Interspecies variation in orbital bone structure of psittaciform birds (with emphasis on Psittacidae)

Objectives: This text presents an anatomical study of the normal bony orbital structure of a sample of different bird species belonging to the order Psittaciformes.Procedures: the bony anatomy of Psittaciformes' skulls was examined and described using cadavers of birds that were presented already dead to the Federal University of Parana, Brazil or had been euthanized for humane reasons. Dissections of the orbital cavity were performed under 2-4 x magnification, and descriptions of the orbital bones were made from observations of macerated skulls that had been boiled and cleaned. The present paper discusses the main features of the bony orbit of psittaciform birds, describing known anatomical information but also bringing new information, mainly concerning species differences that might help not only veterinary anatomists but also zoologists, clinicians, researchers, and students of veterinary ophthalmology to better comprehend this order of birds.Results and conclusions: Variations in the anatomic conformation of the bony elements of the orbit were observed in different species of Psittaciformes. Based on these differences, Psittaciformes were classified into two different groups. The first group of Psittaciformes shows an enclosed (complete) bony orbit formed by the junction of the orbital with the postorbital processes, creating a suborbital arch. The second group of Psittaciformes essentially lacked a suborbital arch, presenting an open (incomplete) bony orbit, typical of most modern birds. In the latter group, orbital and postorbital processes are present.

Pumped double quantum dot with spin-orbit coupling

We study driven by an external electric field quantum orbital and spin dynamics of electron in a one-dimensional double quantum dot with spin-orbit coupling. Two types of external perturbation are considered: a periodic field at the Zeeman frequency and a single half-period pulse. Spin-orbit coupling leads to a nontrivial evolution in the spin and orbital channels and to a strongly spin-dependent probability density distribution. Both the interdot tunneling and the driven motion contribute into the spin evolution. These results can be important for the design of the spin manipulation schemes in semiconductor nanostructures.

Selective formation of a polar incomplete coordination cage induced by remote ligand substituents

Instead of highly symmetrical T-symmetry cages common in self-assembly, the p-NMe2-substituted triphosphine CH3C{CH2P(4-C6H4NMe2)(3) gives open, polar C-3 symmetry cages [Ag-6(triphos)(4)X-3](3+) which lack one of the expected face-capping anions; despite its subtlety this difference occurs selectively in solution and two examples have been crystallographically characterised.

Essays in open economy macroeconomics with borrowing frictions

Cette thèse comporte trois essais en macroéconomie en économie ouverte et commerce international. Je considère tour à tour les questions suivantes: sous quelles conditions est-il optimal pour un pays de former une union économique? (essai 1); l'augmentation de la dispersion transversale des avoirs extérieurs nets des pays est-elle compatible avec une dispersion relativement stable des taux d'investissement? (essai 2); le risque de perte de marché à l'exportation du fait de l'existence des zones de commerce préférentiel joue t-il un rôle dans la décision des pays exclus de négocier des accords commerciaux à leur tour? (essai 3). Le premier essai examine les conditions d'optimalité d'une union économique. Il s'intéresse à une motivation particulière: le partage du risque lié aux fluctuations du revenu. Dans la situation initiale, les pays ont très peu d'opportunités pour partager le risque à cause des frictions: les marchés financiers internationaux sont incomplets et il n'y pas de mécanisme pour faire respecter les contrats de crédit entre pays. Dans ce contexte, une union économique apparait comme un arrangement qui pallie à ces frictions entre les pays membres seulement. Cependant, l'union dans son ensemble continue de faire face à ces frictions lorsqu'elle échange avec le reste du monde. L'arbitrage clé dans le modèle est le suivant. D'un coté, l'intégration économique permet un meilleur partage du risque entre pays membres et la possibilité pour le partenaire pauvre d'utiliser la ligne de crédit du partenaire riche en cas de besoin. De l'autre coté, l'union peut faire face à une limite de crédit plus restrictive parce que résilier la dette extérieure est moins coûteux pour les membres l'union. De plus, le fait que le partenaire pauvre peut utiliser la limite de crédit du partenaire riche génère une externalité négative pour ce dernier qui se retrouve plus fréquemment contraint au niveau des marchés internationaux des capitaux. En conformité avec les faits observés sur l'intégration économique, le modèle prédit que les unions économiques sont relativement peu fréquentes, sont plus susceptibles d'être créées parmi des pays homogènes, et généralement riches. Le deuxième essai porte sur la dispersion des avoirs extérieurs nets et la relation avec la dispersion des taux d'investissement. Au cours des récentes décennies, la dispersion croissante des déséquilibres extérieurs et les niveaux record atteints par certaines grandes économies ont reçu une attention considérable. On pourrait attribuer ce phénomène à une réduction des barrières aux mouvements internationaux des capitaux. Mais dans ce cas, il est légitime de s'attendre à une augmentation de la dispersion au niveau des taux d'investissement; ceci, parce que le financement des besoins en investissements constitue une raison fondamentale pour laquelle les pays échangent les capitaux. Les données indiquent cependant que la dispersion des taux d'investissement est restée relativement stable au cours des récentes décennies. Pour réconcilier ces faits, je construis un modèle d'équilibre général dynamique et stochastique où les pays sont hétérogènes en raison des chocs idiosyncratiques à leurs niveaux de productivité totale des facteurs. Au niveau des marchés internationaux des capitaux, le menu des actifs disponibles est restreint à une obligation sans risque et il n'y a pas de mécanisme pour faire respecter les contrats de crédit entre pays. A tout moment, un pays peut choisir de résilier sa dette extérieure sous peine d'exclusion financière et d'un coût direct. Ce coût direct reflète les canaux autres que l'exclusion financière à travers lesquels les pays en défaut sont pénalisés. Lorsque le modèle est calibré pour reproduire l'évolution de la dispersion transversale des avoirs extérieurs nets, il produit une dispersion relativement stable des taux d'investissement. La raison principale est que les incitations que les pays ont à investir sont liées à la productivité. Avec l'intégration financière, même si les opportunités d'emprunt se sont multipliées, les incitations à investir n'ont pas beaucoup changé. Ce qui permet de générer une dispersion accrue de la position des avoirs extérieurs nets des pays avec une dispersion relativement stable des taux d'investissement. Le troisième essai analyse un aspect de l'interdépendance dans la formation des accords commerciaux préférentiels: j'examine empiriquement si le risque de diversion des exportations en faveur des pays membres des zones de commerce préférentiel est un facteur déterminant dans la décision des pays exclus de ces accords de négocier un accord à leur tour. Je construis un indicateur qui mesure le potentiel de diversion des exportations auquel font face les pays et estime un modèle probit de formation des zones de commerce préférentiel créées entre 1961 et 2005. Les résultats confirment que les pays confrontés à un plus grand potentiel de détournement des échanges sont plus susceptibles de former une zone de commerce préférentiel à leur tour.

The method of least squares used to invert an orbit problem

Six parameters uniquely describe the orbit of a body about the Sun. Given these parameters, it is possible to make predictions of the body's position by solving its equation of motion. The parameters cannot be directly measured, so they must be inferred indirectly by an inversion method which uses measurements of other quantities in combination with the equation of motion. Inverse techniques are valuable tools in many applications where only noisy, incomplete, and indirect observations are available for estimating parameter values. The methodology of the approach is introduced and the Kepler problem is used as a real-world example. (C) 2003 American Association of Physics Teachers.

Extended cusp-like regions and their dependence on the Polar orbit, seasonal variations, and interplanetary conditions

Extended cusp-like regions (ECRs) are surveyed, as observed by the Magnetospheric Ion Composition Sensor (MICS) of the Charge and Mass Magnetospheric Ion Composition Experiment (CAMMICE) instrument aboard Polar between 1996 and 1999. The first of these ECR events was observed on 29 May 1996, an event widely discussed in the literature and initially thought to be caused by tail lobe reconnection due to the coinciding prolonged interval of strong northward IMF. ECRs are characterized here by intense fluxes of magnetosheath-like ions in the energy-per-charge range of _1 to 10 keV e_1. We investigate the concurrence of ECRs with intervals of prolonged (lasting longer than 1 and 3 hours) orientations of the IMF vector and high solar wind dynamic pressure (PSW). Also investigated is the opposite concurrence, i.e., of the IMF and high PSW with ECRs. (Note that these surveys are asking distinctly different questions.) The former survey indicates that ECRs have no overall preference for any orientation of the IMF. However, the latter survey reveals that during northward IMF, particularly when accompanied by high PSW, ECRs are more likely. We also test for orbital and seasonal effects revealing that Polar has to be in a particular region to observe ECRs and that they occur more frequently around late spring. These results indicate that ECRs have three distinct causes and so can relate to extended intervals in (1) the cusp on open field lines, (2) the magnetosheath, and (3) the magnetopause indentation at the cusp, with the latter allowing magnetosheath plasma to approach close to the Earth without entering the magnetosphere.

A Galactic ring of minimum stellar density near the solar orbit radius

We analyse the secular effects of a long-lived Galactic spiral structure on the stellar orbits with mean radii close to the corotation resonance. By test-particle simulations and different spiral potential models with parameters constrained on observations, we verified the formation of a minimum with amplitude ∼30–40 per cent of the background disc stellar density at corotation. Such a minimum is formed by the secular angular momentum transfer between stars and the spiral density wave on both sides of corotation. We demonstrate that the secular loss (gain) of angular momentum and decrease (increase) of mean orbital radius of stars just inside (outside) corotation can counterbalance the opposite trend of exchange of angular momentum shown by stars orbiting the librational points L4/5 at the corotation circle. Such secular processes actually allow steady spiral waves to promote radial migration across corotation. We propose some pieces of observational evidence for the minimum stellar density in the Galactic disc, such as its direct relation to the minimum in the observed rotation curve of the Galaxy at the radius r ∼ 9 kpc (for R0 = 7.5 kpc), as well as its association with a minimum in the distribution of Galactic radii of a sample of open clusters older than 1Gyr. The closeness of the solar orbit adius to the corotation resonance implies that the solar orbit lies inside a ring of minimum surface density (stellar + gas). This also implies a correction to larger values for the estimated total mass of the Galactic disc, and consequently, a greater contribution of the disc componente to the inner rotation curve of the Galaxy.

DIMENSION REDUCTION FOR POWER SYSTEM MODELING USING PCA METHODS CONSIDERING INCOMPLETE DATA READINGS

Principal Component Analysis (PCA) is a popular method for dimension reduction that can be used in many fields including data compression, image processing, exploratory data analysis, etc. However, traditional PCA method has several drawbacks, since the traditional PCA method is not efficient for dealing with high dimensional data and cannot be effectively applied to compute accurate enough principal components when handling relatively large portion of missing data. In this report, we propose to use EM-PCA method for dimension reduction of power system measurement with missing data, and provide a comparative study of traditional PCA and EM-PCA methods. Our extensive experimental results show that EM-PCA method is more effective and more accurate for dimension reduction of power system measurement data than traditional PCA method when dealing with large portion of missing data set.

A high-resolution binocular video-oculography system: assessment of pupillary light reflex and detection of an early incomplete blink and an upward eye movement

Background: The pupillary light reflex characterizes the direct and consensual response of the eye to the perceived brightness of a stimulus. It has been used as indicator of both neurological and optic nerve pathologies. As with other eye reflexes, this reflex constitutes an almost instantaneous movement and is linked to activation of the same midbrain area. The latency of the pupillary light reflex is around 200 ms, although the literature also indicates that the fastest eye reflexes last 20 ms. Therefore, a system with sufficiently high spatial and temporal resolutions is required for accurate assessment. In this study, we analyzed the pupillary light reflex to determine whether any small discrepancy exists between the direct and consensual responses, and to ascertain whether any other eye reflex occurs before the pupillary light reflex. Methods: We constructed a binocular video-oculography system two high-speed cameras that simultaneously focused on both eyes. This was then employed to assess the direct and consensual responses of each eye using our own algorithm based on Circular Hough Transform to detect and track the pupil. Time parameters describing the pupillary light reflex were obtained from the radius time-variation. Eight healthy subjects (4 women, 4 men, aged 24–45) participated in this experiment. Results: Our system, which has a resolution of 15 microns and 4 ms, obtained time parameters describing the pupillary light reflex that were similar to those reported in previous studies, with no significant differences between direct and consensual reflexes. Moreover, it revealed an incomplete reflex blink and an upward eye movement at around 100 ms that may correspond to Bell’s phenomenon. Conclusions: Direct and consensual pupillary responses do not any significant temporal differences. The system and method described here could prove useful for further assessment of pupillary and blink reflexes. The resolution obtained revealed the existence reported here of an early incomplete blink and an upward eye movement.

GU Monocerotis: A high-mass eclipsing overcontact binary in the young open cluster Dolidze 25

Context. The eclipsing binary GU Mon is located in the star-forming cluster Dolidze 25, which has the lowest metallicity measured in a Milky Way young cluster. Aims. GU Mon has been identified as a short-period eclipsing binary with two early B-type components. We set out to derive its orbital and stellar parameters. Methods. We present a comprehensive analysis, including B and V light curves and 11 high-resolution spectra, to verify the orbital period and determine parameters. We used the stellar atmosphere code FASTWIND to obtain stellar parameters and create templates for cross-correlation. We obtained a model to fit the light and radial-velocity curves using the Wilson-Devinney code iteratively and simultaneously. Results. The two components of GU Mon are identical stars of spectral type B1 V with the same mass and temperature. The light curves are typical of an EW-type binary. The spectroscopic and photometric analyses agree on a period of 0.896640 ± 0.000007 d. We determine a mass of 9.0 ± 0.6 M⊙ for each component and for temperatures of 28 000 ± 2000 K. Both values are consistent with the spectral type. The two stars are overfilling their respective Roche lobes, sharing a common envelope and, therefore the orbit is synchronised and circularised. Conclusions. The GU Mon system has a fill-out factor above 0.8, containing two dwarf B-type stars on the main sequence. The two stars are in a very advanced stage of interaction, with their extreme physical similarity likely due to the common envelope. The expected evolution of such a system very probably leads to a merger while still on the main sequence.

[Letter regarding the taxing of Harvard College real estate] (incomplete draft), [1798]

Two leaves of a draft of a letter in Eliphalet Pearson's hand addressed to "Gentleman,"detailing the Committee of the town of Cambridge's attempts to tax real estate owned the College.