910 resultados para In situ characterization


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Este vídeo forma parte de la Enciclopedia Audiovisual de las Ciencias y las Técnicas, y se estructura en capítulos de cuatro minutos. Cada capítulo expone el estudio de un objeto o fenómeno científico y propone: recordatorios, definiciones, exploraciones para entender mejor un funcionamiento, animaciones para representar fenómenos complejos, descubrimientos y aplicaciones y puntos que remiten a otros capítulos de la enciclopedia directamente relacionados con el tema que se trata. Los capítulos incluidos en este volumen son: el electrocardiograma; la ecografía; el microscopio electrónico; la radiografía; el escáner y la resonancia magnética; las tomografías médicas; el SIDA; el paludismo; la diabetes; la miopía; el infarto; la arterioesclerosis, y el cáncer.

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Este vídeo forma parte de la Enciclopedia Audiovisual de las Ciencias y las Técnicas, y se estructura en capítulos de cuatro minutos. Cada capítulo expone el estudio de un objeto o fenómeno científico y propone: recordatorios, definiciones, exploraciones para entender mejor un funcionamiento, animaciones para representar fenómenos complejos, descubrimientos y aplicaciones y puntos que remiten a otros capítulos de la enciclopedia directamente relacionados con el tema que se trata. Los capítulos incluidos en este volumen son: el lector láser; el televisor; el magnetoscopio; la cámara de vídeo; el tubo catódico; el receptor de radio; el amplificador; los circuitos integrados; el transistor; el efecto transistor; el diodo; los semiconductores y, el circuito lógico.

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Este vídeo forma parte de la Enciclopedia Audiovisual de las Ciencias y las Técnicas, y se estructura en capítulos de cuatro minutos. Cada capítulo expone el estudio de un objeto o fenómeno científico y propone: recordatorios, definiciones, exploraciones para entender mejor un funcionamiento, animaciones para representar fenómenos complejos, descubrimientos y aplicaciones y puntos que remiten a otros capítulos de la enciclopedia directamente relacionados con el tema que se trata. Los capítulos incluidos en este volumen son: la cámara fotográfica; la luz de colores; la propagación de la luz; el láser; las ondas electromagnéticas; los rayos X y los rayos gamma; el sónar; el radar; las ondas sonoras; la guitarra; el micrófono; el altavoz; la modulación y la frecuencia, y, las antenas.

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Laboratory measurements of the attenuation and velocity dispersion of compressional and shear waves at appropriate frequencies, pressures, and temperatures can aid interpretation of seismic and well-log surveys as well as indicate absorption mechanisms in rocks. Construction and calibration of resonant-bar equipment was used to measure velocities and attenuations of standing shear and extensional waves in copper-jacketed right cylinders of rocks (30 cm in length, 2.54 cm in diameter) in the sonic frequency range and at differential pressures up to 65 MPa. We also measured ultrasonic velocities and attenuations of compressional and shear waves in 50-mm-diameter samples of the rocks at identical pressures. Extensional-mode velocities determined from the resonant bar are systematically too low, yielding unreliable Poisson's ratios. Poisson's ratios determined from the ultrasonic data are frequency corrected and used to calculate the sonic-frequency compressional-wave velocities and attenuations from the shear- and extensional-mode data. We calculate the bulk-modulus loss. The accuracies of attenuation data (expressed as 1000/Q, where Q is the quality factor) are +/- 1 for compressional and shear waves at ultrasonic frequency, +/- 1 for shear waves, and +/- 3 for compressional waves at sonic frequency. Example sonic-frequency data show that the energy absorption in a limestone is small (Q(P) greater than 200 and stress independent) and is primarily due to poroelasticity, whereas that in the two sandstones is variable in magnitude (Q(P) ranges from less than 50 to greater than 300, at reservoir pressures) and arises from a combination of poroelasticity and viscoelasticity. A graph of compressional-wave attenuation versus compressional-wave velocity at reservoir pressures differentiates high-permeability (> 100 mD, 9.87 X 10(-14) m(2)) brine-saturated sandstones from low-permeability (< 100 mD, 9.87 X 10 (14) m(2)) sandstones and shales.

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We investigated diurnal nitrate (NO3-) concentration variability in the San Joaquin River using an in situ optical NO3- sensor and discrete sampling during a 5-day summer period characterized by high algal productivity. Dual NO3- isotopes (delta N-15(NO3) and delta O-18(NO3)) and dissolved oxygen isotopes (delta O-18(DO)) were measured over 2 days to assess NO3- sources and biogeochemical controls over diurnal time-scales. Concerted temporal patterns of dissolved oxygen (DO) concentrations and delta O-18(DO) were consistent with photosynthesis, respiration and atmospheric O-2 exchange, providing evidence of diurnal biological processes independent of river discharge. Surface water NO3- concentrations varied by up to 22% over a single diurnal cycle and up to 31% over the 5-day study, but did not reveal concerted diurnal patterns at a frequency comparable to DO concentrations. The decoupling of delta N-15(NO3) and delta O-18(NO3) isotopes suggests that algal assimilation and denitrification are not major processes controlling diurnal NO3- variability in the San Joaquin River during the study. The lack of a clear explanation for NO3- variability likely reflects a combination of riverine biological processes and time-varying physical transport of NO3- from upstream agricultural drains to the mainstem San Joaquin River. The application of an in situ optical NO3- sensor along with discrete samples provides a view into the fine temporal structure of hydrochemical data and may allow for greater accuracy in pollution assessment.

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A new method of measuring the total conductivity of atmospheric air is described. It depends on determination of the electrical relaxation time of a horizontal wire, mounted between two insulators, which is initially grounded and then allowed to charge freely. The total air conductivity derived is compared with that from an ion mobility spectrometer. Results from the two techniques agreed to within 1.2 fS m(-1). (c) 2006 American Institute of Physics.

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A method for in situ detection of atmospheric turbulence has been developed using an inexpensive sensor carried within a conventional meteorological radiosonde. The sensor-a Hall effect magnetometer-was used to monitor the terrestrial magnetic field. Rapid time scale (10 s or less) fluctuations in the magnetic field measurement were related to the motion of the radiosonde, which was strongly influenced by atmospheric turbulence. Comparison with cloud radar measurements showed turbulence in regions where rapid time-scale magnetic fluctuations occurred. Reliable measurements were obtained between the surface and the stratosphere.

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In paper 1, we showed that the Heliospheric Imager (HI) instruments on the pair of NASA STEREO spacecraft can be used to image the streamer belt and, in particular, the variability of the slow solar wind which originates near helmet streamers. The observation of intense intermittent transient outflow by HI implies that the corresponding in situ observations of the slow solar wind and corotating interaction regions (CIRs) should contain many signatures of transients. In the present paper, we compare the HI observations with in situ measurements from the STEREO and ACE spacecraft. Analysis of the solar wind ion, magnetic field, and suprathermal electron flux measurements from the STEREO spacecraft reveals the presence of both closed and partially disconnected interplanetary magnetic field lines permeating the slow solar wind. We predict that one of the transients embedded within the second CIR (CIR‐D in paper 1) should impact the near‐Earth ACE spacecraft. ACE measurements confirm the presence of a transient at the time of CIR passage; the transient signature includes helical magnetic fields and bidirectional suprathermal electrons. On the same day, a strahl electron dropout is observed at STEREO‐B, correlated with the passage of a high plasma beta structure. Unlike ACE, STEREO‐B observes the transient a few hours ahead of the CIR. STEREO‐A, STEREO‐B, and ACE spacecraft observe very different slow solar wind properties ahead of and during the CIR analyzed in this paper, which we associate with the intermittent release of transients.