The specific nature of the detention of foreigners, and its exploration : the Polish context

This text seeks to present basic knowledge on the detention of foreigners in Poland and the research perspective adopted in the project involving the authors of the papers published in this volume. The article has been divided into two parts. The first one contains characteristics of the detention of foreigners in the Polish context: directions of migration flows resulting from the location of our country, as well as the whereabouts and profiles of the centres administered by the Border Guard. Part two familiarises the reader with the specific nature of our detention study project: its conceptual apparatus, the adopted research paradigms, the applied methodology, and the challenges related to our exploratory efforts being performed in a very specific place - the guarded centres for foreigners. In the authors’ intention, all this information is to constitute a useful background to the detailed considerations contained in the subsequent papers presented in this volume of the journal

Nauki o polityce publicznej

Uniwersytet Warszawsk

Egzoszkielet na rękę - koncepcja i rozwój w ramach grantu "Rzeczy są dla ludzi"

The Institute of Computer Science and the Faculty of Mechatronics at Kazimierz Wielki University, together with Edurewolucje Sp. z o. o. z/s in Bydgoszcz, received funding under the 'Things are for people' competition of the National Centre for Research and Development for the project entitled 'Development of a functional arm exoskeleton for active training and rehabilitation'. The aim of the project is to carry out research and development work leading to the development of an innovative technology allowing for the independent rehabilitation ofpeople with special needs (with the participation of rehabilitators and physiotherapists). The project envisages the construction of a prototype of a mechanical rehabilitation robot, the so-called hand exoskeleton, which will support the process of rehabilitation of people with paresis and other specific needs regarding lack of mobility in the hand area. The project will develop specialised, dedicated software that will adapt the strength and type of work of the hand exoskeleton to the current needs and goals of the patient's rehabilitation programme. The aim ofthis paper is to provide an insight into the origins and development of the above concept within the project team during the project work to date.Instytut Informatyki oraz Wydział Mechatroniki Uniwersytetu Kazimierza Wielkiego wraz z firmą Edurewolucje Sp. z o. o. z/s w Bydgoszczy w ramach konkursu Narodowego Centrum Badań i Rozwoju "Rzeczy są dla ludzi" otrzymali dofinansowanie na realizacjęprzedsięwzięcia pn. „Opracowanie funkcjonalnego egzoszkieletu ręki do aktywnego treningu i rehabilitacji”. Celem projektu jest realizacja prac badawczo-rozwojowych prowadzących do opracowania innowacyjnej technologii pozwalającej na samodzielną rehabilitację osób zeszczególnymi potrzebami (przy udziale rehabilitantów i fizjoterapeutów). Projekt przewiduje skonstruowanie prototypu mechanicznego robota rehabilitacyjnego tzw. egzoszkieletu ręki, który wspomoże proces rehabilitacji osób z jej niedowładem oraz innymi szczególnymipotrzebami dotyczącymi braku mobilności w obszarze ręki. W ramach projektu powstanie specjalistyczne, dedykowane oprogramowanie, które będzie dostosowywało siłę i rodzaj pracy egzoszkieletu na rękę do aktualnych potrzeb i celów programu rehabilitacyjnego pacjenta. Celem niniejszej pracy jest przybliżenie powstania i rozwoju ww. koncepcji w ramach zespołu projektowego podczas dotychczasowych prac projektowych

Correlation between Oxygen Vacancies and Oxygen Evolution Reaction Activity for a Model Electrode: PrBaCo2O5+δ

The role of the perovskite lattice oxygen in the oxygen evolution reaction (OER) is systematically studied in the PrBaCo2O5+δ family. The reduced number of physical/chemical variables combined with in-depth characterizations such as neutron dif-fraction, O K-edge X-ray absorption spectroscopy (XAS), electron energy loss spectroscopy (EELS), magnetization and scanning transmission electron microscopy (STEM) studies, helps investigating the complex correlation between OER activity and a single perovskite property, such as the oxygen content. Larger amount of oxygen vacancies appears to facilitate the OER, possibly contributing to the mechanism involving the oxidation of lattice oxygen, i.e., the lattice oxygen evolution reaction (LOER). Furthermore, not only the number of vacancies but also their local arrangement in the perovskite lattice influences the OER activity, with a clear drop for the more stable, ordered stoichiometry.The X-ray absorption measurements were performed on the EPFL/PSI X-Treme beamline (O K-edge) and at the SuperXAS beamline (Co K-edge) at the Swiss Light Source, Paul Scherrer Institute, Villigen, Switzerland. The diffraction measurements were performed at the HRPT instrument at the Swiss spallation neutron source SINQ and at the MS-beamline at the Swiss Light Source at the Paul Scherrer Institute. The authors acknowledge the MS team for the measurements (Mesquik proposal 20182326). J.G. acknowledges Ramón y Cajal contract RYC-2012-11709 and the Severo Ochoa SEV-2015-0496 Project. The authors acknowledge the ICTS-CNME at UCM for offering access to their instruments and expertise and the Paul Scherrer Institute, for financial support through the internal CROSS project. T.J.S. thanks Innosuisse and the Swiss Competence Centre for Energy Research (SCCER) Heat & Electricity Storage.Peer reviewe

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

Structure and phase stability of nanocrystalline Ce1−xLnxO2−x/2−δ (Ln = Yb, Lu) in oxidizing and reducing atmosphere

The structure and phase evolution of nanocrystalline Ce1−xLnxO2−x/2−δ (Ln = Yb, Lu, x = 0 − 1) oxides upon heating in H2 was studied for the first time. Up to 950 °C the samples were single-phase, with structure changing smoothly with x from fluorite type (F) to bixbyite type (C). For the Lu-doped samples heated at 1100 °C in the air and H2, phase separation into coexisting F- and C-type structures was observed for ~0.40 < x < ~0.70 and ~0.25 < x < ~0.70, respectively. It was found also that addition of Lu3+ and Yb3+ strongly hinders the crystallite growth of ceria during heat treatment at 800 and 950 °C in both atmospheres. Valency of Ce and Yb in Ce0.1Lu0.9O1.55−δ and Ce0.95Yb0.05O1.975−δ samples heated at 1100 °C was studied by XANES and magnetic measurements. In the former Ce was dominated by Ce4+, with small contribution of Ce3+ after heating in H2. In the latter, Yb existed exclusively as 3+ in both O2 and H2

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI. Supplemental material in the ancillary file