187,500 research outputs found

    Procopio, P

    No full text

    Procopio di Cesarea, Santa Sofia di Costantinopoli. Un tempio di luce (De Aedificiis I 1, 1-78)

    No full text
    La parte del volume di mia pertinenza evidenzia gli aspetti peculiari del passo sulla basilica di Santa Sofia contenuto nel De Aedificiis di Procopio: l’interesse, raro per l’epoca, per gli aspetti tecnico-strutturali dell’edificio e per gli scienziati-architetti che lo progettarono; il punto di vista dell’osservatore che, in un processo di immedesimazione con l’autore, ci guida alla percezione dello spazio mutevole e complesso della basilica; l’intuizione– che ho inteso sviluppare – che Santa Sofia, in tutte e sue componenti, fu progettata come una gigantesca macchina di luce. Il libro è corredato da un ricco apparato illustrativo e da sette tavole ricostruttive, ideate da chi scrive espressamente per questo volume

    [Nicolai Alemanni De Procopio et arcana eius historia indicium]

    No full text
    Tit. y autor tomados de prefacioTexto paralelo griego-latÞn de p. XIX-XXIII y p. 1-135Pie de imp. tomado de colofónSign.: a¬2-5, e¡3, i¡2, o¡4, A-R¡4, a-c¡4, d¬1, d¬3-4, e¡4, f¬2-3, g-i¡4, k¬1, k¬4, l-u¡4Error de pag., de p. 112 pasa a 115Texto a dos colContiene: Historia arcana / Procopius de Cesarea, p. 1-135Notas históricas a la Historia arcana de Procopio / Nicola s Alemanni, p. 1-14

    Photoluminescent and crystal structure properties of the yellow and orange forms of [Re2(m-Cl)2(CO)6(m- 4,5-trimethyl-silyl-pyridazine]

    No full text
    A series of neutral, dinuclear, luminescent rhenium(I) complexes suitable for phosphorescent organic light emitting devices (OLEDs) has been recently reported1,2. These compounds, of general formula [Re2(μ-Cl)2(CO)6(μ-1,2-diazine)], contain diazines bearing alkyl groups in one or in both the b positions. The complexes show intense green/yellow emissions in toluene solution and in the solid state and some of the complexes possess, in solution, high emission quantum yields (F 0.18-0.22 for the derivatives with disubstituted diazines). The excited state responsible for this emission can be confidentially described as a triplet metal-to-ligand charge transfer (3MLCT) level3. Following the DFT computational suggestions we have now synthetized a new complex of this family using the 4,5-bis(trimetylsilyl)-1,2-diazine ligand namely [Re2(m-Cl)2(CO)6(m- 4,5-trimethyl-silyl-pyridazine] (1, see Scheme). This complex has been completely carachterized in solution and it shows an emission maximum batochromically shifted respect to those of the analogous Re(I) compounds with alkyl-substituted diazine, with a lower quantum yield. Slow evaporation at room temperature of a CH2Cl2 solution containing (1) induces the concomitant formation of orange and yellow single crystals (Figure 1, top). X-ray crystal structure determinations performed at room temperature as well as at 100 K, show that they are two different polymorphs of the same compound. The emission spectra recorded on crystalline samples of the two polymorph (Figure 1, bottom) are hypsochromically shifted respect to the solution one and present higher quantum yields (lem = 537 nm and F = 0.30 for the yellow phase, lem = 575 nm and F = 0.50, for the orange one). References (1) Mauro, M, Quartapelle Procopio, E., Sun,Y., Chien, C-H., Donghi, D., Panicati, M., Mercandelli, P., Mussini, P., D’Alfonso, G., De Cola, L. Adv. Func. Mat. 2009, in press (2) Donghi, D., D’Alfonso, G., Mauro, M, Panigati, M., Mercandelli, P., Sironi, A., Mussini, P., D’Alfonso, L., Inorg. Chem. 2008, 47, 4243. (3) Wrighton, M., Morse, D. L., J. Am. Chem. Soc., 1974, 96, 998

    A numerical code for the solution of the Kompaneets equation in cosmological context

    No full text
    Context. After fundamental ground-based, balloon-born, and space experiments, and, in particular, after the COBE/FIRAS results, confirming that only very small deviations from a Planckian shape can be present in the CMB spectrum, current and future CMB absolute temperature experiments aim at discovering very small distortions such as those associated with the cosmological reionization process or that could be generated by different kinds of earlier processes. Aims. Interpretation of future data calls for a continuous improvement in the theoretical modeling of CMB spectrum. In this work we describe the fundamental approach and, in particular, the update to recent NAG versions of a numerical code, KYPRIX, specifically written to solve the Kompaneets equation in a cosmological context. It was first implemented in the years 1989-1991 to accurately compute the CMB spectral distortions under general assumptions. Methods. Specifically, we describe the structure and the main subdivisions of the code and discuss the most relevant aspects of its technical implementation. After a presentation of the equation formalism and of the boundary conditions added to the set of ordinary differential equations derived from the original parabolic partial differential equation, we provide details on the adopted space variable (i.e. dimensionless frequency) and space discretization, on time variables, on the output results, on the accuracy parameters, and on the used auxiliary integration routines. The problem with introducing the time dependence of the ratio between electron and photon temperatures and of the radiative Compton scattering term, both of them introducing integral terms into the Kompaneets equation, is addressed in the specific context of the recent NAG versions. We describe the introduction of the cosmological constant in the terms controlling the general expansion of the Universe in agreement with the current concordance model, of the relevant chemical abundances, and on the ionization history, from recombination to cosmological reionization. The global computational time, the impact of the various aspects of the code on it, and the accuracy of the numerical integration are also discussed. Results. We present some of fundamental tests we carried out to verify the accuracy, reliability, and performance of the code. We focus on some quantitative tests of energy conservation and the time behavior of electron temperature. A comparison of the results obtained with the update and the original version of the code is presented for some representative cases. Finally, we focus on some properties of the free-free distortions relevant for the long wavelength region of the CMB spectrum. Conclusions. All the tests demonstrate the reliability and versatility of the new code version and its accuracy and applicability to the scientific analysis of current CMB spectrum data and of much more precise measurements that will be available in the future. The recipes and tests described in this work can also be useful for implementing accurate numerical codes for other scientific purposes using the same or similar numerical libraries or for verifying the validity of different codes aimed at the same problem or similar ones

    Going Beyond Counting First Authors in Author Co-citation Analysis

    No full text
    The present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed

    Integration of large-size photovoltaic systems into the distribution grids: a P–Q chart approach to assess reactive support capability

    No full text
    This study addresses the issue of the control of both active (P) and reactive (Q) power flows injected by grid connected photovoltaic (PV) units participating in the provision of the reactive power compensation ancillary service. A model is derived allowing to define a sort of 'capability chart' for the PV unit, that is, the set of points in the P-Q plane which, at steady state, can be reached by properly operating the control system and without exceeding the physical limits of all the involved devices. To this aim, a basic algorithm is developed in the MATLAB environment relying on a simplified description of the system, which neglects the harmonics injected by the voltage source converter inverter used to connect the PV unit with a medium voltage radial distribution grid. The proposed model is used to evaluate all the possible working points in the P-Q chart; a proof of the stability of those points, using the well-known Lyapunov methods, is also annexed. Finally, simulations with the electromagnetic code PSCAD-EMTDC are performed in order to assess the validity of the approximate results and to improve the developed basic algorithm. © 2010 © The Institution of Engineering and Technology
    corecore