Investigations of Optical Interaction Processes in Certain Photonic Materials Using Z-scan and Thermal Lens Techniques

International School of Photonics, Cochin University of Science and Technology

Studies on the, Physical Aspects of the Mud Banks along the Kerala Coast

A detailed survey of the present knowledge on the physical aspects of the mud banks has been presented in chapter 1.The physical geographical and geological aspects of the kerala coast, the shore-line and the sea bed and the various views on the formation,movements and dissipation of the mud banks have been discussed.The scope of the present work and a description of the area of study have also been given in this chapter. The horizontal and vertical distribution and the seasonal variations of the concentration of suspended matter in the mud bank region are discussed in chapter 3.it is seen that the mud bank reses above the bottom in the form of a ridged ,irregular,solid come with a flat top. Chapter vi deals with waves and currents in the region of the mud bank. The orientation of the breakers on either side of the mud bank suggests the possibility of formation of opposing alongshore currents and convergence of energy caused by wave refraction.The distribution of currents during the formative nature and dissipating stages of the mud bank show that the converging alongshore currents give rise to offshore flows

Studies on the littoral processes in relation to stability of beaches around Cchin

The coastal and nearshore areas have played vital role in the trade and economic development of coastal nations since ancient times. In recent years, the demands for utilization of these areas have increased for purposes of navigation, setting up of offshore structures for oil industry, exploitation of the available fishery and mineral resources, and to provide recreational facilities along the coast as a part of the coastal zone management. It is in this context the studies on nearshore processes receive greater priorities. Stability of beaches is controlled by the interaction of various physical parameters such as winds, waves, currents, tides and the nature and constituents of the beaches. The results of studies carried out by the author on the dynamical effects of these environmental parameters on the shoreline processes along the beaches around Cochin are presented in this thesis. The section of the coast investigated is about 57 km of shore from Azhikode to Anthakaranazhi situated on the central Kerala coast. Four regions namely Narakkal, Malipuram, Fort Cochin and Anthakaranazhi were chosen for detailed study

Studies On Sediment Transport In The Surf Zone Along Certain Beaches Of Kerala

Sediment transport in the nearshore areas is an important process in deciding the coastline stability. The design and effective maintenance of navigable waterways, harbours and marine structures depend on the stability of the sediment substrate and the nature of sedimentation in the nearshore zone. The nearshore zone is a complex environment and the exact relationships existing between water motions and the resulting sediment transports are not well understood. During the rough weather season, when the sediment movement is considerable, processes occurring in the nearshore area are much less understood. Moreover, there is a general lack of field measurements, especially during the time of severe storm conditions. The increasing pressures and the concern on the preservation of the valuable coastal environment have led to the development of shore protection programmes. Conservation not only demands knowledge of what needs to be done, but also requires the basic processes to be fully understood. Considering the fragile nature of barrier beaches and intense occupancy of these areas by man, these coastal features have long been a subject of study by coastal oceanographers, geomorphologists and engineers. The present study is an attempt to understand the sediment movement in relation to beach dynamics, especially in the surf zone, along some part of Kerala coast and the response of the beaches to various forcing functions over different seasons

Growth of metal and semiconductor nanostructures for nonlinear optical applications

Nonlinear optics has been a rapidly growing field in recent decades since the invention of lasers. The systematic progress in the laser technology increases our efficiency in the generation and control of coherent optical radiations. Nonlinear optics is based on the study ofeffects and phenomena related to the interaction of intense coherent light radiation with matter. Compared to other light sources laser radiation can provide high directionality, high monochromaticiry, high brightness and high photon degeneracy. At such a very intense incident beam, the matter responds in a nonlinear manner to the incident radiation fields, which endows the media :1 characteristic to change the refractive index or absorption coe fflcient of the media or the wavelength, or the frequency of the incident electromagnetic waves. This thesis encompasses the fabrication of nonlinear optical devices based on semiconductor and metal nanostructures. The presented work focus on the experimental and theoretical discussions on nonlinear optical effects especially nonlinear absorption and refraction exhibitted by metal and semiconductor nanostructures

Variation in radio refractivity index associated with formation of low - pressure systems

Numerous low - pressure systems form in the Arabian Sea and Bay of Bengal. These low-pressure systems are highly useful in bringing the rainfall over the Indian sub continent. The developments of these systems are accompanied by the reduction in air temperature and an increase in atmospheric humidity. The radio refractivity, which is a function of the atmospheric pressure, temperature and humidity, also changes following the development of these systems. Variation of radio refractive index and its vertical gradient are analysed for many low pressure systems formed over the Arabian Sea and Bay of Bengal. It is found that the atmosphere becomes super refractive associated with the formation of these systems, caused by the increase in humidity and decrease in temperature. The maximum gradient is observed near the surface layers, especially in the lowest 1 km. Super refraction leads to increased radar detection range and extension of radio horizon

3D Simultaneous Inversion for Seismic Structure and Local Hypocenters in Germany under Consideration of Seismic Anisotropy in the Upper Mantel

The main task of this work has been to investigate the effects of anisotropy onto the propagation of seismic waves along the Upper Mantle below Germany and adjacent areas. Refraction- and reflexion seismic experiments proved the existence of Upper Mantle anisotropy and its influence onto the propagation of Pn-waves. By the 3D tomographic investigations that have been done here for the crust and the upper mantle, considering the influence of anisotropy, a gap for the investigations in Europe has been closed. These investigations have been done with the SSH-Inversionprogram of Prof. Dr. M. Koch, which is able to compute simultaneously the seismic structure and hypocenters. For the investigation, a dataset has been available with recordings between the years 1975 to 2003 with a total of 60249 P- and 54212 S-phase records of 10028 seismic events. At the beginning, a precise analysis of the residuals (RES, the difference between calculated and observed arrivaltime) has been done which confirmed the existence of anisotropy for Pn-phases. The recognized sinusoidal distribution has been compensated by an extension of the SSH-program by an ellipse with a slow and rectangular fast axis with azimuth to correct the Pn-velocities. The azimuth of the fast axis has been fixed by the application of the simultaneous inversion at 25° - 27° with a variation of the velocities at +- 2.5 about an average value at 8 km/s. This new value differs from the old one at 35°, recognized in the initial residual analysis. This depends on the new computed hypocenters together with the structure. The application of the elliptical correction has resulted in a better fit of the vertical layered 1D-Model, compared to the results of preceding seismological experiments and 1D and 2D investigations. The optimal result of the 1D-inversion has been used as initial starting model for the 3D-inversions to compute the three dimensional picture of the seismic structure of the Crust and Upper Mantle. The simultaneous inversion has showed an optimization of the relocalization of the hypocenters and the reconstruction of the seismic structure in comparison to the geology and tectonic, as described by other investigations. The investigations for the seismic structure and the relocalization have been confirmed by several different tests. First, synthetic traveltime data are computed with an anisotropic variation and inverted with and without anisotropic correction. Further, tests with randomly disturbed hypocenters and traveltime data have been proceeded to verify the influence of the initial values onto the relocalization accuracy and onto the seismic structure and to test for a further improvement by the application of the anisotropic correction. Finally, the results of the work have been applied onto the Waldkirch earthquake in 2004 to compare the isotropic and the anisotropic relocalization with the initial optimal one to verify whether there is some improvement.

A Motion compensated filtering approach to remove sunlight flicker in shallow water images

A common problem in video surveys in very shallow waters is the presence of strong light fluctuations, due to sun light refraction. Refracted sunlight casts fast moving patterns, which can significantly degrade the quality of the acquired data. Motivated by the growing need to improve the quality of shallow water imagery, we propose a method to remove sunlight patterns in video sequences. The method exploits the fact that video sequences allow several observations of the same area of the sea floor, over time. It is based on computing the image difference between a given reference frame and the temporal median of a registered set of neighboring images. A key observation is that this difference will have two components with separable spectral content. One is related to the illumination field (lower spatial frequencies) and the other to the registration error (higher frequencies). The illumination field, recovered by lowpass filtering, is used to correct the reference image. In addition to removing the sunflickering patterns, an important advantage of the approach is the ability to preserve the sharpness in corrected image, even in the presence of registration inaccuracies. The effectiveness of the method is illustrated in image sets acquired under strong camera motion containing non-rigid benthic structures. The results testify the good performance and generality of the approach

Retinoscopía estática: variabilidad interobservadores entre docentes y estudiantes de optometría en una institución universitaria de Bogotá D.C.

Introducción: el gold estándar para el error refractivo es la retinoscopía. Los docentes de optometría al evaluar estudiantes, aceptan una diferencia de ±0,50D en la refracción pero no se ha evaluado estadísticamente si es adecuado para ametropías bajas y altas. El objetivo fue cuantificar el grado de concordancia interobservadores en retinoscopía estática entre docentes y estudiantes, para ametropías altas y bajas. Metodología: estudio de concordancia entre 4 observadores en 40 ojos, 20 con ametropías altas y 20 con bajas; muestreo no probabilístico por conveniencia. Análisis estadístico con coeficiente de correlación intraclase, confiabilidad 95%, poder 90%, y con método gráfico de límites de acuerdo al 95%. Resultados: concordancia para el equivalente esférico entre docentes 0,96 y entre estudiantes 0,56. En estudiantes concordancia de 0,89 para defectos refractivos bajos y docentes 0,96 para defectos altos. Concordancia entre cuatro examinadores 0,78, defectos bajos 0,86 y para altos 0,67. Margen de error entre docentes ±0,87D y estudiantes ±3,15D. En defectos bajos ±0,61D para docentes y ±0,80D para estudiantes y en defectos altos ±1,10D y ±4,22D respectivamente. Discusión: hubo mayor confiabilidad en retinoscopía entre profesionales experimentados. Se comparó la concordancia entre docentes y estudiantes, por eso puede haberse encontrado menor concordancia que la descrita por otros estudios que compararon entre profesionales a pesar haber sido elegidos por sus buenas calificaciones. Se deben formular estrategias de enseñanza que permitan reducir los márgenes de error obtenidos y mejorar la concordancia entre docentes y estudiantes.

Correlación entre el resultado refractivo post-catarata con la predicción biométrica pre-operatoria

La cirugía de cataratas por Facoemulsificación es tal vez uno de los procedimientos más realizados en la práctica de oftalmología general, sin embargo el resultado refractivo de esta cirugía no siempre llena las expectativas del oftalmólogo y del paciente, es por esto que es de gran importancia observar los resultados post quirúrgicos obtenidos y las distintas variables que pudieron influir en dicho resultado. Objetivo: determinar la capacidad predictiva de la formula biométrica empleada en el preoperatorio con el resultado refractivo post operatorio expresada en porcentajes. Materiales y métodos: se realizó un estudio de correlación basándose en la refracción prevista por la biometría y la refracción encontrada en el post operatorio. Se analizó los diferentes grupos de pacientes miopes, hipermétropes y emétropes en de los rangos de 0,50D, 0,75 D y 1,00D. Resultados: el porcentaje de pacientes que presento 0,50D de diferencia con el previsto fue de 57,7% para el total, 100% para hipermétropes, 53,1% para emétropes, 56,3% para miopes. En el rango de 0,75D 71,2% para el total, 62,5% para emétropes y 81,3% para miopes. En el rango de 1,00D 82,7% para el total, 75% para emétropes y 93,8% para miopes. Conclusiones: la formula SRK/T presento un buen desempeño en todos los grupos encontrándose resultados concordantes con los descritos en la literatura.

Comparación de grosor macular y grado de miopía en grupo de pacientes de la Fundación Oftalmológica Nacional

OBJETIVOS: Comparar las medidas de grosor macular, medido por HD-OCT Cirrus®, en pacientes de la Fundación Oftalmológica Nacional con miopía baja y alta. MÉTODOS: Estudio transversal analítico, en el que se incluyeron pacientes con miopía alta, definida como defecto esférico mayor a – 6.0 dioptrías (D), y pacientes con miopía baja, definida como defecto esférico entre -1.00 D y -6.00 D; a los que se le realizó mapa de grosores maculares con el HD-OCT Cirrus®, y se compararon las medias de los grosores (1, 3 y 6 mm). RESULTADOS: Un total de 128 ojos de pacientes entre 12 y 80 años fueron incluidos; 64 ojos en grupo de miopes bajos y 64 ojos en grupo de miopes altos. La media de edad fue: 37.3 y 38.4 años, y el defecto esférico promedio fue de 2.2 D y 11.5 D, respectivamente. El promedio de grosores en mácula interna (319.9 vs. 307.87 micras, P=0.002), y mácula externa (276.08 vs. 270.23 micras, P=0.047) fue significativamente mayor en el grupo de miopía baja que en el de miopía alta. Sin embargo la media del grosor macular central (1 mm) no tuvo diferencia (261.25 vs. 262 micras P=0.891). CONCLUSIÓN: Este estudio muestra que el grosor macular de 3 y 6 mm centrales es más delgado en miopes altos, pero en 1 mm central es similar que en miopes bajos. En los pacientes estudiados no se encontró diferencia en grosores maculares según género o subgrupos de edad.

Plotino y Grosseteste: El neoplatonismo en la cosmología medieval

En este trabajo se estudia el caso de la cosmología del filósofo y científico Robert Grosseteste como un ejemplo de la notable influencia del neoplatonismo en la ciencia medieval. Uno de los propósitos de la cosmología de Grosseteste consistió en explicar la secuencia efectiva de la creación del cosmos. Sostengo que la explicación que ofrece Grosseteste acerca de la creación es una expresión renovada de algunas ideas de Plotino a propósito de cómo el Uno engendra lo múltiple. Me interesa resaltar tres aspectos de la estrecha relación entre el sistema cosmológico de Grosseteste y el sistema metafísico de Plotino: (1) Unidad de principio, (2) Mecanismos de generación y (3) Unidad del sistema.

Reconocimiento geofísico del deslizamiento de Rosiana (depresión de Tirajana, Gran Canaria)

The landslide of Rosiana is considered the largest slope movement amongst those known in historical times in Gran Canana, Canary Islands. It has been activated at least 4 times in the last century, and in the movement of 1956, when about 3.106 m3 of materials were involved, 250 people had to be evacuated and many buildings were destroyed. The present geological hazard has lead to specific studies of the phenomenon which, once characterised, can be used as a guide for the scientific and technical works that are to be made in this or similar areas. This paper wants to increase the knowledge about the unstable mass of Rosiana by using geophysical techniques based on the method of seismic by refraction. The geophysical measues have been interpreted with the aid of the available geomorphologic data, thus obtaining a first approximation to the geometry of the slope movements

Investigación geofísica de los paleovalles pleistocenos del NE de Cataluña: el ejemplo de la Riera de Tossa (Costa Brava meridional)

The geometry of Riera de Tossa (Costa Brava, Catalonia) Pleistocene paleovalley has been studied by two geophysical prospecting methods: vertical electric sounding (VES-DC) and seismic refraction. The results show the existence of a sudden slope change of the thalweg that permits to differentiate two sections where erosion processes operated in unequal intensity. Based on geological and geomorphological available data, it can be inferred that this slope rupture is caused by the litological control imposed by the alineation of resistant materials, which limited the headward erosion extend of the creek during the Upper Pleistocene

The role of eddies in driving the tropospheric response to stratospheric heating perturbations

A simplified general circulation model has been used to investigate the chain of causality whereby changes in tropospheric circulation and temperature are produced in response to stratospheric heating perturbations. Spinup ensemble experiments have been performed to examine the evolution of the tropospheric circulation in response to such perturbations. The primary aim of these experiments is to investigate the possible mechanisms whereby a tropospheric response to changing solar activity over the 11-yr solar cycle could be produced in response to heating of the equatorial lower stratosphere. This study therefore focuses on a stratospheric heating perturbation in which the heating is largest in the tropics. For comparison, experiments are also performed in which the stratosphere is heated uniformly at all latitudes and in which it is heated preferentially in the polar region. Thus, the mechanisms discussed have a wider relevance for the impact of stratospheric perturbations on the troposphere. The results demonstrate the importance of changing eddy momentum fluxes in driving the tropospheric response. This is confirmed by the lack of a similar response in a zonally symmetric model with fixed eddy forcing. Furthermore, it is apparent that feedback between the tropospheric eddy fluxes and tropospheric circulation changes is required to produce the full model response. The quasigeostrophic index of refraction is used to diagnose the cause of the changes in eddy behavior. It is demonstrated that the latitudinal extent of stratospheric heating is important in determining the direction of displacement of the tropospheric jet and storm track.