Reabsorción radicular externa apical en incisivos y caninos superiores e inferiores sometidos a tratamiento de Ortodoncia en etapa inicial

La Reabsorción radicular externa apical es un proceso inflamatorio común asociado con el tratamiento de ortodoncia. El objetivo de este estudio fue comparar la magnitud de la RREA de los incisivos y caninos superiores e inferiores en pacientes sometidos a la fase inicial del tratamiento de ortodoncia con tres diferentes tipos de brackets. La muestra consistió en 23 casos de pacientes con edades comprendidas entre 12 y 27 años, fueron divididos aleatoriamente en 3 grupos. Grupo I (n=9; 5 mujeres y 4 varones), utilizando brackets pasivos de autoligado Damon Q Grupo II (n= 8; 4 mujeres y 4 varones) utilizando brackets convencionales prescripción Roth y MBT. Grupo III (n=6; 4 mujeres y 2 varones) utilizando brackets Biofuncional QR. Se analizaron 264 dientes (caninos e incisivos superiores e inferiores) mediante el uso de tomografía computarizada de haz cónico (NewTom VGi Cone Beam 3D Imaging), con el escáner NNT Viewer (versión 4.6 NewTom). Los resultados obtenidos indican que la media de reabsorción se mostró distinta para los diferentes protocolos de tratamiento, así como diferente de acuerdo a la pieza analizada, sin embargo, la prueba de ANOVA no encontró diferencias estadísticamente significativas al comparar la media de reabsorción de cada pieza por tipo de brackets empleados o tratamiento realizado (p >0,05). Se concluye que la RREA se ha producido en todos los dientes evaluados, durante los 6 primeros meses de tratamiento y el diseño del bracket (autoligado pasivo, convencional o QR) no influye en el grado de reabsorción radicular.

Identificación de neospora caninum en materia fecal de 60 caninos en hatos lecheros en el municipio el Rosal, Cundinamarca

Bogotá (Colombia): Universidad de La Salle. Facultad de Ciencias Agropecuarias. Programa de Medicina Veterinaria

Evaluación de las técnicas quirúrgicas medial VS la técnica lateral en ovariohisterectomía en la especie canina en el municipio de Camoapa, 2014.

El presente trabajo de investigación fue realizado en la ciudad de Camoapa, municipio del Departamento de Boaco, Republica de Nicaragua; el mismo que tuvo como objetivo determinar la técnica quirúrgica de esterilización más adecuada para una pronta recuperación del paciente, tomándose como muestra a 12 hembras canina, cuyas edades fueron comprendidas desde los 6 meses hasta los 24 meses de edad de toda raza. Las técnicas empleadas fueron la técnica medial y la técnica lateral, el tamaño requerido de la población para este trabajo fue de 12 hembras caninas las cuales se dividieron en cuatro grupos de 3 animales para cada grupo, generando 7 observaciones para cada grupo. Dichas intervenciones siguieron un protocolo de asepsia, anestesia y quirúrgico. De esta manera de acuerdo, a los procedimientos estadísticos se desprendieron las siguientes conclusiones: no existe una interacción entre la edad, las técnicas y el tiempo de recuperación del paciente post–quirurgico. Por otra parte, al evaluar la variable de cicatrización, se demostró que los caninos de menor edad tienen una mejor respuesta a la intervención quirúrgica. Y en conclusión para tener una cicatrización en menor tiempo, se recomienda aplicar una laparotomía lateral, en perras de cualquier edad, por cuanto la técnica utilizada y el tiempo de cicatrización se comportan de manera independiente en relación a la edad del animal.

Modelo de canal para caracterizar la señal dispersada por un parque eólico en la banda UHF e influencia sobre la calidad de servicio de DVB-T

288 p. : il.

Mechanistic study on spraying of blended biodiesel using phase Doppler anemometry

Droplet size and dynamics of blended palm oil-based fatty acid methyl ester (FAME) and diesel oil spray were mechanistically investigated using a phase Doppler anemometry. A two-fluid atomizer was applied for dispersing viscous blends of blended biodiesel oil with designated flow rates. It was experimentally found that the atomizer could generate a spray with large droplets with Sauter mean diameters of ca. 30 mm at low air injection pressure. Such large droplets traveled with a low velocity along their trajectory after emerging from the nozzle tip. The viscosity of blended biodiesel could significantly affect the atomizing process, resulting in the controlled droplet size distribution. Blended biodiesel with a certain fraction of palm oil-based FAME would be consistently atomized owing to its low viscosity. However, the viscosity could exert only a small effect on the droplet velocity profile with the air injection pressure higher than 0.2 MPa.

The Superresolution Problem in Doppler Difference Laser Anemometry

info:eu-repo/semantics/published

Charge-state distribution and Doppler effect in an expanding photoionized plasma.

The charge state distributions of Fe, Na, and F are determined in a photoionized laboratory plasma using high resolution x-ray spectroscopy. Independent measurements of the density and radiation flux indicate unprecedented values for the ionization parameter ���¾=20 25 erg cm s-1 under near steady-state conditions. Line opacities are well fitted by a curve-of-growth analysis which includes the effects of velocity gradients in a one-dimensional expanding plasma. First comparisons of the measured charge state distributions with x-ray photoionization models show reasonable agreement.

Doppler cooling of gallium atoms: 1. Fine structure effects and transient coherences

A realistic model of the dipole radiation forces in transverse Doppler cooling (with a s+-s- laser configuration) of an atomic beam of group 13 elements is studied within the quantum-kinetic equation framework. The full energy level sub-structure for such an atom with I = 0 (such as 66Ga) is analysed. Two cooling strategies are investigated; the first involving the 2P3/2 ? 2D5/2 transition and the second a dual laser cooling experiment involving transitions 2P1/2 and 2P3/2 ? 2S1/2. The latter scheme creates a velocity-independent dark-state resonance that inhibits a steady-state dipole cooling force. However, time-dependent calculations show that transient cooling forces are present that could be exploited for laser cooling purposes in pulsed laser fields.

Stokes imaging, Doppler mapping and Roche tomography of the AM Herculis system V834 Cen

We report on new simultaneous phase-resolved spectroscopic and polarimetric observations of the polar (AM Herculis star) V834 Cen during a high state of accretion. Strong emission lines and high levels of variable circular and linear polarization are observed over the orbital period. The polarization data are modelled using the Stokes imaging technique of Potter et al. The spectroscopic emission lines are investigated using the Doppler tomography technique of Marsh and Horne and the Roche tomography technique of Dhillon and Watson. Up to now, all three techniques have been used separately to investigate the geometry and accretion dynamics in cataclysmic variables. For the first time, we apply all three techniques to simultaneous data for a single system. This allows us to compare and test each of the techniques against each other and hence to derive a better understanding of the geometry, dynamics and system parameters of V834 Cen.

Doppler cooling of gallium atoms: 2. Simulation in complex multilevel systems

This paper derives a general procedure for the numerical solution of the Lindblad equations that govern the coherences arising from multicoloured light interacting with a multilevel system. A systematic approach to finding the conservative and dissipative terms is derived and applied to the laser cooling of p-block elements. An improved numerical method is developed to solve the time-dependent master equation and results are presented for transient cooling processes. The method is significantly more robust, efficient and accurate than the standard method and can be applied to a broad range of atomic and molecular systems. Radiation pressure forces and the formation of dynamic dark states are studied in the gallium isotope 66Ga.

The Doppler shadow of WASP-3b. A tomographic analysis of Rossiter-McLaughlin observations

Context. Hot-Jupiter planets must form at large separations from their host stars where the temperatures are cool enough for their cores to condense. They then migrate inwards to their current observed orbital separations. Different theories of how this migration occurs lead to varying distributions of orbital eccentricity and the alignment between the rotation axis of the star and the orbital axis of the planet. Aims: The spin-orbit alignment of a transiting system is revealed via the Rossiter-McLaughlin effect, which is the anomaly present in the radial velocity measurements of the rotating star during transit due to the planet blocking some of the starlight. In this paper we aim to measure the spin-orbit alignment of the WASP-3 system via a new way of analysing the Rossiter-McLaughlin observations. Methods: We apply a new tomographic method for analysing the time variable asymmetry of stellar line profiles caused by the Rossiter-McLaughlin effect. This new method eliminates the systematic error inherent in previous methods used to analyse the effect. Results: We find a value for the projected stellar spin rate of v sin i = 13.9 ± 0.03 km s-1 which is in agreement with previous measurements but has a much higher precision. The system is found to be well aligned, with ? = 5-5+6° which favours an evolutionary history for WASP-3b involving migration through tidal interactions with a protoplanetary disc. From comparison with isochrones we put an upper limit on the age of the star of 2 Gyr.