Природа легитимности власти в дискурсе переходного типа социальности

Рассмотрена природа легитимности власти в дискурсе переходного типа социальности, раскрыта специфика социальных институтов и ценностей переходного времени, рассмотрена проблема сохранения стабильности общества

Development of knowledge management systems on the basis of unified ontological knowledge base

Creation of knowledge management system on the basis of a united model of knowledge organisation described in the form of the system of ontologies supplement each other is suggested. The base organization ontology and a set of ontologies of knowledge fields are included in the system. The construction variant of such model of knowledge is described and structure of knowledge control system on its basis is suggested

Геоэкологическая характеристика и оценка влияния автотранспорта на компоненты окружающей среды города Томска

В дипломной работе рассматривается геоэкологическая характеристика г. Томска и приводится анализ факторов, обуславливающих геоэкологичсекие проблемы территории. Одним из основных антропогенных источников загрязнения компонентов природной среды города выделен автотранспорт. В работе приводятся индикаторные особенности загрязнения депонирующих природных сред на территории г. Томска вследствие воздействия от автотранспорта.The research paper contains the physical features of Tomsk and an analysis of the factors causing the ecological problem of Tomsk territory. One of the major anthropogenic sources of pollution of environmental components selected city vehicles. The paper gives particular indicator depositing pollution of the environment on the territory of Tomsk as a result of the impact from vehicles. Thesis consists of 98 printed pages of text, 33 figures, 25 tables, bibliography includes 65 sources

Проект создания модульной теплицы с использованием технологии гидропоники и оценка его экономической эффективности

В работе рассматриваются современные проблемы сельского хозяйства, в частности выращивание овощей и бахчевых культур в регионах с средне-годовой температурой до минус 2 градусов цельсияGrowing vegetables in areas with cold winters

Геостатистические методы и алгоритмы построения объемных моделей параметров геологической среды

Целью данной работы является разработка метода оценки параметров геологической среды, обладающего разрешающей способностью данных геофизических исследований скважин и пространственной неоднородностью сейсмических атрибутов. Метод, предлагаемый в рамках данной работы, относится к классу геостатистических, однако в отличие от классических геостатситических методов, не требует введения предположения об однородности моделируемого параметра и использует сейсмические атрибуты для оценки пространственной корреляции. Предлагаемый метод также позволяет осуществлять оценку качества рассчитываемых моделей в любой точке исследуемого объёма.The main task of this work is to develop a method for assessing the geological environment parameters, with the geological well logging resolution and seismic attributes spatial heterogeneity. The proposed method is belongs to the geostatistics, however, unlike classical geostatistics methods, does not require the assumption of the modeled parameter homogeneity and uses seismic attributes to assess spatial correlation. The proposed method also allows you to assess the quality of the calculated models at any point in the investigated volume

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

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