Análise econômica mensal sobre o setor de mandioca e derivados: maio/2010.

Menor oferta sustenta cotação em maio – O mês de maio foi caracterizado pela menor oferta de mandioca para a indústria de fécula, levando à diminuição na quantidade de mandioca processada pelas fecularias. Ainda que seja período de safra, a disponibilidade de mandioca de segundo ciclo é menor em relação a anos anteriores e, além disso, agricultores mantiveram-se retraídos em relação à colheita. Esses produtores não tiveram necessidade de caixa e aguardam preços ainda maiores nos próximos meses. O excesso de chuvas em alguns períodos de maio prejudicou a colheita, dificultando os trabalhos e diminuindo a quantidade ofertada à indústria. Vale destacara, também, que houve menor número de mão-de-obra disponível para a colheita, visto que parte dos agricultores já começou o preparo de solo para o plantio da safra 2010/11. Apesar da menor oferta em maio, o preço médio mensal da raiz de mandioca, considerando as regiões pesquisadas pelo Cepea, foi de R$217,61/tonelada (R$ 0,3785/grama de amido na balança hidrostática de 5 kg), ligeira baixa de 0,5% frente à de abril. Já entre a última semana de abril e a última de maio, o preço médio subiu 18,8%, passando para R$ 237,81/t.Os preços médios mensais nos estados de São Paulo e Mato Grosso do Sul tiveram respectivas quedas de 4,9% e de 2,7% entre abril e maio.bitstream/item/23998/1/05MaiCEPEA.pd

Análise econômica mensal sobre o setor de mandioca e derivados: março/2010.

Mandioca: Preços recuam após três meses de alta ? A oferta de mandioca seguiu elevada para a indústria de fécula das regiões acompanhadas pelo Cepea em março. Este quadro foi atribuído aos preços favoráveis da cultura e também pelo clima favorável ao longo do período. Por conta destes fatores, as cotações que vinham se valorizando expressivamente em meses anteriores, passaram a ter elevações menos intensas. Em março, a tonelada da raiz destinada às fecularias foi cotada à média de R$249,71 (R$ 0,4343/ grama de amido, considerando a balança hidrostática de 5 kg), subindo 5,4% frente à de fevereiro (R$236,89/t). Esta alta é pouco expressiva quando comparada com a de meses anteriores, que foi de até 15$ 236,89/t da última semana de fevereiro com o de R$243,23 em igual período de março, a desvalorização é de 4,0$ 269,13/t, aumento de 6,5% frente ao valor do mês anterior. No Mato Grosso do Sul, no mesmo período, houve valorização de 4,6%, com o produto cotado a R$231,48/t. O estado de São Paulo teve a variação mais expressiva, de 11,9$ 195,81/t (Figura 1). Em âmbito regional, os preços tiveram alta em todas as regiões em março. A mais expressiva ocorreu na região de Assis (SP), de 11,9%, porém a mesma área teve a menor média do período (R$195,81/t). Já o maior preço do mês ocorreu no noroeste paranaense (R$ 272,17/t), onde a valorização foi de 5,5%. A alta menos expressiva foi observada no sudeste do Mato Grosso do Sul, de 4,0%, com o produto cotado à média de R$ 234,06/t (Figura 2).bitstream/item/25774/1/03Mar.pd

Análise econômica mensal sobre o setor de mandioca e derivados: junho/2010.

Mandioca: Cotações se sustentam em junho – Junho caracterizou-se pelo aumento da oferta da raiz para a indústria de derivados de mandioca, por ser período de pico de safra. Diante deste quadro, principalmente na segunda quinzena do mês, houve pressão sobre as cotações do produto. Apesar disso, a média de junho ainda foi maior que a de maio. O preço médio da mandioca para fecularias foi de R$246,31/t (R$ 0,4238/grama de amido na balança hidrostática de 5 kg) em junho, alta de 13,2% frente à de maio, que foi de R$217,64/t. Considerando a média da última semana de maio (R$ 237,81/t) e igual período de junho (R$239,31/t), houve aumento de 0,6$ 270,18/tonelada. A maior média de junho, de R$ 273,18/t, ocorreu no noroeste paranaense, com alta de 12,1% em relação à de maio.bitstream/item/24002/1/CEPEA06Jun.pd

MazeLogic: Jogo Educacional para Ensino de Lógica de Programação

Resumo. A área de jogos educacionais tem crescido de forma exponencial noBrasil e no mundo, pois estes têm sido usados por muitos alunos como objetode aprendizagem. Os jogos apresentam o conhecimento de modo divertido elúdico e pode ser aplicado a qualquer área e assunto. Este trabalho destina-seao desenvolvimento de um jogo educacional para ensino-aprendizagem para adisciplina de Lógica de Programação.Palavras-chave: Ensino aprendizagem, Jogo Educacional, Lógica deProgramação

Low-level Laser Therapy to the Mouse Femur Enhances the Fungicidal Response of Neutrophils against Paracoccidioides brasiliensis

Neutrophils (PMN) play a central role in host defense against the neglected fungal infection paracoccidioidomycosis (PCM), which is caused by the dimorphic fungus Paracoccidioides brasiliensis (Pb). PCM is of major importance, especially in Latin America, and its treatment relies on the use of antifungal drugs. However, the course of treatment is lengthy, leading to side effects and even development of fungal resistance. the goal of the study was to use low-level laser therapy (LLLT) to stimulate PMN to fight Pb in vivo. Swiss mice with subcutaneous air pouches were inoculated with a virulent strain of Pb or fungal cell wall components (Zymosan), and then received LLLT (780 nm; 50 mW; 12.5 J/cm2; 30 seconds per point, giving a total energy of 0.5 J per point) on alternate days at two points on each hind leg. the aim was to reach the bone marrow in the femur with light. Non-irradiated animals were used as controls. the number and viability of the PMN that migrated to the inoculation site was assessed, as well as their ability to synthesize proteins, produce reactive oxygen species (ROS) and their fungicidal activity. the highly pure PMN populations obtained after 10 days of infection were also subsequently cultured in the presence of Pb for trials of protein production, evaluation of mitochondrial activity, ROS production and quantification of viable fungi growth. PMN from mice that received LLLT were more active metabolically, had higher fungicidal activity against Pb in vivo and also in vitro. the kinetics of neutrophil protein production also correlated with a more activated state. LLLT may be a safe and non-invasive approach to deal with PCM infection.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de Minas Gerais (FAPEMIG)National Institute of Health (US NIH)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Fed Univ Alfenas UNIFAL MG, Inst Biomed Sci, Dept Microbiol & Immunol, Alfenas, MG, BrazilFed Univ Alfenas UNIFAL MG, Inst Biomed Sci, Dept Biochem, Alfenas, MG, BrazilState Univ Campinas UNICAMP, Inst Biol, Dept Struct & Funct Biol, São Paulo, BrazilFed Univ São Paulo UNIFESP, Dept Microbiol Immunol & Parasitol, São Paulo, SP, BrazilMassachusetts Gen Hosp, Wellman Ctr Photomed, Boston, MA 02114 USAHarvard Univ, Sch Med, Dept Dermatol, Boston, MA 02115 USAMIT, Harvard Mit Div Hlth Sci & Technol, Cambridge, MA 02139 USAFed Univ Alfenas UNIFAL MG, Inst Biomed Sci, Dept Pathol & Parasitol, Alfenas, MG, BrazilFed Univ São Paulo UNIFESP, Dept Microbiol Immunol & Parasitol, São Paulo, SP, BrazilCNPq: 486135/2012-8CNPq: 304827/2012-6FAPEMIG: CBB-PPM-00119-14National Institute of Health (US NIH): R01AI050875CAPES: AEX-9765-14-0Web of Scienc

Constraints on (2060) Chiron's size, shape, and surrounding material from the November 2018 and September 2019 stellar occultations

After the discovery of rings around the largest known Centaur object, (10199) Chariklo, we carried out observation campaigns of stellar occultations produced by the second-largest known Centaur object, (2060) Chiron, to better characterize its physical properties and presence of material on its surroundings. We predicted and successfully observed two stellar occultations by Chiron. These observations were used to constrain its size and shape by fitting elliptical limbs with equivalent surface radii in agreement with radiometric measurements. Constraints on the (2060) Chiron shape are reported for the first time. Assuming an equivalent radius of R$_{equiv}$ = 105$^{+6}_{-7}$ km, we obtained a semi-major axis of a = 126 $\pm$ 22 km. Considering Chiron's true rotational light curve amplitude and assuming it has a Jacobi equilibrium shape, we were able to derive a 3D shape with a semi-axis of a = 126 $\pm$ 22 km, b = 109 $\pm$ 19 km, and c = 68 $\pm$ 13 km, implying in a volume-equivalent radius of R$_{vol}$ = 98 $\pm$ 17 km, implying a density of 1119 $\pm$ 4 kg m$^{-3}$. We determined the physical properties of the 2011 secondary events around Chiron, which may then be directly compared with those of Chariklo rings, as the same method was used. Data obtained from SAAO in 2018 do not show unambiguous evidence of the proposed rings, mainly due to the large sampling time. Meanwhile, we discarded the possible presence of a permanent ring similar to (10199) Chariklo's C1R in optical depth and extension. Using the first multi-chord stellar occultation by (2060) Chiron and considering it to have a Jacobi equilibrium shape, we derived its 3D shape. New observations of a stellar occultation by (2060) Chiron are needed to further investigate the material's properties around Chiron, such as the occultation predicted for September 10, 2023

Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020

Context. The Centaur (10199) Chariklo has the first ring system discovered around a small object. It was first observed using stellar occultation in 2013. Stellar occultations allow sizes and shapes to be determined with kilometre accuracy, and provide the characteristics of the occulting object and its vicinity. Aims. Using stellar occultations observed between 2017 and 2020, our aim is to constrain the physical parameters of Chariklo and its rings. We also determine the structure of the rings, and obtain precise astrometrical positions of Chariklo. Methods. We predicted and organised several observational campaigns of stellar occultations by Chariklo. Occultation light curves were measured from the datasets, from which ingress and egress times, and the ring widths and opacity values were obtained. These measurements, combined with results from previous works, allow us to obtain significant constraints on Chariklo's shape and ring structure. Results. We characterise Chariklo's ring system (C1R and C2R), and obtain radii and pole orientations that are consistent with, but more accurate than, results from previous occultations. We confirm the detection of W-shaped structures within C1R and an evident variation in radial width. The observed width ranges between 4.8 and 9.1 km with a mean value of 6.5 km. One dual observation (visible and red) does not reveal any differences in the C1R opacity profiles, indicating a ring particle size larger than a few microns. The C1R ring eccentricity is found to be smaller than 0.022 (3σ), and its width variations may indicate an eccentricity higher than ~0.005. We fit a tri-axial shape to Chariklo's detections over 11 occultations, and determine that Chariklo is consistent with an ellipsoid with semi-axes of 143.8-1.5+1.4, 135.2-2.8+1.4, and 99.1-2.7+5.4 km. Ultimately, we provided seven astrometric positions at a milliarcsecond accuracy level, based on Gaia EDR3, and use it to improve Chariklo's ephemeris.Fil: Morgado, B.E.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Sicardy, Bruno. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Braga Ribas, Felipe. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Universidade Tecnologia Federal do Parana; BrasilFil: Desmars, Josselin. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Gomes Júnior, Altair Ramos. Universidade de Sao Paulo; BrasilFil: Bérard, D.. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Leiva, Rodrigo. Universidad de Chile; Chile. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Vieira Martins, Roberto. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Universidade Federal do Rio de Janeiro; BrasilFil: Benedetti Rossi, G.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Universidade Federal de Sao Paulo; BrasilFil: Santos Sanz, Pablo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Camargo, Julio Ignacio Bueno. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Duffard, R.. Universidade Federal do Rio de Janeiro; BrasilFil: Rommel, F.L.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Assafin, M.. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Boufleur, R.C.. Universidad Nacional de Córdoba; ArgentinaFil: Colas, F.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Kretlow, Mike. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Beisker, W.. University of North Carolina; Estados UnidosFil: Sfair, Rafael. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Snodgrass, Colin. University of Edinburgh; Reino UnidoFil: Morales, N.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; ChileFil: Fernández Valenzuela, E.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; ChileFil: Amaral, L.S.. Massachusetts Institute of Technology; Estados UnidosFil: Amarante, A.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; BrasilFil: Artola, R.A.. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Backes, M.. Universidad Nacional de Córdoba; ArgentinaFil: Bath, K. L.. University of North Carolina; Estados UnidosFil: Bouley, S.. University of St. Andrews; Reino UnidoFil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Schneiter, Ernesto Matías. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Ingeniería Económica y Legal; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentin

Direct evidence for phosphorus limitation on Amazon forest productivity

The productivity of rainforests growing on highly weathered tropical soils is expected to be limited by phosphorus availability1. Yet, controlled fertilization experiments have been unable to demonstrate a dominant role for phosphorus in controlling tropical forest net primary productivity. Recent syntheses have demonstrated that responses to nitrogen addition are as large as to phosphorus2, and adaptations to low phosphorus availability appear to enable net primary productivity to be maintained across major soil phosphorus gradients3. Thus, the extent to which phosphorus availability limits tropical forest productivity is highly uncertain. The majority of the Amazonia, however, is characterized by soils that are more depleted in phosphorus than those in which most tropical fertilization experiments have taken place2. Thus, we established a phosphorus, nitrogen and base cation addition experiment in an old growth Amazon rainforest, with a low soil phosphorus content that is representative of approximately 60% of the Amazon basin. Here we show that net primary productivity increased exclusively with phosphorus addition. After 2 years, strong responses were observed in fine root (+29%) and canopy productivity (+19%), but not stem growth. The direct evidence of phosphorus limitation of net primary productivity suggests that phosphorus availability may restrict Amazon forest responses to CO2 fertilization4, with major implications for future carbon sequestration and forest resilience to climate change.The authors acknowledge funding from the UK Natural Environment Research Council (NERC), grant number NE/L007223/1. This is publication 850 in the technical series of the BDFFP. C.A.Q. acknowledges the grants from Brazilian National Council for Scientific and Technological Development (CNPq) CNPq/LBA 68/2013, CNPq/MCTI/FNDCT no. 18/2021 and his productivity grant. C.A.Q., H.F.V.C., F.D.S., I.A., L.F.L., E.O.M. and S.G. acknowledge the AmazonFACE programme for financial support in cooperation with Coordination for the Improvement of Higher Education Personnel (CAPES) and the National Institute of Amazonian Research as part of the grants CAPES-INPA/88887.154643/2017-00 and 88881.154644/2017-01. T.F.D. acknowledges funds from FundacAo de Amparo a Pesquisa do Estado de SAo Paulo (FAPESP), grant 2015/50488-5, and the Partnership for Enhanced Engagement in Research (PEER) programme grant AID-OAA-A-11-00012. L.E.O.C.A. thanks CNPq (314416/2020-0)

Lower Richness of Small Wild Mammal Species and Chagas Disease Risk

A new epidemiological scenario involving the oral transmission of Chagas disease, mainly in the Amazon basin, requires innovative control measures. Geospatial analyses of the Trypanosoma cruzi transmission cycle in the wild mammals have been scarce. We applied interpolation and map algebra methods to evaluate mammalian fauna variables related to small wild mammals and the T. cruzi infection pattern in dogs to identify hotspot areas of transmission. We also evaluated the use of dogs as sentinels of epidemiological risk of Chagas disease. Dogs (n = 649) were examined by two parasitological and three distinct serological assays. kDNA amplification was performed in patent infections, although the infection was mainly sub-patent in dogs. The distribution of T. cruzi infection in dogs was not homogeneous, ranging from 11–89% in different localities. The interpolation method and map algebra were employed to test the associations between the lower richness in mammal species and the risk of exposure of dogs to T. cruzi infection. Geospatial analysis indicated that the reduction of the mammal fauna (richness and abundance) was associated with higher parasitemia in small wild mammals and higher exposure of dogs to infection. A Generalized Linear Model (GLM) demonstrated that species richness and positive hemocultures in wild mammals were associated with T. cruzi infection in dogs. Domestic canine infection rates differed significantly between areas with and without Chagas disease outbreaks (Chi-squared test). Geospatial analysis by interpolation and map algebra methods proved to be a powerful tool in the evaluation of areas of T. cruzi transmission. Dog infection was shown to not only be an efficient indicator of reduction of wild mammalian fauna richness but to also act as a signal for the presence of small wild mammals with high parasitemia. The lower richness of small mammal species is discussed as a risk factor for the re-emergence of Chagas disease