Produção Nacional
Revisado por pares
Daniel P. Grosvenor, T. W. Choularton, Hugh Coe, Gerhard Held,
... the IPMet (Instituto de Pesquisas Meteorológicas, Universidade Estadual Paulista) radar (S-band type at 2.8 Ghz) to have the ...
Tópico(s): Ionosphere and magnetosphere dynamics
2007 - Copernicus Publications | Atmospheric chemistry and physics
Produção Nacional
Revisado por pares
A. A. Pimenta, M. C. Kelley, Y. Sahai, J. A. Bittencourt, P. R. Fagundes,
... and 13 July 1999, when the low‐intensity band passed over Cachoeira Paulista. It should be pointed out that these thermospheric events are not related to geomagnetic disturbed conditions, as the nights for which data are presented are geomagnetically quiet (Kp < 2). In this paper we present and discuss the first observations of these thermospheric dark band structures in the Brazilian sector and their effects ...
Tópico(s): Solar and Space Plasma Dynamics
2008 - American Geophysical Union | Journal of Geophysical Research Atmospheres
Produção Nacional
Revisado por pares
H. Takahashi, Y. Sahai, N. R. Teixeira,
... filter photometer, have been carried out at Cachoeira Paulista (22.7 deg. S, 45.0 deg. W), Brazil, since 1983. The band intensities of the O2(0,1) band, I( ...
Tópico(s): Solar and Space Plasma Dynamics
1990 - Elsevier BV | Advances in Space Research
S. M. L. Melo, I. C. McDade, H. Takahashi,
... 1) band, and the OH Meinel (9–4) band emissions made at Cachoeira Paulista, Brazil (23°S, 45°W) from January 1987 ...
Tópico(s): Geophysics and Gravity Measurements
2001 - American Geophysical Union | Journal of Geophysical Research Atmospheres
Produção Nacional
Revisado por pares
H. Takahashi, Y. Sahai, P. P. Batista,
... type photometers, have been carried out at Cachoeira Paulista (22.7°S, 45.0°W), Brazil, since February 1983. The O2A(0, 1) band intensities occasionally vary from 200 to 1000 R ...
Tópico(s): Atmospheric chemistry and aerosols
1986 - Elsevier BV | Planetary and Space Science
Produção Nacional
Revisado por pares
... of a multichannel tilting filter photometer at Cachoeira Paulista (22.7°S, 45.0°W), Brazil. It is observed that the nocturnal variations of the five bands show good correlation between them but that there ...
Tópico(s): Atmospheric chemistry and aerosols
1981 - American Geophysical Union | Journal of Geophysical Research Atmospheres
Produção Nacional
Revisado por pares
H. Takahashi, P. P. Batista, B. R. Clemesha, D. M. Simonich, Y. Sahai,
... airglow OI 5577 Å and OH (8,3) band have been carried out at Cachoeira Paulista (23°S, 45°W), Brazil since 1976. Cross ...
Tópico(s): Atmospheric chemistry and aerosols
1979 - Elsevier BV | Planetary and Space Science
Produção Nacional
C. M. Wrasse, H. Takahashi, D. Gobbi,
The airglow OH (8-3) and (6-2) band rotational temperatures were measured and compared using two scanning photometer at Cachoeira Paulista (23ºS, 45ºW) in 1999. The rotational temperature were obtained from the ratio between the P1(5) and P1(3) in the case of the (8-3) band and P1(4) and P1(2) lines for ...
Tópico(s): Solar and Space Plasma Dynamics
2004 - Brazilian Society of Geophysics | Brazilian Journal of Geophysics
Produção Nacional
Revisado por pares
Karina Rodrigues dos Santos, Bianca C. Carlos, K.S. Paduan, Samir Moura Kadri, T. H. Barrella, M.R.V. Amarante, Paulo Eduardo Martins Ribolla, Reinaldo José da Silva,
... Serpentes, Colubridae) collected in the municipality of Lençóis Paulista, State of São Paulo, Brazil. DNA amplification by polymerase chain reaction (PCR) resulted in a 350 bp band for samples containing S. ophidiae and Strongyloides venezuelensis ...
Tópico(s): Helminth infection and control
2009 - Cambridge University Press | Journal of Helminthology
Brian A. Tinsley, R. P. Rohrbaugh, Y. Sahai, Nilton Rodrigues Teixeira,
... Haleakala, Hawaii (dip lat.∼22°N) and Cachoeira Paulista, Brasil (dip lat.∼12°S) of emissions excited by particle precipitation during periods of magnetic activity. The first negative bands of N 2 + were found to have a ...
Tópico(s): Solar and Space Plasma Dynamics
1982 - American Geophysical Union | Geophysical Research Letters
Produção Nacional
Revisado por pares
H. Takahashi, Y. Sahai, P. P. Batista, B. R. Clemesha,
... band (864.5 nm) and OH(9,4) band (774.6 nm) emissions have been carried out at Cachoeira Paulista (22.7oS, 45.0oW) since 1983. We present ...
Tópico(s): GNSS positioning and interference
1992 - Elsevier BV | Advances in Space Research
Produção Nacional
P. R. Fagundes, H. Takahashi, Y. Sahai, D. Gobbi,
... 0,1) band, NaD and OH (9,4) band emissions obtained during the period October November 1989 at Cachoeira Paulista (23°S, 45°W), Brazil, have been analysed ...
Tópico(s): GNSS positioning and interference
1995 - Elsevier BV | Journal of Atmospheric and Terrestrial Physics
Produção Nacional
Revisado por pares
E. R. de Paula, I. J. Kantor, J. H. A. Sobral, H. Takahashi, D.C. Santana, D. Gobbi, A. F. Medeiros, L. A. T. Limiro, H. Kil, P. M. Kintner, M. J. Taylor,
... drift velocity of nighttime ionospheric irregularities from Cachoeira Paulista (22.41°S,45°W, dip latitude −17.43°), a station under the Equatorial Anomaly, from December 1998 to February 1999 using L1 band GPS receivers and OI 630nm all-sky images. ...
Tópico(s): Solar and Space Plasma Dynamics
2002 - Elsevier BV | Journal of Atmospheric and Solar-Terrestrial Physics
Produção Nacional
Revisado por pares
Ana de Lourdes Sá de Lira, Ageu Lima da Costa, Guilherme Henrique Alves da Fonseca, Nayra Rafaelle Fernandes da Silva, Keila Rejane de Jesus Martins,
Aim: To investigate the prevalence of the early unitary loss of deciduous and the need for space maintainer in the posterior region, of the band-loop type. Methods: The clinical examination of 568 children between 6 and 12 years of age in mixed dentition was performed in two municipal schools. After the diagnosis of premature loss of one or two deciduous molars (unilateral, one or both arches, respectively), without successors initiating the eruptive process in the oral cavity, the child was referred ...
Tópico(s): Dental Health and Care Utilization
2019 - UNIVERSIDADE EST.PAULISTA JÚLIO DE MESQUITA FILHO | Brazilian Dental Science
H. Takahashi, B. R. Clemesha, Y. Sahai, P. P. Batista, D. M. Simonich,
... at 589.3 nm and OH(9,4) band at 774.6 nm have been observed since 1977 at Cachoeira Paulista (22.7°S, 45.0°W), Brazil. The ...
Tópico(s): Solar and Space Plasma Dynamics
1992 - American Geophysical Union | Journal of Geophysical Research Atmospheres
Produção Nacional
Revisado por pares
Amilcar Pérez-Riverol, Franco Dani Campos Pereira, Alexis Musacchio, Luís Gustavo Romani Fernandes, José Roberto Aparecido dos Santos‐Pinto, Débora Justo-Jacomini, Gabriel Oliveira de Azevedo, Murilo Luiz Bazon, Mário Sérgio Palma, Ricardo de Lima Zollner, Márcia Regina Brochetto-Braga,
... IgE-reactivity of the sera from 10 P. paulista venom-allergic patients to rPoly p 1 and nPoly p 1. High levels of insoluble rPoly p 1 were obtained during heterologous expression. After solubilization of inclusion bodies and purification of the recombinant protein, a unique band of ∼34 kDa was detected in SDS-PAGE analysis. Allergen-specific IgE (sIgE) from allergic patients' sera recognized rPoly p 1, nPoly p 1 and crude venom extract to a similar extent. Our results showed that rPoly p 1 could be used for development of component-resolved diagnosis (CRD) and molecular-defined SIT of P. paulista venom allergy.
Tópico(s): Contact Dermatitis and Allergies
2016 - Elsevier BV | Toxicon
Produção Nacional
Revisado por pares
C. A. O. B. Figueiredo, H. Takahashi, C. M. Wrasse, Y. Otsuka, K. Shiokawa, Diego Barros,
... ionospheric disturbances (MSTIDs) have been observed at Cachoeira Paulista (22.4°S; 45.0°W), Brazil, from June 2013 to December 2015, using airglow OI 630.0‐nm images. During the period, 58 MSTIDs were identified and classified as follows: dark band MSTIDs (around 10 events) and periodic MSTIDs (48 ...
Tópico(s): Seismic Waves and Analysis
2018 - Wiley | Journal of Geophysical Research Space Physics
Produção Nacional
Revisado por pares
C. M. N. Cândido, A. A. Pimenta, J. A. Bittencourt, F. Becker‐Guedes,
... scale traveling ionospheric disturbances (MSTIDs) observed over Cachoeira Paulista (22.7°S, 45.0°W, −13.2° mag lat), Brazil. The optical signatures of the low‐latitude MSTIDs in the southern hemisphere observed in the OI 630.0 nm emission images can be a single dark band structure or alternating dark/light bands aligned in ...
Tópico(s): Geomagnetism and Paleomagnetism Studies
2008 - American Geophysical Union | Geophysical Research Letters
Produção Nacional
Juliana Cristina Alves Silva, Marcello Felipe de Jesus Múscari,
... Paulista e regiao da Luz. Chegando a Av. Paulista: plumas, pouca roupa, band...
Tópico(s): Urban and sociocultural dynamics
2016 - | Ponto Urbe
... Anatomie der Zahne. Die Zahn-, Mund-und Kieferheilkunde, Band I. Urban and Schwarzenberg, Munich Google Scholar Delia Serra, O. 1951 Observacoes morfologicas sobre os dentes jugais humanos. Associacao Paulista de Cirurgioes Dentistas, 5: 37–45. Google Scholar ...
Tópico(s): Orthodontics and Dentofacial Orthopedics
1959 - Wiley | American Journal of Physical Anthropology
Produção Nacional
Revisado por pares
H. Takahashi, B. R. Clemesha, Y. Sahai, P. P. Batista,
... rotational temperature of the airglow OH(9,4) band emission at two ground-based locations, one in the equatorial region, Fortaleza (3.9°S, 38.4°W) and the other at low latitude, Cachoeira Paulista (22.7°S, 45.0°W). The data ...
Tópico(s): Solar and Space Plasma Dynamics
1994 - Elsevier BV | Advances in Space Research
Produção Nacional
Revisado por pares
A. A. Pimenta, J. A. Bittencourt, P. R. Fagundes, Y. Sahai, R. A. Buriti, H. Takahashi, M. J. Taylor,
... the west-east motion of the intensity depleted bands it is possible to infer the ionospheric plasma bubble zonal velocity. All-sky images from São João do Cariri (7.4°S, 36.5°W) and from Cachoeira Paulista (22.7°S, 45.0°W), Brazil, between ...
Tópico(s): Solar and Space Plasma Dynamics
2003 - Elsevier BV | Journal of Atmospheric and Solar-Terrestrial Physics
Produção Nacional
Revisado por pares
P. R. Fagundes, D. Gobbi, H. Takahashi, Y. Sahai,
... OH(9, 4) and O2 atmospheric (0,1) band emission intensities and their rotational temperatures T(OH) and T(O2), respectively, observed at Cachoeira Paulista (23°S, 45°W), Brazil, during the period from October 1989 to December 1990, have been analyzed to study the nighttime mesospheric energy loss rates through the radiations from the vibrationally excited OH* and electronically excited O2* bands. The total emission rates of the OH Meinel ...
Tópico(s): Solar and Space Plasma Dynamics
1997 - Copernicus Publications | Annales Geophysicae
R. P. Rohrbaugh, Brian A. Tinsley, H. K. Rassoul, Y. Sahai, N. R. Teixeira, Robert G. Tull, D. R. Doss, A. L. Cochran, W. D. Cochran, E. S. Barker,
... low‐latitude sites (Mt. Haleakala, Hawaii and Cachoeira Paulista, Brazil) and one mid‐latitude site (McDonald Observatory, Southwest Texas). Results are compared for magnetic storms of April 13, 1981 and July 14, 1982. The emissions have the characteristics appropriate to the precipitation into the thermosphere of energetic neutral atoms and/or ions originating in the ring current. These characteristics include high rotational/vibrational excitation of the N 2 + 1 N bands and at times the occurrence of HBaβ emission ...
Tópico(s): Atmospheric Ozone and Climate
1983 - American Geophysical Union | Journal of Geophysical Research Atmospheres
Produção Nacional
Revisado por pares
H. Takahashi, D. Gobbi, P. P. Batista, S. M. L. Melo, N. R. Teixeira, R. A. Buriti,
... OH (9,4) and O2 atmospheric (0,1) bands and their rotational temperatures have been measured using ground-based multichannel airglow photometers, one located near the equator at Fortaleza (3.9 S, 38.4 W) and the other at lowmiddle latitude Cachoeira Paulista (22.7 S, 45.0 W). Monthly averaged ...
Tópico(s): Atmospheric chemistry and aerosols
1998 - Elsevier BV | Advances in Space Research
Produção Nacional
Danielle Cristina de Morais Amorim, A. A. Pimenta, Aline Amorim de Almeida,
... obtainedby an all-sky imager installed at Cachoeira Paulista (22.7◦S, 45◦W), show dark band structures propagating from southeast to northwest with velocities ...
Tópico(s): Solar and Space Plasma Dynamics
2012 - Brazilian Society of Geophysics | Brazilian Journal of Geophysics
Produção Nacional
H. Takahashi, B. R. Clemesha, P. P. Batista,
... 589.3 mn and the OH (9,4) band and its rotational temperature have been measured using a ground-based multichannel airglow photometer located at Fortaleza (3.9°S, 38.4°W) since 1986. The observed emission intensities show predominantly semi-annual oscillations with maxima at the equinoxes and minima during the solstices. The amplitudes of the oscillations are larger than those observed from the low latitude station, Cachoeira Paulista (22.7°S, 45.0°W). The OH ...
Tópico(s): Solar and Space Plasma Dynamics
1995 - Elsevier BV | Journal of Atmospheric and Terrestrial Physics
... Nogueira Machado. – 5. ed. – Petrópolis, RJ : Vozes : Bragança Paulista, Editora Universitária São Francisco, 2008. MARX, Karl. Das Kapital: Der Produktionprozess des Kapitals. Erster Band, Erstes Buch (Kapitel XVI-LII). Hamburg, Nikol Verlag., ...
Tópico(s): Critical Theory and Philosophy
2019 - | Trilhas Filosóficas
Produção Nacional
Revisado por pares
Isabelle Magalhães Guedes Freitas, Josiane Aparecida de Miranda, Pedro Augusto de Carvalho Mira, Carla Márcia Moreira Lanna, Jorge Roberto Perrout de Lima, Mateus Camaroti Laterza,
... spectral analysis, low (LF) and high frequency (HF) bands, besides the low and high frequencies ratio (LF/ ... versus 43±23, p=0.015) and HF band (54±20 versus 64±14 normalized units - n. ... were lower in the Obese Group. The LF band (46±20 versus 36±14 n.u., p= ...
Tópico(s): Cardiovascular Syncope and Autonomic Disorders
2014 - Elsevier BV | Revista Paulista de Pediatria
Larissa O. Paulista, Josep Albero, Ramiro José Espinheira Martins, Rui A.R. Boaventura, Vítor J.P. Vilar, Tânia F.C.V. Silva, Hermenegildo Garcı́a,
... allows the visible light harvest and narrows the band gap energy (ca. 14–20%); (ii) the selectivity ...
Tópico(s): Catalytic Processes in Materials Science
2021 - Multidisciplinary Digital Publishing Institute | Catalysts