5,928 research outputs found
The Health System and the Russian Orthodox Church: Prospects for Development
The article examines the participation and assistance of the Orthodox Church in solving problems that allowed to give a scientific justification for the cooperation of health care and Orthodox religious institutions, to determine their role in the historical context and structure of modern healthcare in Russia. The article presents an algorithm for organizing sisters of mercy, their system of upbringing. Particular attention is given to the possibility of teaching the course "Foundations of Orthodox Culture" in secular educational institutions.
Research materials can serve as a basis for the formation of morally sound positions of medical workers and the population on the main problems of medical activity.
Based on the study, the authors published a series of articles in which the experience of the work of the Orthodox Church in the charitable sphere has been summarized. This experience can be used to create new charitable institutions, including those who provided medical assistance.
In preparing the article, the authors used concrete historical, civilizational, formational and social methods of research that allowed us to uncover facts, phenomena and processes in the interconnection and unity of the past, present and future
A Model of Interindustry Interaction in the USSR
A quantitative analysis of the development of interindustry flows in the Soviet economy showed that traditional input-output methods needed to be expanded and generalized for use in Soviet medium-term (5-7 year) planning. In particular, it is necessary to account for supply constraints on some products and relative surpluses of others. This paper describes a model which accounts for these influences, fits closely the development of the Soviet economy from 1950 to 1975, and can be and has been used in the exploratory stages of Soviet planning
Color Cerberus
Simple convolutional neural network was able to win ISISPA color constancy
competition. Partial reimplementation of (Bianco, 2017) neural architecture
would have shown even better results in this setup
Jointly Optimal Channel Pairing and Power Allocation for Multichannel Multihop Relaying
We study the problem of channel pairing and power allocation in a
multichannel multihop relay network to enhance the end-to-end data rate. Both
amplify-and-forward (AF) and decode-and-forward (DF) relaying strategies are
considered. Given fixed power allocation to the channels, we show that channel
pairing over multiple hops can be decomposed into independent pairing problems
at each relay, and a sorted-SNR channel pairing strategy is sum-rate optimal,
where each relay pairs its incoming and outgoing channels by their SNR order.
For the joint optimization of channel pairing and power allocation under both
total and individual power constraints, we show that the problem can be
decoupled into two subproblems solved separately. This separation principle is
established by observing the equivalence between sorting SNRs and sorting
channel gains in the jointly optimal solution. It significantly reduces the
computational complexity in finding the jointly optimal solution. It follows
that the channel pairing problem in joint optimization can be again decomposed
into independent pairing problems at each relay based on sorted channel gains.
The solution for optimizing power allocation for DF relaying is also provided,
as well as an asymptotically optimal solution for AF relaying. Numerical
results are provided to demonstrate substantial performance gain of the jointly
optimal solution over some suboptimal alternatives. It is also observed that
more gain is obtained from optimal channel pairing than optimal power
allocation through judiciously exploiting the variation among multiple
channels. Impact of the variation of channel gain, the number of channels, and
the number of hops on the performance gain is also studied through numerical
examples.Comment: 15 pages. IEEE Transactions on Signal Processin
Stable monopole and dyon solutions in the Einstein-Yang-Mills theory in asymptotically anti-de Sitter Space
A continuum of new monopole and dyon solutions in the Einstein-Yang-Mills
theory in asymptotically anti-de Sitter space are found. They are regular
everywhere and specified with their mass, and non-Abelian electric and magnetic
charges. A class of monopole solutions which have no node in non-Abelian
magnetic fields are shown to be stable against spherically symmetric linear
perturbations.Comment: 9 pages with 5 figures. Revised version. To appear in Phys Rev Let
Π‘ΠΠΠ ΠΠΠΠΠΠ«Π ΠΠΠΠΠΠΠΠ’ΠΠ Π« ΠΠΠ― ΠΠΠ ΠΠΠΠΠΠΠΠ― ΠΠΠΠ’Π ΠΠΠ’ΠΠΠΠ ΠΠ¬ΠΠΠ¬ΠΠΠΠ―
Current review covers all main stages of the quantitative determination of nitrogen by the Kjeldahl method: preparation and acid mineralization of samples, distillation, and various chemical and instrumental options for determining the ammonia released after the treatment of mineralization products with alkali. The review also describes the latest technical solutions used to improve and automate certain stages of analysis such as the usage of block and IR digesters that significantly increases the efficiency of sample mineralization and reduces its duration; the usage of automatic lifts for the mineralized samples, which reduces the work of the operator with the heavy and hot chemical samples as much as possible; the usage of autosampler, which provides the automatic transfer of mineralized samples to the distiller; the automation of distillation and titration processes; the use of software for processing the analysis results. The following technical characteristics of the basic components of automatic analyzers for the nitrogen determination by the Kjeldahl method are systematized: digesters, distillers, and titrators produced by such well-known companies as Buchi (Switzerland), C. Gerhardt, Behr Labor-Technik GmbH and FoodALYT GmbH (Germany), Foss Tecator (Denmark, Sweden), VELP Scientifica (Italy), J.P.Selecta (Spain), Hanon Instruments (China), OOO VPK Sibagropribor and OOO Vilitek (Russia). The data on the characteristics of the analyzers is also provided and includes the number and volume of test tubes (flasks), the time of mineralization, distillation and analysis, mass (volume) of the sample, and the lower limit of nitrogen detection.Keywords: Kjeldahl method, acid mineralization, distillation and quantitative determination of ammonia, automatic nitrogen analyzerDOI: http://dx.doi.org/10.15826/analitika.2019.23.2.002(Russian)E.A. Zauer, A.B. ErshovVolgograd State Technical University, pr. Lenina, 28, Volgograd, 400005,Russian FederationΠ ΠΏΡΠ΅Π΄Π»Π°Π³Π°Π΅ΠΌΠΎΠΌ ΠΎΠ±Π·ΠΎΡΠ΅ ΡΠ°ΡΡΠΌΠΎΡΡΠ΅Π½Ρ ΠΎΡΠ½ΠΎΠ²Π½ΡΠ΅ ΡΡΠ°Π΄ΠΈΠΈ ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½ΠΈΡ Π°Π·ΠΎΡΠ° ΠΌΠ΅ΡΠΎΠ΄ΠΎΠΌ ΠΡΠ΅Π»ΡΠ΄Π°Π»Ρ: ΠΏΠΎΠ΄Π³ΠΎΡΠΎΠ²ΠΊΠ° ΠΈ ΠΊΠΈΡΠ»ΠΎΡΠ½Π°Ρ ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·Π°ΡΠΈΡ ΠΏΡΠΎΠ±, ΠΎΡΠ³ΠΎΠ½ΠΊΠ° ΠΈ ΡΠ°Π·Π»ΠΈΡΠ½ΡΠ΅ Π²Π°ΡΠΈΠ°Π½ΡΡ (Ρ
ΠΈΠΌΠΈΡΠ΅ΡΠΊΠΈΠ΅ ΠΈ ΠΈΠ½ΡΡΡΡΠΌΠ΅Π½ΡΠ°Π»ΡΠ½ΡΠ΅) ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½ΠΈΡ Π°ΠΌΠΌΠΈΠ°ΠΊΠ°, Π²ΡΠ΄Π΅Π»ΠΈΠ²ΡΠ΅Π³ΠΎΡΡ ΠΏΠΎΡΠ»Π΅ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ ΠΏΡΠΎΠ΄ΡΠΊΡΠΎΠ² ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·Π°ΡΠΈΠΈ ΡΠ΅Π»ΠΎΡΡΡ. ΠΡΠΈΠ²Π΅Π΄Π΅Π½Ρ Π½ΠΎΠ²ΡΠ΅ ΡΠ΅Ρ
Π½ΠΈΡΠ΅ΡΠΊΠΈΠ΅ ΡΠ΅ΡΠ΅Π½ΠΈΡ ΠΏΠΎΡΠ»Π΅Π΄Π½ΠΈΡ
Π»Π΅Ρ ΠΏΠΎ ΡΠΎΠ²Π΅ΡΡΠ΅Π½ΡΡΠ²ΠΎΠ²Π°Π½ΠΈΡ ΠΈ Π°Π²ΡΠΎΠΌΠ°ΡΠΈΠ·Π°ΡΠΈΠΈ ΠΎΡΠ΄Π΅Π»ΡΠ½ΡΡ
ΡΡΠ°Π΄ΠΈΠΉ Π°Π½Π°Π»ΠΈΠ·Π°: ΠΏΡΠΈΠΌΠ΅Π½Π΅Π½ΠΈΠ΅ Π±Π»ΠΎΡΠ½ΡΡ
ΠΈ ΠΠ-Π΄ΠΈΠ³Π΅ΡΡΠΎΡΠΎΠ², ΡΡΡΠ΅ΡΡΠ²Π΅Π½Π½ΠΎ ΠΏΠΎΠ²ΡΡΠΈΠ²ΡΠΈΡ
ΡΡΡΠ΅ΠΊΡΠΈΠ²Π½ΠΎΡΡΡ ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·Π°ΡΠΈΠΈ ΠΎΠ±ΡΠ°Π·ΡΠΎΠ² ΠΈ ΡΠ½ΠΈΠ·ΠΈΠ²ΡΠΈΡ
Π΅Π΅ Π΄Π»ΠΈΡΠ΅Π»ΡΠ½ΠΎΡΡΡ; ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΠ΅ Π°Π²ΡΠΎΠΌΠ°ΡΠΈΡΠ΅ΡΠΊΠΈΡ
ΠΏΠΎΠ΄ΡΠ΅ΠΌΠ½ΠΈΠΊΠΎΠ² ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·ΠΎΠ²Π°Π½Π½ΡΡ
ΠΏΡΠΎΠ±, ΠΌΠ°ΠΊΡΠΈΠΌΠ°Π»ΡΠ½ΠΎ ΡΠΎΠΊΡΠ°ΡΠΈΠ²ΡΠΈΡ
ΡΠ°Π±ΠΎΡΡ ΠΎΠΏΠ΅ΡΠ°ΡΠΎΡΠ° Ρ ΡΡΠΆΠ΅Π»ΡΠΌΠΈ ΠΏΡΠΎΠ±Π°ΠΌΠΈ ΠΈ Π³ΠΎΡΡΡΠΈΠΌΠΈ Ρ
ΠΈΠΌΠΈΡΠ΅ΡΠΊΠΈΠΌΠΈ Π²Π΅ΡΠ΅ΡΡΠ²Π°ΠΌΠΈ; Π°Π²ΡΠΎΡΠ΅ΠΌΠΏΠ»Π΅ΡΠΎΠ², ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠΈΠ²Π°ΡΡΠΈΡ
Π°Π²ΡΠΎΠΌΠ°ΡΠΈΡΠ΅ΡΠΊΡΡ ΠΏΠ΅ΡΠ΅Π΄Π°ΡΡ ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·ΠΎΠ²Π°Π½Π½ΡΡ
ΠΏΡΠΎΠ± Π² Π΄ΠΈΡΡΠΈΠ»Π»ΡΡΠΎΡ; Π°Π²ΡΠΎΠΌΠ°ΡΠΈΠ·Π°ΡΠΈΡ ΠΏΡΠΎΡΠ΅ΡΡΠΎΠ² Π΄ΠΈΡΡΠΈΠ»Π»ΡΡΠΈΠΈ ΠΈ ΡΠΈΡΡΠΎΠ²Π°Π½ΠΈΡ; ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΠ΅ ΠΏΡΠΎΠ³ΡΠ°ΠΌΠΌΠ½ΠΎΠ³ΠΎ ΠΎΠ±Π΅ΡΠΏΠ΅ΡΠ΅Π½ΠΈΡ Π΄Π»Ρ ΠΎΠ±ΡΠ°Π±ΠΎΡΠΊΠΈ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΠΎΠ² Π°Π½Π°Π»ΠΈΠ·Π°. Π‘ΠΈΡΡΠ΅ΠΌΠ°ΡΠΈΠ·ΠΈΡΠΎΠ²Π°Π½Ρ ΡΠ΅Ρ
Π½ΠΈΡΠ΅ΡΠΊΠΈΠ΅ Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊΠΈ ΠΎΡΠ½ΠΎΠ²Π½ΡΡ
ΡΠ·Π»ΠΎΠ² Π°Π²ΡΠΎΠΌΠ°ΡΠΈΡΠ΅ΡΠΊΠΈΡ
Π°Π½Π°Π»ΠΈΠ·Π°ΡΠΎΡΠΎΠ² Π΄Π»Ρ ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½ΠΈΡ Π°Π·ΠΎΡΠ° ΠΌΠ΅ΡΠΎΠ΄ΠΎΠΌ ΠΡΠ΅Π»ΡΠ΄Π°Π»Ρ β Π΄ΠΈΠ³Π΅ΡΡΠΎΡΠΎΠ², Π΄ΠΈΡΡΠΈΠ»Π»ΡΡΠΎΡΠΎΠ² ΠΈ ΡΠΈΡΡΠ°ΡΠΎΡΠΎΠ², Π²ΡΠΏΡΡΠΊΠ°Π΅ΠΌΡΡ
ΡΠ°ΠΊΠΈΠΌΠΈ ΠΈΠ·Π²Π΅ΡΡΠ½ΡΠΌΠΈ ΡΠΈΡΠΌΠ°ΠΌΠΈ, ΠΊΠ°ΠΊ Buchi (Π¨Π²Π΅ΠΉΡΠ°ΡΠΈΡ), C. Gerhardt, Behr Labor-Technik GmbH ΠΈ FoodALYT GmbH (ΠΠ΅ΡΠΌΠ°Π½ΠΈΡ), Foss Tecator (ΠΠ°Π½ΠΈΡ, Π¨Π²Π΅ΡΠΈΡ), VELP Scientifica (ΠΡΠ°Π»ΠΈΡ), J.P.Selecta (ΠΡΠΏΠ°Π½ΠΈΡ), Hanon Instruments (ΠΠΈΡΠ°ΠΉ), ΠΠΠ ΠΠΠ Π‘ΠΈΠ±Π°Π³ΡΠΎΠΏΡΠΈΠ±ΠΎΡ ΠΈ ΠΠΠ Β«ΠΠΈΠ»ΠΈΡΠ΅ΠΊΒ» (Π ΠΎΡΡΠΈΡ). Π’Π°ΠΊΠΆΠ΅ ΠΏΡΠΈΠ²Π΅Π΄Π΅Π½Ρ Π΄Π°Π½Π½ΡΠ΅ ΠΎΠ± ΠΎΡΠ½ΠΎΠ²Π½ΡΡ
Π°Π½Π°Π»ΠΈΡΠΈΡΠ΅ΡΠΊΠΈΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊΠ°Ρ
Π°Π½Π°Π»ΠΈΠ·Π°ΡΠΎΡΠΎΠ²: ΡΠΈΡΠ»Π΅ ΠΈ ΠΎΠ±ΡΠ΅ΠΌΠ΅ ΠΏΡΠΎΠ±ΠΈΡΠΎΠΊ (ΠΊΠΎΠ»Π±), Π²ΡΠ΅ΠΌΠ΅Π½ΠΈ ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·Π°ΡΠΈΠΈ, Π΄ΠΈΡΡΠΈΠ»Π»ΡΡΠΈΠΈ ΠΈ Π°Π½Π°Π»ΠΈΠ·Π°; ΠΌΠ°ΡΡΠ΅ (ΠΎΠ±ΡΠ΅ΠΌΠ΅) ΠΏΡΠΎΠ±Ρ, Π½ΠΈΠΆΠ½Π΅ΠΌ ΠΏΡΠ΅Π΄Π΅Π»Π΅ ΠΎΠ±Π½Π°ΡΡΠΆΠ΅Π½ΠΈΡ Π°Π·ΠΎΡΠ°.ΠΠ»ΡΡΠ΅Π²ΡΠ΅ ΡΠ»ΠΎΠ²Π°: ΠΌΠ΅ΡΠΎΠ΄ ΠΡΠ΅Π»ΡΠ΄Π°Π»Ρ, ΠΊΠΈΡΠ»ΠΎΡΠ½Π°Ρ ΠΌΠΈΠ½Π΅ΡΠ°Π»ΠΈΠ·Π°ΡΠΈΡ, ΠΎΡΠ³ΠΎΠ½ΠΊΠ° ΠΈ ΠΎΠΏΡΠ΅Π΄Π΅Π»Π΅Π½ΠΈΠ΅ Π°ΠΌΠΌΠΈΠ°ΠΊΠ°, Π°Π²ΡΠΎΠΌΠ°ΡΠΈΡΠ΅ΡΠΊΠΈΠΉ Π°Π½Π°Π»ΠΈΠ·Π°ΡΠΎΡ Π°Π·ΠΎΡΠ°DOI: http://dx.doi.org/10.15826/analitika.2019.23.2.00
The Evolution of NGC 7027 at Radio Frequencies: A New Determination of the Distance and Core Mass
We present the results of a 25-year program to monitor the radio flux
evolution of the planetary nebula NGC7027. We find significant evolution of the
spectral flux densities. The flux density at 1465 MHz, where the nebula is
optically thick, is increasing at a rate of 0.251+-0.015 % per year, caused by
the expansion of the ionized nebula. At frequencies where the emission is
optically thin, the spectral flux density is changing at a rate of
-0.145+-0.005 % per year, caused by a decrease in the number of ionizing
photons coming from the central star. A distance of 980+-100 pc is derived. By
fitting interpolated models of post-AGB evolution to the observed changes, we
find that over the 25-yr monitoring period, the stellar temperature has
increased by 3900+-900 K and the stellar bolometric luminosity has decreased by
1.75+-0.38 %. We derive a distance-independent stellar mass of 0.655+-0.01
solar masses adopting the Bloecker stellar evolution models, or about 0.04
solar masses higher when using models of Vassiliadis & Wood which may provide a
better fit. A Cloudy photoionization model is used to fit all epochs at all
frequencies simultaneously. The differences between the radio flux density
predictions and the observed values show some time-independent residuals of
typically 1 %. A possible explanation is inaccuracies in the radio flux scale
of Baars et al. We propose an adjustment to the flux density scale of the
primary radio flux calibrator 3C286, based on the Cloudy model of NGC7027. We
also calculate precise flux densities for NGC7027 for all standard continuum
bands used at the VLA, as well as for some new 30GHz experiments.Comment: submitted to the Astrophysical Journa
Monopoles, Dyons and Black Holes in the Four-Dimensional Einstein-Yang-Mills Theory
A continuum of monopole, dyon and black hole solutions exist in the
Einstein-Yang-Mills theory in asymptotically anti-de Sitter space. Their
structure is studied in detail. The solutions are classified by non-Abelian
electric and magnetic charges and the ADM mass. The stability of the solutions
which have no node in non-Abelian magnetic fields is established. There exist
critical spacetime solutions which terminate at a finite radius, and have
universal behavior. The moduli space of the solutions exhibits a fractal
structure as the cosmological constant approaches zero.Comment: 36 Pages, 16 Figures. Minor typos corrected and one figure modifie
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