1,559 research outputs found

    Optimal read/write memory system components

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    Two holographic data storage and display systems, voltage gradient ionization system, and linear strain manipulation system are discussed in terms of creating fast, high bit density, storage device. Components described include: novel mounting fixture for photoplastic arrays; corona discharge device; and block data composer

    Modeling of SAR signatures of shallow water ocean topography

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    A hydrodynamic/electromagnetic model was developed to explain and quantify the relationship between the SEASAT synthetic aperture radar (SAR) observed signatures and the bottom topography of the ocean in the English Channel region of the North Sea. The model uses environmental data and radar system parameters as inputs and predicts SAR-observed backscatter changes over topographic changes in the ocean floor. The model results compare favorably with the actual SEASAT SAR observed backscatter values. The developed model is valid for only relatively shallow water areas (i.e., less than 50 meters in depth) and suggests that for bottom features to be visible on SAR imagery, a moderate to high velocity current and a moderate wind must be present

    Optical read/write memory system components

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    The optical components of a breadboard holographic read/write memory system have been fabricated and the parameters specified of the major system components: (1) a laser system; (2) an x-y beam deflector; (3) a block data composer; (4) the read/write memory material; (5) an output detector array; and (6) the electronics to drive, synchronize, and control all system components. The objectives of the investigation were divided into three concurrent phases: (1) to supply and fabricate the major components according to the previously established specifications; (2) to prepare computer programs to simulate the entire holographic memory system so that a designer can balance the requirements on the various components; and (3) to conduct a development program to optimize the combined recording and reconstruction process of the high density holographic memory system

    Monte-Carlo methods for NLTE spectral synthesis of supernovae

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    We present JEKYLL, a new code for modelling of supernova (SN) spectra and lightcurves based on Monte-Carlo (MC) techniques for the radiative transfer. The code assumes spherical symmetry, homologous expansion and steady state for the matter, but is otherwise capable of solving the time-dependent radiative transfer problem in non-local-thermodynamic-equilibrium (NLTE). The method used was introduced in a series of papers by Lucy, but the full time-dependent NLTE capabilities of it have never been tested. Here, we have extended the method to include non-thermal excitation and ionization as well as charge-transfer and two-photon processes. Based on earlier work, the non-thermal rates are calculated by solving the Spencer-Fano equation. Using a method previously developed for the SUMO code, macroscopic mixing of the material is taken into account in a statistical sense. In addition, a statistical Markov-chain model is used to sample the emission frequency, and we introduce a method to control the sampling of the radiation field. Except for a description of JEKYLL, we provide comparisons with the ARTIS, SUMO and CMFGEN codes, which show good agreement in the calculated spectra as well as the state of the gas. In particular, the comparison with CMFGEN, which is similar in terms of physics but uses a different technique, shows that the Lucy method does indeed converge in the time-dependent NLTE case. Finally, as an example of the time-dependent NLTE capabilities of JEKYLL, we present a model of a Type IIb SN, taken from a set of models presented and discussed in detail in an accompanying paper. Based on this model we investigate the effects of NLTE, in particular those arising from non-thermal excitation and ionization, and find strong effects even on the bolometric lightcurve. This highlights the need for full NLTE calculations when simulating the spectra and lightcurves of SNe.Comment: Accepted for publication by Astronomy & Astrophysic

    АсимптотичСскоС ΠΏΠΎΠ²Π΅Π΄Π΅Π½ΠΈΠ΅ ΠΎΠ΄Π½ΠΎΠ³ΠΎ класса Ρ€Π΅ΡˆΠ΅Π½ΠΈΠΉ Π½Π΅Π»ΠΈΠ½Π΅ΠΉΠ½Ρ‹Ρ… Π½Π΅Π°Π²Ρ‚ΠΎΠ½ΠΎΠΌΠ½Ρ‹Ρ… Π΄ΠΈΡ„Ρ„Π΅Ρ€Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½Ρ‹Ρ… ΡƒΡ€Π°Π²Π½Π΅Π½ΠΈΠΉ Π²Ρ‚ΠΎΡ€ΠΎΠ³ΠΎ порядка

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    For the ordinary differential second-kind equation containing in a right member the sum composed with correctly varying concerning unknown function and its derivative of the first order by nonlinearities, necessary and sufficient existence enough a wide class of monotone solutions, and as exact asymptotic representations of solutions from the given class in a neighborhood of a singular point are established

    Условия сущСствования ΠΈ асимптотика ΠΎΠ΄Π½ΠΎΠ³ΠΎ класса Ρ€Π΅ΡˆΠ΅Π½ΠΈΠΉ сущСствСнно Π½Π΅Π»ΠΈΠ½Π΅ΠΉΠ½Ρ‹Ρ… Π΄ΠΈΡ„Ρ„Π΅Ρ€Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½Ρ‹Ρ… ΡƒΡ€Π°Π²Π½Π΅Π½ΠΈΠΉ Π²Ρ‚ΠΎΡ€ΠΎΠ³ΠΎ порядка

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    We consider the ordinary differential equation of the second order containing in the righthand side the sum of nonlinearities correctly varying concerning unknown function and its derivative of the first order. Necessary and sufficient conditions of existence of a wide class of monotone solutions, and exact asymptotic representations of solutions from the given class in a neighborhood of a singular point are established.Для ΠΎΠ±Ρ‹ΠΊΠ½ΠΎΠ²Π΅Π½Π½ΠΎΠ³ΠΎ Π΄ΠΈΡ„Ρ„Π΅Ρ€Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½ΠΎΠ³ΠΎ уравнСния Π²Ρ‚ΠΎΡ€ΠΎΠ³ΠΎ порядка, содСрТащСго Π² ΠΏΡ€Π°Π²ΠΎΠΉ части сумму слагаСмых с ΠΏΡ€Π°Π²ΠΈΠ»ΡŒΠ½ΠΎ ΠΌΠ΅Π½ΡΡŽΡ‰ΠΈΠΌΠΈΡΡ ΠΎΡ‚Π½ΠΎΡΠΈΡ‚Π΅Π»ΡŒΠ½ΠΎ нСизвСстной Ρ„ΡƒΠ½- ΠΊΡ†ΠΈΠΈ ΠΈ Π΅Ρ‘ ΠΏΡ€ΠΎΠΈΠ·Π²ΠΎΠ΄Π½ΠΎΠΉ ΠΏΠ΅Ρ€Π²ΠΎΠ³ΠΎ порядка нСлинСйностями, установлСны Π½Π΅ΠΎΠ±Ρ…ΠΎΠ΄ΠΈΠΌΡ‹Π΅ ΠΈ Π΄ΠΎ- статочныС условия сущСствования ΡˆΠΈΡ€ΠΎΠΊΠΎΠ³ΠΎ класса ΠΌΠΎΠ½ΠΎΡ‚ΠΎΠ½Π½Ρ‹Ρ… Ρ€Π΅ΡˆΠ΅Π½ΠΈΠΉ, Π° Ρ‚Π°ΠΊΠΆΠ΅ Ρ‚ΠΎΡ‡Π½Ρ‹Π΅ асимптотичСскиС прСдставлСния для Ρ€Π΅ΡˆΠ΅Π½ΠΈΠΉ ΠΈΠ· Π΄Π°Π½Π½ΠΎΠ³ΠΎ класса Π² окрСстности особой Ρ‚ΠΎΡ‡ΠΊΠΈ

    Consensus formation on coevolving networks: groups' formation and structure

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    We study the effect of adaptivity on a social model of opinion dynamics and consensus formation. We analyze how the adaptivity of the network of contacts between agents to the underlying social dynamics affects the size and topological properties of groups and the convergence time to the stable final state. We find that, while on static networks these properties are determined by percolation phenomena, on adaptive networks the rewiring process leads to different behaviors: Adaptive rewiring fosters group formation by enhancing communication between agents of similar opinion, though it also makes possible the division of clusters. We show how the convergence time is determined by the characteristic time of link rearrangement. We finally investigate how the adaptivity yields nontrivial correlations between the internal topology and the size of the groups of agreeing agents.Comment: 10 pages, 3 figures,to appear in a special proceedings issue of J. Phys. A covering the "Complex Networks: from Biology to Information Technology" conference (Pula, Italy, 2007

    Evolution equation for a model of surface relaxation in complex networks

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    In this paper we derive analytically the evolution equation of the interface for a model of surface growth with relaxation to the minimum (SRM) in complex networks. We were inspired by the disagreement between the scaling results of the steady state of the fluctuations between the discrete SRM model and the Edward-Wilkinson process found in scale-free networks with degree distribution P(k)∼kβˆ’Ξ» P(k) \sim k^{-\lambda} for Ξ»<3\lambda <3 [Pastore y Piontti {\it et al.}, Phys. Rev. E {\bf 76}, 046117 (2007)]. Even though for Euclidean lattices the evolution equation is linear, we find that in complex heterogeneous networks non-linear terms appear due to the heterogeneity and the lack of symmetry of the network; they produce a logarithmic divergency of the saturation roughness with the system size as found by Pastore y Piontti {\it et al.} for Ξ»<3\lambda <3.Comment: 9 pages, 2 figure

    АсимптотичСскиС прСдставлСния Ρ€Π΅ΡˆΠ΅Π½ΠΈΠΉ Π΄ΠΈΡ„Ρ„Π΅Ρ€Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½Ρ‹Ρ… ΡƒΡ€Π°Π²Π½Π΅Π½ΠΈΠΉ Π²Ρ‚ΠΎΡ€ΠΎΠ³ΠΎ порядка с ΠΏΡ€Π°Π²ΠΈΠ»ΡŒΠ½ΠΎ ΠΌΠ΅Π½ΡΡŽΡ‰ΠΈΠΌΠΈΡΡ ΠΎΡ‚Π½ΠΎΡΠΈΡ‚Π΅Π»ΡŒΠ½ΠΎ нСизвСстной Ρ„ΡƒΠ½ΠΊΡ†ΠΈΠΈ ΠΈ Π΅Π΅ ΠΏΡ€ΠΎΠΈΠ·Π²ΠΎΠ΄Π½ΠΎΠΉ ΠΏΠ΅Ρ€Π²ΠΎΠ³ΠΎ порядка нСлинСйностями

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    диссСртацияРабота носит тСорСтичСский Ρ…Π°Ρ€Π°ΠΊΡ‚Π΅Ρ€. Π Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹ диссСртации ΠΈ Ρ€Π°Π·Ρ€Π°Π±ΠΎΡ‚Π°Π½Π½Ρ‹Π΅ Π² Π½Π΅ΠΉ ΠΌΠ΅Ρ‚ΠΎΠ΄Ρ‹ исслСдования ΠΌΠΎΠ³ΡƒΡ‚ Π±Ρ‹Ρ‚ΡŒ ΠΈΡΠΏΠΎΠ»ΡŒΠ·ΠΎΠ²Π°Π½Ρ‹ ΠΏΡ€ΠΈ ΠΈΠ·ΡƒΡ‡Π΅Π½ΠΈΠΈ асимптотичСских свойств Ρ€Π΅ΡˆΠ΅Π½ΠΈΠΉ Π΄ΠΈΡ„Ρ„Π΅Ρ€Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½Ρ‹Ρ… ΡƒΡ€Π°Π²Π½Π΅Π½ΠΈΠΉ Π±ΠΎΠ»Π΅Π΅ высоких порядков с ΠΏΡ€Π°Π²ΠΈΠ»ΡŒΠ½ΠΎ ΠΌΠ΅Π½ΡΡŽΡ‰ΠΈΠΌΠΈΡΡ нСлинСйностями. ΠšΡ€ΠΎΠΌΠ΅ Ρ‚ΠΎΠ³ΠΎ, Π΄Π°Π½Π½Ρ‹Π΅ Ρ€Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹ ΠΌΠΎΠ³ΡƒΡ‚ Π±Ρ‹Ρ‚ΡŒ ΠΏΡ€ΠΈΠΌΠ΅Π½Π΅Π½Ρ‹ для рассмотрСния ΠΊΠΎΠ½ΠΊΡ€Π΅Ρ‚Π½Ρ‹Ρ… Π½Π΅Π»ΠΈΠ½Π΅ΠΉΠ½Ρ‹Ρ… Π΄ΠΈΡ„Ρ„Π΅Ρ€Π΅Π½Ρ†ΠΈΠ°Π»ΡŒΠ½Ρ‹Ρ… ΡƒΡ€Π°Π²Π½Π΅Π½ΠΈΠΉ Π²Ρ‚ΠΎΡ€ΠΎΠ³ΠΎ порядка, Π²ΠΎΠ·Π½ΠΈΠΊΠ°ΡŽΡ‰ΠΈΡ… Π² Ρ€Π°Π·Π»ΠΈΡ‡Π½Ρ‹Ρ… областях СстСствознания
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