluna cromatográfica fornecendo uma substância isolada (S1). Analisou-se o EEHS, a fração majoritária obtida na coluna cromatográfica (F71), FAHS2 DCM e S1 por cromatografia liquida acoplada a espectrometria de massas (CL-EM). O espectro no infravermelho foi obtido para F71 e S1. A estrutura química de S1 foi definida como sendo o plumierídeo por ressonância magnética nuclear. A avaliação de atividade antiplasmódica foi realizada com EEHS, EEHSP, FrDCM EEHS, FrAcOET EEHS, FrMeOH EEHS, FAHS1 DCM, FAHS2 DCM, FAEEHS, FNEEHS, FNHS DCM e S1 pelo método da lactato desidrogenase parasitária (pLDH). Na prospecção fitoquímica, EEHS e EEHSP apresentaram resultados positivos para polifenóis e taninos, saponinas, triterpenos e esteroides, alcaloides e geninas flavônicas. EEHS e frações analisadas por CLAE-DAD mostraram os picos mais intensos sugestivos de iridoides, comprovados por CL-EM de EEHS que mostrou como substância majoritária o iridóide plumierídeo, coerente com o espectro no IV de F71 e S1 que revelou absorções de grupos funcionais presentes em iridóides. Nas análises destas por CL-EM, observou-se um pico a m/z 471 (M+H), atribuído ao íon pseudomolecular do plumierídeo e/ou isoplumierídeo. S1 foi identificada como plumierídeo. Até o presente momento não foi relatada a presença de alcaloides para a espécie, porém nas frações alcaloídicas (FAHS1 DCM, FAHS2 DCM, FAEEHS) e de neutros (FNEEHS e FNHS DCM) em análise por CCD revelada com reagente Dragendorff observaram-se manchas sugestivas de alcalóides, coerente com análise por CLAE-DAD de FAHS2 DCM, a qual mostrou pico majoritário com cromóforo sugestivo de alcaloide β-carbolínico. Em análises por CL-EM de FAHS2 DCM observou-se pico majoritário sugestivo do alcalóide 10-hidroxi-antirina-N-óxido com massa molecular 328 u. Os ensaios de atividade antiplasmódica foram negativos para EEHS, EEHSP, FrDCM EEHS, FrAcOET EEHS, FrMeOH EEHS, S1, FAEEHS, FAHS1 DCM, FNEEHS, FNHS DCM e moderadamente ativo (CI₅₀ 22,89 μg/mL) para FAHS2 DCM. Estes resultados indicam que a atividade antiplasmódica da planta pode se atribuída aos alcaloides, cuja presença em H. articulatus é descrita pela primeira vez.

Análise de atividade epileptiforme com uso simultâneo de eletrencefalografia e ressonância magnética funcional

The use of multimodal neuroimaging techniques has been helpful in the investigation of epileptogenic zone in patients with refractory epilepsies. This work aims to describe an ictal event during EEG-fMRI performed simultaneously in a 39-year-old man with refractory epilepsy. The EEG data were recorded at a sampling rate of 5 kHz, using a BrainAmp (BrainProducts, München, Germany) amplifier, with 64 MR (magnetic resonance) compatible Ag/AgCl electrodes. MR images were acquired using a 3T scanner in 3 sequences of 6 minutes of echo-planar images (EPIs), with TR = 2s, being the last sequence stopped after the ictal event. The EEG was corrected for gradient and pulse artifacts using the Brain Vision Analyzer2 software (BrainProducts), and the functional images were realigned, slice-timing corrected, normalized and smoothed. The start of the ictal changes was used for the evaluation of the BOLD response in MR images, using a t-test with a minimum cluster of 5 voxels, p <0.005 (T>2.5). The patient had a partial complex seizure, as noted by neurologist. The fMRI data showed positive BOLD responses (activation) in dysplastic areas, but showed the most significant activation outside the lesion, in areas compatible with secondary spread of the epileptic focus, probably caused by motor reaction also observed during the seizure. As a conclusion, we note that the technique of EEG-fMRI can detect the epileptogenic zone in patients with refractory epilepsy, but areas of dissemination of primary epileptogenic focus may show significant activation, introducing additional difficulties to the interpretation of the results

Ressonância magnética funcional: mapeamento do córtex motor através do efeito BOLD

Introdução – A ressonância magnética funcional (RMf) é hoje uma ferramenta fundamental na investigação funcional do cérebro humano, quer em indivíduos saudáveis quer em doentes com patologias diversas. É uma técnica complexa que necessita de uma aplicação cuidada e rigorosa e uma compreensão dos mecanismos biofísicos, de modo a serem obtidos resultados fiáveis e com melhor aceitação clínica. O efeito BOLD (Blood Oxygenation Level Dependent), que se baseia nas propriedades magnéticas da hemoglobina, é o método mais utilizado para medir a atividade cerebral por RMf. Objetivos – Otimizar um protocolo de RMf por efeito BOLD em voluntários saudáveis para mapeamento do córtex motor, de modo a que possa ser aplicado no futuro em doentes com patologias diversas. Metodologia – Foram estudados 34 voluntários saudáveis divididos em 2 grupos de estudo: BOLD 1 e BOLD 2. Com vista à otimização, foram testados no subgrupo BOLD 1 diferentes paradigmas e no subgrupo BOLD 2 foi estudada a influência do tempo de eco (TE). Para as várias condições foram comparados os volumes da região ativada e os níveis de ativação obtidos. Resultados/Discussão – O córtex motor foi identificado em todos os voluntários estudados. Não foram detetadas diferenças estatisticamente significativas quando comparados os resultados obtidos com os diferentes parâmetros de aquisição. Conclusão – O protocolo foi otimizado tendo em conta o nível de conforto reportado pelos voluntários. Uma vez que se pretende aplicar este mesmo protocolo no estudo de doentes, este fator torna-se particularmente relevante.

Atividade larvicida de taninos isolados de Magonia pubescens St. Hil. (Sapindaceae) sobre Aedes aegypti (Diptera, Culicidae)

Apresenta-se, pela primeira vez, o estudo fitoquímico das frações larvicidas, isoladas da Magonia pubescens, monitorado pelo estudo de eficácia sobre larvas de 3º estádio de Aedes aegypti, na busca de alternativas para o controle desse mosquito e obtenção de estruturas químicas passíveis de aprimoramento da atividade pela via sintética de outros derivados. As frações bioativas foram monitoradas quimicamente através de cromatografia de camada delgada, utilizando como revelador uma solução ácida de vanilina, e analisadas por ressonância magnética nuclear de hidrogênio e espectrometria de massas. Os bioensaios com as frações foram realizados em quintuplicata, à temperatura de 28±1ºC, 80±5% de umidade relativa e fotofase de 12 horas. As concentrações letais encontradas da fração MP-9, que apresentou o maior potencial larvicida, CL50 e CL90, foram de 3,1 e 36,6ppm, respectivamente. Todos os experimentos foram acompanhados por uma série controle, contendo o mesmo número de larvas.

Estudo farmacognóstico e atividade in vitro sobre a coagulação sanguínea e agregação plaquetária das folhas de Passiflora nitida Kunth (Passifloraceae)

O gênero Passiflora (Passifloraceae) é utilizado principalmente para tratar doenças do SNC e cardiovasculares. A espécie Passiflora nitida Kunth é comumente conhecida como “maracujá-do-mato". A literatura relata o consumo in natura dos frutos desta espécie pela população local para distúrbios gastrointestinais. Considerando o potencial farmacológico do gênero, este trabalho teve por objetivo realizar estudo de caracterização fitoquímica desta espécie e estudar os efeitos dos extratos aquoso (EA), etanólico (EE) e hexânico (EH) de suas folhas sobre a coagulação sanguínea e agregação plaquetária. Para a caracterização fitoquímica foram realizados testes de cromatografia em camada delgada e ressonância magnética nuclear. O efeito dos extratos sobre a coagulação foi avaliado pelos testes de tempo de protrombina (TP) e tempo de tromboplastina parcial ativada (TTPa). O efeito sobre a agregação plaquetária foi avaliado em plasma rico em plaquetas por método espectrofotométrico, usando adenosina difosfato (ADP) e adrenalina (ADR) como indutores da agregação. Os extratos EA, EE e EH apresentaram atividade coagulante pelo teste do TP e o EE apresentou atividade anticoagulante para o TTPa. Quando induzidos por ADP, os extratos EA, EE e EH apresentaram valores de concentração inibitória 50% (CI50, µg/mL) de 450,5 ± 50,7; 511,2 ± 35,5 e 394,4 ± 8,9, respectivamente, e quando induzidos por ADR apresentaram valores de 438,7 ± 5,2; 21,0 ± 1,9 e 546,9 ± 49,9, respectivamente. O EE apresentou atividade inibitória sobre a agregação. A caracterização fitoquímica foi sugestiva da presença de flavonóides e cumarinas, aos quais podem ser atribuídos, em parte, os efeitos biológicos estudados.

Especificidade de Pyrenophora avenae aos tecidos da semente de Avena sativa e sua atividade enzimática

Manchas nos grãos de aveia (Avena sativa) é limitante à sua comercialização por tornar o produto escuro e não permitir seu uso pela indústria alimentícia. A localização do micélio de Pyrenophora avenae nos grãos de aveia e sua atividade enzimática podem esclarecer a causa das manchas. O objetivo deste trabalho foi determinar a localização de P. avenae, na cariopse de aveia, avaliar a sua atividade enzimática e seu efeito sobre proteínas e lipídios dos grãos de aveia. A localização do micélio nos tecidos da cariopse foi determinada após hidratação e cortes da mesma, seguido da análise dos tecidos sob lupa e microscópio. Para avaliação da atividade enzimática foram utilizados 18 isolados de P. avenae obtidos das principais regiões produtoras de aveia do Brasil, avaliando-os quanto às suas atividades amilolítica, proteolítica e lipolítica, sendo realizada por plaqueamento das estruturas vegetativas em meio sólido específico para as enzimas testadas. As determinações do percentual de proteínas e lipídios foram obtidas pelos métodos de Kjeldahl e Bligh & Dyer, respectivamente. O micélio de P. avenae é a principal causa da mancha nos grãos de aveia, localizando-se nos três tecidos do pericarpo. O fitopatógeno apresenta boa atividade enzimática para lipase e protease porém insignificante para a amilase. Os grãos de aveia manchados e sadios não diferiram nos teores de proteínas e de lipídios. Esses teores foram mais elevados nos tecidos superficiais do pericarpo e aleurona independente da presença ou não de manchas, justificando o crescimento superficial de P. avenae sobre os grãos de aveia.

Cogumelo "shiitake" (Lentinula edodes) reduz o crescimento de fitopatógenos e a severidade de manchas foliares em sorgo

Lentinula edodes (cogumelo "shiitake") é um fungo basidiomiceto que apresenta propriedades nutricionais, medicinais e antibióticas. Compostos de interesse para o homem têm sido isolados do basidiocarpo e dos filtrados de cultura obtidos a partir do crescimento micelial. O presente trabalho teve como objetivos avaliar o efeito de diferentes preparações de L. edodes sobre patógenos da cultura do sorgo, Exserohilum turcicum e Colletotrichum sublineolum, bem como a proteção das plantas de sorgo contra estes patógenos. Em testes com placas de Petri e lâminas de vidro para microscopia, extratos aquosos obtidos do basidiocarpo inteiro e de suas partes individualizadas, píleo e estipe, reduziram a taxa de crescimento micelial e inibiram a germinação de esporos dos fungos, enquanto a atividade antifúngica do filtrado de crescimento micelial foi menos pronunciada. Em mesocótilos de sorgo, as diferentes preparações do "shiitake" não provocaram o acúmulo de fitoalexinas. O extrato aquoso do basidiocarpo e o composto lentinana reduziram parcialmente a severidade das doenças provocadas por E. turcicum na cv. Brandes e por C. sublineolum na cv. Tx-398-B, quando pulverizados 48 horas antes da inoculação das plantas, sob condições de casa de vegetação. Portanto, L. edodes apresenta potencial como agente de controle biológico ou como um modelo para a síntese de substâncias fungicidas.