848 resultados para permanent and transitory shocks
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Sigara dorsalis belongs to a very closely related group of six species forming the sub-genus Sigara sensu strictu. Each of the six species has a distinct allopatric geographical distribution in Europe. Studies were started on a series of populations in the north west Midlands of England. All the populations examined, except one, contained only males with the typical diagnostic features of S. dorsalis, albeit with considerable variation. One pond near Congleton, Cheshire situated in a permanent-ley pasture and apparently free from pollution contained typical S. dorsalis males but, in addition, many atypical individuals. From one sample of forty-six males, all possessed left parameres with the slight point on the dorsal surface characteristic of S. dorsalis. However, almost half possessed additional morphological features intermediate between S. dorsalis and S. striata.
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The importance of ponds for biodiversity in Britain has been demonstrated by a number of studies. However, most of the research and interest has been directed at permanent waterbodies, and temporary ponds have been largely neglected. In this article the author present some preliminary findings from a project which aims to fill some of the many gaps in our knowledge of temporary ponds in Britain. The project, which runs for three years until the end of 2001, aims specifically to investigate the ecology of temporary ponds in England and Wales by describing (i) their wetland plant and macroinvertebrate communities, (ii) their physico-chemical characteristics, and (iii) their value as a biodiversity resource. The article focuses on the assessment of temporary ponds as a biodiversity resource and briefly considers aspects of species richness, rarity and distinctiveness. Where possible, temporary ponds are compared with other waterbody types, mainly permanent ponds from the National Pond Survey (NPS), to give the results a broader context.
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The Advanced LIGO and Virgo experiments are poised to detect gravitational waves (GWs) directly for the first time this decade. The ultimate prize will be joint observation of a compact binary merger in both gravitational and electromagnetic channels. However, GW sky locations that are uncertain by hundreds of square degrees will pose a challenge. I describe a real-time detection pipeline and a rapid Bayesian parameter estimation code that will make it possible to search promptly for optical counterparts in Advanced LIGO. Having analyzed a comprehensive population of simulated GW sources, we describe the sky localization accuracy that the GW detector network will achieve as each detector comes online and progresses toward design sensitivity. Next, in preparation for the optical search with the intermediate Palomar Transient Factory (iPTF), we have developed a unique capability to detect optical afterglows of gamma-ray bursts (GRBs) detected by the Fermi Gamma-ray Burst Monitor (GBM). Its comparable error regions offer a close parallel to the Advanced LIGO problem, but Fermi's unique access to MeV-GeV photons and its near all-sky coverage may allow us to look at optical afterglows in a relatively unexplored part of the GRB parameter space. We present the discovery and broadband follow-up observations (X-ray, UV, optical, millimeter, and radio) of eight GBM-IPTF afterglows. Two of the bursts (GRB 130702A / iPTF13bxl and GRB 140606B / iPTF14bfu) are at low redshift (z=0.145 and z = 0.384, respectively), are sub-luminous with respect to "standard" cosmological bursts, and have spectroscopically confirmed broad-line type Ic supernovae. These two bursts are possibly consistent with mildly relativistic shocks breaking out from the progenitor envelopes rather than the standard mechanism of internal shocks within an ultra-relativistic jet. On a technical level, the GBM--IPTF effort is a prototype for locating and observing optical counterparts of GW events in Advanced LIGO with the Zwicky Transient Facility.
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Part I: The dynamic response of an elastic half space to an explosion in a buried spherical cavity is investigated by two methods. The first is implicit, and the final expressions for the displacements at the free surface are given as a series of spherical wave functions whose coefficients are solutions of an infinite set of linear equations. The second method is based on Schwarz's technique to solve boundary value problems, and leads to an iterative solution, starting with the known expression for the point source in a half space as first term. The iterative series is transformed into a system of two integral equations, and into an equivalent set of linear equations. In this way, a dual interpretation of the physical phenomena is achieved. The systems are treated numerically and the Rayleigh wave part of the displacements is given in the frequency domain. Several comparisons with simpler cases are analyzed to show the effect of the cavity radius-depth ratio on the spectra of the displacements.
Part II: A high speed, large capacity, hypocenter location program has been written for an IBM 7094 computer. Important modifications to the standard method of least squares have been incorporated in it. Among them are a new way to obtain the depth of shocks from the normal equations, and the computation of variable travel times for the local shocks in order to account automatically for crustal variations. The multiregional travel times, largely based upon the investigations of the United States Geological Survey, are confronted with actual traverses to test their validity.
It is shown that several crustal phases provide control enough to obtain good solutions in depth for nuclear explosions, though not all the recording stations are in the region where crustal corrections are considered. The use of the European travel times, to locate the French nuclear explosion of May 1962 in the Sahara, proved to be more adequate than previous work.
A simpler program, with manual crustal corrections, is used to process the Kern County series of aftershocks, and a clearer picture of tectonic mechanism of the White Wolf fault is obtained.
Shocks in the California region are processed automatically and statistical frequency-depth and energy depth curves are discussed in relation to the tectonics of the area.
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The cosmic-ray positron and negatron spectra between 11 and 204 MeV have been measured in a series of 3 high-altitude balloon flights launched from Fort Churchill, Manitoba, on July 16, July 21, and July 29, 1968. The detector system consisted of a magnetic spectrometer utilizing a 1000-gauss permanent magnet, scintillation counters, and a lucite Čerenkov counter.
Launches were timed so that the ascent through the 100 g/cm2 level of residual atmosphere occurred after the evening geomagnetic cutoff transition. Data gathered during ascent are used to correct for the contribution of atmospheric secondary electrons to the flux measured at float altitude. All flights floated near 2.4 g/cm2.
A pronounced morning intensity increase was observed in each flight. We present daytime positron and negatron data which support the interpretation of the diurnal flux variation as a change in the local geomagnetic cutoff. A large diurnal variation was observed in the count rate of positrons and negatrons with magnetic rigidities less than 11 MV and is evidence that the nighttime cutoff was well below this value.
Using nighttime data we derive extraterrestrial positron and negatron spectra. The positron-to-total-electron ratio which we measure indicates that the interstellar secondary, or collision, source contributes ≾50 percent of the electron flux within this energy interval. By comparing our measured positron spectrum with the positron spectrum calculated for the collision source we derive the absolute solar modulation for positrons in 1968. Assuming negligible energy loss during modulation, we derive the total interstellar electron spectrum as well as the spectrum of directly accelerated, or primary, electrons. We examine the effect of adiabatic deceleration and find that many of the conclusions regarding the interstellar electron spectrum are not significantly altered for an assumed energy loss of up to 50 percent of the original energy.
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[ES]Ikasnabar es una conferencia para hablar de tendencias en educación, sobre las nuevas tecnologías en el ámbito educativo y conocer personas que están generando buenas ideas y prácticas en su quehacer diario. Este libro intenta recoger todo ello con las contribuciones de autores noveles y de renombre que buscan la excelencia en los procesos de enseñanza-aprendizaje. Tres tendencias importantes de aprendizaje se están expandiendo. Microcontenidos, aprendizaje móvil y MOOCs son la cara de una misma moneda: microaprendizaje con contenido rico, abierto y desmenuzado. A medida que el consumo de Internet desde dispositivos móviles aumenta, el aprendizaje móvil con tecnologías como HTML5, software para MOOC, plataformas de contenidos de vídeo, etc., están siendo algunas de las claves de la nueva revolución en el ámbito educativo. El microcontenido hace referencia a los pequeños trozos de información digital en un estado permanente de flujo y circulación. Es a menudo un único tema, limitado en longitud, que se consume rápidamente y con frecuencia limitado por el software o por el dispositivo. Se trata de la puesta en común de recursos. Se basa en la interacción humano-a-humano con los medios de comunicación de Internet. El otro tema central de esta conferencia es el de los MOOC realizados por los profesores que quieren tomar ventaja en el comienzo de esta nueva era de la educación abierta con calidad. MOOCs son, básicamente, cursos abiertos y es necesario recordar los puntos esenciales de este tipo de instrucción. Los miniMOOCs son alternativas con menos horas en el proceso de aprendizaje. Hoy en día, un buen MOOC podrá ser la mejor tarjeta de presentación para profesores, expertos y estudiantes. Vivimos en tiempos de cambio con ámbitos en los que se mezcla el aprendizaje formal e informal, y las universidades y colegios deberíamos estar atentos a esto.
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Femtosecond pulsed lasers have been widely used for materials microprocessing. Due to their ultrashort pulse width and ultrahigh light intensity, the process is generally characterized by the nonthermal diffusion process. We observed various induced microstructures such as refractive-index-changed structures, color center defects, microvoids and microcracks in transparent materials (e.g., glasses after the femtosecond laser irradiation), and discussed the possible applications of the microstructures in the fabrication of various micro optical devices [e.g., optical waveguides, microgratings, microlenses, fiber attenuators, and three-dimensional (3D) optical memory]. In this paper, we review our recent research developments on single femtosecond-laser-induced nanostructures. We introduce the space-selective valence state manipulation of active ions, precipitation and control of metal nanoparticles and light polarization-dependent permanent nanostructures, and discuss the mechanisms and possible applications of the observed phenomena.
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A tese intitulada No cenário do tempo presente: um estudo sobre os valores hodiernos nas culturas juvenis, constitui uma investigação analítica acerca dos valores permanentes socializados pela cultura juvenil contemporânea. No fluxo transitório inerente à conjuntura da sociedade hodierna, postula-se a existência de valores compartilhados por jovens oriundos de distintas realidades sociais, familiares e educacionais. A pesquisa se propõe a apreender os ditos valores em meio aos contextos particulares das experiências juvenis. Para tal, adota como lócus de investigação, escolas públicas e privadas com características pedagógicas, filosóficas e socioeconômicas diferenciadas. Propugna-se o desenvolvimento da análise sobre três eixos principais: a questão do tempo presente, com suas características dinâmicas e a própria história que a define no seu processo em desenvolvimento; a questão da juventude, desdobrada nos jovens específicos desta pesquisa localizados nas culturas juvenis consideradas como unidade que encampa a diversidade; a questão dos valores observados tanto à luz da história, que os produz como a dos jovens que os elege desde o exercício da liberdade enquanto pessoa humana. Assim, pretendemos realizar um trabalho profícuo no tocante ao avanço e aprofundamento no conhecimento das questões atinentes à Juventude e Ética no tempo presente.
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The following brief is to ensure standard criteria and format are used for the scoping and environmental assessment of water resources projects leading to the production of an environmental report or Environmental Statement. This volume is one of a series giving guidance on water resources projects. The water resources projects will predominantly comprise drought orders and permits, time limited and permanent licences. Smaller projects, such as spray irrigation licences, will not require an environmental assessment. This document forms the basis for discussions between the Environment Agency North East Region, consultees and the applicant. The process aims to produce a thorough assessment. Each section addresses consecutive elements of the assessment process. Section 2 outlines the structure for a scoping document, section 3 outlines the structure for an Environmental Statement and section 4 gives guidance on the role of an Environmental Action Plan. Appendices 1 and 2 should be used in conjunction with the scoping process and cover a wide range of aspects. However, some projects may not require all of them to be included, whilst for others, the inclusion of additional factors may be appropriate.
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Belugas, Delphinapterus leucas, groups were videotaped concurrent to observer counts during annual NMFS aerial surveys of Cook Inlet, Alaska, from 1994 to 2000. The videotapes provided permanent records of whale groups that could be examined and compared to group size estimates ade by aerial observers.Examination of the video recordings resulted in 275 counts of 79 whale groups. The McLaren formula was used to account for whales missed while they were underwater (average correction factor 2.03; SD=0.64). A correction for whales missed due to video resolution was developed by using a second, paired video camera that magnified images relative to the standard video. This analysis showed that some whales were missed either because their image size fell below the resolution of hte standard video recording or because two whales surfaced so close to each other that their images appeared to be one large whale. The correction method that resulted depended on knowing the average whale image size in the videotapes. Image sizes were measured for 2,775 whales from 275 different passes over whale groups. Corrected group sizes were calcualted as the product of the original count from video, the correction factor for whales missed underwater, and the correction factor for whales missed due to video resolution (averaged 1.17; SD=0.06). A regression formula was developed to estimate group sizes from aerial observer counts; independent variables were the aerial counts and an interaction term relative to encounter rate (whales per second during the counting of a group), which were regressed against the respective group sizes as calculated from the videotapes. Significant effects of encounter rate, either positive or negative, were found for several observers. This formula was used to estimate group size when video was not available. The estimated group sizes were used in the annual abundance estimates.
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The genesis and the early history of the Woods Hole Laboratory (WHL), to a lesser extent the Marine Biological Laboratory (MBL), and to some degree the Woods Hole Oceanographic Institution (WHOI), were elegantly covered by Paul S. Galtsoff (1962) in his BCF Circular "The Story of the Bureau of Commercial Fisheries Biological Laboratory, Woods Hole, Massachusetts." It covers the period from the beginning in 1871 to 1958. Galtsoffs more than 35-year career in the fishery service was spent almost entirely in Woods Hole. I will only briefly touch on that portion of the Laboratory's history covered by Galtsoff. Woods Hole, as a center of marine science, was conceived and implemented largely by one man, Spencer Fullerton Baird, at that time Assistant Secretary of the Smithsonian and who was also instrumental in the establishment of the National Museum and Permanent Secretary of the newly established American Association for the Advancement of Science. He was appointed by President Ulysses S. Grant in 1871 as the first U.S. Commissioner of Fisheries. Fisheries research began here as early as 1871, but a permanent station did not exist until 1885.
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A Hipóxia-isquemia (HI) perinatal é um problema de saúde pública, e ocorrem aproximadamente 1,5 casos de encefalopatias por HI por 1000 nascidos vivos. Dos que sobrevivem 25-60% sofrem de deficiências permanentes do desenvolvimento neurológico, incluindo paralisia cerebral, convulsões, retardo mental, e dificuldade de aprender. Neurônios e oligodendrócitos, especialmente os progenitores, são os mais afetados pela HI. Existem vários modelos de HI, no entanto, poucos levam em consideração as intercorrências maternas, a importância da atividade placentária, e as trocas entre mãe-filho, que são clinicamente observadas em humanos. Robinson estabeleceu um modelo de HI sistêmica pré-natal transitório, onde o fluxo das artérias uterinas da rata grávida era obstruído por 45 minutos no décimo oitavo dia (E18) de gestação. Neste modelo foram observadas alterações que são similares às observadas em cérebros humanos que passaram por hipóxia perinatal, dentre as quais foram relatados aumento no nível de apoptose. Caspase-3 é descrita como uma enzima que atua na apoptose, e é amplamente utilizada como marcador para células apoptóticas. Vários autores vêm mostrando, entretanto, que a enzima caspase-3 pode estar ativada para fins não apoptóticos. No modelo de HI sistêmica pré-natal, foram observados astrogliose na substância branca, morte de oligodendrócitos, lesão em axônios tanto na substância branca como no córtex cerebral, e danos motores. Pouco se sabe da influencia do insulto HI no desenvolvimento do cerebelo, considerando que o cerebelo junto com o córtex motor, contribui para o controle motor. O objetivo desse trabalho foi avaliar a distribuição da caspase-3 clivada durante o desenvolvimento do cerebelo em um modelo de HI pré-natal. Os resultados deste trabalho demonstram que as células caspase-3 clivadas apresentaram duas morfologias distintas em ambos os grupos. Uma onde a caspase-3 foi observada apenas no núcleo, oscilando entre células com imunorreatividade fraca a intensa, e de células com a presença da caspase-3 no corpo celular, nos prolongamentos condensados e presença de fragmentos ao redor do soma, morfologia típica de célula em apoptose. A HI pré-natal, assim como nos hemisférios cerebrais, levou ao aumento de células caspase-3 clivadas com morfologia de progenitores de oligodendrócitos no cerebelo do grupo HI em P2, mas não em P9 e P23. Também foi demonstrado que a HI pré-natal não levou a uma ativação da apoptose em oligodendrócitos, neurônios e microglia (identificados por seus respectivos marcadores, CNPase, NeuN e ED1) apresentando marcação no núcleos de células GFAP+, na substância branca, camada granular e nas células da glia de Bergmann, em P9 e P23 no cerebelo. Podemos concluir que a HI pré-natal aumentou o número de células imunorreativas para a caspase-3 em um período crítico do desenvolvimento da oligodendroglia no cerebelo, e que a diminuição de progenitores de oligodendrócitos no cerebelo decorrente do insulto pré-natal visto em trabalhos anteriores, pode estar relacionada a morte celular por apoptose, embora não se possa descartar a hipótese da participação dessas células que apresentam caspase-3 clivada em outros eventos não apoptóticos desencadeados pela hipóxia-isquemia.