Results of various studies made with the NCAR Thermospheric General Circulation Model (TGCM) (invited review)

The NCAR thermospheric general circulation model (TGCM) has been used for a variety of thermospheric dynamic studies. It has also been used to compare model predictions with measurements made from various ground-based Fabry-Perot interferometer stations, incoherent scatter radar stations and the Dynamics Explorer satellites. The various input and output features of the model are described. These include the specification of solar EUV fluxes, and descriptions of empirical models to specify auroral particle precipitation, ion drag, and magnetospheric convection. Results are presented for solstice conditions giving the model perturbation temperature and circulation response to solar heating forcing alone and also with the inclusion of magnetospheric convections for two different dawn-dusk potential drops, 20 and 60 kV respectively. Results at two constant pressure levels Z =+1 at 300 km and Z= -4 at 120 km are presented for both the winter and summer polar cap regions. The circulation over the Northern Hemisphere polar cap in both the upper and lower thermosphere are presented along with a figure showing that the circulation is mainly a non-divergent irrotational flow responding to ion drag. The results of a study made on the Southern Hemisphere polar cap during October 1981 where Dynamics Explorer satellite measurements of winds, temperature and composition are compared to TGCM predictions are also presented. A diagnostic package that has been developed to analyze the balance of forces operating in the TGCM is presented next illustrating that in the F-region ion drag and pressure provide the main force balance and in the E-region ion drag, pressure and the coriolis forces provide the main balance. The TGCM prediction for the June 10, 1983 total solar eclipse are next presented showing a thermospheric disturbance following the path of totality. Finally, results are presented giving the global circulation, temperature and composition structure of the thermosphere for solar minimum conditions at equinox with 60 kV magnetospheric convection forcing at high latitudes

Orbital atmospheric physics and dynamics

There are two ways of modeling the upper atmosphere. One is the empirical model that makes use of experimental data on means and excursions from the mean and fits the data in a self-consistent manner. The other approach is to deal directly with the physical processes. This is difficult since what is happening is extremely complex. Data measured using an interferometer to give Doppler shifts of airglow lines showed 300 to 800 m/sec winds with a complex structure in the upper region of the thermosphere at high latitudes. Ionospheric electric fields, strongly influenced by interaction with the solar wind, drive the ionized component and large neutral winds result due to momentum transfer between the charged particles and the neutrals. Frictional heating results from movement of ions through the neutrals, which also influences the compositional structure. These are examples of the complex interactions involved. The NCAR General Circulation Model (tropospheric) was adapted for use at thermospheric altitudes: the Thermospheric General Circulation Model (TGCM). The model makes use partly of primitive equations and partly of empirical data for some quantities such as electron density, magnetic field, and ion drift

Development of production systems for raw cassava starch bioconversion in novel bioreactors with cells immobilized in loofa (Luffa cylindrica) sponge

Thesis (Ph. D. in Agriculture)--University of Tsukuba, (A), no. 3357, 2004.3.25Includes bibliographical reference

Un estudio sobre las nociones de conservación que tienen estudiantes universitarios

En educación en ciencias, la idea de conservación y los principios asociados presentan dificultades en el aprendizaje. La idea de conservación es central en ciencias, en particular en Física, porque está implicada en principios fundamentales, los cuales resultan útiles para describir y predecir fenómenos. En este trabajo, se propone estudiar, en forma exploratoria, las ideas que tienen los estudiantes universitarios de primer año de Ingeniería, sobre el concepto de conservación. Se diseñó un cuestionario con preguntas abiertas y preguntas cerradas con justificación. Los registros se analizaron a partir de categorías emergentes y categorías encontradas en investigaciones anteriores. Los resultados preliminares muestran que la idea de conservación se asocia a “algo constante”, “inicial igual a final”; también se observa el uso del tiempo como recurso explicativo

Applications of a Venus thermospheric circulation model

A variety of Pioneer Venus observations suggest a global scale, day-to-night Venus thermospheric circulation. Model studies of the dynamics and energetics of the Venus thermosphere are presented in order to address new driving, mixing and cooling mechanisms for an improved model simulation. The adopted approach was to reexamine the circulation by first using a previous two dimensional code to quantify those physical processes which can be inferred from the Pioneer Venus observations. Specifically, the model was used to perform sensitivity studies to determine the degree to which eddy cooling, eddy or wave drag, eddy diffusion and 15 micrometer radiational cooling are necessary to bring the model temperature and composition fields into agreement with observations. Three EUV heating cases were isolated for study. Global temperature and composition fields in good agreement with Pioneer data were obtained. Large scale horizontal winds 220 m/s were found to be consistent with the observed cold nightside temperatures and dayside bulges of O, CO and CO2. Observed dayside temperatures were obtained by using a 7 to 19% EUV heating efficiency profile. The enhanced 15 micrometer cooling needed for thermal balance is obtained using the best rate coefficient available for atomic O collisional excitation of CO2(0,1,0). Eddy conduction was not found to be a viable cooling mechanism due to the weakened global circulation. The strong 15 micrometer damping and low EUV efficiency imply a very weak dependence of the general circulation to solar cycle variability. The NCAR terrestrial thermospheric general circulation model was adapted for Venus inputs using the above two dimensional model parameters, to give a three dimensional benchmark for future Venus modelling work

Report from upper atmospheric science

Most of the understanding of the thermosphere resulted from the analysis of data accrued through the Atmosphere Explorer satellites, the Dynamics Explorer 2 satellite, and observations from rockets, balloons, and ground based instruments. However, new questions were posed by the data that have not yet been answered. The mesosphere and lower thermosphere have been less thoroughly studied because of the difficulty of accessibility on a global scale, and many rather fundamental characteristics of these regions are not well understood. A wide variety of measurement platforms can be used to implement various parts of a measurement strategy, but the major thrusts of the International Solar Terrestrial Physics Program would require Explorer-class missions. A remote sensing mission to explore the mesosphere and lower thermosphere and one and two Explorer-type spacecraft to enable a mission into the thermosphere itself would provide the essential components of a productive program of exploration of this important region of the upper atomsphere. Theoretical mission options are explored

Study of the technique of stellar occultation

The results are reported of a study of the stellar occultation technique for measuring the composition of the atmosphere. The intensity of starlight was monitored during the occultation using the Wisconsin stellar ultraviolet photometers aboard the Orbiting Astronomical Observatory (OAO-A2). A schematic diagram of an occultation is shown where the change in intensity at a given wavelength is illustrated. The vertical projection of the attenuation region is typically 60 km deep for molecular oxygen and 30 km deep for ozone. Intensity profiles obtained during various occultations were analyzed by first determining the tangential columm density of the absorbing gases, and then Abel inverting the column densities to obtain the number density profile. Errors are associated with each step in the inversion scheme and have been considered as an integral part of this study

Transport des particules dans une géométrie réaliste

La thématique engagée dans cette recherche consiste donc à mettre en place une modélisation numérique fiable et complète du transport et du dépôt des particules dans un écoulement pulmonaire en se basant sur l’utilisation du code de calcul commercial CFD-ACE. Ce code intègre un solveur fluide qui résout les équations de Navier-Stokes incompressibles dans une formulation volumes finis. Le logiciel CFD-GEOM a été utilisé pour créer les surfaces en 3D de la géométrie générique du modèle de Weibel et ainsi générer le maillage non-structuré tétraèdrique en volumes finis. Dans le cadre de ce travail, il est supposé que le flux d’air est laminaire, stationnaire (ou instationnaire uniquement dans les modèles bronchiques) et incompressible ; les particules de diamètre 5 µm sont sphériques et sans interaction. Le pourcentage global et local du dépôt des particules dans les poumons peut s’exprimer comme une efficacité de dépôt et se définit par le rapport entre le nombre de particules déposées dans une région donnée et le nombre total de particules admises initialement à l’entrée de la conduite. L’efficacité de dépôt dépend fortement du nombre de Stokes d’entrée, des conditions d’admission en termes de profil de vitesse du fluide (nombre de Reynolds d’entrée), de la distribution et des caractéristiques des particules. Nous avons donc modélisé avec succès les écoulements ainsi que le transport et le dépôt de particules dans des configurations simples (modèles de Weibel) et des configurations réalistes (poumons de rat et du lapin) et ce que l’on en peut dire c’est que la simulation, bien que coûteuse (surtout pour le dépôt des particules), ne présente pas de difficultés insurmontables. Par contre l’obtention d’une géométrie réaliste et la génération du maillage associé reste une étape délicate

Reading habits in university students of careers in science and technology

La comunicación y difusión de la ciencia son una parte integral de la ciencia misma, de donde la lectura, como complemento, debe ser un aspecto constitutivo de la formación científica. Especialmente, la lectura de obras de divulgación puede transformarse en una excelente herramienta para la formación integral de los estudiantes de carreras científicas o tecnológicas. La presente investigación es un diagnóstico preliminar sobre los hábitos de lectura de 158 estudiantes de la Facultad de Ingeniería de la Universidad de Buenos Aires, llevado a cabo mediante una encuesta escrita. A partir de los resultados obtenidos, concluimos que los estudiantes no carecen de hábitos de lectura, pero que los mismos tienen poca interacción con su formación como profesionales. El libro impreso continúa siendo el vehículo principal de lectura, superando ampliamente a los formatos electrónicos. Surge un problema con la temática de la divulgación científica, pues los estudiantes manifiestan desconocer hasta la naturaleza misma de este género. Se propone para próximos trabajos la elaboración de estrategias de intervención que tomen en consideración los resultados de la presente investigación.Communication and dissemination of science are an integral part of science itself, where the reading, in addition, must be a constitutive aspect of scientific training. Especially, reading works of scientific divulgation can become an excellent tool for the integral formation of students in scientific or technological careers. This research is a preliminary diagnosis on the reading habits of 158 students of the Faculty of Engineering of the University of Buenos Aires, conducted by a written survey. From the results, we conclude that students are not whitout reading habits, but that they have little interaction with his training as a professionals. The printed book is still the main vehicle for reading, well above the electronic formats. A problem arises with the issue of scientific divulgation, as students manifest ignore to the very nature of this genre. Future work is proposed for the development of intervention strategies that take into account the results of this research