SGR J1550–5418 Bursts Detected with the Fermi Gamma-Ray Burst Monitor during its Most Prolific Activity

We have performed detailed temporal and time-integrated spectral analysis of 286 bursts from SGR J1550–5418 detected with the Fermi Gamma-ray Burst Monitor (GBM) in 2009 January, resulting in the largest uniform sample of temporal and spectral properties of SGR J1550–5418 bursts. We have used the combination of broadband and high time-resolution data provided with GBM to perform statistical studies for the source properties. We determine the durations, emission times, duty cycles, and rise times for all bursts, and find that they are typical of SGR bursts. We explore various models in our spectral analysis, and conclude that the spectra of SGR J1550–5418 bursts in the 8-200 keV band are equally well described by optically thin thermal bremsstrahlung (OTTB), a power law (PL) with an exponential cutoff (Comptonized model), and two blackbody (BB) functions (BB+BB). In the spectral fits with the Comptonized model, we find a mean PL index of –0.92, close to the OTTB index of –1. We show that there is an anti-correlation between the Comptonized E_(peak) and the burst fluence and average flux. For the BB+BB fits, we find that the fluences and emission areas of the two BB functions are correlated. The low-temperature BB has an emission area comparable to the neutron star surface area, independent of the temperature, while the high-temperature BB has a much smaller area and shows an anti-correlation between emission area and temperature. We compare the properties of these bursts with bursts observed from other SGR sources during extreme activations, and discuss the implications of our results in the context of magnetar burst models

Guidewire-mounted thermal sensors to assess coronary hemodynamics

The vessels of the coronary circulation are prone to arteriosclerotic disease, which can lead to the development of obstructions to blood flow. The conventional way to diagnose the severity of this type of disease is by coronary angiography. This method, however, only provides insight into the morphology of the coronary vessels, whereas for an accurate diagnosis a measure for the actual flow impediment is needed. To perform these measurements, sensor-tipped guidewires have been developed to measure intra-coronary pressure and blood flow velocity. Diagnosis of coronary disease based on the time-average of these measurements have been shown to improve the clinical outcome of treatment significantly. However, since the coronary vessels are embedded in the (contracting) cardiac muscle, the interpretation of these indices is complicated and can be improved by simultaneously assessing the dynamics of coronary pressure and flow. The research described in this thesis therefore focusses on the one hand on developing devices for the simultaneous assessment of coronary pressure and flow dynamics and on the other hand on modeling the heart and coronary vessels to support the interpretation of these dynamic measurements. In the development of a device which can measure both coronary pressure and flow, two different strategies have been chosen. In the first strategy, a method has been developed to operate an already clinically used pressure sensor-tipped guidewire (pressure wire) as a thermal anemometer to also measure flow. In an in-vitro model it has been demonstrated that the power required to electrically heat the sensor is a measure for the shear rate at the sensor surface and that the method can be used to assess coronary flow reserve (CFR). By slightly adapting the method and combining it with a continuous thermodilution method, it has also been shown that the dynamics of both pressure and volumetric flow can be measured simultaneously in physiological representative in-vitro and ex-vivo experiments. The main drawbacks of this thermal method with a pressure wire are the relatively high sensor temperature required and the inability to detect flow reversal. In the second strategy, a new flow sensor, embedded in a flexible polyimide chip, has been specially designed to be mounted on a guidewire. The flow sensing element consists of a heater, operated at constant power, and thermocouples measuring the temperature difference up- and downstream from the heater. To gain insight into the working principle and the importance of the different design parameters, an analytical model has been developed. Experiments where upscaled sensors have been subjected to steady and pulsatile flow, indicate that the model is able to reproduce the experimental results fairly well but that the sensitivity to shear rate is rather limited in the physiological range. This sensitivity to shear rate can possibly be improved by operating the heater at constant temperature, which has been investigated with invitro experiments with upscaled sensors and a finite element analysis of the real, small size sensor. These studies have demonstrated that constant temperature operation of the heater is beneficial over constant power operation and that the dynamics of physiological coronary shear rate, including retrograde flow, can be assessed at an overheat temperature of only 5 K. From these characterization studies a new design of the sensor has been proposed, which is currently being manufactured to be tested in both in-vitro and ex-vivo experiments. To support the interpretation of the dynamic pressure and flow measurements, a numerical model of the heart and coronary circulation has been developed. The model is based on the coupling of four interacting parts: A model for the left ventricle which is based on the mechanics of a single myofiber, a 1D wave propagation model for the large epicardial coronary arteries, a stenosis element, and a Windkessel representation of the coronary micro-vessels. Comparison of the results obtained with the model with experimental observations described in literature has shown that the model is able to simulate the effect of different types of disease on coronary hemodynamics. After further validation, the model can be used as a tool to study the effect of combinations of epicardial and/or microcirculatory disease on pressure- and flow-based indices. To model the relation between the pressure and flow waves in the coronary arteries correctly, as well as to assist in the decision-making regarding the mechanical treatment of coronary stenoses, the mechanical behaviour of the coronary arterial wall is required. Therefore, a mixed numerical-experimental method has been employed to fit a micro-structurally based constitutive model to in-situ extensioninflation experiments on porcine coronary arteries. It has been demonstrated that the model can accurately describe the experimental data and, additionally, it has been found that the most influential parameter, describing the collagen fiber orientation, can be considered constant at physiological loading. In further research, this can be used to tackle over-parameterization issues inherent to fitting similar constitutive models to data obtained in a clinical setting. In this thesis, a computational model of the coronary circulation is presented and methods for simultaneous pressure and flow assessment are introduced. By operating an already clinically used pressure wire as a thermal anemometer, a methodology was developed which is close to clinical application, while a new sensor was designed to be more accurate in different flow conditions

On the design of a real-time volume rendering engine

An architecture for a Real-Time Volume Rendering Engine (RT-VRE) is given, capable of computing 750 × 750 × 512 samples from a 3D dataset at a rate of 25 images per second. The RT-VRE uses for this purpose 64 dedicated rendering chips, cooperating with 16 RISC-processors. A plane interpolator circuit and a composition circuit, both capable to operate at very high speeds, have been designed for a 1.6 micron VLSI process. Both the interpolator and composition circuit are back from production. They have been tested and both complied with our specifications

Exploring the electron density in plasmas induced by extreme ultraviolet radiation in argon

The new generation of lithography tools use high energy EUV radiation which ionizes the present background gas due to photoionization. To predict and understand the long term impact on the highly delicate mirrors It is essential to characterize these kinds of EUV-induced plasmas. We measured the electron density evolution in argon gas during and just after irradiation by a short pulse of EUV light at 13.5 nm by applying microwave cavity resonance spectroscopy. Dependencies on EUV pulse energy and gas pressure have been explored over a range relevant for industrial applications. Our experimental results show that the maximum reached electron density depends linearly on pulse energy. A quadratic dependence - caused by photoionization and subsequent electron impact ionization by free electrons - is found from experiments where the gas pressure is varied. This is demonstrated by our theoretical estimates presented in this manuscript as well.Comment: submitted to J. Phys. D. 16 pages, 8 figure

Applying an accurate spherical model to gamma-ray burst afterglow observations

We present results of model fits to afterglow data sets of GRB970508, GRB980703 and GRB070125, characterized by long and broadband coverage. The model assumes synchrotron radiation (including self-absorption) from a spherical adiabatic blast wave and consists of analytic flux prescriptions based on numerical results. For the first time it combines the accuracy of hydrodynamic simulations through different stages of the outflow dynamics with the flexibility of simple heuristic formulas. The prescriptions are especially geared towards accurate description of the dynamical transition of the outflow from relativistic to Newtonian velocities in an arbitrary power-law density environment. We show that the spherical model can accurately describe the data only in the case of GRB970508, for which we find a circumburst medium density consistent with a stellar wind. We investigate in detail the implied spectra and physical parameters of that burst. For the microphysics we show evidence for equipartition between the fraction of energy density carried by relativistic electrons and magnetic field. We also find that for the blast wave to be adiabatic, the fraction of electrons accelerated at the shock has to be smaller than 1. We present best-fit parameters for the afterglows of all three bursts, including uncertainties in the parameters of GRB970508, and compare the inferred values to those obtained by different authors

ASAS/WHO ICF Core Sets for ankylosing spondylitis (AS): how to classify the impact of AS on functioning and health

Objective: To report on the results of a standardised consensus process agreeing on concepts typical and/or relevant when classifying functioning and health in patients with ankylosing spondylitis (AS) based on the International Classification of Functioning and Health (ICF).Methods: Experts in AS from different professional and geographical backgrounds attended a consensus conference and were divided into three working groups. Rheumatologists were selected from members of the Assessment of SpondyloArthritis international Society (ASAS). Other health professionals were recommended by ASAS members. The aim was to compose three working groups with five to seven participants to allow everybody's contribution in the discussions. Experts selected ICF categories that were considered typical and/or relevant for AS during a standardised consensus process by integrating evidence from preceding studies in alternating working group and plenary discussions. A Comprehensive ICF Core Set was selected for the comprehensive classification of functioning and a Brief ICF Core Set for application in trials.Results: The conference was attended by 19 experts from 12 countries. Eighty categories were included in the Comprehensive Core Set, which included 23 Body functions, 19 Body structures, 24 Activities and participation and 14 Environmental factors. Nineteen categories were selected for the Brief Core Set, which included 6 Body functions, 4 Body structures, 7 Activities and participation and 2 Environmental factors.Conclusion: The Comprehensive and Brief ICF Core Sets for AS are now available and aim to represent the external reference to define consequences of AS on functioning

Broadband modelling of short gamma-ray bursts with energy injection from magnetar spin-down and its implications for radio detectability

The magnetar model has been proposed to explain the apparent energy injection in the X-ray light curves of short gamma-ray bursts (SGRBs), but its implications across the full broadband spectrum are not well explored. We investigate the broadband modelling of four SGRBs with evidence for energy injection in their X-ray light curves, applying a physically motivated model in which a newly formed magnetar injects energy into a forward shock as it loses angular momentum along open field lines. By performing an order of magnitude search for the underlying physical parameters in the blast wave, we constrain the characteristic break frequencies of the synchrotron spectrum against their manifestations in the available multi-wavelength observations for each burst. The application of the magnetar energy injection profile restricts the successful matches to a limited family of models that are self-consistent within the magnetic dipole spin-down framework.We produce synthetic light curves that describe how the radio signatures of these SGRBs ought to have looked given the restrictions imposed by the available data, and discuss the detectability of these signatures with present-day and near-future radio telescopes. Our results show that both the Atacama Large Millimetre Array and the upgraded Very Large Array are now sensitive enough to detect the radio signature within two weeks of trigger in most SGRBs, assuming our sample is representative of the population as a whole. We also find that the upcoming Square Kilometre Array will be sensitive to depths greater than those of our lower limit predictions.Comment: 15 pages, 4 figures, 6 tables, accepted for publication in MNRA

Growth and production of Bullia rhodostoma on an open sandy beach in Algoa Bay

The plough shell, Bullia rhodostoma (Mollusca: Gastropoda), has been studied on an open sandy beach where it is a common scavenger. Samples taken over a year indicate hatching of young individuals from December to February. They reach a length of about 10 mm after 1 year and 40 mm after 10 years. The von Bertalanffy growth equation is Lt = 47 (1 - e-0,19(t+0,23)) and the annual mortality rate is 0,79. Mean decalcified dry biomass is 209 mg m-2 and production by growth 189 mg m-2 y-1 giving a P/B of 0,9. Most production by adults (>15 mm shell length) goes into reproduction, particularly In the females which grow larger than the males. Production by reproduction is estimated to be about 135 mg m-2 y-1. Average calorific values are 19,04 kJ g-1 dry tissueDie ploegskulp, Bullia rhodostoma (Mollusca: Gastropoda), is op 'n oop sandstrand bestudeer waar dit 'n algemeen teenwoordige aasvreter is. Monsters wat oor 'n jaar geneem is, dui aan dat die jong individue tussen Desember en Februarie uitbroei. Hulle bereik 'n lengte van ongeveer 10 mm na 1 jaar en 40 mm na 10 jaar. Die Von Bertalanffy groeivergelyking is Lt = 47 (1 - e-0,19(t+0,23))) en die jaarlikse mortaliteitstempo is 0,79. Gemiddelde kalklose drofi biomassa is 209 mg m-2 y-1 wat 'n P/B van 0,9 gee. Die meeste volwasse (>15 mm skulplengte) produksie is in die vorm van voortplanting, veral in die wyfies wat groter as die mannetjies word. Produksie deur voortplanting is omtrent 135 mg m-2 y-1 Gemiddelde kaloriewaardes is 19,04 kJ g-1 droe weefsel